Jan. 20, 2026

Solar Storm Hits Early! Plus China's Reusable Rockets & Exoplanet Magnetic Shields

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.

WEBVTT

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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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00:13:30.170 --> 00:13:33.090
schedules can slip. But if everything stays

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00:13:33.090 --> 00:13:35.570
on track, we could see Xuntian launching on a

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long March 5th B rocket sometime in the

340
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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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00:13:57.810 --> 00:14:00.370
complex. The Hubble Space Telescope has

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00:14:00.370 --> 00:14:02.730
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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00:14:11.640 --> 00:14:14.280
protostars, right? Stars that haven't quite

356
00:14:14.280 --> 00:14:15.000
grown up yet?

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Avery: That's right. Protostars are young stellar

358
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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.

365
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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

368
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that shape their surroundings in dramatic

369
00:14:41.880 --> 00:14:44.880
ways. These jets and winds carve out bubbles

370
00:14:44.880 --> 00:14:47.320
and caverns in the surrounding gas. And

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00:14:47.320 --> 00:14:49.480
astrophysicists have been trying to better

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00:14:49.480 --> 00:14:51.120
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

375
00:14:56.200 --> 00:14:58.920
molecular cloud first forms a disk around the

376
00:14:58.920 --> 00:15:01.680
protostar. Not all of that material makes it

377
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onto the star itself. Some gets accelerated

378
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to high speeds along the star's magnetic

379
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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.

382
00:15:14.750 --> 00:15:17.030
Avery: That's a good analogy. And in addition to

383
00:15:17.030 --> 00:15:19.830
these focused jets, protostars also produce

384
00:15:19.830 --> 00:15:22.510
wide angle stellar winds that flow in all

385
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directions. These winds from young stars are

386
00:15:25.310 --> 00:15:27.510
actually far more powerful than the solar

387
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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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00:15:32.520 --> 00:15:35.040
Avery: The three new images show protostars at

391
00:15:35.040 --> 00:15:37.840
different stages, all in the Orion molecular

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complex. You can actually see the cavernous

393
00:15:40.520 --> 00:15:42.720
shapes these young stars have carved out from

394
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the surrounding gas. It's quite striking

395
00:15:44.960 --> 00:15:47.560
visually, these dark, sometimes intricate

396
00:15:47.560 --> 00:15:49.720
structures against the glowing background of

397
00:15:49.720 --> 00:15:50.440
the nebula.

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00:15:50.520 --> 00:15:52.840
Anna: But there was a surprising finding in the

399
00:15:52.840 --> 00:15:53.800
research, wasn't there?

400
00:15:54.200 --> 00:15:56.200
Avery: Yes, and it challenges some assumptions.

401
00:15:56.630 --> 00:15:58.830
Researchers found that the cavities carved by

402
00:15:58.830 --> 00:16:01.470
these jetson winds didn't grow larger as the

403
00:16:01.470 --> 00:16:03.430
stars moved through their later formation

404
00:16:03.430 --> 00:16:06.030
stages. You might expect the cavities to keep

405
00:16:06.030 --> 00:16:08.190
expanding over time, but that's not what they

406
00:16:08.190 --> 00:16:08.790
observed.

407
00:16:09.270 --> 00:16:10.710
Anna: So what does that tell us?

408
00:16:10.950 --> 00:16:13.270
Avery: Well, the Orion molecular cloud has been

409
00:16:13.270 --> 00:16:15.910
experiencing a declining star formation rate.

410
00:16:15.990 --> 00:16:18.590
And these protostars also have lower rates of

411
00:16:18.590 --> 00:16:21.110
mass accretion over time. Scientists

412
00:16:21.110 --> 00:16:22.790
initially thought maybe this could be

413
00:16:22.790 --> 00:16:25.110
attributed to the jets and winds carving out

414
00:16:25.110 --> 00:16:27.740
all the available gas. But the new findings

415
00:16:27.740 --> 00:16:30.500
suggest that's not the case. The cavity sizes

416
00:16:30.500 --> 00:16:31.780
weren't the limiting factor.

417
00:16:32.180 --> 00:16:34.580
Anna: So something else is controlling the star

418
00:16:34.580 --> 00:16:35.380
formation rate.

