Solar Storm Hits Early! Plus China's Reusable Rockets & Exoplanet Magnetic Shields
The Sun's latest outburst arrived ahead of schedule! A powerful X1.9 solar flare and massive CME triggered severe G4 geomagnetic storms on January 19th, bringing spectacular auroras as far south as Alabama. Hosts Anna and Avery break down what happened and what to expect.
Also in today's episode: China successfully tests the Long March 12B reusable rocket, giving us a preview of their next-gen launch capabilities. We get an exclusive look at the Xuntian space telescope set to launch in 2027, which could rival Hubble with 300x the field of view. Plus, stunning new Hubble images reveal how baby stars carve out cosmic homes in the Orion Molecular Cloud.
We'll run through this week's packed launch schedule featuring SpaceX, Blue Origin, Rocket Lab, and China, and explore groundbreaking research showing how hidden magma oceans might protect rocky exoplanets from deadly radiation.
**Episode Highlights:**
• BREAKING: Severe G4 solar storm strikes Earth early - aurora forecast through Jan 20
• China's Long March 12B reusable rocket passes critical static fire test
• Xuntian telescope preview: China's answer to Hubble launches 2027
• Hubble reveals protostar jets and cavities in Orion Molecular Cloud
• 7 launches from 6 sites this week: Your complete guide
• Basal magma oceans could generate protective magnetic fields on super-Earths
**Topics Covered:**
Space Weather, Solar Flares, CMEs, Geomagnetic Storms, Auroras, Reusable Rockets, Chinese Space Program, Space Telescopes, Star Formation, Orbital Launches, Exoplanets, Planetary Magnetism, Astrobiology
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This episode includes AI-generated content.
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Anna: Welcome to Astronomy Daily, your daily dose
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of space and astronomy news. I'm Anna.
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Avery: And I'm Avery. Today is Tuesday, January
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20, 2026, and we've got a
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fantastic lineup of stories covering
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everything from solar storms to Chinese space
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technology and some fascinating discoveries
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about how young stars shape their cosmic
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neighborhoods.
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Anna: That's right. We're going to dive into some
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breaking news about the Sun's latest
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outburst. There's been quite a development
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there that aurora chasers definitely need to
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about.
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Avery: Plus, China continues to make impressive
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strides in reusable rocket technology with
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the long 3-12-B. And we'll get a sneak peek
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at their upcoming Xuntian Space Telescope
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that's set to rival some of the best
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observatories in orbit.
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Anna: We'll also journey into the Orion molecular
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cloud to see how baby stars are literally
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carving out their homes in space. Check out
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this week's busy launch schedule and explore
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a fascinating new theory about how some
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exoplanets might protect themselves from
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deadly radiation.
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Avery: So grab your coffee, settle in, and let's get
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started with today's Astronomy Daily.
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Anna: Alright, Avery, let's jump right into our top
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story. And this one's developing even as we
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speak. The sun threw a massive tantrum this
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weekend, and Earth is already feeling the
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effects.
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Avery: That's right, Anna. Uh, on Sunday, January
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18, the sun unleashed a powerful X
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1.9 class solar flare from Sunspot
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region AR4341. For our
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listeners who might not be familiar, X class
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flares are the most powerful category of
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solar eruptions. And this one came with a
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particularly energetic friend.
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Anna: A, uh, coronal mass ejection, or a cme.
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Right.
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Avery: Exactly. This CME was what
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forecasters call a, uh, full halo event,
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meaning it was aimed directly at Earth. The
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interesting twist here is that it arrived
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much sooner than predicted. Space weather
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forecasters initially expected it to hit
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sometime within 24 hours of the flare, but
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it actually slammed into Earth's
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magnetosphere yesterday, January 19th
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at 2:38pm Eastern Time.
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Anna: And I'm guessing from the reports I've been
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seeing, this wasn't a gentle arrival.
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Avery: Not at all. The CME triggered severe
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G4 geomagnetic storms. According
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to NOAA's Space Weather Prediction center,
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this is actually a pretty rare event. We're
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also dealing with an S IV severe solar
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radiation storm that's ongoing.
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Anna: Now, for those wondering why this matters,
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let's talk about what makes a CME GEO
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effective or not. It's all about magnetic
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field orientation, isn't it?
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Avery: That's the crucial factor when a CME
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arrives. If its magnetic field is oriented
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southward, what scientists call a negative
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BZ component, it can connect with Earth's
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northward pointing magnetic field. Think of
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it like opening a door. The southward
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orientation essentially allows solar wind
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energy to pour into our magnetosphere,
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triggering geomagnetic storms.
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Anna: And in this case, that door was wide open.
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Avery: Exactly. Data from the DSCOVR
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and a spacecraft which monitor the solar wind
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upstream of Earth confirmed that southward
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BZ component. That's what made this storm so
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potent.
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Anna: So what does this mean for people on the
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ground? Obviously, there's the spectacular
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side with Auroras, but there are practical
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concerns too, right?
