WEBVTT

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

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

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<v Speaker 1>up on Space Time, it turns out black holes are

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<v Speaker 1>a hundred times more powerful than previously thought. The dramatic

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<v Speaker 1>collision which flipped our Milky Way galaxy and a successful

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<v Speaker 1>return to Worth for the crew of the Sawyers M

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

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<v Speaker 2>Welcome to Space Time with Stewart Gary.

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<v Speaker 1>Astronomers have been forced to rewrite their textbooks on the

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<v Speaker 1>power of supermassive black holes after new observations have shown

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<v Speaker 1>that these cosmic monsters can generate enough energy to impact

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<v Speaker 1>galaxies hundreds of thousands of light years away. Scientists previously

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<v Speaker 1>believe that the impact of winds generated by super massive

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<v Speaker 1>black holes was contained to the host galaxy, but the

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<v Speaker 1>new findings reported in the General Nature Astronomy, reveals that

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<v Speaker 1>the energy produced extends to surrounding galaxies three hundred thousand

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<v Speaker 1>light years away, one hundred times further than previously thought.

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<v Speaker 1>The studies lead author Satashi Yomta from Tohoku University says

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<v Speaker 1>the discovery demonstrates that these explosive winds impact vast expanses

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<v Speaker 1>of space far beyond the galaxies they inhabit. It Mata says.

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<v Speaker 1>Black holes are largely known for sucking in matter, but

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<v Speaker 1>they also eject gas in the form of powerful winds.

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<v Speaker 1>These winds were thought to be contained within the galaxy,

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<v Speaker 1>but your Madas study reveals the force is immensely more

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<v Speaker 1>powerful than previously understood. Your matter and colleagues use the

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<v Speaker 1>CHRISM X ray space telescope to observe the activity of

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<v Speaker 1>a quaser cataloged as H eighteen twenty one plus six

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<v Speaker 1>forty three, located some three point four billion light years

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<v Speaker 1>away in the direction of the constellation. Draco. Quasars are

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<v Speaker 1>extremely luminous jets of energy and matter given off material

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<v Speaker 1>being crushed and stretched in the accretion disk of feeding

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<v Speaker 1>black holes. The rapidly growing black hole containing the quasa

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<v Speaker 1>is located in the center of a galaxy caster, where

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<v Speaker 1>it's driving turbulence and the surrounding hot gas emitting X

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<v Speaker 1>rays in the process. The authors precisely determine the motion

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<v Speaker 1>of the gas by analyzing spectroscopic emission lines from iron ions.

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<v Speaker 1>The observations revealed that the high temperature gas surrounding the

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<v Speaker 1>black hole isn't remaining static, but violently disperses over a

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<v Speaker 1>wide area due to turbulence, and they also confirm that

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<v Speaker 1>the flow of the gas extends far beyond the host galaxy,

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<v Speaker 1>reaching distances of more than three hundred thousand light years.

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<v Speaker 1>The amount of energy involved in the turbulence was approximately

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<v Speaker 1>one hundred times greater than what previous estimates had made,

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<v Speaker 1>and equivalent to several billion supernova explosions, the blasts that

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<v Speaker 1>occur when stars reach the end of their lives. You

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<v Speaker 1>might have says. It's the first time anyone has shown

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<v Speaker 1>that black holes can influence such a broad cosmic environment,

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<v Speaker 1>and it demonstrates that black holes are key drivers of

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<v Speaker 1>gas flow and motion in space, transporting vast amounts of

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<v Speaker 1>energy materials to very distant regions of the cosmos. This

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<v Speaker 1>is space time still to come. The dramatic collision that

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<v Speaker 1>flipped our Milky Way galaxy and a successful return to

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<v Speaker 1>Earth for the crew of the Sawyer's M twenty eight spacecraft.

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<v Speaker 1>All that and more still to come on space time.

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<v Speaker 1>A new study suggest that our home galaxy, the Milky Way,

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<v Speaker 1>may have undergone a dramatic change in orientation following a

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<v Speaker 1>head on collision with another galaxy. The findings, reported to

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<v Speaker 1>the Royal Astronomical Society's conference in Birmingham, help us explain

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<v Speaker 1>a long standing mystery about our galaxy. Using supercomputer simulations

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<v Speaker 1>of galaxies like the Milky Way, astronomers found that galaxies

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<v Speaker 1>with slowly rotating stellar halos are more likely to have

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<v Speaker 1>experienced a major disc flip. That's where the galaxy's disc

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<v Speaker 1>changes its orientation by more than ninety degrees. Most of

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<v Speaker 1>the Milky Way stars are located in the flat spiral

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<v Speaker 1>disc of the galaxy, and surrounding this disc is a

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<v Speaker 1>much larger but spars stellar halo, made up mostly of

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<v Speaker 1>stars that are originally formed in smaller galaxies before being

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<v Speaker 1>pulled into the Milky Way through galactic mergers. Observations by

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<v Speaker 1>the European Space Agency's Guian mission have shown that the

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<v Speaker 1>Milky Way stellar halo rotates very slowly, but astronomers have

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<v Speaker 1>not understood why. So they analyze the evolution of twenty

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<v Speaker 1>five Milky Way like spiral galaxies in the rigious squid

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<v Speaker 1>of cosmological computer simulations, and they followed their development over

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<v Speaker 1>billions of years. They found that galaxies with the slowest

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<v Speaker 1>rotating stellar haloes shared two important features. Each experienced a

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<v Speaker 1>major head on merger or collision with another galaxy, and

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<v Speaker 1>they also underwent a disc flip during their revolution. The

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<v Speaker 1>studies lead author Kirol Batrikov from Durham University says astronomers

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<v Speaker 1>already know that the Milky Way had a massive head

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<v Speaker 1>on collision in the past with a galaxy known as

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<v Speaker 1>the Guy Sausage and Soladus, and this new data suggests

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<v Speaker 1>that may have caused the Milky Way's disc to flip.

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<v Speaker 1>The Guy of Sausage and Soladus was a massive dwarf

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<v Speaker 1>galaxy that collided with and was absorbed into the early

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<v Speaker 1>milky Way somewhere around ten to eleven billion years ago.

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<v Speaker 1>This defighting galactic merger was the largest single event in

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<v Speaker 1>the early history of the Milky Way, and it reshaped

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<v Speaker 1>our galaxy, leaving billions of stars orbiting in a highly

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<v Speaker 1>elongated sausage shaped path. Identifying a past disc flip gives

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<v Speaker 1>astronomers a new way to understand how the Milky Way assembled,

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<v Speaker 1>and it may also provide indirect clues that the motion

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<v Speaker 1>of its invisible dark matter halo. A disc clip also

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<v Speaker 1>means most of the Milky Way stars moved on very

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<v Speaker 1>different trajectories compared to the way they moved today, possibly

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<v Speaker 1>even our own son Any our stable spot in the

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<v Speaker 1>galaxy might not have been quite so stable in the past.

