Eta Carinae is a star system 8,000 light years from the solar system. It contains a luminous blue hypergiant star which probably has about 100 times the mass of the sun and shines 4 million times more brightly. For those of you keeping tally, that gives the star approximately the same mass as 33 million earths!
Eta Carinae was originally cataloged by Edmond Halley in 1677 (hence its stylish Latin name) as a comparatively dim 4th magnitude star, however astronomers noticed that its brightness varied greatly over the decades. In 1827 it began to become significantly more luminous and by 1843 it was the second brightest star in the night sky (after Sirius, our next door stellar neighbor which is only 8.6 light years away). The star then dimmed down to the eighth magnitude—becoming invisible to the naked eye. Today it is believed that this strange occurrence was a supernova impostor event in which the star nearly exploded. Looking at Eta Carinae now through the Hubble telescope reveals two huge hemispheres of material ejected from the star. Scientists have named this cloud the Homunculus nebula and it is nearly a light year in diameter.
Eta Carinae and the Homunculus Nebula as photographed by the Hubble Space Telescope
Stars as massive as Eta Carinae are very rare. At this stage of galactic development there are perhaps a dozen in a galaxy the size of the Milky Way (which contains 200 billion to 400 billion stars). Eta Carinae is probably fated to die in a hypernova explosion (an immense supernova event). A similar impostor event to Eta Carinae’s 1843 flare-up was witnessed on SN 2006jc, a star within galaxy UGC 4904 (perhaps you now appreciate the Latin and Arabic names of familiar nearby astronomical objects). SN 2006jc went hypernova two years after its impostor nova event. It is very possible that Eta Carinae no longer exists but was destroyed a long time ago. The light we see now is eight thousand years old. Who knows what happened since then?
When Eta Carinae goes hypernova it will destroy star systems nearby. Additionally, a massive gamma ray burst will shoot from both of its poles as its center collapses into a black hole. Any living, earth-like world caught in such a beam would be sterilized completely–although we are mercifully not currently in Eta Carinae’s polar vector…
Eta Carinae’s Fate? A Hypothetical Illustration of a Hypernova Event with Gamma Ray Burst (Credit: Nicolle Rager Fuller/NSF)
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May 4, 2010 at 3:32 PM
Rachel
Neat. I’m curious, how do you pick your topics for your blog?
Super massive stars (those over 20 solar masses) are pretty unstable. There’s academic debate about how they can even form. I listened to a lecture on that at a conference, but now I can’t remember the details.
May 4, 2010 at 5:41 PM
Hieronymo
I blog about what I’m thinking about on any given day–however there are a few underlying themes which crop up (and which I’m trying to concentrate on). Space is the most difficult of my favorite themes to write about since I’m not an astronomer.
When I was surfing super massive stars on the internet, I encountered some of the scientific controversy surrounding them, however the debate superseded my understanding of stellar physics!