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<v Speaker 1>You see, something's going to happen. What's going to happen?

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<v Speaker 1>What I help? On a winter night in sixteen oh four,

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<v Speaker 1>a new star burned through the velvet of the sky

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<v Speaker 1>in Prague, A thin, nearsighted mathematician stood at a window

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<v Speaker 1>and took notes by kindlelight. That man Johannes Kepler believed

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<v Speaker 1>the heavens were legible, that number and harmony were the

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<v Speaker 1>alphabet of creation. I made this episode because Keppler sits

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<v Speaker 1>exactly where our show loves to work, at the scene

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<v Speaker 1>where mysticism meets measurement, where sacred geometry becomes celestial mechanics,

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<v Speaker 1>and we're an astrologer, school teacher, refugee, and court mathematician

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<v Speaker 1>chisel law out of wonder. Kepler's life is a parable

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<v Speaker 1>for anyone trying to keep faith and reason in the

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<v Speaker 1>same room. He cast horoscopes to pay rent and scrapped

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<v Speaker 1>circles for eclipses because the data said so. He wrote

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<v Speaker 1>prayers into his proofs. He defended his mother in a

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<v Speaker 1>witchcraft trial and still found the patients to compute mars

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<v Speaker 1>for years. His voice, equal parts devout and defiant, tells

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<v Speaker 1>us that truth is the daughter of time, and in

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<v Speaker 1>his time, we let him speak tonight. We follow him

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<v Speaker 1>step by step, from Wilderstadt to the lecture halls of Tubingan,

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<v Speaker 1>from the platonic dreams of Mysterium Cosmographicum to the hard,

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<v Speaker 1>stubborn numbers of Estronomia Nova, from the music of the

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<v Speaker 1>spheres and Harmonisius Mundi to the glass and light of Diopters.

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<v Speaker 1>From Graz to Prague to Linn's to Ulm, carrying tables,

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<v Speaker 1>depths and a vision of order that outlived the Thirty

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<v Speaker 1>Years War. We're here to read Kepler in his own words,

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<v Speaker 1>to place him in the world. He walked mud streets,

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<v Speaker 1>church bells, printing presses, played cards, and to ask what

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<v Speaker 1>his laws, his optics, his reformed astrology, and his lunar

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<v Speaker 1>dream mean for art, ritual and the modern imagination. If

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<v Speaker 1>you ever looked up and felt that hush, the sense

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<v Speaker 1>the sky isn't just scenery but syntax, this is your episode.

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<v Speaker 1>Johannes Kepler lived from fifteen seventy one to sixteen thirty

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<v Speaker 1>and he lived in an age of religious turmoil and

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<v Speaker 1>scientific rebirth. He was a German astronomer, mathematician, astrologer and

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<v Speaker 1>natural philosopher, a visionary who helped transform Renaissance s mysticism

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<v Speaker 1>into empirical science of the Scientific Revolution. Kepler is best

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<v Speaker 1>known for discovering the laws of planetary motion, foundational principles

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<v Speaker 1>that guided later scientists like Isaac Newton towards the theory

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<v Speaker 1>of gravity. But Kepler was more than a mathematician. He

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<v Speaker 1>was a man of deep faith and imagination, convinced that

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<v Speaker 1>the cosmos was an orderly creation imbued with meaning. Those

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<v Speaker 1>laws of nature are within the grasp of the human mind.

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<v Speaker 1>God wanted us to recognize by creating us after his

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<v Speaker 1>own image, so that we could share in his own thoughts.

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<v Speaker 1>Kepler wrote expressing the belief that deciphering the heavens was

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<v Speaker 1>a way to think God's thoughts after him. His life's

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<v Speaker 1>work was driven by this almost spiritual quest for cosmic

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<v Speaker 1>harmony and truth. And telling Kepler's story one finds a

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<v Speaker 1>narrative as dramatic as the times in which he lived.

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<v Speaker 1>He witnessed the fading of old certainties, the geocentric Earth,

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<v Speaker 1>Earth centered universe, and the sharp divide between science and superstition,

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<v Speaker 1>and he helped usher in new understanding, grounding, and observation

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<v Speaker 1>geometry and physics. Yet Kepler's path was not easy. He

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<v Speaker 1>endured war, religious persecution, personal tragedies, and even a witchcraft

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<v Speaker 1>trial against his own mother. Through it all, he remained

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<v Speaker 1>scrupulously honest to the data and to his convictions. The

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<v Speaker 1>result was a legacy that spans astronomy and optics, music

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<v Speaker 1>and mysticism, religion and philosoph This episode follows Kepler's journey

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<v Speaker 1>chronologically from his humble beginnings and education, through his wanderings

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<v Speaker 1>across Europe in search of intellectual refuge, to his scientific triumphs,

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<v Speaker 1>while also exploring the rich tapestry of influences, ideas, and

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<v Speaker 1>historical events that shaped his work. As we shall see,

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<v Speaker 1>Kepler much preferred the sharpest criticism of a single intelligent

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<v Speaker 1>man to the thoughtless approval of the masses, forging a

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<v Speaker 1>unique path that married rigorous science with a profound sense

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<v Speaker 1>of wonder. Johannes Kepler was born on December twenty seventh,

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<v Speaker 1>fifteen seventy one, and the small Swabian town of Weilderstadt

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<v Speaker 1>in the Holy Roman Empire in modern Germany. He came

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<v Speaker 1>from a modest and tumultuous family background. His father, Heinrich

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<v Speaker 1>Keppler was a mercenary soldier who left home when Johannes

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<v Speaker 1>was young and likely died abroad by fifteen seventy seven,

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<v Speaker 1>and his mother, Katharina Goldenman, was the daughter of an

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<v Speaker 1>innkeeper known for her herbal remedies and folkilling. The Kepler

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<v Speaker 1>family had been respected in earlier generations. Johannas's grandfather, Sebald Kepler,

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<v Speaker 1>had even served as mayor of their city, but by

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<v Speaker 1>the time of Johanna's birth, their fortunes had dwindled. Born

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<v Speaker 1>prematurely and frequently ill in childhood, Keppler was a frail

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<v Speaker 1>boy with weak vision. A bout of smallpox left his

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<v Speaker 1>eyes damaged and his hands crippled, Yet he showed early

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<v Speaker 1>intellectual gifts and in an almost mystical awe for the heavens.

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<v Speaker 1>In fifteen seventy seven, at just six years old, Johannes's

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<v Speaker 1>mother took him to a high place to witness the

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<v Speaker 1>Great Comet of fifteen seventy seven, a spectacle that captivated

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<v Speaker 1>astronomers across Europe. He later recalled being entranced by the

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<v Speaker 1>bright comet hanging in the sky. Two years later, in

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<v Speaker 1>fifteen eighty, he was called outside at night to see

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<v Speaker 1>a lunar eclipse, noting how the moon appeared quite red,

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<v Speaker 1>another formative experience for the young stargazer. These childhood events

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<v Speaker 1>kindled a passion for astronomy that would last his entire

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<v Speaker 1>even though his poor eyesight meant he would never be

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<v Speaker 1>known from making telescopic discoveries like Alileo, Kepler himself joked

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<v Speaker 1>that although his mind was sky bound, the shadow of

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<v Speaker 1>his body lies here on earth, a poignant reflection he

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<v Speaker 1>will later choose for his epitheph. Encouraged by his family's

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<v Speaker 1>Lutheran faith and by his own evident intellect, Kepler pursued

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<v Speaker 1>an education that combined classical learning with religious training. He

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<v Speaker 1>attended local Latin schools, and in fifteen eighty four, at

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<v Speaker 1>age thirteen, he entered the Protestant seminary at Eldenburg. He

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<v Speaker 1>proved to be a brilliant student. By fifteen eighty nine,

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<v Speaker 1>Kepler earned a scholarship to the University of Tubajin, a

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<v Speaker 1>leading Protestant university, to study theology and prepare for the

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<v Speaker 1>Lutheran ministry. At Tubingan's Tubingerstiff Seminary, Kepler received a thorough

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<v Speaker 1>grounding in classical philosophy, mathematics, and astronomy. His mentor in

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<v Speaker 1>mathematics and astronomy was Michael Maslin, one of the few

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<v Speaker 1>academics of the time who embraced the Copernican heliocentric model,

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<v Speaker 1>though cautiously and only in private lectures. Under Maslin's guidance,

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<v Speaker 1>Kepler learned both the traditional Polemaic Earth centered system and

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<v Speaker 1>the revolutionary Copernican Sun centered system of planetary motion. Kepler

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<v Speaker 1>was quickly won over to Copernican's vision. He later wrote

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<v Speaker 1>that it was a tubingin that he became a Copernican

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<v Speaker 1>for what he called physical or if you prefer metaphysical reasons.

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<v Speaker 1>In other words, he sensed that a sun centered cosmos

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<v Speaker 1>had a deeper natural truth and harmony to it. Indeed,

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<v Speaker 1>Kepler's faith in a rational God created order predisposed him

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<v Speaker 1>to favor a system where the Sun, symbol of God's light,

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<v Speaker 1>sat at the center. As a student, he even engaged

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<v Speaker 1>in a public disputation defending heliocentrism on both scientific and

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<v Speaker 1>theological grounds, arguing that the Sun is the principal source

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<v Speaker 1>of motion to the universe. This was bold given that

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<v Speaker 1>Lutheran and Catholic authorities alike still regarded heliocentrism with suspicion.

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<v Speaker 1>Kepler's subtle deviations from strict Lutheran doctrine already began causing friction.

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<v Speaker 1>He refused to fully subscribe to the formula of Concord

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<v Speaker 1>in fifteen seventy seven, a Lutheran confession of faith, because

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<v Speaker 1>he had private doubts on points of theology. Because of

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<v Speaker 1>these scruples, Kepler's hopes of becoming a pastor dimmed. Nevertheless,

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<v Speaker 1>he saw no conflict between faith and science. I wanted

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<v Speaker 1>to become a theologian. For a long time. I was unhappy.

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<v Speaker 1>Now behold, God is praised by my work, even in astronomy.

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<v Speaker 1>Kepler later reflected to him uncovering the mathematical laws of

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<v Speaker 1>creation was a form of devotion. This conviction set the

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<v Speaker 1>stage for his life's work. In fifteen ninety four, at

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<v Speaker 1>the age of twenty two, Johannes Kepler left academia to

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<v Speaker 1>begin a career in teaching and incidentally, in government service

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<v Speaker 1>as an astrologer. He was recommended for and accepted a

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<v Speaker 1>post as professor of mathematics at the Protestant Seminary in

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<v Speaker 1>Gratz in the US Austrian province of Steria. In this role,

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<v Speaker 1>he taught arithmetic, geometry, and sometimes Greek and rhetoric to

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<v Speaker 1>the school students. He also carried the title of district mathematician,

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<v Speaker 1>which meant he was responsible for issuing official calendars in

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<v Speaker 1>astrological almanacs, a lucrative and respected task at the time.

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<v Speaker 1>In the late sixteenth century, there was no firm separation

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<v Speaker 1>between astronomy and astrology. The two were considered two sides

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<v Speaker 1>of the same coin. Like other learned astronomers, even Tycho

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<v Speaker 1>Brahe and Galileo, Kepler practiced astrology to earn his keep.

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<v Speaker 1>He cast horoscopes for wealthy patrons and local nobility, and

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<v Speaker 1>made weather and political predictions in annual calendars. Though he

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<v Speaker 1>privately disdained the more superstitious aspects of astrology, he conceded

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<v Speaker 1>that mother astronomy would surely have to suffer hunger if

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<v Speaker 1>the daughter astrology did not earn their bread. In other words,

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<v Speaker 1>it was astrology that paid the bills, allowing him to

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<v Speaker 1>pursue pure astronomy. Kepler spent a huge amount of time

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<v Speaker 1>trying to reform astrology on a sounder footing, composing over

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<v Speaker 1>eight hundred horoscopes and several treaties on the subject. He

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<v Speaker 1>aimed to distill whatever he thought scientifically plausible, for instance,

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<v Speaker 1>effects of the sun, moon, and planets mediated through an

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<v Speaker 1>Earth's soul via harmonies or light from what he called

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<v Speaker 1>the Swinnish rashness of fortune tellers. In sixteen oh one,

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<v Speaker 1>he even wrote a short work on giving astrology sounder

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<v Speaker 1>foundations to accompany one of his almanacs, and in sixteen ten,

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<v Speaker 1>when two other authors feuded over astrology merits, Kepler intervened

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<v Speaker 1>with attract third party intervening, cautioning that while much astrological

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<v Speaker 1>superstition deserves rejection, one must not throw the baby out

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<v Speaker 1>with the bath water by dismissing real cosmic influences. This

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<v Speaker 1>balanced approach typified Kepler's unque blend of mysticism and empiricism

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<v Speaker 1>during his grazzias. Even while he fulfilled his public duties,

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<v Speaker 1>Kepler was pursuing an arditious private research program, an attempt

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<v Speaker 1>to decipher the geometrical plan of the cosmos. Shortly after

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<v Speaker 1>arriving at Grotz, he experienced what he described as a

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<v Speaker 1>moment of illumination. On July nineteenth, fifteen ninety five, while

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<v Speaker 1>teaching a class, Kepler was explaining the periodic conjunctions of

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<v Speaker 1>Saturn and Jupiter and the Zodiac when he had an epiphany.

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<v Speaker 1>He realized that the intervals between planets might be explained

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<v Speaker 1>by pure geometry. Initially, Kepler tried inscribing and circumscribing one

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<v Speaker 1>circle between another using regular polygons, seeking a unique geometric

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<v Speaker 1>spacing for the six known planets, but this approach failed

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<v Speaker 1>to much observations. He then contemplated three dimensional shapes. In

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<v Speaker 1>a breakthrough, Kepler imagined nesting the five periodic platonic solids

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<v Speaker 1>one inside another, each separated by circumscribed and inscribed sphere.

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<v Speaker 1>There were only five such polyhedra, and placing them in

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<v Speaker 1>the proper order produced six layers, which he identified with

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<v Speaker 1>the six planets Mercury, Venus, Earth, Mars, Jupiter, Saturn. To

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<v Speaker 1>Kepler's delight, the model roughly matched the relative sizes of

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<v Speaker 1>the planet's orbits as known from Copernicus's data, Especially for

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<v Speaker 1>planets beyond Mercury. He believed he had glimpsed the very

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<v Speaker 1>geometric blueprint of God. Geometry is co eternal with God,

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<v Speaker 1>and God used it in laying out the world Keppelo

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<v Speaker 1>would write later reflecting his neoplatonic conviction that geometrical forms

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<v Speaker 1>give structure to creation. With almost evangelical zeal, the young

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<v Speaker 1>astronomer set out to share his revelation. In fifteen ninety six,

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<v Speaker 1>at just twenty five years old, Keppela published his first book,

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<v Speaker 1>Pisterium Cosmographicum Mystery of the Cosmos. This was his first

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<v Speaker 1>bold attempt to decipher the divine geometric plan of the universe.

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<v Speaker 1>Kepplo was a deeply religious thinker who believe that God,

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<v Speaker 1>the great mathematician, had built the cosmos with mathematical harmony.

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<v Speaker 1>Inspired by quasi mystical revelation while teaching in Gods, he

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<v Speaker 1>became convinced that the spacing of the six known planets

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<v Speaker 1>was no accident. It must be patterned after the five

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<v Speaker 1>perfect platonic solids of antiquity. Kepler set out to prove

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<v Speaker 1>that each planetary orbit is separated by a nested polyhedron,

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<v Speaker 1>inscribed and circumscribed by spheres matching the orbit of one

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<v Speaker 1>planet to the next. This elegant model, he thought, explained

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<v Speaker 1>why there were exactly six planets and provided a compelling

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<v Speaker 1>geometric rationale for Copernicus's son's censored system. Keppler's Mysterium was

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<v Speaker 1>the first published defense of copernicant heliocentrism since Copernicus himself,

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<v Speaker 1>and it was strikingly unusual for the blending rigorous astronomy

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<v Speaker 1>with neoplatonic mysticism. In the book's preface, he declared his

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<v Speaker 1>mission to show that God, in creating the universe and

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<v Speaker 1>regulating the order of the cosmos, had in view the

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<v Speaker 1>fire irregular bodies of geometry, and that he has fixed,

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<v Speaker 1>according to those geometric dimensions, the number of the heavens,

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<v Speaker 1>their proportions, and relations of their movements. The Mysterium did

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<v Speaker 1>more than propose a poetic model. It insisted that astronomy

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<v Speaker 1>must explain the actual spacing of planetary orbits in three

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<v Speaker 1>dimensional space, not just their abstract order. To Kepler, Copernicus's

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<v Speaker 1>system implied a physical reality in which nothing could be

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<v Speaker 1>altered without upsetting the harmony of the whole. This mindset

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<v Speaker 1>led him to consider the Sun's force as it caused

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<v Speaker 1>a planetary motion weakening with distance, oppressing, and insight that

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<v Speaker 1>nudged astronomy away from purely kinematic models towards physics. Although

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<v Speaker 1>the platonic solid model itself was not quantitatively accurate, its

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<v Speaker 1>beauty and haunting strangeness captivated Kepler and set him on

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<v Speaker 1>a path of asking deeper questions. He even published a

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<v Speaker 1>second edition twenty five years later, unwilling to aband and

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<v Speaker 1>in the idea that some fundamental harmonies underlies the cosmos.

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<v Speaker 1>With hindsight, we see Mysterium Cosmographicum as an important stepping

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<v Speaker 1>stone and empirically inaccurate but esthetically beautiful hypothesis that nevertheless

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<v Speaker 1>prompted Kepler to seek physical causes and would ultimately lead

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<v Speaker 1>to his monumental Laws of planetary motion. While in Grotz,

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<v Speaker 1>Kepler also began side studies in chronology and astrology, even

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<v Speaker 1>trying to link planetary positions to weather and earthly events.

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<v Speaker 1>He speculated about the Earth having a soul that responds

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<v Speaker 1>to the positions of the planets. This was part of

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<v Speaker 1>a grand plan that he had sketched out to write

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<v Speaker 1>several books on the stationary sun and fixed stars, on

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<v Speaker 1>planetary motions, on the physical nature of planets, and on

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<v Speaker 1>the influences of the heavens on Earth. The Mysterium was

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<v Speaker 1>only the first installment of this ambitious program. However, events

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<v Speaker 1>in Grots would soon disrupt Kepler's work and force him

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<v Speaker 1>to flee. Our Reformation was gathering steam under Archduke Shun

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<v Speaker 1>Emperor Ferdinand the second, a staunch Catholic, determined to root

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<v Speaker 1>out Protestantism in his realms. Tensions in Steria mounted in

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<v Speaker 1>September fifteen ninety eight, and decree expelled all Protestant teachers

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<v Speaker 1>and preachers from Gratz. Initially, Keppel was exempted from expulsion

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<v Speaker 1>because of his valuable status as district mathematician. The authorities

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<v Speaker 1>did not want to lose the calendar maker, but Kepler

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<v Speaker 1>felt far from safe. That year, he wrote to a

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<v Speaker 1>friend that he foresore dark times ahead. Sure enough, by

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<v Speaker 1>fifteen ninety nine his position was untenable. Meanwhile, in Prague,

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<v Speaker 1>Tycho brahe had been appointed Imperial mathematician to Emperor Rudolph

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<v Speaker 1>the second. Ticho, the Great Danish astronomer, was eager for

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<v Speaker 1>a skilled assistant to help make sense of his vast

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<v Speaker 1>treasury of planetary observations. He had heard of Kepler's talent

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<v Speaker 1>for theoretical insight. In December fifteen ninety nine, Tycho intended

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<v Speaker 1>an invitation to Kepler to join him in Prague. Kepler

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<v Speaker 1>leapt at the opportunity, without even waiting for the formal

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<v Speaker 1>letter to arrive. He set off from Gratz on January first,

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<v Speaker 1>sixteen hundred, heading north to Bohemia in hopes that Tycho's

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<v Speaker 1>patronage could solve both his scientific quandaries and his precarious

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<v Speaker 1>political situation. Kepler's departure from Grotz was abrupt. He left

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<v Speaker 1>behind his post and the home that he had established there,

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<v Speaker 1>and it must be noted he left in the company

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<v Speaker 1>of some emotional turmoil. During his Grotz years, Keppler had

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<v Speaker 1>fallen in love and married. In December fifteen ninety five,

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<v Speaker 1>he met Barbara Muller, a twenty three year old, twice

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<v Speaker 1>widowed young woman with a small daughter. Barbara came from

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<v Speaker 1>a prosperous family, for Falla was a successful mill owner,

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<v Speaker 1>whereas Keppler was an impecuineous scholar. Her Falla was initially

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<v Speaker 1>opposed to the match, considering Kepler's poverty unacceptable despite his

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<v Speaker 1>noble ancestry. Only after Kepler finished Mysterium Cosmographicum, perhaps proving

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<v Speaker 1>his potential, did her family rely, and Barbara and Johannes

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<v Speaker 1>married on April twenty seventh, fifteen ninety seven. The marriage

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<v Speaker 1>in its early years was reportedly strained by financial worries

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<v Speaker 1>and by Kepler's single minded focus on his studies. They

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<v Speaker 1>had two children in Grotz in fifteen ninety eight and

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<v Speaker 1>fifteen ninety nine, but tragically both infants, a son, Heinrich

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<v Speaker 1>and a daughter, Susannah, died in infancy. It was amid

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<v Speaker 1>these personal trials that Kepler abandoned Grotz. By September sixteen hundred,

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<v Speaker 1>after a final edict demanded that all Protestants convert to

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<v Speaker 1>Catholicism or leave Steria. Kepler and Barbara, pregnant again, packed

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<v Speaker 1>their belongings and fled grots for Prague, effectively as religious refugees.

