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Anna: Hello, space enthusiasts. I'm Anna.

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Avery: And I'm, um, Avery. Welcome to Astronomy

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Daily, your daily dose of space and

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astronomy news, brought to you by

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astronomydaily IO and what

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a.

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Anna: Day we have for you today, Avery. If you were

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lucky enough to catch the auroras last night,

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you know what we're leading with.

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Avery: Absolutely, Anna. We're following up on

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yesterday's story about that powerful X class

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solar flare and the coronal mass ejection

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that was racing toward Earth. Well, it hit

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and it hit hard.

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Anna: That's right. We've got stunning photos from

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around the world of the resulting northern

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lights. And a retirement announcement from a

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legendary NASA astronaut. An incredible

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space rescue story from China, and some

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exciting updates from the commercial space

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sector.

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Avery: Plus, we'll tell you about NASA's latest

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mission that's preparing to study the Sun's

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most powerful eruptions. And we'll take you

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on a cosmic journey billions of years into

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the past with some fascinating new telescope

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observations.

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Anna: So grab your coffee, settle in, and let's get

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into today's space news.

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Avery: All right, Anna, let's dive into our lead

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story and what a spectacular show it

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was yesterday. We told our listeners about

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that x 1.9 solar flare and

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coronal mass ejection headed our way.

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Well, it arrived right on schedule. In fact,

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a little early.

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Anna: It certainly did, Avery. The CME

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slammed into Earth's magnetic field on

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January 19th at around 2:38pm

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Eastern Time. And it packed quite a punch.

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Space weather forecasters at NOAA's Space

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Weather Prediction center confirmed that

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geomagnetic conditions escalated to

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G4 level. That's classified as

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severe on their five point scale.

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Avery: And the results were absolutely

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breathtaking. What made the CME

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particularly noteworthy was just how fast it

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traveled. Remember, it was ejected from the

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sun on January 18th during that powerful

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solar flare, which means it covered roughly

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93 million miles in just over a day.

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That's exceptionally quick.

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Anna: The aurora displays that followed were truly

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global in scope. We're seeing reports and

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photographs from locations that rarely get to

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witness the northern lights. One

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photographer, Greg Gage, captured stunning

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red auroras from Deming, New Mexico. That's

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at 32 degrees latitude. He told

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Space.com he was on vacation there and never

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expected to see auroras that far south.

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Avery: That's incredible. And it wasn't just North

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America. The displays stretched across

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Europe, Asia and beyond. In

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Germany, vivid red and green auroras danced

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above the River Mughelspree near Berlin,

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Hungary, saw intense red and green hues

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filling the skies over the village of.

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Anna: Oboivar, uh, France had some particularly

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eerie displays with rich magenta

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auroras above Brittany. And in China, the

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northern lights were visible Above Beiji

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village in Heilongjiang province, with

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photographers capturing everything from

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magenta to green to even hints of blue

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in the curtains of light.

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Avery: What's particularly interesting about these

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displays Is the variety of colors. The

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red auroras we're seeing indicate that oxygen

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atoms at, uh, very high altitudes around 200

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to 300 miles up, are being energized.

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The green we typically associate with auroras

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Comes from oxygen at lower altitudes, While

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any blue would be from nitrogen.

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Anna: The geomagnetic conditions throughout the

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night Were quite dynamic, too. Storm levels

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fluctuated between G1, G2,

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G3, and G4 as the CME

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passed through Earth's magnetic field.

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According to the UK Met Office, this kept

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Earth's magnetic field In a highly disturbed

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state for hours, Producing repeated surges of

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auroral activity.

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Avery: And there's more good news for aurora

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watchers. While geomagnetic activity Is

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expected to gradually ease, Forecasters

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say conditions remain unsettled. That means

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there's still a chance the northern lights

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could make another appearance tonight if

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solar, uh, wind conditions cooperate.

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Anna: So if you missed last night's show, keep

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those cameras charged and your aurora alert

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apps turned on. The sun is clearly in an

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active phase, and we could see more displays

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in the coming days and weeks.

