WEBVTT

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<v Speaker 1>This is Spacetime Series twenty nine, episode ninety three, for

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<v Speaker 1>broadcast on the fifth of August twenty twenty six. Coming

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<v Speaker 1>up on Space Time, the strongest evidence yet that Bettlegurs

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<v Speaker 1>is not alone is the mighty Andromeda galaxy dying and

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<v Speaker 1>the most volcanically active world in the Solar System. All

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<v Speaker 1>that and more coming up on space Time.

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<v Speaker 2>Welcome to space Time with Stuart Gary.

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<v Speaker 1>Astronomers have finally demonstrated that the red supergiant star Bettlegurs

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<v Speaker 1>has a binary companion star about two to three times

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<v Speaker 1>the mass of our Sun. The findings, reported in the

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<v Speaker 1>journal Astronomy in Astrophysics provides the strongest evidence yet that

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<v Speaker 1>one of the biggest and brightest stars in the night

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<v Speaker 1>sky as a faint Stella companion, Bettlegirls b orbiting the

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<v Speaker 1>primary star located somewhere between five hundred and thirty and

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<v Speaker 1>six hundred and forty three light years away. Bettle Girls

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<v Speaker 1>is the brightest star in the constellation of Ryan the

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<v Speaker 1>Hunter and represents the scorpion sting on Oryan's shoulder. It's

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<v Speaker 1>the ninth brightest star in the night sky and one

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<v Speaker 1>of the largest and most luminous stars visible with the

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<v Speaker 1>unaided eye, commonly called beetlejuice. Don't say it three times.

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<v Speaker 1>Its name has been tortured through centuries of mispronunciations. It

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<v Speaker 1>originally started as ipdal Jaza, meaning the hand of the

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<v Speaker 1>big Man in Arabic, big man being a ryon the hunter.

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<v Speaker 1>Bettle Girls began its life around ten million years ago

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<v Speaker 1>as a spectral type O B blue star. Calculations of

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<v Speaker 1>Bettlegirls's mass range from slightly under ten to a little

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<v Speaker 1>more than twenty times that of our Sun, with some

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<v Speaker 1>one hundred thousand times the Sun's brightness and around eleven

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<v Speaker 1>hundred times its diameter. In fact, if Bettle Girls were

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<v Speaker 1>placed at the center of our solar system, its surface

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<v Speaker 1>would extend almost as far out as Jupiter, thereby engulfing

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<v Speaker 1>the orbits of Mercury, Venus, Earth, Mars, and the main

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<v Speaker 1>asteroid belt. Bettle Gurls is now a bloated old semiregular

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<v Speaker 1>variable red supergiant. Red supergiants are the largest stars in

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<v Speaker 1>the universe in terms of volume, although they're not necessarily

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<v Speaker 1>the most massive luminous. After spending billions of years fusing

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<v Speaker 1>hydrogen into helium in their cores, a star's core hydrogen

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<v Speaker 1>supply eventually runs out, and the balancing act between nuclear

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<v Speaker 1>fusion pushing out gravity pushing in stomps and gravity wins.

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<v Speaker 1>The huge mass of the star crashing down on the

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<v Speaker 1>core causes a dramatic increase in core pressure, consequently temperature

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<v Speaker 1>that triggers helium in the core to flash, which causes

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<v Speaker 1>the helium to start fusing into carbon and oxygen. At

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<v Speaker 1>the same time, the hydrogen rich region around the stellar

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<v Speaker 1>core has moved down towards the core into a region

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<v Speaker 1>where temperatures and pressures are high enough for hydrogen fusion

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<v Speaker 1>into helium to commence in the shell around the core. Meanwhile,

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<v Speaker 1>the increasing core temperature results in increasing luminosity, and the

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<v Speaker 1>resulting radiation pressure from shell burning causes the outer diffuse

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<v Speaker 1>gaseous envelope of the star to expand to hundreds of

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<v Speaker 1>times its previous radius. As the now bloated star's chromosphere

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<v Speaker 1>or visible surface, moves further away from the core, it

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<v Speaker 1>cools down, turning redder. Hence the star becomes a red giant.

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<v Speaker 3>Sun.

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<v Speaker 1>Like stars, eventually lose the outer envelope, which continues expanding outwards,

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<v Speaker 1>forming a planetary nebula. This ultimately exposes the star's white

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<v Speaker 1>hot stellar core as a white dwarf, which will slowly

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<v Speaker 1>cool over the eons. However, stars with masses more than

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<v Speaker 1>a round eight times that of our Sun experience a

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<v Speaker 1>very different fate. Unlike the Sun, their fusion cycle doesn't

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<v Speaker 1>end with helium fusing into carbon and oxygen. They've got

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<v Speaker 1>enough mass to fuse carbon and oxygen in their core

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<v Speaker 1>into progressively heavier and heavier elements, while shell burning around

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<v Speaker 1>the core also fuses progressively heavier and heavier elements carbon, nitrogen, oxygen, neon, magnesium, silicon, sulfur, nickel,

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<v Speaker 1>and eventually iron. These stars have become red super giants. Now,

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<v Speaker 1>no matter how massive a star is, it can't fuse

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<v Speaker 1>iron into heavier elements, and so once again gravity wins,

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<v Speaker 1>causing the entire mass of the start to collapse down

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<v Speaker 1>onto the core. The collapse is so powerful that the

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<v Speaker 1>billions of tons of material causes a rebound, and the

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<v Speaker 1>star explodes as a core collapse supernova so bright it

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<v Speaker 1>briefly outshines an entire galaxy. The star eventually ends up

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<v Speaker 1>as either a neutron star or an even stranger object

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<v Speaker 1>called a black hole. Singularities of infinite density and zero volume.