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<v Speaker 1>Keppeler did not know it yet, but he would never

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<v Speaker 1>return into the life of a provincial school teacher, ahead

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<v Speaker 1>lay his most productive scientific years under the patronage of

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<v Speaker 1>the Holy Roman Emperor. When Keppeler arrived in Prague in

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<v Speaker 1>early sixteen hundred, he entered an environment that must have

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<v Speaker 1>seemed like the Promised Land to a man obsessed with astronomy.

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<v Speaker 1>Tycho Brahe welcomed him to the Imperial Observatory and soon

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<v Speaker 1>put Keplar to work analyzing observations of Mars. Mars was

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<v Speaker 1>famously the most troublesome planet for astronomers. Its apparent backward

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<v Speaker 1>retrograde motions and changes in brightness had defied simple explanation

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<v Speaker 1>in circular orbit models. Tycho possessed the most precise Mars

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<v Speaker 1>data ever obtained, measured without telescopes using giant citing instruments.

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<v Speaker 1>His measurements were accurate within a arc minute or two.

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<v Speaker 1>For the first time, Kepler had the accurate empirical foundation

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00:19:35.359 --> 00:19:39.359
<v Speaker 1>he needed. However, Tycho was protective of his data. He

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<v Speaker 1>did not initially allow Kepler unlimited access or copies of

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<v Speaker 1>his observations. Kepler estimated it might take him up to

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<v Speaker 1>two years of hard work to test his geometric theories

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<v Speaker 1>against Tycho's Mars data, since he would have to perform

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<v Speaker 1>calculations on site. He and Tycho had a brief falling

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<v Speaker 1>out in the spring of sixteen hundred over for more

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00:20:00.000 --> 00:20:02.759
<v Speaker 1>employment terms and salary that led Kepler to leave for

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00:20:02.799 --> 00:20:07.480
<v Speaker 1>a short time. Fortunately, the reconciled quickly and reached an agreement.

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<v Speaker 1>Tycho recognized Keppler's value and secured him a position as

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<v Speaker 1>an imperial collaborator. By summer of sixteen hundred, after returning

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<v Speaker 1>to Gratz briefly to collect his family, Kepler settled in

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<v Speaker 1>Prague for good. Tragically, Kepler's direct collaboration with the illustrious

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<v Speaker 1>Tycho would be short lived. In October sixteen oh one,

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<v Speaker 1>only about a year after Kepler arrived, Tycho Brahe died suddenly.

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<v Speaker 1>Tycho's death threatened to leave Kepler stranded, but the Emperor

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<v Speaker 1>Rudolph the Second promptly appointed Kepler as Tycho's successor Imperial Mathematician.

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<v Speaker 1>This was the most prestigious post for a mathematician in Europe,

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<v Speaker 1>essentially making Kepler the court astronomer. It also gave him

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<v Speaker 1>custody of Tycho's precious astronomical data. After some wrangling with

316
00:20:55.799 --> 00:20:58.920
<v Speaker 1>Tycho's heirs, who tried to claim that data was private property,

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<v Speaker 1>Kepler gained access to the observations he needed. He was

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<v Speaker 1>keenly aware of the importance of this moment. He had

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<v Speaker 1>in his hands the raw material to revolutionize astronomy, to

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<v Speaker 1>us on whom divine benevolence has bestowed the most diligent

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<v Speaker 1>of observers, Tycho Brahe, from whose observations this eight minute

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<v Speaker 1>error in the orbit of Mars is deduced. It is

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<v Speaker 1>fitting that we accept with grateful minds this gift from

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<v Speaker 1>God and both acknowledge and build upon it. Referring to

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<v Speaker 1>a tiny discrepancy Tycho had found in Mars's orbit that

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<v Speaker 1>hinted the ancient models were wrong, Kepla would indeed build

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<v Speaker 1>upon Tycho's legacy, and in doing so he changed our

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<v Speaker 1>view of the cosmos. As imperial mathematician and Prague, Keppler's

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<v Speaker 1>duties were twofold, for example, providing astrological forecasts and calendars

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<v Speaker 1>to the Emperor, and to conduct astronomical research, including the

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<v Speaker 1>completion of the new Rudolphine Tables, an updated set of

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<v Speaker 1>astronomical tables, planetary positions, star catalogs, et cetera, using tycho

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<v Speaker 1>superior observations and per Rudolph the second was an enlightened

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<v Speaker 1>and eccentric patron of the sciences, interested in astronomy, alchemy,

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<v Speaker 1>and all matter of esoteric knowledge. He tolerated Keppler's Lutheran faith,

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<v Speaker 1>despite Prague being officially Catholic. In practice, Kepler had a

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<v Speaker 1>fair degree of intellectual freedom at Ruolph's court, even as

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<v Speaker 1>he struggled with intermittent salary payments from the cash strapped

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<v Speaker 1>Imperial Treasury. It was an invigorating situation. Kepler rubbed shoulders

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<v Speaker 1>with other learned men in Prague from Jeweler's turned mathematicians

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<v Speaker 1>like Josh Bergee, tou scalars like Johannes Mathaus, Whacker and

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<v Speaker 1>David Fabricius. This collegial atmosphere, combined with Keppler's own single

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<v Speaker 1>minded determination, led to an explosion of productivity. The eleven

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<v Speaker 1>years Kepler spent in Prague sixteen oh one to sixteen

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<v Speaker 1>twelve would be the most scientifically fruitful time of his life.

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<v Speaker 1>One of Kepler's first targets of study was the orbit

347
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<v Speaker 1>of Mars. Continuing the work Tycho had assigned him, Kepeler

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<v Speaker 1>approached the problem with a novel mindset. He was willing

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<v Speaker 1>to abandon the ancient insumption that planetary motions must be

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<v Speaker 1>combinations of uniform circular paths. Instead, he sought a single,

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<v Speaker 1>unified orbit from Mars, shaped by a physical cause, what

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<v Speaker 1>he called a celestial physics. He suspected the Sun was

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<v Speaker 1>the source of a force that drove the planets, an

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<v Speaker 1>idea inspired by his belief that the son symbolized God

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<v Speaker 1>the Father, and likely influenced by William Gilbert's sixteen hundred

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<v Speaker 1>book d Magneti, which posited a magnetic soul in the Earth.

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<v Speaker 1>Keppler theorized that a force emanating from the Sun weakened

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<v Speaker 1>with distance, causing planets further out to move more slowly,

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<v Speaker 1>a remarkable prescient intuition we can recognize in it an

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<v Speaker 1>early notion of a gravitational or magnetic inverse square law.

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<v Speaker 1>Armed with Tycho's precise measurements of Mars positions at various

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<v Speaker 1>points in its orbits, Kepler attacked the data with tireless calculations.

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<v Speaker 1>He tried one geometric model after another, measuring the error

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<v Speaker 1>each time. Initially, he attempted to use a small oval

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<v Speaker 1>like path, and even tried incorporating the old equon a

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<v Speaker 1>mathematical point that Copernicus had eliminated to see if he

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<v Speaker 1>could fit the data, but nothing gave a perfect match.

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<v Speaker 1>Mars observed positions differed by as much as eight arc

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<v Speaker 1>minutes eight sixtieth of a degree from the best circular

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<v Speaker 1>or oval models Kepler could construct. Instead of dismissing this

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<v Speaker 1>tiny discrepancy, Kepler famously said that the commander of eight minutes.

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<v Speaker 1>It the error will lead us to complete reform of astronomy.

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<v Speaker 1>His contemporaries might have swept such a small error under

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<v Speaker 1>the rug, but Kepler trusted the data with Tycho's observations.

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<v Speaker 1>This eight minute discrepancy is a gift of God, he wrote,

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<v Speaker 1>believing that such anomalies were clues to the true theory.

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<v Speaker 1>After numerous failed attempts, Kepler made his greatest discovery in

378
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<v Speaker 1>late sixteen o four. Hed had what one might call

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<v Speaker 1>his second epiphany, the first being the platonic solids model.

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<v Speaker 1>Having tried over forty different geometrical constructions to fit Mars's orbit,

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<v Speaker 1>he finally considered that the path might be an ellipse

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<v Speaker 1>rather than a circle or arbitrary oval. The ellipses were

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<v Speaker 1>a simple conic section, a familiar shape, Yet no astronomer

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<v Speaker 1>before had dad suggests the planets literally travel on ellipses.

385
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<v Speaker 1>Kepler had initially thought an ellipse was too simple. Surely,

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<v Speaker 1>he imagined the great minds of antiquity would have tried

387
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<v Speaker 1>it if it worked. But when he plotted Mars's position

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<v Speaker 1>as an elliptical path with the Sun at once focus

389
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<v Speaker 1>of the ellipse, the data fit beautifully, the long standing

390
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<v Speaker 1>mystery of Mars's motion was solved. Mars, and by extension,

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<v Speaker 1>the other planets move around the Sun in ellipses rather

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<v Speaker 1>than perfect circles. Kepler immediately generalized this insight into what

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<v Speaker 1>we now call Kepler's first law, the orbits of the

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<v Speaker 1>planets or ellipses with the Sun at one time focus. Furthermore,

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<v Speaker 1>he had already deduced a rule for how a planet

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<v Speaker 1>speed varies along its orbit. By sixteen oh two. Through

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<v Speaker 1>laborious calculations, Kepler found that the line connecting a planet

398
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<v Speaker 1>to the Sun sweeps out equal areas in equal times,

399
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<v Speaker 1>implying that a planet moves faster when nearer the Sun

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<v Speaker 1>and slower when farther. This became Kepler's second law of

401
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<v Speaker 1>planetary motion, the area law. It was intimately linked to

402
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<v Speaker 1>his assumption of a solar force. This area law mathematically

403
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<v Speaker 1>represents a conserved motion consistent with a type influence, though

404
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<v Speaker 1>he didn't formulate it in those terms. The aerial law

405
00:26:40.000 --> 00:26:44.359
<v Speaker 1>mathematically represents a conserved motion consistent with a one R

406
00:26:44.400 --> 00:26:48.039
<v Speaker 1>two type influence, though he didn't formulate it in those terms.

407
00:26:48.799 --> 00:26:51.839
<v Speaker 1>By combining the aerial law with the elliptical shape. Kepler

408
00:26:51.880 --> 00:26:55.960
<v Speaker 1>had constructed the first accurate physic based model of planetary motion.

409
00:26:56.960 --> 00:26:59.559
<v Speaker 1>While still in gross in astronomy, Kepler turned his analytical

410
00:26:59.640 --> 00:27:03.200
<v Speaker 1>genius to the science of light and vision. In sixteen

411
00:27:03.200 --> 00:27:06.240
<v Speaker 1>o four he published additions to Matello in which the

412
00:27:06.279 --> 00:27:09.839
<v Speaker 1>optical part of astronomy is taught. Often known more simply

413
00:27:09.920 --> 00:27:14.839
<v Speaker 1>as astronomy pars optica, this tone was a truly groundbreaking

414
00:27:14.880 --> 00:27:19.000
<v Speaker 1>work on optical signs. Kepler built upon the medieval optics

415
00:27:19.039 --> 00:27:23.039
<v Speaker 1>of al Hahazan and Wtello, but he far surpassed his predecessors,

416
00:27:23.319 --> 00:27:27.319
<v Speaker 1>earning the title of father of modern optics. An Astronomy

417
00:27:27.400 --> 00:27:31.200
<v Speaker 1>pars optica, Kepler essentially founded the modern understanding of how

418
00:27:31.240 --> 00:27:36.319
<v Speaker 1>we see and how light behaves light intensity. He formulated

419
00:27:36.359 --> 00:27:40.240
<v Speaker 1>the inverse square law of light propagation, recognizing that the

420
00:27:40.240 --> 00:27:43.079
<v Speaker 1>apparent brightness of a light source decreases with the square

421
00:27:43.119 --> 00:27:47.680
<v Speaker 1>of the distance. This was a critical insight for astronomy, explaining,

422
00:27:47.720 --> 00:27:51.839
<v Speaker 1>for example, the dwindling light of distant stars that we

423
00:27:51.920 --> 00:27:56.319
<v Speaker 1>have reflection and pinhole images. Kepler systematically described the behavior

424
00:27:56.359 --> 00:27:59.960
<v Speaker 1>of light upon reflection from flat and curved mirrors, laying

425
00:28:00.079 --> 00:28:03.960
<v Speaker 1>groundwork from mirror optics. He also explained the principles of

426
00:28:03.960 --> 00:28:08.119
<v Speaker 1>the pinhole camera, showing how a small aperture projects an

427
00:28:08.119 --> 00:28:11.839
<v Speaker 1>inverted image, an analogy that would prove vital for understanding

428
00:28:11.920 --> 00:28:18.880
<v Speaker 1>the eye's images. Then we have astronomical optics. Anticipating telescopic astronomy,

429
00:28:19.160 --> 00:28:24.200
<v Speaker 1>Kepler treated the optical phenomena affecting astronomical observation. He analyzed

430
00:28:24.200 --> 00:28:28.279
<v Speaker 1>how atmospheric refraction bends light making, for instance, the sun

431
00:28:28.319 --> 00:28:32.519
<v Speaker 1>appeared distorted near the horizon, and investigated parallax and apparent

432
00:28:32.559 --> 00:28:35.960
<v Speaker 1>sizes of celestial bodies. By doing so, he made it

433
00:28:36.000 --> 00:28:39.960
<v Speaker 1>clear that astronomical sightings must account for optical efforts, hence

434
00:28:39.960 --> 00:28:45.000
<v Speaker 1>the book's subtitle, The Optical Part of Astronomy. He touched

435
00:28:45.000 --> 00:28:48.279
<v Speaker 1>on the vision of the eye. Most famously, Kepler solved

436
00:28:48.279 --> 00:28:51.839
<v Speaker 1>the age old riddle of how vision works. Rejecting h

437
00:28:51.920 --> 00:28:55.079
<v Speaker 1>and ideas that the eye emits visual rays, Kepler proved

438
00:28:55.079 --> 00:28:57.599
<v Speaker 1>instead that an image of the world is formed inside

439
00:28:57.640 --> 00:29:00.559
<v Speaker 1>the eye. He was the first to understand that the

440
00:29:00.640 --> 00:29:03.279
<v Speaker 1>lens of the eye projects an inverted picture of the

441
00:29:03.319 --> 00:29:07.599
<v Speaker 1>scene into the retina. I say there is vision, Kepler wrote,

442
00:29:07.759 --> 00:29:10.519
<v Speaker 1>when a representation of the whole hemisphere of the world,

443
00:29:10.640 --> 00:29:13.920
<v Speaker 1>that is, before the eye fixes itself on the concave

444
00:29:14.000 --> 00:29:17.359
<v Speaker 1>surface of the retina. He likened the eye to a

445
00:29:17.359 --> 00:29:21.559
<v Speaker 1>camera obscurre, with the retinal image as its painting. Crucially,

446
00:29:21.680 --> 00:29:25.160
<v Speaker 1>Kepler acknowledged that although the image is inverted, the mind

447
00:29:25.240 --> 00:29:29.960
<v Speaker 1>interprets it correctly, effectively kicking off the study of physiological optics.

448
00:29:31.240 --> 00:29:35.359
<v Speaker 1>Kepler's insights into vision were revolutionary. He explained the operation

449
00:29:35.440 --> 00:29:38.680
<v Speaker 1>of corrective lenses for the first time, as well describing

450
00:29:38.680 --> 00:29:42.200
<v Speaker 1>how concave lenses diverge light for the myopic and convex

451
00:29:42.279 --> 00:29:45.559
<v Speaker 1>lenses converge light for the far sighted. This was not

452
00:29:45.599 --> 00:29:49.160
<v Speaker 1>an invention of eyeglasses, they predated him by centuries, but

453
00:29:49.200 --> 00:29:51.960
<v Speaker 1>it was the first scientific explanation of why lenses work

454
00:29:52.000 --> 00:29:56.759
<v Speaker 1>to remedy vision. For all these contributions, Kepler's sixteen oh

455
00:29:56.799 --> 00:29:59.680
<v Speaker 1>four Optica is considered a major turning point in the

456
00:29:59.720 --> 00:30:04.039
<v Speaker 1>dea development of the discipline of optics. A modern historian

457
00:30:04.079 --> 00:30:06.559
<v Speaker 1>notes that the book contains the first statement that the

458
00:30:06.640 --> 00:30:09.599
<v Speaker 1>image is created in the eye on the retina and

459
00:30:09.720 --> 00:30:14.759
<v Speaker 1>not in the crystal lens. Kepler's contemporaries were astonished his

460
00:30:14.839 --> 00:30:17.680
<v Speaker 1>work on optics was truly ahead of its time, so

461
00:30:17.839 --> 00:30:20.759
<v Speaker 1>much that Galileo, who built telescopes around the same years,

462
00:30:21.200 --> 00:30:26.079
<v Speaker 1>largely ignored these new optical insights. Nonetheless, Kepler's blend of

463
00:30:26.160 --> 00:30:29.400
<v Speaker 1>theory and practical explanation, he even delved into the phyrix

464
00:30:29.440 --> 00:30:32.799
<v Speaker 1>of camera obscurers and the nature of lenses, justifies his

465
00:30:32.920 --> 00:30:37.400
<v Speaker 1>reputation as the founder of modern optics and Kepler's own

466
00:30:37.440 --> 00:30:41.759
<v Speaker 1>delighted words. Through understanding light and vision were standing on

467
00:30:41.839 --> 00:30:48.880
<v Speaker 1>the shoulders of giants, uncovering nature's secrets with new found clarity.

