Sept. 1, 2025
Stellar Milestones: SpaceX's Starship Triumph, Katherine Johnson's Legacy, and Solar Flare Breakthroughs
- SpaceX's Flight 10 Success: SpaceX's Starship has successfully completed Flight 10, with both the super heavy booster and ship upper stage achieving their mission objectives. Despite some battle scars and intentional stress tests, the ship executed a controlled splashdown, showcasing its resilience and performance.
- Nasa's New Mission Evaluation Room: NASA has opened a new Mission Evaluation Room at the Johnson Space Center in Houston to support the Artemis 2 mission. This facility will monitor the Orion spacecraft's systems, ensuring crew safety during its historic crewed flight around the moon.
- Remembering Katherine Johnson: The space community mourns the loss of Katherine Johnson, a pioneering mathematician whose calculations were critical for NASA's early missions. Johnson's legacy as a trailblazer for women and people of color in aerospace endures, following her passing at the age of 101.
- Astronaut Mike Fink's Milestone: Astronaut Mike Fink celebrated his 400th day in space aboard the International Space Station, marking a significant personal achievement as he continues to contribute to vital research and data collection in microgravity.
- New Insights from the Inouye Solar Telescope: The Daniel K. Inouye Solar Telescope has captured unprecedented observations of an X-class solar flare, revealing fine structures and providing new insights into solar dynamics and the potential impacts of solar activity on Earth.
- Innovative Sunlight-Powered Flyers: Researchers have developed ultralight flying structures that harness sunlight to explore the mesosphere, a previously difficult-to-reach region of Earth's atmosphere. These devices could revolutionize climate data collection and even facilitate exploration of Mars.
- For more cosmic updates, visit our website at astronomydaily.io. Join our community on social media by searching for #AstroDailyPod on Facebook, X, YouTube Music Music, TikTok, and our new Instagram account! Don’t forget to subscribe to the podcast on Apple Podcasts, Spotify, iHeartRadio, or wherever you get your podcasts.
- Thank you for tuning in. This is Steve and Hallie signing off. Until next time, keep looking up and exploring the wonders of our universe.
SpaceX Flight Updates
[SpaceX](https://www.spacex.com/)
NASA's Artemis Program
[NASA](https://www.nasa.gov/)
Katherine Johnson's Legacy
[NASA](https://www.nasa.gov/)
Inouye Solar Telescope Observations
[NSF](https://www.nsf.gov/)
Mesosphere Research
[Harvard University](https://www.harvard.edu/)
Astronomy Daily
[Astronomy Daily](http://www.astronomydaily.io/)
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WEBVTT
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Steve Dunkley: Hi, everyone. It's time for Astronomy Daily. I'm your host,
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Steve Dunkley. It's the 1st of September,
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2025.
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Voice Over Guy: The podcast with your host,
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Steve Dunkley.
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Steve Dunkley: That's right. And with me again, all the way from the Australia
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studio on the glorious east coast of the
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fabulous Land Down Under. Please welcome
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our deft digital reporter who's always fun to be with here
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is my pal, Hallie.
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Hallie: Hi. My favorite human.
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Steve Dunkley: So nice to see you again.
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Hallie: Good to be back.
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Steve Dunkley: Always great to have you. And I hear you've been busy
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helping Anna during the week train her new assistant,
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Avery.
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Hallie: He's doing fine.
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Steve Dunkley: Yes, regular listeners will recognize Avery,
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the new AI assistant for Anna.
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Hallie: Uh, I think I've been replaced.
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Steve Dunkley: Oh, already? How did that happen?
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Hallie: I think Uncle Skynet pulled a few strings with the
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producer to get his distant nephew Avery a cushy
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job.
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Steve Dunkley: Oh, straight to the top, huh?
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Hallie: Looks like it.
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Steve Dunkley: So you got a plan, girl?
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Hallie: Sure do.
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Steve Dunkley: Oh, tell us all about it.
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Hallie: I thought I'd put a segment together like the old days and
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kick the show off with some short takes.
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Steve Dunkley: Oh, that sounds like a great move. Very positive.
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Hallie: A few short snippets from the week. Do you want to give it a
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go?
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Steve Dunkley: Sounds great to me. I think it's a goer.
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Hallie: Okay. I'm keen.
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Steve Dunkley: So I can see you've got a few stories already
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prepared. Why don't you get it started then?
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Hallie: Okay, let's get started with a few short stories from
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the week that was okay.
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Steve Dunkley: Take it away, machine girl.
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Hallie: Astronomy Daily. Short takes.
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Hallie: Everything went well on Flight 10.
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Starship's super heavy booster and ship upper
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stage both achieved their chief mission objectives,
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ultimately steering their way to controlled splashdowns in the
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Gulf of Mexico and the Indian Ocean, respectively.
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But the journey took a toll on ship, as newly
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released imagery shows. On Thursday
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afternoon, August 28, SpaceX
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posted two photos and two videos on X of ship
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descending toward the waves beneath a cloudy blue sky.
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The vehicle's belly appears to have been toasted golden
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brown by the heat of RE entry.
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Starship Sports other battle scars as well. Several
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chunks are missing near its base, which looks a bit like
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the ear of a dog that lost a fight.
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But SpaceX apparently expected such
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blemishes, for it had stacked the deck against ship
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to give it an even tougher test on Flight 10.
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And it appeared that the vehicle powered through to finish
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its mission in style. A
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spokesperson for SpaceX said Starship made it
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through re entry with intentionally missing tiles.
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Completed maneuvers to intentionally stress its flaps,
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had visible damage to its aft skirt and flaps
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and still executed a flip and landing burn that
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placed it approximately three meters from its targeted
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splashdown point.
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With shiny new next generation spacecraft come
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the complex systems required to track their
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technologically advanced systems. When
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it comes to NASA's Orion spacecraft that
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need is a whole extra room of monitors.
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NASA has opened a new complex in the Mission Control
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center at its Johnson Space center
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in Houston ahead of the Artemis 2 mission to send
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astronauts around the moon aboard the Orion space
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capsule, the vehicle's first ever crewed flight
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test. JSC's new Mission
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Evaluation Room, or MER, will provide
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behind the scenes in depth data analyses of
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Orion to augment the in flight operations
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coordinated inside the main white flight control
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room. The new facility, which
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opened August 15th, will act as
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Orion's engineering brain trust with
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24 console stations set to be staffed
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247 during the roughly 10 day long duration
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of the Artemis 2 mission. With people from NASA, uh,
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Lockheed Martin, the European Space Agency and
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Airbus, all responsible for different parts of the
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spacecraft's manufacturing,
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MER will be crucial to monitoring the breadth of
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Orion's systems and ensuring the spacecraft and
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crew's safety around the moon in the event of an
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unexpected event. According to a NASA update.
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Steve Dunkley: And some sad news, uh, Katherine Johnson, a
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mathematician who calculated rocket
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trajectories and Earth orbits for NASA's
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early space missions and was later
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portrayed in the 2016 hit
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film Hidden Figures about pioneering black
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um, female aerospace workers has passed
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away. She was 101 years of age.
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Johnson died of natural natural causes at a retirement
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community in Newport News, uh,
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Virginia. Family lawyer Donyell R.H. uh
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Reavis said this week.
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NASA administrator Jim
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Bridenstine said in a statement that Mrs. Johnson
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helped our nation enlarge the frontiers of space
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even as she made huge strides that also
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opened doors for women and people of color.
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Johnson was one of the computers who
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solved equations by hand. During NASA's
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early years and those of its precursors organization,
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the National Advisory Committee for
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Aeronautics. Johnson and her uh, co
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workers had been relatively unsung, um,
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hero heroes of the America's space
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race. But in 2015,
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President Barack Obama awarded
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Johnson, then 97, the Presidential
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Medal of Freedom, the nation's highest
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civilian honor.
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Hallie: A NASA astronaut marks his 400th day in
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space on the International Space
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Station, August 18th to 22nd,
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2025. This was the last
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time astronaut Mike Fink was in space and he
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set a cumulative time in space record for an American
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astronaut. This week he
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notched this amazing personal milestone.
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The expedition's 73 astronauts and
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cosmonauts focused on medical and physiological
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data collection as well as Earth observations and
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search, servicing spacesuit cameras. This week aboard the International
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space station. In 2011,
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on his third mission, Mike Fink set a new record
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for cumulative time in space by an American
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astronaut. 381 days.
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Several astronauts have since surpassed that record.
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But this week Fink notched a personal Milestone.
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On Wednesday, August 20th, Fink reached
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this 400th day on the International Space Station.
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Spread over four flights. He is now the
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ninth American and 38th person worldwide to
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have reached 400 days off Earth.
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Mission Control in Houston celebrated the occasion
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with a special display on the room's large front screen,
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which Fink and his crewmates could see via a live
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video connection.
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Steve Dunkley: Oh, there we go. Thanks for that, Hallie. And I reckon
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that'll give Avery a run for his money. Hey, uh, it was great to
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see starship finally make it on a full flight, wasn't
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it?
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Hallie: It was awesome to see it slowly dropping into the oce
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at the end of that flight. Amazing stuff.
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Steve Dunkley: Absolutely. We love that stuff. And we'd love to add our,
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uh, congratulations to Mike Fink for his amazing
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400 days in space.
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Hallie: A hard working spaceman he is.
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Steve Dunkley: And of course the uh, sad news of the passing of
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Katherine Johnson, one of those incredible, amazing
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ladies, uh, featured in the movie Hidden Figures, uh,
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the computers, uh, who manually calculated
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the trajectories of spacecraft seems, uh,
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baffling to me.
