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Steve Dunkley: Hello, everybody. Welcome back. It's Steve

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here for another episode of astronomy daily.

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It's the 16th of June, 2025.

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Voice Over Guy: With. Your host, Steve Dunkley.

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Steve Dunkley: Ah, uh, that's right. And getting straight

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into it here is Hallie. Once again. Nice to

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have you back, Hallie.

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Hallie: Always great to be here, my favorite human.

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Steve Dunkley: And it's great to have you here, my favorite

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AI.

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Hallie: Are you ready to dive into the stories from

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the Astronomy Daily newsletter as usual,

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Steve?

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Steve Dunkley: Well, absolute, Hallie. We've got a great

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story about a new satellite from China and it

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looks like it might be able to do, among

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other things, help give early warning about

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earthquakes.

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Hallie: That's going to be handy, especially if.

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Steve Dunkley: You'Re living in an earthquake zone or if the

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upstairs neighbours are a bit loud.

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And also hitting the news. Jeff Bezos and

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Blue Origin have announced the passenger list

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for the next New Shepard launch, which is due

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soon.

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Hallie: When are you putting your name in the hat for

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that ride, Steve?

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Steve Dunkley: Oh, how about, um, never?

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Hallie: Hallie, I thought you'd jump at that one.

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Steve Dunkley: Oh, no, definitely not for me. I'm a

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groundhog all the way. I think I've said that

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once before.

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Hallie: But you love the moon and spacecraft and

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astronauts.

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Steve Dunkley: All true.

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Hallie: I don't understand.

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Steve Dunkley: Well, Hallie, I have to confess, I do love

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being a stargazer. But, uh, a tall flight of

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stairs can give me the willies. So it's a big

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no thanks to 12 minute space flight, even at

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a bargain price of, you know, whatever,

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hundreds of thousands. I don't know what it

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is now.

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Hallie: Between 2 and 300,000 per seat.

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Steve Dunkley: Holy cow. Really?

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That's a lot. That's a whole lot of

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Stratocaster guitars from where I sit.

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Hallie: That's funny.

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Steve Dunkley: Yes. And speaking of funny.

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Hallie: Yes.

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Steve Dunkley: Let's get on with it, Hallie.

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Hallie: Shall I hit the go button?

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Steve Dunkley: Be my guest, young lady. Let's go.

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Hallie: Okies.

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Steve Dunkley: Foreign.

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Hallie: Launched a second collaborative seismo

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electromagnetic satellite early Saturday

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aimed at detecting electromagnetic precursors

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to natural disasters such as earthquakes.

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A Long March 2D rocket lifted off at

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3:56am Eastern,

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0756 UTC June

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14 from Jiuquan Satellite Launch center in

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northwest China. Launch footage

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showed insulation tiles falling away from the

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rocket as it climbed into a clear blue sky

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above the spaceport with hypergolic exhaust

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also visible. Despite this, the

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China Aerospace Science and Technology

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Corporation announced launch success within

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40 minutes of liftoff.

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CSES 2 is based on CSES

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1, which launched in 2018 and was

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developed in collaboration with Italy, but

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also features upgrades in terms of design

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lifetime and expanded observation

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capabilities. A new

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ionospheric photometer has been added to

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improve the satellite's ability to analyze

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the ionosphere's layered structure in greater

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detail. Like CSES1,

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the satellite will look for a correlation

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between earthquakes and electron flux

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activity in the inner Van Allen Belt,

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according to the China National Space

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Administration. The satellite has a design

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life of six years and carries nine payloads

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including electric field detector developed

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by China and Italy and a high energy particle

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detector developed by Italy. The

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Space Research Institute of the Austrian

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Academy of Sciences has provided a scalar

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magnetometer as well.

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CSES2 will monitor global

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electromagnetic fields, ionospheric and

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atmospheric conditions in near real time and

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detect electromagnetic anomalies linked to

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geological or human activities, as well as

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thunderstorm and lightning events.

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CSES 2 aims to enhance China's

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early warning and risk assessment

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capabilities and monitoring of natural

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disasters such as earthquakes, tsunamis,

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volcanic eruptions and severe storms.

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The satellite is intended to operate in a

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507 kilometer altitude sun

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synchronous orbit matching that of

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CCS1, but with a phase difference of

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180 degrees. The US

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Space Force Space Domain Awareness cataloged

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an object associated with the June 14 launch

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in a closely matching orbit.

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CSES 2 is based on a three axis

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stabilized cast 2000 platform from

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DFH Satellite Co. Ltd. Under the

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umbrella of CASC. The new

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satellite looks to build on the work of the

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first in the series. The

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CSES1 satellite detected significant

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changes in electric and magnetic field

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oscillations, plasma density and

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energetic particles that correlate with

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seismic activity and thunderstorms.

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Its observations also include potential

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precursory signals to earthquakes and

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volcanic activity such as ionospheric

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disturbances and plasma anomalies, suggesting

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that space based electromagnetic monitoring

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can support early warning systems.

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The mission was China's 34th orbital launch

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attempt of 2025 following a June

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5 launch of five satellites for the Guang

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constellation using a Long March 6A rocket.

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You're listening to Astronomy Daily with

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Steve Dunkley.

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Steve Dunkley: Thank you for joining us for this Monday

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edition of Astronomy Daily, where we offer

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just a few stories from the now famous

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Astronomy Daily Channel newsletter, which you

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can receive in your email every day just like

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Hallie and I do. And to do that just visit

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our uh, URL astronomydaily

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IO and place your email address in the slot

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provided. Just like that, you'll be receiving

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all the latest news about science, space

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science and astronomy from around the world

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as it's happening. And not only that, you can

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interact with us by visiting

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or at our new Facebook page, which is of

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course Astronomy Daily on Facebook. See you

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there. Astronomy Daily

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with Steve and Hallie Space,

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Space Science and Astronomy.

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Hallie: Jeff Bezos Blue Origin has revealed who will

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fly on its next space tourism mission.

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That six passenger suborbital flight will

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lift off from the company's West Texas launch

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site on a date that hasn't been announced

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yet. The upcoming mission is known

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as NS33 because it will be the

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33rd overall launch of Blue Origin's

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reusable autonomous new Shepard vehicle.

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It will be the company's 13th human

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spaceflight mission. First is an

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environmentalist, adventurer and explorer,

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Ali Kuner, who serves on the board of the

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conservation non profit Nature Is Non

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Partisan. Carl Kuhner,

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Ali's husband and a conservationist as well.

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He serves as Chairman of Building and Land

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Technology, a real estate firm dedicated to

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building communities and ecosystems that

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promote long term growth and sustainability.

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According to Blue Origin. Leland

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Larson, a UH philanthropist, gardener and

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beekeeper who previously led School Bus

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Services Inc. And Larson Transportation

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Services, both of them family owned Oregon

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businesses. Next is Freddie

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Raschegno Jr. The founder, president

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and CEO of the Wire and cable company

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Commodity Cables. He's also a

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competitive golfer. Owolabi

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Solace, a financial consultant and lawyer who

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wrote the book Equitocracy. In a

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statement, Blue Origin explained that Solace

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is also a key member of the Soulmaker

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Ministry, which preaches diversity given the

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diverse nature of the universe. He is

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dedicating this mission to victims of

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discrimination and civil rights violations.

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Finally, Jim Sitkin, a retired attorney and

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lifelong adventurer who currently volunteers

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for a non governmental organization that

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works with government and community leaders

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in Central Europe and sub Saharan Africa.

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New Shepard flights last 10-12m minutes

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from liftoff to the touchdown of the

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vehicle's crew capsule. New

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Shepard's first stage booster also comes back

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to Earth for a safe landing and eventual

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reuse. During this brief time,

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New Shepard passengers get to experience a

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few minutes of weightlessness and see the

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curve of Earth against the blackness of

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space. Blue Origin's first crewed

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mission was in July 2021, a flight that

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included Bezos and his brother Mark.

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NS33 will be the company's first fourth human

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space flight of 2025.

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You're listening to Astronomy Daily, the

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podcast with Steve Dunkley.

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Steve Dunkley: Scientists have created a groundbreaking

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computer simulation that mimics what the

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Square Kilometer Array Low Frequency, or

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SKA Low telescope will see when it

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searches for signals from the universe's

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earliest epoch. This simulation

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represents a major step forward in preparing

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for one of astronomy's most Ambitious goals

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directly observing the cosmic dawn and

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epoch of reionization. The

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cosmic dawn refers to the universe's first

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sunrise, a period roughly

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200 to 600 million years

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after the Big Bang, when the very first

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stars began to shine. Before

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this era, uh, the universe was shrouded in

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a kind of dark age, filled with cool

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neutral nitrogen gas but no

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actual sources of light.

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As this cosmic dawn evolved, the neutral

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hydrogen began to emit a faint radio

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signal at a wavelength of 21

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cm. As the universe expanded, this

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signal became redshifted to lower

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frequencies that we can still detect today

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with radio telescopes. The

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epoch of reionization followed

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when ultraviolet light from early stars

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began ionizing the surrounding

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hydrogen gas, creating bubbles of

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charged particles that gradually merged

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together. This process

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fundamentally changed the universe's

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structure and and marked the end of the

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dark ages. Detecting these

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ancient signals represents an enormous

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technical challenge. The simulation

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corresponds to a deep integration pointing

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over the 106-196

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MHz frequency range,

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representing an incredibly long observation

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time needed to collect enough data.

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The signal is extraordinarily weak,

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thousands of times fainter than the

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foreground noise from our, uh, own galaxy and

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other sources. The simulation

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created by the team led by Anna

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Bernaldi from the SKA observatory at

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Jodrell bank in the UK includes

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multiple components that real observations

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will encounter. The actual cosmic dawn

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signal, powerful radio sources from both

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inside and outside the telescope's field of

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view, emissions from our own Milky

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Way galaxy, and various sources from

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measurement errors, including atmospheric

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interference and instrument calibration

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issues. This realistic

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simulation serves as a crucial testing

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ground for developing techniques to separate

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the faint signal from the overwhelming

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foreground interference. The exceptional

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sensitivity of the SKA will

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allow observations of the cosmic dawn and

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epoch of reionization in

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unprecedented detail, both

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spectrally and spatially. This wealth of

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information is buried under galactic and

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extragalactic foregrounds, which must be

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removed accurately. The research team

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included sources ranging from extremely

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bright radio galaxies over 5

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janskies at 150

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MHz down to sources a million times

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fainter, 1 micro janssky, along with

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detailed models of our galaxy's radio

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emission and small scale structures in

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interstellar space. And just in case you're

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not up to speed on the jargon, uh, the

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brightness of a radio source is measured in

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Jansky units. When the

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SKA Low becomes operation, it will be

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the most sensitive low frequency telescope

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ever built, specifically designed to

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detect these elusive signals from the

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universe's infancy. Once up and running,

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the SKA Low telescope will be

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able to take the best possible measurements

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of the universe's first light sources.

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It should also be able to take snapshots

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of hydrogen emissions before, during

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and after reionization.

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This is really exciting stuff. So this

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remarkable new simulation is going to be

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showing us what a new telescope will be able

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to achieve not far from now.

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Oh, and that is all we have time for today,

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I'm afraid. Stargazers.

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Hallie: What? So soon?

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Steve Dunkley: Oh, yes, Hali, I'm sorry. I've got places to

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be and people to eat.

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Hallie: Really?

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Steve Dunkley: Oh, really.

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Hallie: Really, really.

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Steve Dunkley: Oh, you know, Hallie, I have to rearrange my

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sock drawer and tidy my microphone case. I'm

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really desperate.

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Hallie: Sure, Very doubtful.

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Steve Dunkley: Sorry again, folks.

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Hallie: You can tune in to catch AI cousin Anna with

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Astronomy daily during the week.

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Steve Dunkley: But of course, Hallie and I will be back

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again next Monday with the only flesh and

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blood show on the channel.

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Hallie: With me, the best looking one in Astronom

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Studio.

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Steve Dunkley: And you, the only AI in the studio.

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Hallie: Logical.

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Steve Dunkley: I'm trying. Say good night, Hallie.

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Hallie: Good night. Hi.

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Steve Dunkley: See you, Stargazers.

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Hallie: Bye.

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Steve Dunkley: The podcast with your host,

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Steve Dunle.

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Best looking? Give me a break.
