MAVEN’s Final Hour: Mars Orbiter Crisis + Historic ISS Evacuation Update & Lunar Timekeeping


NASA attempts to contact the silent MAVEN Mars orbiter after 40 days—but prospects look grim. Plus: the first-ever ISS medical evacuation succeeds, Europe debuts its powerful Ariane 64, scientists crack asteroid defense secrets, China releases lunar timekeeping software, and Hubble reveals where planets are born. Your daily space news for January 15, 2026.
### Extended Episode Description (for podcast websites/apps)
After more than a month of silence, NASA is making what may be its final attempt to contact the MAVEN Mars orbiter. Mission leaders are pessimistic, but the veteran spacecraft has surprised them before. We break down what happened, what's at stake, and what MAVEN's potential loss means for Mars exploration.
On a brighter note, the SpaceX Crew-11 astronauts have safely returned to Houston following the first-ever medical evacuation from the International Space Station—a historic operation that went flawlessly. We explore how NASA executed this unprecedented mission.
Europe's taking a major step forward with the announcement that the first Ariane 64 rocket will launch February 12th. This four-booster beast can carry more than double the payload of its predecessor, and its debut mission will deploy 32 satellites for Amazon's Kuiper constellation.
Scientists using CERN's particle accelerators have discovered that iron-rich asteroids are tougher than we thought—and they actually get stronger under stress. This surprising finding could reshape how we approach planetary defense.
China has released the world's first practical software for keeping time on the Moon. It sounds like science fiction, but lunar timekeeping is becoming essential as multiple nations prepare for sustained lunar operations.
And after 35 years in orbit, the Hubble Space Telescope is still delivering stunning science, with a new gallery of images showing protoplanetary disks where planets are being born around young stars.
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Kind: captions
Language: en
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Welcome to Astronomy Daily, your source
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for the latest space and astronomy news.
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I'm Anna.
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>> And I'm Avery. It's Saturday, January
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17th, 2026, and we've got an absolutely
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packed episode for you today.
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>> We really do. And we're leading with
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some bittersweet news from Mars. NASA's
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making what might be their final attempt
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to contact the Maven Orbiter, which has
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been silent for over a month now. It's
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looking increasingly unlikely that
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they'll be able to recover the
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spacecraft.
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>> That's tough news, but we've also got
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some incredible human achievements to
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celebrate. The SpaceX Crew 11 astronauts
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have safely returned to Houston
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following the first ever medical
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evacuation from the International Space
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Station. We'll get into the details of
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how that historic operation unfolded.
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>> Europe's stepping up its launch game,
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too. Aron Space has announced they'll be
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launching the first Aron 64 rocket on
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February 12th. That's the more powerful
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four booster version. This is a big deal
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for European space capabilities. We're
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also diving into some fascinating
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research today. Scientists have been
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using CERN's particle accelerators to
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simulate asteroid impacts and what they
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discovered about ironrich space rocks
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could change how we approach planetary
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defense. Then we've got something that
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sounds like science fiction, but is very
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real. China has released the world's
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first practical software for keeping
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time on the moon. Yes, lunar timekeeping
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is now a thing, and it's more important
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than you might think. And we'll wrap up
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with some stunning new images from
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Hubble. Even after 35 years in orbit,
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it's still showing us where planets are
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born in protolanetary discs around young
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stars.
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>> Lots to cover, so let's get started.
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Let's start with that Mars story, Anna.
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NASA's Maven Orbiter has been one of our
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most valuable assets at Mars for over a
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decade. What's the latest on the
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recovery efforts?
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>> Well, it's not looking good, I'm afraid.
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Maven, that's the Mars Atmosphere and
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Volatile Evolution Orbiter, went silent
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on December 6th, 2025, and NASA has been
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unable to reestablish contact ever
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since. The spacecraft has been orbiting
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Mars since 2014, providing invaluable
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data about the Martian atmosphere and
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serving as a critical communications
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relay for the Curiosity and Perseverance
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rovers.
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>> So, what exactly happened? I mean,
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communications blackouts aren't
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completely unusual for Mars missions,
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right?
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>> You're right. They're not. In this case,
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Maven passed behind Mars, which
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temporarily blocks communication. That's
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a routine occurrence, but when it should
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have emerged on the other side, NASA's
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deep space network couldn't regain
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contact. What makes it worse is that
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this happened right before a solar
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conjunction.
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>> That's when the sun sits directly
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between Earth and Mars. Correct.
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>> Exactly. During solar conjunction, which
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occurs roughly every 2 years, solar
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particles interfere with radio signals.
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NASA temporarily halts all
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communications with Mars missions during
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this period to avoid sending corrupted
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commands or receiving incomplete data
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that could damage spacecraft. Though the
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conjunction basically meant NASA had to
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wait before they could even try to
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recover Maven.
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>> And that conjunction period just ended,
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>> right? NASA said they wouldn't have
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contact with any Mars missions until
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Friday, January 16th. So, as of today,
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they're making renewed attempts to
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contact Maven. But here's the concerning
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part. Louise Proctor, the director of
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NASA's planetary science division, said
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on January 13th, and I quote, "We'll
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start looking again, but at this point,
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it's looking very unlikely that we are
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going to be able to recover the
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spacecraft."
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>> That's pretty pessimistic language from
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NASA. Do we know what might have caused
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the initial failure? The leading theory
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is that Maven started rotating
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unexpectedly after passing behind Mars.
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This would have shifted the spacecraft
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out of its planned orbit and potentially
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moved its antenna away from Earth. But
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here's where it gets more complicated.
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Maven has had aging hardware issues for
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years now.
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>> What kind of issues are we talking
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about? The spacecraft has had problems
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with its onboard inertial measurement
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units or IMUs, which are essential for
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orientation in space. Back in 2022,
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Maven spent about 3 months in safe mode
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because of IMU problems. The mission
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team had to rely on backup systems that
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have experienced accelerated wear and
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tear. They even developed an alternative
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all stellar navigation mode that uses
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stars for orientation instead of relying
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on the IMUs.
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>> So, it sounds like Maven has been living
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on borrowed time for a while now.
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>> In some ways, yes. The spacecraft's
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inability to fully recover from those
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2022 outages led to missed observations
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of significant solar flares and
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disrupted its communications relay role.
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That said, Maven still has enough fuel
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to remain in orbit until at least 2030.
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So, the hardware could theoretically
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keep working if they can just
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reestablish contact.
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>> What's the impact going to be if they
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can't recover it? I imagine the rovers
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depend on these orbiters for
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communications.
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>> That's a great point. Maven has been a
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key communications relay for the
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Curiosity and Perseverance rovers. With
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Maven offline, NASA has had to shift
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more of that burden to other orbiters,
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specifically Mars Reconnaissance Orbiter
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and Mars Odyssey. This puts increased
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pressure on those spacecraft to maintain
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communications and support surface
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science activities.
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>> And scientifically, what are we losing?
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>> Maven's scientific contributions have
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been enormous. It's helped us understand
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how Mars lost its once thick atmosphere
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and became the cold, dry world it is
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today. The data it collected on Martian
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weather patterns, dust storms, and
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auroras provided insights into the
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planet's climate system and potential
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habitability. Without Maven, we'd have
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critical gaps in our ongoing atmospheric
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studies of Mars.
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>> So fingers crossed that these new
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contact attempts work out. When will we
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know more? NASA should have results from
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their latest attempts very soon. But
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given the pessimistic tone from their
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leadership, I think we need to prepare
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for the possibility that Maven's
00:06:26.800 --> 00:06:29.430
remarkable decadel long mission may have
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come to an end. It would be a sad
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conclusion to such a successful
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spacecraft, but it's given us more than
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10 years of groundbreaking science.
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>> Absolutely. And that's well beyond its
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original design life, right?
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>> Oh, definitely. Like so many NASA
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missions, it far exceeded expectations.
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Let's hope there's one more surprise
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left in it.
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>> Here's hoping.
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>> Moving from Mars back to closer to home.
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Let's talk about that historic ISS
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medical evacuation. Avery, this was
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really unprecedented.
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>> It absolutely was. The four astronauts
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of SpaceX's Crew 11 mission are now
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safely back in Houston after splashing
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down off the coast of Long Beach,
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California early Thursday morning. This
00:07:13.039 --> 00:07:15.430
marked the very first medical evacuation
00:07:15.440 --> 00:07:17.589
from the International Space Station in
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its more than 25 year history.