468
00:30:49.599 --> 00:30:52.279
<v Speaker 1>Kepler spent the next few years preparing a major treatise

469
00:30:52.359 --> 00:30:56.119
<v Speaker 1>to announce these discoveries to the world. In sixteen oh

470
00:30:56.160 --> 00:30:59.720
<v Speaker 1>five he completed the manuscript, which, by imperial privilege he

471
00:30:59.759 --> 00:31:06.039
<v Speaker 1>taught Astronomia Nova the New Astronomy. Due to delays, including

472
00:31:06.079 --> 00:31:09.559
<v Speaker 1>legal disputes with Tycho's family over data ownership, the book

473
00:31:09.720 --> 00:31:13.720
<v Speaker 1>was not published until sixteen o nine. When it finally appeared,

474
00:31:14.039 --> 00:31:18.319
<v Speaker 1>it was nothing short of revolutionary. In it, Kepler narrates

475
00:31:18.400 --> 00:31:21.440
<v Speaker 1>in the first person the long saga of his analysis

476
00:31:21.440 --> 00:31:24.799
<v Speaker 1>of Mars, giving a candid account of false starts and

477
00:31:24.839 --> 00:31:28.720
<v Speaker 1>failed hypothesis on the weight of the truth. This was

478
00:31:28.920 --> 00:31:32.759
<v Speaker 1>the first published account wherein a scientist documents how he

479
00:31:32.839 --> 00:31:36.119
<v Speaker 1>has copied with a multitude of imperfect data to forge

480
00:31:36.160 --> 00:31:41.079
<v Speaker 1>a theory of surpassing accuracy. As historian Owen Jingerich noted

481
00:31:42.640 --> 00:31:47.200
<v Speaker 1>in essence, Kepler was practicing a modern scientific method. He

482
00:31:47.319 --> 00:31:50.440
<v Speaker 1>led observations guy theory, and he was willing to abandon

483
00:31:50.559 --> 00:31:55.200
<v Speaker 1>beautiful ideas like nested polyhedra or combinations of circles when

484
00:31:55.240 --> 00:31:59.880
<v Speaker 1>the data disproved them. He also firmly introduced physics in

485
00:32:00.079 --> 00:32:05.000
<v Speaker 1>to astronomy. In the very preface of Astronomia Nova, Keppler

486
00:32:05.039 --> 00:32:09.240
<v Speaker 1>described his work as celestial physics, an excursion into Aristotle's

487
00:32:09.279 --> 00:32:12.799
<v Speaker 1>metaphysics of motion applied to the heavens. He even likened

488
00:32:12.799 --> 00:32:16.200
<v Speaker 1>the celestial machine not to a divine living being, but

489
00:32:16.279 --> 00:32:19.440
<v Speaker 1>to a mechanical clock. My aim is to show that

490
00:32:19.480 --> 00:32:22.240
<v Speaker 1>the celestial machine is to be likened not to a

491
00:32:22.240 --> 00:32:26.599
<v Speaker 1>divine organism, but rather to a clockwork. In it, almost

492
00:32:26.640 --> 00:32:29.240
<v Speaker 1>all the varied motions are carried out by means of

493
00:32:29.279 --> 00:32:33.240
<v Speaker 1>a single, quite simple magnetic force, as in a clock,

494
00:32:33.359 --> 00:32:36.880
<v Speaker 1>all motions derived from a simple weight. He wrote this

495
00:32:37.039 --> 00:32:40.640
<v Speaker 1>metaphor of the clockwork universe driven by physical force was

496
00:32:40.680 --> 00:32:43.920
<v Speaker 1>a radical departure from the traditional view of heavenly spheres

497
00:32:43.960 --> 00:32:48.200
<v Speaker 1>moved by guided intelligences or angels. Kepler had paved the

498
00:32:48.200 --> 00:32:51.759
<v Speaker 1>way for understanding planetary motion as governed by natural law.

499
00:32:52.880 --> 00:32:56.400
<v Speaker 1>While Mars in the Astronomya nova occupied much of Kepler's

500
00:32:56.440 --> 00:32:59.640
<v Speaker 1>time in Prague, other remarkable events and works also came

501
00:32:59.720 --> 00:33:03.680
<v Speaker 1>during this period. In October sixteen oh four, a bright

502
00:33:03.720 --> 00:33:07.200
<v Speaker 1>new star appeared in the constellation of Fucus, a supernova

503
00:33:07.319 --> 00:33:11.559
<v Speaker 1>now known as Kepler's supernova. Initially skeptical of the rumors,

504
00:33:11.839 --> 00:33:15.960
<v Speaker 1>Keppeler observed it himself and began a meticulous study. This

505
00:33:16.119 --> 00:33:19.319
<v Speaker 1>new star shone for over a year before fading, and

506
00:33:19.400 --> 00:33:24.319
<v Speaker 1>it stirred fevered astrological speculation. Coincided with a great conjunction year,

507
00:33:24.599 --> 00:33:28.279
<v Speaker 1>which some took as an omen. Keppeler published a book

508
00:33:28.319 --> 00:33:31.720
<v Speaker 1>in sixteen oh six on the new star in Opfucus.

509
00:33:32.279 --> 00:33:36.960
<v Speaker 1>Analyzing the phenomenon, he demonstrated, via the lack of measurable parallax,

510
00:33:37.039 --> 00:33:39.759
<v Speaker 1>that the star was far beyond the planets in the

511
00:33:39.799 --> 00:33:43.680
<v Speaker 1>realm of the fixed stars. This provided more evidence against

512
00:33:43.720 --> 00:33:47.880
<v Speaker 1>the old Aristolian doctrine of an unchanging celestial realm. The

513
00:33:47.960 --> 00:33:51.920
<v Speaker 1>heavens could change, new stars could appear, and then vanish.

514
00:33:52.480 --> 00:33:58.400
<v Speaker 1>Keppler also cautiously addressed the astrological frenzy while cataloging others interpretations,

515
00:33:58.799 --> 00:34:02.119
<v Speaker 1>He himself remained scared reptical that the supernova herald anything

516
00:34:02.160 --> 00:34:08.880
<v Speaker 1>specific beyond the general observation that nature occasionally produces rare events. Interestingly,

517
00:34:09.360 --> 00:34:11.960
<v Speaker 1>Kepler appended to this book an essay on the Star

518
00:34:12.119 --> 00:34:16.239
<v Speaker 1>of Bethlehem, prompted by a chronology study by Laurentius Sousilia.

519
00:34:16.800 --> 00:34:20.000
<v Speaker 1>Soslieger argued that the calendar of Christ's birth was off

520
00:34:20.039 --> 00:34:25.400
<v Speaker 1>by several years, placing the Nativity around four or five BC. Kepler,

521
00:34:25.440 --> 00:34:28.199
<v Speaker 1>connecting the dots, noted that a series of great conjunctions

522
00:34:28.199 --> 00:34:32.559
<v Speaker 1>of Jupiter and Saturn occurred around seven BC. He speculated

523
00:34:32.599 --> 00:34:35.519
<v Speaker 1>that the Star of Bethlehem might have been such a conjunction,

524
00:34:35.960 --> 00:34:38.920
<v Speaker 1>possibly with a nova analogoust to the new Star of

525
00:34:38.960 --> 00:34:42.519
<v Speaker 1>sixteen oh four. This was an early example of Kepler's

526
00:34:42.559 --> 00:34:46.440
<v Speaker 1>habit of blending scientific inquiry with religious and historical questions,

527
00:34:46.840 --> 00:34:50.199
<v Speaker 1>an approach he expanded in other works on chronology. Kepler

528
00:34:50.239 --> 00:34:53.559
<v Speaker 1>also made fundamental contributions to the field of optics during

529
00:34:53.599 --> 00:34:57.639
<v Speaker 1>his produce in sixteen o nine to sixteen ten. The

530
00:34:57.679 --> 00:35:00.639
<v Speaker 1>invention of the telescope by Galileo and other opened a

531
00:35:00.679 --> 00:35:06.119
<v Speaker 1>new frontier in astronomy. Galileo's startling telescope discoveries mountains on

532
00:35:06.159 --> 00:35:09.440
<v Speaker 1>the Moon, moons around Jupiter, phases of Venus, and so on,

533
00:35:09.679 --> 00:35:15.880
<v Speaker 1>were published in March sixteen ten Insiderius Nunsius the Starry Messenger, Galileo,

534
00:35:15.960 --> 00:35:21.800
<v Speaker 1>facing skepticism, short Kepler's endorsement. Kepler responded eagerly. In April

535
00:35:21.840 --> 00:35:25.320
<v Speaker 1>sixteen ten, he wrote an open letter of support conversation

536
00:35:25.440 --> 00:35:28.840
<v Speaker 1>with Starry Messenger, in which he praised Galileo's findings and

537
00:35:28.880 --> 00:35:33.280
<v Speaker 1>speculated on what they meant for cosmology. He enthusiastically confirmed

538
00:35:33.280 --> 00:35:36.960
<v Speaker 1>that Galileo's reported phenomena were a plausible and argued readers

539
00:35:37.000 --> 00:35:41.400
<v Speaker 1>to trust the observations. Later that year, Kepler obtained a

540
00:35:41.400 --> 00:35:45.079
<v Speaker 1>telescope himself, courtesy of Duke Ernst of Cologne, and trained

541
00:35:45.079 --> 00:35:49.360
<v Speaker 1>it on Jupiter. By August sixteen ten, he had independently

542
00:35:49.440 --> 00:35:53.360
<v Speaker 1>observed Jupiter's four largest moons, and in sixteen eleven he

543
00:35:53.440 --> 00:35:58.559
<v Speaker 1>published narrative about four satellites of Jupiter observed, further validating

544
00:35:58.559 --> 00:36:03.320
<v Speaker 1>Galileo's discoveries. It was Keppler who first coined the term

545
00:36:03.480 --> 00:36:07.800
<v Speaker 1>satellite for these secondary bodies, a term still used today.

546
00:36:08.639 --> 00:36:12.599
<v Speaker 1>Kepler support was immensely valuable to Galileo, who never publicly

547
00:36:12.639 --> 00:36:17.239
<v Speaker 1>acknowledged Astronomya Nova, but certainly appreciated Kepler's championship of the

548
00:36:17.239 --> 00:36:22.840
<v Speaker 1>Copernican cause onm With Brahees unpresentedly precise observation of the planets,

549
00:36:23.119 --> 00:36:26.800
<v Speaker 1>especially Mars, Kepler spent the next decade in a tireless

550
00:36:26.920 --> 00:36:30.920
<v Speaker 1>war with Mars, an intensive battle to reconcile theory with observation.

551
00:36:32.000 --> 00:36:36.920
<v Speaker 1>The outcome was Astronomya Nova new astronomy. Kepler did not

552
00:36:37.039 --> 00:36:41.440
<v Speaker 1>stop at observations. He turned his formidable analytical skills to

553
00:36:41.519 --> 00:36:44.880
<v Speaker 1>the theory of telescopes. By late sixteen ten, he had

554
00:36:44.920 --> 00:36:48.559
<v Speaker 1>completed a manuscript on the optic of lenses and telescopic combinations.

555
00:36:49.440 --> 00:36:53.639
<v Speaker 1>In sixteen eleven, he published this work as Diaptress. In Diaptriss,

556
00:36:53.719 --> 00:36:57.800
<v Speaker 1>Kepler explained how convex and concave lenses converge a diverged light,

557
00:36:58.159 --> 00:37:01.840
<v Speaker 1>and he presented the design of a new improved telescope,

558
00:37:01.960 --> 00:37:06.440
<v Speaker 1>the Kepileririan telescope, also known as the astronomical telescope. It

559
00:37:06.559 --> 00:37:10.840
<v Speaker 1>used two convex lenses, an objective and an eyepiece, resulting

560
00:37:10.840 --> 00:37:13.559
<v Speaker 1>in a higher magnification and wider field of view than

561
00:37:13.599 --> 00:37:18.719
<v Speaker 1>Galileo's original design, which used a concave eyepiece. The trade

562
00:37:18.760 --> 00:37:22.320
<v Speaker 1>off was that the kepplerin telescope produced an inverted image,

563
00:37:22.639 --> 00:37:25.320
<v Speaker 1>but astronomers readily accepted that for the sake of the

564
00:37:25.360 --> 00:37:30.239
<v Speaker 1>better performance. Essentially, all later refracting telescopes followed Kepler's design.

565
00:37:31.159 --> 00:37:34.840
<v Speaker 1>The Optris also discussed the phenomenon of total internal reflection

566
00:37:35.239 --> 00:37:37.639
<v Speaker 1>and the optics of the human eye, making it a

567
00:37:37.719 --> 00:37:41.559
<v Speaker 1>foundational text in optical physics. By the end of his

568
00:37:41.679 --> 00:37:44.599
<v Speaker 1>Progue period, Kepler had laid out groundwork not only in

569
00:37:44.639 --> 00:37:49.119
<v Speaker 1>astronomy but in optics as well, showcasing his extraordinary broad

570
00:37:49.159 --> 00:37:53.119
<v Speaker 1>scientific reach. Now a little bit more about this book.

571
00:37:54.079 --> 00:37:57.679
<v Speaker 1>In sixteen ten, Galileo's telescope had unveiled the moons of

572
00:37:57.719 --> 00:38:01.039
<v Speaker 1>Jupiter and mountains on the Moon. This new instrument worked

573
00:38:01.079 --> 00:38:04.159
<v Speaker 1>was a mystery to most. Kepler, with his deep knowledge

574
00:38:04.199 --> 00:38:07.639
<v Speaker 1>of optics, took up the challenge. In sixteen eleven, he

575
00:38:07.639 --> 00:38:11.559
<v Speaker 1>published Diopterris, the first theoretical Treatise on the Optics of Telescopes.

576
00:38:12.360 --> 00:38:15.679
<v Speaker 1>Dioptriss Is a slim volume, but its impact was enormous.

577
00:38:16.280 --> 00:38:20.199
<v Speaker 1>It laid the theoretical foundation for the modern telescope, introducing

578
00:38:20.239 --> 00:38:23.519
<v Speaker 1>even the very term dioptrics the study of refraction that

579
00:38:23.639 --> 00:38:29.280
<v Speaker 1>we still use today. Keppeler's diopters systematically explained how lenses

580
00:38:29.320 --> 00:38:33.360
<v Speaker 1>bend in focus light to produce magnified images, something never

581
00:38:33.440 --> 00:38:37.559
<v Speaker 1>before clarified. He began by giving the first correct explanation

582
00:38:37.679 --> 00:38:41.000
<v Speaker 1>of the Dutch refracting telescope, the type invented in sixteen

583
00:38:41.000 --> 00:38:44.840
<v Speaker 1>oh eight and used by Galileo. A convex objective lens

584
00:38:44.920 --> 00:38:48.159
<v Speaker 1>gathers light from a distant object, and a concave eyepiece

585
00:38:48.239 --> 00:38:52.639
<v Speaker 1>lens spreads it into a large virtual image. More importantly,

586
00:38:53.000 --> 00:38:57.119
<v Speaker 1>Kepler didn't stop there. He imagined new designs. In a

587
00:38:57.159 --> 00:39:01.159
<v Speaker 1>stroke of genius, Dioptris proposed a telescope with two convex lenses,

588
00:39:01.360 --> 00:39:05.639
<v Speaker 1>a convex objective and a convex eyepiece. This configuration would

589
00:39:05.639 --> 00:39:08.639
<v Speaker 1>produce an inverted image, but Kepler showed it would allow

590
00:39:08.679 --> 00:39:11.840
<v Speaker 1>a much wider field of view and higher magnification the

591
00:39:11.840 --> 00:39:17.199
<v Speaker 1>Galileo's design. This Kepleriian telescope, also called the astronomical telescope,

592
00:39:17.440 --> 00:39:20.480
<v Speaker 1>is a direct ancestor of the refracting telescopes used in

593
00:39:20.559 --> 00:39:24.800
<v Speaker 1>observatories to this day. He even explored more complex arrangements,

594
00:39:24.880 --> 00:39:28.760
<v Speaker 1>for instance, adding a third convex lens to reinvert the image,

595
00:39:28.960 --> 00:39:33.199
<v Speaker 1>creating an erecting telescope for terrestrial viewing, and a rudimentary

596
00:39:33.280 --> 00:39:36.880
<v Speaker 1>version of a telephoto lens system for greater focused distance.

597
00:39:37.599 --> 00:39:40.920
<v Speaker 1>All of this was purely theoretical. Kepler himself did not

598
00:39:40.960 --> 00:39:43.960
<v Speaker 1>build these telescopes, but the designs he published were soon

599
00:39:44.039 --> 00:39:48.440
<v Speaker 1>realized by others, validating his ideas. Within a few decades,

600
00:39:48.559 --> 00:39:52.760
<v Speaker 1>the Keplerian telescope became the standard astronomical tool once lens

601
00:39:52.760 --> 00:39:56.039
<v Speaker 1>makers learned to mitigate the inverted image and lens imperfections.

602
00:39:56.800 --> 00:40:00.519
<v Speaker 1>It is remarkable that diapts also extended Kepler's investing gations

603
00:40:00.519 --> 00:40:04.320
<v Speaker 1>of vision. He revisited the problem of how lenses form images,

604
00:40:05.159 --> 00:40:09.519
<v Speaker 1>reinforcing the explanation that real inverted images or formed whether

605
00:40:09.599 --> 00:40:12.760
<v Speaker 1>in a camera or inside the eye, a concept directly

606
00:40:12.800 --> 00:40:16.079
<v Speaker 1>building on his sixteen or four optical work. In fact,

607
00:40:16.199 --> 00:40:20.360
<v Speaker 1>Kepler included an appendix responding to Galileo's reports, the narrative

608
00:40:20.400 --> 00:40:25.039
<v Speaker 1>on Galileo's Serial Messenger, in which he enthusiastically endorsed Galileo's

609
00:40:25.039 --> 00:40:28.800
<v Speaker 1>discoveries and discussed how his own optical principles could explain

610
00:40:28.840 --> 00:40:32.920
<v Speaker 1>the telescope's function. Thanks to Dioptrius, what had been a

611
00:40:32.960 --> 00:40:37.119
<v Speaker 1>magical device was put on firm scientific footing. Kepler was

612
00:40:37.159 --> 00:40:39.800
<v Speaker 1>the first to explain how lenses could be combined to

613
00:40:39.920 --> 00:40:44.480
<v Speaker 1>magnify distant objects, a theory still relevant in today's optical sciences.

614
00:40:45.480 --> 00:40:48.679
<v Speaker 1>For this, Kepler is often credited with inventing the improved

615
00:40:48.719 --> 00:40:52.239
<v Speaker 1>refracting telescope, and indeed the design he outlined is known

616
00:40:52.280 --> 00:40:55.800
<v Speaker 1>by his name. Historically, a Jesuit astronomer built the first

617
00:40:55.840 --> 00:40:59.880
<v Speaker 1>working Keplerian telescope a few years later, corroborating Kepler's design.

618
00:41:00.880 --> 00:41:04.440
<v Speaker 1>In some dioptrist transformed the telescope from a curious gadget

619
00:41:04.599 --> 00:41:08.199
<v Speaker 1>into a subject of science. It completed Kepler's trilogy of

620
00:41:08.280 --> 00:41:11.400
<v Speaker 1>optical works with the sixteen oh four Optica in sixteen

621
00:41:11.440 --> 00:41:15.239
<v Speaker 1>ten Optical part of Astronomy Supplement, securing his legacy as

622
00:41:15.239 --> 00:41:19.360
<v Speaker 1>a pioneer in both astronomy and optics. As a twenty

623
00:41:19.400 --> 00:41:22.840
<v Speaker 1>twenty five reissue of the Optus aptly noted. Kepler's work

624
00:41:22.920 --> 00:41:26.159
<v Speaker 1>introduced the design of the Keplerian telescope and coined the

625
00:41:26.280 --> 00:41:31.519
<v Speaker 1>term dioptrics, still in use today. The death of Emperor

626
00:41:31.599 --> 00:41:34.280
<v Speaker 1>Rudolph the Second in sixteen twelve and the succession of

627
00:41:34.320 --> 00:41:38.679
<v Speaker 1>Matthias marked the end of Kepler's relatively secure tenure in Prague.