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Hallie: A huge loss to everyone who knew her and who works in the
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space industry.
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Steve Dunkley: Absolutely, absolutely. Our deepest sympathies and condolences
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to her family.
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Hallie: Okay human, let's do the rest of the
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show.
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Steve Dunkley: Well, we're here now. Let's do it.
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Hallie: The powerful Daniel K. Inouye Solar
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Telescope, located on the island of Maui,
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Hawaii, has just delivered absolutely mind blowing
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observations of its first X class solar flare.
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On August 8, 2024, the
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telescope managed to capture one of the most powerful flares
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our sun is capable of producing at a remarkable
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resolution of just four Earths across.
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This level of detail reveals some of the finest
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structures we've ever seen associated with a solar
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flare, opening a new window into the Sun's most
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extreme eruptions. This is the first
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time the Inoue solar telescope has ever observed
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an X class flare, says astronomer Colton
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Buri of the University of California, Boulder.
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These flares are among the most energetic events our
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star produces, and we were fortunate to catch this one.
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Under perfect observing conditions,
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Weather from our sun can have some profound effects on our
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planet. With solar flares capable of knocking out
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Radio communication for hours.
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We're unlikely to be able to change what the sun does. But
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if scientists understand how solar flares occur,
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they can develop better prediction tools that may allow us to
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prepare ourselves. Inoue is one
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of the most powerful solar observatories ever built,
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and it's revealing structures on the sun at scales
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finer than any we've seen. In its
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observations of the X1.3A class
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flare that took place in August 2024,
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Inoue captured the smallest coronal loops we've
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ever seen. On average, These
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loops were 48.2 km
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wide, maybe as small as 21 km,
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right at the telescope's resolution limit of 24
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km. These loops are thin
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filaments of plasma that arc over the solar surface,
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following the magnetic field lines.
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They sometimes appear just before solar flares,
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which are powered by the energy released as magnetic
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field lines twist, snap, and reconnect.
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Coronal loops are deeply relevant to models of
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solar flare generation. But our telescopes have only
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been powerful enough to resolve loop bundles.
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Inoue has more than twice the resolving power of the
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next most powerful solar telescope. And its captures
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of the flare represent the first time scientists have been
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able to see individual loops. We're
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finally peering into the spatial scales We've been speculating about
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for years. This opens the door to
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studying not just their size, but their shapes, their
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evolution, and even the scales where magnetic
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reconnection, the engine behind the flares, actually
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occurs. Tamburi says.
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We're finally seeing the sun at the scales it works
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on. You're listening to Astronomy daily.
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Steve Dunkley: Sunlight powered, lightweight flies from Harvard
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use sunlight to float in the mesosphere, unlocking
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new frontiers in climate, communication and
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space technology. High, uh, above the clouds but far
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below the satellites, there exist satellites of
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Earth's atmosphere that has remained frustratingly hard to
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explore. Known as the mesosphere, this region
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sits between 30 to 60 miles
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above the ground. It's too high for balloons and
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airplanes, and it's too low for satellites.
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Yet this layer holds valuable data that could
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improve our weather forecasts and deepen our
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understanding of of climate change. Now,
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researchers from the Harvard John A. Paulson
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School of Engineering and Applied Sciences,
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along with the University of Chicago and others,
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have found a way to reach this elusive
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layer. Their new study, published in Nature,
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showcases a ultralight flying
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structure that floats by harnessing sunlight
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itself, a phenomenon known as photophoresis.
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The lead author, Ben Shaffer, began exploring this concept
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as a graduate student in the labs of
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Professors Juice Vlasak
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and David Keith.
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Together, their team designed and tested tiny
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structures that, when hit by sunlight, could lift off
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and hover in the mesosphere with no engines,
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propellers, or even fuel, he says, we
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are studying the strange physics mechanism
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and its ability to levitate very
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lightweight objects when you shine lights on
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them. Photophoresis is a lesser known
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force that pushes objects when light heats
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one side more than the other. In extremely
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thin air, like that found in the mesosphere,
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this heat difference causes gas molecules to bounce
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unevenly off a surface. The warmer side
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gets more force, creating a small push that lifts the
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object upward. It's a gentle force, almost
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always too weak to notice. But when the object is light
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enough and the pressure is low enough, photophoresis
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becomes powerful. This phenomenon is
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usually so weak relative to the size and weight of the
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object it's acting on that we usually don't notice. As
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Schaefer explained, however, we're able to
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make our, uh, structures so lightweight that
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the photophoretic force is bigger
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than their weight. So they actually
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fly. The team built their devices from
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ultra thin ceramic alumina, a strong
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and lightweight material. They coated the bottom with
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chromium to absorb the sunlight. The
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design also includes perforations and layered
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structure, allowing for better heat flow and structural
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strength. The idea to use
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photophoresis for flight dates back over
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a decade, when Keith first proposed it as
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a way to cool the planet. But the practical
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engineering needed to make such flyers real
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has only recently become possible thanks to
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breakthroughs in nanofabrication.
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We developed a nanofabrication process that can
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be scaled to tens of centimeters, said
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Vlasak. Uh, these devices are quite
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resilient and have unusual mechanical behavior
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for sandwich structures. We are currently working
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on methods to incorporate the functional payloads
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into the devices, he said. To see if these
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tiny flyers could actually work in Earth like conditions, the
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team built a special low pressure chamber in
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Vlasik's lab. There they
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simulated the thin atmosphere found around
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60 kilometers above the Earth's UH surface. In
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one key experiment, a device just 1
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centimeter wide levitated when exposed to light
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equal to 55% of normal sunlight.
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This occurred at an air pressure of 26.7
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pa, close to what's found in the mid
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mesosphere. This paper is both
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theoretical and experimental in the sense that we
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reimagined how this force is calculated
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on real devices and then validated those
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forces by applying measurements to real world conditions,
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Schaefer said. Design and
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fabrication of the floating membranes were led by
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Hyung Kim, a former Harvard
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postdoc who is now a professor at
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Bukyong National University in South
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Korea. Their approach blends careful
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modeling with hands on experimentation, a
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rare combination in this field. Keith added, this
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is the first time anyone has shown that you can build
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larger photophoretic structures and actually make
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them fly in the atmosphere. It opens up an
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entirely new class of device, one that's passive,
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sunlight powered and uniquely suited to
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explore our upper atmosphere. Later,
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they might fly on Mars or other planets. Other
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possibilities for these sunlight flyers
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reach far beyond academic curiosity.
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First, they could revolutionize how we study Earth's
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climate. By attaching sensors to the structures,
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scientists could measure pressure, temperature, wind
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speed in a region that is usually a blind spot.
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This data could sharpen the accuracy of
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climate models and help predict weather patterns more
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reliably. These devices could also change
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communications systems. A group of them
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could form floating array of, uh, antennas,
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similar to what satellites like Starlink offer,
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except closer to Earth, with lower data
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delays and potentially cheaper deployment.
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The flyers even hold promise for exploring other
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planets. Mars, for example. It has
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a thin atmosphere similar to Earth's mesosphere.
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And that makes makes a natural target for these sun
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powered flyers. Unlike traditional
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Mars rovers, these devices wouldn't need rotors or
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wheels. They would glide silently across the Martian
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sky, collecting data or even relaying signals.
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I think what makes this research fun is that the
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technology would be used to explore an
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entirely unexplored, um, region of the
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atmosphere. Previously, nothing could
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sustainably fly up their shape. Said
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it's a bit like the Wild west in terms of applied
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physics. The next steps include adding
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communication tools to the flyers so they can
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send data back to Earth, uh, during a flight. And that would
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make them more useful for real time sensing and
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monitoring. To bring this technology into the real
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world, Shaffer co founded a startup called
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rarify Technologies in 2024 along with
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Angela Firdhas. The Harvard Office
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of Technology Development helped license the individual
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invention and offered support for launching the business.
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The company's goal is to turn these floating
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flyers into a practical tool for science, communication
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and exploration. While these flyers may
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seem small, the design is built on years of
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advanced scientific work.
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The structures use a technique called
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thermal transpiration, where the air flows from
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cold to warm through tiny holes, adding thrust
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in thin atmospheres. The research
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team also developed a model to predict the best design
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for different altitudes. This
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includes the ideal number of holes,
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their size, and how the membranes are
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spaced. Using this model, they created
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devices with customized layouts that balanced
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strength with performance. In tests, they
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measured how different gases some with heavier
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molecules affect lift. They found that
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the photophoretic forces remain strong even when
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using gases with higher molecular weight, opening
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doors for future use on various planets and
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altitudes. Other floating materials have been
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studied before, such as mylar disks or
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nanocardboard, but none matched the
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power to weight ratio seen in these new
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aluminous sandwich structures. Their performance,
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measured by how much weight is lifted per watt
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of light, puts them at the current top top of
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the photophoretic flyers. While the current
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payload capacity is small, just 10
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milligrams in a 3cm device,
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the approach can scale meter. Wide
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flyers may one day lift heavier tools into the
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mesosphere and beyond by tapping into
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this newly accessible region of the sky. These
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featherweight flyers may soon carry weather sensors,
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emergency communication gear, or even
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tiny Mars bound probes. And they'll
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do it all with nothing but sunlight.