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<v Speaker 1>With the lures of physics a science understands them no

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<v Speaker 1>longer apply, and this will be the fate of Bettle Girls.

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<v Speaker 1>In fact, it could explode as a core collapse or

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<v Speaker 1>type two supernova any day now, which in astronomical terms

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<v Speaker 1>means it could be tomorrow or a million years from now.

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<v Speaker 1>Whenever it happens. When it does explode, it'll temporarily outshine

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<v Speaker 1>all the other stars in the galaxy, and it'll be

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<v Speaker 1>clearly visible in the daytime sky here on Earth, and

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<v Speaker 1>that'll be a fascinating experience. Star seen by humans to

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<v Speaker 1>go super and ova in our galaxy was Tiger Star

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<v Speaker 1>in the year fifteen seventy two, and that was before

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<v Speaker 1>the invention of the telescope. This new study is lead

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<v Speaker 1>author Miguel Montagas from the Paris Observatory, says astronomers of

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<v Speaker 1>look for potential companions as a possible explanation for Bettelegirls's

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<v Speaker 1>regular changes in brightness. Two studies published in twenty twenty

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<v Speaker 1>four predicted that the companion would be furthest from Bettlegirls

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<v Speaker 1>in December of that year, and hence easier to spot,

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<v Speaker 1>so Montagas and colleagues used the European Southern Observatories very

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<v Speaker 1>large telescope the VLT in December of twenty twenty four

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<v Speaker 1>and spent several months observing the star, and eventually they

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<v Speaker 1>obtained the clearest image ever of what likely is Bettelegirls By.

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<v Speaker 1>Montager says he was concerned he didn't have the sensitivity

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<v Speaker 1>in his instruments that detech Bettlegirls b because it was

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<v Speaker 1>thought to be too similar to the Sun in brightness

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<v Speaker 1>and so it would be obscured by the primary stars glare.

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<v Speaker 1>But it turned out to be at least two to

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<v Speaker 1>three times the mass of the Sun and so it

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<v Speaker 1>could be directly imaged, meaning the light from the star

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<v Speaker 1>itself was detected. While there has been some early evidence

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<v Speaker 1>of the possible existence of a companion star, including a

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<v Speaker 1>possible direct detection by the Gemini North telescope in Away,

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<v Speaker 1>this is the strongest evidence for and the clearest image

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<v Speaker 1>jet of Bettleghost be now to be certain the companion's

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<v Speaker 1>really there, the authors still need to observe it in

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<v Speaker 1>a year's time on the other side of the star,

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<v Speaker 1>but Montegas believes this very little space left for doubt.

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<v Speaker 1>A few years back, Bettlegoes was the subject of attention

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<v Speaker 1>from astronomers around the world when it visibly started dimming.

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<v Speaker 1>It quickly went from being the ninth brightest star in

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<v Speaker 1>the sky being the twentieth brightest. As we mentioned earlier,

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<v Speaker 1>as an evolved super giant star, Bettlegoes is expected to

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<v Speaker 1>explode as a supernova any day now, and so that

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<v Speaker 1>dimming led some to suspect that this could be what

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<v Speaker 1>was about to happen, but observations by Montegas and colleagues

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<v Speaker 1>eventually determined the star was simply being obscured by a

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<v Speaker 1>cloud of dust. This is space time still to come.

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<v Speaker 1>Is the mighty Andromeda galaxy dying and the most volcanically

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<v Speaker 1>active world in our Solar System? All that and more

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<v Speaker 1>still to come on space time. A new study has

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<v Speaker 1>found that star formation appears to be winding down in

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<v Speaker 1>the nearest big neighboring galaxy, Andromeda. The new findings reported

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<v Speaker 1>in the Astrophysical Journal, based on observations by NASA's Hubble

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<v Speaker 1>Space Telescope. Astronomer's study Andromeda because it provides them with

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<v Speaker 1>an opportunity to examine its stellar populations in great detail,

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<v Speaker 1>leading to a better understanding of the past of galaxies

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<v Speaker 1>like our own. The Andromeda galaxy M thirty one is

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<v Speaker 1>located about two and a half million light years away,

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<v Speaker 1>and like our own Milky Way, it's a spiral galaxy.

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<v Speaker 1>It's close enough and big enough to be seen with

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<v Speaker 1>the unaided eye from dark skies. It's the largest member

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<v Speaker 1>of our local galactic group, with around twice the diameter

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<v Speaker 1>of our Milky Way, spanning some two hundred and twenty

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<v Speaker 1>five thousand, two hundred and sixty thousand light years across.