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Avery: Absolutely. And this really highlights why we

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track space weather so closely. While these

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auroras are beautiful, the same geomagnetic

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storms can affect satellites, power grids,

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and radio communications. It's a reminder of

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how our technological society is connected

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to what's happening 93 million miles away

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on the sun.

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Anna: Moving on to our next story. Avery. And this

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one marks the end of an era. After

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27 years of distinguished service,

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NASA astronaut Suni Williams has officially

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retired from the agency.

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Avery: This is definitely a significant moment.

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Anna, uh, Suni Williams has been such an

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inspiring figure in human spaceflight. Her

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retirement became effective on December 27,

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2025, though NASA just announced

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it this week. Let's talk about her remarkable

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achievements.

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Anna: Where do we even start? Over the course of

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her career, Williams logged an impressive

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608 days in space. That

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makes her second on the list for cumulative

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time and space by a NASA astronaut. She

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completed three missions to the International

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Space Station and held numerous records

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throughout her career.

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Avery: Her most recent mission was particularly

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interesting. Williams and fellow astronaut

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Butch Wilmore launched aboard Boeing

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Starliner spacecraft in June 2024

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as part of NASA's Boeing Crew Flight Test

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mission, both tied for sixth place on the

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list. Of longest single spaceflight by an

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American logging 286

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days during their combined Starliner and

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SpaceX Crew 9 missions.

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Anna: That's right. And during that mission,

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Williams once again took command of the space

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station for Expedition 72. She's also

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renowned for her spacewalking expertise. She

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completed nine spacewalks totaling 62

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hours and six minutes over her career.

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Avery: That gives her the record for most spacewalk

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time by a woman and fourth most on the all

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time cumulative spacewalk duration list.

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Oh, and here's a fun fact. She was also the

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first person to run a marathon in space.

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Anna: Beyond her spaceflight experience, Williams

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held numerous important roles at NASA. She

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served as Deputy Chief of the Astronaut

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Office, was Director of Operations in Star

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City, Russia, and most recently helped

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establish a helicopter training platform to

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prepare astronauts for future moon landings.

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Avery: NASA Administrator Jared Eichman had some

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wonderful words about her legacy. He called

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her a trailblazer in human spaceflight whose

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work advancing science and technology has

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laid the foundation for Artemis missions to

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the moon and future missions to Mars.

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Anna: It's worth noting her background too. She's a

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retired US Navy captain and an accomplished

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pilot with more than 4,000 flight hours in

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40 different aircraft. She holds a bachelor's

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degree in Physical science from the United

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States Naval Academy and a master's degree in

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Engineering Management.

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Avery: In her retirement statement, Williams said,

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anyone who knows me knows that space is my

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absolute favorite place to be. She expressed

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gratitude for her 27 year career and the

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support she received from her colleagues and

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mentioned she's excited to watch NASA make

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history as the agency continues its

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exploration efforts.

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Anna: It's a well deserved retirement for someone

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who has contributed so much to human

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spaceflight. Her achievements will

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undoubtedly inspire the next generation of

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astronauts and space explorers.

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Avery: Alright, Anna, um, our next story is quite

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dramatic. It involves a successful space

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rescue, emergency repairs, and some

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impressive quick thinking by China's space

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program.

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Anna: This is really a remarkable story, avery.

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China's Shenzhou 20 capsule safely

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landed in Inner Mongolia on January 19,

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2026 after spending 270

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days in orbit. But the journey

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back wasn't exactly routine. This

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mission became one of the most technically

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demanding in China's human spaceflight

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history.

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Avery: The Shenzhou 20 was originally launched back

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on April 24, 2025 from

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the Jiuquan Satellite Launch Center. It was

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expected to complete its mission and return

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in November 2025. But then

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came the complication. A, uh, suspected

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impact with space debris damaged one of the

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capsule's portholes.