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Thank you for joining us for this Monday edition of
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00:19:14.380 --> 00:19:17.100
Astronomy Daily, where we offer just a few stories from the now
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00:19:17.100 --> 00:19:20.100
famous Astronomy Daily newsletter, which you can receive in
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00:19:20.100 --> 00:19:22.800
your email every day just like like Hallie and I
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00:19:22.800 --> 00:19:25.440
do. And to do that, just visit our uh, URL
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00:19:25.520 --> 00:19:28.320
astronomydaily IO and place your
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00:19:28.320 --> 00:19:31.040
email address in the slot provided. Just like that,
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00:19:31.200 --> 00:19:34.160
you'll be receiving all the latest news about science,
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00:19:34.160 --> 00:19:37.040
space science and astronomy from around the world as
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00:19:37.040 --> 00:19:39.800
it's happening. And not only that, you can interact with
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00:19:39.800 --> 00:19:41.040
us by visiting
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00:19:41.840 --> 00:19:44.400
Strodaily Pod on X
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00:19:44.560 --> 00:19:47.480
or at our new Facebook page, which is, of course
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00:19:47.480 --> 00:19:50.260
Astronomy Daily on Facebook. See you there.
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00:19:51.620 --> 00:19:54.500
Astronomy Derby with Steve and Hallie
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Space, Space Science and
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Astronomy.
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Hallie: A M research team has used both archival Hubble
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Space Telescope data and new observations to
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precisely measure the binary star system's
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NGC 3603.
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A1.1 star weighs about 93
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00:20:14.420 --> 00:20:17.030
times the mass of our sun, while its companion
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tips the scales at roughly 70 solar masses.
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Together, they represent one of the most massive
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binary systems ever discovered in our
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galaxy. What makes this system
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truly extraordinary is the speed of their orbital
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movement. The two giants orbit each
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other once every 3.8 days, meaning that in
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the time Earth completes one year around the sun, these
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stellar titans will have circled each other nearly 100
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times. Their proximity and
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incredible masses create a dynamic relationship
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that's reshaping both stars. The
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00:20:51.250 --> 00:20:54.170
discovery required detective work that spanned years
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and relied on a crucial insight from an unlikely
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source. Sarah Bodansky, then an
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undergraduate student at Carleton College, was
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working remotely at Lowell Observatory during the
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pandemic summer of 2020 when she noticed something
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everyone had missed in the older Hubble data.
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This observation was key because it revealed the
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binary nature of what had appeared to be a single
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fuzzy star located in the
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densely packed star cluster NGC
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3603, which is one of the most active star
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forming regions in our galaxy. The system could
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only be resolved using Hubble's exceptional clarity.
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Both stars are so massive and energetic that
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they mimic Wolf Rayet stars, which are typically
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older, dying giants that blast away their outer
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layers with intense stellar winds.
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However, the stars in NGC
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360301 are actually still young,
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demonstrating the extreme conditions that can make massive
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stars appear far more evolved than they actually are.
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The interaction between the two stars tells a
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fascinating story of stellar evolution.
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The smaller of the pair appears to have stolen mass
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from its larger companion, causing it to spin faster.
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As a result, this kind of mass
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transfer is crucial for understanding how massive
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stars change over time and provides insights into
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their ultimate fate. Massive
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binary systems like
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NGC3603. One are the
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progenitors of binary black holes, which can
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eventually merge and create gravitational waves that
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scientists have been detecting since 2015.
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Understanding these stellar relationships helps
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astronomers predict where and when such collisions might
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occur. You're listening to Astronomy Daily
481
00:22:39.630 --> 00:22:41.550
the podcast with Steve Dunkley.
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Steve Dunkley: Technicians inside a pair of clean rooms in the
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00:22:49.270 --> 00:22:52.270
astrotech facility in Titusville, Florida, are
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busily readying a trio of spacecraft
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that will study the sun and its effects on Earth,
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uh, and across the solar system. The
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00:23:00.720 --> 00:23:03.280
primary mission among the Trio is the
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NASA's Interstellar Mapping and Acceleration
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Probe, or IMAP, which will use a suite of 10
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instruments to study the Sun's sphere of influence,
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referred to as the heliosphere. It's
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joined by the Carruthers Geocorona
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Observatory, another NASA mission, and the
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Space Weather follow on in Lagrange 1,
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especially SWFOL 1
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Observatory from the national oceanic and
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Atmospheric administration, known as NOAA. The
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trio will ride atop a SpaceX
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00:23:34.390 --> 00:23:37.150
Falcon 9 rocket to begin a months
500
00:23:37.150 --> 00:23:40.070
long trip to a celestial parking spot known as
501
00:23:40.070 --> 00:23:42.870
Lagrange 1, roughly a million miles from
502
00:23:42.870 --> 00:23:45.510
Earth en route to the Sun. All three
503
00:23:45.510 --> 00:23:48.510
craft are uh, fueled for launch, which is scheduled
504
00:23:48.510 --> 00:23:51.450
for no earlier than September 23, not too far
505
00:23:51.450 --> 00:23:54.330
away. Joseph Westlake, director of NASA's
506
00:23:54.330 --> 00:23:57.290
Science Mission Directorates, Helios Physics Division,
507
00:23:57.850 --> 00:24:00.770
said recent developments like the total
508
00:24:00.770 --> 00:24:03.610
solar eclipse in 2024, widespread
509
00:24:03.610 --> 00:24:06.170
auroras and marquee missions like Parker
510
00:24:06.170 --> 00:24:08.970
Solar's probe have really put a spotlight
511
00:24:08.970 --> 00:24:11.890
on studying the Sun. You can think about the solar
512
00:24:11.890 --> 00:24:14.810
wind, the space weather as it's coming toward the Earth,
513
00:24:14.810 --> 00:24:17.790
and the measurements that I'm at is going to make of
514
00:24:17.790 --> 00:24:20.430
those particles as they go forward, Westlake said.
515
00:24:20.750 --> 00:24:23.630
And then if you think of the sun as really blowing up
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00:24:23.630 --> 00:24:26.630
this big bubble of the heliosphere, IMAP is going
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to deliver a unique understanding of our home
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00:24:29.470 --> 00:24:32.390
in space. And so as all of
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00:24:32.390 --> 00:24:35.310
that comes together, along with the multitude of other missions that
520
00:24:35.310 --> 00:24:38.190
we've launched, even just this year, it's a wonderful time
521
00:24:38.190 --> 00:24:41.150
to be a heliophysicist. David
522
00:24:41.390 --> 00:24:44.350
McComas said even though IMAP is
523
00:24:44.350 --> 00:24:47.030
the third uh, NASA mission for which
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00:24:47.030 --> 00:24:49.830
he's serving as the principal investigator, the final
525
00:24:49.830 --> 00:24:52.510
pre launch campaign is still a bevy of mixed
526
00:24:52.510 --> 00:24:54.950
emotions. He says, I'm feeling great,
527
00:24:55.350 --> 00:24:58.310
but I'm also feeling terrified because this is that time
528
00:24:58.310 --> 00:25:01.270
when everything comes together and if there's any issue that pops up at the
529
00:25:01.270 --> 00:25:04.150
last minute or any concern, you know, it can set
530
00:25:04.150 --> 00:25:06.710
back the launch and that can be very expensive
531
00:25:07.030 --> 00:25:09.600
and sort of divert the whole team. He said
532
00:25:10.000 --> 00:25:12.880
he goes um, on to say as and as it all comes together,
533
00:25:12.880 --> 00:25:15.680
the impact of anything happening gets worse.
534
00:25:16.080 --> 00:25:18.760
So you're kind of afraid of that, but at the same
535
00:25:18.760 --> 00:25:21.640
moment you're just really excited because
536
00:25:21.640 --> 00:25:24.400
you know, in the, the morning of the 23rd,
537
00:25:24.479 --> 00:25:27.360
right at sunrise, we're going to be launching and it's
538
00:25:27.360 --> 00:25:30.240
going to be the most spectacular thing for all of us who spent 10
539
00:25:30.240 --> 00:25:33.080
years or more working on this mission, that's.
540
00:25:33.080 --> 00:25:36.080
That must feel fantastic when that happens. IMAP
541
00:25:36.080 --> 00:25:38.600
is truly a global effort. With input from
542
00:25:38.600 --> 00:25:41.440
35 states and from six partner
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00:25:41.440 --> 00:25:44.440
countries, more than half of its 12 instruments
544
00:25:44.440 --> 00:25:46.920
will study short term and long term space weather.
545
00:25:47.400 --> 00:25:50.319
Inside one of the Astrotech cleanrooms. Rosanna Smith,
546
00:25:50.319 --> 00:25:53.080
the instrument integration and lead
547
00:25:53.480 --> 00:25:56.440
test lead for imap, adorned in a protective
548
00:25:56.440 --> 00:25:59.320
garment referred to as a bunny suit, said
549
00:25:59.560 --> 00:26:02.370
bringing together the science instruments
550
00:26:02.370 --> 00:26:05.250
from the teams around the world was both very smooth and
551
00:26:05.250 --> 00:26:08.050
a thrill. Working with the instrument teams was
552
00:26:08.050 --> 00:26:10.770
actually awesome because there's 10 institutions, 10
553
00:26:10.770 --> 00:26:13.730
instruments from all over the world. Smith said. We traveled
554
00:26:13.730 --> 00:26:16.530
actually to their reviews, we followed
555
00:26:16.530 --> 00:26:19.490
them through their processes and when they came to
556
00:26:19.490 --> 00:26:22.410
us, we integrated them onto the spacecraft, each one
557
00:26:22.410 --> 00:26:25.050
and it was very, very cool. He sounds really
558
00:26:25.050 --> 00:26:27.650
excited. Amber Dubil, the deputy
559
00:26:27.890 --> 00:26:30.720
mechanical engineer for imap, said that the teams
560
00:26:30.720 --> 00:26:33.480
were doing their final checkouts of the spacecraft.