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<v Speaker 1>That compares to the Milky Ways diameter of between one

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<v Speaker 1>hundred thousand and one hundred and twenty thousand light years. However,

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<v Speaker 1>astronomers now suspect the two galaxies probably have similar masses,

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<v Speaker 1>with both weighing roughly eight hundred billion to one point

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<v Speaker 1>five trillion times a mass of our Sun. The new

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<v Speaker 1>observations indicate star formation in Andromeda has undergone a five

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<v Speaker 1>hundred million year decline, with an even steeper drop in

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<v Speaker 1>the last forty million years. The findings are based on

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<v Speaker 1>data from two Hubble surveys, the panchromatic Hubble Andromeda Treasury

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<v Speaker 1>and the pan chromatic Hubble Andromeda Southern treasury. Together, they've

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<v Speaker 1>mapped two thirds of Andromeda's disc in ultra sharp detail.

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<v Speaker 1>In total, the author has measured about two hundred million

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<v Speaker 1>individual stars across the galaxy, giving them a detailed picture

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<v Speaker 1>of andromedais past activity. One of the studies authors, Ben

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<v Speaker 1>Williams from the University of Washington, says astronomers need to

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<v Speaker 1>measure the individual stars because they're the fossil record of

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<v Speaker 1>the galaxy's formation, and Hubble is the only telescope that

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<v Speaker 1>can provide high enough spatial resolution over a large enough

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<v Speaker 1>area to be able to do that. In Andromeda. The

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<v Speaker 1>key is that massive stars are bluer and shorter lived,

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<v Speaker 1>or less massive stars are redder and longer lived. As

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<v Speaker 1>a result, areas that have experienced recent star formation tend

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<v Speaker 1>to have a larger fraction of blue stars, or areas

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<v Speaker 1>with less recent star formation typically have a reader population.

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<v Speaker 1>So Williams and colleagues divided Andromeda's images into thousands of squares,

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<v Speaker 1>each spanning roughly three hundred light years per side. They

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<v Speaker 1>determine the history of star formation within each pixel in

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<v Speaker 1>order to gain a comprehensive view of the galaxy's past.

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<v Speaker 1>Previous research showed that the Andromeda galaxy experienced a dramatic

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<v Speaker 1>burst of star formation around two billion years ago that

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<v Speaker 1>was likely due to a past interaction or merger with

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<v Speaker 1>another galaxy, but since then star formation has steadily declined.

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<v Speaker 1>Astronomers measure the rate of star formation in terms of mass,

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<v Speaker 1>or the amount of gas and dust converted into stars

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<v Speaker 1>every year. The authors calculated that five hundred million years

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<v Speaker 1>years ago, Andromeda form stars at a rate of about

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<v Speaker 1>one solar mass per year. That's about the same as

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<v Speaker 1>the Milky Way today. However, formation rate dropped in Andromeda

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<v Speaker 1>to about half of that figure by about forty million

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<v Speaker 1>years ago. The current rate is now plummeted even further,

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<v Speaker 1>to just a fifth of the mass of our Sun

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<v Speaker 1>per year. They also examined whether that decline was consistent

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<v Speaker 1>across the entire galaxy, were just concentrated in certain specific areas,

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<v Speaker 1>and they found that much of the recent star formation

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<v Speaker 1>occurred in a start forming ring located around thirty two

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<v Speaker 1>thousand lay years from the galaxy center. As a result,

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<v Speaker 1>much of the decline they measured was driven by decreasing

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<v Speaker 1>activity within that ring, rather than being the result of

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<v Speaker 1>reduced material from which new stars can form. The authors

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<v Speaker 1>think the declines are more likely to be a natural

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<v Speaker 1>winding down from its previous, more active state. Williams and

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<v Speaker 1>colleagues also investigated whether there was any connection between the

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<v Speaker 1>decreasing activity and Andromeda. At its proximity to the satellite

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<v Speaker 1>galaxy Messia thirty two. M thirty two separated from Andromeda

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<v Speaker 1>by about sixteen thousand light years in the plane of

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<v Speaker 1>the sky. However, it's three D location in space is uncertain.

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<v Speaker 1>As a result, astronomers are unsure if or when it

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<v Speaker 1>might have interacted with Andromeda in the past. Survey data

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<v Speaker 1>from the panchromatic hubble Andromeda Southern Treasury allowed the authors

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<v Speaker 1>to study the history of star formation and Andromeda in

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<v Speaker 1>and near M thirty two, and they found this area

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<v Speaker 1>showed signs of decreased star formation compared to other regions.

