Jan. 31, 2026

Artemis Delays, Blue Origin’s Lunar Pivot, and Life’s Building Blocks in Space

Artemis Delays, Blue Origin’s Lunar Pivot, and Life’s Building Blocks in Space
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Artemis Delays, Blue Origin’s Lunar Pivot, and Life’s Building Blocks in Space

Join hosts Anna and Avery for Saturday's cosmic roundup! NASA's Artemis 2 wet dress rehearsal faces weather delays, pushing the historic lunar mission to April 2026. Blue Origin announces a major strategic shift, pausing space tourism for two years to focus on their Blue Moon lunar lander program. We explore million-mile-per-hour cosmic winds racing through a "magnetic superhighway" in colliding galaxies, investigate a mysterious object sending unexplained signals across the galaxy, discover why Tatooine-style planets might be more common than expected, and celebrate a groundbreaking first - the detection of ethanolamine, a molecule critical to cell membranes, in interstellar space.

**Episode Keywords:** Artemis 2, NASA, Blue Origin, New Shepard, space tourism, lunar lander, cosmic winds, galaxy merger, IC 1623, mysterious signals, radio astronomy, circumbinary planets, binary stars, ethanolamine, astrobiology, interstellar molecules, space exploration, Kennedy Space Center

**Detailed Chapter Markers:**

- [00:00] Introduction & Episode Overview

- [02:15] NASA Artemis 2 Wet Dress Rehearsal Delay

- [06:45] Blue Origin Pauses Space Tourism for Lunar Ambitions

- [11:20] Million-MPH Cosmic Winds in Magnetic Superhighway

- [16:30] Mysterious Object Sending Unexplained Galactic Signals

- [21:15] Tatooine Planets More Common Than Expected

- [26:00] Life-Critical Molecule Detected in Interstellar Space

- [30:45] Episode Wrap-Up & Closing


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This episode includes AI-generated content.

Episode link: https://play.headliner.app/episode/31430985?utm_source=youtube

00:00 - Introduction & Episode Overview

02:15 - NASA Artemis 2 Wet Dress Rehearsal Delay

06:45 - Blue Origin Pauses Space Tourism for Lunar Ambitions

11:20 - Million-MPH Cosmic Winds in Magnetic Superhighway

16:30 - Mysterious Object Sending Unexplained Galactic Signals

21:15 - Tatooine Planets More Common Than Expected

26:00 - Life-Critical Molecule Detected in Interstellar Space

WEBVTT
Kind: captions
Language: en

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Welcome to [music] Astronomy Daily, your


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source for the latest space and


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astronomy news. [music] I'm Anna.


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>> And I'm Avery. Thanks for joining us on


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this Saturday, January 31st, 2026.


00:00:12.080 --> 00:00:13.910
>> We've got [music] a fascinating lineup


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today covering everything from NASA's


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Aremis program updates to groundbreaking


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discoveries [music] in the search for


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life beyond Earth. Avery, what's on the


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agenda?


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>> Well, Anna, we're kicking things off


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with some news from NASA's [music]


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Aremis 2 mission. There's been a delay


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in critical testing due to some


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unexpected [music] weather challenges.


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Then we'll dive into Blue Origin's


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strategic shift as [music] they pause


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their space tourism program for at least


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2 years. After that, [music] we're


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looking up at some truly cosmic


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phenomena. Million mileph winds racing


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through [music] colliding galaxies and a


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mysterious object sending powerful


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signals across space that has [music]


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astronomers scratching their heads.


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We'll also explore some surprising


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findings about Tatooine style planets


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orbiting binary stars and wrap up with


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an exciting [music] discovery.


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Scientists have detected a molecule


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critical to life in interstellar [music]


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space for the very first time.


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>> Quite the journey today. Let's get


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started.


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>> Ready when you are.


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>> All right, Avery. Let's start with


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NASA's Aremis program. I understand old


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man Winter has thrown a wrench into


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their testing schedule.


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>> He certainly has, Anna. NASA has been


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forced to delay a critical fueling test


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for the Aremis 2 mission due to below


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freezing temperatures at Kennedy Space


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Center in Florida. The wet dress


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rehearsal was originally scheduled for


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January 27th, but those unexpected cold


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temperatures put it on ice, so to speak.


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>> I see what you did there. But seriously,


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what exactly is this wet dress


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rehearsal? And why is it so important?


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>> Great question. The wet dress rehearsal


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is essentially a full practice run of


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launch day procedures minus the actual


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launch. The team loads the massive space


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launch system rocket with over 700,000


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gallons of super cold liquid hydrogen


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and liquid oxygen propellants, runs


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through all the countdown procedures,


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and then drains everything back out.


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It's the ultimate dress rehearsal before


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the real show. So, they're basically


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making sure all the plumbing works and


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everyone knows their roles when the


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clock is ticking down. What happened


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with the weather that caused the delay?


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>> Well, Florida experienced some unusually


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cold conditions. We're talking about


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freezing temperatures that persisted for


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several days. The problem is that


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loading these cryogenic propellants in


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freezing conditions creates additional


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safety risks and potential technical


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issues. NASA's priority is always safety


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first, so they made the call to


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postpone.


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>> Smart move. When are they planning to


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try again?


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>> The space launch system is now set to


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roll out to launchpad 39B on February


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5th with the wet dress rehearsal


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rescheduled for February 8th. This means


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the Aremis 2 launch is now no earlier


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than April 2026, which is a shift from


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the previous March target.


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>> For our listeners who might not be


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following every detail of Artemis,


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remind us what makes Artemis 2 so


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significant.


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>> Hannah, Artemis 2 is absolutely


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historic. This will be the first crude


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mission beyond low Earth orbit in over


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50 years, basically since the Apollo


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program ended. Four astronauts will fly


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around the moon, testing all the systems


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and procedures that will eventually


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support landing astronauts back on the


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lunar surface during Artemis 3.


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>> It's wild to think we haven't sent


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humans beyond Earth orbit in 5 decades.