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Anna: Talk about a critical issue. A cracked

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porthole on a spacecraft is serious business,

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especially when you're thinking about the

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intense heat and forces of re entry through

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Earth's atmosphere. So how did China's

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space program respond?

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Avery: With remarkable speed and coordination.

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First they authorized astronauts aboard the

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Shenzhou 21 spacecraft to photograph the

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damaged porthole during a spacewalk on

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December 9. They used high definition

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cameras to get a detailed diagnosis of the

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problem.

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Anna: And then came an unprecedented move.

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China launched Shenzhou 22 on

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November 25. Marking the first rapid

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response emergency deployment in China's

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space history. This uncrewed craft delivered

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a specially engineered repair device

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designed to enhance the capsule's heat

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resistance and sealing for re entry.

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Avery: Meanwhile, for safety reasons, the crew of

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Shenzhou 20 was evacuated ahead of

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schedule. They returned aboard Shenzhou

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21 on November 14th in what the China

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Manned Space Agency called an emergency

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reroute.

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Anna: So uh, the Shenzhou 20 capsule came home

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empty, but it came home safe. According

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to cgtn, the China Manned Space

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Agency declared the mission uh, a complete

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success after an on site inspection

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confirmed the capsule was in good condition

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despite everything it went through.

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Avery: What really stands out here is the

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operational capability. This demonstrates

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China executed three overlapping missions,

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Shenzhou 20, 21 and 22

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over a span of just weeks. That shows

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significant operational depth and uh, the

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ability to respond to emergencies in space.

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Anna: Absolutely. And it's not just about the

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technical achievement. This validates China's

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long term approach to maintaining crew

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vehicles in orbit. The Shenzhou 20

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stayed up there for 270 days

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which demonstrates the reliability of their

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spacecraft systems.

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Avery: This mission also underscores something we

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talk about often, the very real danger

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posed by space debris. Even small particles

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traveling at orbital velocities can cause

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significant damage as we saw here with the

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porthole crack.

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Anna: And China's ability to handle this situation

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adds to their growing reputation in space

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exploration. They're now capable of managing

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multi vessel operations under pressure with

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modular mission architecture and long term

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crew support capabilities.

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Avery: Congratulations to all involved in this very

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successful mission. In the end.

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Anna: Moving on to our next story, Avery. And we're

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heading to West Texas where Blue Origin is

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preparing for its next suborbital space

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tourism mission.

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Avery: That's right Anna. Uh, Blue Origin is

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scheduled to launch six space tourists on its

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NS38 mission this Thursday, January

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22nd. The launch window opens at

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9:30am Eastern Time. That's

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8:30am M local Texas time.

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Anna: This will be the 38th flight of Blue

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Origin's New Shepard rocket capsule system.

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And if all goes according to plan, the 17th

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crewed mission they've flown the mission

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follows the same profile we've seen before.

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About 10 to 12 minutes from liftoff to the

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capsule's parachute aided touchdown.

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Avery: During that brief but spectacular journey,

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passengers will experience a few minutes of

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weightlessness and get to see Earth against

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the blackness of space from an altitude above

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the Karman Line, which is generally

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recognized as the boundary of space.

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Anna: Now, let's talk about who's flying. We have

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entrepreneur and pilot Tim Drexler,

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retired obstetrician and gynecologist Linda

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Edwards, real estate developer and investor

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Elaine Fernandez, entrepreneur and

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technologist Alberto Gutierrez, and

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retired US Air Force Colonel Jim Hendren,

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who founded Hendren Plastics, Inc. And

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there's an interesting.

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Avery: Late addition to the crew manifest. Blue

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Origin just announced that Lara Stiles, who

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is Blue Origin's director of New Shepard

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launch Operations, will be flying on this

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mission.

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Anna: That's a pretty cool opportunity for someone

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who's been so involved in making these

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missions happen. Dials is actually a late

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replacement for a passenger who had to drop

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out due to illness. Though that person will

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get to fly on a future mission.