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<v Speaker 1>The timing of this decrease, which the study finance began

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<v Speaker 1>roughly sixty million years ago, could help constrain when M

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<v Speaker 1>thirty two interacted with Andromeda's disc The authors say they

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<v Speaker 1>can't explicitly say they're seeing a decrease in star formation

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<v Speaker 1>because of M thirty two, but hey, it's right there,

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<v Speaker 1>and it's definitely the most likely suspect. This is space

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<v Speaker 1>time still to come, the most volcanically active word in

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<v Speaker 1>the Solar System, and later in the science report, a

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<v Speaker 1>new study wards that mining is now a threat and

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<v Speaker 1>more than twelve thousand species across the planet. All that

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<v Speaker 1>and more still to come on space time. NASA's Guno

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<v Speaker 1>spacecraft has provided the first measurements of the temperature below

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<v Speaker 1>the surface of Jupiter's volcanic moon Io. The findings, reported

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<v Speaker 1>in the Journal of Geophysical Research Planets, shows significant heating

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<v Speaker 1>within the shallow subsurface of what is the most volcanically

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<v Speaker 1>active world in our Solar System, collected during two close flybys.

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<v Speaker 1>The data also shows that most of Io's surface is

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<v Speaker 1>remarkably smooth and composed of material with very low density.

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<v Speaker 1>Io's extreme volcanism is powered by tidal heating. See the

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<v Speaker 1>Moon's constantly being stretched and squeezed by the immense gravity

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<v Speaker 1>of its host planet Jupiter as it travels in its

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<v Speaker 1>slightly elliptical orbit around the gas giant, then the refurther

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<v Speaker 1>grap vitational tugs during its journey from its sister Jovian moons.

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<v Speaker 1>Io is the innermost and smallest ob Jubiter's for Galilean moons,

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<v Speaker 1>but the three thousand, six hundred and sixty kilometer wide

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<v Speaker 1>world is still slightly larger than the Earth's moon. Until now,

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<v Speaker 1>virtually everything astronomers know about Io's tidal heating has come

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<v Speaker 1>from infrared observations, which can really only sense the temperature

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<v Speaker 1>of the surface. But these latest findings are based on

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<v Speaker 1>data collected by Juno's microwave radiometer. JUNO Principal investigator Scott

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<v Speaker 1>Bolton from the Southwest Research Institute in San Antonio, Texas,

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<v Speaker 1>says the surprising discovery that we can see below the

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<v Speaker 1>rocky Moon's surface as important implications for studding volcanoes here

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<v Speaker 1>on Earth. He says June's taught scientists that if they

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<v Speaker 1>look with a microwave radiometer instrument near a volcano on Earth,

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<v Speaker 1>they might see similar signatures in the subsurface temperature gradients,

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<v Speaker 1>providing new information and our Earth volcanoes work. Juno's microwave

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<v Speaker 1>radiometer was designed by Bob to peer beneath Jupiter's cloud

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<v Speaker 1>tops in order to investigate the dynamics and composition the

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<v Speaker 1>gas giants deep atmosphere. Its six microwave antennas act as

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<v Speaker 1>a single instrument simultaneously detecting microwaves at a range of

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<v Speaker 1>different wavelengths. During Jurney's extended phase, It's provided scientists an

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<v Speaker 1>opportunity observe three of the planets, so called Galilean moons,

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<v Speaker 1>gain he made, Europa and Io. So far, only Callisto

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<v Speaker 1>has been left out of the study. They're called Galilean

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<v Speaker 1>moons because they were first observed by Galileo Galilee when

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<v Speaker 1>he turned his telescope onto the orb of Jupiter. Seeing

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<v Speaker 1>the Moon's orbiting around Jupiter, Galileo realized that the Earth

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<v Speaker 1>and all the other planets in the Solar System were

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<v Speaker 1>simply doing the same thing around the Sun, a discovery

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<v Speaker 1>which ended with him not only being sentenced to house

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<v Speaker 1>detention by the Catholic Church for the rest of his life,

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<v Speaker 1>but he was also forced to renounce his discovery on

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<v Speaker 1>pain of death. Yet even then, under his breath he whispered,

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<v Speaker 1>and yet it moves, referring to Earth orbiting around the

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<v Speaker 1>Sun rather than the Earth's centric view of the universe

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<v Speaker 1>favored by the Catholic Church at the time. Bolton says

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<v Speaker 1>each wavelength within the microwave radiometer explores different depths providing

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<v Speaker 1>a new way to characterize the deb atmosphere of the

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<v Speaker 1>giant planets, as well as the subsurface crusts of icy

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<v Speaker 1>and rocky moons. At Gannymeat in Europa, Geno explored tens

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<v Speaker 1>of kilometers below the surface, assuming that ice shells were

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<v Speaker 1>mostly pure water, but the ability to probe the volcanic

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<v Speaker 1>rock on Io was an unexpected discovery. During flybys on

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<v Speaker 1>de seven thirtieth in twenty twenty three and February thirty,

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<v Speaker 1>twenty twenty four, the Genos spacecraft came within fifteen hundred

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<v Speaker 1>kilometers of iOS surface.

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<v Speaker 3>Bolton and colleagues.