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Avery: The good news is that this storm could push
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the northern lights much further south than
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usual. According to NOAA scales, G4
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storms can make auroras visible as far south
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as Alabama and Northern California. But there
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are some downsides. These storms can disrupt
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GPS navigation, affect satellite
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operations, increase atmospheric drag on
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spacecraft, and potentially impact power
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grids and high frequency radio commun.
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Anna: And the flare itself caused immediate
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problems when it erupted, correct?
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Avery: Yes. The X dot 1.9 flare
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triggered strong R3 level radio blackouts
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across the sunlit side of Earth, with the
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Americas taking the biggest hit. Radio
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blackouts happen because the intense X rays
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and extreme ultraviolet radiation from the
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flare ionized the upper atmosphere,
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disrupting radio.
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Anna: Signals for our aurora chasers out
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there. What's the forecast looking like?
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Avery: Well, geomagnetic storm conditions are
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expected to continue through at least today,
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January 20th. The best viewing times
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are typically between 10pm and 4am
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local time. Of course, you'll want to get
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away from city lights and find the darkest
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location possible. And keep in mind you need
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clear skies to see them.
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Anna: The timing is interesting too, isn't it?
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We're well into solar maximum.
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Avery: We are solar. Cycle 25 has been
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particularly active, and we're seeing the
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effects. The sun has been consistently active
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throughout late 2025 and into
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2026, with multiple X class
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flares and CMEs. This is exactly
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the kind of activity we expect during solar
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maximum.
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Anna: It's yet another reminder that our star is a
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dynamic, powerful force. What's
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fascinating to me is how much we've learned
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about predicting these events. Even if this
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one arrived earlier than expected.
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Avery: Absolutely. Space weather forecasting has
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come a long way, but CMEs are still
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notoriously tricky. Their speed,
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direction, and crucially, their magnetic
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orientation all factor into how they'll
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interact with Earth. We often don't know the
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full picture until spacecraft like
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DSCOVR sample them directly when
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they're almost at our doorstep.
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Anna: Well, if you're in the northern tier states
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of the US Or Canada. Keep your eyes on the
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sky tonight. This could be a spectacular
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display.
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Avery: Shifting gears from solar fireworks to human
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engineering.
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Let's talk about China's latest achievement
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in reusable rocket technology. The China
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Aerospace Science and Technology Corporation
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has successfully conducted a static fire test
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of the Long March 12B.
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Anna: This is China's follow up to the Long March
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12A, which we covered when it made its maiden
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flight back in late December 2025, right?
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Avery: Exactly. And if you recall, that first
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flight was partially successful. The second
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stage successfully delivered its payload to
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orbit, but the reusable first stage
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crashed near the intended recovery area in
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Gansu Province. So there's definitely been
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some lessons learned.
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Anna: Let's talk specs. What can you tell us about
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the Long March 12B?
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Avery: It's a fairly substantial vehicle. The
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rocket stands approximately 70 meters tall.
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That's about 230ft with a
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diameter of 4 meters. Both stages use
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liquid oxygen and kerosene propellants, which
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is interesting because it's the same
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propellant combination that SpaceX uses in
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their Falcon 9.
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Anna: And in terms of capability, in its.
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Avery: Baseline configuration, the long March 12B
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can lift about 20 metric tons to low Earth
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orbit. That puts it firmly in the heavy
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medium lift category. When fully fueled, the
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entire vehicle has a liftoff mass of around
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700 tons.
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Anna: So what exactly did this static fire test
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accomplish?
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Avery: The test, which took place Friday at the
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Jiuquan Satellite Launch center in northwest
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China, was all about validation. Ground
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teams ignited the first stage engines and
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sustained combustion for a period while
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monitoring performance and control
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parameters. They were verifying fueling
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procedures, ignition sequences, and making
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sure all the propulsion and support systems
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worked smoothly under planned conditions.
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Anna: And the reusability aspect, how does that
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work?
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Avery: This is where it gets really interesting. The
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first stage is designed to separate from the
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second stage during flight, then flip itself
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around for re entry, using aerodynamic grid
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fins for guidance. Picture those waffle like
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fins you see on Falcon 9 boosters. Then
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it uses deployable landing legs to touch down
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vertically at a designated landing zone.
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Anna: So it's very much following the SpaceX
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playbook.
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Avery: It is. Though China has been developing this
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technology independently, the goal is the
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same reusability to cut mission costs and
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increase launch cadence. This is especially
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important for China's commercial space sector
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and their growing Satellite Constellation
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projects.
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Anna: And you mentioned The Long March 12A's
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landing attempt failed. Are they
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incorporating what they learned from that
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into the 12B?
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Avery: Absolutely. Engineering teams are still
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investigating what went wrong with that
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December landing attempt. And the lessons
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from that mission are being fed directly into
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refinements for the long March 12th B's
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reentry and landing systems. That's actually
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a really important part of the development
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process.
