Category Archives: star death

A Haunting Gallery of Destruction

The Deaths of Stars

This HST mosaic image of the Crab Nebula shows a six-light-year-wide expanding remnant of a supernova explosion. Courtesy STScI.

Stardeath produces some of the most intricate-looking objects in astronomy. If you have ever gone to the Hubble Space Telescope’s Web site and searched for planetary nebulae, you know what I mean. Giant stars produce giant explosions, like the long-known Crab Nebula.

The Eskimo Nebula (NGC 2392). The intricate "face" is a bubble of material being blown into space by the central star's intense "wind". Courtesy STScI.

This Hubble Space Telescope image shows us what the supernova remnant is made of (hydrogen gas, particles of heavier elements), and also shows us the structure of the nebula and how it’s influenced by the neutron star at the center. That neutron star is what’s left of the original star — a dense object spinning more than 30 times per second.

Stars like the Sun go a bit less violently, huffing off their atmospheres for millions of years before collapsing to make white dwarfs. The radiation from the central star continues to light up the remains of the former star, creating complicated visions of stellar death. The Eskimo Nebula (right), is a fine example of such a sun-like star’s death. The remains are called a planetary nebula, one of those odd misnomers in astronomy that has nothing to do with a planet, but is a nebula. This sunlike star began to die some 10,000 years ago, blowing bubbles of gas out away from itself and flinging its outer atmosphere to space. Our own Sun might look like this some billions of years from now.

Well, I’ve been long fascinated with the images of star death, ever since I wrote my first book (with Jack Brandt), about Hubble Space Telescope science (called Hubble Vision).  A few years ago when I did an update of one of my more-popular planetarium shows, called Hubble Vision 2, I had a great selection of star death images to choose from to tell the story of stellar demise. I wrote about sun-like stars, “Hubble’s images of these stars in their death throes comprise a haunting gallery of destruction.”

As is always the case with my shows, I knew that the soundtrack artist (who also happens to be my husband and co-producer) would find a way to make the scene  memorable with his trademark space music and video choreography. The scene in the show is a solemn, beautiful procession of planetary nebula images that bring home to audiences the majesty of a star’s passing.

Fast-forward a few years to this month, and Mark has now released the music from that show soundtrack in an album called Geodesium Stella Novus (where you can preview and buy the album if you’re interested). And, he created a music video based on that planetary nebula scene that really does bring home the majesty of that haunting gallery of destruction we first introduced in the show. We created a fulldome version of the music video, which you might get to see someday at your local digital planetarium.

But, we’ve also got a “flat-screen” version available on our Youtube channel for people to watch and I’ve embedded it below.  The piece of music is called “Light Echoes”, and it accompanies these gorgeous views of star death, ranging from supernova remnants to planetary nebula, as cosmic art.  It’s not a new concept — the universe as art. But, you have to admit, when you see the way nature has arranged the aftermath of stardeath, it can look evocative, haunting… and artistic!

Exploring Cosmic Clouds of Light

Carina’s Starry Nebulous Beauty

The hot Wolf-Rayet star WR 22, part of the Carina Nebula's population of hot, massive stars. MPG/ESO La Silla.

Astronomers have their favorite places to study in the cosmos — places they return to again and again.  They do this not just because the places look pretty or are easy to spot.  Some places in the cosmos just command our attention because they have SO much going on and can teach us a great deal about processes like starbirth and star death.

Such is the case with the Carina Nebula. It lies a few thousand light-years from Earth and contains regions of starbirth, one very eye-catching example of incipient star death, and a lot of gorgeous clouds of gas and dust that are stellar nurseries.  Astronomers used the European Southern Observatory’s Wide-Field Imager to zero in on a very bright, very unusual star called WR 22.  It’s a Wolf-Rayet star, a rare and very massive (some 70 times the mass of the Sun) object that is shedding its atmosphere into surrounding space — contributing to the rich collection of recyclable star materials in the Carina Nebula. WR 22 is actually one member of a double star stystem.

WR 22 fronts a backdrop of glowing hydrogen and other gases. Heat and intense ultraviolet radiation from stars such as this one causes those clouds to light up. If the radiation is intense enough, it can eat away at the clouds.   This leaves less material to create new stars, resulting in a sort of cosmic cannibalism by the massive stars already in existence.  In the not-too-distant future, WR 22 will probably evolve to become what’s called a luminous blue variable star, and then spend much of its remaining time going through different phases of hydrogen and helium burning before dying as a Type Ic supernova.  Their future is a pretty standard one for stars of their mass and type.  But, since there are only a few hundred known Wolf-Rayet stars such as WR 22, they are objects that astronomers watch as much as possible, returning to them often to chart their progress down their evolutionary sequences.  For the rest of us, we get to peer over the shoulders of astronomers who study these babies — and we get to marvel at the gorgeous scenes in which these stars appear.