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<v Speaker 1>Found that everywhere they looked, they saw temperature increases of

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<v Speaker 1>roughly five degrees celsius every few centimeters, a fast steeper

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<v Speaker 1>gradient and solar heating alone can explain, and that suggests

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<v Speaker 1>only two likely explanations. Either the heat is right steadily

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<v Speaker 1>through a conductive crust, or the signal could be coming

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<v Speaker 1>from cooling lava flows cap by roughly ten meters of

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<v Speaker 1>solidified crust, covering about ten percent of the Moon's surface

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<v Speaker 1>at any given time. Bolton says Io provides a unique

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<v Speaker 1>window matter how tidal heating works throughout the cosmos a

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<v Speaker 1>fundamental process providing energy and heat to worlds that could

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<v Speaker 1>be orbiting far from the hearth star. This process not

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<v Speaker 1>only it creates the most volcanically active world in our

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<v Speaker 1>Solar system, but it also fuels the subsurface oceans on

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<v Speaker 1>the ice moons of the giant planets like Europa, Enceladus.

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<v Speaker 3>And Ganny Made.

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<v Speaker 1>Another major insight gained from Juno's two flybys of Io

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<v Speaker 1>is just how smooth the little world is. For these findings,

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<v Speaker 1>the Moon was known for its tall mountains, but the

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<v Speaker 1>new observations indicate that apart from this visible topography, the

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<v Speaker 1>surface features expansive smooth patches that can stretch for hundreds

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<v Speaker 1>of kilometers or more. Because Uno flew by overlapping regions

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<v Speaker 1>of Io at different angles, you alsos are able to

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<v Speaker 1>map just how the surface reflects marcrowaves, showing them just

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<v Speaker 1>how flat this distant world really is. But of course

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<v Speaker 1>Io has an ever changing geography. Living on Io, you

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<v Speaker 1>wouldn't have weather reports, you'd have geological reports, with lava

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<v Speaker 1>lakes forming in the north, mountain building in the south,

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<v Speaker 1>ground solidification in the west. This report on Geno's mission

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<v Speaker 1>to Jupiter comes from NESTV.

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<v Speaker 4>Humanity has had its eyes on Jupiter for surgeries. First

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<v Speaker 4>telescopes and in recent decades, eight deep space pros were

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<v Speaker 4>used to examine the largest planet in the Solar System.

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<v Speaker 3>Equipped with unique sensors.

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<v Speaker 4>JUNO looked deeper into the planet's structure than ever before

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<v Speaker 4>to find out the answers to basic questions about Jupiter's

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<v Speaker 4>makeup and how it formed.

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<v Speaker 5>Juno's looking for how Jupiter formed and really how planets

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<v Speaker 5>are made in general. We're very much looking for the

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<v Speaker 5>recipe for planets. The special thing about JUNO is is

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<v Speaker 5>we're really looking at one of the first steps, the

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<v Speaker 5>earliest time in our Solar System's history, right after the

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<v Speaker 5>Sun formed. What happened that allowed the planets to form?

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<v Speaker 5>And why are the planets slightly different composition than the Sun.

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<v Speaker 4>Jupiter is so far away from Earth, then, even when

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<v Speaker 4>it's at as closest to us, it will still take

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<v Speaker 4>a radio signal moving at the speed of light about

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<v Speaker 4>thirty four minutes to cross the distance.

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<v Speaker 1>Pretty challenging missions, pretty challenging payloads. I'd say it's pretty robust.

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<v Speaker 6>So it's those kind of challenges with making sure you

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<v Speaker 6>do all the little things necessary to maximize the opportunities

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<v Speaker 6>that you get.

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<v Speaker 4>Aside from distance, Jupiter offers unique challenges to a spacecraft,

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<v Speaker 4>such as a radiation field rivaled in intensity only by

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<v Speaker 4>the Sun.

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<v Speaker 5>We have a box in the middle of the spacecraft

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<v Speaker 5>that we call a vault, and it's made out of titanium,

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<v Speaker 5>and that shield all the electronics from these hazardous radiation

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<v Speaker 5>and we're very much an armoured tank going to Jupiter.

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<v Speaker 4>Justice JUNO is building on the knowledge gained with past

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<v Speaker 4>missions to Jupiter. Future missions will build on Juno's findings.

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<v Speaker 5>If we could start to understand the role that Jupiter

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<v Speaker 5>played and how the planet formed and how that eventually

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<v Speaker 5>governed the creation of all the other planets and Earth

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<v Speaker 5>and maybe even life itself, then we know a little

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<v Speaker 5>bit about how to look for other Earth like planets

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<v Speaker 5>maybe orbiting other stars, and how common those might be,

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<v Speaker 5>and the roles that those giant planets that we see

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<v Speaker 5>orbiting the other stars play.

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<v Speaker 6>Really, all these missions that LSPs involved in, the NASSAS

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<v Speaker 6>involved in are all precursors to the bigger picture of

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<v Speaker 6>getting humans out beyond low Orth orbit to Mars, to

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<v Speaker 6>an asteroid and be honest.

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<v Speaker 1>And in that report, from MESSATV. We heard from JUNA

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<v Speaker 1>Principal investigator Scott Bolton from the Southwest Research Institutions, San Antonio, Texas,

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<v Speaker 1>as well as GUNO Launch Director Omar Bayes and JUNO

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<v Speaker 1>Mission Manager John Culvert, both from NASSA.