628
00:41:39.519 --> 00:41:42.599
<v Speaker 1>Political and religious tensions, which had been brewing and would

629
00:41:42.599 --> 00:41:45.920
<v Speaker 1>soon ignite the Thirty Years War in sixteen eighteen, made

630
00:41:46.039 --> 00:41:52.199
<v Speaker 1>Prague increasingly inhospitable for a Protestant scientist. Furthermore, Kepler had

631
00:41:52.239 --> 00:41:56.519
<v Speaker 1>just undergone personal heartbreak. In sixteen eleven, an epidemic of

632
00:41:56.599 --> 00:42:00.360
<v Speaker 1>Hungarian spotted fever struck Prague, and Kepler's wife, Barbara fell

633
00:42:00.400 --> 00:42:04.800
<v Speaker 1>gravely ill with seizures. Though she recovered initially. That autumn,

634
00:42:04.840 --> 00:42:08.519
<v Speaker 1>all three of their children court smallpox. Six year old Frederick,

635
00:42:08.880 --> 00:42:12.880
<v Speaker 1>Kepler's oldest son, died and the other two, Susanna and Ludwig,

636
00:42:12.960 --> 00:42:16.400
<v Speaker 1>were very sick. As if these blows were not enough,

637
00:42:16.800 --> 00:42:19.519
<v Speaker 1>Keppler found himself entangled in a legal dispute over his

638
00:42:19.599 --> 00:42:22.960
<v Speaker 1>late wife's modest estate. She had a small inheritance from

639
00:42:22.960 --> 00:42:26.360
<v Speaker 1>her family. Worn out by these trials, Keppler sought to

640
00:42:26.440 --> 00:42:30.239
<v Speaker 1>leave Prague. He attempted to return to Tubingan. The Lutheran

641
00:42:30.280 --> 00:42:33.760
<v Speaker 1>authorities still there viewed him with suspicion for his theological

642
00:42:33.840 --> 00:42:37.760
<v Speaker 1>non conformity. They dubbed him too Calvinist leaning. Since Kepler

643
00:42:37.800 --> 00:42:42.159
<v Speaker 1>advocated for intercommunion between Lutherans and Calvinists, even the Duke

644
00:42:42.199 --> 00:42:46.599
<v Speaker 1>of Woodemberg turned him down on the advice of churchmen. Interestingly,

645
00:42:47.079 --> 00:42:50.039
<v Speaker 1>the University of Padawa in Italy, where Galileo had taught,

646
00:42:50.360 --> 00:42:54.679
<v Speaker 1>reached out to Kepler in sixteen eleven. Galileo himself departing

647
00:42:54.679 --> 00:42:59.280
<v Speaker 1>Padawa for Florence, had recommended Kepler as his successor. Kepler

648
00:42:59.320 --> 00:43:04.519
<v Speaker 1>considered the pristigious Padowit chair, but ultimately declined, preferring to

649
00:43:04.639 --> 00:43:07.960
<v Speaker 1>keep his family in a German Protestant region and perhaps

650
00:43:07.960 --> 00:43:10.719
<v Speaker 1>sensing that as a Protestant he might not thrive under

651
00:43:10.760 --> 00:43:15.360
<v Speaker 1>Venice's Catholic oversight. Instead, Kepler secured an appointment as a

652
00:43:15.360 --> 00:43:19.320
<v Speaker 1>provincial mathematician, similar to his old role in Gratz, in

653
00:43:19.360 --> 00:43:23.440
<v Speaker 1>the Upper Austrian city of Linz, and per Mathaeus permitted

654
00:43:23.519 --> 00:43:26.320
<v Speaker 1>Kepler to leave Prague for Lynz in sixteen twelve. While

655
00:43:26.360 --> 00:43:30.480
<v Speaker 1>technically retaining his title and Mega salary as an Imperial mathematician,

656
00:43:32.119 --> 00:43:35.199
<v Speaker 1>and would remain based there for the next fourteen years.

657
00:43:35.840 --> 00:43:39.280
<v Speaker 1>This period was marked by further personal turbulence, but also

658
00:43:39.400 --> 00:43:44.840
<v Speaker 1>major scientific achievements. In Linz, Kepler's official tasks included teaching

659
00:43:44.880 --> 00:43:48.800
<v Speaker 1>at the local gymnasium school and continuing to provide astrological

660
00:43:48.800 --> 00:43:53.559
<v Speaker 1>and astronomical services such as calendars for the province. Compared

661
00:43:53.599 --> 00:43:57.920
<v Speaker 1>to Prague, Linz offered more religious freedom at first. Matthias's

662
00:43:57.920 --> 00:44:02.079
<v Speaker 1>regime was less actively repressive in Austria, and Kepler initially

663
00:44:02.159 --> 00:44:06.119
<v Speaker 1>enjoyed the ability to practice his Lutheran faith openly. However,

664
00:44:06.199 --> 00:44:09.880
<v Speaker 1>Kepler's stubborn individualism in matters of doctrine soon caused friction

665
00:44:10.239 --> 00:44:14.239
<v Speaker 1>with the Lutheran establishment because Kepela would not affirm the

666
00:44:14.360 --> 00:44:17.840
<v Speaker 1>orthodox Lutheran view of the Eucharist. He rejected the idea

667
00:44:17.840 --> 00:44:20.840
<v Speaker 1>of Christ's physical ubiquity in the Bread and Wine, and

668
00:44:20.880 --> 00:44:23.840
<v Speaker 1>he refused to sign the strict formula of concord. The

669
00:44:23.920 --> 00:44:27.840
<v Speaker 1>Lutheran clergy excommunicated him forbidding him from the Lord's Supper

670
00:44:27.880 --> 00:44:32.039
<v Speaker 1>in sixteen thirteen. In their eyes, Kepler was a heretic

671
00:44:32.239 --> 00:44:36.719
<v Speaker 1>leaning toward Calvinism. Thus, ironically, this devout Christian found himself

672
00:44:36.760 --> 00:44:41.360
<v Speaker 1>alienated by both Protestant and Catholic authorities. Christ the Lord

673
00:44:41.639 --> 00:44:46.159
<v Speaker 1>neither is Lutheran, nor Calvinist, nor papist. Kepler once remarked,

674
00:44:46.280 --> 00:44:50.440
<v Speaker 1>urging more tolerance, his religious isolation and lens was a

675
00:44:50.440 --> 00:44:52.880
<v Speaker 1>heavy blow, but he bore it as the price of

676
00:44:52.880 --> 00:44:57.119
<v Speaker 1>intellectual honesty. Some historians see the harsh treatment Kepler received

677
00:44:57.159 --> 00:45:01.039
<v Speaker 1>from Lutheran pastors, his excommunication, and a few years later

678
00:45:01.239 --> 00:45:02.880
<v Speaker 1>the targeting of his mother as a witch in the

679
00:45:02.920 --> 00:45:06.559
<v Speaker 1>Lutheran town as indicative of the counter attack he faced

680
00:45:06.559 --> 00:45:10.760
<v Speaker 1>from his own camp for being so unorthodox. Despite these difficulties,

681
00:45:10.920 --> 00:45:15.360
<v Speaker 1>Keppela found happiness again in his personal life. His first wife, Barbara,

682
00:45:15.360 --> 00:45:18.360
<v Speaker 1>had died in Prague in sixteen eleven during the tumultuous times,

683
00:45:18.800 --> 00:45:23.039
<v Speaker 1>leaving Keppelo a widower with two surviving young children in Linz.

684
00:45:23.280 --> 00:45:26.559
<v Speaker 1>Keppler decided to remarry. His approach to finding his second

685
00:45:26.599 --> 00:45:30.840
<v Speaker 1>wife was characteristically analytical. He considered no fewer than eleven

686
00:45:30.920 --> 00:45:35.159
<v Speaker 1>potential matches, evaluating their qualities and even making a ranked list,

687
00:45:35.639 --> 00:45:38.440
<v Speaker 1>a process often cited as an early example of the

688
00:45:38.480 --> 00:45:43.480
<v Speaker 1>optimal marriage problem in decision theory. His first several choices

689
00:45:43.519 --> 00:45:48.039
<v Speaker 1>fell through. Some candidates rejected him, others redeemed unsuitable, But

690
00:45:48.119 --> 00:45:51.199
<v Speaker 1>eventually Kepler returned to one of the earliest prospects, a

691
00:45:51.239 --> 00:45:55.840
<v Speaker 1>twenty four year old named Susanna Rudinger. Susannah was not wealthy,

692
00:45:56.000 --> 00:45:58.880
<v Speaker 1>but Kepler wrote that she won me over with love,

693
00:45:59.199 --> 00:46:03.239
<v Speaker 1>humble loyalty, the economy of household diligence, and the love

694
00:46:03.360 --> 00:46:06.559
<v Speaker 1>she gave to step children. The married on October thirtieth,

695
00:46:06.679 --> 00:46:10.199
<v Speaker 1>sixteen thirteen. By all accounts, the second marriage was a

696
00:46:10.280 --> 00:46:15.000
<v Speaker 1>much happier and more stable union than Kepler's first. Susanna

697
00:46:15.039 --> 00:46:20.960
<v Speaker 1>and Joannis had six children together. Tragically, the first three, Margaretta, Regina, Catharina,

698
00:46:21.199 --> 00:46:25.880
<v Speaker 1>and Sebald, died in childhood, but the younger three, Cordula, Fridmar,

699
00:46:26.000 --> 00:46:30.599
<v Speaker 1>and Hidelbert, survived to adulthood. Through these family ups and downs,

700
00:46:30.920 --> 00:46:34.159
<v Speaker 1>Susanna provided a loving home life that sustained Kepler through

701
00:46:34.159 --> 00:46:37.519
<v Speaker 1>his later travails. Kepler resumed his scientific work with the

702
00:46:37.599 --> 00:46:40.760
<v Speaker 1>vigorant Lynds. One of his early publications there was Di

703
00:46:41.000 --> 00:46:45.119
<v Speaker 1>Vero Anno sixteen thirteen, a treatise on pinpointing the year

704
00:46:45.239 --> 00:46:49.960
<v Speaker 1>of Christ's birth. Using historical records and astronomy, the sighting

705
00:46:49.960 --> 00:46:53.599
<v Speaker 1>of Herod's death and the Star of Bethlehem calculations, Kepler

706
00:46:53.639 --> 00:46:57.239
<v Speaker 1>concluded that Jesus was born in four BC, a result

707
00:46:57.280 --> 00:47:00.880
<v Speaker 1>which is now standard in historical scholarship. He has also

708
00:47:00.960 --> 00:47:04.119
<v Speaker 1>became involved in a project to persuade the Protestant German

709
00:47:04.159 --> 00:47:08.079
<v Speaker 1>states to adopt the improved Gregorian calendar, which had been

710
00:47:08.079 --> 00:47:12.039
<v Speaker 1>introduced by the Catholic Church in fifteen eighty two. Many

711
00:47:12.159 --> 00:47:16.679
<v Speaker 1>Protestant regions were hesitant to accept a papal reform. Kepler,

712
00:47:16.880 --> 00:47:21.039
<v Speaker 1>pragmatic as ever, participated in deliberations in sixteen fifteen to

713
00:47:21.119 --> 00:47:25.079
<v Speaker 1>sixteen sixteen to show that the Gregorian calendar was scientifically

714
00:47:25.119 --> 00:47:29.320
<v Speaker 1>sound and not a tool of povery. Protestant states did

715
00:47:29.400 --> 00:47:32.880
<v Speaker 1>eventually adopt it in Germany by seventeen hundred, thanks in

716
00:47:32.960 --> 00:47:37.360
<v Speaker 1>part to such efforts. Even as Kepler published these works,

717
00:47:37.800 --> 00:47:41.280
<v Speaker 1>a dark cloud was forming on his horizon the witchcraft

718
00:47:41.280 --> 00:47:46.480
<v Speaker 1>trial of his mother Katharina. In sixteen fifteen, back in

719
00:47:46.519 --> 00:47:50.400
<v Speaker 1>Kepler's native Werdeenberg, an ugly series of accusations led to

720
00:47:50.519 --> 00:47:55.440
<v Speaker 1>Katharina Kepler, then in her seventies, being charged with practicing witchcraft.

721
00:47:56.519 --> 00:48:00.000
<v Speaker 1>The charges arose from local feuds. A woman had claimed

722
00:48:00.079 --> 00:48:03.320
<v Speaker 1>Katherina bewitched her with a potion, but in the fevered

723
00:48:03.360 --> 00:48:07.519
<v Speaker 1>atmosphere of the time, the threat was deadly serious. Dozens

724
00:48:07.519 --> 00:48:09.920
<v Speaker 1>of the lead witches were being executed in the region.

725
00:48:10.639 --> 00:48:14.960
<v Speaker 1>Kepler was horrified. In sixteen sixteen, he traveled to Wittenberg

726
00:48:15.039 --> 00:48:19.639
<v Speaker 1>to intervene on his mother's behalf. For the next several years,

727
00:48:19.679 --> 00:48:22.119
<v Speaker 1>amid his own work, he fought a legal battle to

728
00:48:22.199 --> 00:48:26.280
<v Speaker 1>save her. The trial dragged on, with Katherina imprisoned in

729
00:48:26.320 --> 00:48:31.360
<v Speaker 1>atrocious conditions from sixteen twenty to sixteen twenty one. Kepler

730
00:48:31.360 --> 00:48:35.400
<v Speaker 1>prepared an exhaustive legal defense, drawing on his scientific mind

731
00:48:35.440 --> 00:48:39.320
<v Speaker 1>to refute the ridiculous claims point by point. He even

732
00:48:39.360 --> 00:48:42.000
<v Speaker 1>invoked his knowledge of astronomy to explain that a certain

733
00:48:42.039 --> 00:48:47.039
<v Speaker 1>herb wolfbane she gathered was for legitimate medicinal use, not sorcery,

734
00:48:47.239 --> 00:48:52.079
<v Speaker 1>and the reported apparitions could be explained naturally. His efforts succeeded.

735
00:48:52.639 --> 00:48:56.639
<v Speaker 1>In late sixteen twenty, Katherina was acquitted and released, narrowly

736
00:48:56.800 --> 00:49:01.199
<v Speaker 1>escaping a possible death sentence. Kepler's de during this crisis

737
00:49:01.199 --> 00:49:04.440
<v Speaker 1>showed a very personal side of the scientist, a loving

738
00:49:04.480 --> 00:49:08.639
<v Speaker 1>son who applied reason and eloquence to combat superstition. Some

739
00:49:08.679 --> 00:49:14.440
<v Speaker 1>scholars have speculated that this episode also influenced Kepler's literary side.

740
00:49:14.480 --> 00:49:17.400
<v Speaker 1>For years, since around sixteen oh nine, Kepler had been

741
00:49:17.440 --> 00:49:21.679
<v Speaker 1>tinkering with a manuscript called Somnium the Dream, a fanciful

742
00:49:21.719 --> 00:49:24.159
<v Speaker 1>story about a voyage to the moon framed as a

743
00:49:24.199 --> 00:49:27.639
<v Speaker 1>dream narrated by a student of Tychos. In the story,

744
00:49:27.639 --> 00:49:30.320
<v Speaker 1>a which and a demon helped transport the protagonist to

745
00:49:30.360 --> 00:49:34.119
<v Speaker 1>observe Earth from the lunar surface. The Somnium was partly

746
00:49:34.159 --> 00:49:37.639
<v Speaker 1>an allegory defending Copernican astronomy by showing how the sky

747
00:49:37.679 --> 00:49:41.039
<v Speaker 1>would look from another world, thus normalizing the idea the

748
00:49:41.119 --> 00:49:45.719
<v Speaker 1>Earth as a planet, but it also contained autobiographical elements.

749
00:49:46.559 --> 00:49:49.440
<v Speaker 1>The mother of the protagonists was a wise woman clearly

750
00:49:49.440 --> 00:49:53.280
<v Speaker 1>inspired by Catherina. A distorted version of some Nium's manuscripts

751
00:49:53.280 --> 00:49:56.159
<v Speaker 1>circulated during the trial, and some have argued it might

752
00:49:56.199 --> 00:49:59.880
<v Speaker 1>have fueled the witchcraft accusations, as ignorant folk took Kepler's

753
00:49:59.880 --> 00:50:03.079
<v Speaker 1>f fictional demonology as evidence of his family dealings with

754
00:50:03.119 --> 00:50:08.719
<v Speaker 1>the occult. After Catherina's ordeal, Kepler added extensive footnotes to

755
00:50:08.800 --> 00:50:12.400
<v Speaker 1>the Somnium two hundred and twenty three, footnotes much larger

756
00:50:12.400 --> 00:50:16.599
<v Speaker 1>than the story itself, explaining the scientific content and clarifying

757
00:50:16.639 --> 00:50:19.960
<v Speaker 1>the allegory. This work, often called the first piece of

758
00:50:20.000 --> 00:50:23.599
<v Speaker 1>science fiction, was only published in sixteen thirty four, but

759
00:50:23.679 --> 00:50:26.679
<v Speaker 1>it stands today as a testament to Kepler's imaginative and

760
00:50:26.760 --> 00:50:31.639
<v Speaker 1>humanistic side. Amid these personal battles, Kepler pushed toward the

761
00:50:31.679 --> 00:50:36.199
<v Speaker 1>frontiers of astronomy. In sixteen seventeen, he began publishing parts

762
00:50:36.239 --> 00:50:40.559
<v Speaker 1>of a long promised textbook, The Epitome of Copernican Astrology.

763
00:50:41.360 --> 00:50:44.639
<v Speaker 1>The Epitome, published in three volumes between sixteen seventeen and

764
00:50:44.679 --> 00:50:48.039
<v Speaker 1>sixteen twenty one, was intended as a comprehensive guide to

765
00:50:48.159 --> 00:50:55.960
<v Speaker 1>heliocentric astronomy for the uninitiated, modeled after Maslin's old geocentric textbook. However,

766
00:50:56.000 --> 00:50:58.280
<v Speaker 1>as Kepler wrote it, it became much more than a

767
00:50:58.320 --> 00:51:03.480
<v Speaker 1>beginner's guide, the summation of his own astronomical system, including

768
00:51:03.599 --> 00:51:06.400
<v Speaker 1>all three of his planetary laws, and his attempts to

769
00:51:06.440 --> 00:51:11.679
<v Speaker 1>explain celestial motion by physical causes. The epitomey was written

770
00:51:11.719 --> 00:51:15.039
<v Speaker 1>in question and answer dialog form and was quite accessible

771
00:51:15.119 --> 00:51:19.480
<v Speaker 1>by the standards of the day. It explicitly extended Kepler's

772
00:51:19.480 --> 00:51:23.239
<v Speaker 1>first two laws previously shown from Mars, to all the planets,

773
00:51:23.239 --> 00:51:26.760
<v Speaker 1>and even to the moon and Jupiter's moons. It did

774
00:51:26.800 --> 00:51:31.000
<v Speaker 1>not mathematically derive elliptical orbits from observations, something that was

775
00:51:31.039 --> 00:51:33.519
<v Speaker 1>too complex for a handbook, but it taught readers how

776
00:51:33.519 --> 00:51:36.199
<v Speaker 1>the planets move and encouraged them to accept the Copernican

777
00:51:36.280 --> 00:51:41.760
<v Speaker 1>worldview free of ptomomaic crutches. Initially, Volume one, books through

778
00:51:41.800 --> 00:51:46.519
<v Speaker 1>one to three, was printed in sixteen seventeen, then Volume two,

779
00:51:46.519 --> 00:51:50.480
<v Speaker 1>Book four in sixteen twenty, and Volume three, Books five

780
00:51:50.559 --> 00:51:54.760
<v Speaker 1>through seven in sixteen twenty one. This staggering publication was

781
00:51:54.800 --> 00:51:58.639
<v Speaker 1>partly due to disruptions. In sixteen sixteen, the Catholic Church

782
00:51:58.719 --> 00:52:01.599
<v Speaker 1>placed all copernicuan book looks on the index of prohibited

783
00:52:01.599 --> 00:52:06.400
<v Speaker 1>books pending correction, making it dangerous to publish on Heliocentrism

784
00:52:06.719 --> 00:52:11.320
<v Speaker 1>under Catholic rule. Kepler was in Protestant territory, but he

785
00:52:11.400 --> 00:52:15.119
<v Speaker 1>still took care. After sixteen eighteen, as the Thirty Years

786
00:52:15.199 --> 00:52:20.119
<v Speaker 1>War began, even Protestant publishers grew anxious to avoid religious censure.

787
00:52:20.599 --> 00:52:24.360
<v Speaker 1>Kepler pitched the later volumes of Epittomey to more specialist readers.