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Anna: Uh, so when might we see an actual
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launch of the long March 12b.
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Avery: Based on this successful static fire test?
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We're probably looking at flight tests in the
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near future. They still need to do more
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ground testing and verification, but
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successful engine testing is a major
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milestone on the path to orbital flight.
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Anna: It's interesting to watch multiple countries
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and companies working on reusable rocket
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technology. It really does seem to be the
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future of spaceflight.
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Avery: No question. When you can land and reuse your
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first stage, which is the most expensive part
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of the rocket, the economics of space access
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change dramatically. China positioning
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themselves with both the 12A and 12B
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shows they're committed to competing in this
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arena.
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Anna: Staying with China's space program, let's
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look ahead to what could be one of the most
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capable space telescopes ever launched.
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The Chinese space station telescope known as
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Xuntian is gearing up for launch as soon
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as early 2027.
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Avery: And scientists just completed something
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pretty important. A, uh, full end to end
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observation simulation to test how the
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telescope will perform once it's in orbit.
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Anna: Let's start with the basics. How big is this
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thing?
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Avery: Xuntian features a 2 meter primary
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mirror that's about 6.6ft across.
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For comparison, that's slightly smaller than
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Hubble's 2.4 meter mirror. But here's
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where it gets interesting. Juntian is
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designed specifically as a survey instrument.
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And in that role, it's going to be far more
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capable than Hubble.
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Anna: How so?
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Avery: It's all about field of view. Juntian's
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field of view is about 300 times larger than
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Hubble's. That means it can survey the sky
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much more efficiently. Combine that with a
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2.5 billion pixel camera and the
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ability to observe from near ultraviolet to
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near infrared wavelengths, and you've got
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yourself an extremely powerful sky surveying
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machine.
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Anna: That's impressive. What will it be looking
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for?
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Avery: The science goals are pretty ambitious.
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According to the National Astronomical
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Observatories under the Chinese Academy of
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Sciences, Chuntian should make major
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contributions across multiple
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cosmology, galaxy formation and evolution,
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the structure and evolution of our own Milky
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Way, and studies of stars and planets.
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Anna: I've also heard it might help us understand
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dark matter and dark energy.
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Avery: Exactly. Those are two of the biggest
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mysteries in astrophysics. And a wide Field
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survey telescope like Shuntian is perfectly
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suited to contribute to that research by
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mapping large areas of the sky and observing
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how galaxies cluster and move, Scientists
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can gather evidence about the nature of dark
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matter and dark energy.
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Anna: Now what makes Xuntian really unique is how
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it will operate in relation to China's
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Tiangong Space Station. Right.
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Avery: That's one of the coolest aspects. Chun Tian
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will fly independently in low Earth orbit, co
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orbiting with Tiangong, but doing its own
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thing. However. And um, this is the really
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neat part. It's designed to dock with the
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space.
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Anna: Station when needed dough astronauts can
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service it exactly.
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Avery: Just like NASA astronauts serviced Hubble
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five times between 1993 and
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2009. According to recent video from
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China Central Television astronauts will be
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able to conduct spacewalks to maintain,
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repair or even upgrade the observatory.
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This is a huge advantage because it extends
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the operational life of the telescope and
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allows for technology upgrades over time.
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Anna: That's actually brilliant. Hubble's servicing
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missions turned it from a disappointment into
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one of the most productive scientific
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instruments ever built.
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Avery: Absolutely. And China clearly learned from
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that example. Being able to service a space
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telescope in orbit is enormously valuable.
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Anna: Tell us about these simulations they just
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completed.
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Avery: The research team built what they call an end
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to end simulation suite. Basically they
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created mock observations that replicate the
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expected instrumental and observational
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conditions. They tested both the optical
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systems and other observation systems to
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evaluate the telescope's overall performance
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before it ever leaves the ground.
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Anna: That makes sense. Better to find problems in
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simulation than after launch.
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Avery: The results were published in the journal
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Research in Astronomy and Astrophysics in
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early January. This kind of validation work
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is crucial for a mission of this scale and
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complexity.
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Anna: When you say early 2027, how
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firm is that timeline?
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Avery: It's a no earlier than timeline. These
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large space telescopes are complex beasts and
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schedules can slip. But if everything stays
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on track, we could see Xuntian launching on a
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long March 5th B rocket sometime in the
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first half of 2027.
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Anna: It's going to be really interesting to see
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what Chuntian discovers once it's
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operational. Having another major space
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telescope conducting surveys will be
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fantastic for astronomy.
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Avery: Next, let's head out to one of the most
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famous star forming regions in our cosmic
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neighborhood. The Orion Molecular Cloud
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complex. The Hubble Space Telescope has
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captured some stunning new images that reveal
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how baby stars are literally carving out
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space for themselves in the surrounding gas
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and dust.