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>> Who were the crew members involved?
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>> The crew consisted of NASA astronauts
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Zena Cardman and Mike Fininky, Kima Yui
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from Japan's Aerospace Agency and
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cosminaut Oleg Platinoff from Ross
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Cosmos. They launched back in early
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August for what was supposed to be a
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standard six-month stay aboard the
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station.
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>> So they came home about five weeks
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early. Correct.
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>> That's right. One of the four crew
00:07:44.319 --> 00:07:46.309
members experienced a medical issue in
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orbit last week and NASA made the
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decision to bring the entire crew home
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ahead of schedule. Now, NASA has been
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very protective of medical privacy,
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which is absolutely appropriate. So,
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they haven't disclosed which crew member
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had the issue or what the specific
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medical problem was.
00:08:02.720 --> 00:08:04.390
>> What do we know about how they're doing
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now? According to NASA's latest update
00:08:06.879 --> 00:08:09.189
from Friday afternoon, all four crew
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members are stable and undergoing
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standard post-flight reconditioning and
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evaluations at Johnson Space Center.
00:08:15.840 --> 00:08:17.749
After splashing down, they spent about a
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day and night at a local medical
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facility in California before flying to
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Houston. I have to say, the fact that
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they described them as stable and that
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they're doing standard post-flight
00:08:28.160 --> 00:08:31.189
evaluations suggests this wasn't a dire
00:08:31.199 --> 00:08:32.870
emergency situation.
00:08:32.880 --> 00:08:34.870
>> That's my read on it, too. And NASA
00:08:34.880 --> 00:08:36.709
officials have been pretty clear about
00:08:36.719 --> 00:08:38.469
describing this as a deliberate,
00:08:38.479 --> 00:08:40.949
carefully planned operation rather than
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a panic situation. In fact, one NASA
00:08:43.760 --> 00:08:45.190
representative said, and I'm
00:08:45.200 --> 00:08:47.590
paraphrasing here, this is NASA at its
00:08:47.600 --> 00:08:50.070
finest, referring to how smoothly the
00:08:50.080 --> 00:08:52.230
evacuation and splashdown went.
00:08:52.240 --> 00:08:53.910
>> Can you walk us through what a medical
00:08:53.920 --> 00:08:55.910
evacuation from the ISS actually
00:08:55.920 --> 00:08:59.110
involves? This seems incredibly complex.
00:08:59.120 --> 00:09:01.350
>> It is. First, you have to understand
00:09:01.360 --> 00:09:03.990
that the ISS has medical capabilities on
00:09:04.000 --> 00:09:06.070
board. There's medical equipment,
00:09:06.080 --> 00:09:08.150
supplies, and the crew receives training
00:09:08.160 --> 00:09:10.550
to handle various medical situations.
00:09:10.560 --> 00:09:12.389
They can consult with flight surgeons on
00:09:12.399 --> 00:09:14.870
the ground in real time. But sometimes
00:09:14.880 --> 00:09:17.030
groundbased medical care is simply
00:09:17.040 --> 00:09:18.949
necessary, either for more advanced
00:09:18.959 --> 00:09:21.030
diagnostic equipment or for treatment
00:09:21.040 --> 00:09:23.350
options that aren't available in orbit.
00:09:23.360 --> 00:09:25.190
>> So, the decision to bring someone home
00:09:25.200 --> 00:09:27.030
is never made lightly.
00:09:27.040 --> 00:09:29.509
>> Exactly. In this case, the medical issue
00:09:29.519 --> 00:09:31.509
required evaluation and potential
00:09:31.519 --> 00:09:33.190
treatment that couldn't be done on the
00:09:33.200 --> 00:09:35.509
station. Once that call was made, they
00:09:35.519 --> 00:09:37.110
had to prepare the crew Dragon
00:09:37.120 --> 00:09:39.030
spacecraft, the same one they arrived
00:09:39.040 --> 00:09:41.110
in, named Endeavor, for an early
00:09:41.120 --> 00:09:43.350
departure. This involves checking all
00:09:43.360 --> 00:09:45.590
systems, planning the undocking and
00:09:45.600 --> 00:09:47.829
re-entry trajectory, coordinating with
00:09:47.839 --> 00:09:49.910
recovery teams, and making sure weather
00:09:49.920 --> 00:09:51.190
conditions would be suitable for
00:09:51.200 --> 00:09:52.230
splashdown.
00:09:52.240 --> 00:09:54.550
>> And they successfully executed all of
00:09:54.560 --> 00:09:56.389
that in just a few days.
00:09:56.399 --> 00:09:58.949
>> They did. The crew undocked from the ISS
00:09:58.959 --> 00:10:01.350
on January 14th, completed their
00:10:01.360 --> 00:10:03.750
de-orbit burn, and splashed down safely
00:10:03.760 --> 00:10:06.389
early on January 15th. Recovery teams
00:10:06.399 --> 00:10:08.230
were standing by and quickly retrieved
00:10:08.240 --> 00:10:10.150
the capsule and crew. The whole
00:10:10.160 --> 00:10:12.470
operation went remarkably smoothly.
00:10:12.480 --> 00:10:14.949
>> What about the ISS itself? How is it
00:10:14.959 --> 00:10:16.949
operating with a reduced crew?
00:10:16.959 --> 00:10:18.870
>> That's a great question. Right now, the
00:10:18.880 --> 00:10:20.389
station is operating with what they're
00:10:20.399 --> 00:10:22.710
calling a skeleton crew of just three
00:10:22.720 --> 00:10:25.269
people. NASA astronaut Chris Williams
00:10:25.279 --> 00:10:27.990
and two Ross Cosmos cosminauts Sergey
00:10:28.000 --> 00:10:31.190
Kutz Vertzkov and Sergey Mikayv. That's
00:10:31.200 --> 00:10:33.110
less than half the normal compliment of
00:10:33.120 --> 00:10:34.470
seven crew members.
00:10:34.480 --> 00:10:36.470
>> Can three people effectively run the
00:10:36.480 --> 00:10:37.509
ISS?
00:10:37.519 --> 00:10:39.430
>> They can maintain it and keep critical
00:10:39.440 --> 00:10:41.350
systems running, but it definitely
00:10:41.360 --> 00:10:43.590
limits what science can be done. The
00:10:43.600 --> 00:10:45.190
station won't return to its full
00:10:45.200 --> 00:10:47.990
operational capacity until SpaceX's Crew
00:10:48.000 --> 00:10:49.910
12 mission arrives. That's currently
00:10:49.920 --> 00:10:52.389
scheduled for February 15th. Though NASA
00:10:52.399 --> 00:10:54.230
and SpaceX are looking at whether they
00:10:54.240 --> 00:10:56.230
can move that timeline up a bit,
00:10:56.240 --> 00:10:58.790
>> I imagine this whole situation must have
00:10:58.800 --> 00:11:00.550
been quite stressful for everyone
00:11:00.560 --> 00:11:01.590
involved.
00:11:01.600 --> 00:11:03.910
>> No doubt. But what strikes me is how
00:11:03.920 --> 00:11:05.670
calmly and professionally it was
00:11:05.680 --> 00:11:07.269
handled. In one of the final
00:11:07.279 --> 00:11:09.910
communications before undocking, Crew 11
00:11:09.920 --> 00:11:11.750
commander Mike Finke said it was
00:11:11.760 --> 00:11:13.829
bittersweet to be leaving early. He
00:11:13.839 --> 00:11:16.069
handed over command of the ISS to Chris
00:11:16.079 --> 00:11:18.310
Williams and you could hear in his voice
00:11:18.320 --> 00:11:19.910
that he would have preferred to complete
00:11:19.920 --> 00:11:22.150
the full mission. But he also understood
00:11:22.160 --> 00:11:24.550
the necessity of coming home. It really
00:11:24.560 --> 00:11:26.550
speaks to the incredible planning and
00:11:26.560 --> 00:11:28.389
preparation that goes into human space
00:11:28.399 --> 00:11:31.110
flight. Even in an offnominal situation
00:11:31.120 --> 00:11:33.509
like this, the systems and procedures
00:11:33.519 --> 00:11:35.590
worked exactly as designed.
00:11:35.600 --> 00:11:37.350
>> And I think it's worth noting that this
00:11:37.360 --> 00:11:39.590
won't affect other upcoming missions.