419
00:16:35.460 --> 00:16:37.860
Avery: Exactly. There must be other factors at play

420
00:16:37.860 --> 00:16:40.580
in regulating how quickly stars form and grow

421
00:16:40.580 --> 00:16:43.260
in this region. It's a reminder that even in

422
00:16:43.260 --> 00:16:45.740
well studied regions like Orion, we're still

423
00:16:45.740 --> 00:16:47.900
learning the details of how star formation

424
00:16:47.900 --> 00:16:48.340
works.

425
00:16:48.500 --> 00:16:50.780
Anna: I love that these images aren't just pretty

426
00:16:50.780 --> 00:16:53.140
pictures. They're revealing actual physics.

427
00:16:53.530 --> 00:16:55.530
Avery: That's what makes astronomy so exciting.

428
00:16:55.770 --> 00:16:58.170
Every observation adds a piece of the puzzle.

429
00:16:58.410 --> 00:17:00.090
In this case, we're learning that the

430
00:17:00.090 --> 00:17:02.330
feedback from young stars through their jets

431
00:17:02.330 --> 00:17:04.850
and winds. While dramatic and visually

432
00:17:04.850 --> 00:17:07.610
spectacular, might not be the main factor

433
00:17:07.610 --> 00:17:09.290
controlling star formation in the region.

434
00:17:09.530 --> 00:17:11.610
Anna: It's also interesting to think about our own

435
00:17:11.610 --> 00:17:13.570
sun going through this phase billions of

436
00:17:13.570 --> 00:17:14.090
years ago.

437
00:17:14.410 --> 00:17:17.170
Avery: Absolutely. When the sun was young, it was in

438
00:17:17.170 --> 00:17:19.410
a cluster with its siblings, probably in a

439
00:17:19.410 --> 00:17:21.950
molecular cloud, much like Orion. It would

440
00:17:21.950 --> 00:17:24.510
have had these same powerful jets and winds

441
00:17:24.510 --> 00:17:26.590
shaping the gas and dust around it.

442
00:17:26.910 --> 00:17:29.510
Eventually the molecular cloud dispersed, the

443
00:17:29.510 --> 00:17:32.150
star cluster broke up and the sun ended up as

444
00:17:32.150 --> 00:17:34.030
the solitary star we know today.

445
00:17:34.190 --> 00:17:36.270
Anna: Orion is close enough that we can study these

446
00:17:36.270 --> 00:17:38.550
processes in detail, which is really lucky

447
00:17:38.550 --> 00:17:39.390
for astronomers.

448
00:17:39.630 --> 00:17:42.590
Avery: Very lucky. At about 1350

449
00:17:42.590 --> 00:17:44.710
light years away, it's one of the nearest

450
00:17:44.710 --> 00:17:47.510
large star forming regions. We can resolve

451
00:17:47.510 --> 00:17:49.790
individual protostars and their surrounding

452
00:17:49.790 --> 00:17:52.070
structures, which gives us insights we can

453
00:17:52.070 --> 00:17:54.010
apply to understanding star formation

454
00:17:54.010 --> 00:17:55.930
throughout the galaxy and beyond.

455
00:17:56.170 --> 00:17:58.650
Anna: Alright, let's shift from natural cosmic

456
00:17:58.650 --> 00:18:00.970
phenomena to human made space activities.

457
00:18:01.290 --> 00:18:03.290
We've got a busy week of launches coming up.

458
00:18:03.290 --> 00:18:03.850
Avery.

459
00:18:03.930 --> 00:18:06.650
Avery: We do indeed. Seven launches from six

460
00:18:06.650 --> 00:18:08.850
different sites across the globe. Let's run

461
00:18:08.850 --> 00:18:09.290
through them.

462
00:18:09.370 --> 00:18:11.450
Anna: The week actually started this morning with a

463
00:18:11.450 --> 00:18:12.570
Chinese launch, correct?

464
00:18:12.730 --> 00:18:15.250
Avery: That's right. A uh, Chang Zhang 12 rocket,

465
00:18:15.250 --> 00:18:18.090
also known as Long March 12, lifted off

466
00:18:18.090 --> 00:18:21.090
from Commercial Launch Complex 2 at Wenchang

467
00:18:21.090 --> 00:18:24.070
Space Launch Site in Hainan, China. This was

468
00:18:24.070 --> 00:18:26.670
at 7:48 UTC. Carrying nine

469
00:18:26.670 --> 00:18:29.550
SatNet satellites to low Earth orbit. The

470
00:18:29.550 --> 00:18:32.190
CZ12 can lift about 12,000

471
00:18:32.270 --> 00:18:34.430
kilograms to LEO. And this was a

472
00:18:34.430 --> 00:18:36.470
demonstration of China's commercial launch

473
00:18:36.470 --> 00:18:36.990
capabilities.

