Previous: The Planets with Inside-Out Weather
Next: Satellite Squad Goals: The Cluster Mission to the Magnetic Field



View count:104,844
Last sync:2023-05-21 22:15
We knew some stars created large amounts of calcium, but no one really ever knew how...until now! Plus, astrophysicists believe they’ve finally seen evidence of the star that created one of the most important supernovas ever!

Hosted by: Caitlin Hofmeister

SciShow has a spinoff podcast! It's called SciShow Tangents. Check it out at
Support SciShow by becoming a patron on Patreon:
Huge thanks go to the following Patreon supporters for helping us keep SciShow free for everyone forever:

Bd_Tmprd, Jeffrey Mckishen, James Knight, Christoph Schwanke, Jacob, Matt Curls, Sam Buck, Christopher R Boucher, Eric Jensen, Lehel Kovacs, Adam Brainard, Greg, Sam Lutfi, Piya Shedden, Katie Marie Magnone, Scott Satovsky Jr, Charles Southerland, Charles george, Alex Hackman, Chris Peters, Kevin Bealer

Like SciShow? Want to help support us, and also get things to put on your walls, cover your torso and hold your liquids? Check out our awesome products over at DFTBA Records:
Looking for SciShow elsewhere on the internet?

Image Sources:
Thumbnail Credit: Credit: ALMA (ESO/NAOJ/NRAO)/Alexandra Angelich (NRAO/AUI/NSF)

You've probably heard Carl Sagan's famous saying that “we're made of starstuff.” And it's true! Aside from hydrogen—which was created right after the Big Bang— basically everything inside your body was once part of a star that burst in a supernova explosion and blasted its contents across the universe.

But supernovas don't just spew elements that have already formed within the star— the extreme forces within the blast can forge new elements in an instant, during the explosion itself. And this week, we got our best look yet at how that process can create huge amounts of calcium— the same stuff that's in our bones and teeth. In a paper published this week in The Astrophysical Journal, an international team described a recently discovered blast that turned out to be a rare calcium-rich supernova.

These supernovas are fascinating because they're extremely uncommon, yet astronomers estimate that they're responsible for around half the calcium in the universe. The thing is, no one knew how any of them produced such large amounts of calcium —until now. This blast was first discovered in April 2019 by an amateur astronomer in Seattle, looking through his new telescope.

He noticed a bright spot in M100, a beautiful spiral galaxy about 50 million light-years away. After reporting his potential supernova discovery to the pros, it took just hours for telescopes around the world and in space to focus on this spot and begin making their own observations. It was a supernova, and since they'd acted so quickly, astronomers were able to start observing it just 10 hours after it exploded.

And that early start paid off. In the first few days,. NASA's Swift space telescope caught something unexpected: bright X-ray emissions, which disappeared just five days after the explosion.

The existence of such bright X-ray emission for that short period of time led the research team to suspect that the death of this particular star happened in two phases. At first, the star's outer layers probably just drifted away into space, which happens sometimes as a massive star becomes unstable. Then, when the core exploded, the blast of energy superheated that loose material, emitting X-rays.

Along the way, it formed tons of calcium— in fact, more calcium than astronomers have ever observed in a single astronomical event. And that formation happened with astonishing speed. The extreme energy of the explosion drove chemical reactions that generated as much calcium as regular stars typically do over billions of years.

As for what actually exploded, though, that's still a mystery. Astronomers looked through old images from Hubble, which has studied this galaxy frequently over the last 25 years, hoping to identify the star that exploded. But they didn't find it.

That means the star must have been pretty small and dim—possibly a white dwarf, which is the leftover remains of a star that is no longer burning fuel. Whatever it was, the end result was a lot of brand-new calcium for the universe. That wasn't the only supernova news we've gotten recently.

In another pair of papers published last week in The Astrophysical Journal, astronomers described observations that may finally point towards the remains of the star that created the famous supernova 1987A. It's hard to overstate how important this supernova has been for astronomy. It exploded just 168 thousand light-years away in the Large Magellanic Cloud.

Thousand is not a number we talk about in astronomy very often! And when it was discovered in 1987, it was not only the brightest supernova in hundreds of years, but also the first nearby one since the development of modern astronomy. That means that this explosion has been studied in excruciating detail since the day its light reached Earth.

Hubble alone has made hundreds of observations over the course of three decades. And yet, in all that time, no one was ever able to spot what had happened to the dead star's core… which is odd. See, supernova 1987A showed the clear signature of a core-collapse supernova, in which the star's core crunches down into either a neutron star or a black hole.

Astronomers suspected it had formed a neutron star, since they'd detected lots of neutrinos, which are associated with these stars, but they couldn't see anything through the debris surrounding the explosion. They even thought maybe the core had collapsed all the way into a black hole after all. But recently, thanks to data from the giant ALMA radio telescope in.

Chile's Atacama Desert, astronomers uncovered the first clear evidence that it's there. In 2015, ALMA detected a blob of super hot material surrounding the location where the neutron star ought to be. The blob was so bright that at first the research team thought it couldn't possibly be heated by a neutron star.

But theoretical work laid out in the second paper shows that that isn't true. We just haven't ever seen a neutron star this young before. At just 33 years old, it's ten times younger than the next-youngest one studied closely by astronomers, making it hotter and brighter than anything we've seen before.

And that's why it's able to heat up the surrounding debris as much as it does. Astronomers will probably have to wait for the supernova's dust to settle a bit more before they can see the neutron star itself and put this decades-long mystery to bed. That might still take a few more decades, but, in the meantime, we'll keep watching the life story of this supernova play out in unprecedented detail, one observation at a time.

Thanks for watching this episode of SciShow Space News! And a special thank you to our. President of Space, Faisal Saud.

Thank you! And thanks to all patrons,. We wouldn't be here without you!

If you're not yet a patron and you'd like to join our wonderful community of supporters, you can find out more at {♫Outro♫}.