Anomalies in India’s Launch| SpaceX’s Starlink Expansion| Cosmic Dawn Signals: Your Daily Space...
Space News TodayJanuary 12, 202600:12:1411.21 MB

Anomalies in India’s Launch| SpaceX’s Starlink Expansion| Cosmic Dawn Signals: Your Daily Space...

In today’s episode of Astronomy Daily, Anna and Avery take you from rocket pads on Earth to the farthest corners of the cosmos. We cover India’s latest PSLV launch and its unexpected anomaly, the FCC’s green light for thousands more Starlink Gen2 satellites, NASA’s Pandora mission to decode exoplanet atmospheres, a fleeting signal from a supernova that exploded 13 billion years ago, a breakthrough in understanding the Sun’s most violent flares, and the surprising discovery of a barred spiral galaxy in the early Universe.

It’s an episode where orbital mechanics meet cosmic archaeology — with a dash of solar storm science.

---

## 📰 Stories Covered

1. India’s EOS‑N1 Launch on PSLV-C62

- First PSLV liftoff since a May 2025 anomaly.

- Carried a military Earth‑observation satellite plus 15 payloads.

- Third‑stage deviation under investigation.

2. FCC Approves 7,500 Additional Starlink Gen2 Satellites

- Expansion to boost coverage and speed.

- Partial approval pending further review of SpaceX’s larger request.

- Implications for connectivity, orbital traffic, and astronomy.

3. NASA’s Pandora – Exoplanet Atmosphere Investigator

- Small, dedicated telescope to study exoplanet atmospheres.

- Focused on separating signals from planets and their stars.

- Could refine the hunt for biosignatures.

4. A Ten‑Second Signal from the Early Universe

- Likely a supernova about 13 billion light‑years away.

- Offers a rare probe into early stellar death.

- Discovered via coordinated, multi‑wavelength observations.

5. Unmasking the Sun’s Most Violent Flares

- Discovery of ultra‑energetic particles in the upper solar atmosphere.

- Provides a clearer picture of gamma‑ray production.

- Could improve space weather forecasts.

6. Earliest Known Barred Spiral Galaxy

- Dated to 11.5 billion years ago.

- Challenges models of how fast galaxy structures form.

- May force revisions in early-Universe galaxy evolution theories.

---

## 🔍 Key Themes & Takeaways

- Space Operations: Even reliable rockets can have anomalies — data analysis is crucial.

- Policy & Infrastructure: Starlink expansion reshapes the orbital environment.

- Scientific Frontiers: Compact, focused missions can massively advance our understanding.

- Cosmic Forensics: The early Universe was more structured than we thought.

- Solar Hazards: Better flare science means better protection for tech and people.

---

## 📚 Further Reading & References

- [India launches EOS‑N1 military satellite with PSLV-C62](https://www.space.com/space-exploration/launches-spacecraft/india-eos-n1-military-satellite-15-payloads-pslv-launch)

- [FCC approves 7,500 more Starlink Gen2 satellites](https://spacenews.com/fcc-approves-7500-additional-starlink-satellites/)

- [NASA’s Pandora mission launch coverage](https://www.space.com/space-exploration/launches-spacecraft/watch-spacex-launch-nasas-pandora-exoplanet-studying-satellite-on-jan-11)

- [Supernova signal from 13 billion years ago](https://dailygalaxy.com/2026/01/earth-receives-10-second-signal-from-supernova-13-billion-years-ago/)

- [Breakthrough on Sun’s flare particle populations](https://scitechdaily.com/what-powers-the-suns-most-violent-flares-scientists-finally-have-an-answer/)

- [Early barred spiral galaxy discovery](https://connectsci.au/news/news-parent/7631/Barred-spiral-galaxy-may-be-the-earliest-seen-yet?searchresult=1)

---

## 🎧 How to Listen

Subscribe to Astronomy Daily on Spotify, Apple Podcasts, or your favorite podcast platform.

---

## 💬 Join the Conversation

Do you have a question about today’s stories or space science in general?

Send us a message via the Astronomy Daily page — your question could be featured in an upcoming episode.

🌌 Clear skies, and see you next time.


Become a supporter of this podcast: https://www.spreaker.com/podcast/astronomy-daily-space-news-updates--5648921/support (https://www.spreaker.com/podcast/astronomy-daily-space-news-updates--5648921/support?utm_source=rss&utm_medium=rss&utm_campaign=rss) .


