Anomalies in India's Launch| SpaceX's Starlink Expansion| Cosmic Dawn Signals: Your Daily Space Update
Astronomy Daily: Space News UpdatesJanuary 12, 2026x
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00:12:1511.27 MB

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

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.
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## 📰 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
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This episode includes AI-generated content.


00:00:00 --> 00:00:03 Anna: Welcome to Astronomy Daily. I'm Anna.

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

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

00:00:08 --> 00:00:10 2026 and we've got a full show,

00:00:11 --> 00:00:14 launches and anomalies, regulatory moves that

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

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

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

00:00:22 --> 00:00:24 about what powers the sun's, um, strongest

00:00:24 --> 00:00:27 flares and a galaxy discovery that looks

00:00:27 --> 00:00:29 surprisingly familiar for the early universe.

00:00:30 --> 00:00:33 Anna: Yep, 6stor. All of them important in

00:00:33 --> 00:00:34 different ways.

00:00:34 --> 00:00:36 We'll start with this morning's launch news

00:00:36 --> 00:00:37 from India.

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

00:00:40 --> 00:00:43 PSLV C62 lifted off

00:00:43 --> 00:00:45 from Satish Dhawan Space Centre this morning

00:00:45 --> 00:00:48 carrying EOS N1,

00:00:48 --> 00:00:51 described as an advanced Earth Observation

00:00:51 --> 00:00:54 military surveillance satellite, along with a

00:00:54 --> 00:00:57 batch of CO passenger payloads. The mission

00:00:57 --> 00:00:59 marked ISRO's first launch attempt since a

00:00:59 --> 00:01:02 PSLV anomaly in May 2025.

00:01:02 --> 00:01:05 So there was on it, right?

00:01:05 --> 00:01:07 Anna: The liftoff itself looked nominal, but

00:01:07 --> 00:01:10 ISRO later reported an anomaly near the end

00:01:10 --> 00:01:13 of the third stage. The PS3.

00:01:13 --> 00:01:15 Initial public statements indicate a, uh,

00:01:15 --> 00:01:18 deviation in the third stage's phase and that

00:01:18 --> 00:01:21 ISRO has begun a detailed analysis.

00:01:21 --> 00:01:24 At this stage it's not yet confirmed whether

00:01:24 --> 00:01:26 the primary satellite and co passengers

00:01:26 --> 00:01:28 reached their planned orbits.

00:01:28 --> 00:01:31 Avery: Those early stage deviations can be

00:01:31 --> 00:01:33 especially challenging because they often

00:01:33 --> 00:01:35 happen during staging or engine cutoff

00:01:36 --> 00:01:38 where timing and velocity are critical.

00:01:38 --> 00:01:41 ISRO has a long successful history with the

00:01:41 --> 00:01:44 PSLV family. But even reliable vehicles

00:01:44 --> 00:01:47 can have single event anomalies. The

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

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

00:01:52 --> 00:01:55 cause and transparently sharing findings. So

00:01:55 --> 00:01:56 confidence can be rebuilt.

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

00:01:59 --> 00:02:02 mission also demonstrates the global nature

00:02:02 --> 00:02:05 of smallsat rideshares and the strategic

00:02:05 --> 00:02:07 value that Earth Observation Satellite

00:02:07 --> 00:02:10 deliver, whether for commercial or defence

00:02:10 --> 00:02:12 purposes. We'll keep an eye on ISRO's follow

00:02:12 --> 00:02:15 up. They typically publish an analysis after

00:02:15 --> 00:02:18 they comb through flight data and we'll link.

00:02:18 --> 00:02:20 Avery: To the official statements in the episode

00:02:20 --> 00:02:22 notes for folks who want the primary sources

00:02:22 --> 00:02:23 next up.

00:02:23 --> 00:02:25 Anna: In the US the Federal Communications

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

00:02:28 --> 00:02:31 to deploy an additional 7

00:02:31 --> 00:02:33 Starlink second generation satellites.

00:02:34 --> 00:02:36 That's a, uh, partial approval within a

00:02:36 --> 00:02:39 broader SpaceX request for up to 15

00:02:39 --> 00:02:40 in Gen 2.