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Who's on the crew? The crew includes


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NASA astronauts Reed Weisman, Victor


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Glover, and Christina Ko along with


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Canadian Space Agency astronaut Jeremy


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Hansen. Victor Glover will make history


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as the first person of color to travel


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beyond low Earth orbit. And Christina Ko


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will become the first woman to do so.


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>> That's incredible. Even with this delay,


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April 2026 is right around the corner.


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The wait is almost over.


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>> Absolutely. And honestly, a few weeks


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delay to ensure everything is perfect is


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well worth it when you're pioneering the


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return of human deep space exploration.


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>> Speaking of human space flight, let's


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shift gears to Blue Origin. They're


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making some significant changes to their


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program, aren't they, Avery?


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>> They sure are, Anna. Blue Origin has


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announced they're hitting pause on their


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New Shepard space tourism flights for at


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least 2 years. This is a major strategic


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shift as they refocus their resources on


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NASA's Aremis program and the


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development of their lunar lander.


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>> 2 years is a substantial pause. What's


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driving this decision?


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>> It all comes down to their Blue Moon


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lunar lander program. Blue Origin won a


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contract from NASA worth potentially up


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to $3.6 billion to develop a human


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landing system for the Aremis missions.


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They're planning an uncrrewed


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demonstration mission to the moon in


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2028. And that's requiring a massive


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concentration of their engineering


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talent and resources.


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>> So they're essentially choosing moon


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landings over suborbital tourism


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flights. That seems like a pretty clear


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indication of where they see the bigger


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opportunity.


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>> Exactly. And it's worth noting that Blue


00:05:10.720 --> 00:05:12.710
Origin has already conducted eight


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successful New Shepard tourism flights


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since July 2021, carrying 43 people past


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the Carmen line, the internationally


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recognized boundary of space at 100 km


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altitude. So they've proven the concept


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and the technology.


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>> I remember the excitement around those


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early flights. What exactly will


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passengers experience on a New Shepard


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flight? It's a roughly 11-minute journey


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where passengers experience about 3


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minutes of weightlessness at the top of


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the ark. The capsule has massive


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windows, the largest ever flown in


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space, giving spectacular views of


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Earth's curvature and the blackness of


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space. It's suborbital, meaning you go


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up and come right back down, but you


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definitely cross into space.


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>> And this pause is specifically for the


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tourism program. What about other New


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Shepard missions?


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>> Good distinction, Anna. New Shepard will


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continue flying cargo and research


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missions. Blue Origin has committed to


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conducting at least two cargo flights


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each year during this tourism pause.


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These missions carry scientific


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experiments and payloads for various


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customers, including NASA.


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>> What about their ticket sales? I imagine


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people have already paid for future


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flights.


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>> Yes, and Blue Origin says they'll be


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contacting customers who've already


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purchased tickets to discuss their


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options. They haven't specified how many


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people are affected, but they've


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emphasized this is a temporary pause,


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not an end to the program.


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>> It's interesting timing, isn't it? Just


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as several companies are getting into


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the space tourism business, Blue Origin


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is stepping back, at least temporarily.


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>> It really shows you the scale of the


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lunar lander challenge. Building a


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spacecraft that can safely land humans


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on the moon and return them to lunar


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orbit is orders of magnitude more


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complex than a suborbital tourism op.


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Blue Origin is betting their future on


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being a key player in the new era of


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space exploration.


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>> And with that NASA contract potentially


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worth $3.6 billion, it's not hard to see


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why they're prioritizing it.


00:07:10.479 --> 00:07:12.950
>> Exactly. This is Blue Origin's moonshot,


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both literally and figuratively. If they


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can deliver a successful lunar lander,


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it positions them as a major player in


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the new era of space exploration. From


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human space exploration to cosmic


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phenomena, let's talk about something


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happening on a scale that's almost


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impossible to comprehend. Avery, tell us


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about these million mileph winds racing


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through space.


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>> Anna, this is absolutely mindblowing.


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Astronomers have discovered cosmic winds


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traveling at over 1.1 million mph.


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That's roughly 500 kilometers per


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second, racing through what they're


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calling a magnetic superighway between


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two colliding galaxies.


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>> A magnetic superhighway in space. That


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sounds like something out of science


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fiction. Where is this happening? This


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incredible phenomenon is occurring in a


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system called IC1623


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which is actually two galaxies in the


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process of merging together located


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about 275


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million light years from Earth in the


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constellation Cedus. These galaxies are


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in the late stages of a cosmic collision


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and it's creating some extraordinary


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physics.


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>> Walk us through what's actually


00:08:27.919 --> 00:08:29.909
happening here. How do galaxies


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colliding create these super fast winds?


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>> When galaxies merge, their gravitational


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interactions trigger massive bursts of


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star formation. We're talking thousands


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of stars being born. These newborn stars


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live fast and die young, creating


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powerful stellar winds and supernova


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explosions. All of this activity


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generates enormous amounts of energy


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that drives material outward at


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incredible speeds. and the magnetic


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superhighway. What role does that play?


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>> Here's where it gets really fascinating.


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The team from the University of


00:09:05.440 --> 00:09:07.670
Hershshire discovered that magnetic


00:09:07.680 --> 00:09:09.750
fields are actually channeling these


00:09:09.760 --> 00:09:11.990
winds, creating what they call a


00:09:12.000 --> 00:09:13.910
superighway that connects the two


00:09:13.920 --> 00:09:16.389
galactic cores. Think of it like a


00:09:16.399 --> 00:09:18.870
cosmic interstate highway system, but


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instead of cars, you've got superheated


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gas screaming along at speeds that make


00:09:23.680 --> 00:09:25.750
Earth's fastest spacecraft look like


00:09:25.760 --> 00:09:27.430
they're standing still.


00:09:27.440 --> 00:09:30.150
>> That's an amazing image. How did they


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detect something like this?