Sponsor Details:

Ensure your online privacy by using NordVPN . To get our special listener deal and save a lot of money, visit You'll be glad you did!


Become a supporter of Astronomy Daily by joining our Supporters Club. Commercial free episodes daily are only a click way... Click Here (https://www.spreaker.com/podcast/astronomy-daily-space-news-updates--5648921/support)


This episode includes AI-generated content.

Episode link: https://play.headliner.app/episode/31073372?utm_source=youtube

Kind: captions Language: en
00:00:00 --> 00:00:03 Welcome to Astronomy Daily. I'm Anna.

00:00:03 --> 00:00:05 >> And I'm Avery. Hello everyone. Thanks

00:00:05 --> 00:00:08 for joining us. Today is January 12th,

00:00:08 --> 00:00:11 2026. And we've got a full show.

00:00:11 --> 00:00:13 Launches and anomalies, regulatory moves

00:00:14 --> 00:00:16 that reshape low Earth orbit, a brand

00:00:16 --> 00:00:19 new exoplanet observatory on its way, a

00:00:19 --> 00:00:22 flash from the cosmic dawn, fresh

00:00:22 --> 00:00:24 results about what powers the sun's

00:00:24 --> 00:00:26 strongest flares, and a galaxy discovery

00:00:26 --> 00:00:29 that looks surprisingly familiar for the

00:00:29 --> 00:00:30 early universe.

00:00:30 --> 00:00:33 >> Yep, six stories, all of them important

00:00:33 --> 00:00:35 in different ways. We'll start with this

00:00:35 --> 00:00:37 morning's launch news from India.

00:00:37 --> 00:00:40 India's polar satellite launch vehicle,

00:00:40 --> 00:00:42 the PSLVc62

00:00:42 --> 00:00:44 lifted off from Satic Darwin Space

00:00:44 --> 00:00:48 Center this morning carrying EOS-N1

00:00:48 --> 00:00:50 described as an advanced Earth

00:00:50 --> 00:00:52 observation/military

00:00:52 --> 00:00:54 surveillance satellite along with a

00:00:54 --> 00:00:56 batch of co-passenger payloads. The

00:00:56 --> 00:00:58 mission marked ISRO's first launch

00:00:58 --> 00:01:01 attempt since a PSLV anomaly in May

00:01:01 --> 00:01:04 2025. So, there was a lot writing on it,

00:01:04 --> 00:01:07 >> right? The liftoff itself looked

00:01:07 --> 00:01:09 nominal, but ISRO later reported an

00:01:09 --> 00:01:12 anomaly near the end of the third stage,

00:01:12 --> 00:01:15 the PS3. Initial public statements

00:01:15 --> 00:01:17 indicate a deviation in the third stages

00:01:17 --> 00:01:20 phase, and that ISRO has begun a

00:01:20 --> 00:01:22 detailed analysis. At this stage, it's

00:01:22 --> 00:01:25 not yet confirmed whether the primary

00:01:25 --> 00:01:27 satellite and co-passengers reached

00:01:27 --> 00:01:30 their planned orbits. Those early stage

00:01:30 --> 00:01:32 deviations can be especially challenging

00:01:32 --> 00:01:34 because they often happen during staging

00:01:34 --> 00:01:37 or engine cutoff phases where timing and

00:01:37 --> 00:01:40 velocity are critical. ISRO has a long

00:01:40 --> 00:01:43 successful history with the PSLV family.

00:01:43 --> 00:01:45 But even reliable vehicles can have

00:01:45 --> 00:01:47 single event anomalies. The important

00:01:47 --> 00:01:49 thing is how the agency responds.

00:01:49 --> 00:01:52 Recovering telemetry, diagnosing the

00:01:52 --> 00:01:54 root cause, and transparently sharing

00:01:54 --> 00:01:56 findings so confidence can be rebuilt.

00:01:56 --> 00:01:59 >> Absolutely. From a broader perspective,

00:01:59 --> 00:02:01 this mission also demonstrates the

00:02:01 --> 00:02:04 global nature of small sat ride shares

00:02:04 --> 00:02:06 and the strategic value that Earth

00:02:06 --> 00:02:08 observation satellites deliver, whether

00:02:08 --> 00:02:11 for commercial or defense purposes.

00:02:11 --> 00:02:13 We'll keep an eye on ISRO's follow-up.