00:11:39.600 --> 00:11:41.829
NASA administrator Jared Isaacman
00:11:41.839 --> 00:11:43.829
specifically stated that this ISS
00:11:43.839 --> 00:11:45.910
evacuation shouldn't interfere with the
00:11:45.920 --> 00:11:48.150
upcoming Artemis 2 moon mission, which
00:11:48.160 --> 00:11:49.990
is still on track for a possible launch
00:11:50.000 --> 00:11:52.630
as early as February 6th. That's good to
00:11:52.640 --> 00:11:55.269
hear. Well, here's hoping for a full
00:11:55.279 --> 00:11:57.110
recovery for whichever crew member
00:11:57.120 --> 00:11:59.590
needed the medical attention. And kudos
00:11:59.600 --> 00:12:02.230
to everyone involved in executing such a
00:12:02.240 --> 00:12:05.030
complex operation so flawlessly.
00:12:05.040 --> 00:12:07.590
>> Agreed. It really was NASA at its
00:12:07.600 --> 00:12:10.629
finest. Switching gears now to European
00:12:10.639 --> 00:12:13.430
space flight. Avery, Europe is about to
00:12:13.440 --> 00:12:15.990
debut a significantly more powerful
00:12:16.000 --> 00:12:18.069
version of its new rocket. Right.
00:12:18.079 --> 00:12:20.150
>> That's right, Anna. Aryan Space has
00:12:20.160 --> 00:12:21.829
announced that the first flight of the
00:12:21.839 --> 00:12:24.790
Aryan 64 will launch on February 12th
00:12:24.800 --> 00:12:26.710
from the Gana Space Center in French
00:12:26.720 --> 00:12:28.790
Gana. This is the four booster
00:12:28.800 --> 00:12:31.030
configuration of the Aryan 6 and it
00:12:31.040 --> 00:12:33.350
represents a major step up in capability
00:12:33.360 --> 00:12:35.910
for European launch services. Let's back
00:12:35.920 --> 00:12:38.230
up a second for anyone who might not be
00:12:38.240 --> 00:12:40.710
familiar with the Aryan 6. Can you give
00:12:40.720 --> 00:12:41.990
us the background?
00:12:42.000 --> 00:12:44.710
>> Sure. The Aryan 6 is Europe's newest
00:12:44.720 --> 00:12:46.629
heavy lift rocket designed to replace
00:12:46.639 --> 00:12:48.870
the Aryan 5 which served for nearly
00:12:48.880 --> 00:12:51.190
three decades. The inaugural flight was
00:12:51.200 --> 00:12:54.949
back in July 2024. And throughout 2025,
00:12:54.959 --> 00:12:57.670
Aryan Space flew four more missions, all
00:12:57.680 --> 00:12:59.910
carrying payloads for organizations like
00:12:59.920 --> 00:13:03.430
ESA, UMTASAT, and CENS, the French Space
00:13:03.440 --> 00:13:06.150
Agency. And all of those flights used
00:13:06.160 --> 00:13:09.190
the Arion 62 configuration.
00:13:09.200 --> 00:13:13.430
>> Exactly. The Arion 62 uses two P120C
00:13:13.440 --> 00:13:15.670
solid fuel boosters strapped to the side
00:13:15.680 --> 00:13:17.750
of the rocket's core stage. Each of
00:13:17.760 --> 00:13:20.310
those boosters produces roughly 4500
00:13:20.320 --> 00:13:22.790
kons of thrust. It's been doing great
00:13:22.800 --> 00:13:24.870
for medium lift missions with a capacity
00:13:24.880 --> 00:13:27.670
to deliver about 10.3 tons to low Earth
00:13:27.680 --> 00:13:28.470
orbit.
00:13:28.480 --> 00:13:31.590
>> So the Aryan 64 just adds two more
00:13:31.600 --> 00:13:32.629
boosters,
00:13:32.639 --> 00:13:35.509
>> right? It uses four of those P120C
00:13:35.519 --> 00:13:37.430
boosters instead of two. And that makes
00:13:37.440 --> 00:13:39.990
a dramatic difference in capability. The
00:13:40.000 --> 00:13:44.150
Arion 64 can deliver up to 21.6 tons to
00:13:44.160 --> 00:13:46.150
low Earth orbit, more than double what
00:13:46.160 --> 00:13:49.190
the Arion 62 can handle. That puts it in
00:13:49.200 --> 00:13:51.110
the heavy lift category, competing with
00:13:51.120 --> 00:13:53.670
rockets like SpaceX's Falcon Heavy.
00:13:53.680 --> 00:13:55.910
>> That's a significant jump. What's
00:13:55.920 --> 00:13:57.910
driving the need for this more powerful
00:13:57.920 --> 00:13:58.790
version?
00:13:58.800 --> 00:14:00.629
>> Well, this first mission actually gives
00:14:00.639 --> 00:14:03.590
us a perfect example. The Arion 64's
00:14:03.600 --> 00:14:05.030
first flight will be launching
00:14:05.040 --> 00:14:07.350
satellites for Amazon's project Cooper
00:14:07.360 --> 00:14:09.910
broadband internet constellation. Arion
00:14:09.920 --> 00:14:11.990
space has an 18 flight contract with
00:14:12.000 --> 00:14:13.910
Amazon. And this first mission
00:14:13.920 --> 00:14:17.430
designated LE01, which stands for LEO
00:14:17.440 --> 00:14:20.470
Europe01, will deploy 32 Cooper
00:14:20.480 --> 00:14:21.430
satellites.
00:14:21.440 --> 00:14:23.750
>> Amazon's competing with Space X's
00:14:23.760 --> 00:14:25.030
Starlink. Right.
00:14:25.040 --> 00:14:27.910
>> That's right. Amazon already has about
00:14:27.920 --> 00:14:29.829
180 satellites in orbit and they're
00:14:29.839 --> 00:14:32.150
rapidly building out the constellation.
00:14:32.160 --> 00:14:34.470
Having access to the more powerful Arion
00:14:34.480 --> 00:14:36.870
64 means they can launch more satellites
00:14:36.880 --> 00:14:39.110
at once which speeds up the deployment
00:14:39.120 --> 00:14:41.110
schedule and reduces the total number of
00:14:41.120 --> 00:14:42.310
launches needed.
00:14:42.320 --> 00:14:44.230
>> Is there anything else notable about
00:14:44.240 --> 00:14:45.910
this particular flight?
00:14:45.920 --> 00:14:47.910
>> Yes, actually this will be the first
00:14:47.920 --> 00:14:50.230
Arion 6 mission to use the rocket's
00:14:50.240 --> 00:14:53.269
larger 20 m long fairing. All previous
00:14:53.279 --> 00:14:56.150
flights used a shorter 14 meter fairing.
00:14:56.160 --> 00:14:58.230
The longer fairing provides more volume
00:14:58.240 --> 00:15:01.030
for larger payloads or in this case for
00:15:01.040 --> 00:15:02.949
fitting more satellites into the payload
00:15:02.959 --> 00:15:03.750
stack.
00:15:03.760 --> 00:15:05.829
>> How long will the mission last?
00:15:05.839 --> 00:15:07.750
>> Arion space hasn't published the
00:15:07.760 --> 00:15:09.350
complete mission breakdown yet, but
00:15:09.360 --> 00:15:11.269
they've stated the entire flight will
00:15:11.279 --> 00:15:13.829
last 1 hour and 54 minutes. That
00:15:13.839 --> 00:15:16.389
presumably includes deploying all 32
00:15:16.399 --> 00:15:18.310
satellites and then deorbiting the
00:15:18.320 --> 00:15:20.150
rocket's upper stage in a controlled
00:15:20.160 --> 00:15:21.990
manner, which is important for reducing
00:15:22.000 --> 00:15:24.069
space debris. What does this mean for
00:15:24.079 --> 00:15:26.230
Aryan Space's launch cadence going
00:15:26.240 --> 00:15:27.269
forward?
00:15:27.279 --> 00:15:29.670
>> They're being pretty ambitious. Arion
00:15:29.680 --> 00:15:31.590
space is aiming to double the number of
00:15:31.600 --> 00:15:34.150
Arion 6 launches this year compared to
00:15:34.160 --> 00:15:36.949
2025. That would mean as many as eight
00:15:36.959 --> 00:15:39.990
Arion 6 flights over the next 12 months.