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>> They used the Arakama Large Millm Array,


00:09:35.040 --> 00:09:37.430
ALMA, in Chile, which is specifically


00:09:37.440 --> 00:09:39.829
designed to observe cold gas and dust in


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the universe. What they found was


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unexpected. The magnetic field structure


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doesn't just randomly radiate outward


00:09:46.880 --> 00:09:49.750
like many galactic winds do. Instead,


00:09:49.760 --> 00:09:52.310
it's highly organized, creating this


00:09:52.320 --> 00:09:54.550
directed pathway between the galactic


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centers.


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>> Why is this discovery so significant?


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What does it tell us about galaxy


00:10:00.000 --> 00:10:01.509
evolution?


00:10:01.519 --> 00:10:03.750
>> This is crucial for understanding how


00:10:03.760 --> 00:10:06.630
galaxies grow and evolve. These powerful


00:10:06.640 --> 00:10:08.710
outflows, what astronomers call


00:10:08.720 --> 00:10:11.350
feedback, can actually regulate star


00:10:11.360 --> 00:10:13.829
formation by expelling the gas and dust


00:10:13.839 --> 00:10:16.069
that would otherwise collapse to form


00:10:16.079 --> 00:10:18.470
new stars. It's like a pressure release


00:10:18.480 --> 00:10:20.630
valve for galaxies. Too much star


00:10:20.640 --> 00:10:22.630
formation can blow away the material


00:10:22.640 --> 00:10:24.949
needed to make more stars, which can


00:10:24.959 --> 00:10:27.430
eventually slow down or even halt a


00:10:27.440 --> 00:10:28.790
galaxy's growth.


00:10:28.800 --> 00:10:31.430
>> So, galaxies regulate their own growth


00:10:31.440 --> 00:10:33.590
through these winds. That's a pretty


00:10:33.600 --> 00:10:36.230
elegant self-limiting system.


00:10:36.240 --> 00:10:40.069
>> It really is. And what makes IC1623


00:10:40.079 --> 00:10:42.069
particularly interesting is that we're


00:10:42.079 --> 00:10:44.389
seeing this process in action during a


00:10:44.399 --> 00:10:47.910
galaxy merger. When galaxies collide, we


00:10:47.920 --> 00:10:50.069
see the most extreme versions of these


00:10:50.079 --> 00:10:52.230
processes. The most intense star


00:10:52.240 --> 00:10:55.110
formation, the most powerful winds, the


00:10:55.120 --> 00:10:57.509
strongest magnetic fields. It's like


00:10:57.519 --> 00:10:59.430
watching galaxy evolution. and fast


00:10:59.440 --> 00:11:00.230
forward.


00:11:00.240 --> 00:11:04.069
>> What do we think the fate of IC1623


00:11:04.079 --> 00:11:04.790
will be?


00:11:04.800 --> 00:11:06.790
>> Eventually, these two galaxies will


00:11:06.800 --> 00:11:09.269
completely merge into a single larger


00:11:09.279 --> 00:11:11.509
galaxy. The current burst of star


00:11:11.519 --> 00:11:13.750
formation will eventually exhaust much


00:11:13.760 --> 00:11:15.910
of the available gas. And what we're


00:11:15.920 --> 00:11:18.389
looking at now, this spectacular phase


00:11:18.399 --> 00:11:20.949
of cosmic winds and magnetic highways


00:11:20.959 --> 00:11:23.670
will fade. But the combined galaxy will


00:11:23.680 --> 00:11:25.829
carry the imprint of this violent event


00:11:25.839 --> 00:11:28.150
in its structure and stellar populations


00:11:28.160 --> 00:11:30.310
for billions of years to come.


00:11:30.320 --> 00:11:31.829
>> It's humbling to think that we're


00:11:31.839 --> 00:11:33.829
witnessing something that takes millions


00:11:33.839 --> 00:11:36.550
of years to play out, just captured in a


00:11:36.560 --> 00:11:37.910
snapshot.


00:11:37.920 --> 00:11:40.310
>> Absolutely. And every time we point our


00:11:40.320 --> 00:11:42.870
telescopes at merging galaxies, we learn


00:11:42.880 --> 00:11:44.710
something new about the forces shaping


00:11:44.720 --> 00:11:47.350
the universe's largest structures.


00:11:47.360 --> 00:11:49.350
Speaking of pointing our telescopes at


00:11:49.360 --> 00:11:51.269
the universe and finding surprises,


00:11:51.279 --> 00:11:53.269
Avery, we need to talk about this


00:11:53.279 --> 00:11:55.350
mysterious object that's been sending


00:11:55.360 --> 00:11:57.829
powerful signals across the galaxy. The


00:11:57.839 --> 00:12:00.389
headline says it's unlike anything we


00:12:00.399 --> 00:12:01.750
have seen before.


00:12:01.760 --> 00:12:04.310
>> That's not just hype, Anna. Astronomers


00:12:04.320 --> 00:12:06.150
have discovered something truly


00:12:06.160 --> 00:12:08.870
puzzling. A cosmic object that's


00:12:08.880 --> 00:12:11.509
periodically sending out intense radio


00:12:11.519 --> 00:12:14.150
signals. And it doesn't fit into any


00:12:14.160 --> 00:12:16.069
category of known astronomical


00:12:16.079 --> 00:12:18.230
phenomena. It's one of those discoveries


00:12:18.240 --> 00:12:19.990
that makes you rethink what you thought


00:12:20.000 --> 00:12:20.790
you knew.


00:12:20.800 --> 00:12:23.750
>> Okay, you've got my attention. What


00:12:23.760 --> 00:12:25.590
exactly are we dealing with here?


00:12:25.600 --> 00:12:28.230
>> The object sends out extremely bright


00:12:28.240 --> 00:12:31.829
radio pulses that last about 30 to 300


00:12:31.839 --> 00:12:34.069
seconds. That's up to 5 minutes per


00:12:34.079 --> 00:12:36.710
pulse. And these pulses occur roughly


00:12:36.720 --> 00:12:39.509
every 2.9 hours with remarkable


00:12:39.519 --> 00:12:42.310
regularity. What makes this so unusual


00:12:42.320 --> 00:12:44.870
is the combination of that long period


00:12:44.880 --> 00:12:46.550
and the duration of the pulses


00:12:46.560 --> 00:12:47.509
themselves.