788
00:52:24.719 --> 00:52:27.760
<v Speaker 1>He made the arguments more rigorous and mathematical, and even

789
00:52:27.840 --> 00:52:30.440
<v Speaker 1>left Copernican out of the titles of some parts so

790
00:52:30.599 --> 00:52:35.519
<v Speaker 1>as not to draw overt attention. Nevertheless, that Epotomy became

791
00:52:35.559 --> 00:52:39.079
<v Speaker 1>the most widely used astronomy textbook in Europe and the

792
00:52:39.159 --> 00:52:43.719
<v Speaker 1>decades after Kepler's death. Between sixteen thirty and sixteen fifty,

793
00:52:44.000 --> 00:52:47.639
<v Speaker 1>it effectively spread Kepler's ellipse based astronomy to the next

794
00:52:47.639 --> 00:52:52.039
<v Speaker 1>generation of astronomers. Many who were initially unconvinced by Kepler's

795
00:52:52.039 --> 00:52:55.440
<v Speaker 1>sixteen or nine new astronomy came to accept his models

796
00:52:55.719 --> 00:52:59.800
<v Speaker 1>through the didactic Epotomy. Thus, even if Kepler himself did

797
00:52:59.840 --> 00:53:03.719
<v Speaker 1>not converts stalwarts like Galileo, his ideas steadily permeated the

798
00:53:03.719 --> 00:53:12.320
<v Speaker 1>scientific community via this work. Kepler's other towering achievement in

799
00:53:12.320 --> 00:53:15.400
<v Speaker 1>the Linz Error was the completion of Tycho's legacy, the

800
00:53:15.480 --> 00:53:20.039
<v Speaker 1>Ridolphine Tables. These were new planetary tables and star catalog

801
00:53:20.519 --> 00:53:24.440
<v Speaker 1>named after Emperor Rudolph the Second. Since sixteen oh one,

802
00:53:24.599 --> 00:53:27.760
<v Speaker 1>Kepler had been obligated to produce them, but only in

803
00:53:27.840 --> 00:53:31.000
<v Speaker 1>Lens did he have the piece to finish the laborious calculations.

804
00:53:32.000 --> 00:53:35.559
<v Speaker 1>The project was huge, required computing the positions of the

805
00:53:35.559 --> 00:53:39.719
<v Speaker 1>planets over time, using Kepler's laws and Tycho's data, now

806
00:53:39.760 --> 00:53:44.519
<v Speaker 1>employing the latest aid logarithms. John Napier had published the

807
00:53:44.519 --> 00:53:48.320
<v Speaker 1>invention of logarithms in sixteen fourteen, and Kepler soon grasped

808
00:53:48.320 --> 00:53:52.039
<v Speaker 1>their value for reducing calculation drudgery. He even published a

809
00:53:52.039 --> 00:53:55.360
<v Speaker 1>book of logarithm tables in sixteen twenty four and developed

810
00:53:55.360 --> 00:53:59.159
<v Speaker 1>some of the underlying theory independently. By sixteen twenty three,

811
00:53:59.480 --> 00:54:03.199
<v Speaker 1>Kepler had finished the manuscript of the Ridolphine Tables. However,

812
00:54:03.239 --> 00:54:06.760
<v Speaker 1>the calamities of war delayed their printing. In sixteen twenty

813
00:54:06.800 --> 00:54:09.559
<v Speaker 1>five to twenty six, a bitter peasant uprising and the

814
00:54:09.559 --> 00:54:14.760
<v Speaker 1>invasion of imperial forces turned Upper Austria into a battleground.

815
00:54:15.000 --> 00:54:18.800
<v Speaker 1>In sixteen twenty six, rebels actually beseized Linz, and during

816
00:54:18.800 --> 00:54:21.199
<v Speaker 1>the chaos a fire broke out that burned down the

817
00:54:21.199 --> 00:54:25.039
<v Speaker 1>printing house where Kepler's tables were in press, destroying a

818
00:54:25.079 --> 00:54:28.199
<v Speaker 1>large portion of the work in progress. Keppela had to

819
00:54:28.239 --> 00:54:30.920
<v Speaker 1>start over with a new publisher and the Free City

820
00:54:30.960 --> 00:54:34.880
<v Speaker 1>of Ohm. He left Lins in late sixteen twenty six

821
00:54:35.360 --> 00:54:38.719
<v Speaker 1>as the war made it impossible to stay. Soldiers have

822
00:54:38.800 --> 00:54:41.760
<v Speaker 1>even been courted in his home, and by sixteen twenty

823
00:54:41.760 --> 00:54:45.119
<v Speaker 1>seven he succeeded in publishing the finished Radolphine Tables in

824
00:54:45.159 --> 00:54:49.480
<v Speaker 1>om These tables were a triumph four more accurate than

825
00:54:49.519 --> 00:54:53.679
<v Speaker 1>any previous. They allowed astronomers and navigators to calculate planetary

826
00:54:53.719 --> 00:54:58.760
<v Speaker 1>positions with unprecedented precision. To illustrate the power of his tables,

827
00:54:59.440 --> 00:55:02.000
<v Speaker 1>keppel U used them to predict a transit of Mercury

828
00:55:02.000 --> 00:55:05.159
<v Speaker 1>across the Sun on November seventh, sixteen thirty one, and

829
00:55:05.199 --> 00:55:07.639
<v Speaker 1>a transit of Venus in December of sixteen thirty one,

830
00:55:07.960 --> 00:55:12.320
<v Speaker 1>rare events. He sent out words to astronomers to watch. Indeed,

831
00:55:12.360 --> 00:55:15.519
<v Speaker 1>the first prediction was vindicated when the French astronomer Pierre

832
00:55:15.519 --> 00:55:20.800
<v Speaker 1>Gassendi observed Mercury's transit on the predicted date. Kepeler's table

833
00:55:20.880 --> 00:55:24.159
<v Speaker 1>slightly missed Venus transit. It happened, but was not visible

834
00:55:24.239 --> 00:55:27.960
<v Speaker 1>in most of Europe, which Gassende didn't realize. The young

835
00:55:28.000 --> 00:55:32.760
<v Speaker 1>English astronomer Jeremiah Horrocks corrected the parameters and successfully observed

836
00:55:32.800 --> 00:55:36.000
<v Speaker 1>the transit of Venus in sixteen thirty nine, further confirming

837
00:55:36.079 --> 00:55:40.599
<v Speaker 1>Kepler's system. The Adolphine tables remained the principal reference for

838
00:55:40.679 --> 00:55:44.719
<v Speaker 1>planetary motion for many decades until su planted by Newtonian

839
00:55:44.760 --> 00:55:48.480
<v Speaker 1>tables in the eighteenth century. The star catalog portion of

840
00:55:48.519 --> 00:55:52.199
<v Speaker 1>the tables contained one thousand and five stars, far more

841
00:55:52.239 --> 00:55:56.760
<v Speaker 1>than any other previous catalog, each with updated coordinates. Title's

842
00:55:56.760 --> 00:56:00.719
<v Speaker 1>original catalog had seven hundred and seventy seven stars. Kepler

843
00:56:00.760 --> 00:56:04.639
<v Speaker 1>increased it by incorporating additional observations and even some Aptolemy's

844
00:56:04.679 --> 00:56:08.639
<v Speaker 1>and Johann Bayer's entries for southern stars. It was the

845
00:56:08.719 --> 00:56:12.760
<v Speaker 1>first pre telescopic star catalog ever compiled. The positions were

846
00:56:12.800 --> 00:56:16.480
<v Speaker 1>calibrated to Tycho's precise naked eye measurements and refined by

847
00:56:16.559 --> 00:56:21.639
<v Speaker 1>Kepler's calculations, achieving accuracies of one arcminut or better from

848
00:56:21.719 --> 00:56:27.119
<v Speaker 1>many stars. Alongside the fixed stars, the Rudolphine tables provided

849
00:56:27.159 --> 00:56:31.920
<v Speaker 1>planetary tables, essentially almanac data in formulas by which one

850
00:56:31.960 --> 00:56:36.599
<v Speaker 1>to determine each planet's position on any date. These planetary

851
00:56:36.639 --> 00:56:41.079
<v Speaker 1>tables were rooted in Kepler's model heliocentric with elliptical orbits

852
00:56:41.119 --> 00:56:45.880
<v Speaker 1>and area law motion. Because of this, they dramatically outperformed

853
00:56:45.920 --> 00:56:51.199
<v Speaker 1>all the tables based on circular or geocentric models. For example,

854
00:56:51.400 --> 00:56:54.360
<v Speaker 1>the widely used Brutenic tables of the fifteen hundreds based

855
00:56:54.400 --> 00:56:58.639
<v Speaker 1>on Copernicus's circular orbits, could err by many degrees for Mars.

856
00:56:59.079 --> 00:57:02.480
<v Speaker 1>Kepler's tables using ellipses hit much closer to the mark.

857
00:57:03.280 --> 00:57:07.440
<v Speaker 1>As University of Rostock's history summary notes, the Radolphine tables

858
00:57:07.440 --> 00:57:11.039
<v Speaker 1>were considerably more precise than earli as such tables, and

859
00:57:11.159 --> 00:57:15.760
<v Speaker 1>finally made heliocentric calculations practical and trusted. In a way,

860
00:57:15.840 --> 00:57:18.840
<v Speaker 1>these tables were the proof of the pudding. If Copernicus

861
00:57:18.840 --> 00:57:22.320
<v Speaker 1>and Kepler were right, the tables would predict celestial events correctly,

862
00:57:22.599 --> 00:57:26.199
<v Speaker 1>and they did. Kepler meticulous as ever included in the

863
00:57:26.239 --> 00:57:29.000
<v Speaker 1>tables all the tools in astronomer would need. He added

864
00:57:29.079 --> 00:57:32.960
<v Speaker 1>corrections for atmospheric refraction so that users could adjust apparent

865
00:57:33.039 --> 00:57:36.400
<v Speaker 1>star and planet altitudes to true values. This was the

866
00:57:36.440 --> 00:57:39.440
<v Speaker 1>first time refraction was accounted for in such tables. He

867
00:57:39.480 --> 00:57:43.039
<v Speaker 1>also incorporated the new aid of logarithms, recently invented by

868
00:57:43.079 --> 00:57:46.679
<v Speaker 1>John Dappier, providing a table of logarithms and anti logarithms

869
00:57:46.719 --> 00:57:51.440
<v Speaker 1>to facilitate computations. This made the calculations far quicker and

870
00:57:51.559 --> 00:57:56.639
<v Speaker 1>less error prone, a very modern touch. The Redulphin Tables

871
00:57:56.679 --> 00:57:59.000
<v Speaker 1>even came with a set of instructions and examples on

872
00:57:59.039 --> 00:58:01.840
<v Speaker 1>how to use the data to determine things like planetary

873
00:58:01.880 --> 00:58:06.239
<v Speaker 1>longitudes and latitudes. Kepler included a world map with this book,

874
00:58:06.719 --> 00:58:10.119
<v Speaker 1>illustrating how one might find longitude by using lunar eclipses

875
00:58:10.320 --> 00:58:13.239
<v Speaker 1>and the tabulated positions of the moon. The road to

876
00:58:13.280 --> 00:58:17.280
<v Speaker 1>publishing the Rudolphine Tables were long and fraud Kepler inherited

877
00:58:17.320 --> 00:58:20.320
<v Speaker 1>Tycho's observational data in sixteen oh one when Tycho died,

878
00:58:20.800 --> 00:58:23.719
<v Speaker 1>under the condition that he produced the tables and credit Tycho.

879
00:58:24.719 --> 00:58:27.639
<v Speaker 1>He started the work in Prague, but soon came turmoil.

880
00:58:28.159 --> 00:58:31.440
<v Speaker 1>Emperor Rudolph the Second, who had supported the project, was deposed.

881
00:58:31.440 --> 00:58:34.840
<v Speaker 1>By sixteen twelve, Kepler lost his position in Prague and

882
00:58:34.920 --> 00:58:37.639
<v Speaker 1>had to move to Linz. The outbreak of the war

883
00:58:37.679 --> 00:58:40.199
<v Speaker 1>and personal hardships, including the witch trial of his mother

884
00:58:40.280 --> 00:58:44.360
<v Speaker 1>and the deaths of his children, delayed his progress. Moreova,

885
00:58:44.639 --> 00:58:48.760
<v Speaker 1>tycho brahes heirs hounded Kepler attempting to claim Tycho's data

886
00:58:48.840 --> 00:58:53.039
<v Speaker 1>and the profits of the tables. In letters, Kepler sometimes

887
00:58:53.039 --> 00:58:56.760
<v Speaker 1>expressed weariness at the sheer drudgery of number crunching required.

888
00:58:57.480 --> 00:59:01.440
<v Speaker 1>I beseech thee my friends do not sentenced me entirely

889
00:59:01.480 --> 00:59:05.079
<v Speaker 1>to the treadmill of mathematical computations and leave me time

890
00:59:05.119 --> 00:59:10.039
<v Speaker 1>for philosophical speculations, which are my only delight. He pleaded

891
00:59:10.039 --> 00:59:13.679
<v Speaker 1>to one impatient correspondent who pressed him for the tables. Indeed,

892
00:59:13.760 --> 00:59:17.599
<v Speaker 1>calculating and checking hundred subplanetary positions by hand was a

893
00:59:17.639 --> 00:59:21.920
<v Speaker 1>mammoth task in an error before mechanical calculators, and Kepler

894
00:59:21.960 --> 00:59:26.159
<v Speaker 1>was understandably reluctant, but his sense of duty in Tycho's

895
00:59:26.199 --> 00:59:29.719
<v Speaker 1>dying wish compelled him to finish. By sixteen twenty three,

896
00:59:29.760 --> 00:59:33.320
<v Speaker 1>he had completed the manuscript. Securing funds to publish, however,

897
00:59:33.480 --> 00:59:37.199
<v Speaker 1>was another challenge. Keppler literally chased down back pay and

898
00:59:37.239 --> 00:59:41.519
<v Speaker 1>stipends across Central Europe to finance the printing. He finally

899
00:59:41.519 --> 00:59:44.440
<v Speaker 1>gathered enough money for paper and paid the printer, largely

900
00:59:44.719 --> 00:59:48.079
<v Speaker 1>out of his own pocket. Initially, he hoped to print

901
00:59:48.079 --> 00:59:50.639
<v Speaker 1>and lens, but the city became engulfed in the chaos

902
00:59:50.639 --> 00:59:54.000
<v Speaker 1>of the Thirty Years War, so Kepler moved the operation

903
00:59:54.119 --> 00:59:57.039
<v Speaker 1>to the Free City of Ohm. There After, quarrels with

904
00:59:57.039 --> 01:00:00.000
<v Speaker 1>the printer about accuracy. The first edition of one thousand

905
01:00:00.119 --> 01:00:02.760
<v Speaker 1>copies rolled off the press in September sixteen twenty seven,

906
01:00:03.440 --> 01:00:07.159
<v Speaker 1>just in time for the Autumn Frankfurt book Fair. The

907
01:00:07.239 --> 01:00:11.760
<v Speaker 1>Radolphine Tables were immediately recognized as a monumental achievement. Astronomers

908
01:00:11.760 --> 01:00:14.679
<v Speaker 1>and navigators everywhere adopted them. For the first time, one

909
01:00:14.679 --> 01:00:18.360
<v Speaker 1>could make reliable predictions of astronomical events. Within a decade.

910
01:00:18.440 --> 01:00:21.159
<v Speaker 1>Johannes Shrek and others brought them to China, where in

911
01:00:21.199 --> 01:00:24.840
<v Speaker 1>sixteen thirty five they helped Jesuit astronomer Adam Shawl van

912
01:00:24.880 --> 01:00:30.079
<v Speaker 1>Bell reform the Chinese calendar. In essence, the Radolphine Tables

913
01:00:30.119 --> 01:00:33.239
<v Speaker 1>did more to further the acceptance of a heliosectric model

914
01:00:33.559 --> 01:00:38.039
<v Speaker 1>of the cosmos than any argument alone could. Their accuracy

915
01:00:38.119 --> 01:00:42.079
<v Speaker 1>was convincing. They remained the premier reference until mid century,

916
01:00:42.079 --> 01:00:47.239
<v Speaker 1>when newer data and eventually Newtonian theory produced better tables.

917
01:00:48.559 --> 01:00:52.199
<v Speaker 1>Kepler dedicated the work to Rudolph's successor, Emperor Ferdinand the Second,

918
01:00:52.760 --> 01:00:55.639
<v Speaker 1>since Rudolph the Second had died in sixteen twelve, but

919
01:00:55.719 --> 01:00:59.039
<v Speaker 1>he kept Rudolph's name on the title in homage. The

920
01:00:59.079 --> 01:01:02.039
<v Speaker 1>front piece of the publish book is rich in symbolism.

921
01:01:02.800 --> 01:01:07.480
<v Speaker 1>It depicts the great astronomers Hipparchus, Ptolemy, Copernicus, and Tycho

922
01:01:08.079 --> 01:01:11.440
<v Speaker 1>gathered in a grand temple of Urania views of astronomy,

923
01:01:11.760 --> 01:01:16.079
<v Speaker 1>with Kepler himself modestly represented among them. In the center,

924
01:01:16.119 --> 01:01:19.880
<v Speaker 1>Copernicus and Tycho appeared to debate, while nearby a depiction

925
01:01:19.960 --> 01:01:22.800
<v Speaker 1>of Tycho's island observatory in Kepler's model of the Solar

926
01:01:22.800 --> 01:01:27.480
<v Speaker 1>System are shown. It's essentially a monument in print celebrating

927
01:01:27.519 --> 01:01:31.199
<v Speaker 1>the triumph of precise astronomy over the skies. In triumph,

928
01:01:31.320 --> 01:01:35.920
<v Speaker 1>it was the Ridolphine Tables encapsulated Kepler's legacy. They enentrined

929
01:01:35.960 --> 01:01:39.280
<v Speaker 1>his three laws. All the calculations in the tables assumed

930
01:01:39.280 --> 01:01:43.199
<v Speaker 1>the elliptical orbits and area law timing, and they implicitly confirmed

931
01:01:43.199 --> 01:01:46.280
<v Speaker 1>the harmonic law across the planets. They proved that the

932
01:01:46.320 --> 01:01:50.920
<v Speaker 1>heliocentric cosmos was not only philosophically pleasing, but emperodically superior,

933
01:01:51.880 --> 01:01:54.440
<v Speaker 1>in a way when Newton later said, if I had

934
01:01:54.480 --> 01:01:57.639
<v Speaker 1>seen further, it is by standing on the shoulders of giants.

935
01:01:58.400 --> 01:02:01.320
<v Speaker 1>One of those giants was Kepler, and works like Rudolphine

936
01:02:01.320 --> 01:02:06.199
<v Speaker 1>tables formed the very platform in which Newton stood. Kepler,

937
01:02:06.360 --> 01:02:10.599
<v Speaker 1>through incredible perseverance, gave humanity a parting gift. The sky

938
01:02:11.199 --> 01:02:15.039
<v Speaker 1>mapped and tabulated, ready for future explorers to navigate, both

939
01:02:15.079 --> 01:02:21.280
<v Speaker 1>in reality and theory. By sixteen twenty seven, Kepler's scientific

940
01:02:21.320 --> 01:02:24.880
<v Speaker 1>work was essentially completed, but his personal journey was entering

941
01:02:24.920 --> 01:02:28.639
<v Speaker 1>a desperate phase. The Thirty Years War had engulfed Germany

942
01:02:28.719 --> 01:02:33.119
<v Speaker 1>and Kepler's patron, Emperor Ferdinand the Second, who had succeeded Matthaeus,

943
01:02:33.639 --> 01:02:37.840
<v Speaker 1>who had little interest in supporting a Protestant mathematician. Kepler

944
01:02:37.840 --> 01:02:40.119
<v Speaker 1>had also lost his position in Lins when he left.