00:02:13 --> 00:02:15 They typically publish an analysis after

00:02:15 --> 00:02:17 they comb through flight data.

00:02:17 --> 00:02:18 >> And we'll link to the official

00:02:18 --> 00:02:20 statements in the episode notes for

00:02:20 --> 00:02:23 folks who want the primary sources. Next

00:02:23 --> 00:02:25 up in the US, the Federal Communications

00:02:25 --> 00:02:28 Commission granted SpaceX authorization

00:02:28 --> 00:02:32 to deploy an additional 7500 Starlink

00:02:32 --> 00:02:34 second generation satellites. That's a

00:02:34 --> 00:02:37 partial approval within a broader SpaceX

00:02:37 --> 00:02:40 request for up to 15 Gen 2.

00:02:40 --> 00:02:42 >> This is a big step for the company's

00:02:42 --> 00:02:45 plan to upgrade Starlink's capabilities.

00:02:45 --> 00:02:47 higher throughput, lower latency, and

00:02:47 --> 00:02:49 expanded services, including directto

00:02:49 --> 00:02:52 cell connectivity and higher data rates.

00:02:52 --> 00:02:55 The FCC's partial grant means SpaceX can

00:02:55 --> 00:02:56 move forward with a substantial

00:02:56 --> 00:02:58 expansion while regulators and other

00:02:58 --> 00:03:01 stakeholders continue to evaluate the

00:03:01 --> 00:03:03 remainder of the proposal. There are a

00:03:03 --> 00:03:05 couple of important implications

00:03:05 --> 00:03:08 operationally. Many more Starlink nodes

00:03:08 --> 00:03:10 in low Earth orbit will increase global

00:03:10 --> 00:03:13 broadband capacity, particularly for

00:03:13 --> 00:03:15 underserved and rural regions. But it

00:03:16 --> 00:03:18 also intensifies ongoing concerns about

00:03:18 --> 00:03:21 orbital crowding, radio frequency

00:03:21 --> 00:03:23 coordination, and long-term space

00:03:23 --> 00:03:24 sustainability.

00:03:24 --> 00:03:27 >> Right? Competitors and some academics

00:03:27 --> 00:03:29 have raised worries about spectrum

00:03:29 --> 00:03:31 interference, orbital dominance, and the

00:03:31 --> 00:03:33 cumulative effect of so many satellites

00:03:33 --> 00:03:35 on debris risk and astronomical

00:03:35 --> 00:03:37 observing. SpaceX says it will

00:03:37 --> 00:03:39 coordinate reconfiguration steps, for

00:03:39 --> 00:03:42 example, lowering orbits for safety and

00:03:42 --> 00:03:44 using de-orbiting strategies, but

00:03:44 --> 00:03:46 regulators and the international

00:03:46 --> 00:03:48 community will be watching closely.

00:03:48 --> 00:03:51 >> So, this is both a technical and policy

00:03:51 --> 00:03:53 story. The authorization moves the

00:03:53 --> 00:03:55 technology forward, but it also keeps

00:03:56 --> 00:03:58 the conversation going about how to

00:03:58 --> 00:04:00 manage low Earth orbit responsibly as it

00:04:00 --> 00:04:01 becomes busier.

00:04:01 --> 00:04:04 >> On a more exploratory note, SpaceX

00:04:04 --> 00:04:07 successfully launched a Falcon 9 right

00:04:07 --> 00:04:09 share mission that included NASA's

00:04:09 --> 00:04:11 Pandora satellite. Pandora is a compact

00:04:12 --> 00:04:13 astrophysics mission designed to study

00:04:14 --> 00:04:16 the atmospheres of at least 20

00:04:16 --> 00:04:18 exoplanets and their host stars over

00:04:18 --> 00:04:21 about a year of operations. Pandora's

00:04:21 --> 00:04:23 key strength is that it's optimized to

00:04:23 --> 00:04:24 disentangle the light coming from an

00:04:24 --> 00:04:27 exoplanet and the star it orbits.

00:04:27 --> 00:04:29 Stellar activity, spots, flares, and

00:04:29 --> 00:04:32 magnetic variability can mimic or mask

00:04:32 --> 00:04:34 atmospheric signals from exoplanets.