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<v Speaker 3>This is Space Time and time out to.

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<v Speaker 1>Take another brief look at some of the other stories

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<v Speaker 1>making US and science this week with a science report.

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<v Speaker 1>A new study warns that mining is now a threat

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<v Speaker 1>to more than twelve thousand species across the planet, which

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<v Speaker 1>includes almost six thousand that are already listed is threatened.

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<v Speaker 1>The findings, published in the journal Cille Report Sustainability, overlaid

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<v Speaker 1>the space where mining occurs across the planet and noted

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<v Speaker 1>that twenty eight percent of the ranges of threatened species

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<v Speaker 1>overlap with those areas that are being mined. The authors

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<v Speaker 1>say at least one hundred species have some seventy five

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<v Speaker 1>percent of their ranges overlapping in these areas. That's despite

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<v Speaker 1>mining not being recognized as a threat by the International

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<v Speaker 1>Union for Conservation of Nature. They also found that future

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<v Speaker 1>planned mining sites could expose over three thousand threatened species

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<v Speaker 1>to the risks involved around mining sites, eighty three percent

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<v Speaker 1>of which don't have a mining related threat designation. A

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<v Speaker 1>new study claims taking fecal capsules could help people with

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<v Speaker 1>insomnia get a good night's sleep. A report in the

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<v Speaker 1>Journal of Internal Medicine claims a trial involving forty people

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<v Speaker 1>who had chronic insomnia disorder were given either a placebo

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<v Speaker 1>or an antibiotic trip and to clear their gut microbiome,

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<v Speaker 1>and then fecal pills to recolonize their intestinal tract. After

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<v Speaker 1>a month, the participants receiving the fecal pills showed greatly

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<v Speaker 1>improved sleeping patterns compared to those on the placebo. The

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<v Speaker 1>subjects taking the pills also reported feeling that their sleep

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<v Speaker 1>had improved for up to six months after taking them.

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<v Speaker 2>Well.

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<v Speaker 1>Despite Australia's air being relatively unpolluted compared to other parts

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<v Speaker 1>of the world, a new study is found that there's

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<v Speaker 1>a clear link in the Great Southern Land between air

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<v Speaker 1>pollution exposure and the risk of ending up in hospital

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<v Speaker 1>with lung and hard issues. The findings, reported in the

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<v Speaker 1>journal Public Health Research and Practice, used national air pollution

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<v Speaker 1>estimates from twenty sixteen and hospitalization data from one thy

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<v Speaker 1>one hundred and fifty five Public Health areas between twenty

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<v Speaker 1>sixteen and twenty seventeen, representing some twenty three million, two

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<v Speaker 1>hundred and thirty six thousand and forty six people. The

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<v Speaker 1>authors found higher exposure to pollution particles smaller than two

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<v Speaker 1>point five nanometers together with nitrogen dioxide was consistently linked

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<v Speaker 1>with increases and hospitalizations for these issues.

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<v Speaker 3>A new study has.

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<v Speaker 1>Found that people who spent an excessive amount of time

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<v Speaker 1>online tend to be more stressed, have worse moods, and

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<v Speaker 1>neglected other parts of their lives. A report in the

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<v Speaker 1>General plus one monitored the daily Internet use of some

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<v Speaker 1>nine hundred German adults for two weeks. The authors found

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<v Speaker 1>temptation was the biggest thing pushing subjects to go online. However,

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<v Speaker 1>although excessive Internet users had worse moods, spending time online

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<v Speaker 1>didn't improve how they felt. Telstra, Australia's largest telco, is

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<v Speaker 1>expanding its relationship with Elon Musk's Starling broadband satellite network.

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<v Speaker 1>Right now, the starting constellation includes some teny four hundred

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<v Speaker 1>and thirteen satellites in low Earth orbit, and Telstra wants

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<v Speaker 1>to take advantage of that. With the details of the

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<v Speaker 1>new Telstra Starlin deal We're joined by technology editor Alex

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<v Speaker 1>saharov Royt from Tech Advice Start Life.

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<v Speaker 7>Yeah, well the calling of the first for Australia satellite

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<v Speaker 7>to mobile connectivity expands from text to apps. Now before

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<v Speaker 7>you suddenly think, oh, you know I can get a

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<v Speaker 7>high speed bandwidth from the sky, No, this is for

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<v Speaker 7>low data uses. And they were the first launch satellite

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<v Speaker 7>messaging in Australia. This was to send messages beyond the

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<v Speaker 7>range of their mobile network. But now they're rolling out

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<v Speaker 7>access to select satellite apps to eligible consumer and small

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<v Speaker 7>business customers. So this is where their collaboration with Stalin.