945
01:02:40.679 --> 01:02:44.239
<v Speaker 1>Now effectively unemployed with a family to support, Kepler wandered

946
01:02:44.239 --> 01:02:47.159
<v Speaker 1>in search of a new patron. He found temporary refuge

947
01:02:47.199 --> 01:02:50.480
<v Speaker 1>at the court of Albert von Wallenstein, the famous and

948
01:02:50.559 --> 01:02:55.119
<v Speaker 1>infamous general of the Imperial Armies. Lollenstein was a cultured

949
01:02:55.159 --> 01:02:58.280
<v Speaker 1>man with an interest in astrology. He believed importance and

950
01:02:58.360 --> 01:03:02.280
<v Speaker 1>sought advice from astrologers. In sixteen twenty eight, Wallenstein invented

951
01:03:02.360 --> 01:03:05.840
<v Speaker 1>Kepler to his estate and Saggin. Kepler spent some time

952
01:03:05.880 --> 01:03:09.360
<v Speaker 1>as an adviser in Wallenstein's service, casting horoscopes and providing

953
01:03:09.400 --> 01:03:13.239
<v Speaker 1>astronomical Council, yet this was not a long term solution.

954
01:03:13.840 --> 01:03:17.800
<v Speaker 1>In sixteen thirty, hearing that an Imperial diet Assembly would

955
01:03:17.840 --> 01:03:21.719
<v Speaker 1>meet at Regensburg, Kepler decided to attend, hoping to petition

956
01:03:21.760 --> 01:03:23.960
<v Speaker 1>for the payment of back salary still owed to him

957
01:03:24.000 --> 01:03:27.559
<v Speaker 1>from his imperial post years before. It was a risky

958
01:03:27.639 --> 01:03:31.280
<v Speaker 1>journey given the wartime conditions, but Kepler was determined he

959
01:03:31.400 --> 01:03:35.559
<v Speaker 1>had endured financial struggles for too long. He arrived at

960
01:03:35.559 --> 01:03:40.559
<v Speaker 1>Regensburg in Bavaria in October sixteen thirty. There, exhausted from

961
01:03:40.639 --> 01:03:43.800
<v Speaker 1>travel and the distresses of previous years, Kepler fell ill

962
01:03:43.840 --> 01:03:47.159
<v Speaker 1>with the fever, possibly a tropical fever or simply a

963
01:03:47.199 --> 01:03:52.639
<v Speaker 1>feverish cold that turned deadly. On November fifteenth, sixteen thirty,

964
01:03:52.840 --> 01:03:56.400
<v Speaker 1>at the age of fifty eight, Johannes Kepler died in Regensburg.

965
01:03:57.559 --> 01:03:59.840
<v Speaker 1>I used to measure the heavens now. I measure the

966
01:03:59.840 --> 01:04:03.280
<v Speaker 1>shit shadows of the earth. Although my mind was sky bound.

967
01:04:03.840 --> 01:04:07.159
<v Speaker 1>The shadow of my body lies here, reads the epithaph

968
01:04:07.280 --> 01:04:12.559
<v Speaker 1>Kepler composed for himself. Because of ongoing conflict, Kepler's grave

969
01:04:12.599 --> 01:04:15.599
<v Speaker 1>in Regionsburg was neglected and within a few years was destroyed.

970
01:04:16.079 --> 01:04:19.559
<v Speaker 1>The churchyard was ravaged during the war. Thus no physical

971
01:04:19.599 --> 01:04:23.000
<v Speaker 1>monument remained at his burial site. But Kepler's true monument

972
01:04:23.039 --> 01:04:26.079
<v Speaker 1>was his scientific legacy, which soon spread across Europe and

973
01:04:26.199 --> 01:04:30.159
<v Speaker 1>stands to this day. Kepler's contributions to knowledge were vest

974
01:04:30.280 --> 01:04:33.800
<v Speaker 1>and varied. He is most celebrated for the three laws

975
01:04:33.800 --> 01:04:37.880
<v Speaker 1>of planetary motion, which can be summarized as follows. One

976
01:04:38.360 --> 01:04:42.519
<v Speaker 1>planets move in ellipses with the Sun at one focus. Two,

977
01:04:43.119 --> 01:04:46.400
<v Speaker 1>a planet sweeps out equal areas in equal times. Its

978
01:04:46.440 --> 01:04:49.199
<v Speaker 1>speed varies such that it covers the same area segment

979
01:04:49.480 --> 01:04:52.800
<v Speaker 1>of its orbit in a given time. And three, the

980
01:04:52.840 --> 01:04:55.599
<v Speaker 1>square of a planet's orbital period is proportional to the

981
01:04:55.599 --> 01:04:59.280
<v Speaker 1>cube of its average distance from the Sun. These laws

982
01:04:59.320 --> 01:05:02.360
<v Speaker 1>emperiodically to arrived by Kepler from Tycho's data, with the

983
01:05:02.400 --> 01:05:06.639
<v Speaker 1>first natural laws of astronomy, universal precise and expressed in

984
01:05:06.719 --> 01:05:11.000
<v Speaker 1>mathematical form. Kepler published the first two laws in Astromy

985
01:05:11.039 --> 01:05:13.360
<v Speaker 1>and Nova in sixteen o nine, and the third low

986
01:05:13.400 --> 01:05:17.239
<v Speaker 1>a decade later, in Harmonix Monday in sixteen nineteen. It

987
01:05:17.320 --> 01:05:20.800
<v Speaker 1>is hard to overstate how revolutionary they were. They swept

988
01:05:20.800 --> 01:05:24.320
<v Speaker 1>away the complicated epicycles of ptolemaic astronomy and even the

989
01:05:24.360 --> 01:05:28.599
<v Speaker 1>circular orbits of Copernicus, replacing them with a simple, elegant

990
01:05:28.679 --> 01:05:33.719
<v Speaker 1>geometric description that actually matched the heavens. By introducing physical

991
01:05:33.760 --> 01:05:37.760
<v Speaker 1>causality into celestial motions, Kepler also bridged the gap between

992
01:05:37.760 --> 01:05:42.039
<v Speaker 1>astronomy and physics, which had been separate disciplines. This was

993
01:05:42.079 --> 01:05:45.280
<v Speaker 1>considered impious or at least rash by some of his contemporaries.

994
01:05:45.960 --> 01:05:49.079
<v Speaker 1>Kepler's own teacher, Maslin, objected to the idea that the

995
01:05:49.159 --> 01:05:52.559
<v Speaker 1>heavens were mechanical rather than ruled by divine spheres, but

996
01:05:52.800 --> 01:05:56.039
<v Speaker 1>in hindsight, Kepler's approach was a critical step toward the

997
01:05:56.039 --> 01:05:59.840
<v Speaker 1>modern scientific method. Later physicists like Newton would build directly

998
01:05:59.840 --> 01:06:03.880
<v Speaker 1>on Keppler's laws. Famously, Newton proved in sixteen eighty seven

999
01:06:03.920 --> 01:06:06.639
<v Speaker 1>that if gravity poll's planets towards the Sun with an

1000
01:06:06.639 --> 01:06:11.760
<v Speaker 1>inverse square force, then Kepler's laws necessarily follow. Kepler's work

1001
01:06:11.800 --> 01:06:14.760
<v Speaker 1>thus provided one of the key foundations for the concept

1002
01:06:14.800 --> 01:06:21.239
<v Speaker 1>of universal gravitation. Beyond the planetary laws, Kepler achieved many

1003
01:06:21.239 --> 01:06:24.360
<v Speaker 1>firsts and science in the field of optics. He was

1004
01:06:24.400 --> 01:06:26.719
<v Speaker 1>the first to explain how a telescope works and to

1005
01:06:26.760 --> 01:06:30.880
<v Speaker 1>design the improved keppellarian telescope with two convex lenses that

1006
01:06:31.000 --> 01:06:34.599
<v Speaker 1>became the standard for astronomical refractors. He was the first

1007
01:06:34.679 --> 01:06:37.920
<v Speaker 1>to correctly describe the formation of real, virtual, upright and

1008
01:06:37.960 --> 01:06:41.800
<v Speaker 1>inverted images by lenses. He elucidated the role of the

1009
01:06:41.840 --> 01:06:45.519
<v Speaker 1>retina envision, recognizing that the eyes lens projects an inverted

1010
01:06:45.559 --> 01:06:50.000
<v Speaker 1>image on it. He investigated pinhole cameras and mirror reflections,

1011
01:06:50.079 --> 01:06:53.760
<v Speaker 1>laying the groundwork from modern optics so much that Ashroomapar's

1012
01:06:53.800 --> 01:06:58.320
<v Speaker 1>optica had been called the foundation of modern optics. In mathematics,

1013
01:06:58.400 --> 01:07:02.559
<v Speaker 1>Kepler's sixteen fifteen book New Stereometry of Wine Barrels was

1014
01:07:02.559 --> 01:07:05.039
<v Speaker 1>a study in measuring the volume of barrels by thinking

1015
01:07:05.039 --> 01:07:08.239
<v Speaker 1>of them as stacks of cross sectional discs, an approach

1016
01:07:08.320 --> 01:07:12.519
<v Speaker 1>that anticipated the development of integral calculus. Kepler's work on

1017
01:07:12.599 --> 01:07:15.800
<v Speaker 1>volume in the method of indivisibles would later inspire Cavaliery

1018
01:07:16.159 --> 01:07:19.960
<v Speaker 1>and indirectly Libyans in the creation of calculus. Now a

1019
01:07:19.960 --> 01:07:22.400
<v Speaker 1>little bit more about this book of measuring wine barrels.

1020
01:07:23.400 --> 01:07:27.800
<v Speaker 1>Amid his astronomical endeavors, Keppler also produced a gem in mathematics,

1021
01:07:28.639 --> 01:07:31.440
<v Speaker 1>one born from a practical problem that literally rolled into

1022
01:07:31.440 --> 01:07:36.000
<v Speaker 1>his life. In sixteen thirteen, while living in Linz, Kepler remarried.

1023
01:07:37.079 --> 01:07:39.639
<v Speaker 1>As the story goes, he purchased a large barrel of

1024
01:07:39.679 --> 01:07:42.760
<v Speaker 1>local wine for the wedding festivities, But the wine merchant's

1025
01:07:42.880 --> 01:07:45.960
<v Speaker 1>method of gauging the barrel's volume struck Kepler as crude

1026
01:07:45.960 --> 01:07:49.559
<v Speaker 1>and likely inaccurate. The merchant had simply inserted a rod

1027
01:07:49.599 --> 01:07:51.960
<v Speaker 1>through the whole and measured the phil height to set

1028
01:07:51.960 --> 01:07:56.199
<v Speaker 1>the price, and irked Kepler suspected the gaging stick method

1029
01:07:56.239 --> 01:07:59.639
<v Speaker 1>did not properly account for the barrel's shape. Could a

1030
01:07:59.719 --> 01:08:02.800
<v Speaker 1>short squad barrel and a toll skinny barrel of equal

1031
01:08:02.880 --> 01:08:06.960
<v Speaker 1>rod measurement really hold the same volume? Rather than shrug

1032
01:08:07.000 --> 01:08:10.519
<v Speaker 1>it off, the ever curious mathematicians saw a challenge. This

1033
01:08:10.679 --> 01:08:14.039
<v Speaker 1>wine barrel incident inspired Kepler to delve into the mathematics

1034
01:08:14.039 --> 01:08:16.600
<v Speaker 1>of volumes and led him to write this book. In

1035
01:08:16.680 --> 01:08:19.760
<v Speaker 1>doing so, Kepler made one of the earliest contributions to

1036
01:08:19.800 --> 01:08:23.479
<v Speaker 1>what would later be known as integral calculus. Despite its origin,

1037
01:08:23.880 --> 01:08:26.600
<v Speaker 1>this book is a serious work of mathematics. In it,

1038
01:08:26.680 --> 01:08:30.199
<v Speaker 1>Kepler develops a systematic method for calculating areas and volumes

1039
01:08:30.439 --> 01:08:33.359
<v Speaker 1>by an approach that foreshadows the use of infinite tesimals.

1040
01:08:33.840 --> 01:08:37.960
<v Speaker 1>He essentially resurrects and extends the methods of Archimedes, imagining

1041
01:08:38.039 --> 01:08:40.640
<v Speaker 1>shapes to be divided into an infinite number of very

1042
01:08:40.680 --> 01:08:44.199
<v Speaker 1>thin cross sections or indivisibles that can be summed to

1043
01:08:44.359 --> 01:08:48.960
<v Speaker 1>find volume. Kepler begins with simple cases, like the area

1044
01:08:49.000 --> 01:08:52.239
<v Speaker 1>of a circle, which he conceies as made of infinitely

1045
01:08:52.319 --> 01:08:56.319
<v Speaker 1>many triangular wedges, yielding the classic area of formula, and

1046
01:08:56.399 --> 01:09:00.319
<v Speaker 1>then tackles more complex three D solids. A large portion

1047
01:09:00.399 --> 01:09:03.640
<v Speaker 1>of the book is devoted to solids of revolution shapes

1048
01:09:03.720 --> 01:09:06.079
<v Speaker 1>like barrels, which can be generated by rotating a curve

1049
01:09:06.119 --> 01:09:09.960
<v Speaker 1>around an axis. Kepler computed or estimated the volumes of

1050
01:09:10.000 --> 01:09:14.560
<v Speaker 1>over ninety different such solids, ranging from cylinders and spheres

1051
01:09:14.920 --> 01:09:18.920
<v Speaker 1>to ellipsoids and toroids. In each case, he conceptually sliced

1052
01:09:18.960 --> 01:09:23.039
<v Speaker 1>the solid into infinitesimal disks or washes, summed their volumes,

1053
01:09:23.039 --> 01:09:25.600
<v Speaker 1>and arrived at results that are equivalent to what integral

1054
01:09:25.640 --> 01:09:31.479
<v Speaker 1>calculus would give, though he lacked our notion. For example,

1055
01:09:31.560 --> 01:09:33.640
<v Speaker 1>he found the volume of his sphere by summing the

1056
01:09:33.680 --> 01:09:36.439
<v Speaker 1>volumes of an infinite number of thin cones covering it,

1057
01:09:37.119 --> 01:09:41.399
<v Speaker 1>reaching the correct formula. Such reasoning was revolutionary for the time.

1058
01:09:41.800 --> 01:09:46.359
<v Speaker 1>Mathematicians would only much later formalize it. As historians C. H.

1059
01:09:46.560 --> 01:09:49.800
<v Speaker 1>Edwards noted, Kepela's approach in his stereometry was to dissect

1060
01:09:49.800 --> 01:09:52.960
<v Speaker 1>a given solid into an infinite number of infinite tesimal

1061
01:09:53.000 --> 01:09:57.680
<v Speaker 1>pieces convenient to the problem, then add them up. In

1062
01:09:57.720 --> 01:10:01.079
<v Speaker 1>other words, Kepler was doing calculus beforecklace had been invented.

1063
01:10:01.800 --> 01:10:03.800
<v Speaker 1>Little wondered that this work is regarded as one of

1064
01:10:03.880 --> 01:10:07.079
<v Speaker 1>the most significant works in the prehistory of calculus, and

1065
01:10:07.199 --> 01:10:10.079
<v Speaker 1>Kepler is counted among the forerunners of Newton and Libens

1066
01:10:10.119 --> 01:10:14.119
<v Speaker 1>in this domain. This book did not stop a theory.

1067
01:10:14.800 --> 01:10:18.039
<v Speaker 1>Returning to the wine barrels, Kepler applied his methods to

1068
01:10:18.079 --> 01:10:21.239
<v Speaker 1>find out how to accurately measure their volume. He introduced

1069
01:10:21.239 --> 01:10:24.439
<v Speaker 1>the concept of a measuring rod calibrated not just by length,

1070
01:10:24.760 --> 01:10:28.479
<v Speaker 1>but by the barrel's geometry. He computed volumes for different

1071
01:10:28.479 --> 01:10:32.359
<v Speaker 1>barrel shapes, and even posed an optimization problem. Given a

1072
01:10:32.359 --> 01:10:35.800
<v Speaker 1>certain amount of wood a fixed barrel, diagonal or circumference,

1073
01:10:36.239 --> 01:10:38.960
<v Speaker 1>what barrel shape like the ratio of height to diameter

1074
01:10:39.319 --> 01:10:42.840
<v Speaker 1>yields the maximum volume. This was essentially a problem with

1075
01:10:42.920 --> 01:10:47.880
<v Speaker 1>differential calculus, finding a maximum of a continuous function. Kepler

1076
01:10:47.920 --> 01:10:51.199
<v Speaker 1>approached it by intelligent trial. He determined that a barrel

1077
01:10:51.199 --> 01:10:53.600
<v Speaker 1>of a certain squad proportion held the most wine for

1078
01:10:53.680 --> 01:10:57.119
<v Speaker 1>its size. He discovered, in fact, that the merchant's preferred

1079
01:10:57.119 --> 01:11:01.880
<v Speaker 1>barrel design was nearly optimal, which, despite minor differences, vindicated

1080
01:11:01.920 --> 01:11:06.520
<v Speaker 1>the merchant's practice in a way much to Kepler's amusement. Thus,

1081
01:11:06.640 --> 01:11:10.640
<v Speaker 1>Kepler's annoyance turned into insight. He showed the merchant's method

1082
01:11:10.760 --> 01:11:13.279
<v Speaker 1>was not widely wrong, but he offered a far more

1083
01:11:13.399 --> 01:11:16.960
<v Speaker 1>rigorous way to get it right. In the process, he

1084
01:11:17.079 --> 01:11:20.680
<v Speaker 1>essentially formulated what later became known as Kepler's rule for volume,

1085
01:11:21.039 --> 01:11:25.439
<v Speaker 1>an early numerical integration scheme for solids of revolution. To

1086
01:11:25.520 --> 01:11:29.079
<v Speaker 1>share the practical benefits, Kepler even published a short German

1087
01:11:29.119 --> 01:11:32.600
<v Speaker 1>pamphlet in sixteen sixteen explaining the new measuring rules for

1088
01:11:32.680 --> 01:11:36.640
<v Speaker 1>artisans and wine cellars. In summary, this book stands out

1089
01:11:36.680 --> 01:11:40.880
<v Speaker 1>as a brilliant example of Kepler's versatility. Known primarily as

1090
01:11:40.920 --> 01:11:44.359
<v Speaker 1>an astronomer, here Kepler behaves as a true mathematician and

1091
01:11:44.479 --> 01:11:48.399
<v Speaker 1>even an innovator in engineering. He brings the abstract to

1092
01:11:48.439 --> 01:11:51.600
<v Speaker 1>the every day. From calculating a circle's area to determine

1093
01:11:51.600 --> 01:11:55.880
<v Speaker 1>how much wine is in a barrel, all with unprecedented thoroughness.

1094
01:11:56.399 --> 01:11:59.600
<v Speaker 1>As one article puts it, Kepler's work is a systematic

1095
01:11:59.640 --> 01:12:03.279
<v Speaker 1>work the calculation of areas and volumes by infinitesimal techniques.

1096
01:12:04.199 --> 01:12:08.239
<v Speaker 1>Today we use integral calculus to solve these kinds of problems.

1097
01:12:08.319 --> 01:12:11.680
<v Speaker 1>In bridging the gap between Archimedes and modern calculus, Keppel

1098
01:12:11.760 --> 01:12:14.479
<v Speaker 1>once again showed his conviction that nature, whether in the

1099
01:12:14.520 --> 01:12:18.600
<v Speaker 1>heavens or the Cooper's workshop, runs by noble mathematical rules,

1100
01:12:19.439 --> 01:12:21.880
<v Speaker 1>and in doing so he made even the measurement of

1101
01:12:21.960 --> 01:12:25.720
<v Speaker 1>wine an episode in the story of scientific progress. Keppel

1102
01:12:25.760 --> 01:12:29.680
<v Speaker 1>also independently devised a system of logarithms. After Napia's invention,

1103
01:12:30.039 --> 01:12:32.920
<v Speaker 1>Keblisch published his own table of logarithms and contributed to

1104
01:12:32.960 --> 01:12:36.960
<v Speaker 1>their theoretical basis. Keppel published his own table of logarithms

1105
01:12:36.960 --> 01:12:42.560
<v Speaker 1>and contributed to their theoretical basis. In geometrical crystallography, Kepler

1106
01:12:42.600 --> 01:12:46.319
<v Speaker 1>wrote the first scientific essay on snowflakes, A New Year's

1107
01:12:46.319 --> 01:12:50.560
<v Speaker 1>Gift of Hexagonal Snow, in sixteen eleven. In this charming booklet,

1108
01:12:50.880 --> 01:12:54.600
<v Speaker 1>he asked why snowflakes always formed six cornered hexagonal symmetry.