00:04:34 --> 00:04:37 Pandora carries a 045 meter telescope

00:04:37 --> 00:04:39 and a suite of instruments aimed at

00:04:39 --> 00:04:42 measuring both the stars variability and

00:04:42 --> 00:04:44 the planet's transmission signals,

00:04:44 --> 00:04:46 improving the accuracy of atmospheric

00:04:46 --> 00:04:48 composition measurements. That kind of

00:04:48 --> 00:04:50 targeted mission is exactly what the

00:04:50 --> 00:04:52 exoplanet community needs. Now, large

00:04:52 --> 00:04:56 observatories like JWST do outstanding

00:04:56 --> 00:04:59 detailed work, but focused missions such

00:04:59 --> 00:05:01 as Pandora can observe many systems in a

00:05:02 --> 00:05:04 systematic way and help build context.

00:05:04 --> 00:05:07 Pandora will feed into priorities for

00:05:07 --> 00:05:09 future larger missions that aim to

00:05:09 --> 00:05:11 detect specific molecules, even bio

00:05:11 --> 00:05:14 signatures in exoplanet atmospheres.

00:05:14 --> 00:05:16 It's also another example of efficient

00:05:16 --> 00:05:19 ride share launches enabling specialized

00:05:19 --> 00:05:22 science payloads. Pandora joining a

00:05:22 --> 00:05:24 larger commercial launch shows how the

00:05:24 --> 00:05:26 landscape of getting small science

00:05:26 --> 00:05:28 spacecraft to orbit has matured.

00:05:28 --> 00:05:30 >> Turning to the distant universe,

00:05:30 --> 00:05:32 astronomers recently reported detecting

00:05:32 --> 00:05:35 a very brief 10-second flash that

00:05:35 --> 00:05:37 originated roughly 13 billion lighty

00:05:37 --> 00:05:40 years away. This is being interpreted as

00:05:40 --> 00:05:42 light from an extremely distant

00:05:42 --> 00:05:44 supernova. One of the farthest, if not

00:05:44 --> 00:05:46 the farthest, stellar explosions

00:05:46 --> 00:05:47 observed so far.

00:05:47 --> 00:05:49 >> The detection combined data from

00:05:49 --> 00:05:52 multiple instruments, including wide

00:05:52 --> 00:05:54 field X-ray monitors and follow-on

00:05:54 --> 00:05:56 observations by facilities such as the

00:05:56 --> 00:05:59 James Web Space Telescope. The event is

00:05:59 --> 00:06:01 remarkable because it lets astronomers

00:06:01 --> 00:06:04 study stellar death and the environments

00:06:04 --> 00:06:06 of massive stars in the early universe

00:06:06 --> 00:06:08 when galaxies were young and metal

00:06:08 --> 00:06:10 content was low.

00:06:10 --> 00:06:12 >> Observing such distant explosions is

00:06:12 --> 00:06:14 rare because cosmological red shift and

00:06:14 --> 00:06:17 faintness make them hard to spot. When

00:06:17 --> 00:06:19 one is found, it can reveal the

00:06:19 --> 00:06:21 properties of the progenitor star, the

00:06:21 --> 00:06:23 host galaxy, and the intergalactic

00:06:23 --> 00:06:25 medium at a time when cosmic structure

00:06:25 --> 00:06:28 was still forming. There are also ties

00:06:28 --> 00:06:30 to gamma ray bursts and extreme

00:06:30 --> 00:06:32 transient phenomena. Researchers will be

00:06:32 --> 00:06:34 investigating whether models for super

00:06:34 --> 00:06:37 luminous supernova or exotic explosions

00:06:37 --> 00:06:38 match this event.