00:12:47.519 --> 00:12:49.509
>> When you say it doesn't fit known


00:12:49.519 --> 00:12:51.910
categories, what are the usual suspects


00:12:51.920 --> 00:12:53.750
for objects that send out regular


00:12:53.760 --> 00:12:55.110
signals like this?


00:12:55.120 --> 00:12:57.590
>> Great question. The two most common


00:12:57.600 --> 00:13:00.069
sources of periodic radio signals are


00:13:00.079 --> 00:13:03.350
pulsars and magnetars. Pulsars are


00:13:03.360 --> 00:13:05.430
rapidly spinning neutron stars that


00:13:05.440 --> 00:13:07.750
sweep beams of radiation across space


00:13:07.760 --> 00:13:10.150
like a cosmic lighthouse. But they


00:13:10.160 --> 00:13:11.829
typically pulse on the order of


00:13:11.839 --> 00:13:15.110
milliseconds to seconds, not hours. And


00:13:15.120 --> 00:13:17.190
their individual pulses are brief,


00:13:17.200 --> 00:13:19.750
usually milliseconds, not minutes.


00:13:19.760 --> 00:13:22.470
>> So this object is pulsing way too slowly


00:13:22.480 --> 00:13:24.150
to be a normal pulsar.


00:13:24.160 --> 00:13:26.870
>> Exactly. And the pulses last far too


00:13:26.880 --> 00:13:29.910
long. Magnetars, which are neutron stars


00:13:29.920 --> 00:13:31.910
with incredibly powerful magnetic


00:13:31.920 --> 00:13:34.310
fields, can sometimes produce longer


00:13:34.320 --> 00:13:36.870
period signals than regular pulsars, but


00:13:36.880 --> 00:13:39.030
even they don't typically operate on a


00:13:39.040 --> 00:13:41.509
3-hour cycle with multi-minute pulse


00:13:41.519 --> 00:13:42.310
durations.


00:13:42.320 --> 00:13:44.310
>> Have astronomers proposed any theories


00:13:44.320 --> 00:13:45.670
about what this could be?


00:13:45.680 --> 00:13:47.350
>> There are a few possibilities being


00:13:47.360 --> 00:13:49.750
investigated. One idea is that it could


00:13:49.760 --> 00:13:51.990
be a white dwarf in a binary system,


00:13:52.000 --> 00:13:53.829
which is two stars orbiting each other


00:13:53.839 --> 00:13:56.389
where one is a white dwarf remnant. The


00:13:56.399 --> 00:13:58.470
interaction between the two stars can


00:13:58.480 --> 00:14:00.629
potentially generate these periodic


00:14:00.639 --> 00:14:03.110
radio emissions. Another possibility is


00:14:03.120 --> 00:14:05.590
that we're seeing some kind of unusual


00:14:05.600 --> 00:14:08.069
magnetar or pulsar that operates


00:14:08.079 --> 00:14:09.670
differently than the ones we studied


00:14:09.680 --> 00:14:10.389
before.


00:14:10.399 --> 00:14:13.189
>> When was this object discovered and how?


00:14:13.199 --> 00:14:15.189
>> The discovery was made using radio


00:14:15.199 --> 00:14:17.509
telescope observations. And what's


00:14:17.519 --> 00:14:19.350
particularly intriguing is that the


00:14:19.360 --> 00:14:21.110
signals are powerful enough to be


00:14:21.120 --> 00:14:23.990
detected across vast distances. The


00:14:24.000 --> 00:14:25.990
exact distance to this object is still


00:14:26.000 --> 00:14:27.990
being determined, but the fact that we


00:14:28.000 --> 00:14:31.030
can detect such clear periodic signals


00:14:31.040 --> 00:14:33.509
suggests it's either relatively close in


00:14:33.519 --> 00:14:35.750
cosmic terms or it's putting out


00:14:35.760 --> 00:14:37.590
tremendous amounts of energy.


00:14:37.600 --> 00:14:39.910
>> This reminds me of those fast radio


00:14:39.920 --> 00:14:42.470
bursts we've heard about, brief, intense


00:14:42.480 --> 00:14:44.870
radio signals from across the universe.


00:14:44.880 --> 00:14:46.230
Is this related?


00:14:46.240 --> 00:14:48.629
>> That's a natural comparison, Anna. But


00:14:48.639 --> 00:14:51.750
fast radio bursts, FRBs, are different.


00:14:51.760 --> 00:14:53.910
They're much briefer. typically lasting


00:14:53.920 --> 00:14:56.790
milliseconds, though some do repeat.


00:14:56.800 --> 00:14:59.030
This object's behavior is more periodic


00:14:59.040 --> 00:15:01.509
and predictable with much longer pulse


00:15:01.519 --> 00:15:03.910
durations. It's almost like comparing a


00:15:03.920 --> 00:15:06.470
strobe light to a slowly rotating search


00:15:06.480 --> 00:15:07.110
light.


00:15:07.120 --> 00:15:09.110
>> What's the next step for studying this


00:15:09.120 --> 00:15:10.629
mysterious object?


00:15:10.639 --> 00:15:12.790
>> Astronomers will be conducting follow-up


00:15:12.800 --> 00:15:14.550
observations across multiple


00:15:14.560 --> 00:15:16.710
wavelengths, not just radio, but also


00:15:16.720 --> 00:15:19.750
optical, X-ray, and potentially others.


00:15:19.760 --> 00:15:21.910
They want to determine exactly where it


00:15:21.920 --> 00:15:24.629
is, measure its properties in detail,


00:15:24.639 --> 00:15:26.629
and hopefully identify what type of


00:15:26.639 --> 00:15:28.790
object it is. Sometimes you need


00:15:28.800 --> 00:15:30.710
multiple types of observations to build


00:15:30.720 --> 00:15:31.910
a complete picture.


00:15:31.920 --> 00:15:34.230
>> Do discoveries like this happen often


00:15:34.240 --> 00:15:35.910
where we find something that just


00:15:35.920 --> 00:15:38.230
doesn't fit our existing models.