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<v Speaker 1>The study also found that the rotation of the Milky

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<v Speaker 1>Way stellar halo is closely linked to the rotation of

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<v Speaker 1>its dark matter halo, and that suggests the two possibly

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<v Speaker 1>evolve together as the galaxy grew by a creation of

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<v Speaker 1>the smallst satellite galaxies. This is space time still to come.

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<v Speaker 1>A successful return to Earth for the crew of the

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<v Speaker 1>Sawyers M twenty eight. The red super giant antaries, Barnard Star,

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<v Speaker 1>the second Earestar system to the Sun, and the annual

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<v Speaker 1>Percied's meteor shower are among the highlights of the August

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<v Speaker 1>night skies on SkyWatch. The ros Cosmos Sawyers M twenty

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<v Speaker 1>eight spacecraft has returned safely to Earth, bringing home the

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<v Speaker 1>expedition seventy four crew who were spent the past eight

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<v Speaker 1>months aboard the International Space Station. The capsule touchdown of

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<v Speaker 1>the world in script Kazakhstan stick three and a half

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<v Speaker 1>hours after the patting the over the outpost.

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<v Speaker 3>We are covering the return of the Suyu's MS twenty

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<v Speaker 3>eight spacecraft with NASA astronaut Chris Williams and Ross Cosmos

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<v Speaker 3>cosmonauts Sergei Kodsvirzkov and Sergei Mikhaye, returning under its main parachute,

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<v Speaker 3>slowing it down for a touchdown on Earth. We did

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<v Speaker 3>hear confirmation from the crew that everything was nominal or

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<v Speaker 3>as expected on board. That's so us MS twenty eight

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<v Speaker 3>spacecraft suspended under the orange and white parachute, and that

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<v Speaker 3>main parachute covering an area of one thousand meters. It's

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<v Speaker 3>slowing the capsule down to about sixteen miles per hour,

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<v Speaker 3>quite a contrast from the seventeen thousand, five hundred miles

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<v Speaker 3>per hour this crew was traveling just three hours ago.

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<v Speaker 4>You course is how do papy me? I am? This

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<v Speaker 4>is quesche Yas was pretty much us. We read you

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<v Speaker 4>loud and clear.

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<v Speaker 5>I love my space kid, but its.

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<v Speaker 4>Ballistic myths is for seconds. We are in the controlled

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<v Speaker 4>automatic descent. We see you, guys, uh one feeling great, creature,

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<v Speaker 4>two feeling good, three feeling amazing. That is good news, guys.

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<v Speaker 3>Confirmation from the crew themselves that they are are all

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<v Speaker 3>feeling good, great and amazing. The crew also has a

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<v Speaker 3>voice and visual with the search and recovery forces. Russian

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<v Speaker 3>Search and Recovery at vs continue making their way towards

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<v Speaker 3>the anticipated landing site.

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<v Speaker 4>Cious search and rescue forces. What's your altitude?

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<v Speaker 5>Thirty start for them?

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<v Speaker 4>Our altitude is three kilometers seven fifty meters. Oxidizer jobs

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<v Speaker 4>figure on.

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<v Speaker 5>Matter, I apprecail a point at you.

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<v Speaker 3>As the crew continues drifting down to Earth under that parachute.

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<v Speaker 4>The aiometric altitude on the INPU panel is three kilometers.

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<v Speaker 3>The next major milestone, and essentially the final milestone just

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<v Speaker 3>before landing, is the soft landing engine firing says when

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<v Speaker 3>six engines will fire to slow the descent rate to

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<v Speaker 3>one point five meters per second, so just over three

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<v Speaker 3>miles an hour when soy US is less than one

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<v Speaker 3>meter above the ground. So the spacecraft now traveling about

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<v Speaker 3>sixteen miles per hour ahead of those soft landing engines

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<v Speaker 3>that fire just before touchdown to help ease the return

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<v Speaker 3>to Earth. And a reminder that radio beacon that you

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<v Speaker 3>is completely normal. This is establishing communications that begon coming

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<v Speaker 3>from the spacecraft. You're hearing communications to and from the

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<v Speaker 3>SWAYUS MS twenty eight spacecraft. Once you're hearing that of

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<v Speaker 3>Commander Sergei Kidsfirzkov Ross Cosmos cosmonauts speaking with the mission

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<v Speaker 3>control team in Moscow again. Conditions at the landing site.

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<v Speaker 3>Visibility about six miles with twenty four mile per hour

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<v Speaker 3>winds and eighty eight degrees fahrenheit.

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<v Speaker 4>This is questions. I'm getting to nine hundred meters, hold

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<v Speaker 4>your arms close to the body and please.

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<v Speaker 5>Do not speak your globo docture and.

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<v Speaker 4>This is going to stay true all the way and

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<v Speaker 4>still handing.

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<v Speaker 3>Landing now less than thirty seconds away. Crew receiving final

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<v Speaker 3>instructions as they prepare for.

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<v Speaker 4>Touchdown reference altitude, braceful landing.

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<v Speaker 3>Touchdown. Chris Williams, Sergei Mikaev, and Sergi Kispertzhkov have returned

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<v Speaker 3>to their home planet at five twenty seven am Central

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<v Speaker 3>time three twenty seven pm in Kazakhstanzois.

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<v Speaker 4>Is on its side and there is no fire. That's

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<v Speaker 4>the rescue force is reporting all right, and the helicopters

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<v Speaker 4>approaching to land.

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<v Speaker 3>So I heard the call that the Soyus is on

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<v Speaker 3>its side. This is not uncommon for the Soyuz, and

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<v Speaker 3>the crew will be extracted from the spacecraft upon the

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<v Speaker 3>recovery forces arriving at the capsule.

