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

Looking for excitement?

Chamba Casino is here.

Play any time, play anywhere.

Play on the train, play at the store, play at home,

play when you're bored.

Play today for your chance to win and get daily bonuses

when you log in.

So what are you waiting for?

Don't delay.

Chamba Casino is free to play.

Experience social gameplay like never before.

Go to Chamba Casino right now to play hundreds of games,

including online slots, bingo, slingo, and more.

Live the Chamba Life at chambacasino.com.

Don't purchase necessary VGW group void for prohibited by law

21 plus terms and conditions apply.

Welcome to Astronomy Daily.

I'm Anna.

And I'm Avery.

Hello, everyone.

Thanks for joining us.

Today is January 12, 2026.

And we've got a full show.

Launches and anomalies, regulatory moves

that reshape low-earth orbit, a brand-new exoplanet

observatory on its way, a flash from the cosmic dawn.

Fresh results about what powers the sun's strongest

flares, and a galaxy discovery that

looks surprisingly familiar for the early universe.

Yep, six stories.

All of them important in different ways.

We'll start with this morning's launch news from India.

India's polar satellite launch vehicle, the PSLV-C-62,

lifted off from Satish Darwin Space Center this morning,

carrying EOS-N1.

Described as an advanced Earth observation slash military

surveillance satellite, along with

the batch of co-passenger payloads,

the mission marked ISRO's first launch attempt

since a PSLV anomaly in May 2025.

So there was a lot writing on it.

Right, the lift off itself looked nominal,

but ISRO later reported an anomaly

near the end of the third stage, the PS3.

Initial public statements indicate a deviation

in the third stage's phase, and that ISRO

has begun a detailed analysis.

At this stage, it's not yet confirmed

whether the primary satellite and co-passengers

reached their planned orbits.

Those early stage deviations can be especially challenging,

because they often happen during staging

or engine cutoff phases, where timing and velocity

are critical.

ISRO has a long successful history

with the PSLV family, but even reliable vehicles

can have single event anomalies.

The important thing is how the agency responds,

recovering telemetry, diagnosing the root cause

and transparently sharing findings

so confidence can be rebuilt.

Absolutely.

From a broader perspective, this mission also

demonstrates the global nature of small-sat ride shares

and the strategic value that Earth observation satellites

deliver, whether for commercial or defense purposes.

We'll keep an eye on ISRO's follow-up.

They typically publish an analysis

after they comb through flight data.

And we'll link to the official statements

in the episode notes for folks who want the primary sources.

Next up in the US, the Federal Communications Commission

granted SpaceX authorization to deploy

an additional 7500 Starlink second-generation satellites.

That's a partial approval within a broader SpaceX request

for up to 15,000 Gen2.

This is a big step for the company's plan

to upgrade Starlink's capabilities.

Higher throughput, lower latency, and expanded services,

including direct-to-cell connectivity and higher data

rates.

The FCC's partial grant means SpaceX

can move forward with a substantial expansion,

while regulators and other stakeholders

continue to evaluate the remainder of the proposal.

There are a couple of important implications.

Operationally, many more Starlink nodes in low-Earth orbit

will increase global broadband capacity, particularly

for underserved and rural regions.

But it also intensifies ongoing concerns

about orbital crowding, radio frequency coordination,

and long-term space sustainability.

Right.

Competitors and some academics have raised worries

about spectrum interference, orbital dominance,

and the cumulative effect of so many satellites

on debris risk and astronomical observing.

SpaceX says it will coordinate reconfiguration steps,

for example, lowering orbits for safety,

and using the orbiting strategies.

But regulators and the international community

will be watching closely.

So this is both a technical and policy story.

The authorization moves the technology forward,

but it also keeps the conversation going

about how to manage low-Earth orbit responsibly

as it becomes busier.

On a more exploratory note, SpaceX successfully

launched a Falcon 9 right-share mission

that included NASA's Pandora satellite.

Pandora's a compact astrophysics mission,

designed to study the atmospheres of at least 20

exoplanets and their hostars over about a year of operations.

Pandora's key strength is that it's

optimized to disentangle the light coming from an exoplanet

and the star at orbits.

Stellar activity, spots, flares, and magnetic variability

can mimic or mask atmospheric signals from exoplanets.

Pandora carries a 0.45-meter telescope

and a suite of instruments aimed at measuring both the star's

variability and the planet's transmission signals,

improving the accuracy of atmospheric composition

measurements.

That kind of targeted mission is exactly

what the exoplanet community needs now.

Large observatories like JWST do outstanding detailed work,

but focused missions such as Pandora

can observe many systems in a systematic way

and help build context.

Pandora will feed into priorities for future larger missions

that aim to detect specific molecules,

even biosignatures in exoplanet atmospheres.

It's also another example of efficient ride-share launches

enabling specialized science payloads.

Pandora joining a larger commercial launch

shows how the landscape of getting small science spacecraft

to orbit has matured.

Turning to the distant universe, astronomers recently

reported detecting a very brief 10-second flash

that originated roughly 13 billion light years away.

This is being interpreted as light from an extremely distant

supernova, one of the farthest, if not the farthest,

stellar explosions observed so far.