1109
01:12:55.079 --> 01:12:58.399
<v Speaker 1>He mused that nature must arrange small spherical particles in

1110
01:12:58.439 --> 01:13:01.920
<v Speaker 1>the most efficient way, and conjecture that the densest weight

1111
01:13:01.960 --> 01:13:05.680
<v Speaker 1>to pack equals spheres is in a pyramidal lattice, essentially

1112
01:13:05.720 --> 01:13:09.840
<v Speaker 1>stating that kepler conjecture about sphere packing. This conjecture remained

1113
01:13:09.920 --> 01:13:13.199
<v Speaker 1>unproven until nineteen ninety eight. Over three hundred and seventy

1114
01:13:13.239 --> 01:13:17.399
<v Speaker 1>eight years later, an astronomy proper Kepler made the first

1115
01:13:17.439 --> 01:13:20.800
<v Speaker 1>scientific attempt to measure the distance to the stars using parallax.

1116
01:13:21.279 --> 01:13:24.520
<v Speaker 1>He reasoned that if Earth's orbit produces no detectable parallax

1117
01:13:24.560 --> 01:13:28.119
<v Speaker 1>shift in star's positions, the stars must be extremely far away.

1118
01:13:29.119 --> 01:13:32.159
<v Speaker 1>He correctly attributed the tides mainly to the Moon's influence,

1119
01:13:32.399 --> 01:13:35.880
<v Speaker 1>a notion Galileo actually ridiculed at the time, and he

1120
01:13:35.960 --> 01:13:38.640
<v Speaker 1>was the first to realize that the Sun itself rotates

1121
01:13:38.640 --> 01:13:42.319
<v Speaker 1>on an axis, noticing that sun spots, whose discovery by

1122
01:13:42.359 --> 01:13:45.319
<v Speaker 1>others in sixteen ten to sixteen eleven he followed closely

1123
01:13:45.720 --> 01:13:50.600
<v Speaker 1>must imply the Sun's spins. He even coined the words satellite.

1124
01:13:50.880 --> 01:13:53.600
<v Speaker 1>In a sixteen eleven pamphlet, he introduced a term for

1125
01:13:53.720 --> 01:13:57.119
<v Speaker 1>Jupiter's moons, drawing on the idea of attendant followers of

1126
01:13:57.119 --> 01:14:00.800
<v Speaker 1>a planet. So many modern concepts and turn hormonologies can

1127
01:14:00.840 --> 01:14:04.640
<v Speaker 1>be traced to Kepler's fertile mind. So many modern concepts

1128
01:14:04.640 --> 01:14:08.720
<v Speaker 1>and terminologies can be traced back to Kepler. Little wonder

1129
01:14:08.800 --> 01:14:10.880
<v Speaker 1>that he is regarded as one of the founding figures

1130
01:14:10.880 --> 01:14:14.840
<v Speaker 1>of modern astronomy, physics, and science. Yet Keppler was not

1131
01:14:14.880 --> 01:14:17.800
<v Speaker 1>a modern scientist in the narrow sense of excluding metaphysics

1132
01:14:17.880 --> 01:14:21.319
<v Speaker 1>or spirituality. He was a man of the Late Renaissance,

1133
01:14:21.520 --> 01:14:25.399
<v Speaker 1>steeped in Neoplatonism, biblical theory, and even a dose of mysticism.

1134
01:14:26.000 --> 01:14:29.840
<v Speaker 1>Understanding Keppler's philosophy and mysticism is essential to understanding the man.

1135
01:14:30.560 --> 01:14:36.079
<v Speaker 1>He saw mathematics, particularly geometry, as holy. Geometry is one

1136
01:14:36.119 --> 01:14:39.600
<v Speaker 1>an eternal a reflection of the mind of God. That

1137
01:14:39.680 --> 01:14:42.199
<v Speaker 1>share in it accorded to humans is one of the

1138
01:14:42.199 --> 01:14:46.520
<v Speaker 1>reasons that humanity is the image of God. Kepler wrote

1139
01:14:46.640 --> 01:14:49.600
<v Speaker 1>this almost mystical reverence for geometry drove him to the

1140
01:14:49.640 --> 01:14:52.479
<v Speaker 1>platonic solids model and related to the harmonies of the

1141
01:14:52.479 --> 01:14:56.359
<v Speaker 1>planetary motions. Keppeler earnestly believed that the universe is built

1142
01:14:56.359 --> 01:15:01.520
<v Speaker 1>on harmonic principles, a cosmic music. In his magnum Opus

1143
01:15:01.600 --> 01:15:04.920
<v Speaker 1>Harmony of the World. In sixteen nineteen, Kepler delved into

1144
01:15:04.920 --> 01:15:08.680
<v Speaker 1>his Pythagorean dream. He had spent years since the God

1145
01:15:08.760 --> 01:15:13.640
<v Speaker 1>Stays exploring how geometrical ratios, musical intervals, and the structure

1146
01:15:13.680 --> 01:15:17.399
<v Speaker 1>of nature might all be unified, and finally, in book five,

1147
01:15:17.560 --> 01:15:22.000
<v Speaker 1>he examines the harmony in planetary motions. There he articulates

1148
01:15:22.039 --> 01:15:25.560
<v Speaker 1>the third law in a musical context. The ratio of

1149
01:15:25.560 --> 01:15:27.800
<v Speaker 1>the square of planets periods to the cubes of their

1150
01:15:27.840 --> 01:15:31.359
<v Speaker 1>distance is the same for all planets. A silent harmony.

1151
01:15:31.960 --> 01:15:35.159
<v Speaker 1>Kepler imagined that each planet, in its swift and slow motion,

1152
01:15:35.640 --> 01:15:39.800
<v Speaker 1>analogous to high and low notes, emits a tone. At

1153
01:15:39.840 --> 01:15:45.640
<v Speaker 1>different points in their orbits. Planets sing different notes. For example, Earth,

1154
01:15:45.760 --> 01:15:49.439
<v Speaker 1>with its slightly varying speed, sings me fa me, and

1155
01:15:49.520 --> 01:15:52.680
<v Speaker 1>Kepler couldn't resist a word play. The Earth sings me

1156
01:15:53.000 --> 01:15:56.279
<v Speaker 1>fa me. So we can gather from this that misery

1157
01:15:56.359 --> 01:16:00.840
<v Speaker 1>and famine reign in our Habitat this dismal pon his side,

1158
01:16:01.079 --> 01:16:04.399
<v Speaker 1>Keppelo truly thought the celestial motions found a grand pola.

1159
01:16:05.720 --> 01:16:09.560
<v Speaker 1>This dismal ponicide. Keppelo truly thought the celestial motions formed

1160
01:16:09.560 --> 01:16:12.479
<v Speaker 1>a grand polyphony, the music of the spheres that philosophers

1161
01:16:12.479 --> 01:16:17.079
<v Speaker 1>had long hypothesized. He even identified specific musical intervals for

1162
01:16:17.119 --> 01:16:21.479
<v Speaker 1>planetary velocity ranges. For instance, Venus's speed range formed a

1163
01:16:21.520 --> 01:16:25.359
<v Speaker 1>nearly perfect fifth, Earth, a minor third, and so on.

1164
01:16:25.760 --> 01:16:28.560
<v Speaker 1>He had some rivalry with the English neoplatonist Robert Flood

1165
01:16:28.560 --> 01:16:31.720
<v Speaker 1>on these matters. Flood published his own harmonic theory around

1166
01:16:31.760 --> 01:16:34.800
<v Speaker 1>the same time, and Kepler sharply criticized Flood for being

1167
01:16:34.840 --> 01:16:39.199
<v Speaker 1>speculative and numerological. But whereas Flood's harmonies were tied to

1168
01:16:39.239 --> 01:16:43.800
<v Speaker 1>astrological mysticism, Kepler's were anchored in data. He quantified the

1169
01:16:43.840 --> 01:16:47.399
<v Speaker 1>angles and speeds. In the end, this book gave the

1170
01:16:47.399 --> 01:16:50.000
<v Speaker 1>world the Third Law. But it also stands as a

1171
01:16:50.039 --> 01:16:53.800
<v Speaker 1>testament to Kepler's metaphysical vision, a universe where mathematical beauty

1172
01:16:53.880 --> 01:16:57.159
<v Speaker 1>is not just aesthetic but real, where the celestial machine

1173
01:16:57.199 --> 01:16:59.239
<v Speaker 1>is not a kind of divine organism but a kind

1174
01:16:59.279 --> 01:17:03.000
<v Speaker 1>of clockwork created by God, and yet that clockwork produces

1175
01:17:03.039 --> 01:17:07.800
<v Speaker 1>a wondrous harmony perceptible to the intellect. Some say this

1176
01:17:07.840 --> 01:17:11.199
<v Speaker 1>book often reads like a hymn. Kepler's joy and reverence

1177
01:17:11.239 --> 01:17:14.159
<v Speaker 1>burst forth in the final pages as he addresses the divine.

1178
01:17:15.359 --> 01:17:18.239
<v Speaker 1>The heavenly bodies are nothing but a continuous song for

1179
01:17:18.359 --> 01:17:22.600
<v Speaker 1>several voices, perceived not by the year, but by the intellect,

1180
01:17:23.199 --> 01:17:27.199
<v Speaker 1>a music which sets landmarks in the immeasurable flow of time.

1181
01:17:28.079 --> 01:17:32.119
<v Speaker 1>It is no longer surprising that man, an imitation of

1182
01:17:32.159 --> 01:17:36.079
<v Speaker 1>his creator, has at last discovered the art of figured song.

1183
01:17:37.399 --> 01:17:41.239
<v Speaker 1>And even in more feverent prayer, he writes, the wisdom

1184
01:17:41.279 --> 01:17:47.159
<v Speaker 1>of the Lord is infinite. Ye heavens sing his praise, sun, moon,

1185
01:17:47.279 --> 01:17:51.279
<v Speaker 1>and planets. Glorify him in your ineffable language. Praise him

1186
01:17:51.399 --> 01:17:55.720
<v Speaker 1>celestial harmonies and all ye who can comprehend them. These

1187
01:17:55.720 --> 01:17:59.520
<v Speaker 1>poetic lines show Kepler saw his scientific work as profoundly spiritual.

1188
01:18:00.239 --> 01:18:03.840
<v Speaker 1>He felt he was thinking God's thoughts after him. With

1189
01:18:04.000 --> 01:18:07.840
<v Speaker 1>the Third Law, the Copernian cosmos had a new harmonious

1190
01:18:07.920 --> 01:18:11.640
<v Speaker 1>order that only a divinely inspired geometrical mind could have arranged.

1191
01:18:12.119 --> 01:18:16.079
<v Speaker 1>Kepler's religious faith was absolutely central to his life, albeit

1192
01:18:16.119 --> 01:18:19.680
<v Speaker 1>an unorthodox one, and frequently spoke of God in his works.

1193
01:18:20.800 --> 01:18:23.960
<v Speaker 1>He saw scientific vocation as a priesthood of sorts. I

1194
01:18:24.000 --> 01:18:27.159
<v Speaker 1>am merely thinking God's thoughts after him. He is often

1195
01:18:27.239 --> 01:18:31.199
<v Speaker 1>quoted a paraphrase of his own words, He believed God

1196
01:18:31.239 --> 01:18:34.760
<v Speaker 1>has designed the cosmos according to an intelligible plan accessible

1197
01:18:34.800 --> 01:18:37.960
<v Speaker 1>through reason, since humans are made of God's image with

1198
01:18:38.039 --> 01:18:43.560
<v Speaker 1>the capacity for understanding. This theological optimism fueled Kepler's dog

1199
01:18:43.640 --> 01:18:48.960
<v Speaker 1>perseverance through years of calculation and frustration. He was convinced

1200
01:18:48.960 --> 01:18:51.680
<v Speaker 1>the underlying patterns would be simple and elegant, because a

1201
01:18:51.680 --> 01:18:56.000
<v Speaker 1>perfect God would choose a perfect geometry. His faith also

1202
01:18:56.039 --> 01:18:59.039
<v Speaker 1>made him unafraid of upevil By placing the Son at

1203
01:18:59.039 --> 01:19:01.520
<v Speaker 1>the center and Earth the moondong the planets, Keppela felt

1204
01:19:01.520 --> 01:19:05.359
<v Speaker 1>he was glorifying God's work rather than demoting Earth. In

1205
01:19:05.359 --> 01:19:07.720
<v Speaker 1>one of the beautiful passages at the end of Astronomy

1206
01:19:07.800 --> 01:19:11.279
<v Speaker 1>and Nova, after working out Mars's orbit, Keppelo offers a

1207
01:19:11.279 --> 01:19:14.479
<v Speaker 1>prayer of thanks. I feel carried away and possessed by

1208
01:19:14.520 --> 01:19:18.560
<v Speaker 1>an unutterable rapture over the divine spectacle of heavenly harmony.

1209
01:19:18.640 --> 01:19:22.359
<v Speaker 1>He exults. He expresses gratitude that God permitted him to

1210
01:19:22.359 --> 01:19:26.800
<v Speaker 1>discover truths hidden for ages. Such spiritual language runs through

1211
01:19:26.800 --> 01:19:31.000
<v Speaker 1>many of Kepler's writings. At the same time, Keppler had

1212
01:19:31.039 --> 01:19:34.479
<v Speaker 1>an eerie humanist side to his religion, Living amidst the

1213
01:19:34.560 --> 01:19:39.600
<v Speaker 1>Catholic Protestant conflict, he longed for reconciliation. As noted, Keppelo

1214
01:19:39.680 --> 01:19:43.119
<v Speaker 1>was condemned by Lutheran authorities for being soft on Calvinists.

1215
01:19:43.680 --> 01:19:47.159
<v Speaker 1>He openly argued for toleration among Christian sects. Christ the

1216
01:19:47.199 --> 01:19:50.239
<v Speaker 1>Law was neither Lutheran, nor Calvinist, nor papist, he wrote,

1217
01:19:50.560 --> 01:19:54.680
<v Speaker 1>childing partisans on all sides. This spirit won him no

1218
01:19:54.760 --> 01:19:58.319
<v Speaker 1>friends in Orthodoxy, but it speaks to Kepler's independent mind

1219
01:19:58.359 --> 01:20:02.600
<v Speaker 1>and moral courage. He managed remarkably to maintain patriots under

1220
01:20:02.640 --> 01:20:06.119
<v Speaker 1>Catholic emperors and friendships with Jesuit scientists like those who

1221
01:20:06.239 --> 01:20:09.880
<v Speaker 1>vetted his mother's trial, even as he personally remained Protestant.

1222
01:20:10.840 --> 01:20:13.279
<v Speaker 1>His ultimate loyalty was to truth as he saw it,

1223
01:20:13.800 --> 01:20:18.159
<v Speaker 1>whether in science or faith. Keppel's blend of occult and

1224
01:20:18.239 --> 01:20:21.439
<v Speaker 1>rational thinking is best illustrated by his stance on astrology

1225
01:20:21.439 --> 01:20:25.960
<v Speaker 1>and witches. As we described, Keppler practiced astrology, but sought

1226
01:20:25.960 --> 01:20:28.640
<v Speaker 1>to reform it by stripping out superstition and basing it

1227
01:20:28.680 --> 01:20:32.199
<v Speaker 1>on empirical correlations. For example, he believed the weather might

1228
01:20:32.239 --> 01:20:35.359
<v Speaker 1>be influenced by planetary aspects, and he thought the human

1229
01:20:35.359 --> 01:20:38.279
<v Speaker 1>soul could resonate with cosmic harmonies, but he mocked the

1230
01:20:38.319 --> 01:20:44.079
<v Speaker 1>simplistic horoscope predictions of quacks and his Turtius intervenians. He

1231
01:20:44.159 --> 01:20:46.920
<v Speaker 1>calls out both the thick headed band of fat bellied

1232
01:20:46.920 --> 01:20:51.560
<v Speaker 1>astrologers and those who dismiss astrology entirely, urging a middle way.

1233
01:20:52.279 --> 01:20:54.800
<v Speaker 1>To him, astrology was the vestige of an older mode

1234
01:20:54.800 --> 01:20:57.279
<v Speaker 1>of thought that could be modernized or at least used

1235
01:20:57.319 --> 01:21:02.279
<v Speaker 1>carefully regarding the occult, Keppler showed deep personal bravery in

1236
01:21:02.319 --> 01:21:06.439
<v Speaker 1>saving his mother from a witchtrial, effectively pitting scientific reasoning

1237
01:21:06.479 --> 01:21:11.520
<v Speaker 1>against fear and ignorance. After that, in the Somnium's extensive footnotes,

1238
01:21:11.760 --> 01:21:14.520
<v Speaker 1>he explained at length that what appeared as demons and

1239
01:21:14.560 --> 01:21:18.840
<v Speaker 1>spirits in his story were actually astronomical allegories or natural phenomena.

1240
01:21:19.399 --> 01:21:22.000
<v Speaker 1>For instance, he detailed the physical conditions of the moon

1241
01:21:22.079 --> 01:21:26.520
<v Speaker 1>and described how one might experience weightlessness. There all couched

1242
01:21:26.520 --> 01:21:30.199
<v Speaker 1>in a fantastical narrative as a clever literary device. It

1243
01:21:30.279 --> 01:21:32.960
<v Speaker 1>is a little wonder that some Niam earned Kepler recognition

1244
01:21:33.039 --> 01:21:36.880
<v Speaker 1>as a pregenitor of science fiction. The novel strained mixture

1245
01:21:36.880 --> 01:21:39.960
<v Speaker 1>of witchcraft in space travel mirrors Kepler's own life, striving

1246
01:21:40.000 --> 01:21:44.800
<v Speaker 1>as superstitious pass and a scientific future. Some astronomers accepted

1247
01:21:44.800 --> 01:21:48.880
<v Speaker 1>elliptical orbits but not the area law. For example, some

1248
01:21:48.960 --> 01:21:53.359
<v Speaker 1>astronomers accepted elliptical orbits but not the area law. Others,

1249
01:21:53.439 --> 01:21:56.800
<v Speaker 1>like seth Ward, tweaked Keppler's model to fit their comfort.

1250
01:21:57.199 --> 01:22:00.239
<v Speaker 1>Giants of science, such as Galileo or Renee Discards, paid

1251
01:22:00.279 --> 01:22:05.720
<v Speaker 1>surprisingly little public attention to Kepler's eschero mia nova. Galileo,

1252
01:22:05.880 --> 01:22:08.680
<v Speaker 1>though a friend and ally of Kepler in the Compernican cause,

1253
01:22:09.039 --> 01:22:13.239
<v Speaker 1>never explicitly endorsed the elliptical orbits. He stuck to circular

1254
01:22:13.319 --> 01:22:16.560
<v Speaker 1>orbits in his writings, possibly because he lacked the physics

1255
01:22:16.600 --> 01:22:21.159
<v Speaker 1>to justify ellipses. Descartes, too, formulated a cosmology of vortices

1256
01:22:21.239 --> 01:22:24.000
<v Speaker 1>that ignored Kepler's laws. It would take time and new

1257
01:22:24.079 --> 01:22:27.279
<v Speaker 1>observational proofs like the transit of mercury in sixteen thirty one,

1258
01:22:27.600 --> 01:22:31.039
<v Speaker 1>observed right on schedule by Gascinde, using Kepler's prediction, to

1259
01:22:31.159 --> 01:22:35.000
<v Speaker 1>convince the broader scientific community that Kepler's system was truly superior.