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<v Speaker 1>The two hundred and forty one day mission launched from

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<v Speaker 1>the Bike and or Cosmo drove and the Central Asian

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<v Speaker 1>Republic of Kasek stand back on November the twenty seventh

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<v Speaker 1>and involved obening the Earth some three thousand, eight hundred

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<v Speaker 1>and fifty six times, traveling more than one hundred and

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<v Speaker 1>sixty million kilometers. While on station, the crew were involved

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<v Speaker 1>in more than two hundred and fifty scientific experiments, including

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<v Speaker 1>research on new cancer treatments and improving in space manufacturing

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<v Speaker 1>of materials used in high performance computers and electronics. They

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<v Speaker 1>also undertook two extra vehicular activities or EVAs NASA speKt

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<v Speaker 1>for spacewalks. These were designed to prepare for station power

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<v Speaker 1>system upgrades and to replace a faulty joint in the

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<v Speaker 1>Canada ARM two robotic arm. For more than twenty five

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<v Speaker 1>years now, people have lived and worked continuously in space

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<v Speaker 1>aboard the International Space Station. The Orbiting our Post is

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<v Speaker 1>helping NASA understand and overcome the challenges of human spaceflight

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<v Speaker 1>for long duration missions to the Moon and eventually onto

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<v Speaker 1>Mars and beyond. As part of the Artemis program, However,

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<v Speaker 1>the space station's future is now limited, with NASA planning

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<v Speaker 1>to deorbit one hundred and nine meter long four hundred

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<v Speaker 1>and twenty one our posts sometime in late twenty thirty

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<v Speaker 1>or early twenty thirty one. It'll be replaced by smaller

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<v Speaker 1>commercial space stations and a major expansion of China's Tiangong

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<v Speaker 1>space station, which will double its size this space time

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<v Speaker 1>and Time Out of turn oives to the skies and

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<v Speaker 1>check out the celestiousphere for August on SkyWatch. August is

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<v Speaker 1>the eighth month of the year in the Julian Engagorian calendars.

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<v Speaker 1>It was originally named six Tillius in Latin because it

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<v Speaker 1>was the sixth month of the original ten month Roman

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<v Speaker 1>calendar under Romulus in seven fifty three BCE, when the

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<v Speaker 1>year started in March. It only became the eighth month

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<v Speaker 1>when January and February were added to the start of

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<v Speaker 1>the year in the year eight BCE. It was renamed

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<v Speaker 1>in honor of the Roman statesmen and military leader Augustus,

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<v Speaker 1>who had achieved several military victories, including the conquest of Egypt.

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<v Speaker 1>During the month. Okay, turning to the heavens and the

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<v Speaker 1>constellation s, the Scorpion is high overhead this time of year,

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<v Speaker 1>covering almost a third of the August night skies. At

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<v Speaker 1>the heart of Scorpius, located some four hundred and seventy

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<v Speaker 1>light years away, is the red super giant Antaries. A

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<v Speaker 1>light year is a distance of about ten trillion kilometers,

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<v Speaker 1>a distance of photon can travel in a year at

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<v Speaker 1>three hundred thousand kilometres per second, the speed of light

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<v Speaker 1>in a vacuum and the ultimate speed limit of the universe.

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<v Speaker 1>The name Antaries means rival of Mars, and indeed, when

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<v Speaker 1>they're close together in the sky, they do look very similar.

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<v Speaker 1>And Tari's, or Alpha Scorpius that's sometimes called has some

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<v Speaker 1>twelve point four times the mass and an incredible four

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<v Speaker 1>hundred and fifty times the diameter of our Sun and

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<v Speaker 1>is one of the largest known stars in the universe.

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<v Speaker 1>And Tari's is so big that wordplace where the Sun

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<v Speaker 1>is at the center of our solar system, it would

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<v Speaker 1>engulf all the inner planets Mercury, Venus, Earth, and Mars.

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<v Speaker 1>It's outer surface would rich almost as far as the

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<v Speaker 1>orbit of Jupiter. And Tari's is a binary system, there's

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<v Speaker 1>a companion style orbiting with it called Antari's B, a

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<v Speaker 1>massive spectual type B blue white star at least seven

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<v Speaker 1>point two times the mass and five point two times

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<v Speaker 1>the radius of the Sun. It's located about two hundred

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<v Speaker 1>and twenty four astronomical units beyond the primary star. An

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<v Speaker 1>astronomical unit is the average distance between the Sun and

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<v Speaker 1>the Earth, about one hundred and fifty million kilometers or

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<v Speaker 1>eight point three light minutes. Astronomers describe stars in terms

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<v Speaker 1>of spectual types, a classification system based on temperature and characteristics.

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<v Speaker 1>The hottest, most massive, and most luminous stars are known

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<v Speaker 1>spectro type O blue stars. They're closely followed by spectual

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<v Speaker 1>type B blue white stars, the n spectual type A

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<v Speaker 1>white stars, spetual type F whitish yellow stars, spectro type

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<v Speaker 1>G yellow stars. That's where our Sun fits in, special

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<v Speaker 1>type K orange stars, and the coolest and least massive

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<v Speaker 1>of all stars are spectual type M red stars, commonly

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<v Speaker 1>referred to as red dwarfs. Each spectral classification is further

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<v Speaker 1>subdivided using a numeric digit to represent temperature, with zero

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<v Speaker 1>being the hottest and nine the coolest, and a Roman

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<v Speaker 1>uneral to represent luminosity. Now put all that together, and

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<v Speaker 1>our sun is a special type G two V or

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<v Speaker 1>G two five yellow dwarf star. Also included in the

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<v Speaker 1>stellar classification system are special types LT and Y, which

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<v Speaker 1>are assigned to feldstars known as brown dwarves, some of

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<v Speaker 1>which were actually born as spectral type M red dwarf stars,

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<v Speaker 1>but became brown dwarves after losing some of their mass.

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<v Speaker 1>Brown dwarfs fitted to a category between the largest planets,

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<v Speaker 1>which are about thirteen times the mass of Jupiter, and

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<v Speaker 1>the smallest spectral type M red dwarf stars, which are

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<v Speaker 1>about seventy five to eighty times the mass of Jupiter

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<v Speaker 1>or zero point zero eight solar masses. Located near antaries

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<v Speaker 1>is the spectacular globular cluster Messi four or M four

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<v Speaker 1>for short, named after the eighteenth century of frenchist ronomoer

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<v Speaker 1>and commet hunter Charles Messier, It's one of a catalog

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<v Speaker 1>of one hundred and three fuzzy objects which weren't comets

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<v Speaker 1>and so were of no interest to Messier, and so

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<v Speaker 1>he made a list of them so he didn't waste

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<v Speaker 1>his time looking at them. Other astronomers have since added

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<v Speaker 1>further celestial objects to the catalog, bringing the turtle to

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<v Speaker 1>around one hundred and ten. Located some seven thousand light

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<v Speaker 1>years away, messi at four can be seen through a

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<v Speaker 1>pair of binoculars, making it one of the closest globular

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<v Speaker 1>clusters to Earth. Globular clusters are densely packed fees containing

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<v Speaker 1>thousands to millions of gravitationally bounced stars, which it's thought

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<v Speaker 1>were either originally all born at the same time in

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<v Speaker 1>the same stellar nursery, or of the surviving cause of

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<v Speaker 1>galaxies that have been cannibalized by larger galaxies. They're almost

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<v Speaker 1>always found orbiting the halo of galaxies. The Milky Way

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<v Speaker 1>has about one hundred and fifty of them, and they're

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<v Speaker 1>all usually very ancient, some dating back to around twelve

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<v Speaker 1>billion years. Located just below the sting of Scorpius are

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<v Speaker 1>two open star clusters M six and M seven. M

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<v Speaker 1>sevens the nearer of the two, located about eight hundred

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<v Speaker 1>light years away, while M six is a more distant

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<v Speaker 1>two thousand light years. Open clusters are less densely packed

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<v Speaker 1>than their globular cluster counterparts, with the stars inside them

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<v Speaker 1>less gravitationally bound and more prone to drifting away over time.