The detection combined data from multiple instruments,

including wide field x-ray monitors

and follow-on observations by facilities

such as the James Webb Space Telescope.

The event is remarkable because it

lets astronomers study stellar death

and the environments of massive stars

in the early universe when galaxies were young

and metal content was low.

Observing such distant explosions is rare

because cosmological redshift and faintness

make them hard to spot.

When one is found, it can reveal the properties

of the progenitor star, the host galaxy,

and the intergalactic medium at a time

when cosmic structure will still forming.

There are also ties to gamma-ray bursts

and extreme transient phenomena.

Researchers will be investigating whether models

for superluminous supernovae or exotic explosions

match this event.

This detection emphasizes how multi-wavelength

coordinated observing campaigns, fast alerts from one instrument

followed by deep telescope follow-up,

are essential for studying the transient universe,

especially at high redshift.

Back closer to home, solar physicists

have new insight into the engine behind the sun's

most violent flares and the intense gamma-rays

they sometimes unleash.

Researchers identified a previously unrecognized population

of extremely energetic particles in the sun's upper atmosphere

that appeared to be a major source

of those high energy photons.

The finding comes from combining

long-duration observations and specialized instruments

capable of measuring particle populations and gamma-ray

signatures.

The upshot is that magnetic reconnection

and particle acceleration processes in flare regions

are more complex than some simple models suggested.

In particular, the upper layers of the solar atmosphere

where magnetic fields reconnect and release energy

can trap and accelerate particles to mega-electron volts

energies that then produce gamma rays.

This matters for space weather prediction.

Gamma rays and energetic particles

accompany the most extreme flares

and can affect satellites, radio communications,

and radiation exposure for astronauts

and high flying aircraft.

By better understanding where and how

particles are accelerated, models of flare impact

and forecast of space weather can be improved.

It's also a good reminder that our sun still surprises us,

even with decades of observations and multiple solar

missions, new diagnostics and longer observation

windows revealed previously hidden physics.

Finally, one of the most visually intriguing stories.

Astronomers have identified a barred spiral galaxy whose

light comes from approximately 11.5 billion years ago,

about 2 billion years after the Big Bang.

If confirmed, this object would be among the earliest bars

and spiral structures seen in the universe.

Bars are elongated stellar structures

that can drive internal evolution in galaxies.

They funnel gas toward the center, trigger star formation,

and rearrange angular momentum.

Finding a well-defined bar so early means

that disc galaxies could develop mature internal structures

sooner than many models predicted.

The discovery was enabled by deep spectroscopically confirmed

imaging from powerful telescopes, Hubble and other facilities,

and careful analysis of the galaxy's stellar

and morphological properties.

The object sits in a growing collection

of surprising early galaxies.

Some are massive and evolved earlier than expected.

Others show complex morphologies previously

thought to require long time scales to form.

These results feed directly into galaxy formation theory.

They force modelers to consider rapid disk settling,

efficient angular momentum redistribution,

and other processes that could build bars early.

It's an exciting reminder that the early universe

may have been both more active and more varied

than our simplest expectations.

So looking across today's stories,

we have an operational launch with an anomaly

that will require analysis, a regulatory decision

that reshapes near Earth space, a dedicated exoplanet mission

now in orbit, a signal from the cosmic dawn

giving a rare window into early stellar depths,

improved understanding of particle acceleration on the sun,

and an early galaxy that challenges our ideas

of how quickly structure forms.

It's a nice mix, isn't it?

Local space operations and policy, near-Earth infrastructure

and its implications, targeted planetary science,

time-domain extragalactic astronomy, solar physics,

and cosmological structure formation.

For listeners, it shows how broad and interconnected

modern astronomy and space activity are.

Two quick takeaways.

First, watch for Israel's follow-up on the PSLV anomaly.

That will affect launch schedules

and the broader small-sac community.

Second, the more we push instruments and coordination,

like fast transients and small science satellites,

the more corner cases we find that reshape theory.

Discoveries often come when new instruments

or different organizational approaches are applied.

And for the non-scientists out there

wondering what to look for tonight,

Jupiter is still a good target if you're out stargazing.

And Aurora Watchers should keep an eye on space

weather forecasts as the sun's activity

continues to produce strong events.

That's it for today's episode.

If you enjoyed the show, subscribe to astronomy daily

on your preferred podcast platform.

You can find links, source articles, and further

reading in the episode notes, so you can dig deeper if you wish.

We love hearing from listeners.

If you have questions, science topics you'd like us to cover,

or feedback about the show, drop us a note

through the Astronomy Daily website.

You can find us at astronomydaily.io.

Thanks for listening.

I'm Avery.

And I'm Anna.

Clear skies, and we'll see you tomorrow on Astronomy Daily.

The star is the toe.

The star is the toe.

The star is the toe.

Hey, it's Cole Swindle.

And when I spend 200 days a year rolling down the highway,

the bus can start to feel smaller than a guitar case.

Everyone wonders how I stay chill while the hours crawl by.

Truth is, one good luck spent on Chamba,

and suddenly the trip does a whole lot shorter.

Find in your space even when there is a much despair.

Need some chill?

Let's Chamba.

No purchase necessary.

VGW Group Boyd were prohibited by law, 21 plus TNC supply.

Sponsored by Chamba Casino.