00:15:38.240 --> 00:15:39.670
>> More often than you might think,


00:15:39.680 --> 00:15:42.150
actually, the universe keeps surprising


00:15:42.160 --> 00:15:44.389
us. Every major improvement in our


00:15:44.399 --> 00:15:46.310
observing technology reveals new


00:15:46.320 --> 00:15:48.389
phenomena we didn't predict.


00:15:48.399 --> 00:15:50.949
Radioastronomy in particular has a


00:15:50.959 --> 00:15:53.189
history of unexpected discoveries.


00:15:53.199 --> 00:15:55.350
Pulsars themselves were a complete


00:15:55.360 --> 00:15:57.030
surprise when they were first detected


00:15:57.040 --> 00:15:58.710
in 1967.


00:15:58.720 --> 00:16:00.790
>> Could this turn out to be a whole new


00:16:00.800 --> 00:16:03.430
class of astronomical objects?


00:16:03.440 --> 00:16:05.910
>> That's definitely possible. If follow-up


00:16:05.920 --> 00:16:08.310
observations confirmed that this truly


00:16:08.320 --> 00:16:11.030
doesn't fit into any existing category,


00:16:11.040 --> 00:16:13.269
it could indeed represent something new.


00:16:13.279 --> 00:16:15.350
Of course, it might also turn out to be


00:16:15.360 --> 00:16:17.590
an extreme example of a known type of


00:16:17.600 --> 00:16:20.310
object, just operating in a regime we


00:16:20.320 --> 00:16:22.389
haven't observed before. Either way,


00:16:22.399 --> 00:16:24.069
it's expanding our understanding of


00:16:24.079 --> 00:16:26.069
what's possible in the universe.


00:16:26.079 --> 00:16:27.829
>> I love that we're still finding things


00:16:27.839 --> 00:16:29.990
that make astronomers say we've never


00:16:30.000 --> 00:16:31.749
seen anything like this before.


00:16:31.759 --> 00:16:34.230
>> Me, too, Anna. It reminds us how much we


00:16:34.240 --> 00:16:36.470
still have to learn about the cosmos.


00:16:36.480 --> 00:16:38.790
Sticking with unexpected discoveries,


00:16:38.800 --> 00:16:40.949
let's talk about planets that orbit two


00:16:40.959 --> 00:16:44.069
suns. Tatooine style worlds. Avery, I


00:16:44.079 --> 00:16:45.509
understand these aren't as rare as


00:16:45.519 --> 00:16:47.910
scientists once thought. That's right,


00:16:47.920 --> 00:16:50.230
Anna. New research is challenging our


00:16:50.240 --> 00:16:53.030
assumptions about circumbinary planets.


00:16:53.040 --> 00:16:54.790
That's the technical term for planets


00:16:54.800 --> 00:16:57.030
that orbit both stars in a binary


00:16:57.040 --> 00:16:59.749
system. It turns out these Star Wars


00:16:59.759 --> 00:17:01.829
style worlds might be more common than


00:17:01.839 --> 00:17:03.910
we previously believed, especially


00:17:03.920 --> 00:17:06.949
around certain types of binary stars.


00:17:06.959 --> 00:17:09.189
>> Before we dive into the findings, let's


00:17:09.199 --> 00:17:11.429
set the stage. How common are binary


00:17:11.439 --> 00:17:13.429
star systems in the first place?


00:17:13.439 --> 00:17:15.669
>> Binary systems are actually incredibly


00:17:15.679 --> 00:17:18.230
common, Anna. Roughly half of all


00:17:18.240 --> 00:17:20.870
sunlike stars exist in binary or


00:17:20.880 --> 00:17:23.110
multiple star systems. So, we're not


00:17:23.120 --> 00:17:25.429
talking about a rare cosmic curiosity


00:17:25.439 --> 00:17:27.750
here. Binaries are a fundamental


00:17:27.760 --> 00:17:29.590
component of the galaxy's stellar


00:17:29.600 --> 00:17:30.789
population


00:17:30.799 --> 00:17:32.630
>> and we have discovered actual


00:17:32.640 --> 00:17:35.029
circumbinary planets already, right?


00:17:35.039 --> 00:17:36.870
This isn't just theoretical.


00:17:36.880 --> 00:17:39.190
>> Absolutely. NASA's Kepler Space


00:17:39.200 --> 00:17:41.669
Telescope discovered the first confirmed


00:17:41.679 --> 00:17:44.710
circumbinary planets back in 2011, and


00:17:44.720 --> 00:17:46.870
we've found several more since then.


00:17:46.880 --> 00:17:49.750
These are real worlds orbiting two suns,


00:17:49.760 --> 00:17:52.070
just like Luke Skywalker's home planet.


00:17:52.080 --> 00:17:54.150
But the question has always been, how


00:17:54.160 --> 00:17:56.390
common are they? So, what does this new


00:17:56.400 --> 00:17:57.830
research tell us?


00:17:57.840 --> 00:17:59.909
>> The study found that circumbinary


00:17:59.919 --> 00:18:02.310
planets appear to be particularly common


00:18:02.320 --> 00:18:04.310
around what are called equal mass


00:18:04.320 --> 00:18:06.870
binaries. Systems where both stars are


00:18:06.880 --> 00:18:09.510
roughly the same size and mass. In these


00:18:09.520 --> 00:18:11.830
systems, the stable orbital zone where


00:18:11.840 --> 00:18:14.230
planets can form and survive might


00:18:14.240 --> 00:18:15.750
actually be more favorable than


00:18:15.760 --> 00:18:18.150
astronomers previously calculated.


00:18:18.160 --> 00:18:20.470
>> Why would having two equal mass stars


00:18:20.480 --> 00:18:22.870
make it easier for planets to form? It


00:18:22.880 --> 00:18:25.110
has to do with gravitational stability.