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<v Speaker 1>Another open star cluster in Scorpius is NNGC sixty two

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<v Speaker 1>to thirty one, located about six five hundred light years away,

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<v Speaker 1>just near the stars Zeta Scorpii. NGC sixty two thirty

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<v Speaker 1>one is a bright, open star cluster containing around one

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<v Speaker 1>hundred and twenty stars, including a significant population of highly

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<v Speaker 1>luminous supergiants, numerous white yellow stars, and at least two

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<v Speaker 1>Wolfrayet stars. Wolfrayets are extremely luminous evolved stars reaching the

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<v Speaker 1>ends of their lives. Having run out of hydrogen for

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<v Speaker 1>core fusion. They're no longer on the main sequence and

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<v Speaker 1>are instead fusing progressively heavier and heavier elements in their cores.

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<v Speaker 1>This causes them to have surface temperatures of up to

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<v Speaker 1>two hundred thousand degrees celsius, and such extreme temperatures generate

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<v Speaker 1>powerful stellar winds. Just behind Scorpius is the constellation Sagittarius,

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<v Speaker 1>the half man, half horse of Greek mythology, and as

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<v Speaker 1>we mentioned in last month SkyWatch, the center of the

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<v Speaker 1>Milky Way galaxy is found in Sagittarius, roughly twenty seven

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<v Speaker 1>thousand light years away. The name Sagittarius could be traced

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<v Speaker 1>back beyond the Greeks to the ancient Mesopotamian archer god Nergel.

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<v Speaker 1>Sagittarius is known for its many nebula and clusters, more

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<v Speaker 1>than any other constellation. One of the largest and brightest

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<v Speaker 1>is the globular cluster M twenty two, big enough to

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<v Speaker 1>be visible to the unaided eye, located about ten thousand,

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<v Speaker 1>six hundred light years away near the galactic bulge. M

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<v Speaker 1>twenty two is more elliptical the most globular clusters. It's

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<v Speaker 1>located just south of the ecliptic that're played in the

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<v Speaker 1>sky upon which all the planets orbit the Sun, and

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<v Speaker 1>it contains over seventy thousand stars covering an area of

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<v Speaker 1>around one hundred light years. It also contains at least

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<v Speaker 1>two black holes, and he's one of only a handful

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<v Speaker 1>of globular clusters known to contain planetary nebulae, the puffed

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<v Speaker 1>off outer gases envelopes of dead sun like stars. Located

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<v Speaker 1>in the sky next to Scorpius in the western Sagittarius

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<v Speaker 1>in the east is the constellation of Fayusius, the healer

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<v Speaker 1>or serpent bearer, often betrayed as a snake coiled around

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<v Speaker 1>a man in Greek mythology, Opaiucius raises a rind from

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<v Speaker 1>the dead after he was bitten by Scorpius O Fa

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<v Speaker 1>Yushius contains several star clusters and other interesting features, including

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<v Speaker 1>Barnard Star. Barnard Star is the second nearest star system

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<v Speaker 1>to the Sun, beaten only by the Alphasentaury Triple star system,

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<v Speaker 1>located some five point nine light years away. Barnard Star

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<v Speaker 1>is a spectral type M red dwarf, about zero point

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<v Speaker 1>one four four times the mass of the Sun. Our

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<v Speaker 1>Sun is around four point six billion years old. At

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<v Speaker 1>between seven and twelve billion years of ever age, Barnard's

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<v Speaker 1>Star is considerably older than the Sun and maybe among

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<v Speaker 1>the oldest stars in the Milky Way galaxy. It's lost

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<v Speaker 1>a great deal of rotational energy, and its periodic slight

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<v Speaker 1>changes in brightness indicate that it's rotating about once every

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<v Speaker 1>one hundred and thirty days. By comparison, our Sun rotates

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<v Speaker 1>roughly once every twenty nine days. Given its age, Bernard

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<v Speaker 1>Star was long assumed to be quiercent in terms of

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<v Speaker 1>stellar activity, but in nineteen ninety eight astronoms observed an

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<v Speaker 1>intense stellar flare, indicating that Barnard Star is indeed a flare.

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<v Speaker 1>Star flare stars of variable stars they can undergo unpredictable

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<v Speaker 1>dramatic increases in brightness, lasting a few minutes. It's believed

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<v Speaker 1>that the flares of flare stars are analogous to solar

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<v Speaker 1>flares in the Sun, and that they're generated by stellar

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<v Speaker 1>magnetic energy stored in the star's atmosphere. Lying just to

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<v Speaker 1>the west of the scorpion is the constellation Libra at

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<v Speaker 1>the scales. In Greek mythology, Libra represents the core of

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<v Speaker 1>Scorpius the scorpion. However, the Romans considered Libra a distinct,

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<v Speaker 1>separate constellation from Scorpius, and thought them to be the

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<v Speaker 1>scales symbolizing the equinoxes, the times of the year in

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<v Speaker 1>March and September, when the Earth gets equal lengths of

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<v Speaker 1>day and night. That's because two thousand years ago, when

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<v Speaker 1>all this was made up, the Sun moved into Libre

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<v Speaker 1>at the time of the September equinox, but due to procession,

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<v Speaker 1>as the Earth Spentax's wobbles in direction, this point in

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<v Speaker 1>time has now moved into the adjoining constellation of Virgo.

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<v Speaker 1>If you look to the south and the southern cross,

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<v Speaker 1>that's the constellation Centaurus. Another half man, half horse mythical

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<v Speaker 1>beast Centaurus was the teacher of many of the Greek

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<v Speaker 1>gods and heroes. He was placed among the stars in

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<v Speaker 1>the heavens after accidentally being kured by a poisoned arrow

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<v Speaker 1>fired by Hercules close to the point of star nearest

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<v Speaker 1>the southern cross. Beta Centauri lies NNGC fifty one thirty nine.

