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The John Batchelor Show

S8 Ep510: Preview for later today: Astronomer Kishalay De discusses a supernova from a 13-solar-mass star, challenging theories that only larger stars explode and revealing complexities in predicting stellar deaths.

The John Batchelor Show

John Batchelor

Arts, News, Society & Culture, Books

4.52.8K Ratings

🗓️ 24 February 2026

⏱️ 2 minutes

🧾️ Download transcript

Summary

Preview for later today: Astronomer Kishalay De discusses a supernova from a 13-solar-mass star, challenging theories that only larger stars explode and revealing complexities in predicting stellar deaths.
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Transcript

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0:00.0

This is John Batchel.

0:02.1

Conversation with the astronomer Kishelay Day of Columbia University.

0:06.7

He and his team have discovered, have revealed a supernova that begins with a much smaller sun, star, than was heretofore assumed.

0:19.4

13 solar masses.

0:21.7

It was assumed you needed to be much higher to turn into a supernova

0:25.6

and then turn into a black hole.

0:29.7

This very likely increases the audit when and if it happens

0:34.2

of black holes in the immediate region of the Milky Way,

0:39.2

but globally, no, cosmically, much larger.

0:44.5

Kishlai Day describing what they discovered and how they want more information,

0:50.4

what makes it happen.

0:52.8

Much more of this tonight.

0:56.0

Professor Kishelay Day, Columbia University.

1:00.0

Supernovas, black holes, and what?

1:04.8

More of this tonight?

1:07.4

So that's a good question.

1:09.1

I think it's still quite up in the air. that's primarily because what we know is that stars in this mass range, 13 solar masses or so, we do know that some of them do explode, but clearly this one did not. So what that means is that whether a star decides to explode or not explode might not be uniquely determined

1:29.5

by its mass. There might be other processes, maybe processes that are somewhat chaotic even,

1:36.1

in that you can't predict it beforehand of whether a star is able to explode at the end of its

1:41.3

life. So, you know, to make a prediction like that, one would have to assume certain things about what mass

1:48.0

ranges to start explode, starts explode in, but this discovery really makes that much more

1:52.6

complicated because it shows that stars at very similar masses can either explode or not

...

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