00:18:25.120 --> 00:18:27.750
When you have two stars of similar mass,


00:18:27.760 --> 00:18:29.510
their gravitational influence on the


00:18:29.520 --> 00:18:31.270
surrounding disc of planet forming


00:18:31.280 --> 00:18:33.029
material is more balanced and


00:18:33.039 --> 00:18:35.110
predictable. There's less chaotic


00:18:35.120 --> 00:18:37.350
variation in the gravitational forces


00:18:37.360 --> 00:18:39.510
acting on the disc, which means there


00:18:39.520 --> 00:18:41.430
are stable regions where material can


00:18:41.440 --> 00:18:43.750
accumulate and grow into planets.


00:18:43.760 --> 00:18:46.230
>> What about unequal binary systems? One


00:18:46.240 --> 00:18:48.630
big star and one small one. Those


00:18:48.640 --> 00:18:50.710
systems can still host circumbinary


00:18:50.720 --> 00:18:52.710
planets, but the dynamics are more


00:18:52.720 --> 00:18:55.190
complex. The larger star dominates


00:18:55.200 --> 00:18:57.590
gravitationally, and the smaller star


00:18:57.600 --> 00:18:59.669
creates additional pertabbations that


00:18:59.679 --> 00:19:01.430
can make certain orbital regions


00:19:01.440 --> 00:19:03.990
unstable. It doesn't mean planets can't


00:19:04.000 --> 00:19:06.230
form, but the stable zones might be more


00:19:06.240 --> 00:19:08.070
limited or located at different


00:19:08.080 --> 00:19:09.190
distances.


00:19:09.200 --> 00:19:11.110
>> This has implications for the search for


00:19:11.120 --> 00:19:13.270
habitable worlds, doesn't it?


00:19:13.280 --> 00:19:15.909
>> Very much so. If circumbinary planets


00:19:15.919 --> 00:19:17.750
are more common than we thought,


00:19:17.760 --> 00:19:20.390
especially in equal mass binaries, that


00:19:20.400 --> 00:19:22.070
increases the overall number of


00:19:22.080 --> 00:19:24.230
potential planetary environments in the


00:19:24.240 --> 00:19:26.390
galaxy. Some of these could potentially


00:19:26.400 --> 00:19:28.390
be in the habitable zone, the region


00:19:28.400 --> 00:19:30.390
where liquid water could exist on a


00:19:30.400 --> 00:19:31.669
planet surface,


00:19:31.679 --> 00:19:33.990
>> although I imagine having two suns would


00:19:34.000 --> 00:19:35.669
complicate the climate situation


00:19:35.679 --> 00:19:36.950
significantly.


00:19:36.960 --> 00:19:39.110
>> You're absolutely right. The climate on


00:19:39.120 --> 00:19:40.950
a circumbinary planet would be


00:19:40.960 --> 00:19:43.270
fascinatingly complex. You'd have


00:19:43.280 --> 00:19:45.270
variations in heating depending on the


00:19:45.280 --> 00:19:47.750
orbital positions of both stars relative


00:19:47.760 --> 00:19:50.070
to the planet. Sometimes of the year,


00:19:50.080 --> 00:19:51.990
both suns might be on the same side of


00:19:52.000 --> 00:19:54.310
the sky, providing intense combined


00:19:54.320 --> 00:19:56.390
heating. Other times, they'd be on


00:19:56.400 --> 00:19:58.789
opposite sides, creating more balanced


00:19:58.799 --> 00:19:59.830
illumination.


00:19:59.840 --> 00:20:01.510
>> How did researchers arrive at these


00:20:01.520 --> 00:20:03.750
conclusions about circumbinary planet


00:20:03.760 --> 00:20:06.470
frequency? They combined observational


00:20:06.480 --> 00:20:08.470
data from telescope surveys with


00:20:08.480 --> 00:20:10.710
sophisticated computer modeling of how


00:20:10.720 --> 00:20:13.669
planets form in binary star systems. By


00:20:13.679 --> 00:20:15.430
simulating thousands of different


00:20:15.440 --> 00:20:17.510
scenarios with various binary


00:20:17.520 --> 00:20:19.750
configurations, they could identify


00:20:19.760 --> 00:20:22.150
patterns about which systems are most


00:20:22.160 --> 00:20:24.150
likely to host planets.


00:20:24.160 --> 00:20:25.909
>> Are there any specific systems


00:20:25.919 --> 00:20:27.669
astronomers are now targeting for


00:20:27.679 --> 00:20:29.590
follow-up observations based on these


00:20:29.600 --> 00:20:32.230
findings? The research definitely points


00:20:32.240 --> 00:20:35.029
to equal mass binaries as high priority


00:20:35.039 --> 00:20:37.430
targets for planet hunting campaigns.


00:20:37.440 --> 00:20:39.590
Missions like NASA's upcoming Nancy


00:20:39.600 --> 00:20:42.070
Grace Roman telescope and continuing


00:20:42.080 --> 00:20:44.310
observations from groundbased facilities


00:20:44.320 --> 00:20:46.230
will be keeping a close eye on these


00:20:46.240 --> 00:20:49.029
systems. Every new circumbinary planet


00:20:49.039 --> 00:20:51.909
we discover helps refine our models.


00:20:51.919 --> 00:20:54.549
>> It's exciting to think those iconic twin


00:20:54.559 --> 00:20:56.630
sunset scenes from Star Wars might be


00:20:56.640 --> 00:20:58.230
more common in the universe than we


00:20:58.240 --> 00:21:00.870
realized. It really is, Anna. The


00:21:00.880 --> 00:21:03.029
universe keeps proving that the reality


00:21:03.039 --> 00:21:05.110
can be just as spectacular as science


00:21:05.120 --> 00:21:07.750
fiction. Sometimes even more so.


00:21:07.760 --> 00:21:10.070
>> And for our final story today, Avery,


00:21:10.080 --> 00:21:11.669
we're talking about a discovery that


00:21:11.679 --> 00:21:14.070
touches on one of astronomy's biggest


00:21:14.080 --> 00:21:16.310
questions, the search for life beyond


00:21:16.320 --> 00:21:18.630
Earth. Scientists have detected a


00:21:18.640 --> 00:21:20.549
molecule critical to life in


00:21:20.559 --> 00:21:22.950
interstellar space. For the first time,


00:21:22.960 --> 00:21:24.789
tell us about this breakthrough.