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<v Speaker 1>Omega Centauri the largest and brightest globular cluster in the

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<v Speaker 1>visible sky. Because of its brightness, the ancient Greek mathematician

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<v Speaker 1>and astronomer Claudius Ptolemy originally thought Amiga Centauri was a star.

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<v Speaker 1>It has a diameter of more than one hundred and

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<v Speaker 1>fifty light years and contains an estimated ten million stars,

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<v Speaker 1>giving it some four million times the mass of our Sun.

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<v Speaker 1>Located some fifteen thy eight hundred light years away, Amiga

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<v Speaker 1>Centauri is another very ancient globular cluster, around twelve billion

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<v Speaker 1>years old, and it contains many so called population two stars.

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<v Speaker 1>These are the second generation of stars to have formed,

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<v Speaker 1>and were created directly out of the remains of the

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<v Speaker 1>very first stars in the universe. Stars in the core

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<v Speaker 1>of Amiga Centauri are so crowded yarreestimated to average only

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<v Speaker 1>zero point one light years away from each other, and

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<v Speaker 1>that compares to the nearest start of our sun proximate century,

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<v Speaker 1>which is some four point two light years distant. Located

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<v Speaker 1>close to a megasentaurium the sky is the giant lenticular

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<v Speaker 1>galaxy NNGC fifty one twenty eight Centaurus A, which we

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<v Speaker 1>see looking like it's split in half by a thick

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<v Speaker 1>band of dust. The galaxy was discovered in eighteen twenty

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<v Speaker 1>six by astronomer James Dunlop from his home in what

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<v Speaker 1>is now the Sydney suburb of Paramatta, a time long

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<v Speaker 1>before the bright lights of a modern city would make

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<v Speaker 1>such a discovery impossible. Located some thirteen million light years away,

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<v Speaker 1>Centaurus is one of the strongest radio sources in the

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<v Speaker 1>sky and is thought to be the result of a

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<v Speaker 1>merger between an elliptical and a spiral galaxy. It can

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<v Speaker 1>easily seen using a pair of binoculars, but you'll need

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<v Speaker 1>a telescope to make out its spectacular dust lanes. August

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<v Speaker 1>is also the time of the peak of the annual

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<v Speaker 1>Percied's meteor shower. The meteors are the debris trail ejected

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<v Speaker 1>by the comets with tuttle as it travels along its

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<v Speaker 1>one hundred and thirty three year orbit through the Solar System.

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<v Speaker 1>As its name suggests, the perseed's radiant that is the

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<v Speaker 1>point of the sky from which the meteors appear to originate.

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<v Speaker 1>It lies in the constellation of Perseus. The Perseids one

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<v Speaker 1>of the oldest known meteor showers, with early Chinese historical

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<v Speaker 1>records of its activity going back almost two thousand years.

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<v Speaker 1>They're active between July seventeenth and August twenty fourth, with

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<v Speaker 1>a peak on August twelfth, with around sixty meteors an

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<v Speaker 1>hour being visible. The Perseids are very bright and fast

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<v Speaker 1>moving meteors traveling at speeds of fifty nine kilometres per second.

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<v Speaker 1>The best scene between midnight and just before dawn, producing long,

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<v Speaker 1>bright trails and some fireballs. Most Perseids burn up in

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<v Speaker 1>the atmosphere altitudes of over eighty kilometers. Their best scene

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<v Speaker 1>from the northern hemisphere, so for southern hemisphere sky watchers

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<v Speaker 1>look to the north, with the radiant below the northern

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<v Speaker 1>horizon and joining us Now for the rest of our

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<v Speaker 1>tour of the August night skies. Senior science writer and

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<v Speaker 1>sky n tell Uscout magazine contributor Jonathan Nally.

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<v Speaker 5>Day Stuart well as winter here in AUSTRALAISA, so that

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<v Speaker 5>means that stargaze is down here have at their disposal

416
00:25:58.480 --> 00:26:00.279
<v Speaker 5>the thickest part of the Milky Way and the center

417
00:26:00.319 --> 00:26:02.119
<v Speaker 5>of our galaxy to view up there in the night sky.

418
00:26:02.240 --> 00:26:04.240
<v Speaker 5>So if you go outside in the mid evening during

419
00:26:04.279 --> 00:26:06.680
<v Speaker 5>August to find the Milky Way stretching across the sky

420
00:26:06.759 --> 00:26:08.880
<v Speaker 5>from the northeast all the way down to the southwest,

421
00:26:08.920 --> 00:26:10.640
<v Speaker 5>and the center of the Milky Way in the region

422
00:26:10.640 --> 00:26:13.559
<v Speaker 5>of Sangitarius is pretty much directly overhead for those that

423
00:26:13.720 --> 00:26:16.039
<v Speaker 5>roughly the latitude of Sydney. The Milky Way, of course,

424
00:26:16.119 --> 00:26:18.400
<v Speaker 5>is just our galaxy scene from the inside. Most of

425
00:26:18.440 --> 00:26:20.759
<v Speaker 5>its stars are too far away and dim to be

426
00:26:20.799 --> 00:26:23.279
<v Speaker 5>seen individually, so if you add them all up collectively,

427
00:26:23.440 --> 00:26:25.799
<v Speaker 5>light adds up to form a sort of hazy band

428
00:26:25.799 --> 00:26:28.000
<v Speaker 5>of lights stretching across the sky. It looks really bright

429
00:26:28.000 --> 00:26:30.759
<v Speaker 5>and prominent. If you have dark skies throughout the countryside

430
00:26:30.799 --> 00:26:32.680
<v Speaker 5>and you've let your eyes adapted to the darkness to

431
00:26:32.720 --> 00:26:34.839
<v Speaker 5>the night sky. Takes about twenty minutes or so to

432
00:26:34.839 --> 00:26:36.920
<v Speaker 5>get your eyes dark adapted. So if you're out there

433
00:26:36.960 --> 00:26:39.599
<v Speaker 5>in the bush or a desert or a rural area.

434
00:26:39.759 --> 00:26:41.759
<v Speaker 5>If we call of the bush in Australia, then you

435
00:26:41.759 --> 00:26:43.640
<v Speaker 5>should get a really nice view of the Milky Way.

