Category Archives: star death

Warming Your Hands at The Fire of a Dying Star

Since it’s snowing like mad and the wind is blowing like a banshee here (and the temperature is a toasty 21 degrees Fahrenheit) right now, I want to talk about hot stars. Specifically, let’s talk about hot, dying stars that were once like the Sun. Here’s NGC 2440 to help me take my mind off the cold weather! (For you folks in sunnier climes, count your blessings!)

HST Looks at NGC 2440 again
HST Looks at NGC 2440 again

So, NGC 2440 first came to my attention back when I was working on my first book with Jack Brandt, called Hubble Vision. We wanted to show a nice array of stars at different stages in their lives. Star lives, by the way, are way longer than ours, but like us, they proceed in stages. There’s the infancy part—that takes place in a cocoon of gas and dust. Then, there’s the “living” part, where the star consumes nuclear fuel in its core for some amount of time. Then, there’s the old age part, where the star starts to lose mass in huge quantities and finally gives up the ghost. If the star is massive (like more than 8 or 10 times the mass of the Sun), then it sheds lots of its atmosphere before blowing itself to smithereens in a supernova explosion.

If the star is like the Sun, then it litters its environment with material that it blows away from itself. It does it maybe once, or maybe several times, creating shells of gas (nitrogen, hydrogen, oxygen, and helium, for example). That “exhaled” matter forms a shell around the star. Then, the interior star contracts (shrinks), and in the process, heats up.

So, NGC 2440 (what’s left of it) is very hot—like 400,000 degrees Fahrenheit (try more than 400,000 times hotter than your oven gets). All that heat has to go somewhere and do something, so it’s lighting up the huge cloud of mass that the star lost earlier in its life.

There was more than one outburst from NGC 2440 during its old age, which is why we see two “lobes” of material surrounding the central star.

If you want to see a huge version of the image above, go here (the HST news center). The highest-resolution image almost looks three-dimensional.

Now, I feel a bit warmer. How about you?

Keeping It Working

So, they’re going to fix Hubble and bring it up to modern spec in 2008. That’s great and about time somebody used some common sense about our nation’s (the world’s, actually) valuable astronomy asset. Sure the mission can be dangerous, but the dangers are known. And the return is great. As is the respect for what HST can do.

HSTs view of 838 Monocerotis. Read more here.
HST's view of 838 Monocerotis. Read more here.

HST does drop-dead gorgeous images, like the recent view of V838 Monocerotis, above. It delivers multi-wavelength views (very near infrared and ultraviolet) of objects to let us know how they look in different parts of the electromagnetic spectrum. And, since its launch and first servicing mission, HST has taken us farther out to the most distant reaches of the cosmos. What’s not to like about that?

So, I’m glad they’re going to restore HST and bring it up to date. It’s a respectable and famous observatory, and worth far more to humanity than a lot of other things our tax dollars fund.