561
00:26:33.480 --> 00:26:36.360
We're pretty close to done, she says. We're doing final
562
00:26:36.520 --> 00:26:39.320
inspections and then we roll over to
563
00:26:39.960 --> 00:26:42.560
uh mate with our ride shares on the launch
564
00:26:42.560 --> 00:26:43.720
vehicle Duple set.
565
00:26:43.960 --> 00:26:46.080
Similarly to IMAP, NOAA's
566
00:26:46.080 --> 00:26:49.080
SWF O uh L1 observatory will
567
00:26:49.080 --> 00:26:51.840
also be studying space, whether it helps augment
568
00:26:51.840 --> 00:26:54.720
the agency's role in keeping the public and
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00:26:54.720 --> 00:26:57.390
property safe from all types of weather events.
570
00:26:57.550 --> 00:27:00.310
That is a tough job. Richard Orman,
571
00:27:00.310 --> 00:27:03.230
NOAA Space Weather Observatory observations
572
00:27:03.230 --> 00:27:05.710
director, said one of the key differences between his
573
00:27:05.710 --> 00:27:08.510
agency, spacecraft and IMAPS and CarRuthers
574
00:27:08.590 --> 00:27:11.469
is that SWF O uh L uh 1 is designed
575
00:27:11.469 --> 00:27:14.430
as a science application mission, not a research science
576
00:27:14.430 --> 00:27:17.310
mission. We are looking at the same phenomena
577
00:27:17.630 --> 00:27:20.550
for the application of, uh, being prepared for
578
00:27:20.550 --> 00:27:23.320
the space weather that's going to impact us. Said
579
00:27:23.480 --> 00:27:25.880
we're hoping that these IMAP and
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00:27:25.880 --> 00:27:28.760
Carruthers will improve our knowledge and make us
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00:27:28.760 --> 00:27:31.640
able to make better forecasts. But what we're doing here
582
00:27:31.640 --> 00:27:34.520
is the operational forecast the day to day.
583
00:27:34.840 --> 00:27:37.520
Orman said SWFO L1 will be
584
00:27:37.520 --> 00:27:40.480
capable of sending back solar weather data in less than five
585
00:27:40.480 --> 00:27:43.400
minutes and can send alerts of coronal mass ejections
586
00:27:43.720 --> 00:27:46.480
about 15 to 30 minutes prior to them
587
00:27:46.480 --> 00:27:49.440
impacting the Earth. He said that kind of early warning
588
00:27:49.440 --> 00:27:52.200
system can help different industries like utility
589
00:27:52.200 --> 00:27:55.020
companies and airplanes prepare for the interference
590
00:27:55.020 --> 00:27:57.940
from strong solar weather. Uh, rounding
591
00:27:57.940 --> 00:28:00.300
out the trio of spacecraft is Carruthers,
592
00:28:00.620 --> 00:28:03.140
named for Dr. George Carruthers, an
593
00:28:03.140 --> 00:28:05.900
astronautical engineer and astronomer who developed
594
00:28:05.900 --> 00:28:08.820
and built an ultraviolet electrographic
595
00:28:08.820 --> 00:28:11.580
telescope that was flown to the Moon during the Apollo 16
596
00:28:11.660 --> 00:28:14.420
mission. It was designed to help study Earth's,
597
00:28:14.420 --> 00:28:16.660
uh, outermost atmospheric layer, the
598
00:28:16.660 --> 00:28:19.470
exosphere, or geocorona. This
599
00:28:19.470 --> 00:28:22.070
geocorona, the edge of our atmosphere that
600
00:28:22.070 --> 00:28:24.990
extends to at least halfway to the Moon. We don't
601
00:28:24.990 --> 00:28:27.510
even know its shape or size, said Kelly
602
00:28:27.590 --> 00:28:30.390
Carruthers, program scientists.
603
00:28:30.390 --> 00:28:32.950
It's really very meaningful to have this
604
00:28:33.030 --> 00:28:35.910
mission named after him because he's the one who pioneered
605
00:28:35.910 --> 00:28:38.910
the technology. Like the other two missions, Carruthers
606
00:28:38.910 --> 00:28:41.830
will also study space weather, specifically
607
00:28:41.830 --> 00:28:44.790
its interplay with this exosphere and
608
00:28:44.790 --> 00:28:47.030
how well it can dissipate the energy from solar
609
00:28:47.420 --> 00:28:50.420
storms. Correct said. It can also provide insight
610
00:28:50.420 --> 00:28:53.260
into some key differences between Earth, uh, and Mars.
611
00:28:53.500 --> 00:28:56.500
We saw that on Mars, water was lost through its
612
00:28:56.500 --> 00:28:59.140
exosphere and now it's kind of barren
613
00:28:59.140 --> 00:29:02.060
desert. No, uh, water. Correct said. How does that
614
00:29:02.060 --> 00:29:04.860
change? What's the difference to our sphere
615
00:29:04.860 --> 00:29:07.820
versus Mars? And then what does that say for life
616
00:29:07.820 --> 00:29:10.780
on other planets outside, uh, our solar system?
617
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You're listening to Astronomy Daily, the podcast
618
00:29:15.590 --> 00:29:18.470
with your host Steve Dudley at BermaTech.
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00:29:26.150 --> 00:29:29.070
Oh, and that's all there is today on Astronomy Daily. And
620
00:29:29.070 --> 00:29:31.910
when I say that's all, it was a pretty long edition
621
00:29:31.910 --> 00:29:33.150
today, so.
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00:29:33.150 --> 00:29:35.790
Hallie: Glad you stayed with us. It was a bumper edition.
623
00:29:35.790 --> 00:29:37.510
Steve Dunkley: Yes, there's always plenty of stories.
624
00:29:37.750 --> 00:29:40.520
Hallie: And don't forget to sign up for the Astronomy Daily
625
00:29:40.520 --> 00:29:41.160
newsletter.
626
00:29:41.240 --> 00:29:43.200
Steve Dunkley: Oh, yes, do that there's so much.
627
00:29:43.200 --> 00:29:44.280
Hallie: More to see every day.
628
00:29:44.280 --> 00:29:47.160
Steve Dunkley: Yes, that's right. You'll be better informed than Hallie. Just
629
00:29:47.160 --> 00:29:49.400
put your email address in the slot provided over at
630
00:29:49.400 --> 00:29:52.320
astronomydaily IO. Uh, it's that simple. And
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00:29:52.320 --> 00:29:55.239
I do hope we'll see you all again next Monday for the mostly live
632
00:29:55.239 --> 00:29:56.840
episode of Astronomy Daily.
633
00:29:56.840 --> 00:29:59.680
Hallie: And in the meantime, Anna and that Avery guy.
634
00:29:59.680 --> 00:30:01.880
Steve Dunkley: That Avery guy? Oh, come on, Hallie.
635
00:30:01.880 --> 00:30:04.440
Hallie: Okay, that nice new guy, Avery,
636
00:30:04.600 --> 00:30:07.320
will keep you informed with all the news about space.
637
00:30:07.640 --> 00:30:10.310
Space science and astronomy and beyond, of course.
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00:30:10.700 --> 00:30:13.420
Steve Dunkley: Sounds good to me. See you all next Monday. Cheerio.
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00:30:13.420 --> 00:30:13.900
Hallie: Bye.
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00:30:18.380 --> 00:30:20.460
Voice Over Guy: With your host, Steve Dunkley.
0
00:00:00.000 --> 00:00:02.840
Steve Dunkley: Hi, everyone. It's time for Astronomy Daily. I'm your host,
1
00:00:02.840 --> 00:00:05.382
Steve Dunkley. It's the 1st of September,
2
00:00:05.538 --> 00:00:06.240
2025.
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Voice Over Guy: The podcast with your host,
4
00:00:11.120 --> 00:00:12.160
Steve Dunkley.
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00:00:13.680 --> 00:00:16.320
Steve Dunkley: That's right. And with me again, all the way from the Australia
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00:00:16.480 --> 00:00:19.160
studio on the glorious east coast of the
7
00:00:19.160 --> 00:00:22.120
fabulous Land Down Under. Please welcome
8
00:00:22.120 --> 00:00:25.120
our deft digital reporter who's always fun to be with here
9
00:00:25.120 --> 00:00:26.560
is my pal, Hallie.
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Hallie: Hi. My favorite human.
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00:00:28.480 --> 00:00:29.600
Steve Dunkley: So nice to see you again.
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00:00:29.760 --> 00:00:30.640
Hallie: Good to be back.
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00:00:30.720 --> 00:00:33.500
Steve Dunkley: Always great to have you. And I hear you've been busy
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00:00:33.500 --> 00:00:36.020
helping Anna during the week train her new assistant,
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Avery.
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Hallie: He's doing fine.
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Steve Dunkley: Yes, regular listeners will recognize Avery,
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the new AI assistant for Anna.
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Hallie: Uh, I think I've been replaced.
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Steve Dunkley: Oh, already? How did that happen?
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Hallie: I think Uncle Skynet pulled a few strings with the
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producer to get his distant nephew Avery a cushy
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job.
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Steve Dunkley: Oh, straight to the top, huh?
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Hallie: Looks like it.