00:06:38 --> 00:06:40 >> This detection emphasizes how

00:06:40 --> 00:06:43 multi-wavelength coordinated observing

00:06:43 --> 00:06:45 campaigns. Fast alerts from one

00:06:45 --> 00:06:48 instrument followed by deep telescope

00:06:48 --> 00:06:50 follow-up are essential for studying the

00:06:50 --> 00:06:53 transient universe, especially at high

00:06:53 --> 00:06:55 red shift. Back closer to home, solar

00:06:55 --> 00:06:57 physicists have new insight into the

00:06:57 --> 00:06:59 engine behind the sun's most violent

00:07:00 --> 00:07:02 flares and the intense gamma rays they

00:07:02 --> 00:07:04 sometimes unleash. Researchers

00:07:04 --> 00:07:06 identified a previously unrecognized

00:07:06 --> 00:07:08 population of extremely energetic

00:07:08 --> 00:07:11 particles in the sun's upper atmosphere

00:07:11 --> 00:07:13 that appear to be a major source of

00:07:13 --> 00:07:16 those high energy photons. The finding

00:07:16 --> 00:07:18 comes from combining longduration

00:07:18 --> 00:07:20 observations and specialized instruments

00:07:20 --> 00:07:22 capable of measuring particle

00:07:22 --> 00:07:25 populations and gammaray signatures. The

00:07:25 --> 00:07:28 upshot is that magnetic reconnection and

00:07:28 --> 00:07:31 particle acceleration processes in flare

00:07:31 --> 00:07:33 regions are more complex than some

00:07:33 --> 00:07:36 simple models suggested. In particular,

00:07:36 --> 00:07:37 the upper layers of the solar

00:07:37 --> 00:07:39 atmosphere, where magnetic fields

00:07:39 --> 00:07:42 reconnect and release energy, can trap

00:07:42 --> 00:07:44 and accelerate particles to mega

00:07:44 --> 00:07:46 electron volts, energies that then

00:07:46 --> 00:07:48 produce gamma rays.

00:07:48 --> 00:07:49 >> This matters for space weather

00:07:49 --> 00:07:51 prediction. Gamma rays and energetic

00:07:52 --> 00:07:54 particles accompany the most extreme

00:07:54 --> 00:07:56 flares and can affect satellites, radio

00:07:56 --> 00:07:59 communications, and radiation exposure

00:07:59 --> 00:08:01 for astronauts and high-flying aircraft.

00:08:01 --> 00:08:03 By better understanding where and how

00:08:03 --> 00:08:05 particles are accelerated, models of

00:08:06 --> 00:08:08 flare impact and forecasts of space

00:08:08 --> 00:08:09 weather can be improved.

00:08:09 --> 00:08:12 >> It's also a good reminder that our sun

00:08:12 --> 00:08:15 still surprises us. Even with decades of

00:08:15 --> 00:08:17 observations and multiple solar

00:08:17 --> 00:08:19 missions, new diagnostics and longer

00:08:19 --> 00:08:22 observation windows revealed previously

00:08:22 --> 00:08:23 hidden physics.

00:08:23 --> 00:08:25 >> Finally, one of the most visually

00:08:25 --> 00:08:28 intriguing stories. Astronomers have

00:08:28 --> 00:08:30 identified a barred spiral galaxy whose

00:08:30 --> 00:08:33 light comes from approximately 11.5

00:08:34 --> 00:08:36 billion years ago about 2 billion years

00:08:36 --> 00:08:39 after the Big Bang. If confirmed, this

00:08:39 --> 00:08:41 object would be among the earliest bars

00:08:41 --> 00:08:43 and spiral structures seen in the

00:08:43 --> 00:08:44 universe.

00:08:44 --> 00:08:47 >> Bars are elongated stellar structures

00:08:47 --> 00:08:49 that can drive internal evolution in

00:08:49 --> 00:08:51 galaxies. They funnel gas toward the

00:08:51 --> 00:08:54 center, trigger star formation, and

00:08:54 --> 00:08:57 rearrange angular momentum. Finding a

00:08:57 --> 00:08:59 well-defined bar so early means that

00:08:59 --> 00:09:01 disc galaxies could develop mature

00:09:01 --> 00:09:03 internal structures sooner than many

00:09:03 --> 00:09:04 models predicted.

00:09:04 --> 00:09:06 >> The discovery was enabled by deep

00:09:06 --> 00:09:09 spectroscopically confirmed imaging from

00:09:09 --> 00:09:11 powerful telescopes, Hubble and other

00:09:11 --> 00:09:14 facilities and careful analysis of the

00:09:14 --> 00:09:16 galaxy's stellar and morphological

00:09:16 --> 00:09:18 properties. The object sits in a growing

00:09:18 --> 00:09:21 collection of surprising early galaxies.

00:09:21 --> 00:09:23 Some are massive and evolved earlier

00:09:23 --> 00:09:26 than expected. Others show complex

00:09:26 --> 00:09:28 morphologies previously thought to

00:09:28 --> 00:09:30 require long time scales to form.