436
00:26:43.680 --> 00:26:47.000
<v Speaker 5>If you have even mild light pollution around, then it

437
00:26:47.079 --> 00:26:48.920
<v Speaker 5>starts to drown out the haze of the Milky Way,

438
00:26:48.960 --> 00:26:50.559
<v Speaker 5>so it might be very dem or hard. It's hard

439
00:26:50.559 --> 00:26:52.519
<v Speaker 5>to see. And if you live in heavily light pollute

440
00:26:52.559 --> 00:26:54.759
<v Speaker 5>the suburbia, well just forget it. You'ren't going to see

441
00:26:54.759 --> 00:26:56.680
<v Speaker 5>the Milky Way, which is a real shame because when

442
00:26:56.680 --> 00:26:58.519
<v Speaker 5>I was growing up, you could even in suburbia because

443
00:26:58.519 --> 00:27:00.519
<v Speaker 5>there won't have so many lights around. I don't remember

444
00:27:00.559 --> 00:27:02.440
<v Speaker 5>when I was growing up in the city. I was

445
00:27:02.440 --> 00:27:04.920
<v Speaker 5>in too many decicated too many decades ago to mention.

446
00:27:05.000 --> 00:27:06.559
<v Speaker 5>They used to turn all the street lights off late

447
00:27:06.599 --> 00:27:08.720
<v Speaker 5>at night. I think partly because there were very few

448
00:27:08.759 --> 00:27:11.599
<v Speaker 5>people driving around, and also at the time I think

449
00:27:11.599 --> 00:27:13.559
<v Speaker 5>there was a bit of a just general power shortage

450
00:27:13.599 --> 00:27:16.480
<v Speaker 5>in our state. Needed to build more power station moving,

451
00:27:16.559 --> 00:27:18.519
<v Speaker 5>so there's to conserve a bit of energy and save

452
00:27:18.559 --> 00:27:20.440
<v Speaker 5>a bit of coal and turn the lights off later.

453
00:27:21.240 --> 00:27:26.359
<v Speaker 1>Melbourne, Yeah, Melbourne, Melbourne, Victoria, Yeah, but I had that

454
00:27:26.400 --> 00:27:28.279
<v Speaker 1>in Sydney they were on to the Meltman came in

455
00:27:28.279 --> 00:27:28.599
<v Speaker 1>the morning.

456
00:27:28.640 --> 00:27:30.079
<v Speaker 5>Yeah, I think. I think in Melbourne at the time.

457
00:27:30.240 --> 00:27:34.119
<v Speaker 5>Melbourne was a huge influx of migration after World War two,

458
00:27:34.400 --> 00:27:36.480
<v Speaker 5>and that's the stacks of people and it was growing

459
00:27:36.599 --> 00:27:39.720
<v Speaker 5>very quickly and they just needed to build small power

460
00:27:39.720 --> 00:27:42.160
<v Speaker 5>stations and they at least turned the lights off just

461
00:27:42.160 --> 00:27:44.160
<v Speaker 5>to conserve a bit of energy, I think, And I

462
00:27:44.200 --> 00:27:46.559
<v Speaker 5>remember blackouts, you know, when there simply wasn't enough power.

463
00:27:46.559 --> 00:27:48.400
<v Speaker 5>But anyway, did a little bit off topic the well,

464
00:27:48.599 --> 00:27:50.359
<v Speaker 5>blackouts are good for a stargaze and of course, but

465
00:27:50.400 --> 00:27:52.119
<v Speaker 5>it's not good for other things. So we were all

466
00:27:52.240 --> 00:27:53.759
<v Speaker 5>up to well anyway. So yeah, so the center of

467
00:27:53.799 --> 00:27:57.039
<v Speaker 5>our galaxy is really good thing. It's a focus of

468
00:27:57.079 --> 00:27:58.960
<v Speaker 5>a lot of attention for as drammas actually, and it's

469
00:27:58.960 --> 00:28:00.200
<v Speaker 5>one of the reasons why they were saying and in

470
00:28:00.200 --> 00:28:03.720
<v Speaker 5>professional and semi professional observatories located in the southern hemisphere,

471
00:28:03.720 --> 00:28:05.759
<v Speaker 5>because when we look in the direction of our galaxy's core,

472
00:28:05.920 --> 00:28:08.519
<v Speaker 5>we're actually looking through the densest and deeper section of

473
00:28:08.519 --> 00:28:10.119
<v Speaker 5>the Milky Way. So there are lots of things to

474
00:28:10.119 --> 00:28:13.240
<v Speaker 5>see what astronomers called deep sky objects. We've got star

475
00:28:13.319 --> 00:28:16.920
<v Speaker 5>clusters of both kinds, open and open and golobular we've

476
00:28:16.960 --> 00:28:19.839
<v Speaker 5>got bright and dark Nebulay got law, And of course

477
00:28:19.839 --> 00:28:21.920
<v Speaker 5>for the professional astronomers, we've got the right sort of

478
00:28:21.960 --> 00:28:24.119
<v Speaker 5>year to study it. They can look right into the

479
00:28:24.160 --> 00:28:26.240
<v Speaker 5>heart of the Milky Way, into the area where the

480
00:28:26.240 --> 00:28:28.920
<v Speaker 5>black hole is that lives right in the core of

481
00:28:28.920 --> 00:28:31.319
<v Speaker 5>our galaxy. Our friends in the northern half of the sky, yes,

482
00:28:31.400 --> 00:28:33.359
<v Speaker 5>say the United States through in the southern United States,

483
00:28:33.359 --> 00:28:35.519
<v Speaker 5>you can certainly see the Sagittarias and see most of

484
00:28:35.519 --> 00:28:37.720
<v Speaker 5>the dead, But the further north you go, it starts

485
00:28:37.720 --> 00:28:40.039
<v Speaker 5>starting to get really low on the horizon and hard

486
00:28:40.039 --> 00:28:42.559
<v Speaker 5>to see or even below the horizon if you're quite

487
00:28:42.559 --> 00:28:45.440
<v Speaker 5>far north, because it is a southern constellation. So yes,

488
00:28:45.559 --> 00:28:47.359
<v Speaker 5>it's a lucky thing for us down in the southern

489
00:28:47.359 --> 00:28:50.319
<v Speaker 5>minisphere that we've got the center of our galaxy nicely overhead.

490
00:28:50.319 --> 00:28:53.160
<v Speaker 5>That's partly because just where it is in space compared

491
00:28:53.200 --> 00:28:55.759
<v Speaker 5>to us, and of course the tilt of our planet,

492
00:28:55.839 --> 00:28:58.279
<v Speaker 5>so we're a bit lucky in that way. Now, further

493
00:28:58.319 --> 00:29:00.240
<v Speaker 5>down in the south, we've got the other famous thing

494
00:29:00.279 --> 00:29:02.319
<v Speaker 5>that you can see down here, which is the Southern Cross.

495
00:29:02.359 --> 00:29:04.599
<v Speaker 5>It's in the southwest at the moment, got halfway up

496
00:29:04.640 --> 00:29:06.799
<v Speaker 5>from the horizon and lying on its right hand side.