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Anna: This is such a beautiful topic. These are
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protostars, right? Stars that haven't quite
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grown up yet?
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Avery: That's right. Protostars are young stellar
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objects that are still in the process of
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accumulating mass from the molecular clouds.
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They're Forming in. They haven't started
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fusing hydrogen into helium yet, which is
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what defines a main sequence star like our
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Sun. But even though they're not doing
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fusion, they're far from quiet.
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Anna: They're quite energetic, actually,
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incredibly so.
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Avery: Protostars generate powerful winds and jets
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that shape their surroundings in dramatic
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ways. These jets and winds carve out bubbles
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and caverns in the surrounding gas. And
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astrophysicists have been trying to better
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understand this feedback process.
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Anna: What's driving these jets?
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Avery: It's a fascinating process. Material from the
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molecular cloud first forms a disk around the
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protostar. Not all of that material makes it
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onto the star itself. Some gets accelerated
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to high speeds along the star's magnetic
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field lines and shot out from the poles as
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focus beams of mostly hydrogen.
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Anna: So they're like cosmic fire hoses.
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Avery: That's a good analogy. And in addition to
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these focused jets, protostars also produce
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wide angle stellar winds that flow in all
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directions. These winds from young stars are
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actually far more powerful than the solar
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wind from our sun or other main sequence
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stars.
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Anna: What did the Hubble images reveal?
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Avery: The three new images show protostars at
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different stages, all in the Orion molecular
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complex. You can actually see the cavernous
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shapes these young stars have carved out from
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the surrounding gas. It's quite striking
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visually, these dark, sometimes intricate
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structures against the glowing background of
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the nebula.
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Anna: But there was a surprising finding in the
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research, wasn't there?
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Avery: Yes, and it challenges some assumptions.
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Researchers found that the cavities carved by
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these jetson winds didn't grow larger as the
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stars moved through their later formation
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stages. You might expect the cavities to keep
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expanding over time, but that's not what they
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observed.
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Anna: So what does that tell us?
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Avery: Well, the Orion molecular cloud has been
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experiencing a declining star formation rate.
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And these protostars also have lower rates of
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mass accretion over time. Scientists
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initially thought maybe this could be
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attributed to the jets and winds carving out
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all the available gas. But the new findings
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suggest that's not the case. The cavity sizes
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weren't the limiting factor.
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Anna: So something else is controlling the star
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formation rate.
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Avery: Exactly. There must be other factors at play
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in regulating how quickly stars form and grow
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in this region. It's a reminder that even in
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well studied regions like Orion, we're still
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learning the details of how star formation
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works.
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Anna: I love that these images aren't just pretty
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pictures. They're revealing actual physics.
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Avery: That's what makes astronomy so exciting.
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Every observation adds a piece of the puzzle.
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In this case, we're learning that the
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feedback from young stars through their jets
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and winds. While dramatic and visually
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spectacular, might not be the main factor
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controlling star formation in the region.
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Anna: It's also interesting to think about our own
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sun going through this phase billions of
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years ago.
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Avery: Absolutely. When the sun was young, it was in
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a cluster with its siblings, probably in a
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molecular cloud, much like Orion. It would
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have had these same powerful jets and winds
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shaping the gas and dust around it.
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Eventually the molecular cloud dispersed, the
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star cluster broke up and the sun ended up as
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the solitary star we know today.
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Anna: Orion is close enough that we can study these
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processes in detail, which is really lucky
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for astronomers.
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Avery: Very lucky. At about 1350
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light years away, it's one of the nearest
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large star forming regions. We can resolve
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individual protostars and their surrounding
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structures, which gives us insights we can
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apply to understanding star formation
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throughout the galaxy and beyond.
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Anna: Alright, let's shift from natural cosmic
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phenomena to human made space activities.
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We've got a busy week of launches coming up.
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Avery.
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Avery: We do indeed. Seven launches from six
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00:18:06.650 --> 00:18:08.850
different sites across the globe. Let's run
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through them.
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Anna: The week actually started this morning with a
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Chinese launch, correct?
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Avery: That's right. A uh, Chang Zhang 12 rocket,
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also known as Long March 12, lifted off
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from Commercial Launch Complex 2 at Wenchang
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Space Launch Site in Hainan, China. This was
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at 7:48 UTC. Carrying nine
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SatNet satellites to low Earth orbit. The
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CZ12 can lift about 12,000
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kilograms to LEO. And this was a
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demonstration of China's commercial launch
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capabilities.
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Anna: Moving on to tomorrow.
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Avery: What do we have tomorrow? January 21st
476
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we have Rocket Lab launching from New
477
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Zealand. Their Electron rocket will be
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carrying two satellites for open Cosmos as
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part of a secure broadband constellation
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being built in the uk. The mission is called
481
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the Cosmos will see you now. And liftoff is
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scheduled for 11:09 UTC. From their
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facility on the Mahia Peninsula.