1260
01:22:35.319 --> 01:22:39.239
<v Speaker 1>The turning point arguably came with Isaac Newton. By the

1261
01:22:39.279 --> 01:22:42.600
<v Speaker 1>late seventeenth century, thinkers like Robert Hook and Giovanni Borelli

1262
01:22:42.600 --> 01:22:46.079
<v Speaker 1>were incorporating Kepler's idea of attractive forces into their theories.

1263
01:22:46.920 --> 01:22:50.199
<v Speaker 1>Newton's Percipia Mathematica in sixteen eighty seven then provided the

1264
01:22:50.279 --> 01:22:54.359
<v Speaker 1>master synthesis. It derived Kepler's three laws from a single

1265
01:22:54.439 --> 01:22:58.840
<v Speaker 1>universal law of gravitation. This not only validated Keppler's laws

1266
01:22:58.840 --> 01:23:01.600
<v Speaker 1>beyond doubt, but elevated them to the status of necessary

1267
01:23:01.640 --> 01:23:06.680
<v Speaker 1>consequences of physical principles. The problem of why planets move

1268
01:23:06.760 --> 01:23:09.560
<v Speaker 1>as they do, which Kepler could only answer with a

1269
01:23:09.680 --> 01:23:12.840
<v Speaker 1>vague motive soul or magnetic force from the Sun, was

1270
01:23:12.880 --> 01:23:17.640
<v Speaker 1>finally answered by Newton with gravity and mechanics. Newton famuously

1271
01:23:17.680 --> 01:23:21.000
<v Speaker 1>acknowledged his depth to Kepler's work, saying that by standing

1272
01:23:21.039 --> 01:23:23.920
<v Speaker 1>on the soldiers of giants like Kepler and Galileo, he

1273
01:23:24.000 --> 01:23:27.920
<v Speaker 1>could see further in solving the Kepler problem, as it

1274
01:23:27.960 --> 01:23:30.479
<v Speaker 1>came to be known, finding the forced law that gives

1275
01:23:30.560 --> 01:23:34.239
<v Speaker 1>rise to Keppeler's orbits. Newton cemented Kepler's place as a

1276
01:23:34.279 --> 01:23:39.920
<v Speaker 1>central figure in the scientific revolution. In the history and

1277
01:23:39.920 --> 01:23:44.000
<v Speaker 1>philosophy of science, Kepler's legacy has also been richly examined.

1278
01:23:44.840 --> 01:23:49.800
<v Speaker 1>Enlightenment era historians sometimes downplayed Keppler's mystical side. By contrast,

1279
01:23:50.199 --> 01:23:53.800
<v Speaker 1>nineteenth century Romantic scholars like E. F. Eppelt, who studied

1280
01:23:53.880 --> 01:23:57.800
<v Speaker 1>Kepler's unpublished manuscripts in detail, celebrated the unity of Kepler's

1281
01:23:57.840 --> 01:24:01.800
<v Speaker 1>scientific and spiritual vision. A. Pelt in eighteen forty nine

1282
01:24:02.000 --> 01:24:05.319
<v Speaker 1>wrote the first full biography of Kepler, portraying him as

1283
01:24:05.319 --> 01:24:08.239
<v Speaker 1>a hero of the revolution of the sciences who fused

1284
01:24:08.239 --> 01:24:12.960
<v Speaker 1>mathematical rigor with esthetic and religious insight. In the twentieth century,

1285
01:24:13.239 --> 01:24:17.079
<v Speaker 1>Alexandre Kore's influential studies of Kepler in the nineteen thirties

1286
01:24:17.479 --> 01:24:20.920
<v Speaker 1>further highlighted Kepper's role in transforming our worldview from an

1287
01:24:20.920 --> 01:24:26.680
<v Speaker 1>ancient closed cosmos to a modern infinite universe. Krey emphasized

1288
01:24:26.720 --> 01:24:30.800
<v Speaker 1>Keppler's platonic and mystical motivations as positive driving forces in

1289
01:24:30.800 --> 01:24:35.359
<v Speaker 1>his scientific breakthroughs. Philosophers of science have repeatedly used Kepler

1290
01:24:35.439 --> 01:24:39.199
<v Speaker 1>as a case study. For instance, Carl Popper pointed to

1291
01:24:39.279 --> 01:24:43.520
<v Speaker 1>Kepler's bold conjectures and attempts at falsification. Kepler tested dozens

1292
01:24:43.520 --> 01:24:47.520
<v Speaker 1>of hypotheses against data, discarding those that didn't work as

1293
01:24:47.600 --> 01:24:51.560
<v Speaker 1>exemplary of the scientific method. Keppler's confrontation with the competing

1294
01:24:51.600 --> 01:24:54.720
<v Speaker 1>world view of flood even got the attention of psychologist

1295
01:24:54.800 --> 01:24:57.680
<v Speaker 1>Wolfgang Poli, who wrote about it in the context of

1296
01:24:57.720 --> 01:25:02.039
<v Speaker 1>conflict between rational analysis and archae type of symbolism. In short,

1297
01:25:02.479 --> 01:25:05.279
<v Speaker 1>Kepler's work has been a treasure trove for scholars examining

1298
01:25:05.319 --> 01:25:08.479
<v Speaker 1>how science evolves and how human creativity bridges the gap

1299
01:25:08.520 --> 01:25:14.399
<v Speaker 1>between mysticism and empiricism. Culturally, Kepler's influence has extended into literature, music,

1300
01:25:14.479 --> 01:25:18.159
<v Speaker 1>and the arts. His life and ideas have inspired novels, operas,

1301
01:25:18.239 --> 01:25:23.119
<v Speaker 1>and artworks. For example, the Irish novelist John Bainville wrote

1302
01:25:23.199 --> 01:25:27.199
<v Speaker 1>Kepler in nineteen eighty one, a lyrical fictionalized biography that

1303
01:25:27.239 --> 01:25:32.279
<v Speaker 1>won the James Tate Black Memorial Prize. Banville's novel explores

1304
01:25:32.319 --> 01:25:35.880
<v Speaker 1>Kepler's in a world, his dreams, his anxieties, his spiritual

1305
01:25:35.920 --> 01:25:39.600
<v Speaker 1>musings against the backdrop of the chaotic seventeenth century, bridging

1306
01:25:39.640 --> 01:25:42.840
<v Speaker 1>the distant figure of life from modern readers. In music,

1307
01:25:43.039 --> 01:25:46.319
<v Speaker 1>the American composed of Philip Glass premiered and opera titled

1308
01:25:46.359 --> 01:25:50.039
<v Speaker 1>Kepler in two thousand and nine. This opera portrays episodes

1309
01:25:50.039 --> 01:25:52.960
<v Speaker 1>of Keppler's life in his series of theatrical scenes set

1310
01:25:53.000 --> 01:25:57.680
<v Speaker 1>to Glass's signature minimalistic but emotionally charged score. Glass was

1311
01:25:57.720 --> 01:26:01.720
<v Speaker 1>fascinated by Kepler's quest for order and juxtaposition of scientific

1312
01:26:01.800 --> 01:26:05.800
<v Speaker 1>and mystical themes. The city of Lenz, where Kepla lived,

1313
01:26:06.000 --> 01:26:08.479
<v Speaker 1>commissioned the opera as part of a celebration of science

1314
01:26:08.479 --> 01:26:12.960
<v Speaker 1>and art. Even in film, Keppler's cosmological ideas have made appearances.

1315
01:26:13.439 --> 01:26:17.600
<v Speaker 1>The twenty twelve science fiction film Mars et Avril opens

1316
01:26:17.640 --> 01:26:21.600
<v Speaker 1>with imagery based on Kepler's model for Harmonius Munday, illustrating

1317
01:26:21.600 --> 01:26:25.600
<v Speaker 1>a universe whose harmony is determined by celestial motion. The

1318
01:26:25.600 --> 01:26:29.359
<v Speaker 1>film's music score, composed by Benir Chorus, was even crafted

1319
01:26:29.359 --> 01:26:33.600
<v Speaker 1>according to Kepler's harmonic theory, translating the planet's orbital ratios

1320
01:26:33.600 --> 01:26:38.199
<v Speaker 1>into musical cues. In the visual arts, Keppeler's own drawings,

1321
01:26:38.319 --> 01:26:41.520
<v Speaker 1>such as his diagram of the nested platonic solids, often

1322
01:26:41.560 --> 01:26:43.920
<v Speaker 1>reproduced as a striking image of his sphere within a

1323
01:26:43.960 --> 01:26:47.000
<v Speaker 1>cube within a sphere and so on, or his sketches

1324
01:26:47.000 --> 01:26:50.239
<v Speaker 1>of Mars orbit are frequently celebrated for their esthetic beauty.

1325
01:26:51.000 --> 01:26:53.479
<v Speaker 1>Modern artists and poets seeing Keppler a figure of the

1326
01:26:53.560 --> 01:26:57.600
<v Speaker 1>contemplative scientists, someone whose sense of wonder and poetic description

1327
01:26:57.680 --> 01:27:00.520
<v Speaker 1>of nature. His writings are full of metaphors in sometimes

1328
01:27:00.560 --> 01:27:04.039
<v Speaker 1>lapses into poetic language, bridges the two cultures of science

1329
01:27:04.079 --> 01:27:07.720
<v Speaker 1>and art. The most famous poem historically associated with Kepler

1330
01:27:07.760 --> 01:27:11.239
<v Speaker 1>is actually one he didn't write, but inspired. The Latin

1331
01:27:11.319 --> 01:27:14.239
<v Speaker 1>verses on the front piece of the Radulphing Tables, written

1332
01:27:14.279 --> 01:27:17.239
<v Speaker 1>by an unknown poet, praised the unity of God's creation

1333
01:27:17.319 --> 01:27:21.079
<v Speaker 1>in the astronomer's task in measuring the stars. Those verses

1334
01:27:21.079 --> 01:27:24.600
<v Speaker 1>call on astronomers to serve eternity by joining the divine

1335
01:27:24.720 --> 01:27:27.479
<v Speaker 1>order of the heavens with human inquiry and apt summation

1336
01:27:27.600 --> 01:27:32.359
<v Speaker 1>of Kepler's ethos. Keppeler's name today adorns many honors and science.

1337
01:27:33.079 --> 01:27:36.119
<v Speaker 1>The Kepler Space Telescope, launched by NASA in two thousand

1338
01:27:36.159 --> 01:27:40.640
<v Speaker 1>and nine, has discovered thousands of exoplanets, truly continuing Keppler's

1339
01:27:40.680 --> 01:27:44.800
<v Speaker 1>legacy of planetary discovery. The mission was named in tribute

1340
01:27:44.800 --> 01:27:48.039
<v Speaker 1>to him. Appropriately. One of its great successes is finding

1341
01:27:48.079 --> 01:27:52.640
<v Speaker 1>planetary systems that confirm that Kepler's laws are universal. Even

1342
01:27:52.680 --> 01:27:56.119
<v Speaker 1>solar systems around other stars follow the same rules. The

1343
01:27:56.199 --> 01:27:59.560
<v Speaker 1>lunar creator Kepler and the asteroid eleven thirty four Kepler

1344
01:27:59.800 --> 01:28:03.319
<v Speaker 1>also bear his name, ensuing he is literally inscribed among

1345
01:28:03.359 --> 01:28:08.119
<v Speaker 1>the heavens. He studied. In Kepler's hometown Wioldstadt and other cities.

1346
01:28:08.119 --> 01:28:11.520
<v Speaker 1>He lived in Lenz, Prague Gratz, there are museums and

1347
01:28:11.600 --> 01:28:15.079
<v Speaker 1>monuments honoring him. A statue of Lens depicts him thoughtfully

1348
01:28:15.079 --> 01:28:17.960
<v Speaker 1>holding a model of orbits, and in Prague, a joint

1349
01:28:17.960 --> 01:28:20.920
<v Speaker 1>monument to Kepler and Tycho Brahe stands as a symbol

1350
01:28:20.920 --> 01:28:24.880
<v Speaker 1>of their cooperation. Kepler's life has also served as an

1351
01:28:24.920 --> 01:28:28.279
<v Speaker 1>inspiration in reflections on the relationship between science and religion.

1352
01:28:28.880 --> 01:28:32.880
<v Speaker 1>The MIT Independent Activities Period once ran a series on

1353
01:28:33.039 --> 01:28:36.880
<v Speaker 1>faith of scientists featuring Kepler, noting how his belief and

1354
01:28:36.920 --> 01:28:40.399
<v Speaker 1>cosmic order powered his science in the realm of a

1355
01:28:40.479 --> 01:28:44.479
<v Speaker 1>cult and esoteric Kepler's influence is more indirect, but still notable.

1356
01:28:45.199 --> 01:28:49.479
<v Speaker 1>While Kepler helped discredit traditional astrology among scientists, after his time,

1357
01:28:49.720 --> 01:28:52.920
<v Speaker 1>the two fields decisively split. By the eighteenth century, no

1358
01:28:53.000 --> 01:28:57.880
<v Speaker 1>serious astronomer practiced astrology. There remains an astrological Kepler in

1359
01:28:57.920 --> 01:29:00.039
<v Speaker 1>the sense that some astrologists today view him as a

1360
01:29:00.199 --> 01:29:05.279
<v Speaker 1>reformer of their art. Kepler College in Seattle, an astrology school,

1361
01:29:05.720 --> 01:29:09.640
<v Speaker 1>is named after him. Somewhat paradoxically giving Kepler's own mixed

1362
01:29:09.640 --> 01:29:14.880
<v Speaker 1>feelings about astrology. Additionally, Kepler's emphasis on geometric harmony influenced

1363
01:29:14.960 --> 01:29:18.520
<v Speaker 1>later mystics in New Age thinkers who romanticize sacred geometry.

1364
01:29:19.520 --> 01:29:22.359
<v Speaker 1>The image of the five platonic solids governing the cosmos,

1365
01:29:22.359 --> 01:29:26.079
<v Speaker 1>for example, resurfaces in esoteric literature as a symbol of

1366
01:29:26.159 --> 01:29:30.720
<v Speaker 1>hidden order. Kepler's successful blending of mystical intuition and empirical

1367
01:29:30.760 --> 01:29:34.560
<v Speaker 1>rigor stands as a challenge and model to anyone, even today,

1368
01:29:34.640 --> 01:29:39.399
<v Speaker 1>who seeks to reconcile holistic or spiritual perspectives with scientific method.

1369
01:29:41.159 --> 01:29:45.920
<v Speaker 1>Johannes Kepler's life was a tapestry woven with threads of genius, faith, hardship,

1370
01:29:46.039 --> 01:29:49.159
<v Speaker 1>and perseverance. He was born into a world defined by

1371
01:29:49.239 --> 01:29:53.239
<v Speaker 1>rigansphers and divine immutability. Yet he imagined a new world

1372
01:29:53.279 --> 01:29:55.760
<v Speaker 1>and lived to see it start to take hold, a

1373
01:29:55.800 --> 01:29:59.079
<v Speaker 1>world where planets soar along ellipses in an infinite universe

1374
01:29:59.359 --> 01:30:03.119
<v Speaker 1>governed by mathematical law. It is hard to picture the

1375
01:30:03.159 --> 01:30:06.000
<v Speaker 1>courage it took for Kepler to pursue his vision. He

1376
01:30:06.119 --> 01:30:09.960
<v Speaker 1>labored for years virtually alone, calculating by hand, often under

1377
01:30:09.960 --> 01:30:13.600
<v Speaker 1>financial duress and personal anguish. Guided only by a fierce

1378
01:30:13.640 --> 01:30:17.119
<v Speaker 1>conviction that the cosmos had a rational order, he could discern.

1379
01:30:17.800 --> 01:30:20.000
<v Speaker 1>Truth is the daughter of Time, and I feel no

1380
01:30:20.119 --> 01:30:23.840
<v Speaker 1>shame in being her midwife, Kepler wrote, expressing his willingness

1381
01:30:23.880 --> 01:30:26.880
<v Speaker 1>to endure doubt and ridicule in order to eventually birth

1382
01:30:26.960 --> 01:30:32.560
<v Speaker 1>the truth. Indeed, time has vindicated him. The treasures hidden

1383
01:30:32.560 --> 01:30:35.680
<v Speaker 1>in the heavens proved richer than anyone knew, and Kepler

1384
01:30:35.720 --> 01:30:38.560
<v Speaker 1>opened those treasure trolls with keys of geometry and physics.

1385
01:30:39.560 --> 01:30:42.760
<v Speaker 1>Through his laws, we launched satellites to Mars and predict eclipses.

1386
01:30:43.279 --> 01:30:45.119
<v Speaker 1>Through his optics, we peered to the edge of the

1387
01:30:45.199 --> 01:30:48.479
<v Speaker 1>universe with giant telescopes. Every time a spacecraft uses an

1388
01:30:48.520 --> 01:30:51.920
<v Speaker 1>orbital transfer or a transit method and finds a new exoplanet,

1389
01:30:52.159 --> 01:30:56.680
<v Speaker 1>Kepler's legacy is alive, and yet, beyond the technical triumphs,

1390
01:30:56.680 --> 01:30:59.520
<v Speaker 1>there is something profouling, human and heartfelt in Kepler's story.

1391
01:31:00.159 --> 01:31:03.439
<v Speaker 1>He was, as he said, moved by the geometry of

1392
01:31:03.439 --> 01:31:06.199
<v Speaker 1>the universe, by the shapes of the stars and the planets,

1393
01:31:06.520 --> 01:31:09.399
<v Speaker 1>and by the perfection of the forms of nature. In

1394
01:31:09.439 --> 01:31:12.479
<v Speaker 1>an era of war and witch hunts, Keppela held fast

1395
01:31:12.520 --> 01:31:14.960
<v Speaker 1>to the belief that the world is intelligible and beautiful.

1396
01:31:15.560 --> 01:31:18.079
<v Speaker 1>He never lost his sense of wonder. At the end

1397
01:31:18.079 --> 01:31:20.600
<v Speaker 1>of the harmony of the world, upon discovering the Third Law,

1398
01:31:20.920 --> 01:31:23.920
<v Speaker 1>Kepler broke into a prayer of gratitude and awe. I

1399
01:31:23.960 --> 01:31:27.079
<v Speaker 1>feel carried away and possessed by an unutterable rapture over

1400
01:31:27.119 --> 01:31:31.159
<v Speaker 1>the divine spectacle of the heavenly harmony. He gushed, Lord,

1401
01:31:31.560 --> 01:31:34.039
<v Speaker 1>I thank you that you have allowed me to see

1402
01:31:34.079 --> 01:31:37.800
<v Speaker 1>the beauty in your work. Such words remind us that science,

1403
01:31:37.800 --> 01:31:40.640
<v Speaker 1>for Keppla was not merely about cold numbers, but a

1404
01:31:40.640 --> 01:31:43.840
<v Speaker 1>passionate quest to touch the mind of God. After a

1405
01:31:43.840 --> 01:31:47.800
<v Speaker 1>lifetime of struggle, Keppla died far from home, without wealth

1406
01:31:47.920 --> 01:31:50.680
<v Speaker 1>or high rank. But he left us the very equations

1407
01:31:50.680 --> 01:31:54.279
<v Speaker 1>that described the dance of the planets. On his humble grave.

1408
01:31:54.439 --> 01:31:58.479
<v Speaker 1>Before it vanished, a friend recorded Kepler's own self composed epitaph.

1409
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<v Speaker 1>I used to measure the heavens now, I measure the

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<v Speaker 1>shadows of earth, although my mind was skybound. The shadow

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<v Speaker 1>of my body lies here In those lines, speaks a

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<v Speaker 1>man who knew his place in the grand scheme, a

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<v Speaker 1>child of Earth who reached for the stars Johannes Kepler's

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<v Speaker 1>legacy lives on in every orbit calculated, every harmony found

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<v Speaker 1>in nature, and every soul who looks up at the

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<v Speaker 1>night sky and even for a moment, feels carried away

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<v Speaker 1>by the unutterable rapture of its beauty. His life show

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<v Speaker 1>the show of a fearless intellect lighting a candle in

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<v Speaker 1>the dark cosmos, who continues to inspire and resonate, a

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<v Speaker 1>rich and heartfelt testament to the unity of science and wonder.