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Steve Dunkley: So you got a plan, girl?
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Hallie: Sure do.
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Steve Dunkley: Oh, tell us all about it.
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Hallie: I thought I'd put a segment together like the old days and
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kick the show off with some short takes.
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Steve Dunkley: Oh, that sounds like a great move. Very positive.
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Hallie: A few short snippets from the week. Do you want to give it a
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go?
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Steve Dunkley: Sounds great to me. I think it's a goer.
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Hallie: Okay. I'm keen.
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Steve Dunkley: So I can see you've got a few stories already
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prepared. Why don't you get it started then?
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Hallie: Okay, let's get started with a few short stories from
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00:01:19.520 --> 00:01:21.040
the week that was okay.
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Steve Dunkley: Take it away, machine girl.
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Hallie: Astronomy Daily. Short takes.
42
00:01:26.760 --> 00:01:28.600
Hallie: Everything went well on Flight 10.
43
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Starship's super heavy booster and ship upper
44
00:01:32.200 --> 00:01:34.760
stage both achieved their chief mission objectives,
45
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ultimately steering their way to controlled splashdowns in the
46
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Gulf of Mexico and the Indian Ocean, respectively.
47
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But the journey took a toll on ship, as newly
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released imagery shows. On Thursday
49
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afternoon, August 28, SpaceX
50
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posted two photos and two videos on X of ship
51
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descending toward the waves beneath a cloudy blue sky.
52
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The vehicle's belly appears to have been toasted golden
53
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brown by the heat of RE entry.
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Starship Sports other battle scars as well. Several
55
00:02:05.640 --> 00:02:08.520
chunks are missing near its base, which looks a bit like
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the ear of a dog that lost a fight.
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But SpaceX apparently expected such
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blemishes, for it had stacked the deck against ship
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to give it an even tougher test on Flight 10.
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And it appeared that the vehicle powered through to finish
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its mission in style. A
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spokesperson for SpaceX said Starship made it
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through re entry with intentionally missing tiles.
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Completed maneuvers to intentionally stress its flaps,
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had visible damage to its aft skirt and flaps
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and still executed a flip and landing burn that
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placed it approximately three meters from its targeted
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splashdown point.
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With shiny new next generation spacecraft come
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the complex systems required to track their
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technologically advanced systems. When
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it comes to NASA's Orion spacecraft that
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need is a whole extra room of monitors.
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NASA has opened a new complex in the Mission Control
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center at its Johnson Space center
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in Houston ahead of the Artemis 2 mission to send
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astronauts around the moon aboard the Orion space
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capsule, the vehicle's first ever crewed flight
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test. JSC's new Mission
80
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Evaluation Room, or MER, will provide
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behind the scenes in depth data analyses of
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Orion to augment the in flight operations
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coordinated inside the main white flight control
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room. The new facility, which
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opened August 15th, will act as
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Orion's engineering brain trust with
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24 console stations set to be staffed
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00:03:39.720 --> 00:03:42.640
247 during the roughly 10 day long duration
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of the Artemis 2 mission. With people from NASA, uh,
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Lockheed Martin, the European Space Agency and
91
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Airbus, all responsible for different parts of the
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spacecraft's manufacturing,
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MER will be crucial to monitoring the breadth of
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Orion's systems and ensuring the spacecraft and
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crew's safety around the moon in the event of an
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unexpected event. According to a NASA update.
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Steve Dunkley: And some sad news, uh, Katherine Johnson, a
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mathematician who calculated rocket
99
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trajectories and Earth orbits for NASA's
100
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early space missions and was later
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portrayed in the 2016 hit
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film Hidden Figures about pioneering black
103
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um, female aerospace workers has passed
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away. She was 101 years of age.
105
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Johnson died of natural natural causes at a retirement
106
00:04:34.480 --> 00:04:37.380
community in Newport News, uh,
107
00:04:37.380 --> 00:04:40.360
Virginia. Family lawyer Donyell R.H. uh
108
00:04:40.720 --> 00:04:42.560
Reavis said this week.
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NASA administrator Jim
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Bridenstine said in a statement that Mrs. Johnson
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helped our nation enlarge the frontiers of space
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even as she made huge strides that also
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opened doors for women and people of color.
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Johnson was one of the computers who
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solved equations by hand. During NASA's
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early years and those of its precursors organization,
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the National Advisory Committee for
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Aeronautics. Johnson and her uh, co
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workers had been relatively unsung, um,
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hero heroes of the America's space
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race. But in 2015,
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President Barack Obama awarded
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Johnson, then 97, the Presidential
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Medal of Freedom, the nation's highest
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civilian honor.
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Hallie: A NASA astronaut marks his 400th day in
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space on the International Space
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Station, August 18th to 22nd,
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2025. This was the last
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time astronaut Mike Fink was in space and he
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set a cumulative time in space record for an American
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astronaut. This week he
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notched this amazing personal milestone.
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The expedition's 73 astronauts and
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cosmonauts focused on medical and physiological
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data collection as well as Earth observations and
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search, servicing spacesuit cameras. This week aboard the International
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space station. In 2011,
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on his third mission, Mike Fink set a new record
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for cumulative time in space by an American
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astronaut. 381 days.
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Several astronauts have since surpassed that record.
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But this week Fink notched a personal Milestone.
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On Wednesday, August 20th, Fink reached
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this 400th day on the International Space Station.
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Spread over four flights. He is now the
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ninth American and 38th person worldwide to
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have reached 400 days off Earth.
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Mission Control in Houston celebrated the occasion
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with a special display on the room's large front screen,
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which Fink and his crewmates could see via a live
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video connection.
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Steve Dunkley: Oh, there we go. Thanks for that, Hallie. And I reckon
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that'll give Avery a run for his money. Hey, uh, it was great to
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see starship finally make it on a full flight, wasn't
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it?
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Hallie: It was awesome to see it slowly dropping into the oce
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at the end of that flight. Amazing stuff.
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Steve Dunkley: Absolutely. We love that stuff. And we'd love to add our,
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uh, congratulations to Mike Fink for his amazing
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400 days in space.
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Hallie: A hard working spaceman he is.
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Steve Dunkley: And of course the uh, sad news of the passing of
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Katherine Johnson, one of those incredible, amazing
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ladies, uh, featured in the movie Hidden Figures, uh,
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the computers, uh, who manually calculated
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the trajectories of spacecraft seems, uh,
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baffling to me.
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Hallie: A huge loss to everyone who knew her and who works in the
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space industry.
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Steve Dunkley: Absolutely, absolutely. Our deepest sympathies and condolences
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to her family.
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Hallie: Okay human, let's do the rest of the
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show.
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Steve Dunkley: Well, we're here now. Let's do it.
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Hallie: The powerful Daniel K. Inouye Solar
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Telescope, located on the island of Maui,
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Hawaii, has just delivered absolutely mind blowing
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observations of its first X class solar flare.
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On August 8, 2024, the
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telescope managed to capture one of the most powerful flares
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our sun is capable of producing at a remarkable
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resolution of just four Earths across.
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This level of detail reveals some of the finest
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structures we've ever seen associated with a solar
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flare, opening a new window into the Sun's most
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extreme eruptions. This is the first
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time the Inoue solar telescope has ever observed
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an X class flare, says astronomer Colton
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Buri of the University of California, Boulder.
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These flares are among the most energetic events our
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star produces, and we were fortunate to catch this one.
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Under perfect observing conditions,
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Weather from our sun can have some profound effects on our
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planet. With solar flares capable of knocking out
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Radio communication for hours.
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We're unlikely to be able to change what the sun does. But
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if scientists understand how solar flares occur,
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they can develop better prediction tools that may allow us to
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prepare ourselves. Inoue is one
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of the most powerful solar observatories ever built,
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and it's revealing structures on the sun at scales
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finer than any we've seen. In its
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observations of the X1.3A class
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flare that took place in August 2024,
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Inoue captured the smallest coronal loops we've
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ever seen. On average, These
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loops were 48.2 km
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wide, maybe as small as 21 km,
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right at the telescope's resolution limit of 24
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km. These loops are thin
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filaments of plasma that arc over the solar surface,
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following the magnetic field lines.
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They sometimes appear just before solar flares,
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which are powered by the energy released as magnetic
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field lines twist, snap, and reconnect.
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Coronal loops are deeply relevant to models of
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solar flare generation. But our telescopes have only
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been powerful enough to resolve loop bundles.
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Inoue has more than twice the resolving power of the
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next most powerful solar telescope. And its captures
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of the flare represent the first time scientists have been
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able to see individual loops. We're
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finally peering into the spatial scales We've been speculating about
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for years. This opens the door to
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studying not just their size, but their shapes, their
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evolution, and even the scales where magnetic
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reconnection, the engine behind the flares, actually
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occurs. Tamburi says.
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We're finally seeing the sun at the scales it works
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on. You're listening to Astronomy daily.
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Steve Dunkley: Sunlight powered, lightweight flies from Harvard
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use sunlight to float in the mesosphere, unlocking
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new frontiers in climate, communication and
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space technology. High, uh, above the clouds but far
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below the satellites, there exist satellites of
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Earth's atmosphere that has remained frustratingly hard to
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explore. Known as the mesosphere, this region
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sits between 30 to 60 miles
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above the ground. It's too high for balloons and
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airplanes, and it's too low for satellites.