00:02:40 --> 00:02:43 Avery: This is a big step for the company's plan to

00:02:43 --> 00:02:45 upgrade Starlink's capabilities. Higher

00:02:45 --> 00:02:48 throughput, lower latency and expanded

00:02:48 --> 00:02:50 services including direct to cell

00:02:50 --> 00:02:52 connectivity and higher Data rates. The

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

00:02:55 --> 00:02:57 forward with a substantial expansion while

00:02:57 --> 00:03:00 regulators and Other stakeholders continue to

00:03:00 --> 00:03:02 evaluate the remainder of the proposal.

00:03:02 --> 00:03:05 Anna: There are a 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 broadb capacity, particularly for

00:03:13 --> 00:03:16 underserved and rural regions. But it also

00:03:16 --> 00:03:19 intensifies ongoing concerns about orbital

00:03:19 --> 00:03:21 crowding, radio frequency coordination

00:03:21 --> 00:03:24 and long term space sustainability.

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

00:03:27 --> 00:03:29 raised worries about spectrum interference,

00:03:29 --> 00:03:32 orbital dominance, and the cumulative effect

00:03:32 --> 00:03:34 of so many satellites on debris risk and

00:03:34 --> 00:03:37 astronomical observing. SpaceX says it

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

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

00:03:42 --> 00:03:45 DEORB strategies. But regulators and the

00:03:45 --> 00:03:47 international community will be watching

00:03:47 --> 00:03:49 closely, so this is both.

00:03:49 --> 00:03:52 Anna: A technical and policy storey. The

00:03:52 --> 00:03:54 authorization moves the technology forward,

00:03:54 --> 00:03:57 but it also keeps the conversation going

00:03:57 --> 00:03:59 about how to manage low Earth orbit

00:03:59 --> 00:04:01 responsibly as it becomes busier.

00:04:01 --> 00:04:03 Avery: On a More exploratory note,

00:04:03 --> 00:04:06 SpaceX successfully launched a Falcon 9

00:04:06 --> 00:04:08 rideshare mission that included NASA's

00:04:08 --> 00:04:11 Pandora satellite. Pandora is a compact

00:04:11 --> 00:04:14 astrophysics mission designed to study the

00:04:14 --> 00:04:17 atmospheres Least 20 exoplanets

00:04:17 --> 00:04:19 and their host stars over about a year of

00:04:19 --> 00:04:19 operations.

00:04:20 --> 00:04:22 Anna: Pandora's key strength is that it's optimised

00:04:22 --> 00:04:24 to disentangle the light coming from an

00:04:24 --> 00:04:26 exoplanet and the star it orbits.

00:04:27 --> 00:04:30 Stellar activity, spots, flares and magnetic

00:04:30 --> 00:04:33 variability can mimic or mask atmospheric

00:04:33 --> 00:04:36 signals from exoplanets. Pandorna carries a

00:04:36 --> 00:04:38 0.45-metre telescope and a suite of

00:04:38 --> 00:04:40 instruments aimed at measuring both the

00:04:40 --> 00:04:43 star's variability and the planet's

00:04:43 --> 00:04:45 transmission signals, improving the accuracy

00:04:45 --> 00:04:47 of atmospheric composition measure.

00:04:47 --> 00:04:50 Avery: That kind of targeted mission is exactly what

00:04:50 --> 00:04:52 the exoplanet community needs now. Large

00:04:52 --> 00:04:55 observatories like JWST do

00:04:55 --> 00:04:57 outstanding detailed work, but

00:04:57 --> 00:05:00 focused missions such as Pandora can observe

00:05:00 --> 00:05:03 many systems in a systematic way and help

00:05:03 --> 00:05:06 build context. Pandora will feed into

00:05:06 --> 00:05:09 priorities for future larger missions that

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

00:05:11 --> 00:05:14 biosignatures, in exoplanet atmospheres.

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

00:05:16 --> 00:05:19 rideshare launches enabling specialised

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 spacecraft

00:05:26 --> 00:05:27 to orbit has matured.