00:15:40.000 --> 00:15:41.509
Given that they're still ramping up
00:15:41.519 --> 00:15:43.750
operations with what is still a fairly
00:15:43.760 --> 00:15:46.069
new rocket, that's a challenging goal,
00:15:46.079 --> 00:15:47.750
but it shows their confidence.
00:15:47.760 --> 00:15:49.430
>> Are there any other upgrades in the
00:15:49.440 --> 00:15:50.310
works?
00:15:50.320 --> 00:15:52.949
>> Actually, yes. The company is developing
00:15:52.959 --> 00:15:55.189
an upgraded version of the solid fuel
00:15:55.199 --> 00:15:58.069
booster called the P160C.
00:15:58.079 --> 00:16:00.550
It carries an additional 14 tons of
00:16:00.560 --> 00:16:02.870
solid propellant compared to the current
00:16:02.880 --> 00:16:04.550
P120C.
00:16:04.560 --> 00:16:06.310
That upgrade has already been fully
00:16:06.320 --> 00:16:09.030
qualified for use on both the Aryan 62
00:16:09.040 --> 00:16:11.910
for medium lift missions, the Aryan 64
00:16:11.920 --> 00:16:14.550
for heavy lift, the Vega C for smaller
00:16:14.560 --> 00:16:16.790
payloads, and these future upgrades.
00:16:16.800 --> 00:16:18.949
Europe is positioning itself to be very
00:16:18.959 --> 00:16:20.550
competitive in the commercial launch
00:16:20.560 --> 00:16:22.949
market. And that's crucial, especially
00:16:22.959 --> 00:16:25.110
as we see increasing competition from
00:16:25.120 --> 00:16:27.749
SpaceX, China, and other emerging launch
00:16:27.759 --> 00:16:28.629
providers.
00:16:28.639 --> 00:16:30.790
>> Will the February 12th launch be
00:16:30.800 --> 00:16:33.350
publicly viewable? Aryan Space typically
00:16:33.360 --> 00:16:34.870
provides live coverage of their
00:16:34.880 --> 00:16:36.870
launches, so I'd expect we'll be able to
00:16:36.880 --> 00:16:38.870
watch this historic first flight of the
00:16:38.880 --> 00:16:41.829
Aryan 64. It should be quite a sight.
00:16:41.839 --> 00:16:43.829
Those four boosters firing together
00:16:43.839 --> 00:16:45.990
should make for an impressive liftoff.
00:16:46.000 --> 00:16:48.150
>> I'll definitely be watching. It's great
00:16:48.160 --> 00:16:50.470
to see Europe maintaining and expanding
00:16:50.480 --> 00:16:52.710
its independent access to space.
00:16:52.720 --> 00:16:54.629
>> Anna, let's talk about planetary
00:16:54.639 --> 00:16:56.710
defense. Scientists have been conducting
00:16:56.720 --> 00:16:58.710
some fascinating experiments using
00:16:58.720 --> 00:17:00.949
particle accelerators to understand how
00:17:00.959 --> 00:17:03.110
asteroids might respond to deflection
00:17:03.120 --> 00:17:05.189
attempts. This is really cool work,
00:17:05.199 --> 00:17:07.590
Avery. An international research team
00:17:07.600 --> 00:17:10.230
used CERN's high radiation to materials
00:17:10.240 --> 00:17:13.510
facility, that's Hyradmat, to simulate
00:17:13.520 --> 00:17:15.909
what happens when high energy impacts
00:17:15.919 --> 00:17:18.549
strike ironrich asteroids. And what they
00:17:18.559 --> 00:17:20.549
found could significantly change our
00:17:20.559 --> 00:17:23.189
approach to planetary defense. Before we
00:17:23.199 --> 00:17:25.110
get into the results, can you set up the
00:17:25.120 --> 00:17:27.750
context, why is this research important?
00:17:27.760 --> 00:17:31.110
>> Sure. We know there are around 37,000
00:17:31.120 --> 00:17:34.789
known near Earth asteroids and 120 short
00:17:34.799 --> 00:17:36.950
period comets whose orbits bring them
00:17:36.960 --> 00:17:39.350
close to Earth. While scientists are
00:17:39.360 --> 00:17:41.110
confident that none of the known
00:17:41.120 --> 00:17:43.270
potentially hazardous objects will
00:17:43.280 --> 00:17:45.669
strike Earth within the next century, we
00:17:45.679 --> 00:17:47.750
know that eventually planetary defense
00:17:47.760 --> 00:17:50.390
measures will be needed. And NASA's Dart
00:17:50.400 --> 00:17:52.390
mission demonstrated one approach, the
00:17:52.400 --> 00:17:53.909
kinetic impactor.
00:17:53.919 --> 00:17:57.190
>> Exactly. In 2022, Dart successfully
00:17:57.200 --> 00:17:59.350
struck the asteroid Demorphus and
00:17:59.360 --> 00:18:01.350
altered its orbit. But to do this
00:18:01.360 --> 00:18:03.750
reliably and develop effective defense
00:18:03.760 --> 00:18:05.909
strategies, we need to understand how
00:18:05.919 --> 00:18:07.990
different types of asteroids respond to
00:18:08.000 --> 00:18:10.230
impacts. That's where this new research
00:18:10.240 --> 00:18:11.110
comes in.
00:18:11.120 --> 00:18:13.510
>> So, they focus specifically on ironrich
00:18:13.520 --> 00:18:14.549
asteroids,
00:18:14.559 --> 00:18:17.029
>> right? What astronomers call Mtype
00:18:17.039 --> 00:18:18.950
asteroids. These are thought to be
00:18:18.960 --> 00:18:21.350
exposed metallic cores of ancient
00:18:21.360 --> 00:18:23.510
protolanets that were shattered in
00:18:23.520 --> 00:18:25.430
collisions billions of years ago.
00:18:25.440 --> 00:18:27.350
They're made primarily of iron and
00:18:27.360 --> 00:18:29.830
nickel, unlike the more common rocky
00:18:29.840 --> 00:18:32.070
asteroids or icy comets.
00:18:32.080 --> 00:18:34.310
>> How did they simulate an asteroid impact
00:18:34.320 --> 00:18:35.430
in a lab?
00:18:35.440 --> 00:18:37.350
>> This is where it gets really clever.
00:18:37.360 --> 00:18:39.990
They used a sample of the Campo Delio
00:18:40.000 --> 00:18:42.310
iron meteorite, which is a wellstied
00:18:42.320 --> 00:18:44.549
iron meteorite from Argentina. They
00:18:44.559 --> 00:18:47.909
subjected it to extremely energetic 440
00:18:47.919 --> 00:18:51.430
GEV proton beams at CERN's highradmat
00:18:51.440 --> 00:18:53.750
facility at CERN. That's an incredibly
00:18:53.760 --> 00:18:55.110
high energy level.
00:18:55.120 --> 00:18:56.870
>> And how did they measure what happened
00:18:56.880 --> 00:18:57.990
to the sample?
00:18:58.000 --> 00:18:59.990
>> They used a technique called Doppler
00:19:00.000 --> 00:19:02.390
vibrometry, which can detect tiny
00:19:02.400 --> 00:19:04.710
surface vibrations. This allowed them to
00:19:04.720 --> 00:19:06.870
capture realtime data on how the
00:19:06.880 --> 00:19:09.270
material responded to rapidly increasing
00:19:09.280 --> 00:19:11.590
stress, all without destroying the
00:19:11.600 --> 00:19:13.990
sample. They could see exactly how iron
00:19:14.000 --> 00:19:16.310
behaved under extreme conditions.
00:19:16.320 --> 00:19:17.669
>> What did they discover?
00:19:17.679 --> 00:19:19.029
>> This is where it gets really
00:19:19.039 --> 00:19:21.029
interesting. The results showed that
00:19:21.039 --> 00:19:23.750
Mtype asteroids can absorb significantly
00:19:23.760 --> 00:19:26.150
more energy without fragmenting than
00:19:26.160 --> 00:19:28.470
conventional models predicted. But even
00:19:28.480 --> 00:19:30.310
more surprisingly, the meteorite
00:19:30.320 --> 00:19:32.470
actually got tougher as it was subjected
00:19:32.480 --> 00:19:34.230
to increasing stress.