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Anna: Rocket Lab has really established a solid
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cadence with Electron.
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Avery: They have. This will be Electron's 80th
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mission. That's a remarkable achievement for
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a small rocket. The vehicle has proven itself
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reliable and capable, especially for these
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small satellite constellation deployments.
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Anna: It's Wednesday. That gets particularly
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interesting with the Isar Aerospace launch.
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Avery: Yes, this is Isar's second attempt to launch
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their Spectrum rocket from the Andoya rocket
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range in Norway. The mission is called Onward
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and Upward, which is fitting given that their
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first attempt in March 2025 failed
498
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shortly after liftoff due to an engine issue.
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Anna: What's different this time?
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Avery: Well, they've been investigating what went
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wrong on that first flight and making
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refinements. Spectrum is a two stage
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rocket Powered by Aquila engines using
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propane and liquid oxygen, it's designed for
505
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the satellite Constellation market and can
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lift about a thousand kilograms to leo.
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They're carrying several cubesats for the
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European Space Agency's Boost program.
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Anna: So fingers crossed for ISAR on Wednesday.
510
00:20:03.690 --> 00:20:04.410
What else?
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Avery: Wednesday is also when SpaceX has their first
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Falcon 9 launch of the week. They're
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launching 24 Starlink satellites from
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Vandenberg Space Force Base in California.
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Liftoff is currently targeted for 2:43
516
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UTC on January 22, which
517
00:20:20.290 --> 00:20:22.610
is 6:43pm Pacific Time on the
518
00:20:22.610 --> 00:20:23.350
21st.
519
00:20:23.350 --> 00:20:25.590
Anna: Vandenberg has been busy lately.
520
00:20:25.670 --> 00:20:28.590
Avery: Very busy. This mission will use booster
521
00:20:28.590 --> 00:20:30.950
B1093 on its 10th flight.
522
00:20:31.270 --> 00:20:33.550
Landing on the drone ship Of Course I Still
523
00:20:33.550 --> 00:20:35.790
Love youe in the Pacific. It's another
524
00:20:35.790 --> 00:20:38.310
example of SpaceX's routine reuse.
525
00:20:38.470 --> 00:20:41.030
This particular booster has previously flown
526
00:20:41.030 --> 00:20:43.350
seven Starlink missions and two military
527
00:20:43.350 --> 00:20:43.750
missions.
528
00:20:43.910 --> 00:20:46.590
Anna: Do we have a New Shepard launch from Blue
529
00:20:46.590 --> 00:20:47.510
Origin this week?
530
00:20:47.750 --> 00:20:50.310
Avery: Correct. Blue Origin is targeting Thursday,
531
00:20:50.630 --> 00:20:53.016
January 22nd at 1430
532
00:20:53.164 --> 00:20:55.780
UTC. That's 9:30am Eastern
533
00:20:55.940 --> 00:20:58.820
for New Shepard's 17th crewed mission,
534
00:20:58.820 --> 00:21:01.740
designated NS38. This will
535
00:21:01.740 --> 00:21:04.460
be a suborbital flight from Launch Site 1 in
536
00:21:04.460 --> 00:21:07.180
West Texas, carrying six people past the
537
00:21:07.180 --> 00:21:09.500
Karman Line and into space for a few minutes
538
00:21:09.500 --> 00:21:10.339
of weightlessness.
539
00:21:10.580 --> 00:21:12.620
Anna: New Shepard has really become a regular
540
00:21:12.620 --> 00:21:13.700
operation for them.
541
00:21:13.940 --> 00:21:16.540
Avery: It has. The capsule will separate from the
542
00:21:16.540 --> 00:21:18.780
booster, which will return for a propulsive
543
00:21:18.780 --> 00:21:20.820
landing while the capsule lands under
544
00:21:20.820 --> 00:21:23.460
parachutes with retro thrusters firing just
545
00:21:23.460 --> 00:21:25.620
before touchdown to soften the landing for
546
00:21:25.620 --> 00:21:26.320
the crew.
547
00:21:26.480 --> 00:21:28.560
Anna: And we round out the week with.
548
00:21:28.880 --> 00:21:31.840
Avery: Two more launches on Sunday, January 25.
549
00:21:32.400 --> 00:21:35.000
First, China will conduct the sea launch of a
550
00:21:35.000 --> 00:21:37.840
Geelong 3 rocket from the South China Sea.
551
00:21:38.240 --> 00:21:40.560
Details on the payload are still under wraps.
552
00:21:40.560 --> 00:21:42.560
They'll likely release that information after
553
00:21:42.560 --> 00:21:45.434
the launch. Liftoff is scheduled for 6:30
554
00:21:45.566 --> 00:21:46.160
UTC.
555
00:21:46.320 --> 00:21:48.240
Anna: Sea launches are always interesting.