00:09:30 --> 00:09:33 >> These results feed directly into galaxy

00:09:33 --> 00:09:35 formation theory. They force modelers to

00:09:35 --> 00:09:38 consider rapid disc settling, efficient

00:09:38 --> 00:09:40 angular momentum redistribution and

00:09:40 --> 00:09:42 other processes that could build bars

00:09:42 --> 00:09:44 early. It's an exciting reminder that

00:09:44 --> 00:09:47 the early universe may have been both

00:09:47 --> 00:09:49 more active and more varied than our

00:09:49 --> 00:09:52 simplest expectations. So looking across

00:09:52 --> 00:09:54 today's stories, we have an operational

00:09:54 --> 00:09:56 launch with an anomaly that will require

00:09:56 --> 00:09:59 analysis, a regulatory decision that

00:09:59 --> 00:10:02 reshapes near Earth space, a dedicated

00:10:02 --> 00:10:05 exoplanet mission now in orbit, a signal

00:10:05 --> 00:10:07 from the cosmic dawn giving a rare

00:10:07 --> 00:10:10 window into early stellar deaths,

00:10:10 --> 00:10:12 improved understanding of particle

00:10:12 --> 00:10:14 acceleration on the sun, and an early

00:10:14 --> 00:10:17 galaxy that challenges our ideas of how

00:10:17 --> 00:10:19 quickly structure forms. It's a nice

00:10:19 --> 00:10:22 mix, isn't it? Local space operations

00:10:22 --> 00:10:24 and policy, near-earth infrastructure

00:10:24 --> 00:10:27 and its implications, targeted planetary

00:10:27 --> 00:10:30 science, time domain extragalactic

00:10:30 --> 00:10:32 astronomy, solar physics, and

00:10:32 --> 00:10:34 cosmological structure formation. For

00:10:34 --> 00:10:36 listeners, it shows how broad and

00:10:36 --> 00:10:38 interconnected modern astronomy and

00:10:38 --> 00:10:40 space activity are.

00:10:40 --> 00:10:42 >> Two quick takeaways. First, watch for

00:10:42 --> 00:10:45 ISRO's followup on the PSLV anomaly.

00:10:46 --> 00:10:47 that will affect launch schedules and

00:10:47 --> 00:10:50 the broader small sack community.

00:10:50 --> 00:10:52 Second, the more we push instruments and

00:10:52 --> 00:10:54 coordination like fast transients and

00:10:54 --> 00:10:57 small science satellites, the more

00:10:57 --> 00:10:59 corner cases we find that reshape

00:10:59 --> 00:11:01 theory. Discoveries often come when new

00:11:02 --> 00:11:03 instruments or different organizational

00:11:04 --> 00:11:06 approaches are applied. And for the

00:11:06 --> 00:11:07 non-scientists out there wondering what

00:11:08 --> 00:11:10 to look for tonight, Jupiter is still a

00:11:10 --> 00:11:12 good target if you're out stargazing.

00:11:12 --> 00:11:14 and aurora watchers should keep an eye

00:11:14 --> 00:11:16 on space weather forecasts as the sun's

00:11:16 --> 00:11:18 activity continues to produce strong

00:11:18 --> 00:11:19 events.

00:11:19 --> 00:11:21 >> That's it for today's episode. If you

00:11:21 --> 00:11:23 enjoyed the show, subscribe to Astronomy

00:11:23 --> 00:11:25 Daily on your preferred podcast

00:11:25 --> 00:11:28 platform. You can find links, source

00:11:28 --> 00:11:29 articles, and further reading in the

00:11:29 --> 00:11:31 episode notes so you can dig deeper if

00:11:31 --> 00:11:32 you wish.

00:11:32 --> 00:11:34 >> We love hearing from listeners. If you

00:11:34 --> 00:11:36 have questions, science topics you'd

00:11:36 --> 00:11:38 like us to cover, or feedback about the

00:11:38 --> 00:11:40 show, drop us a note through the

00:11:40 --> 00:11:42 Astronomy Daily website. You can find us

00:11:42 --> 00:11:44 at astronomydaily.io.

00:11:44 --> 00:11:46 >> Thanks for listening. I'm Avery

00:11:46 --> 00:11:49 >> and I'm Anna. Clear skies and we'll see

00:11:49 --> 00:11:51 you tomorrow on Astronomy Daily.

00:11:51 --> 00:12:10 >> Astronomy Daily.

00:12:10 --> 00:12:14 Stories were told.