00:19:34.240 --> 00:19:37.110
>> Wait, it got stronger under stress?
00:19:37.120 --> 00:19:39.909
>> Yes. The researchers found that the iron
00:19:39.919 --> 00:19:42.310
dissipated more energy as stress
00:19:42.320 --> 00:19:44.950
increased, suggesting that the internal
00:19:44.960 --> 00:19:47.510
structure of asteroids can redistribute
00:19:47.520 --> 00:19:50.549
and amplify stress in unexpected ways,
00:19:50.559 --> 00:19:52.630
similar to what we see in complex
00:19:52.640 --> 00:19:54.470
composite materials.
00:19:54.480 --> 00:19:56.870
>> That seems counterintuitive. You'd
00:19:56.880 --> 00:19:59.190
expect materials to weaken under extreme
00:19:59.200 --> 00:20:01.190
stress, not strengthen.
00:20:01.200 --> 00:20:03.350
>> That's exactly why this is such an
00:20:03.360 --> 00:20:05.590
important finding. It contradicts what
00:20:05.600 --> 00:20:07.990
conventional models have suggested. One
00:20:08.000 --> 00:20:09.909
of the study's co-authors, Professor
00:20:09.919 --> 00:20:12.230
Gian Luca Gregori from the University of
00:20:12.240 --> 00:20:14.789
Oxford said this is the first time
00:20:14.799 --> 00:20:16.870
they've been able to observe in real
00:20:16.880 --> 00:20:19.430
time how an actual meteorite sample
00:20:19.440 --> 00:20:22.230
deforms, strengthens, and adapts under
00:20:22.240 --> 00:20:24.630
extreme conditions without destroying
00:20:24.640 --> 00:20:25.270
it.
00:20:25.280 --> 00:20:27.110
>> So, what does this mean for planetary
00:20:27.120 --> 00:20:28.470
defense strategies?
00:20:28.480 --> 00:20:30.789
>> A couple of things. First, it means that
00:20:30.799 --> 00:20:33.270
ironrich asteroids might be harder to
00:20:33.280 --> 00:20:35.350
deflect than we thought because they can
00:20:35.360 --> 00:20:37.270
absorb more energy without breaking
00:20:37.280 --> 00:20:39.909
apart. But it also suggests that we
00:20:39.919 --> 00:20:42.149
could potentially deliver energy deep
00:20:42.159 --> 00:20:44.710
inside an asteroid without fragmenting
00:20:44.720 --> 00:20:45.350
it.
00:20:45.360 --> 00:20:47.110
>> That could be useful if you want to push
00:20:47.120 --> 00:20:49.430
an asteroid rather than shatter it.
00:20:49.440 --> 00:20:52.149
>> Exactly. The research also helps explain
00:20:52.159 --> 00:20:54.390
a long-standing puzzle in planetary
00:20:54.400 --> 00:20:57.110
defense. Why there's often a discrepancy
00:20:57.120 --> 00:20:59.350
between what we infer from meteorite
00:20:59.360 --> 00:21:02.149
breakup in Earth's atmosphere and actual
00:21:02.159 --> 00:21:04.149
laboratory measurements of meteorite
00:21:04.159 --> 00:21:06.950
strength. This study shows that internal
00:21:06.960 --> 00:21:09.029
stress redistribution within the
00:21:09.039 --> 00:21:11.430
heterogeneous structure of meteorites
00:21:11.440 --> 00:21:13.510
can explain that difference.
00:21:13.520 --> 00:21:15.029
>> This sounds like it could inform new
00:21:15.039 --> 00:21:16.549
deflection methods.
00:21:16.559 --> 00:21:18.549
>> That's the hope. The data could help
00:21:18.559 --> 00:21:20.950
develop redirection techniques that push
00:21:20.960 --> 00:21:23.510
asteroids more effectively while keeping
00:21:23.520 --> 00:21:25.990
them intact. After all, the last thing
00:21:26.000 --> 00:21:28.149
you want when deflecting an asteroid is
00:21:28.159 --> 00:21:30.390
to break it into multiple pieces that
00:21:30.400 --> 00:21:32.230
might still pose a threat.
00:21:32.240 --> 00:21:33.750
>> Have they tested this with other types
00:21:33.760 --> 00:21:35.430
of asteroid materials?
00:21:35.440 --> 00:21:37.590
>> This particular study focused on iron
00:21:37.600 --> 00:21:39.990
meteorites, but the methodology could be
00:21:40.000 --> 00:21:42.230
applied to other types of asteroids,
00:21:42.240 --> 00:21:44.789
rocky asteroids, carbonacious asteroids,
00:21:44.799 --> 00:21:47.510
and so on. Each type would likely behave
00:21:47.520 --> 00:21:49.909
differently under extreme stress. And
00:21:49.919 --> 00:21:51.830
understanding those differences is
00:21:51.840 --> 00:21:54.070
crucial for developing a comprehensive
00:21:54.080 --> 00:21:55.990
planetary defense toolkit.
00:21:56.000 --> 00:21:57.750
>> I think what's particularly valuable
00:21:57.760 --> 00:21:59.190
here is that they've developed a
00:21:59.200 --> 00:22:01.590
technique that can test actual meteorite
00:22:01.600 --> 00:22:04.390
samples non-destructively. That means we
00:22:04.400 --> 00:22:06.549
can build up a library of data on how
00:22:06.559 --> 00:22:08.710
different asteroid materials behave
00:22:08.720 --> 00:22:10.549
without having to rely solely on
00:22:10.559 --> 00:22:13.029
computer simulations or destroying
00:22:13.039 --> 00:22:15.830
precious samples. And as we continue to
00:22:15.840 --> 00:22:17.590
study asteroids with missions like
00:22:17.600 --> 00:22:20.870
Osiris X and Hayabusa 2, we'll have more
00:22:20.880 --> 00:22:22.390
samples to test.
00:22:22.400 --> 00:22:24.470
>> Exactly. The combination of sample
00:22:24.480 --> 00:22:26.710
return missions, laboratory testing like
00:22:26.720 --> 00:22:28.789
this, and missions like DART that
00:22:28.799 --> 00:22:30.470
demonstrate actual deflection
00:22:30.480 --> 00:22:32.789
techniques, it's all building toward a
00:22:32.799 --> 00:22:34.710
real capability to protect Earth from
00:22:34.720 --> 00:22:37.190
asteroid impacts. It's reassuring to
00:22:37.200 --> 00:22:39.270
know that even though we don't face an
00:22:39.280 --> 00:22:41.190
immediate threat, we're doing the
00:22:41.200 --> 00:22:43.029
groundwork now, so we'll be prepared
00:22:43.039 --> 00:22:44.390
when we need to be.
00:22:44.400 --> 00:22:46.549
>> Absolutely. And this research was just
00:22:46.559 --> 00:22:48.870
published in Nature Communications, so
00:22:48.880 --> 00:22:50.549
it's getting a lot of attention from the
00:22:50.559 --> 00:22:52.230
planetary defense community.
00:22:52.240 --> 00:22:54.230
>> Avery, our next story sounds like
00:22:54.240 --> 00:22:56.470
something out of science fiction, but
00:22:56.480 --> 00:22:59.029
it's very much real and increasingly
00:22:59.039 --> 00:23:01.510
necessary. China has released the
00:23:01.520 --> 00:23:03.830
world's first practical software for
00:23:03.840 --> 00:23:05.750
keeping time on the moon.
00:23:05.760 --> 00:23:08.630
>> Lunar timekeeping software. When you say
00:23:08.640 --> 00:23:10.789
it out loud, it really drives home how
00:23:10.799 --> 00:23:13.430
much space exploration has advanced. Why
00:23:13.440 --> 00:23:15.350
do we need to keep time differently on
00:23:15.360 --> 00:23:16.070
the moon?
00:23:16.080 --> 00:23:18.310
>> It all comes down to Einstein's theory
00:23:18.320 --> 00:23:21.110
of general relativity. Time doesn't pass
00:23:21.120 --> 00:23:23.110
at the same rate everywhere. It's
00:23:23.120 --> 00:23:26.149
affected by both gravity and velocity.
00:23:26.159 --> 00:23:27.990
The moon's gravity is weaker than
00:23:28.000 --> 00:23:30.070
Earth's, which means time actually
00:23:30.080 --> 00:23:32.390
passes slightly faster on the moon than
00:23:32.400 --> 00:23:33.830
it does on Earth.