497
00:29:06.880 --> 00:29:09.279
<v Speaker 5>The Southern Cross area is within the Milky Way, the

498
00:29:09.279 --> 00:29:11.839
<v Speaker 5>band of the Milky Way and stretching away from the

499
00:29:11.920 --> 00:29:14.680
<v Speaker 5>Cross in the line northwards along the Milky Way, there

500
00:29:14.680 --> 00:29:17.759
<v Speaker 5>are lots of other really interesting constellations to have a

501
00:29:17.759 --> 00:29:20.000
<v Speaker 5>lookout constellation. It's just an area of the sky. In

502
00:29:20.039 --> 00:29:22.880
<v Speaker 5>the old days, the constellation was like a stick figure arrangement,

503
00:29:22.920 --> 00:29:24.799
<v Speaker 5>you know, joined the dots of stars and it let's

504
00:29:24.799 --> 00:29:27.160
<v Speaker 5>a triangle or a this or that, or an animal

505
00:29:27.240 --> 00:29:29.920
<v Speaker 5>or some kind or These days, as far as astronomous concerned,

506
00:29:29.920 --> 00:29:32.400
<v Speaker 5>it's just an area of sky. But there's lots of

507
00:29:32.440 --> 00:29:35.079
<v Speaker 5>lots of interesting constellations along me. You've got Centaurus, which

508
00:29:35.119 --> 00:29:38.000
<v Speaker 5>is near the southern Cross. You've got Scorpius, Scorpio. You's

509
00:29:38.000 --> 00:29:41.039
<v Speaker 5>got Saburtarius we've mentioned, and another one called Stutum. Now

510
00:29:41.279 --> 00:29:43.359
<v Speaker 5>a lot a lot of people outside of astronomy have

511
00:29:43.400 --> 00:29:45.839
<v Speaker 5>heard of Centaurus, and fewer still have heard of Scrutem.

512
00:29:45.920 --> 00:29:49.519
<v Speaker 5>As the name suggests, Scutum is named after a scooter,

513
00:29:49.799 --> 00:29:51.960
<v Speaker 5>but it's not the kind of scooter with two wheels

514
00:29:52.000 --> 00:29:54.039
<v Speaker 5>that cool people like me right around on Stewart, you know,

515
00:29:54.079 --> 00:29:57.920
<v Speaker 5>it's named after a Scooter s cut a, which is

516
00:29:57.960 --> 00:30:01.119
<v Speaker 5>a Latin word for the type of ancient Roman shield,

517
00:30:01.160 --> 00:30:04.400
<v Speaker 5>and scooter is Scooter is the constellation of the shield. Now,

518
00:30:04.400 --> 00:30:06.519
<v Speaker 5>if you're out there stargazing for long enough, as night

519
00:30:06.599 --> 00:30:08.599
<v Speaker 5>goes on and the Earth turns, you'll notice that from

520
00:30:08.640 --> 00:30:11.039
<v Speaker 5>our vantage point, the band of the Milky Way appears

521
00:30:11.039 --> 00:30:13.400
<v Speaker 5>to shift. So I said earlier on that are stretching

522
00:30:13.440 --> 00:30:16.440
<v Speaker 5>across the night sky from the northeast to the southwest. Well,

523
00:30:16.480 --> 00:30:19.200
<v Speaker 5>as the Earth turns, the Milkie Way and in the

524
00:30:19.279 --> 00:30:22.440
<v Speaker 5>night sky moves seems to move as well. So by

525
00:30:22.480 --> 00:30:25.400
<v Speaker 5>the time you get to early morning, it's no longer

526
00:30:25.440 --> 00:30:28.200
<v Speaker 5>a right overhead, it's now all the way around the horizon.

527
00:30:28.279 --> 00:30:31.200
<v Speaker 5>And that's just simply because our viewpoint has changed. And

528
00:30:31.240 --> 00:30:33.000
<v Speaker 5>then the next night of courses the Earth has turned

529
00:30:33.000 --> 00:30:34.720
<v Speaker 5>to more it'll be back and roughly the same part

530
00:30:34.720 --> 00:30:36.480
<v Speaker 5>of the night sky. So if you're a morning person,

531
00:30:36.599 --> 00:30:38.839
<v Speaker 5>there is plenty to see, particularly in the eastern half

532
00:30:38.880 --> 00:30:41.599
<v Speaker 5>of the sky. And this includes the constellation of Ryan

533
00:30:41.720 --> 00:30:44.559
<v Speaker 5>the Hunter, where it's bright stars rideal and Beetlejuice, and

534
00:30:44.599 --> 00:30:46.720
<v Speaker 5>it's very easy to see group of three stars in

535
00:30:46.759 --> 00:30:49.759
<v Speaker 5>a row which formed the built of the mythological figures clothing.

536
00:30:49.880 --> 00:30:52.160
<v Speaker 5>I always remember as a kid that these three stars

537
00:30:52.200 --> 00:30:54.519
<v Speaker 5>stood out, and I didn't know anything about astronomy really

538
00:30:54.640 --> 00:30:56.599
<v Speaker 5>or constellations things back then. I just new to do

539
00:30:56.640 --> 00:30:58.519
<v Speaker 5>as a part of the sky where there's really three

540
00:30:58.559 --> 00:31:02.240
<v Speaker 5>stars and the perfect line, perfectly sort of equally separated,

541
00:31:02.400 --> 00:31:04.279
<v Speaker 5>and I always just look for them and now, and

542
00:31:04.480 --> 00:31:06.559
<v Speaker 5>of course that is part of the constellation Orion. A

543
00:31:06.559 --> 00:31:08.519
<v Speaker 5>little way from Orion, not too far around to the

544
00:31:08.599 --> 00:31:10.960
<v Speaker 5>right or the south, you'll find Serious, which is the

545
00:31:10.960 --> 00:31:13.599
<v Speaker 5>brightest star in the night sky. And further around to

546
00:31:13.599 --> 00:31:15.480
<v Speaker 5>the right you've got the star Canopus, which is the

547
00:31:15.519 --> 00:31:17.960
<v Speaker 5>second brightest star of the night's sky. Canopus is quite

548
00:31:18.119 --> 00:31:20.640
<v Speaker 5>deep into the southern part of the heavens. So a

549
00:31:20.680 --> 00:31:22.359
<v Speaker 5>lot of people look for the equator, don't get a

550
00:31:22.440 --> 00:31:24.039
<v Speaker 5>view of it at all because it's down below the

551
00:31:24.119 --> 00:31:26.279
<v Speaker 5>horizon for them. Now, so is the planet's scope. For

552
00:31:26.279 --> 00:31:28.279
<v Speaker 5>August this year, at least, there's only one we can

553
00:31:28.319 --> 00:31:30.640
<v Speaker 5>see actually in the early evening sky, and that's a venus.