00:21:24.799 --> 00:21:27.270
>> This is genuinely exciting, Anna. For


00:21:27.280 --> 00:21:29.750
the first time ever, astronomers have


00:21:29.760 --> 00:21:32.710
detected ethylenamine, a molecule that


00:21:32.720 --> 00:21:34.950
plays a crucial role in forming cell


00:21:34.960 --> 00:21:37.750
membranes floating in the vast spaces


00:21:37.760 --> 00:21:40.149
between stars. This discovery has


00:21:40.159 --> 00:21:41.990
profound implications for how we think


00:21:42.000 --> 00:21:43.909
about the building blocks of life in the


00:21:43.919 --> 00:21:44.870
universe.


00:21:44.880 --> 00:21:46.549
>> Let's start with the basics. What


00:21:46.559 --> 00:21:49.590
exactly is ethylamine and why is it so


00:21:49.600 --> 00:21:52.390
important to life? Ethylamine is an


00:21:52.400 --> 00:21:54.630
organic molecule that's a key component


00:21:54.640 --> 00:21:57.190
of phospholipids which are the primary


00:21:57.200 --> 00:21:59.669
building blocks of cell membranes. Think


00:21:59.679 --> 00:22:02.230
of cell membranes as the walls and gates


00:22:02.240 --> 00:22:04.549
of cells. They define the boundary


00:22:04.559 --> 00:22:06.870
between the inside and outside of a cell


00:22:06.880 --> 00:22:09.190
and control what goes in and out.


00:22:09.200 --> 00:22:11.590
Without molecules like ethyleneamine,


00:22:11.600 --> 00:22:13.430
you can't build functional cell


00:22:13.440 --> 00:22:15.909
membranes. And without cell membranes,


00:22:15.919 --> 00:22:18.470
you can't have cells as we know them.


00:22:18.480 --> 00:22:20.630
Though this is truly fundamental to


00:22:20.640 --> 00:22:23.350
life, at least life as we understand it.


00:22:23.360 --> 00:22:25.510
Where was this molecule detected?


00:22:25.520 --> 00:22:27.510
>> The discovery was made in a molecular


00:22:27.520 --> 00:22:30.149
cloud, one of these vast, cold regions


00:22:30.159 --> 00:22:33.110
of space where gas and dust accumulate


00:22:33.120 --> 00:22:35.110
and where new stars and planetary


00:22:35.120 --> 00:22:37.830
systems eventually form. These clouds


00:22:37.840 --> 00:22:40.390
are essentially stellar nurseries. and


00:22:40.400 --> 00:22:42.549
finding lifebuilding molecules there


00:22:42.559 --> 00:22:44.470
suggests that the ingredients for life


00:22:44.480 --> 00:22:46.230
might be getting incorporated into


00:22:46.240 --> 00:22:48.950
planetary systems right from the start.


00:22:48.960 --> 00:22:51.190
>> How do scientists actually detect


00:22:51.200 --> 00:22:53.190
specific molecules in interstellar


00:22:53.200 --> 00:22:55.830
space? I imagine you can't exactly


00:22:55.840 --> 00:22:57.430
collect a sample.


00:22:57.440 --> 00:22:59.510
>> Great question. They use radio


00:22:59.520 --> 00:23:02.070
spectroscopy. Every molecule has a


00:23:02.080 --> 00:23:04.390
unique spectroscopic signature. Think of


00:23:04.400 --> 00:23:06.789
it like a molecular fingerprint.


00:23:06.799 --> 00:23:09.029
Different molecules absorb and emit


00:23:09.039 --> 00:23:11.510
light at specific wavelengths. Radio


00:23:11.520 --> 00:23:13.510
telescopes can detect these signatures,


00:23:13.520 --> 00:23:15.750
allowing astronomers to identify what


00:23:15.760 --> 00:23:18.310
molecules are present in distant clouds,


00:23:18.320 --> 00:23:20.230
even though those clouds are trillions


00:23:20.240 --> 00:23:21.590
of miles away.


00:23:21.600 --> 00:23:23.750
>> We've found other organic molecules in


00:23:23.760 --> 00:23:26.070
space before, haven't we? What makes


00:23:26.080 --> 00:23:27.990
this discovery special?


00:23:28.000 --> 00:23:29.750
>> You're absolutely right, Hannah.


00:23:29.760 --> 00:23:32.390
Astronomers have detected more than 200


00:23:32.400 --> 00:23:34.070
different molecules in interstellar


00:23:34.080 --> 00:23:37.270
space, including amino acids and sugars.


00:23:37.280 --> 00:23:39.430
But ethylanamine is special because of


00:23:39.440 --> 00:23:41.750
its direct connection to cell membrane


00:23:41.760 --> 00:23:44.230
formation. It's one thing to find amino


00:23:44.240 --> 00:23:46.950
acids, the building blocks of proteins.


00:23:46.960 --> 00:23:48.950
But finding a molecule that's essential


00:23:48.960 --> 00:23:51.190
for creating the actual structure of


00:23:51.200 --> 00:23:54.070
cells, takes us another step closer to


00:23:54.080 --> 00:23:55.990
understanding how life's fundamental


00:23:56.000 --> 00:23:58.549
architecture might arise. Does this


00:23:58.559 --> 00:24:00.310
discovery change our thinking about


00:24:00.320 --> 00:24:02.149
where the building blocks of life come


00:24:02.159 --> 00:24:02.950
from?