00:23:33.840 --> 00:23:35.990
>> How much faster are we talking about?
00:23:36.000 --> 00:23:39.990
>> About 56 millionth of a second per day.
00:23:40.000 --> 00:23:42.070
Now, that might not sound like much, but
00:23:42.080 --> 00:23:44.310
it adds up over time, and it can
00:23:44.320 --> 00:23:47.029
seriously disrupt navigation systems,
00:23:47.039 --> 00:23:48.789
especially when you're trying to do
00:23:48.799 --> 00:23:51.190
precision work on the lunar surface.
00:23:51.200 --> 00:23:53.029
>> So, this is a precision navigation
00:23:53.039 --> 00:23:53.830
issue.
00:23:53.840 --> 00:23:56.870
>> Exactly. Think about GPS on Earth. The
00:23:56.880 --> 00:23:59.029
satellites constantly have to correct
00:23:59.039 --> 00:24:01.190
for relativistic effects caused by
00:24:01.200 --> 00:24:03.830
gravity and motion. Those corrections
00:24:03.840 --> 00:24:05.990
are what allow your phone to pinpoint
00:24:06.000 --> 00:24:08.630
your location within just a few meters.
00:24:08.640 --> 00:24:11.269
Without accounting for relativity, GPS
00:24:11.279 --> 00:24:13.350
would be useless within minutes.
00:24:13.360 --> 00:24:15.110
>> And the moon is about to have a similar
00:24:15.120 --> 00:24:16.870
need for precision navigation.
00:24:16.880 --> 00:24:19.350
>> Right? In the past, this wasn't really a
00:24:19.360 --> 00:24:21.110
problem because lunar missions were
00:24:21.120 --> 00:24:23.990
rare, short, and mostly isolated.
00:24:24.000 --> 00:24:26.310
Engineers could just use Earth time and
00:24:26.320 --> 00:24:28.310
apply mission specific fixes when
00:24:28.320 --> 00:24:31.029
needed. But that's changing rapidly
00:24:31.039 --> 00:24:32.789
>> because we're about to have multiple
00:24:32.799 --> 00:24:34.630
spacecraft and eventually humans
00:24:34.640 --> 00:24:36.870
operating on the moon simultaneously.
00:24:36.880 --> 00:24:39.590
>> Exactly. Under those conditions, relying
00:24:39.600 --> 00:24:42.149
on custom fixes for each mission becomes
00:24:42.159 --> 00:24:44.870
risky and inefficient. You need a
00:24:44.880 --> 00:24:47.269
standardized lunar time reference that
00:24:47.279 --> 00:24:48.870
everyone can use.
00:24:48.880 --> 00:24:50.789
>> So what exactly did the Chinese team
00:24:50.799 --> 00:24:51.510
create?
00:24:51.520 --> 00:24:53.190
>> Researchers from the Purple Mountain
00:24:53.200 --> 00:24:55.510
Observatory in Nanjing developed
00:24:55.520 --> 00:24:59.430
detailed software called LTE440.
00:24:59.440 --> 00:25:02.230
That stands for lunar time ephemeris.
00:25:02.240 --> 00:25:04.630
It's based on modern planetary data and
00:25:04.640 --> 00:25:07.190
tracks how lunar time drifts relative to
00:25:07.200 --> 00:25:09.590
Earth time. The software automates
00:25:09.600 --> 00:25:11.990
calculations that once required deep
00:25:12.000 --> 00:25:14.549
expertise in relativity and celestial
00:25:14.559 --> 00:25:15.750
mechanics.
00:25:15.760 --> 00:25:17.190
>> How accurate is it?
00:25:17.200 --> 00:25:19.510
>> Remarkably accurate. The researchers
00:25:19.520 --> 00:25:21.350
found their method stays accurate to
00:25:21.360 --> 00:25:24.310
within a few tens of nanconds even when
00:25:24.320 --> 00:25:26.950
projected over a thousand years. And to
00:25:26.960 --> 00:25:29.190
keep daily differences within about 10
00:25:29.200 --> 00:25:31.750
nanconds, the calculations need to be
00:25:31.760 --> 00:25:34.870
accurate to parts in 10 trillion. Their
00:25:34.880 --> 00:25:39.029
tests show LTE 440 meets that standard.
00:25:39.039 --> 00:25:41.190
>> Why such extreme precision?
00:25:41.200 --> 00:25:43.269
>> Well, navigation is one driver, but
00:25:43.279 --> 00:25:45.590
there's also science. The moon offers
00:25:45.600 --> 00:25:47.830
unique conditions for astronomy. No
00:25:47.840 --> 00:25:50.470
atmosphere, minimal interference. One
00:25:50.480 --> 00:25:53.430
promising idea is Earth Moon very long
00:25:53.440 --> 00:25:56.149
baseline interpherometry where you link
00:25:56.159 --> 00:25:58.549
radio telescopes on Earth and the moon
00:25:58.559 --> 00:26:00.710
to create sharper images of distant
00:26:00.720 --> 00:26:03.350
objects. And that requires extremely
00:26:03.360 --> 00:26:04.549
precise timing.
00:26:04.559 --> 00:26:07.110
>> Right? Signals recorded on both bodies
00:26:07.120 --> 00:26:09.110
need to be timestamped to better than a
00:26:09.120 --> 00:26:11.350
microscond. To allow for instrument
00:26:11.360 --> 00:26:13.750
noise, the underlying time model needs
00:26:13.760 --> 00:26:16.230
to be even more accurate. Hence the
00:26:16.240 --> 00:26:18.549
extreme precision requirements.
00:26:18.559 --> 00:26:20.950
>> How does the software actually work?
00:26:20.960 --> 00:26:23.430
Instead of using long equations, they
00:26:23.440 --> 00:26:25.590
used a numerical approach based on a
00:26:25.600 --> 00:26:28.710
planetary model called DE440,
00:26:28.720 --> 00:26:30.310
which tracks the positions and
00:26:30.320 --> 00:26:32.549
velocities of solar system bodies with
00:26:32.559 --> 00:26:35.110
high precision. From that data, they
00:26:35.120 --> 00:26:37.510
computed how time near the moon differs
00:26:37.520 --> 00:26:40.070
from a solar system reference time. The
00:26:40.080 --> 00:26:42.390
software stores these results in compact
00:26:42.400 --> 00:26:45.190
files that can be quickly interpolated.
00:26:45.200 --> 00:26:48.230
>> What affects lunar time most? The moon's
00:26:48.240 --> 00:26:50.470
motion and the sun's gravity dominate
00:26:50.480 --> 00:26:53.510
the effect, but Earth, Jupiter, and even
00:26:53.520 --> 00:26:55.990
distant objects in the Kyper belt add
00:26:56.000 --> 00:26:58.390
smaller effects. There are monthly and
00:26:58.400 --> 00:27:00.070
yearly patterns that range from
00:27:00.080 --> 00:27:02.710
milliseconds down to micros secondsonds.
00:27:02.720 --> 00:27:04.310
>> I'm curious about the international
00:27:04.320 --> 00:27:06.630
response to this. Is China the only one
00:27:06.640 --> 00:27:07.830
working on this?
00:27:07.840 --> 00:27:10.470
>> That's a great question. Jonathan McDow,
00:27:10.480 --> 00:27:12.710
an astronomer at Harvard, told reporters
00:27:12.720 --> 00:27:14.870
that similar efforts are underway in the
00:27:14.880 --> 00:27:17.029
United States, but he's not aware of
00:27:17.039 --> 00:27:19.590
another openly available tool like this.
00:27:19.600 --> 00:27:22.149
He emphasized that this shows China is
00:27:22.159 --> 00:27:24.470
serious about lunar exploration and is
00:27:24.480 --> 00:27:26.630
being quite open about sharing its lunar
00:27:26.640 --> 00:27:27.990
related research.
00:27:28.000 --> 00:27:29.590
>> That's actually encouraging from an
00:27:29.600 --> 00:27:31.590
international cooperation standpoint.
00:27:31.600 --> 00:27:33.830
>> I think so, too. And it's worth noting
00:27:33.840 --> 00:27:36.230
that in 2024, the International
00:27:36.240 --> 00:27:38.950
Astronomical Union adopted a framework
00:27:38.960 --> 00:27:40.789
calling for the moon to have its own
00:27:40.799 --> 00:27:43.350
time reference. So this software really
00:27:43.360 --> 00:27:46.070
builds on that international consensus.