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<v Speaker 7>There's now a selection of satellite optimized apps and this

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<v Speaker 7>includes things like navigation apps, Apple Maps, Google Maps, all trails,

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<v Speaker 7>messaging apps including I Message, What'sapp, Facebook Messengers, Signal and

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<v Speaker 7>Google Messages. You've also got weather apps Apples Weather, ACU

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<v Speaker 7>Weather and Google Weather, and then also Google Fitness and

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<v Speaker 7>of course the Mind telstra app. And these are apps

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<v Speaker 7>that have been specifically optimized to send and receive data

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<v Speaker 7>over what is effectively intermittent satellite connectivity. Over what'sapp. You

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<v Speaker 7>can do voice and video calls, but it's going to

418
00:24:23.839 --> 00:24:25.880
<v Speaker 7>drop out. You just want to send text messages, but

419
00:24:26.039 --> 00:24:29.279
<v Speaker 7>eventually you will have a lot more direct to device

420
00:24:29.519 --> 00:24:33.680
<v Speaker 7>capability from updated Stylink and other satellites are designed to

421
00:24:33.839 --> 00:24:36.359
<v Speaker 7>connect directly the mobile phones and give a proper higher

422
00:24:36.400 --> 00:24:39.400
<v Speaker 7>bandwidth experience. And this will work with iPhone thirteen on

423
00:24:39.440 --> 00:24:41.960
<v Speaker 7>newer the new Samsung Galaxy S twenty six, and it

424
00:24:42.000 --> 00:24:44.559
<v Speaker 7>will expand to some of the older Galaxy range by

425
00:24:44.559 --> 00:24:46.240
<v Speaker 7>the end of the year. It's really for people who

426
00:24:46.279 --> 00:24:48.880
<v Speaker 7>are outside of the mobile network, and it will mean

427
00:24:48.960 --> 00:24:51.240
<v Speaker 7>that over the next few years you will have a

428
00:24:51.279 --> 00:24:55.000
<v Speaker 7>lot more services connecting directly to satellites without needing a

429
00:24:55.000 --> 00:24:57.559
<v Speaker 7>special SAT phone. And it's kind of put into question

430
00:24:57.880 --> 00:25:01.160
<v Speaker 7>what you need to be connected to your local provider

431
00:25:01.240 --> 00:25:03.759
<v Speaker 7>forman there will come a time when starling elon must

432
00:25:03.759 --> 00:25:06.000
<v Speaker 7>well just have a global plan, and you're already talking

433
00:25:06.039 --> 00:25:09.240
<v Speaker 7>about wanting to buy existing telcos for their spectrum or

434
00:25:09.279 --> 00:25:12.240
<v Speaker 7>bidding on spectrum services so that he can have terrestrial

435
00:25:12.319 --> 00:25:15.119
<v Speaker 7>and satellite connectivity. And imagine if you just had a

436
00:25:15.160 --> 00:25:18.559
<v Speaker 7>global plan through Staralink that worked with any phone would

437
00:25:18.559 --> 00:25:19.039
<v Speaker 7>pretty cool.

438
00:25:19.160 --> 00:25:21.920
<v Speaker 1>During the thirteenth test flight or the Starship. On board

439
00:25:21.920 --> 00:25:25.920
<v Speaker 1>that starship, we're twenty test versions of the Starlink Version

440
00:25:25.960 --> 00:25:28.160
<v Speaker 1>three satellites. They're a little bit bigger than the current

441
00:25:28.240 --> 00:25:31.200
<v Speaker 1>version two and they're the ones that will in fact

442
00:25:31.359 --> 00:25:36.680
<v Speaker 1>allow every cell phone to become a satellite phone for voice, video, everything.

443
00:25:36.759 --> 00:25:38.480
<v Speaker 1>And that's how close we are. We just need to

444
00:25:38.480 --> 00:25:39.839
<v Speaker 1>get more of those satellites up there.

445
00:25:39.880 --> 00:25:42.119
<v Speaker 7>And look, the thing about the satellites is that I mean,

446
00:25:42.160 --> 00:25:44.240
<v Speaker 7>I remember when three or four years ago Elon was

447
00:25:44.279 --> 00:25:46.519
<v Speaker 7>talking about launching version two satellites. So here we are

448
00:25:46.559 --> 00:25:48.960
<v Speaker 7>in twenty twenty six is launching version three. And these

449
00:25:49.119 --> 00:25:52.720
<v Speaker 7>satellites they're not permanent fixtures in space. They slowly get

450
00:25:52.720 --> 00:25:54.319
<v Speaker 7>out of all but I mean the only supposed to

451
00:25:54.359 --> 00:25:55.799
<v Speaker 7>last five or six years before they have to be

452
00:25:55.880 --> 00:25:57.920
<v Speaker 7>de orbited. Anyway, that's why it keeps launching the new

453
00:25:57.960 --> 00:26:00.799
<v Speaker 7>satellites all the time and replacing them with more advanced

454
00:26:00.799 --> 00:26:03.160
<v Speaker 7>ones which have these extra capabilities every time I launched

455
00:26:03.160 --> 00:26:05.440
<v Speaker 7>a new one. As you just explained, well after a

456
00:26:05.480 --> 00:26:07.359
<v Speaker 7>certain period of time, there'll be a Version four and

457
00:26:07.400 --> 00:26:08.119
<v Speaker 7>a Version.