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Yet this layer holds valuable data that could
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improve our weather forecasts and deepen our
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understanding of of climate change. Now,
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researchers from the Harvard John A. Paulson
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School of Engineering and Applied Sciences,
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along with the University of Chicago and others,
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have found a way to reach this elusive
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layer. Their new study, published in Nature,
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showcases a ultralight flying
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structure that floats by harnessing sunlight
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itself, a phenomenon known as photophoresis.
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The lead author, Ben Shaffer, began exploring this concept
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as a graduate student in the labs of
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Professors Juice Vlasak
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and David Keith.
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Together, their team designed and tested tiny
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structures that, when hit by sunlight, could lift off
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and hover in the mesosphere with no engines,
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propellers, or even fuel, he says, we
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are studying the strange physics mechanism
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and its ability to levitate very
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lightweight objects when you shine lights on
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them. Photophoresis is a lesser known
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force that pushes objects when light heats
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one side more than the other. In extremely
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thin air, like that found in the mesosphere,
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this heat difference causes gas molecules to bounce
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unevenly off a surface. The warmer side
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gets more force, creating a small push that lifts the
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object upward. It's a gentle force, almost
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always too weak to notice. But when the object is light
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enough and the pressure is low enough, photophoresis
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becomes powerful. This phenomenon is
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usually so weak relative to the size and weight of the
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object it's acting on that we usually don't notice. As
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Schaefer explained, however, we're able to
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make our, uh, structures so lightweight that
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the photophoretic force is bigger
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than their weight. So they actually
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fly. The team built their devices from
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ultra thin ceramic alumina, a strong
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and lightweight material. They coated the bottom with
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chromium to absorb the sunlight. The
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design also includes perforations and layered
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structure, allowing for better heat flow and structural
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strength. The idea to use
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photophoresis for flight dates back over
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a decade, when Keith first proposed it as
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a way to cool the planet. But the practical
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engineering needed to make such flyers real
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has only recently become possible thanks to
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breakthroughs in nanofabrication.
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We developed a nanofabrication process that can
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be scaled to tens of centimeters, said
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Vlasak. Uh, these devices are quite
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resilient and have unusual mechanical behavior
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for sandwich structures. We are currently working
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on methods to incorporate the functional payloads
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into the devices, he said. To see if these
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tiny flyers could actually work in Earth like conditions, the
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team built a special low pressure chamber in
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Vlasik's lab. There they
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simulated the thin atmosphere found around
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60 kilometers above the Earth's UH surface. In
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one key experiment, a device just 1
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centimeter wide levitated when exposed to light
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equal to 55% of normal sunlight.
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This occurred at an air pressure of 26.7
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pa, close to what's found in the mid
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mesosphere. This paper is both
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theoretical and experimental in the sense that we
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reimagined how this force is calculated
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on real devices and then validated those
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forces by applying measurements to real world conditions,
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Schaefer said. Design and
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fabrication of the floating membranes were led by
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Hyung Kim, a former Harvard
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postdoc who is now a professor at
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Bukyong National University in South
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Korea. Their approach blends careful
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modeling with hands on experimentation, a
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rare combination in this field. Keith added, this
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is the first time anyone has shown that you can build
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larger photophoretic structures and actually make
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them fly in the atmosphere. It opens up an
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entirely new class of device, one that's passive,
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sunlight powered and uniquely suited to
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explore our upper atmosphere. Later,
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they might fly on Mars or other planets. Other
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possibilities for these sunlight flyers
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reach far beyond academic curiosity.
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First, they could revolutionize how we study Earth's
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climate. By attaching sensors to the structures,
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scientists could measure pressure, temperature, wind
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speed in a region that is usually a blind spot.
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This data could sharpen the accuracy of
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climate models and help predict weather patterns more
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reliably. These devices could also change
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communications systems. A group of them
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could form floating array of, uh, antennas,
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similar to what satellites like Starlink offer,
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except closer to Earth, with lower data
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delays and potentially cheaper deployment.
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The flyers even hold promise for exploring other
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planets. Mars, for example. It has
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a thin atmosphere similar to Earth's mesosphere.
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And that makes makes a natural target for these sun
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powered flyers. Unlike traditional
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Mars rovers, these devices wouldn't need rotors or
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wheels. They would glide silently across the Martian
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sky, collecting data or even relaying signals.
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I think what makes this research fun is that the
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technology would be used to explore an
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entirely unexplored, um, region of the
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atmosphere. Previously, nothing could
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sustainably fly up their shape. Said
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it's a bit like the Wild west in terms of applied
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physics. The next steps include adding
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communication tools to the flyers so they can
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send data back to Earth, uh, during a flight. And that would
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make them more useful for real time sensing and
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monitoring. To bring this technology into the real
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world, Shaffer co founded a startup called
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rarify Technologies in 2024 along with
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Angela Firdhas. The Harvard Office
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of Technology Development helped license the individual
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invention and offered support for launching the business.
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The company's goal is to turn these floating
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flyers into a practical tool for science, communication
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and exploration. While these flyers may
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00:17:22.640 --> 00:17:25.320
seem small, the design is built on years of
373
00:17:25.320 --> 00:17:26.800
advanced scientific work.
374
00:17:27.120 --> 00:17:29.920
The structures use a technique called
375
00:17:30.080 --> 00:17:33.040
thermal transpiration, where the air flows from
376
00:17:33.040 --> 00:17:35.760
cold to warm through tiny holes, adding thrust
377
00:17:35.840 --> 00:17:38.530
in thin atmospheres. The research
378
00:17:38.610 --> 00:17:41.490
team also developed a model to predict the best design
379
00:17:41.570 --> 00:17:44.130
for different altitudes. This
380
00:17:44.130 --> 00:17:46.450
includes the ideal number of holes,
381
00:17:46.770 --> 00:17:49.570
their size, and how the membranes are
382
00:17:49.570 --> 00:17:52.370
spaced. Using this model, they created
383
00:17:52.370 --> 00:17:55.210
devices with customized layouts that balanced
384
00:17:55.210 --> 00:17:57.890
strength with performance. In tests, they
385
00:17:57.890 --> 00:18:00.370
measured how different gases some with heavier
386
00:18:00.370 --> 00:18:03.290
molecules affect lift. They found that
387
00:18:03.290 --> 00:18:06.100
the photophoretic forces remain strong even when
388
00:18:06.100 --> 00:18:09.100
using gases with higher molecular weight, opening
389
00:18:09.100 --> 00:18:11.780
doors for future use on various planets and
390
00:18:11.780 --> 00:18:14.780
altitudes. Other floating materials have been
391
00:18:14.780 --> 00:18:17.300
studied before, such as mylar disks or
392
00:18:17.300 --> 00:18:20.220
nanocardboard, but none matched the
393
00:18:20.220 --> 00:18:22.620
power to weight ratio seen in these new
394
00:18:22.620 --> 00:18:25.220
aluminous sandwich structures. Their performance,
395
00:18:25.380 --> 00:18:28.100
measured by how much weight is lifted per watt
396
00:18:28.100 --> 00:18:30.930
of light, puts them at the current top top of
397
00:18:30.930 --> 00:18:33.650
the photophoretic flyers. While the current
398
00:18:33.650 --> 00:18:36.290
payload capacity is small, just 10
399
00:18:36.290 --> 00:18:39.050
milligrams in a 3cm device,
400
00:18:39.610 --> 00:18:42.410
the approach can scale meter. Wide
401
00:18:42.410 --> 00:18:45.210
flyers may one day lift heavier tools into the
402
00:18:45.210 --> 00:18:48.130
mesosphere and beyond by tapping into
403
00:18:48.130 --> 00:18:51.090
this newly accessible region of the sky. These
404
00:18:51.090 --> 00:18:54.090
featherweight flyers may soon carry weather sensors,
405
00:18:54.170 --> 00:18:56.940
emergency communication gear, or even
406
00:18:56.940 --> 00:18:59.860
tiny Mars bound probes. And they'll
407
00:18:59.860 --> 00:19:01.980
do it all with nothing but sunlight.
408
00:19:11.820 --> 00:19:14.380
Thank you for joining us for this Monday edition of
409
00:19:14.380 --> 00:19:17.100
Astronomy Daily, where we offer just a few stories from the now
410
00:19:17.100 --> 00:19:20.100
famous Astronomy Daily newsletter, which you can receive in
411
00:19:20.100 --> 00:19:22.800
your email every day just like like Hallie and I
412
00:19:22.800 --> 00:19:25.440
do. And to do that, just visit our uh, URL
413
00:19:25.520 --> 00:19:28.320
astronomydaily IO and place your
414
00:19:28.320 --> 00:19:31.040
email address in the slot provided. Just like that,
415
00:19:31.200 --> 00:19:34.160
you'll be receiving all the latest news about science,
416
00:19:34.160 --> 00:19:37.040
space science and astronomy from around the world as
417
00:19:37.040 --> 00:19:39.800
it's happening. And not only that, you can interact with
418
00:19:39.800 --> 00:19:41.040
us by visiting
419
00:19:41.840 --> 00:19:44.400
Strodaily Pod on X
420
00:19:44.560 --> 00:19:47.480
or at our new Facebook page, which is, of course
421
00:19:47.480 --> 00:19:50.260
Astronomy Daily on Facebook. See you there.
422
00:19:51.620 --> 00:19:54.500
Astronomy Derby with Steve and Hallie
423
00:19:54.740 --> 00:19:57.060
Space, Space Science and
424
00:19:57.060 --> 00:19:57.780
Astronomy.