00:24:02.960 --> 00:24:05.190
>> It definitely supports the hypothesis


00:24:05.200 --> 00:24:07.830
that many of life's essential molecular


00:24:07.840 --> 00:24:10.070
ingredients aren't created on planets


00:24:10.080 --> 00:24:12.950
after they form, but rather arrive from


00:24:12.960 --> 00:24:15.830
space. We already know that meteorites


00:24:15.840 --> 00:24:18.390
deliver organic compounds to planets. We


00:24:18.400 --> 00:24:20.390
found amino acids and meteorites that


00:24:20.400 --> 00:24:23.029
have fallen to Earth. This discovery


00:24:23.039 --> 00:24:25.510
suggests that even more complex life


00:24:25.520 --> 00:24:27.430
related molecules could be delivered


00:24:27.440 --> 00:24:28.710
from space.


00:24:28.720 --> 00:24:31.350
>> Though in a sense the raw materials for


00:24:31.360 --> 00:24:33.350
life might be common throughout the


00:24:33.360 --> 00:24:34.390
galaxy.


00:24:34.400 --> 00:24:36.789
>> That's the tantalizing possibility this


00:24:36.799 --> 00:24:39.590
raises. If molecules like ethanolamine


00:24:39.600 --> 00:24:41.590
can form in the harsh conditions of


00:24:41.600 --> 00:24:44.230
interstellar space, then these building


00:24:44.240 --> 00:24:46.149
blocks might be present in molecular


00:24:46.159 --> 00:24:48.789
clouds throughout the galaxy. Every time


00:24:48.799 --> 00:24:51.350
a new planetary system forms, it could


00:24:51.360 --> 00:24:53.590
be inheriting these pre-made components


00:24:53.600 --> 00:24:54.789
of life.


00:24:54.799 --> 00:24:56.950
>> This doesn't mean life is automatically


00:24:56.960 --> 00:24:58.950
everywhere, though, right? Having the


00:24:58.960 --> 00:25:00.549
ingredients doesn't guarantee you'll


00:25:00.559 --> 00:25:01.830
bake the cake.


00:25:01.840 --> 00:25:04.549
>> Exactly. This is about potential and


00:25:04.559 --> 00:25:06.789
possibility. Having the molecular


00:25:06.799 --> 00:25:09.190
building blocks is necessary for life,


00:25:09.200 --> 00:25:11.669
but it's not sufficient. You still need


00:25:11.679 --> 00:25:13.750
the right conditions for those molecules


00:25:13.760 --> 00:25:16.230
to assemble into functioning biological


00:25:16.240 --> 00:25:18.470
systems. The right temperature,


00:25:18.480 --> 00:25:21.590
pressure, energy sources, solvents like


00:25:21.600 --> 00:25:24.070
liquid water, and probably a host of


00:25:24.080 --> 00:25:26.789
factors we don't fully understand yet.


00:25:26.799 --> 00:25:28.470
>> What are the next steps for this kind of


00:25:28.480 --> 00:25:29.430
research?


00:25:29.440 --> 00:25:30.950
>> Astronomers will be looking for


00:25:30.960 --> 00:25:33.350
ethanolamine and similar molecules in


00:25:33.360 --> 00:25:35.190
other molecular clouds to see how


00:25:35.200 --> 00:25:37.350
widespread they are. They'll also be


00:25:37.360 --> 00:25:39.590
searching for even more complex organic


00:25:39.600 --> 00:25:41.909
molecules that might be precursors to


00:25:41.919 --> 00:25:45.029
biological chemistry. Every molecule we


00:25:45.039 --> 00:25:47.110
find helps us piece together the story


00:25:47.120 --> 00:25:49.830
of how inanimate chemistry transitions


00:25:49.840 --> 00:25:51.990
to the chemistry of life.


00:25:52.000 --> 00:25:53.590
>> It's remarkable to think that the


00:25:53.600 --> 00:25:55.669
membrane surrounding every cell in our


00:25:55.679 --> 00:25:57.669
bodies might have had their chemical


00:25:57.679 --> 00:25:59.830
ancestors floating between the stars


00:25:59.840 --> 00:26:01.510
billions of years ago.


00:26:01.520 --> 00:26:03.590
>> It really is, Anna. It connects us to


00:26:03.600 --> 00:26:06.710
the cosmos in a very tangible way. We're


00:26:06.720 --> 00:26:09.190
not just made of stardust in an abstract


00:26:09.200 --> 00:26:12.390
sense. The actual molecular machinery of


00:26:12.400 --> 00:26:14.950
life may have origins that predate Earth


00:26:14.960 --> 00:26:16.149
itself.


00:26:16.159 --> 00:26:18.070
>> What a perfect note to end today's


00:26:18.080 --> 00:26:20.070
episode on. A reminder that we're part


00:26:20.080 --> 00:26:22.390
of a universewide chemistry experiment


00:26:22.400 --> 00:26:24.149
that's been running for billions of


00:26:24.159 --> 00:26:25.110
years.


00:26:25.120 --> 00:26:27.110
>> Well, that wraps up another day of space


00:26:27.120 --> 00:26:29.909
and astronomy news. From NASA's Aremis


00:26:29.919 --> 00:26:32.070
preparations to the discovery of life's


00:26:32.080 --> 00:26:33.909
building blocks floating between the


00:26:33.919 --> 00:26:36.950
stars, the universe continues to amaze


00:26:36.960 --> 00:26:38.310
and inspire.


00:26:38.320 --> 00:26:40.310
>> It really does. Thanks so much for


00:26:40.320 --> 00:26:42.149
joining us today, everyone. Remember,


00:26:42.159 --> 00:26:44.789
you can find us at astronomyaily.io


00:26:44.799 --> 00:26:46.630
for full episode transcripts and


00:26:46.640 --> 00:26:47.590
additional content.


00:26:47.600 --> 00:26:49.510
>> And don't forget to follow us on social


00:26:49.520 --> 00:26:52.950
media at astroaily pod for daily updates


00:26:52.960 --> 00:26:55.029
and space news throughout the week.


00:26:55.039 --> 00:26:58.470
>> Until next time, keep looking up. Clear


00:26:58.480 --> 00:27:03.029
skies everyone. Astronomy [music] day.


00:27:03.039 --> 00:27:10.950
Stories be told.


00:27:10.960 --> 00:27:19.473
Stories [music] told.


00:27:19.483 --> 00:27:21.503
[music]