556
00:21:48.560 --> 00:21:51.440
Avery: They are. The Jialong 3 is a four stage
557
00:21:51.440 --> 00:21:53.560
solid fueled rocket that launches from a
558
00:21:53.560 --> 00:21:55.780
maritime platform. It's an interesting
559
00:21:55.780 --> 00:21:58.180
capability that gives China flexibility in
560
00:21:58.180 --> 00:22:01.100
launch azimuth and location. And finally,
561
00:22:01.420 --> 00:22:04.380
Sunday also brings SpaceX's second Falcon
562
00:22:04.380 --> 00:22:06.940
9 launch of the week. Also from Vandenberg,
563
00:22:07.260 --> 00:22:09.700
another batch of 24 Starlink satellites
564
00:22:09.700 --> 00:22:12.540
heading to orbit at 1517 UTC.
565
00:22:12.860 --> 00:22:14.788
This one will use booster
566
00:22:15.012 --> 00:22:17.580
B0088 on its 13th flight,
567
00:22:17.660 --> 00:22:19.660
another testament to booster reusability.
568
00:22:19.980 --> 00:22:22.780
Anna: That's quite a week. Seven launches from
569
00:22:22.780 --> 00:22:25.740
six sites. It really shows how routine space
570
00:22:27.240 --> 00:22:27.640
it does.
571
00:22:27.720 --> 00:22:29.880
Avery: And it's only going to get busier as more
572
00:22:29.880 --> 00:22:32.040
commercial Constellations come online and
573
00:22:32.040 --> 00:22:33.800
more providers enter the launch market.
574
00:22:34.120 --> 00:22:37.080
Anna: And May we wish them all successful launches.
575
00:22:37.400 --> 00:22:38.040
Avery: Indeed.
576
00:22:38.360 --> 00:22:41.080
Moving along for our final story, let's
577
00:22:41.080 --> 00:22:43.480
journey to distant worlds and explore a
578
00:22:43.480 --> 00:22:45.920
fascinating new theory about how some rocky
579
00:22:45.920 --> 00:22:48.080
exoplanets might protect themselves from
580
00:22:48.080 --> 00:22:49.560
deadly cosmic radiation.
581
00:22:49.800 --> 00:22:52.610
Anna: This involves super Earths. Right? Those
582
00:22:52.610 --> 00:22:55.130
planets that are larger than our Earth but
583
00:22:55.130 --> 00:22:57.410
smaller than ice giants like Neptune.
584
00:22:57.490 --> 00:23:00.370
Avery: Exactly. Super Earths are actually the most
585
00:23:00.370 --> 00:23:02.490
common type of exoplanet we've found in our
586
00:23:02.490 --> 00:23:04.930
galaxy, which makes understanding them really
587
00:23:04.930 --> 00:23:07.090
important. But here's an interesting
588
00:23:08.049 --> 00:23:10.050
Many of these worlds might not be able to
589
00:23:10.050 --> 00:23:12.530
generate magnetic fields the way Earth does.
590
00:23:12.850 --> 00:23:15.170
Anna: And magnetic fields are crucial for
591
00:23:15.170 --> 00:23:17.090
protecting a planet's surface from harmful
592
00:23:17.090 --> 00:23:17.650
radiation.
593
00:23:18.180 --> 00:23:20.820
Avery: Right. Earth's magnetic field is generated by
594
00:23:20.820 --> 00:23:23.020
movement in our liquid iron outer core
595
00:23:23.020 --> 00:23:25.460
Through a process called a dynamo. But
596
00:23:25.460 --> 00:23:28.220
larger, rocky worlds like super Earths Might
597
00:23:28.220 --> 00:23:30.340
have cores that are completely solid or
598
00:23:30.420 --> 00:23:32.780
completely liquid, Neither of which can
599
00:23:32.780 --> 00:23:34.660
produce a magnetic field through the same
600
00:23:34.660 --> 00:23:35.220
mechanism.
601
00:23:35.620 --> 00:23:37.540
Anna: So how do they protect themselves?
602
00:23:37.860 --> 00:23:39.540
Avery: That's where this new research from the
603
00:23:39.540 --> 00:23:41.820
University of Rochester comes in. They
604
00:23:41.820 --> 00:23:44.740
propose an alternate source. Deep layers of
605
00:23:44.740 --> 00:23:47.660
molten rock called basal Magma Oceans,
606
00:23:47.660 --> 00:23:50.480
or BMOs, which exist at the boundary
607
00:23:50.480 --> 00:23:52.000
between a planet's mantle and.
608
00:23:52.000 --> 00:23:54.600
Anna: Core molten rock generating a
609
00:23:54.600 --> 00:23:55.520
magnetic field.
610
00:23:55.760 --> 00:23:58.080
Avery: It sounds surprising, but the key is what
611
00:23:58.080 --> 00:24:00.440
happens to rock under the extreme pressures
612
00:24:00.440 --> 00:24:03.360
inside super Earths. The research team, led
613
00:24:03.360 --> 00:24:05.680
by Associate Professor Miki Nakajima,
614
00:24:05.840 --> 00:24:08.560
Conducted laser shock experiments and quantum
615
00:24:08.560 --> 00:24:11.280
simulations to recreate the conditions deep
616
00:24:11.280 --> 00:24:12.800
inside these massive planets.