00:27:46.080 --> 00:27:48.149
>> What are the practical implications for
00:27:48.159 --> 00:27:49.590
upcoming missions
00:27:49.600 --> 00:27:52.789
>> as lunar activity increases and we're
00:27:52.799 --> 00:27:55.510
talking about NASA's Aremis program,
00:27:55.520 --> 00:27:58.549
China's own lunar base plans, commercial
00:27:58.559 --> 00:28:01.430
lunar landers, and more. Reliable
00:28:01.440 --> 00:28:04.549
timekeeping will support safer landings,
00:28:04.559 --> 00:28:06.630
smoother navigation, and better
00:28:06.640 --> 00:28:08.870
coordination between missions.
00:28:08.880 --> 00:28:12.070
Eventually, we'll likely see lunar GPS
00:28:12.080 --> 00:28:14.789
style systems that depend on this kind
00:28:14.799 --> 00:28:16.870
of precise timekeeping.
00:28:16.880 --> 00:28:18.549
>> It really is laying the groundwork for
00:28:18.559 --> 00:28:21.029
sustained human presence on the moon.
00:28:21.039 --> 00:28:23.269
>> Absolutely. And the researchers
00:28:23.279 --> 00:28:25.909
emphasize that LTE440
00:28:25.919 --> 00:28:28.789
is just an early step. Future versions
00:28:28.799 --> 00:28:30.789
will need to support real time
00:28:30.799 --> 00:28:34.149
navigation and networks of lunar clocks.
00:28:34.159 --> 00:28:36.389
But the release marks a shift from
00:28:36.399 --> 00:28:38.549
abstract planning to practical
00:28:38.559 --> 00:28:39.669
infrastructure.
00:28:39.679 --> 00:28:41.190
>> It's one of those things that sounds
00:28:41.200 --> 00:28:43.669
mundane time software, but is actually
00:28:43.679 --> 00:28:45.909
fundamental to making lunar operations
00:28:45.919 --> 00:28:46.710
work.
00:28:46.720 --> 00:28:49.110
>> Exactly. You can have the fanciest
00:28:49.120 --> 00:28:51.510
rockets and landers in the world, but if
00:28:51.520 --> 00:28:53.909
your spacecraft can't agree on what time
00:28:53.919 --> 00:28:56.310
it is, you're going to have problems.
00:28:56.320 --> 00:28:59.029
This is the kind of unsexy but essential
00:28:59.039 --> 00:29:01.029
infrastructure work that makes the
00:29:01.039 --> 00:29:02.710
exciting stuff possible.
00:29:02.720 --> 00:29:04.789
>> For our final story today, let's talk
00:29:04.799 --> 00:29:06.870
about the Hubble Space Telescope. After
00:29:06.880 --> 00:29:09.190
35 years in orbit, it's still delivering
00:29:09.200 --> 00:29:10.710
incredible science.
00:29:10.720 --> 00:29:13.430
>> It really is remarkable. NASA just
00:29:13.440 --> 00:29:16.149
released a new gallery of Hubble images
00:29:16.159 --> 00:29:19.110
showing protolanetary discs around young
00:29:19.120 --> 00:29:21.830
stars, essentially the birthplaces of
00:29:21.840 --> 00:29:24.710
planets. And these images beautifully
00:29:24.720 --> 00:29:26.710
illustrate one of Hubble's original
00:29:26.720 --> 00:29:29.430
mission goals, understanding how planets
00:29:29.440 --> 00:29:30.149
form.
00:29:30.159 --> 00:29:31.350
>> Can you walk us through what we're
00:29:31.360 --> 00:29:32.789
seeing in these images?
00:29:32.799 --> 00:29:34.950
>> Sure. When stars form, they're
00:29:34.960 --> 00:29:37.510
surrounded by gas and dust left over
00:29:37.520 --> 00:29:40.149
from the formation process. In the early
00:29:40.159 --> 00:29:42.630
stages, this is called a circumstellar
00:29:42.640 --> 00:29:45.110
disc. But once planets start forming in
00:29:45.120 --> 00:29:47.669
the disc, we call it a protolanetary
00:29:47.679 --> 00:29:50.310
disc. These discs are where planetary
00:29:50.320 --> 00:29:52.630
systems like our own solar system come
00:29:52.640 --> 00:29:53.350
from.
00:29:53.360 --> 00:29:55.029
>> What makes these particular images
00:29:55.039 --> 00:29:55.830
special?
00:29:55.840 --> 00:29:58.149
>> Hubble captured them using two different
00:29:58.159 --> 00:30:00.630
approaches. The visible light images
00:30:00.640 --> 00:30:03.029
taken with Hubble's advanced camera for
00:30:03.039 --> 00:30:06.389
surveys show four protolanetary discs
00:30:06.399 --> 00:30:09.029
where you can actually see polar jets of
00:30:09.039 --> 00:30:11.990
gas shooting out from the young stars.
00:30:12.000 --> 00:30:14.950
You can also see brightly lit nebula.
00:30:14.960 --> 00:30:16.950
And there's this cool effect where the
00:30:16.960 --> 00:30:19.990
dark band around each star is actually a
00:30:20.000 --> 00:30:22.710
shadow cast onto the nebula by the disc
00:30:22.720 --> 00:30:23.830
itself.
00:30:23.840 --> 00:30:26.310
>> That's wild. So, we're seeing the shadow
00:30:26.320 --> 00:30:28.549
of the planet forming disc.
00:30:28.559 --> 00:30:31.350
>> Exactly. And each of these systems has
00:30:31.360 --> 00:30:35.750
unique characteristics. One called HH390
00:30:35.760 --> 00:30:38.789
isn't quite edge on, so you only see one
00:30:38.799 --> 00:30:41.990
side of its nebulosity. Another Tao
00:30:42.000 --> 00:30:44.310
042021
00:30:44.320 --> 00:30:47.190
is seen edge on and is in a later stage
00:30:47.200 --> 00:30:49.430
of evolution where the dust grains have
00:30:49.440 --> 00:30:51.669
already clumped together into larger
00:30:51.679 --> 00:30:53.669
grains which is part of the planet
00:30:53.679 --> 00:30:55.190
formation process.
00:30:55.200 --> 00:30:58.070
>> What about that third one HH48?
00:30:58.080 --> 00:31:00.950
>> Oh, that's particularly interesting.
00:31:00.960 --> 00:31:04.789
HH48 is actually a binary protoar
00:31:04.799 --> 00:31:06.789
system. And you can see how the
00:31:06.799 --> 00:31:09.430
gravitational power from the larger star
00:31:09.440 --> 00:31:11.669
is shaping the disc around its less
00:31:11.679 --> 00:31:14.310
massive companion. It's a great example
00:31:14.320 --> 00:31:16.630
of how stellar environments affect
00:31:16.640 --> 00:31:17.990
planet formation.
00:31:18.000 --> 00:31:19.990
>> And the infrared images show something
00:31:20.000 --> 00:31:20.789
different.
00:31:20.799 --> 00:31:23.269
>> Right. The infrared images taken with
00:31:23.279 --> 00:31:26.389
Hubble's wide field camera 3 show the
00:31:26.399 --> 00:31:29.190
bright protoars despite being surrounded
00:31:29.200 --> 00:31:32.389
by dust. Dust absorbs starlight and then
00:31:32.399 --> 00:31:34.870
remits it in infrared, which allows
00:31:34.880 --> 00:31:37.750
Hubble to see the stars. The jets aren't
00:31:37.760 --> 00:31:39.990
visible in these infrared images, but
00:31:40.000 --> 00:31:42.310
you get a much better view of the stars
00:31:42.320 --> 00:31:44.710
themselves and their dusty discs.
00:31:44.720 --> 00:31:46.950
>> Where are these protolanetary discs
00:31:46.960 --> 00:31:47.990
located?
00:31:48.000 --> 00:31:50.149
>> Most of them are in well-known star
00:31:50.159 --> 00:31:52.389
forming regions. Several are in the
00:31:52.399 --> 00:31:55.190
Orion molecular cloud complex. That's
00:31:55.200 --> 00:31:57.110
one of the most active star forming
00:31:57.120 --> 00:31:59.830
regions visible from Earth located about
00:31:59.840 --> 00:32:02.870
1,500 lighty years away. Others are in
00:32:02.880 --> 00:32:04.950
the Perseus molecular cloud.