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Avery: Blue Origin has been steadily building their

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flight rate. Just last month, they made

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history by flying the first wheelchair user

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to space on their NS37 mission. They're

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really demonstrating that spaceflight can be

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accessible to a diverse range of people.

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Anna: Now, Blue Origin hasn't publicly disclosed

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their ticket prices, but we know their main

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competitor Virgin Galactic charges

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$600,000 per seat for similar

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suborbital flights. So we can probably assume

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Blue Origin's prices are in that same

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ballpark.

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Avery: If you want to watch this launch, Blue Origin

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typically livestreams our missions, and

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Space.com will likely carry the feat as well.

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It's always exciting to watch these launches.

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That New Shepard rocket is quite a sight to

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see.

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Anna: Absolutely. And it's worth noting how routine

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these launches are becoming. Blue Origin is

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really building up their experience with

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regular crewed flights, which is essential

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for the commercial space tourism industry.

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Avery: Our next story takes us from suborbital

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tourism to cutting edge heliophysics

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research.

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Anna. Uh, NASA Sunrise, that's the Sun

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Radio Interometer Space Experiment is moving

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closer to its launch later this year after

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successfully completing a rigorous series of

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tests.

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Anna: This is such a fascinating mission. Avery

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00:14:10.030 --> 00:14:12.750
Sunrise consists of six smallsats.

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They're about the size of a toaster oven that

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will fly in formation to act as one giant

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radio telescope studying the sun.

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Avery: That's the clever part. These six smallsats

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will orbit at about 22,000 miles

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00:14:25.990 --> 00:14:28.270
altitude, which is geosynchronous orbit.

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Flying up to 10 miles apart from each other.

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By combining their observations Using a

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00:14:33.190 --> 00:14:35.580
technique called interferometry, they'll

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create what's essentially A single large

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radio telescope in space.

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Anna: And what will they be looking at? Solar

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radio bursts. These bursts are generated

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by solar energetic particle events Deep

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within the sun's atmosphere, or corona. In

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extreme cases, these events could pose

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00:14:53.700 --> 00:14:56.260
radiation hazards to unprotected astronauts

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and damaged satellites.

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Avery: The spacecraft were built At Utah State

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00:15:00.300 --> 00:15:02.700
University's Space Dynamics laboratory in

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00:15:02.700 --> 00:15:05.290
Logan, Utah, and they just completed what's

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00:15:05.290 --> 00:15:07.410
described As a rigorous testing campaign.

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00:15:07.890 --> 00:15:10.250
This included thermal vacuum testing to

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00:15:10.250 --> 00:15:13.210
simulate orbital conditions, Electromagnetic

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compatibility testing to ensure the

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electronic systems Won't interfere With the

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sensitive instruments, and most dramatically,

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vibration testing.

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Anna: The vibration testing is crucial because

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00:15:25.010 --> 00:15:27.490
launch is an incredibly violent event.

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00:15:28.130 --> 00:15:30.930
Jim Lux, the Sunrise project manager at

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NASA's Jet Propulsion Laboratory, Explained

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00:15:33.820 --> 00:15:35.860
that each spacecraft was loaded with

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propellant to match its launch mass and then

383
00:15:38.820 --> 00:15:41.460
subjected to vibration testing in all three

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axes.

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Avery: They wanted to make the simulated vibrations

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00:15:44.540 --> 00:15:46.900
as true to the actual launch conditions as

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00:15:46.900 --> 00:15:49.180
possible. And here's the important part.

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Pre and post test functional checks were

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00:15:51.940 --> 00:15:54.700
performed and all six spacecraft passed with

390
00:15:54.700 --> 00:15:55.660
flying colors.

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Anna: The mission is scheduled to launch From Cape

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Canaveral Space Force Station in Florida

393
00:16:00.540 --> 00:16:03.460
Aboard a, uh ULA launch Vulcan Centaur

394
00:16:03.460 --> 00:16:06.190
rocket As a rideshare mission. Once in orbit,

395
00:16:06.190 --> 00:16:08.910
each satellite will deploy four telescoping

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antenna booms about 10ft long,

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00:16:11.550 --> 00:16:13.630
forming an X shaped configuration.