458
00:26:07.839 --> 00:26:10.640
<v Speaker 1>Five, and that's part of what Starship's all about. Whereas

459
00:26:10.640 --> 00:26:14.160
<v Speaker 1>a Falcon nine can launch maybe twenty twenty eight satellites

460
00:26:14.160 --> 00:26:16.799
<v Speaker 1>in a single bounce, the Starship will launch sixty at

461
00:26:16.799 --> 00:26:20.200
<v Speaker 1>a single go sixty satellites each launch. That's pretty yeah,

462
00:26:20.240 --> 00:26:20.480
<v Speaker 1>it is.

463
00:26:20.519 --> 00:26:23.559
<v Speaker 7>And that's how, of course, you build out the constellation quickly.

464
00:26:23.559 --> 00:26:25.400
<v Speaker 7>I mean, we did have the situation where a couple

465
00:26:25.480 --> 00:26:28.240
<v Speaker 7>of months ago Jeff Bezos Blue Origin satellite, which was

466
00:26:28.279 --> 00:26:30.440
<v Speaker 7>meant to launch a bunch of the next gen Amazon

467
00:26:30.519 --> 00:26:33.480
<v Speaker 7>Leo satellites that nd N and Australia onced upgraded sky

468
00:26:33.599 --> 00:26:36.319
<v Speaker 7>Muster network with And I mean that explosion blew up

469
00:26:36.359 --> 00:26:38.359
<v Speaker 7>a whole stack of those satellites and blew out most

470
00:26:38.359 --> 00:26:39.920
<v Speaker 7>of the launch pad with it. I was reading that

471
00:26:40.000 --> 00:26:42.319
<v Speaker 7>it normally takes twelve to eighten months to rebuild a

472
00:26:42.400 --> 00:26:44.720
<v Speaker 7>launch pad, but Blue Origin is determined to get it

473
00:26:44.880 --> 00:26:46.720
<v Speaker 7>up by the end of the year, by December twenty

474
00:26:46.720 --> 00:26:47.119
<v Speaker 7>twenty sixth.

475
00:26:47.119 --> 00:26:49.119
<v Speaker 1>The Russian said that problem too. A couple of months ago,

476
00:26:49.200 --> 00:26:52.279
<v Speaker 1>when a Sawyers launch destroyed the launch pad. The Sawyers

477
00:26:52.359 --> 00:26:54.720
<v Speaker 1>was fine, the rocket was fine, the launch pad it

478
00:26:54.759 --> 00:26:57.720
<v Speaker 1>had gone to whatever launch pad heaven there is. Yeah,

479
00:26:57.920 --> 00:26:59.599
<v Speaker 1>thank god. It will be at least two years before

480
00:26:59.640 --> 00:27:02.200
<v Speaker 1>they could get people back into space, because this was

481
00:27:02.240 --> 00:27:05.119
<v Speaker 1>their only launch pad designed to carry manned spacecraft. Yet

482
00:27:05.640 --> 00:27:08.319
<v Speaker 1>in nine months they completely replaced it and they were

483
00:27:08.319 --> 00:27:10.559
<v Speaker 1>back up and running. So Jeff Bezos saying he'll do

484
00:27:10.599 --> 00:27:11.000
<v Speaker 1>it before the.

485
00:27:11.079 --> 00:27:12.440
<v Speaker 3>End of the year, Yeah, I believe that. Yeah.

486
00:27:12.440 --> 00:27:14.599
<v Speaker 7>Well, I mean what I read was it'll be approximately

487
00:27:14.640 --> 00:27:16.920
<v Speaker 7>six months and it's going to be just enough launch

488
00:27:16.960 --> 00:27:18.799
<v Speaker 7>pad for the launch. I mean, I'm sure they'll keep

489
00:27:18.839 --> 00:27:21.079
<v Speaker 7>upgrading it, but you need to get the Amazon Leo

490
00:27:21.119 --> 00:27:23.519
<v Speaker 7>satellite constellation up and running, and to do that you

491
00:27:23.559 --> 00:27:24.279
<v Speaker 7>need another rock.

492
00:27:24.359 --> 00:27:27.160
<v Speaker 1>Dude. I remember as a kid watching James Bond Double

493
00:27:27.359 --> 00:27:31.079
<v Speaker 1>seven Moonraker and thinking to myself, how ridiculous private people

494
00:27:31.200 --> 00:27:33.880
<v Speaker 1>having their own launch systems. Now it's happening. It's no

495
00:27:33.920 --> 00:27:37.079
<v Speaker 1>longer science fiction yesterday. Science fiction is today science fact.

496
00:27:37.200 --> 00:27:38.519
<v Speaker 7>Absolutely absolutely.

497
00:27:38.519 --> 00:27:42.519
<v Speaker 1>That's Alexeharov Rout from Take Advice, Start Life, and this

498
00:27:42.680 --> 00:28:01.799
<v Speaker 1>is space Time, and that's the show for now. Spacetime

499
00:28:01.839 --> 00:28:04.960
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00:28:10.079 --> 00:28:13.799
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