617
00:24:13.120 --> 00:24:14.160
Anna: What did they find?
618
00:24:14.560 --> 00:24:16.840
Avery: Under the crushing pressures found in super
619
00:24:16.840 --> 00:24:19.240
Earths? We're talking planets three to six
620
00:24:19.240 --> 00:24:22.240
times the mass of Earth. Molten rock becomes
621
00:24:22.240 --> 00:24:24.520
electrically conductive. And if you have
622
00:24:24.520 --> 00:24:27.000
electrically conductive material in motion,
623
00:24:27.160 --> 00:24:29.080
you can generate a magnetic field.
624
00:24:29.480 --> 00:24:32.440
Anna: So these basal magma oceans could act like
625
00:24:32.440 --> 00:24:35.240
liquid metal cores, Just using rock
626
00:24:35.240 --> 00:24:35.720
instead?
627
00:24:35.960 --> 00:24:38.520
Avery: Essentially, yes. The movement of this
628
00:24:38.520 --> 00:24:40.680
electrically conductive molten rock could
629
00:24:40.680 --> 00:24:43.600
drive what they call a BMO dynamo. And
630
00:24:43.600 --> 00:24:45.480
according to their models, these dynamos
631
00:24:45.480 --> 00:24:47.360
could generate magnetic fields that are
632
00:24:47.360 --> 00:24:49.640
actually stronger and longer lasting than
633
00:24:49.640 --> 00:24:51.880
those produced by core dynamos like Earth's.
634
00:24:52.270 --> 00:24:54.590
Anna: That's remarkable. How long could these
635
00:24:54.590 --> 00:24:55.230
fields last?
636
00:24:55.630 --> 00:24:58.150
Avery: Billions of years, potentially. That's
637
00:24:58.150 --> 00:25:00.430
important because for a planet to develop and
638
00:25:00.430 --> 00:25:02.990
sustain life, you need stable protection from
639
00:25:02.990 --> 00:25:05.630
radiation over very long timescales.
640
00:25:05.950 --> 00:25:08.590
Anna: Now, Earth probably had a basal magma
641
00:25:08.590 --> 00:25:10.670
ocean early in its history, right?
642
00:25:10.910 --> 00:25:13.870
Avery: Yes, shortly after formation. But Earth is
643
00:25:13.870 --> 00:25:16.710
relatively small, so as it cooled, that magma
644
00:25:16.710 --> 00:25:19.410
ocean eventually solidified. Super Earths,
645
00:25:19.410 --> 00:25:21.290
though, with their higher internal pressures
646
00:25:21.290 --> 00:25:23.810
and temperatures, could maintain these basal
647
00:25:23.810 --> 00:25:26.090
magma oceans for much, much longer,
648
00:25:26.330 --> 00:25:28.730
Potentially throughout their entire lifetime.
649
00:25:28.730 --> 00:25:31.210
Anna: This has pretty significant implications for
650
00:25:31.210 --> 00:25:32.970
the search for habitable worlds.
651
00:25:33.050 --> 00:25:36.050
Avery: Absolutely. One of the Factors in determining
652
00:25:36.050 --> 00:25:38.170
whether a planet might be habitable is
653
00:25:38.170 --> 00:25:40.930
whether it has magnetic protection. Without a
654
00:25:40.930 --> 00:25:43.330
magnetic field, a planet's atmosphere can be
655
00:25:43.330 --> 00:25:45.810
stripped away by stellar wind, making it hard
656
00:25:45.810 --> 00:25:48.330
for life to survive on the surface. If super
657
00:25:48.330 --> 00:25:50.610
Earths can generate magnetic fields through
658
00:25:50.610 --> 00:25:53.250
basal magma oceans, that potentially
659
00:25:53.250 --> 00:25:55.050
increases the number of worlds that could
660
00:25:55.050 --> 00:25:55.810
harbor life.
661
00:25:55.810 --> 00:25:57.490
Anna: How do we test this theory?
662
00:25:57.650 --> 00:26:00.170
Avery: That's the exciting next step. We need to
663
00:26:00.170 --> 00:26:02.650
actually detect and measure magnetic fields
664
00:26:02.650 --> 00:26:05.010
around exoplanets, which is extremely
665
00:26:05.010 --> 00:26:07.490
challenging with current technology. But next
666
00:26:07.490 --> 00:26:09.610
generation telescopes and instruments might
667
00:26:09.610 --> 00:26:12.010
be able to do it. Professor Nakajima
668
00:26:12.010 --> 00:26:14.050
mentioned she can't wait for future magnetic
669
00:26:14.050 --> 00:26:16.090
field observations of exoplanets to test
670
00:26:16.090 --> 00:26:16.930
their hypothesis.