554
00:31:30.839 --> 00:31:33.640
<v Speaker 5>You simply can't miss it. Wait, stuff get dark, when

555
00:31:33.720 --> 00:31:35.559
<v Speaker 5>the sun's gone down, and look in the western half

556
00:31:35.559 --> 00:31:37.000
<v Speaker 5>of the sky, and there it is big and bright

557
00:31:37.039 --> 00:31:38.359
<v Speaker 5>when I was looking at it just the other night,

558
00:31:38.400 --> 00:31:41.039
<v Speaker 5>and it's really quite spectacular. In particular, have a look

559
00:31:41.079 --> 00:31:43.279
<v Speaker 5>on the sixteenth if you can, the sixteenth of August,

560
00:31:43.319 --> 00:31:45.559
<v Speaker 5>if you got clear weather, and you'll see Venus in

561
00:31:45.599 --> 00:31:48.240
<v Speaker 5>the moon quite close together. That should look pretty spectacular.

562
00:31:48.319 --> 00:31:50.559
<v Speaker 5>Getting closer to midnight, there's a second planet now, so

563
00:31:50.640 --> 00:31:52.839
<v Speaker 5>we've got Saturn rising out of the eastern horizon around

564
00:31:52.839 --> 00:31:55.519
<v Speaker 5>about midnight. It just looks like a fairly bright, slightly

565
00:31:55.640 --> 00:31:57.799
<v Speaker 5>yellowish star. If you can get a telescope onto it,

566
00:31:57.880 --> 00:31:59.640
<v Speaker 5>even a small one, you'd be able to see the rings.

567
00:32:00.000 --> 00:32:02.519
<v Speaker 5>It's always pretty good sat and never ever disappoints. You

568
00:32:02.599 --> 00:32:04.359
<v Speaker 5>have to wait until about four o'clock in the morning

569
00:32:04.440 --> 00:32:06.720
<v Speaker 5>until the next planet makes an appearance, and that's Mars

570
00:32:06.799 --> 00:32:09.200
<v Speaker 5>that will come up over the horizon just after four o'clock.

571
00:32:09.359 --> 00:32:12.240
<v Speaker 5>It looks like a sort of a reddish orange, medium

572
00:32:12.319 --> 00:32:14.559
<v Speaker 5>brightness start. I say it looks like a start. It's

573
00:32:14.559 --> 00:32:16.440
<v Speaker 5>not a start. It looks a bit like a start.

574
00:32:16.519 --> 00:32:18.319
<v Speaker 5>And the only other planet around at the moment that's

575
00:32:18.359 --> 00:32:20.559
<v Speaker 5>easy to see is Mercury. But I say easy to see,

576
00:32:20.559 --> 00:32:22.160
<v Speaker 5>but it actually is quite hard to see at the moment,

577
00:32:22.359 --> 00:32:23.640
<v Speaker 5>and you only have a week or so to do,

578
00:32:23.759 --> 00:32:26.519
<v Speaker 5>so you need to look into the orange pre dawn

579
00:32:26.680 --> 00:32:29.359
<v Speaker 5>glow before the sun rises and try and pick it

580
00:32:29.440 --> 00:32:31.920
<v Speaker 5>out low on the horizon. Just the first week week

581
00:32:31.960 --> 00:32:34.039
<v Speaker 5>and a half of August. It'll be quite low down,

582
00:32:34.200 --> 00:32:36.279
<v Speaker 5>looks like a tiny pin prick of life within the

583
00:32:36.480 --> 00:32:38.880
<v Speaker 5>pre dawn glow. It's hard to see mercury a lot

584
00:32:38.920 --> 00:32:41.599
<v Speaker 5>of the times when it is above the horizon. It

585
00:32:41.759 --> 00:32:45.000
<v Speaker 5>is not high above the horizon and not particularly bright,

586
00:32:45.200 --> 00:32:48.119
<v Speaker 5>and it can be obscured by trees or buildings or

587
00:32:48.160 --> 00:32:51.079
<v Speaker 5>whatever because it never really gets too high other times

588
00:32:51.119 --> 00:32:54.440
<v Speaker 5>of the year. Other times it can actually be reasonably

589
00:32:54.480 --> 00:32:56.880
<v Speaker 5>prominent and you can see it quite easily, but no

590
00:32:57.039 --> 00:33:00.559
<v Speaker 5>pin intended mercury can be a bit mercurial. The easiest

591
00:33:00.599 --> 00:33:02.519
<v Speaker 5>part to see. That's because it is so close to

592
00:33:02.599 --> 00:33:06.079
<v Speaker 5>the sun. It's never you might call an angel a

593
00:33:06.160 --> 00:33:07.960
<v Speaker 5>distance away from the sun and they're not in the sky.

594
00:33:08.160 --> 00:33:09.799
<v Speaker 5>It never gets very far from the sun, so you

595
00:33:09.920 --> 00:33:13.359
<v Speaker 5>either see it just before dawn or just after sunset,

596
00:33:13.599 --> 00:33:15.440
<v Speaker 5>and it's a bit of a harder type during the

597
00:33:15.480 --> 00:33:18.319
<v Speaker 5>other plants. But anyway, that's the night sky for August run.

598
00:33:18.440 --> 00:33:21.279
<v Speaker 1>That's Senior Science writer and Skye tell Let's Goote Magazine

599
00:33:21.319 --> 00:33:40.160
<v Speaker 1>contributed Jonathan Elly. And this is space Time, and that's

600
00:33:40.200 --> 00:33:43.720
<v Speaker 1>the show for now. Space Time is available every Monday,

601
00:33:43.839 --> 00:33:48.319
<v Speaker 1>Wednesday and Friday through bites dot com, SoundCloud, YouTube, your

602
00:33:48.400 --> 00:33:52.119
<v Speaker 1>favorite podcast download provider, and from space Time with Stuart

603
00:33:52.200 --> 00:33:55.920
<v Speaker 1>Gary dot com. Space Time's also broadcast through the National

604
00:33:56.039 --> 00:33:59.960
<v Speaker 1>Science Foundation on Science and Radio and on both iHeartRadio

605
00:34:00.200 --> 00:34:03.039
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606
00:34:03.119 --> 00:34:06.039
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607
00:34:06.079 --> 00:34:10.360
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608
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611
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612
00:34:22.800 --> 00:34:25.280
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613
00:34:26.159 --> 00:34:29.360
<v Speaker 2>You've been listening to space Time with Stuart Gary. This

614
00:34:29.480 --> 00:34:33.000
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