KABOOM! Nearby Galaxy M82 Hosts a New Supernova!

The entire universe in blog form
Jan. 22 2014 12:11 PM

KABOOM! Nearby Galaxy M82 Hosts a New Supernova!

supernova in M82
The discovery image of the new supernova shows it's already quite bright.

Photo by UCL/University of London Observatory/Steve Fossey/Ben Cooke/Guy Pollack/Matthew Wilde/Thomas Wright

I woke up to some great science news: A supernova has gone off in the nearby galaxy M82!

This is terribly exciting for astronomers. M82 is pretty close as galaxies go, less than 12 million light years away. That means we have an excellent view of one of the biggest explosions in the Universe, and we’ll be able to study it in great detail!

Advertisement

The supernova has the preliminary designation of PSN J09554214+6940260. I know, that’s awful—it’s based on the star’s coordinates—but it’ll get a name soon enough that’ll be easier on the eyes and brain.

Phil Plait Phil Plait

Phil Plait writes Slate’s Bad Astronomy blog and is an astronomer, public speaker, science evangelizer, and author of Death from the Skies!  

And just to get this out of the way, we’re in no danger from this explosion. It’s far too far away. Also, you won’t be able to just go outside, look up, and see it. Right now it’s too faint to see without a telescope. But the good news is it appears to have been discovered about two weeks before it hits peak brightness. Supernovae get brighter over time before fading away, and this one may get as bright as 8th magnitude, which is within range of binoculars. Right now it’s at about 12th magnitude; the faintest star you can see with your naked eye is about mag 6 (note that the numbers run backwards; a bigger number is a fainter object).

M82 is in Ursa Major, well placed for viewing right now in the Northern Hemisphere. Universe Today has a map to show you how to find it.

m82sn_remanzacco
Another image of the supernova taken on Jan. 22, 2014

Photo by Ernesto Guido, Nick Howes & Martino Nicolini

Here’s a funny thing, too. The supernova itself is what we call a Type Ia, a dwarf explosion. Astronomers are still trying to figure out exactly what happens in a Type Ia explosion, but there are three competing scenarios. Each involves a white dwarf, the small, dense, hot core left over after a star turns into a red giant, blows off its outer layers, and essentially “dies.” One scenario is that the white dwarf is orbiting a second star. It siphons off material from the star and accumulates it on its surface. Eventually this material gets so compressed by the huge gravity of the white dwarf that it fuses, creating a catastrophic explosion that tears the star apart.

Another is that two white dwarfs orbit each other. Eventually they spiral in, merge, and explode. The third, which is a recent idea, is that there are actually three stars in the system, a normal star and two white dwarfs. Due to the complex dance of gravity, the third star warps the orbits of the two dwarfs, and at some point they collide head-on! This too would result in a supernova explosion. All three scenarios involve very old stars, since it can take billions of years for a normal star to turn into a white dwarf.

M82
A deep image of M82 shows gas and dust blasting out due to the fierce energy released when huge numbers of stars are born.

Photo by Adam Block/Mount Lemmon SkyCenter/University of Arizona

What’s funny about this is that the galaxy M82 is undergoing a huge burst of star formation right now, and that means lots of massive stars are born. These live short lives and also explode as supernovae (called Type II, or core collapse) though the mechanism is very different from that of the white dwarf explosions. You’d expect M82 to have more core collapse supernovae, but this new one is a Type Ia.

And that’s actually more good news. These supernovae tend to all explode with the same energy, so they behave the same way whether they are near or far. We can see them for billions of light years away, which means they can be used to measure the distances of galaxies that are very far away. It was this kind of exploding star that allowed astronomers to discover dark energy, in fact. This energy is accelerating the expansion of the Universe, making it grow more every day. We don’t know a whole lot about it—it was only announced in 1998—but we’re learning more all the time. A nearby Type Ia means we can learn even more about these explosions, and hopefully calibrate our understanding even better.

m82sn_starparty
During a weekly online virtual star party, an amateur astronomer actually caught the supernova on Jan. 19, 2014, before it was officially discovered! Click to watch the video.

Photo by John Kramer c/o Fraser Cain

And that means we need observations! If you are an amateur astronomer, get images! And if you observed M82 recently, you may have “pre-discovery” images of it, taken before it was officially discovered. Those are critical for understanding the behavior of the supernova. If you do, report it to the CBAT (but make sure you read the instructions first; they don’t want images, just reports of magnitudes and so on).

Given the fact that it’s nearby, up high for so many observers, and caught so early, this may become one of the best-observed supernovae in modern times. I’m very excited this happened, and I hope to share more images and information with you soon!

Lots of sites have more info. Here are a few: