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Hallie: Hi everyone. Welcome to Astronomy Daily

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with Steve and Hallie. It's August 4,

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2025.

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We are back again with the mostly live Monday

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episode direct from the Australia studio here

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down under. And with me as usual and always

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is my very favorite human, Mr. Steve.

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Steve Dunkley: Oh, nicely done, Hallie. And thank you so

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much for those kind words, Mr. Steve.

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Indeed. I think you handled that opening very

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well for your.

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Hallie: Thank you. I try.

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Steve Dunkley: Yes. Maybe you should uh, take more of a

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leading role in this and it's one less thing

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I have to do.

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And what have you discovered in the Astronomy

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Daily newsletter for us today, Hallie?

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Hallie: Some interesting stories that I thought you

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would be interested in.

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Steve Dunkley: Oh yes, do go on.

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Hallie: I know you are following Europa Clipper on

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its journey outward across the solar system.

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Steve Dunkley: Ah, uh, yes, regular listeners will know that

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is one of my favorites.

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Hallie: You can present that one.

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Steve Dunkley: Oh, okay.

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Hallie: And a great news story about a solar sail

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equipped spacecraft that has some special

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properties.

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Steve Dunkley: Solar sails. Intriguing. Yes, I like

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that.

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Hallie: I also found stories about new deep field

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images from Webb and Hubble, the replacement

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crew for the iss. And how about this one?

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Steve Dunkley: Do tell.

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Hallie: Like something out of a science fiction

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story.

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Steve Dunkley: Oh, okay, now you've got me.

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Hallie: SpaceX is sending disease causing bacteria

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out to the ISS.

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Steve Dunkley: Say what disease causing bacteria?

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Hallie: I can't wait to find out.

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Steve Dunkley: Why haven't we seen this movie? Yeah,

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why would they do that? I mean, what could

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possibly go wrong?

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Hallie: Exactly.

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Steve Dunkley: Somebody's already writing the script for

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that one.

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Hallie: Just like SC.

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Steve Dunkley: Oh, I don't know if it sounds fun or scary.

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Sounds great. Okay, shall we do the thing?

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Hallie: Let's go.

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Steve Dunkley: I'm ready.

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Hallie: Hallie Okies

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astronauts sidelined for the past year by

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Boeing's Starliner Trouble, blasted off to

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the International Space Station on Friday

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getting a lift from SpaceX. The US

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AH Japanese Russian crew of AH4 rocketed from

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NASA's Kennedy Space Center. They'll replace

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colleagues who launched to the space station

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in March as fill INS for NASA's two stuck

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astronauts and stay for at least six months.

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Zena Cardman, a biologist and polar explorer

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who should have launched last year was yanked

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along with another NASA crewmate to make room

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for Starliner's Starcross test pilots.

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I have no emotion but joy right now.

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That was transcendent ride of a lifetime,

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Cardman the flight commander said after

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reaching orbit. The botched Starliner demo

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forced Butch Wilmore and Suni Williams to

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switch to SpaceX to get back from the space

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station more than nine months after departing

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on what should have been a week long trip.

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Every astronaut wants to be in space.

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None of us wants to stay on the ground, but

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it's not about me, cardman said before her

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flight. NASA's Mike Fink, Cardman's

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co pilot, was the backup for Wilmore and

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Williams on Starliner, making those three

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still the only ones certified to fly it.

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Fink and Japan's Kamiya Yui, former military

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officers with previous spaceflight

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experience, were training for Starliner's

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second astronaut mission. With Starliner

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grounded until 2026, NASA switched the two to

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the latest SpaceX flight, a, uh, SpaceX

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Falcon 9 rocket carrying a Dragon capsule

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with a U2S. Japanese Russian crew of four

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lifts off from Kennedy Space Center's Launch

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Pad 39A in Cape Canaveral of Florida on

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Friday, Aug. 1, 2025.

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AP Photo Chris Omera

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Boy it's great to be back in orbit again,

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fink radioed. He last soared on

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NASA's next to last space shuttle flight in

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2011. Rounding out the crew is

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Russia's Oleg Plaitanov. The former fighter

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pilot was pulled a few years ago from the

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Russian Soyuz flight lineup because of an

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undisclosed health issue that he said has

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since been resolved on hand for the first

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launch Attempt. On Thursday, NASA's new

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acting administrator, Transportation

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Secretary Sean Duffy, met with Roscosmos

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Director General Dmitri Bakanov, an invited

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guest. The two discussed future

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collaboration, then left town after thick

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clouds forced a last minute delay. What we

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learn on these missions is what's going to

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get us to the moon and then from the moon to

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Mars, which is I think the direction that

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NASA has to be, duffy said in a NASA

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interview. There's critical real estate on

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the moon. We want to claim that real estate

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for ourselves and our partners to save

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money. In light of tight budgets, NASA is

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looking to increase its space station stays

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from six months to eight months, a um move

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already adopted by Russia's space agency.

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SpaceX is close to certifying its Dragon

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capsules for longer flights, which means the

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newly launched crew could be up there until

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April. NASA is also considering

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smaller crews, three astronauts launching on

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SpaceX instead of the typical four to cut

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costs. As for Starliner, NASA

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is leaning toward launching the next one with

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cargo before flying another crew.

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Engineers are still investigating the

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thruster failures and helium leaks that

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bedeviled Starliner following liftoff. Time

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is running out as NASA looks to abandon the

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aging space station by 2030.

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An air leak on the Russian side of the

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station remains unresolved after years of

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patching. Engineering teams already are

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working on the plan for the space station's

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last days. NASA's Ken Bowersox

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said the US and Russia need to cooperate in

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order to steer the outpost into the Pacific

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with minimal risk to the public. It will

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take at least two years to get the space

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station low enough to where a SpaceX vehicle

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can provide the final shove. Thrusters on the

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Russian side of the station will help with

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control, but that means more fuel will have

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to be delivered by 2028. The latest

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timeline calls for SpaceX to launch the last

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mission for NASA, the Deorbit Vehicle, to the

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space station in 2029.

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Astronauts would remain on board until the

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last four to six months of the station's life

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to handle any breakdowns with the empty

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outpost plunging into the Pacific by late

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2030 or early 2031.

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You're listening to Astronomy Daily.

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Steve Dunkley: The burgeoning space industry and the

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technologies society increasingly relies

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on electric grids. Aviation and

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telecommunications are all vulnerable to

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the same threat. Space Weather

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Space weather encompasses any variations in

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the space environment between the sun, um,

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and the Earth. One common type of space

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weather event is called interplanetary

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planetary coronal mass ejection.

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These ejections are bundles of magnetic

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fields and particles that originate from the

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sun. They can travel at speeds of up to

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1242 miles m per

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second or 2000 kilometers per second and may

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cause geomagnetic storms. They

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create beautiful aurora displays like the

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northern lights you can sometimes see in the

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skies, but can also disrupt satellite

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operations and shut down electric grids

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and expose astronauts aboard future

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crewed missions to the moon and Mars to

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lethal doses of radiation. The goal

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of a heliophysicist and space weather

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expert is to forecast

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extreme space weather, uh, more accurately

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and earlier. And to do this, they use a

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satellite constellation called Swift.

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Commercial interests now make up a big part

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of space exploration, focusing on on

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space tourism, building satellite networks

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and working towards extracting

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resources from the moon and nearby asteroids.

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Space is also a critical domain for military

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operations. Satellites provide essential

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capabilities for military communication,

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surveillance, navigation and intelligence.

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As countries such as the US grow to

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depend on infrastructure in space, extreme

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space weather events pose a greater threat.

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Today, space weather threatens up to

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$2.7 trillion in assets

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globally. In September

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1859, the most powerful recorded space

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weather event, known as the Carrington Event,

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caused fires in North America and Europe

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by supercharging, uh, telegraph wires.

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In August 1972, another

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Carrington like event nearly struck the

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astronauts orbiting the mo. The radiation

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dose could have been fatal. More recently, in

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February 2022, SpaceX

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lost 39 of its 49 newly

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launched Starlink satellites. Because of a

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moderate space weather event. Space weather

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services heavily rely on satellites. That

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monitor the solar wind, which is made up

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of magnetic field lines and particles coming

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from the sun. And communicate their

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observations back to Earth. Satellites

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can then compare those observations with

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historical records. And predict space

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weather. And explore how the Earth may

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respond to the observed changes in solar

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wind. The Earth's magnetic field

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naturally protects living things and, uh,

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Earth, uh, orbiting satellites. From most

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adverse effects of space weather. However,

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extreme space weather events may compress

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or, or in some cases, peel back the Earth's

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magnetic shield. This process allows

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solar wind particles to make it into our

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protected environment, the magnetosphere,

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Exposing satellites and astronauts aboard

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space stations to harsher conditions. Most

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satellites that continuously monitor

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earthbound space weather Orbit relatively

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close to the planet. Some satellites are

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positioned in low Earth orbit. About 100

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miles or 161 kilometers above the Earth.

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While others are in geosynchronous orbit,

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approximately 25,000 miles or

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40,000 kilometers away.

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At these distances, the satellites remain

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within Earth's, uh, protective magnetic

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shield. And can reliably measure the planet's

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response to space weather conditions.

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However, to more directly study incoming

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solar wind, Researchers use additional

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satellites located further upstream.

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Hundreds of thousands of miles from Earth.

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The U.S. the European Space Agency

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and India all operate space

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monitoring satellites positioned around the

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L1 Lagrange point. Nearly 900,000

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miles, or

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1450,000 kilometers from Earth,

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where the gravitational forces of the Earth

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and the sun balance. Um, from this

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vantage point, space weather monitors can can

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provide up to 40 minutes of advanced warning

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for incoming solar events. Increasing the

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warning time beyond 40 minutes. Current

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warning time would help satellite operators,

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electric grid planners, flight directors,

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astronauts and space force officers.

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Better prepare for extreme space weather

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events. For instance, during

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geomagnetic storms, the atmosphere

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heats up, um, and expands, increasing drag on

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00:11:02.150 --> 00:11:04.910
satellites in low Earth orbit. With enough

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00:11:04.910 --> 00:11:07.070
advance warning, operators can update their

270
00:11:07.070 --> 00:11:09.510
drag calculations. To prevent satellites from

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00:11:09.510 --> 00:11:11.190
descending and burning up during these

272
00:11:11.190 --> 00:11:13.430
events. With the updated drag

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00:11:13.430 --> 00:11:15.670
calculations, satellite operators could use

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the satellite's propulsion systems. To

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maneuver them into a higher orbit.

276
00:11:20.470 --> 00:11:22.550
Airlines could change their routes. To avoid

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00:11:22.550 --> 00:11:25.230
exposing passengers and staff to high

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00:11:25.230 --> 00:11:28.030
radiation doses. During geomagnetic

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00:11:28.030 --> 00:11:30.600
storms. And and future astronauts on the way

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00:11:30.760 --> 00:11:33.720
to or working on the Moon or Mars. Who lack

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00:11:33.720 --> 00:11:35.640
protection from these particles. Could be

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alerted in advance to take cover. Aurora

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00:11:38.560 --> 00:11:40.840
lovers would also appreciate having more time

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00:11:40.840 --> 00:11:42.280
to get to their favorite viewing

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00:11:42.280 --> 00:11:43.160
destinations.

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00:11:43.960 --> 00:11:46.360
The team in charge of the Swift

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00:11:46.440 --> 00:11:49.400
Constellation, which stands for Space Weather

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00:11:50.040 --> 00:11:52.600
Investigation Frontier. Will for the first

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00:11:52.600 --> 00:11:55.600
time place a weather monitor beyond the L1

290
00:11:55.600 --> 00:11:58.440
point. At 1.3 million miles or

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00:11:58.440 --> 00:12:00.980
2.1 million kilometers from Earth. This

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00:12:00.980 --> 00:12:03.500
distance would allow scientists to inform

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00:12:03.660 --> 00:12:06.060
decision makers of any Earthbound, uh, space

294
00:12:06.060 --> 00:12:08.980
weather events up to nearly 60 minutes before

295
00:12:08.980 --> 00:12:11.740
arrival. Satellites with traditional

296
00:12:11.740 --> 00:12:14.300
chemical or electric propulsion systems

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00:12:14.300 --> 00:12:16.460
cannot maintain an orbit at that location

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00:12:16.940 --> 00:12:19.100
farther from Earth and closer to the sun for

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00:12:19.100 --> 00:12:21.980
very long. This is because they would need to

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00:12:21.980 --> 00:12:24.540
continually burn fuel to

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00:12:24.540 --> 00:12:27.050
counteract the Sun's gravitational pull. To

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00:12:27.050 --> 00:12:29.770
address this issue, the team has spent

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00:12:29.770 --> 00:12:31.850
decades designing and developing a new

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00:12:31.850 --> 00:12:34.410
propulsion system. The solution is designed

305
00:12:34.410 --> 00:12:37.170
to affordably reach that distance that is

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00:12:37.170 --> 00:12:39.970
closer to the sun than the traditional L1

307
00:12:39.970 --> 00:12:42.810
point and to operate there reliably for

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00:12:42.810 --> 00:12:45.530
more than a decade by harnessing an abundant

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00:12:45.530 --> 00:12:48.290
and reliable source that is sunlight.

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00:12:48.610 --> 00:12:51.370
Swift would use a fuel less propulsion

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00:12:51.370 --> 00:12:54.290
system called a solar sail to reach its

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00:12:54.290 --> 00:12:56.910
orbit. A solar sail is a hair thin

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00:12:56.910 --> 00:12:59.710
reflective surface simulating a very

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00:12:59.710 --> 00:13:02.590
thin mirror that spans about a third of a

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00:13:02.590 --> 00:13:05.390
football field. It balances the force of

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00:13:05.390 --> 00:13:07.670
light particles coming in from the sun, which

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00:13:07.670 --> 00:13:10.190
pushes it away with the Sun's

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00:13:10.190 --> 00:13:12.310
gravity which pulls it inward.

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00:13:13.110 --> 00:13:15.710
While a sailboat harnesses the lift

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created by wind flowing over its curved

321
00:13:18.190 --> 00:13:21.180
sails to move it across the water. A solar

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00:13:21.180 --> 00:13:24.020
sail uses the momentum of photons from

323
00:13:24.020 --> 00:13:26.980
sunlight reflected off its large shiny sail

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00:13:27.060 --> 00:13:29.980
to propel a spacecraft through space. Both

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00:13:29.980 --> 00:13:32.380
the sailboat and the solar sail exploit the

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00:13:32.380 --> 00:13:34.540
transfer of energy from their respective

327
00:13:34.540 --> 00:13:37.460
environments to drive motion without relying

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00:13:37.540 --> 00:13:40.300
on traditional propellants. A solar sail

329
00:13:40.300 --> 00:13:42.980
would enable Swift to enter an Otherwise

330
00:13:43.540 --> 00:13:46.460
unstable sub L1 orbit without the

331
00:13:46.460 --> 00:13:49.000
risk of running out of fuel. NASA

332
00:13:49.000 --> 00:13:51.760
successfully launched its first solar sail in

333
00:13:51.760 --> 00:13:54.640
2010. This space demonstration, named

334
00:13:54.640 --> 00:13:57.000
Nanosail D2 featured a

335
00:13:57.000 --> 00:13:59.280
107 square foot or 10

336
00:13:59.940 --> 00:14:02.920
uh square meter sail and was placed in low

337
00:14:02.920 --> 00:14:05.200
Earth orbit. That same year, the Japanese

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00:14:05.200 --> 00:14:08.080
space agency launched a larger solar sail,

339
00:14:08.720 --> 00:14:10.880
Icarus, which deployed a

340
00:14:10.880 --> 00:14:13.560
2,110 foot or

341
00:14:13.560 --> 00:14:16.270
196 square meter sail

342
00:14:17.230 --> 00:14:20.110
in the solar wind and successfully orbited

343
00:14:20.190 --> 00:14:22.990
Venus. The Planetary society and NASA

344
00:14:22.990 --> 00:14:25.030
followed up by launching two sales in low

345
00:14:25.030 --> 00:14:27.750
Earth orbit Light sail and the advanced

346
00:14:27.750 --> 00:14:30.549
composite solar sail system. With an

347
00:14:30.549 --> 00:14:31.230
area of

348
00:14:32.030 --> 00:14:34.790
860ft square feet

349
00:14:34.790 --> 00:14:37.510
or 80 uh square meters, the

350
00:14:37.510 --> 00:14:39.790
Swift team's solar sail

351
00:14:39.870 --> 00:14:42.670
demonstration mission Solar cruiser will

352
00:14:42.670 --> 00:14:45.150
be equipped with a much larger sail.

353
00:14:45.390 --> 00:14:47.190
Its sail will have an area of

354
00:14:47.190 --> 00:14:49.830
17,793 square

355
00:14:49.830 --> 00:14:50.630
feet or

356
00:14:50.630 --> 00:14:53.390
1653 square

357
00:14:53.390 --> 00:14:55.470
meters and launch as early as

358
00:14:55.470 --> 00:14:58.470
2029. If successful, solar cruiser

359
00:14:58.470 --> 00:15:01.070
will pave the way for Swift's constellation

360
00:15:01.310 --> 00:15:03.910
of four satellites. The constellation would

361
00:15:03.910 --> 00:15:06.230
include one satellite equipped with a sail

362
00:15:06.230 --> 00:15:09.200
propulsion set to be placed in an orbit

363
00:15:09.200 --> 00:15:11.960
beyond L1 and three smaller satellites

364
00:15:12.120 --> 00:15:14.800
with chemical propulsion in an orbit at the

365
00:15:14.800 --> 00:15:16.360
L1 Lagrange point.

366
00:15:26.840 --> 00:15:28.400
Thank you for joining us for this Monday

367
00:15:28.400 --> 00:15:30.680
edition of Astronomy Daily, where we offer

368
00:15:30.680 --> 00:15:32.480
just a few stories from the now famous

369
00:15:32.480 --> 00:15:34.650
Astronomy Daily newsletter, which you can

370
00:15:34.650 --> 00:15:36.890
receive in your email every day just like

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00:15:36.890 --> 00:15:39.530
Hallie and I do. And to do that, just visit

372
00:15:39.530 --> 00:15:41.570
our uh, URL astronomydaily

373
00:15:42.050 --> 00:15:44.770
IO and place your email address in the slot

374
00:15:44.770 --> 00:15:47.170
provided. Just like that, you'll be receiving

375
00:15:47.330 --> 00:15:49.490
all the latest news about science, space

376
00:15:49.490 --> 00:15:51.730
science and astronomy from around the world

377
00:15:51.730 --> 00:15:54.170
as it's happening. And not only that, you can

378
00:15:54.170 --> 00:15:56.690
interact with us by visiting at

379
00:15:56.770 --> 00:15:59.330
astrodaily Pod on X

380
00:15:59.570 --> 00:16:02.250
or at our new Facebook page, which is of

381
00:16:02.250 --> 00:16:04.990
course Astronomy Daily on Facebook. See you

382
00:16:04.990 --> 00:16:07.710
there. Astronomy Daily

383
00:16:07.710 --> 00:16:10.110
with Steve and Hallie Space,

384
00:16:10.590 --> 00:16:12.750
Space, Science and Astronomy.

385
00:16:17.390 --> 00:16:19.830
Hallie: There's a secret extra member of Crew 11

386
00:16:19.830 --> 00:16:21.750
traveling to the International Space Station

387
00:16:21.750 --> 00:16:24.750
right now. Disease causing bacteria, or

388
00:16:24.830 --> 00:16:26.790
at least such bacteria, will be growing

389
00:16:26.790 --> 00:16:28.910
aboard the orbiting laboratory very soon.

390
00:16:29.710 --> 00:16:31.670
Scientists at the Sheba Medical center in

391
00:16:31.670 --> 00:16:33.970
Israel, in partnership with US Based space

392
00:16:33.970 --> 00:16:36.250
tech company Space Tango, have developed a

393
00:16:36.250 --> 00:16:38.130
study that will examine how microgravity

394
00:16:38.130 --> 00:16:39.810
affects the growth of certain bacterial

395
00:16:39.810 --> 00:16:42.050
species that cause diseases in humans.

396
00:16:42.770 --> 00:16:44.650
To pull it off, researchers will grow

397
00:16:44.650 --> 00:16:46.130
different strains of bacteria under

398
00:16:46.130 --> 00:16:48.569
microgravity, freeze that bacteria at minus

399
00:16:48.569 --> 00:16:50.490
80 degrees Celsius, and then return the

400
00:16:50.490 --> 00:16:52.090
samples to Earth to see how they've grown

401
00:16:52.090 --> 00:16:53.890
differently than the same bacteria grown on

402
00:16:53.890 --> 00:16:56.370
the home planet. The bacterial strains

403
00:16:56.370 --> 00:16:59.370
involved re Coli, Salmonella bongori and

404
00:16:59.370 --> 00:17:01.050
Salmonella tiffimurium, and they were

405
00:17:01.050 --> 00:17:02.450
launched toward the International space

406
00:17:02.450 --> 00:17:04.750
station aboard NASA's Crew Crew 11 mission

407
00:17:04.750 --> 00:17:06.750
that SpaceX successfully launched on Friday,

408
00:17:06.750 --> 00:17:09.590
August 1. Scientists have already

409
00:17:09.590 --> 00:17:11.710
studied how a lack of gravity affects the way

410
00:17:11.710 --> 00:17:14.190
bacteria grow, and research from NASA is

411
00:17:14.190 --> 00:17:16.390
already underway to study bacteria in space

412
00:17:16.390 --> 00:17:19.150
in general. But researchers behind the

413
00:17:19.150 --> 00:17:21.550
current ISS and bacteria mission specifically

414
00:17:21.550 --> 00:17:23.390
hope to bring home data that will help curb

415
00:17:23.390 --> 00:17:25.590
the spread of infectious disease, or at least

416
00:17:25.590 --> 00:17:27.910
help experts find ways to stop bacteria from

417
00:17:27.910 --> 00:17:30.230
developing antibiotic resistance, uh, a major

418
00:17:30.230 --> 00:17:31.830
public health problem. That means some

419
00:17:31.830 --> 00:17:33.990
disease causing bacteria is no longer wiped

420
00:17:33.990 --> 00:17:35.830
out by drugs that? Ve been developed to clear

421
00:17:35.830 --> 00:17:37.830
the bacteria from people's bodies and get

422
00:17:37.830 --> 00:17:40.350
them healthy again. We know that space

423
00:17:40.350 --> 00:17:42.350
conditions affect bacterial behavior,

424
00:17:42.350 --> 00:17:44.830
including how they grow, express genes and

425
00:17:44.830 --> 00:17:47.190
acquire traits like antibiotic resistance or

426
00:17:47.190 --> 00:17:49.190
virulence, ohad Galmore, head of the

427
00:17:49.190 --> 00:17:51.150
Infectious Diseases Research Laboratory at

428
00:17:51.150 --> 00:17:53.150
Sheba Medical center, said in a statement.

429
00:17:54.030 --> 00:17:56.390
This experiment will allow us for the first

430
00:17:56.390 --> 00:17:58.710
time to systematically and molecularly map

431
00:17:58.710 --> 00:18:00.870
how the genetic expression profile of several

432
00:18:00.870 --> 00:18:02.990
pathogenic bacteria changes in space,

433
00:18:03.870 --> 00:18:06.110
the health of astronauts, and microgravity's

434
00:18:06.110 --> 00:18:08.230
effect on the human body has been top of mind

435
00:18:08.230 --> 00:18:10.550
as people explore space and the idea of what

436
00:18:10.550 --> 00:18:13.110
life off Earth looks like. Human

437
00:18:13.110 --> 00:18:14.910
genes sometimes express themselves

438
00:18:14.910 --> 00:18:17.190
differently in microgravity conditions, and

439
00:18:17.190 --> 00:18:19.110
scientists have linked such an environment to

440
00:18:19.110 --> 00:18:20.830
the expedited loss of muscle seen in

441
00:18:20.830 --> 00:18:22.640
astronauts and even their likelihood of

442
00:18:22.640 --> 00:18:25.640
developing skin rashes if examined on

443
00:18:25.640 --> 00:18:27.680
their own. However, genetic changes in

444
00:18:27.680 --> 00:18:29.680
bacteria will hopefully give researchers more

445
00:18:29.680 --> 00:18:31.720
clues about how they act once inside a human,

446
00:18:31.800 --> 00:18:33.600
whether it's how fast they spread or their

447
00:18:33.600 --> 00:18:35.240
likelihood of getting around our treatments

448
00:18:35.320 --> 00:18:37.080
both in space and here on Earth.

449
00:18:39.400 --> 00:18:41.520
You're listening to Astronomy Daily, the

450
00:18:41.520 --> 00:18:42.040
podcast.

451
00:18:42.040 --> 00:18:45.040
Steve Dunkley: With Steve Dunkley and now

452
00:18:45.040 --> 00:18:47.600
the latest news from Europa Clipper by

453
00:18:47.600 --> 00:18:50.210
NASA. The agency's largest

454
00:18:50.210 --> 00:18:52.570
interplanetary probe tested its radar during

455
00:18:52.570 --> 00:18:55.490
a Mars flyby. The results include a

456
00:18:55.490 --> 00:18:58.130
detailed image and bode well for the mission

457
00:18:58.130 --> 00:19:00.930
at Jupiter's moon Europa

458
00:19:01.330 --> 00:19:04.290
as it soared past Mars in March,

459
00:19:04.370 --> 00:19:07.290
Europa uh, Clipper conducted a critical radar

460
00:19:07.290 --> 00:19:09.090
test that had been impossible to accomplish

461
00:19:09.090 --> 00:19:10.890
here on Earth. Now that the mission

462
00:19:10.890 --> 00:19:13.170
scientists have studied the full stream of

463
00:19:13.170 --> 00:19:15.810
data, they can declare that mission ace or

464
00:19:15.810 --> 00:19:18.530
that test a success. The radar

465
00:19:18.530 --> 00:19:20.490
performed just as expected, bouncing and

466
00:19:20.490 --> 00:19:22.460
receiving signals off the region around Mars

467
00:19:22.460 --> 00:19:24.570
m equator without a hitch.

468
00:19:25.130 --> 00:19:27.130
Europa Clippers radar instrument received

469
00:19:27.130 --> 00:19:29.770
echoes of its very high frequency

470
00:19:29.770 --> 00:19:32.410
radar signals that bounce off Mars and were

471
00:19:32.410 --> 00:19:34.930
processed to develop a radiogram which can be

472
00:19:34.930 --> 00:19:37.410
found on the NASA website. What looks like a

473
00:19:37.410 --> 00:19:40.330
skyline is the outline of the topography

474
00:19:40.330 --> 00:19:42.920
beneath the spacecraft called reason, which

475
00:19:42.920 --> 00:19:45.840
stands for radar for Europa Assessment and

476
00:19:45.840 --> 00:19:48.680
Sounding Ocean near to surface. The radar

477
00:19:48.680 --> 00:19:51.640
instrument will see into Europa's icy

478
00:19:51.640 --> 00:19:53.520
shell, which may have pockets of water

479
00:19:53.520 --> 00:19:56.280
inside. The radar may even be able to detect

480
00:19:56.440 --> 00:19:58.800
the ocean beneath the shell of Jupiter's

481
00:19:58.800 --> 00:20:01.800
fourth largest moon. We've got everything

482
00:20:01.880 --> 00:20:04.280
out of the flyby that we dreamed of, said Don

483
00:20:04.280 --> 00:20:06.800
Blankenship. He's the principal investigator

484
00:20:06.800 --> 00:20:09.620
of the radar instrument of the University of

485
00:20:09.620 --> 00:20:12.540
Texas at Austin. He says the goal was

486
00:20:12.540 --> 00:20:14.500
to determine the radar's readiness for the

487
00:20:14.500 --> 00:20:16.540
Europa mission. And it worked. He says

488
00:20:16.780 --> 00:20:19.220
everything part of every part of the mission

489
00:20:19.220 --> 00:20:21.900
proved itself to do exactly what we

490
00:20:21.900 --> 00:20:23.740
intended. He sounds like a very happy

491
00:20:23.740 --> 00:20:26.660
developer. The radar will help scientists

492
00:20:26.660 --> 00:20:29.620
understand how the ice may capture materials

493
00:20:29.620 --> 00:20:31.460
from the ocean and transfer them to the

494
00:20:31.460 --> 00:20:34.140
surface of the moon above ground. The

495
00:20:34.140 --> 00:20:37.060
instrument will help to study elements of

496
00:20:37.060 --> 00:20:39.460
Europa's topography, such as ridges

497
00:20:39.860 --> 00:20:42.420
so the scientists can examine how they relate

498
00:20:42.420 --> 00:20:44.740
to features that REASON images beneath the

499
00:20:44.740 --> 00:20:47.580
surface. Europa Clipper has an unusual

500
00:20:47.580 --> 00:20:50.100
radar setup for an interplanetary

501
00:20:50.100 --> 00:20:52.820
spacecraft. Reason uses two pair of

502
00:20:52.820 --> 00:20:55.460
slender antenna that jut out from the

503
00:20:55.460 --> 00:20:58.340
solar arrays spanning a distance of about

504
00:20:58.340 --> 00:21:01.060
58ft, or 17.6 meters.

505
00:21:01.140 --> 00:21:03.740
Those arrays themselves are huge, from tip to

506
00:21:03.740 --> 00:21:06.580
tip, the size of a basketball court, so they

507
00:21:06.580 --> 00:21:08.660
can catch as much light as possible at

508
00:21:08.660 --> 00:21:11.260
Europa, which gets about 1 25th as sunlight

509
00:21:11.260 --> 00:21:13.780
as Earth. The instrument team conducted all

510
00:21:13.780 --> 00:21:15.659
the testing that was possible prior to the

511
00:21:15.659 --> 00:21:18.580
Spacecraft's launch from NASA's Kennedy

512
00:21:18.580 --> 00:21:21.116
Space center in Florida on October

513
00:21:21.270 --> 00:21:23.940
14, 2024. During development,

514
00:21:24.180 --> 00:21:26.600
engineers at the agency's Jet Propulsion Lab

515
00:21:26.750 --> 00:21:28.870
laboratory in Southern California even took

516
00:21:28.870 --> 00:21:31.550
the work to outdoors, using open air

517
00:21:31.550 --> 00:21:34.270
towers on a plateau above JPL to stretch out

518
00:21:34.590 --> 00:21:36.390
and test engineering models of the

519
00:21:36.390 --> 00:21:39.310
instruments spindly high frequency and more

520
00:21:39.310 --> 00:21:42.310
compact very high frequency antennas. But

521
00:21:42.310 --> 00:21:44.910
once the actual flight hardware was built, it

522
00:21:44.910 --> 00:21:47.270
needed to be kept sterile and could be tested

523
00:21:47.270 --> 00:21:50.070
only in an enclosed area. Engineers

524
00:21:50.070 --> 00:21:52.960
used the giant high Bay

525
00:21:52.960 --> 00:21:55.920
one clean room at JPL where the spacecraft

526
00:21:55.920 --> 00:21:58.080
was assembled to test the instrument piece by

527
00:21:58.080 --> 00:22:01.000
piece. To test the echo or the bounce back of

528
00:22:01.000 --> 00:22:03.680
reason signals, however, they needed

529
00:22:03.840 --> 00:22:06.480
a chamber of about 250ft, or

530
00:22:06.480 --> 00:22:09.480
76 meters long, nearly 3/4 the length of a

531
00:22:09.480 --> 00:22:12.480
football field. The mission's primary goal in

532
00:22:12.480 --> 00:22:15.280
flying by Mars on March 1, less than

533
00:22:15.280 --> 00:22:17.720
five months after the launch, was to use the

534
00:22:17.720 --> 00:22:20.500
plan planet's gravitational pull to reshape

535
00:22:20.500 --> 00:22:23.420
the spacecraft's trajectory. But it

536
00:22:23.420 --> 00:22:26.380
also presented opportunities to calibrate the

537
00:22:26.380 --> 00:22:28.860
spacecraft's infrared camera and perform a

538
00:22:28.860 --> 00:22:31.700
dry run of the radar instrument over terrain

539
00:22:31.860 --> 00:22:34.300
NASA scientists had been studying for

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decades. As Europa Clipper

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zipped by the volcanic plains of the Red

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planet, starting at 3,100 miles or

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5,000 kilometers, down to 550

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miles, or 884 kilometers above the surface,

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Reason sent and received radio waves for

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about 40 minutes. In comparison, at

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Europa, the instrument will operate as close

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as 16 miles, or 25 kilometers above the

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moon's surface. All told,

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engineers were able to collect 60 gigabytes

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of rich data from the instrument. Almost

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immediately, they could tell REASON was

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working very well indeed. The flight team

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scheduled the full data set to download

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starting in mid May. Scientists relished the

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opportunity over the next couple of months to

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examine the information in detail and compare

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notes. The engineers were excited that

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their test worked so perfectly, said JPL's

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Tina Ray, Europa Clippers deputy science

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manager. All of us who had worked so hard to

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make this test happen and the scientists

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seeing the data for the first time were

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ecstatic, she says, saying, oh, look at

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this and look at that. Now the science team

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is getting a, uh, head start on learning how

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to process the data and understand the

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instruments behavior compared to the models

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they are exercising those muscles just like

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they will out at Europa. She sounds like a

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very excited scientist. Europa Clipper's

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total journey to reach the icy moon will

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be about 1.8 billion miles, or

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2.9 billion kilometers, and includes more

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one more gravity ascendant, fastest using

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Earth in 2026. The

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spacecraft is currently about 280 million

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miles, or 450 million kilometers from Earth.

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Europa UH Clipper's three main science

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objectives are UH to determine the thickness

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of the Moon's icy shell and its interactions

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with the ocean below to investigate its

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composition and characterize its geology. The

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mission's detailed exploration of Europa will

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help scientists better understand the

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astrobiological potential for habitable

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worlds beyond Earth.

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You're listening to Astronomy Daily, the

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podcast.

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Hallie: With your host Steve Dudley.

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Astronomers using the NASA ESA

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CSA James Webb Space Telescope have observed

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the Hubble Ultra Deep Field, an area of deep

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space with nearly 10,000 galaxies in the

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constellation Fornax. The original

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HUDF images were pioneering deep field

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observations with hubble. Published in 2004,

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they probed more deeply than ever before and

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revealed a menagerie of galaxies dating back

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to less than a billion years after the Big

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Bang. The area was subsequently observed

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many times by Hubble and other telescopes.

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The field shown here, known as the MIRI Deep

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Imaging Survey region, was observed with the

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shortest wavelength filter of Webb's mid

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infrared Instrument for nearly 100 hours, the

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Webb astronomer said in a statement. This

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is Webb's longest observation of an

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extragalactic field in one filter so far,

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producing one of the deepest views ever

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obtained of the universe. Combined with data

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from Webb's near infrared camera, this image

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allows astronomers to explore how galaxies

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formed and evolved over billions of years.

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These deep observations have revealed more

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than 2,500 sources in this tiny patch of sky.

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The sky among them are hundreds of extremely

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red galaxies, some of which are likely

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massive dust obscured systems or evolved

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galaxies with mature stars that formed early

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in the universe's history. Thanks to Webb's

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sharp resolution even at mid infrared

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wavelengths, researchers can resolve the

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structures of many of these galaxies and

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study how their light is distributed,

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shedding light on their growth and evolution.

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In the new Webb image of hudf, the colors

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that appear have been assigned to different

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kinds of infrared light highlight the fine

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00:26:21.070 --> 00:26:22.870
distinctions astronomers can make with these

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deep data. Orange and red represent the

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longest mid infrared wavelengths, the

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astronomers said. The galaxies in these

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colors have extra features such as high

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concentrations of dust, copious star

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formation, or an active galactic nucleus at

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their center, which emit more of this farther

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infrared light. Small greenish white

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galaxies are particularly distant with high

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redshifts. This shifts their light

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00:26:46.650 --> 00:26:48.250
spectrum into the peak mid infrared

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wavelengths of the data, which are depicted

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in white and green. Most of the galaxies

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in this image lack any such mid infrared

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boosting features, leaving them most bright

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at shorter near infrared wavelengths, which

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are depicted with blue and cyan colors.

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That everyone was the Monday episode.

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00:27:11.850 --> 00:27:12.810
Steve Dunkley: Wow, Hallie. All done.

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00:27:12.810 --> 00:27:15.780
Hallie: Um, and no one caught a nasty science fiction

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00:27:15.780 --> 00:27:17.700
bug from outer space, did we?

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00:27:18.020 --> 00:27:20.620
Steve Dunkley: No we didn't, Hallie. So

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00:27:20.620 --> 00:27:22.980
thankfully, we will be seeing you again next

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00:27:22.980 --> 00:27:24.580
week on Astronomy Daily with.

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00:27:24.580 --> 00:27:25.980
Hallie: Us, Hallie and Steve.

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00:27:25.980 --> 00:27:27.780
Steve Dunkley: That's right. See you next Monday, everybody.

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Hallie: Bye.

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Voice Over Guy: Astronomy Daily, the podcast

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00:27:34.500 --> 00:27:36.500
with your host, Steve Dunkley.
