our stellar cousins
Nov. 22nd, 2007 10:21 amI started off the day reading this interesting article about the discovery of "carbon stars"--ancient white dwarfs with atmospheres almost entirely composed of carbon. They're rare, and they challenge our understanding of stellar evolution, and they're bound to end up in a space opera novel before long.
"The great mystery is why these carbon-atmosphere stars are found only between about 18,000 degrees and 23,000 degrees Kelvin. 'These stars are too hot to be explained by the standard convective dredge-up scenario, so there must be another explanation,' Dufour said."
The explanation, of course, is that they're alive.
"The great mystery is why these carbon-atmosphere stars are found only between about 18,000 degrees and 23,000 degrees Kelvin. 'These stars are too hot to be explained by the standard convective dredge-up scenario, so there must be another explanation,' Dufour said."
The explanation, of course, is that they're alive.
no subject
Date: 2007-11-22 12:23 am (UTC)But why? What would need to operate at those temperatures? I guess it's time to start looking at what's orbiting them...
After all, they're too small and too hot to be Dyson spheres, even loose ones like Matrioshkas...
no subject
Date: 2007-11-22 12:27 am (UTC)Maybe the stars are stellar graveyards, where they've dumped all their organic crap.
What could a carbon star provide an advanced civilisation that an ordinary white dwarf couldn't?
Maybe they're furnaces for buckyballs and nanotubes by the gazillions.