474
00:18:37.390 --> 00:18:38.910
Anna: Moving on to tomorrow.

475
00:18:38.910 --> 00:18:41.710
Avery: What do we have tomorrow? January 21st

476
00:18:41.790 --> 00:18:43.990
we have Rocket Lab launching from New

477
00:18:43.990 --> 00:18:46.310
Zealand. Their Electron rocket will be

478
00:18:46.310 --> 00:18:48.910
carrying two satellites for open Cosmos as

479
00:18:48.910 --> 00:18:51.230
part of a secure broadband constellation

480
00:18:51.230 --> 00:18:54.050
being built in the uk. The mission is called

481
00:18:54.050 --> 00:18:57.050
the Cosmos will see you now. And liftoff is

482
00:18:57.050 --> 00:18:59.810
scheduled for 11:09 UTC. From their

483
00:18:59.810 --> 00:19:01.890
facility on the Mahia Peninsula.

484
00:19:01.890 --> 00:19:04.650
Anna: Rocket Lab has really established a solid

485
00:19:04.650 --> 00:19:05.890
cadence with Electron.

486
00:19:05.970 --> 00:19:08.729
Avery: They have. This will be Electron's 80th

487
00:19:08.729 --> 00:19:11.130
mission. That's a remarkable achievement for

488
00:19:11.130 --> 00:19:13.930
a small rocket. The vehicle has proven itself

489
00:19:13.930 --> 00:19:16.570
reliable and capable, especially for these

490
00:19:16.570 --> 00:19:18.610
small satellite constellation deployments.

491
00:19:18.770 --> 00:19:21.010
Anna: It's Wednesday. That gets particularly

492
00:19:21.010 --> 00:19:23.250
interesting with the Isar Aerospace launch.

493
00:19:23.660 --> 00:19:26.420
Avery: Yes, this is Isar's second attempt to launch

494
00:19:26.420 --> 00:19:29.020
their Spectrum rocket from the Andoya rocket

495
00:19:29.020 --> 00:19:32.020
range in Norway. The mission is called Onward

496
00:19:32.020 --> 00:19:34.300
and Upward, which is fitting given that their

497
00:19:34.300 --> 00:19:37.020
first attempt in March 2025 failed

498
00:19:37.020 --> 00:19:39.100
shortly after liftoff due to an engine issue.

499
00:19:39.339 --> 00:19:40.540
Anna: What's different this time?

500
00:19:40.700 --> 00:19:42.620
Avery: Well, they've been investigating what went

501
00:19:42.620 --> 00:19:44.420
wrong on that first flight and making

502
00:19:44.420 --> 00:19:47.100
refinements. Spectrum is a two stage

503
00:19:47.100 --> 00:19:49.460
rocket Powered by Aquila engines using

504
00:19:49.460 --> 00:19:52.290
propane and liquid oxygen, it's designed for

505
00:19:52.290 --> 00:19:54.370
the satellite Constellation market and can

506
00:19:54.370 --> 00:19:56.810
lift about a thousand kilograms to leo.

507
00:19:57.050 --> 00:19:59.210
They're carrying several cubesats for the

508
00:19:59.210 --> 00:20:01.370
European Space Agency's Boost program.

509
00:20:01.610 --> 00:20:03.610
Anna: So fingers crossed for ISAR on Wednesday.

510
00:20:03.690 --> 00:20:04.410
What else?

511
00:20:04.570 --> 00:20:07.450
Avery: Wednesday is also when SpaceX has their first

512
00:20:07.450 --> 00:20:09.570
Falcon 9 launch of the week. They're

513
00:20:09.570 --> 00:20:11.890
launching 24 Starlink satellites from

514
00:20:11.890 --> 00:20:14.490
Vandenberg Space Force Base in California.

515
00:20:14.810 --> 00:20:17.490
Liftoff is currently targeted for 2:43

516
00:20:17.490 --> 00:20:20.290
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.