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00:16:14.110 --> 00:16:16.830
Avery: Sue Lepre, the sunrise principal investigator

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00:16:16.830 --> 00:16:19.110
at the University of Michigan, Points out

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00:16:19.110 --> 00:16:21.390
that these solar radio bursts Are triggered

401
00:16:21.390 --> 00:16:23.830
when vast quantities of energy Stored in the

402
00:16:23.830 --> 00:16:26.550
sun's magnetic field Accelerate solar

403
00:16:26.550 --> 00:16:29.030
particles to high speeds. Tracking these

404
00:16:29.030 --> 00:16:31.150
events will help space agencies Protect

405
00:16:31.150 --> 00:16:32.590
astronauts and spacecraft.

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00:16:33.180 --> 00:16:35.220
Anna: And this mission will work in conjunction

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00:16:35.220 --> 00:16:37.660
with other NASA heliophysics missions like

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00:16:37.660 --> 00:16:40.300
the Solar Terrestrial Relations Observatory,

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00:16:40.540 --> 00:16:43.060
the Parker Solar probe, and Solar

410
00:16:43.060 --> 00:16:44.540
Orbiter, which is an international

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00:16:44.780 --> 00:16:46.540
cooperative mission with esa.

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00:16:46.700 --> 00:16:48.700
Avery: It's exciting to see these missions coming

413
00:16:48.700 --> 00:16:51.340
together Between Parker Solar Probe diving

414
00:16:51.340 --> 00:16:54.260
close to the sun, Solar Orbiter studying the

415
00:16:54.260 --> 00:16:57.140
polar regions, and now Sunrise tracking radio

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00:16:57.140 --> 00:16:59.510
bursts from Earth orbit. We're building a

417
00:16:59.510 --> 00:17:01.790
comprehensive picture of our star's behavior.

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00:17:02.270 --> 00:17:05.230
Anna: And now for our final story. Avery. We're

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00:17:05.230 --> 00:17:07.350
going to talk about something that's never

420
00:17:07.350 --> 00:17:09.390
been seen before in quite this

421
00:17:10.190 --> 00:17:12.750
Planetary systems in their awkward

422
00:17:12.830 --> 00:17:13.790
teenage years.

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00:17:15.310 --> 00:17:17.910
Avery: Love that description, Anna. Astronomers

424
00:17:17.910 --> 00:17:20.110
using the Atacama Large Millimeter

425
00:17:20.190 --> 00:17:23.150
Submillimeter Array, better known as Alma,

426
00:17:23.310 --> 00:17:25.990
have captured the most detailed images ever

427
00:17:25.990 --> 00:17:28.769
of 24 debris disks. These are the

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00:17:28.769 --> 00:17:31.369
dusty belts left behind after planets have

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00:17:31.369 --> 00:17:32.249
finished forming.

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00:17:32.729 --> 00:17:35.569
Anna: The survey is called arcs, which stands for

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00:17:35.569 --> 00:17:37.609
the ALMA Survey to Resolve

432
00:17:37.609 --> 00:17:39.769
Exoker belt substructures.

433
00:17:40.169 --> 00:17:42.689
Meredith Hughes, an associate professor at

434
00:17:42.689 --> 00:17:45.209
Wesleyan University and co principal

435
00:17:45.209 --> 00:17:47.609
investigator, explains it perfectly.

436
00:17:47.849 --> 00:17:50.729
We've often seen the baby pictures of planets

437
00:17:50.729 --> 00:17:53.609
forming, but until now, the teenage years

438
00:17:53.609 --> 00:17:55.209
have been a missing link.

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00:17:56.000 --> 00:17:58.640
Avery: And just like human teenagers, these systems

440
00:17:58.640 --> 00:18:00.720
turned out to be quite dramatic. The

441
00:18:00.720 --> 00:18:03.360
observations revealed incredible diversity.