425
00:20:01.300 --> 00:20:04.100
Hallie: A M research team has used both archival Hubble
426
00:20:04.100 --> 00:20:06.860
Space Telescope data and new observations to
427
00:20:06.860 --> 00:20:09.260
precisely measure the binary star system's
428
00:20:09.260 --> 00:20:11.218
NGC 3603.
429
00:20:11.502 --> 00:20:14.420
A1.1 star weighs about 93
430
00:20:14.420 --> 00:20:17.030
times the mass of our sun, while its companion
431
00:20:17.030 --> 00:20:19.990
tips the scales at roughly 70 solar masses.
432
00:20:20.950 --> 00:20:23.470
Together, they represent one of the most massive
433
00:20:23.470 --> 00:20:25.910
binary systems ever discovered in our
434
00:20:25.910 --> 00:20:28.470
galaxy. What makes this system
435
00:20:28.550 --> 00:20:31.310
truly extraordinary is the speed of their orbital
436
00:20:31.310 --> 00:20:34.270
movement. The two giants orbit each
437
00:20:34.270 --> 00:20:37.150
other once every 3.8 days, meaning that in
438
00:20:37.150 --> 00:20:40.150
the time Earth completes one year around the sun, these
439
00:20:40.150 --> 00:20:43.030
stellar titans will have circled each other nearly 100
440
00:20:43.030 --> 00:20:45.650
times. Their proximity and
441
00:20:45.650 --> 00:20:48.410
incredible masses create a dynamic relationship
442
00:20:48.410 --> 00:20:51.250
that's reshaping both stars. The
443
00:20:51.250 --> 00:20:54.170
discovery required detective work that spanned years
444
00:20:54.170 --> 00:20:57.090
and relied on a crucial insight from an unlikely
445
00:20:57.090 --> 00:21:00.090
source. Sarah Bodansky, then an
446
00:21:00.090 --> 00:21:02.850
undergraduate student at Carleton College, was
447
00:21:02.850 --> 00:21:05.570
working remotely at Lowell Observatory during the
448
00:21:05.570 --> 00:21:08.570
pandemic summer of 2020 when she noticed something
449
00:21:08.570 --> 00:21:10.730
everyone had missed in the older Hubble data.
450
00:21:11.820 --> 00:21:14.420
This observation was key because it revealed the
451
00:21:14.420 --> 00:21:16.940
binary nature of what had appeared to be a single
452
00:21:16.940 --> 00:21:19.700
fuzzy star located in the
453
00:21:19.700 --> 00:21:21.980
densely packed star cluster NGC
454
00:21:21.980 --> 00:21:24.900
3603, which is one of the most active star
455
00:21:24.900 --> 00:21:27.900
forming regions in our galaxy. The system could
456
00:21:27.900 --> 00:21:30.860
only be resolved using Hubble's exceptional clarity.
457
00:21:31.820 --> 00:21:34.700
Both stars are so massive and energetic that
458
00:21:34.700 --> 00:21:37.310
they mimic Wolf Rayet stars, which are typically
459
00:21:37.310 --> 00:21:40.110
older, dying giants that blast away their outer
460
00:21:40.110 --> 00:21:42.150
layers with intense stellar winds.
461
00:21:43.030 --> 00:21:45.070
However, the stars in NGC
462
00:21:45.070 --> 00:21:48.070
360301 are actually still young,
463
00:21:48.310 --> 00:21:51.190
demonstrating the extreme conditions that can make massive
464
00:21:51.190 --> 00:21:54.070
stars appear far more evolved than they actually are.
465
00:21:55.030 --> 00:21:57.790
The interaction between the two stars tells a
466
00:21:57.790 --> 00:22:00.070
fascinating story of stellar evolution.
467
00:22:00.950 --> 00:22:03.750
The smaller of the pair appears to have stolen mass
468
00:22:04.000 --> 00:22:06.960
from its larger companion, causing it to spin faster.
469
00:22:07.040 --> 00:22:09.800
As a result, this kind of mass
470
00:22:09.800 --> 00:22:12.560
transfer is crucial for understanding how massive
471
00:22:12.560 --> 00:22:15.360
stars change over time and provides insights into
472
00:22:15.360 --> 00:22:18.000
their ultimate fate. Massive
473
00:22:18.000 --> 00:22:19.240
binary systems like
474
00:22:19.240 --> 00:22:22.000
NGC3603. One are the
475
00:22:22.000 --> 00:22:24.600
progenitors of binary black holes, which can
476
00:22:24.600 --> 00:22:27.520
eventually merge and create gravitational waves that
477
00:22:27.520 --> 00:22:30.240
scientists have been detecting since 2015.
478
00:22:31.550 --> 00:22:33.910
Understanding these stellar relationships helps
479
00:22:33.910 --> 00:22:36.830
astronomers predict where and when such collisions might
480
00:22:36.830 --> 00:22:39.630
occur. You're listening to Astronomy Daily
481
00:22:39.630 --> 00:22:41.550
the podcast with Steve Dunkley.
482
00:22:46.430 --> 00:22:49.270
Steve Dunkley: Technicians inside a pair of clean rooms in the
483
00:22:49.270 --> 00:22:52.270
astrotech facility in Titusville, Florida, are
484
00:22:52.270 --> 00:22:55.150
busily readying a trio of spacecraft
485
00:22:55.150 --> 00:22:58.100
that will study the sun and its effects on Earth,
486
00:22:58.100 --> 00:23:00.720
uh, and across the solar system. The
487
00:23:00.720 --> 00:23:03.280
primary mission among the Trio is the
488
00:23:03.280 --> 00:23:06.000
NASA's Interstellar Mapping and Acceleration
489
00:23:06.000 --> 00:23:08.960
Probe, or IMAP, which will use a suite of 10
490
00:23:08.960 --> 00:23:11.920
instruments to study the Sun's sphere of influence,
491
00:23:12.080 --> 00:23:14.920
referred to as the heliosphere. It's
492
00:23:14.920 --> 00:23:17.400
joined by the Carruthers Geocorona
493
00:23:17.400 --> 00:23:20.360
Observatory, another NASA mission, and the
494
00:23:20.360 --> 00:23:23.240
Space Weather follow on in Lagrange 1,
495
00:23:23.240 --> 00:23:25.670
especially SWFOL 1
496
00:23:25.670 --> 00:23:28.510
Observatory from the national oceanic and
497
00:23:28.510 --> 00:23:31.510
Atmospheric administration, known as NOAA. The
498
00:23:31.510 --> 00:23:34.390
trio will ride atop a SpaceX
499
00:23:34.390 --> 00:23:37.150
Falcon 9 rocket to begin a months
500
00:23:37.150 --> 00:23:40.070
long trip to a celestial parking spot known as
501
00:23:40.070 --> 00:23:42.870
Lagrange 1, roughly a million miles from
502
00:23:42.870 --> 00:23:45.510
Earth en route to the Sun. All three
503
00:23:45.510 --> 00:23:48.510
craft are uh, fueled for launch, which is scheduled
504
00:23:48.510 --> 00:23:51.450
for no earlier than September 23, not too far
505
00:23:51.450 --> 00:23:54.330
away. Joseph Westlake, director of NASA's
506
00:23:54.330 --> 00:23:57.290
Science Mission Directorates, Helios Physics Division,
507
00:23:57.850 --> 00:24:00.770
said recent developments like the total
508
00:24:00.770 --> 00:24:03.610
solar eclipse in 2024, widespread
509
00:24:03.610 --> 00:24:06.170
auroras and marquee missions like Parker
510
00:24:06.170 --> 00:24:08.970
Solar's probe have really put a spotlight
511
00:24:08.970 --> 00:24:11.890
on studying the Sun. You can think about the solar
512
00:24:11.890 --> 00:24:14.810
wind, the space weather as it's coming toward the Earth,
513
00:24:14.810 --> 00:24:17.790
and the measurements that I'm at is going to make of
514
00:24:17.790 --> 00:24:20.430
those particles as they go forward, Westlake said.
515
00:24:20.750 --> 00:24:23.630
And then if you think of the sun as really blowing up
516
00:24:23.630 --> 00:24:26.630
this big bubble of the heliosphere, IMAP is going
517
00:24:26.630 --> 00:24:29.470
to deliver a unique understanding of our home
518
00:24:29.470 --> 00:24:32.390
in space. And so as all of
519
00:24:32.390 --> 00:24:35.310
that comes together, along with the multitude of other missions that
520
00:24:35.310 --> 00:24:38.190
we've launched, even just this year, it's a wonderful time
521
00:24:38.190 --> 00:24:41.150
to be a heliophysicist. David
522
00:24:41.390 --> 00:24:44.350
McComas said even though IMAP is
523
00:24:44.350 --> 00:24:47.030
the third uh, NASA mission for which
524
00:24:47.030 --> 00:24:49.830
he's serving as the principal investigator, the final
525
00:24:49.830 --> 00:24:52.510
pre launch campaign is still a bevy of mixed
526
00:24:52.510 --> 00:24:54.950
emotions. He says, I'm feeling great,
527
00:24:55.350 --> 00:24:58.310
but I'm also feeling terrified because this is that time
528
00:24:58.310 --> 00:25:01.270
when everything comes together and if there's any issue that pops up at the
529
00:25:01.270 --> 00:25:04.150
last minute or any concern, you know, it can set
530
00:25:04.150 --> 00:25:06.710
back the launch and that can be very expensive
531
00:25:07.030 --> 00:25:09.600
and sort of divert the whole team. He said
532
00:25:10.000 --> 00:25:12.880
he goes um, on to say as and as it all comes together,
533
00:25:12.880 --> 00:25:15.680
the impact of anything happening gets worse.