671
00:26:17.090 --> 00:26:19.750
Anna: It's fascinating how interdisciplinary this
672
00:26:19.750 --> 00:26:22.590
research is, combining experimental physics,
673
00:26:22.670 --> 00:26:25.550
quantum simulations, and planetary evolution
674
00:26:25.550 --> 00:26:25.950
models.
675
00:26:26.190 --> 00:26:28.710
Avery: That's what makes it so robust. They weren't
676
00:26:28.710 --> 00:26:30.510
just working on theory. They actually
677
00:26:30.590 --> 00:26:33.390
recreated the conditions inside super Earths
678
00:26:33.390 --> 00:26:35.070
with laser shock experiments at the
679
00:26:35.070 --> 00:26:37.110
Laboratory for Laser Energetics at the
680
00:26:37.110 --> 00:26:39.550
University of Rochester. Then they combined
681
00:26:39.550 --> 00:26:41.350
that with computational modeling to
682
00:26:41.350 --> 00:26:43.350
understand how these conditions would evolve
683
00:26:43.350 --> 00:26:44.670
over billions of years.
684
00:26:44.910 --> 00:26:46.990
Anna: And this was challenging work for the team,
685
00:26:46.990 --> 00:26:47.510
wasn't it?
686
00:26:47.820 --> 00:26:50.340
Avery: Very much so. Professor Nakajima mentioned
687
00:26:50.340 --> 00:26:52.540
this was her first experimental work. Her
688
00:26:52.540 --> 00:26:55.140
background is primarily computational. She
689
00:26:55.140 --> 00:26:57.260
credited support from collaborators across
690
00:26:57.340 --> 00:26:59.300
various research fields for making this
691
00:26:59.300 --> 00:27:00.860
interdisciplinary work possible.
692
00:27:01.020 --> 00:27:02.860
Anna: It's a great reminder that some of the
693
00:27:02.860 --> 00:27:05.420
biggest scientific questions require bringing
694
00:27:05.420 --> 00:27:07.820
together expertise from multiple disciplines.
695
00:27:07.900 --> 00:27:10.500
Avery: Absolutely. Understanding planetary
696
00:27:10.500 --> 00:27:13.300
interiors, magnetic field generation and
697
00:27:13.300 --> 00:27:15.660
habitability requires geophysics,
698
00:27:15.900 --> 00:27:18.380
astrophysics, planetary science, and
699
00:27:18.380 --> 00:27:20.360
material science all working together.
700
00:27:20.680 --> 00:27:23.520
Anna: So the bottom line is super Earths might
701
00:27:23.520 --> 00:27:25.600
have, ah, a built in radiation shield that we
702
00:27:25.600 --> 00:27:28.080
didn't know about, Potentially making more of
703
00:27:28.080 --> 00:27:29.880
them candidates for harboring life.
704
00:27:30.040 --> 00:27:32.600
Avery: That's exactly right. It expands our
705
00:27:32.600 --> 00:27:34.240
understanding of what makes a planet
706
00:27:34.240 --> 00:27:36.600
potentially habitable and gives us new things
707
00:27:36.600 --> 00:27:38.960
to look for when we're evaluating exoplanets
708
00:27:38.960 --> 00:27:40.280
as possible homes for life.
709
00:27:40.440 --> 00:27:42.560
Anna: Well, that wraps up today's edition of
710
00:27:42.560 --> 00:27:45.320
Astronomy Daily. From solar storms to
711
00:27:45.320 --> 00:27:48.120
baby stars, Chinese space technology to
712
00:27:48.120 --> 00:27:51.090
hidden magma oceans on distant worlds, it's
713
00:27:51.090 --> 00:27:52.890
been quite a journey through the cosmos.
714
00:27:52.970 --> 00:27:55.570
Avery: It really has. And remember, if you're in the
715
00:27:55.570 --> 00:27:58.090
northern tier states of the USA or Canada
716
00:27:58.250 --> 00:28:00.170
tonight, keep an eye on the sky for those
717
00:28:00.170 --> 00:28:02.530
auroras from that solar storm. Could be quite
718
00:28:02.530 --> 00:28:02.890
a show.
719
00:28:02.890 --> 00:28:05.090
Anna: Thanks for joining us for the latest space
720
00:28:05.090 --> 00:28:07.610
and astronomy news delivered fresh every day.
721
00:28:07.770 --> 00:28:10.290
Be sure to subscribe to Astronomy Daily. You
722
00:28:10.290 --> 00:28:13.290
can find us on our website@astronomydaily,IO
723
00:28:13.370 --> 00:28:15.490
or search for us on your favorite podcast
724
00:28:15.490 --> 00:28:17.720
platform. Until next time, keep looking up
725
00:28:17.720 --> 00:28:18.800
Clear skies, everyone.