442
00:18:03.600 --> 00:18:06.440
Not just simple rings, but multi ring

443
00:18:06.440 --> 00:18:09.200
belts, wide smooth halos, sharp

444
00:18:09.200 --> 00:18:12.000
edges, and even unexpected arcs and clumps.

445
00:18:12.480 --> 00:18:15.040
Anna: This phase is really important because these

446
00:18:15.040 --> 00:18:17.680
debris disks represent what's called the

447
00:18:17.680 --> 00:18:19.960
collision dominated phase of planet

448
00:18:19.960 --> 00:18:22.530
formation. Think of it like our own solar

449
00:18:22.530 --> 00:18:25.250
system's Kuiper Belt, that ring of icy

450
00:18:25.250 --> 00:18:28.250
debris beyond Neptune that preserves a record

451
00:18:28.250 --> 00:18:30.770
of massive collisions and planetary

452
00:18:30.770 --> 00:18:33.130
migrations from billions of years ago.

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00:18:33.770 --> 00:18:36.090
Avery: Thomas Henning from the Max Planck Institute

454
00:18:36.090 --> 00:18:38.130
for Astronomy, another co principal

455
00:18:38.130 --> 00:18:40.530
investigator, notes that by characterizing

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00:18:40.530 --> 00:18:42.890
these disk structures, they can find evidence

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00:18:42.890 --> 00:18:45.490
pointing to the presence of planets. They're

458
00:18:45.490 --> 00:18:48.210
using ALMA alongside direct imaging and radio

459
00:18:48.210 --> 00:18:50.690
velocity studies to search for young planets

460
00:18:50.690 --> 00:18:51.450
in these systems.

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00:18:52.150 --> 00:18:54.230
Anna: One of the challenges with studying debris

462
00:18:54.230 --> 00:18:56.630
disks is that they're incredibly faint,

463
00:18:56.870 --> 00:18:59.470
hundreds or even thousands of times dimmer

464
00:18:59.470 --> 00:19:02.270
than the bright gas rich disks where planets

465
00:19:02.270 --> 00:19:04.830
are actively being born. But alma's

466
00:19:04.830 --> 00:19:07.110
sensitivity and resolution made these.

467
00:19:07.110 --> 00:19:09.990
Avery: Observations possible, and the findings

468
00:19:09.990 --> 00:19:12.390
are fascinating. About one third of the

469
00:19:12.390 --> 00:19:15.150
observed disks show clear substructures,

470
00:19:15.150 --> 00:19:17.670
like multiple rings or distinct gaps.

471
00:19:18.240 --> 00:19:20.320
These could be legacy features from earlier

472
00:19:20.480 --> 00:19:22.960
planet building stages, or they could be

473
00:19:22.960 --> 00:19:25.280
sculpted by planets over much longer

474
00:19:25.280 --> 00:19:26.080
timescales.

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00:19:26.560 --> 00:19:29.160
Anna: Perhaps most surprising, several of these

476
00:19:29.160 --> 00:19:32.160
disks retain gas much longer than expected.

477
00:19:32.800 --> 00:19:35.520
In some systems, this lingering gas might

478
00:19:35.520 --> 00:19:37.840
actually shape the chemistry of growing

479
00:19:37.840 --> 00:19:40.560
planets. Or it might push dust into

480
00:19:40.560 --> 00:19:41.600
wide halos.

481
00:19:42.320 --> 00:19:45.040
Avery: Many of the disks also show asymmetries and

482
00:19:45.040 --> 00:19:47.880
arcs. They're lopsided with bright arcs

483
00:19:47.880 --> 00:19:50.290
or eccentric shapes. This hints, uh, at

484
00:19:50.290 --> 00:19:52.490
gravitational interactions with unseen

485
00:19:52.490 --> 00:19:55.210
planets, leftover scars from planetary

486
00:19:55.210 --> 00:19:58.010
migration or interactions between the gas

487
00:19:58.010 --> 00:19:58.690
and dust.