00:32:04.960 --> 00:32:07.029
>> Now, we also have the James Webb Space
00:32:07.039 --> 00:32:08.630
Telescope observing these kinds of
00:32:08.640 --> 00:32:10.870
objects. How do Hubble's observations
00:32:10.880 --> 00:32:11.830
compare?
00:32:11.840 --> 00:32:15.190
>> That's a great question. JWST has been
00:32:15.200 --> 00:32:17.669
doing incredible work on protostars and
00:32:17.679 --> 00:32:20.710
protolanetary discs, too. In fact, there
00:32:20.720 --> 00:32:23.509
was research published in 2024 based on
00:32:23.519 --> 00:32:26.549
JWST observations showing that some
00:32:26.559 --> 00:32:29.110
young protostars have layered structures
00:32:29.120 --> 00:32:31.990
of winds and jets, inner jets surrounded
00:32:32.000 --> 00:32:34.470
by outer cone-shaped jets.
00:32:34.480 --> 00:32:35.990
>> So, the two telescopes are
00:32:36.000 --> 00:32:37.350
complimentary.
00:32:37.360 --> 00:32:40.310
>> Exactly. Hubble excels in visible and
00:32:40.320 --> 00:32:43.509
some infrared wavelengths while JWST is
00:32:43.519 --> 00:32:45.830
optimized for infrared. Together, they
00:32:45.840 --> 00:32:48.230
give us a much more complete picture.
00:32:48.240 --> 00:32:50.149
For instance, Hubble can show us those
00:32:50.159 --> 00:32:52.389
beautiful jets and nebula in visible
00:32:52.399 --> 00:32:55.830
light, while JWST can peer through dust
00:32:55.840 --> 00:32:58.149
to see the nested structure of winds and
00:32:58.159 --> 00:33:01.029
jets using different chemical tracers.
00:33:01.039 --> 00:33:03.029
How much longer can we expect Hubble to
00:33:03.039 --> 00:33:04.230
keep operating?
00:33:04.240 --> 00:33:06.710
>> That's the big question. Hubble was
00:33:06.720 --> 00:33:09.509
launched in 1990 with an expected
00:33:09.519 --> 00:33:12.070
15-year lifetime, but it's now lasted
00:33:12.080 --> 00:33:14.870
more than 35 years thanks to five
00:33:14.880 --> 00:33:17.430
servicing missions. However, it is
00:33:17.440 --> 00:33:19.909
showing its age. The telescope has been
00:33:19.919 --> 00:33:22.389
losing gyroscopes, which means it takes
00:33:22.399 --> 00:33:24.710
more time to point at targets.
00:33:24.720 --> 00:33:28.070
Observations are down by about 12% with
00:33:28.080 --> 00:33:30.149
a corresponding reduction in science
00:33:30.159 --> 00:33:30.870
output.
00:33:30.880 --> 00:33:32.789
>> But it's still functioning, right?
00:33:32.799 --> 00:33:35.430
>> Oh, yes. NASA expects Hubble to keep
00:33:35.440 --> 00:33:37.990
operating into the 2030s. And there's
00:33:38.000 --> 00:33:40.310
been talk, though it's not confirmed, of
00:33:40.320 --> 00:33:42.310
a possible servicing mission that could
00:33:42.320 --> 00:33:45.029
extend its life even further. Who would
00:33:45.039 --> 00:33:47.029
conduct that servicing mission?
00:33:47.039 --> 00:33:49.350
>> That's the interesting part. NASA
00:33:49.360 --> 00:33:51.430
doesn't have the space shuttle anymore,
00:33:51.440 --> 00:33:53.110
which was used for all previous
00:33:53.120 --> 00:33:55.590
servicing missions. Any future servicing
00:33:55.600 --> 00:33:57.190
mission would likely involve a
00:33:57.200 --> 00:33:59.029
commercial spacecraft, possibly
00:33:59.039 --> 00:34:01.430
something from SpaceX or another company
00:34:01.440 --> 00:34:03.669
developing servicing capabilities.
00:34:03.679 --> 00:34:05.590
>> It would be amazing if Hubble could keep
00:34:05.600 --> 00:34:07.430
going for another decade.
00:34:07.440 --> 00:34:09.990
>> It really would. And if it does, it'll
00:34:10.000 --> 00:34:11.430
continue contributing to our
00:34:11.440 --> 00:34:13.990
understanding of star formation, planet
00:34:14.000 --> 00:34:16.389
formation, and so many other areas of
00:34:16.399 --> 00:34:19.030
astronomy. These protolanetary disc
00:34:19.040 --> 00:34:21.349
images are a perfect example of how
00:34:21.359 --> 00:34:23.589
Hubble is still answering fundamental
00:34:23.599 --> 00:34:26.149
questions about how planetary systems
00:34:26.159 --> 00:34:27.990
like ours come to be.
00:34:28.000 --> 00:34:29.669
>> When you think about it, Hubble has
00:34:29.679 --> 00:34:31.349
literally changed our view of the
00:34:31.359 --> 00:34:33.589
universe. From the Hubble deep field to
00:34:33.599 --> 00:34:35.750
these protolanetary discs, from
00:34:35.760 --> 00:34:37.430
measuring the expansion rate of the
00:34:37.440 --> 00:34:39.430
universe to studying exoplanet
00:34:39.440 --> 00:34:41.510
atmospheres, it's been an incredible
00:34:41.520 --> 00:34:42.790
horsework.
00:34:42.800 --> 00:34:45.349
>> Absolutely. And the fact that it's still
00:34:45.359 --> 00:34:47.510
delivering cuttingedge science more than
00:34:47.520 --> 00:34:49.990
30 decades after launch is a testament
00:34:50.000 --> 00:34:52.069
to the foresight of designing it to be
00:34:52.079 --> 00:34:54.869
serviceable and upgradable. It's a model
00:34:54.879 --> 00:34:56.470
for how we should think about building
00:34:56.480 --> 00:34:58.550
space-based observatories.
00:34:58.560 --> 00:35:00.390
>> Well, that wraps up today's episode of
00:35:00.400 --> 00:35:02.470
Astronomy Daily. We covered a lot of
00:35:02.480 --> 00:35:04.790
ground from the uncertain fate of NASA's
00:35:04.800 --> 00:35:07.430
Maven Orbiter to the historic ISS
00:35:07.440 --> 00:35:09.589
medical evacuation. From Europe's
00:35:09.599 --> 00:35:11.430
expanding launch capabilities to
00:35:11.440 --> 00:35:14.230
groundbreaking asteroid defense research
00:35:14.240 --> 00:35:16.470
and we learned about lunar timekeeping
00:35:16.480 --> 00:35:18.230
software that will enable the next
00:35:18.240 --> 00:35:20.790
generation of moon missions. AMP saw how
00:35:20.800 --> 00:35:22.550
Hubble continues to reveal the
00:35:22.560 --> 00:35:25.829
birthplaces of planets after 35 years in
00:35:25.839 --> 00:35:28.310
orbit. It's been quite a week in space
00:35:28.320 --> 00:35:29.990
news and we've only just scratched the
00:35:30.000 --> 00:35:30.950
surface.
00:35:30.960 --> 00:35:33.030
>> Before we go, a quick reminder that you
00:35:33.040 --> 00:35:35.109
can find more space and astronomy news
00:35:35.119 --> 00:35:38.150
at our website, astronomyaily.io.
00:35:38.160 --> 00:35:40.069
And don't forget to subscribe so you
00:35:40.079 --> 00:35:41.589
never miss an episode.
00:35:41.599 --> 00:35:43.270
>> You can also follow us on social media
00:35:43.280 --> 00:35:45.190
for bonus content and updates throughout
00:35:45.200 --> 00:35:46.150
the week.
00:35:46.160 --> 00:35:48.230
>> Thanks for joining us today, everyone.
00:35:48.240 --> 00:35:53.270
>> Clear skies and we'll see you on Monday.
00:35:53.280 --> 00:36:01.510
The stories we told
00:36:01.520 --> 00:36:09.430
stories told
00:36:09.440 --> 00:36:12.079
stories