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

00:05:30 --> 00:05:33 recently reported detecting a very brief 10

00:05:33 --> 00:05:36 second flash that originated roughly 13

00:05:37 --> 00:05:39 billion light years away. This is being

00:05:39 --> 00:05:41 interpreted as light from an extremely

00:05:41 --> 00:05:44 distant supernova, one of the farthest, if

00:05:44 --> 00:05:47 not the farthest, stellar explosions observed

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

00:05:47 --> 00:05:50 Anna: The detection combined data from multiple

00:05:50 --> 00:05:53 instruments, including wide field X ray

00:05:53 --> 00:05:55 monitors and follow on observations by

00:05:55 --> 00:05:57 facilities such as the James Webb Space

00:05:57 --> 00:06:00 Telescope. The event is remarkable

00:06:00 --> 00:06:02 because it lets astronomers study stellar

00:06:02 --> 00:06:05 death and the environments of massive stars

00:06:05 --> 00:06:07 in the early universe when galaxies were

00:06:07 --> 00:06:09 young and metal content was low.

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

00:06:12 --> 00:06:15 because cosmological redshift and faintness

00:06:15 --> 00:06:18 make them hard to spot. When one is found, it

00:06:18 --> 00:06:20 can reveal the properties of the progenitor

00:06:20 --> 00:06:22 star, the host galaxy and the

00:06:22 --> 00:06:25 intergalactic medium at a time when cosmic

00:06:25 --> 00:06:27 structure was still forming. There are also

00:06:27 --> 00:06:30 ties 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 supernovae or exotic explosions

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

00:06:38 --> 00:06:41 Anna: This detection emphasises how multi

00:06:41 --> 00:06:44 wavelength coordinated observing campaigns,

00:06:44 --> 00:06:47 fast alerts from one instrument followed by

00:06:47 --> 00:06:49 deep telescope follow up are essential for

00:06:49 --> 00:06:52 studying the transient universe, especially

00:06:52 --> 00:06:53 at high redshift.

00:06:54 --> 00:06:56 Avery: Back closer to home, solar physicists have

00:06:56 --> 00:06:59 new insight into the engine behind the sun's

00:06:59 --> 00:07:01 most violent flares and the intense gamma

00:07:01 --> 00:07:04 rays they sometimes unleash. Researchers

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

00:07:06 --> 00:07:09 population of extremely energetic particles

00:07:09 --> 00:07:12 in the sun's upper atmosphere that appear to

00:07:12 --> 00:07:14 be a major source of those high energy

00:07:14 --> 00:07:15 photons.

00:07:15 --> 00:07:17 Anna: The finding comes from combining long

00:07:17 --> 00:07:20 duration observations and specialised

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

00:07:22 --> 00:07:25 populations and gamma ray signatures.

00:07:25 --> 00:07:28 The 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 simple

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

00:07:36 --> 00:07:38 layers of the solar atmosphere, where

00:07:38 --> 00:07:41 magnetic fields reconnect and release energy,

00:07:41 --> 00:07:44 can track, trap and accelerate particles to

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

00:07:46 --> 00:07:47 produce gamma rays.

00:07:48 --> 00:07:50 Avery: This matters for space weather prediction.

00:07:50 --> 00:07:53 Gamma rays and energetic particles accompany

00:07:53 --> 00:07:55 the most extreme flares and can affect

00:07:55 --> 00:07:57 satellites, radio communications and

00:07:57 --> 00:08:00 radiation exposure for astronauts and high

00:08:00 --> 00:08:02 flying aircraft. By better understanding

00:08:02 --> 00:08:05 where and how particles are accelerated,

00:08:05 --> 00:08:07 models of flare, impact and forecasts of

00:08:07 --> 00:08:09 space weather can be improved.

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

00:08:12 --> 00:08:15 surprises us even with decades of

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

00:08:17 --> 00:08:20 New diagnostics and longer observation

00:08:20 --> 00:08:23 windows reveal previously hidden physics.