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00:19:59.250 --> 00:20:02.210
Anna: Luca Matra from Trinity College Dublin,

489
00:20:02.210 --> 00:20:04.730
another co principal investigator, puts it

490
00:20:04.730 --> 00:20:07.570
beautifully. These disks record a

491
00:20:07.570 --> 00:20:09.970
period when planetary orbits were being

492
00:20:09.970 --> 00:20:12.850
scrambled and huge impacts like the one

493
00:20:12.850 --> 00:20:15.570
that forged Earth's Moon were shaping young

494
00:20:15.570 --> 00:20:16.530
solar systems.

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00:20:17.320 --> 00:20:19.480
Avery: And here's some great news for the scientific

496
00:20:19.480 --> 00:20:22.080
community. All of the ARC's observations and

497
00:20:22.080 --> 00:20:24.600
process data are being made freely available

498
00:20:24.680 --> 00:20:27.600
to astronomers worldwide. Which means we can

499
00:20:27.600 --> 00:20:29.840
expect even more discoveries from this data

500
00:20:29.840 --> 00:20:31.080
set in the coming years.

501
00:20:31.720 --> 00:20:34.280
Anna: Meredith Hughes sums up the significance

502
00:20:34.520 --> 00:20:37.440
perfectly. This project gives us a new

503
00:20:37.440 --> 00:20:39.840
lens for interpreting the craters on the

504
00:20:39.840 --> 00:20:42.640
Moon, the dynamics of the Kuiper Belt, and

505
00:20:42.640 --> 00:20:45.080
the growth of planets big and small.

506
00:20:45.690 --> 00:20:48.090
It's like adding the missing pages to the

507
00:20:48.090 --> 00:20:49.930
solar system's family album.

508
00:20:50.570 --> 00:20:52.610
Avery: Well, that wraps up today's episode of

509
00:20:52.610 --> 00:20:55.090
Astronomy Daily. What an incredible day of

510
00:20:55.090 --> 00:20:56.250
space news we've covered.

511
00:20:56.410 --> 00:20:59.050
Anna: From spectacular auroras, lighting up

512
00:20:59.050 --> 00:21:01.810
skies around the globe, to the retirement of

513
00:21:01.810 --> 00:21:04.610
a legendary astronaut, emergency space

514
00:21:04.610 --> 00:21:07.370
repairs by China, exciting commercial

515
00:21:07.370 --> 00:21:09.530
space launches, and groundbreaking

516
00:21:09.530 --> 00:21:12.490
observations of planetary systems, it's

517
00:21:12.490 --> 00:21:14.450
been quite a journey through the cosmos.

518
00:21:14.850 --> 00:21:16.810
Avery: And remember, if you want to stay up to date

519
00:21:16.810 --> 00:21:18.930
with all the latest space and astronomy news,

520
00:21:18.930 --> 00:21:19.530
visit our

521
00:21:19.530 --> 00:21:22.490
website@astronomydaily.IO. you

522
00:21:22.490 --> 00:21:24.530
can also find us on all major social media

523
00:21:24.530 --> 00:21:27.170
platforms. Just search for astrodaily

524
00:21:27.170 --> 00:21:27.650
Pod.

525
00:21:28.130 --> 00:21:31.010
Anna: That's astrodaily pod. All one word.

526
00:21:31.090 --> 00:21:32.890
We'd love to hear from you and see your

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00:21:32.890 --> 00:21:34.970
aurora photos if you caught last night's

528
00:21:34.970 --> 00:21:35.410
display.

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00:21:35.570 --> 00:21:38.120
Avery: Thanks for joining us today, space fans. Keep

530
00:21:38.120 --> 00:21:40.040
looking up and we'll see you tomorrow with

531
00:21:40.040 --> 00:21:42.240
more exciting space and astronomy news.

532
00:21:42.880 --> 00:21:45.040
Anna: Until then, clear skies, everyone.

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Avery: Told.