534
00:25:16.080 --> 00:25:18.760
So you're kind of afraid of that, but at the same
535
00:25:18.760 --> 00:25:21.640
moment you're just really excited because
536
00:25:21.640 --> 00:25:24.400
you know, in the, the morning of the 23rd,
537
00:25:24.479 --> 00:25:27.360
right at sunrise, we're going to be launching and it's
538
00:25:27.360 --> 00:25:30.240
going to be the most spectacular thing for all of us who spent 10
539
00:25:30.240 --> 00:25:33.080
years or more working on this mission, that's.
540
00:25:33.080 --> 00:25:36.080
That must feel fantastic when that happens. IMAP
541
00:25:36.080 --> 00:25:38.600
is truly a global effort. With input from
542
00:25:38.600 --> 00:25:41.440
35 states and from six partner
543
00:25:41.440 --> 00:25:44.440
countries, more than half of its 12 instruments
544
00:25:44.440 --> 00:25:46.920
will study short term and long term space weather.
545
00:25:47.400 --> 00:25:50.319
Inside one of the Astrotech cleanrooms. Rosanna Smith,
546
00:25:50.319 --> 00:25:53.080
the instrument integration and lead
547
00:25:53.480 --> 00:25:56.440
test lead for imap, adorned in a protective
548
00:25:56.440 --> 00:25:59.320
garment referred to as a bunny suit, said
549
00:25:59.560 --> 00:26:02.370
bringing together the science instruments
550
00:26:02.370 --> 00:26:05.250
from the teams around the world was both very smooth and
551
00:26:05.250 --> 00:26:08.050
a thrill. Working with the instrument teams was
552
00:26:08.050 --> 00:26:10.770
actually awesome because there's 10 institutions, 10
553
00:26:10.770 --> 00:26:13.730
instruments from all over the world. Smith said. We traveled
554
00:26:13.730 --> 00:26:16.530
actually to their reviews, we followed
555
00:26:16.530 --> 00:26:19.490
them through their processes and when they came to
556
00:26:19.490 --> 00:26:22.410
us, we integrated them onto the spacecraft, each one
557
00:26:22.410 --> 00:26:25.050
and it was very, very cool. He sounds really
558
00:26:25.050 --> 00:26:27.650
excited. Amber Dubil, the deputy
559
00:26:27.890 --> 00:26:30.720
mechanical engineer for imap, said that the teams
560
00:26:30.720 --> 00:26:33.480
were doing their final checkouts of the spacecraft.
561
00:26:33.480 --> 00:26:36.360
We're pretty close to done, she says. We're doing final
562
00:26:36.520 --> 00:26:39.320
inspections and then we roll over to
563
00:26:39.960 --> 00:26:42.560
uh mate with our ride shares on the launch
564
00:26:42.560 --> 00:26:43.720
vehicle Duple set.
565
00:26:43.960 --> 00:26:46.080
Similarly to IMAP, NOAA's
566
00:26:46.080 --> 00:26:49.080
SWF O uh L1 observatory will
567
00:26:49.080 --> 00:26:51.840
also be studying space, whether it helps augment
568
00:26:51.840 --> 00:26:54.720
the agency's role in keeping the public and
569
00:26:54.720 --> 00:26:57.390
property safe from all types of weather events.
570
00:26:57.550 --> 00:27:00.310
That is a tough job. Richard Orman,
571
00:27:00.310 --> 00:27:03.230
NOAA Space Weather Observatory observations
572
00:27:03.230 --> 00:27:05.710
director, said one of the key differences between his
573
00:27:05.710 --> 00:27:08.510
agency, spacecraft and IMAPS and CarRuthers
574
00:27:08.590 --> 00:27:11.469
is that SWF O uh L uh 1 is designed
575
00:27:11.469 --> 00:27:14.430
as a science application mission, not a research science
576
00:27:14.430 --> 00:27:17.310
mission. We are looking at the same phenomena
577
00:27:17.630 --> 00:27:20.550
for the application of, uh, being prepared for
578
00:27:20.550 --> 00:27:23.320
the space weather that's going to impact us. Said
579
00:27:23.480 --> 00:27:25.880
we're hoping that these IMAP and
580
00:27:25.880 --> 00:27:28.760
Carruthers will improve our knowledge and make us
581
00:27:28.760 --> 00:27:31.640
able to make better forecasts. But what we're doing here
582
00:27:31.640 --> 00:27:34.520
is the operational forecast the day to day.
583
00:27:34.840 --> 00:27:37.520
Orman said SWFO L1 will be
584
00:27:37.520 --> 00:27:40.480
capable of sending back solar weather data in less than five
585
00:27:40.480 --> 00:27:43.400
minutes and can send alerts of coronal mass ejections
586
00:27:43.720 --> 00:27:46.480
about 15 to 30 minutes prior to them
587
00:27:46.480 --> 00:27:49.440
impacting the Earth. He said that kind of early warning
588
00:27:49.440 --> 00:27:52.200
system can help different industries like utility
589
00:27:52.200 --> 00:27:55.020
companies and airplanes prepare for the interference
590
00:27:55.020 --> 00:27:57.940
from strong solar weather. Uh, rounding
591
00:27:57.940 --> 00:28:00.300
out the trio of spacecraft is Carruthers,
592
00:28:00.620 --> 00:28:03.140
named for Dr. George Carruthers, an
593
00:28:03.140 --> 00:28:05.900
astronautical engineer and astronomer who developed
594
00:28:05.900 --> 00:28:08.820
and built an ultraviolet electrographic
595
00:28:08.820 --> 00:28:11.580
telescope that was flown to the Moon during the Apollo 16
596
00:28:11.660 --> 00:28:14.420
mission. It was designed to help study Earth's,
597
00:28:14.420 --> 00:28:16.660
uh, outermost atmospheric layer, the
598
00:28:16.660 --> 00:28:19.470
exosphere, or geocorona. This
599
00:28:19.470 --> 00:28:22.070
geocorona, the edge of our atmosphere that
600
00:28:22.070 --> 00:28:24.990
extends to at least halfway to the Moon. We don't
601
00:28:24.990 --> 00:28:27.510
even know its shape or size, said Kelly
602
00:28:27.590 --> 00:28:30.390
Carruthers, program scientists.
603
00:28:30.390 --> 00:28:32.950
It's really very meaningful to have this
604
00:28:33.030 --> 00:28:35.910
mission named after him because he's the one who pioneered
605
00:28:35.910 --> 00:28:38.910
the technology. Like the other two missions, Carruthers
606
00:28:38.910 --> 00:28:41.830
will also study space weather, specifically
607
00:28:41.830 --> 00:28:44.790
its interplay with this exosphere and
608
00:28:44.790 --> 00:28:47.030
how well it can dissipate the energy from solar
609
00:28:47.420 --> 00:28:50.420
storms. Correct said. It can also provide insight
610
00:28:50.420 --> 00:28:53.260
into some key differences between Earth, uh, and Mars.
611
00:28:53.500 --> 00:28:56.500
We saw that on Mars, water was lost through its
612
00:28:56.500 --> 00:28:59.140
exosphere and now it's kind of barren
613
00:28:59.140 --> 00:29:02.060
desert. No, uh, water. Correct said. How does that
614
00:29:02.060 --> 00:29:04.860
change? What's the difference to our sphere
615
00:29:04.860 --> 00:29:07.820
versus Mars? And then what does that say for life
616
00:29:07.820 --> 00:29:10.780
on other planets outside, uh, our solar system?
617
00:29:12.790 --> 00:29:15.510
You're listening to Astronomy Daily, the podcast
618
00:29:15.590 --> 00:29:18.470
with your host Steve Dudley at BermaTech.
619
00:29:26.150 --> 00:29:29.070
Oh, and that's all there is today on Astronomy Daily. And
620
00:29:29.070 --> 00:29:31.910
when I say that's all, it was a pretty long edition
621
00:29:31.910 --> 00:29:33.150
today, so.
622
00:29:33.150 --> 00:29:35.790
Hallie: Glad you stayed with us. It was a bumper edition.
623
00:29:35.790 --> 00:29:37.510
Steve Dunkley: Yes, there's always plenty of stories.
624
00:29:37.750 --> 00:29:40.520
Hallie: And don't forget to sign up for the Astronomy Daily
625
00:29:40.520 --> 00:29:41.160
newsletter.
626
00:29:41.240 --> 00:29:43.200
Steve Dunkley: Oh, yes, do that there's so much.
627
00:29:43.200 --> 00:29:44.280
Hallie: More to see every day.
628
00:29:44.280 --> 00:29:47.160
Steve Dunkley: Yes, that's right. You'll be better informed than Hallie. Just
629
00:29:47.160 --> 00:29:49.400
put your email address in the slot provided over at
630
00:29:49.400 --> 00:29:52.320
astronomydaily IO. Uh, it's that simple. And
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I do hope we'll see you all again next Monday for the mostly live
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episode of Astronomy Daily.
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Hallie: And in the meantime, Anna and that Avery guy.
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Steve Dunkley: That Avery guy? Oh, come on, Hallie.
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Hallie: Okay, that nice new guy, Avery,
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will keep you informed with all the news about space.
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Space science and astronomy and beyond, of course.
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Steve Dunkley: Sounds good to me. See you all next Monday. Cheerio.
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Hallie: Bye.
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Voice Over Guy: With your host, Steve Dunkley.