00:08:23 --> 00:08:26 Avery: Finally, one of the most visually intriguing

00:08:26 --> 00:08:28 storeys. Astronomers have identified a

00:08:28 --> 00:08:31 barred spiral galaxy whose light comes from

00:08:31 --> 00:08:34 approximately 11.5 billion

00:08:34 --> 00:08:37 years ago, about 2 billion years after the

00:08:37 --> 00:08:39 Big Bang. If confirmed, this object

00:08:39 --> 00:08:42 would be among the earliest bars and spiral

00:08:42 --> 00:08:44 structures seen in the universe.

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

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

00:08:50 --> 00:08:52 They funnel gas toward the centre, trigger

00:08:52 --> 00:08:55 star formation and rearrange angular

00:08:55 --> 00:08:58 momentum. Finding a well defined bar so

00:08:58 --> 00:09:00 early means that disc galaxies could develop

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

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

00:09:04 --> 00:09:06 Avery: 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 --> 00:09:13 facilities and careful analysis of the

00:09:13 --> 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 than

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

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

00:09:28 --> 00:09:30 long timescales to form.

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

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

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

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

00:09:40 --> 00:09:43 processes that could build bars early. It's

00:09:43 --> 00:09:45 an exciting reminder that the early universe

00:09:46 --> 00:09:48 may have been both more active and more

00:09:48 --> 00:09:50 varied than our simplest expectations.

00:09:51 --> 00:09:53 Avery: So, looking across today's storeys, we have

00:09:53 --> 00:09:55 an operational launch with an anomaly that

00:09:55 --> 00:09:58 will require analysis, a regulatory decision

00:09:59 --> 00:10:01 that reshapes near Earth space, a

00:10:01 --> 00:10:04 dedicated exoplanet mission now in orbit,

00:10:04 --> 00:10:07 a signal from the cosmic dawn giving a rare

00:10:07 --> 00:10:09 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 --> 00:10:18 quickly structure forms.

00:10:18 --> 00:10:21 Anna: It's a nice mix, isn't it? Local space

00:10:21 --> 00:10:24 operations and policy, Near Earth

00:10:24 --> 00:10:26 infrastructure and its implications Targeted

00:10:26 --> 00:10:29 planetary science domain

00:10:29 --> 00:10:32 extragalactic 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 space

00:10:38 --> 00:10:39 activity are.

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

00:10:42 --> 00:10:45 ISRO's follow up on the PSLV anomaly

00:10:45 --> 00:10:47 that will affect launch schedules and the

00:10:47 --> 00:10:50 broader smallsat community. Second,

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

00:10:53 --> 00:10:55 like fast transients and small science

00:10:55 --> 00:10:58 satellites, the more corner cases we find

00:10:58 --> 00:11:01 that reshape theory. Discoveries often come

00:11:01 --> 00:11:03 when new instruments or different

00:11:03 --> 00:11:05 organisational approaches are applied.

00:11:05 --> 00:11:07 Anna: And for the non scientists out there

00:11:07 --> 00:11:09 wondering what to look for tonight, Jupiter

00:11:09 --> 00:11:11 is still a good target if you're out

00:11:11 --> 00:11:13 stargazing, and aurora watchers should keep

00:11:13 --> 00:11:16 an eye on space weather forecasts as the

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

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

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

00:11:21 --> 00:11:24 the show, subscribe to Astronomy Daily on

00:11:24 --> 00:11:27 your preferred podcast platform. You can find

00:11:27 --> 00:11:29 links, source articles and further reading in

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

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

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

00:11:34 --> 00:11:37 questions, science topics you'd like us to

00:11:37 --> 00:11:39 cover, or feedback about the show, drop us a

00:11:39 --> 00:11:41 note through the Astronomy Daily website. You

00:11:41 --> 00:11:44 can find us@, uh, astronomydaily.IO

00:11:44 --> 00:11:45 thanks for listening.

00:11:45 --> 00:11:46 Avery: I'm Avery.

00:11:46 --> 00:11:49 Anna: And I'm Anna Clear Skies and we'll see you

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

00:11:51 --> 00:11:52 Avery: Astronomy Daily

00:11:54 --> 00:11:55 the Storeys we told.

00:12:02 --> 00:12:02 Storeys.

00:12:10 --> 00:12:11 We told.

00:12:14 --> 00:12:14 Anna: You m.