Stellar evolution. Credit: European Space Agency

1 posted on
03/15/2018 2:01:52 AM PDT by
SunkenCiv
To: SunkenCiv
- 0.08 - 0.4 solar mass
Red dwarf stars leaving a hypothetical helium white dwarf remnant after a few trillion years
- 0.4 - 8 solar mass
Medium-sized stars leaving a carbon/oxygen white dwarf after a few billion years
- 8 - 10.5 solar mass
Large stars leaving a oxygen/neon/magnesium white dwarf after a few 100 million years
- over 10.5 solar mass
Giant stars leaving a neutron star/black hole after a few million years
Most star systems are multiple ones, unlike our own. Combinations are interesting.
To: SunkenCiv
Stars the mass of our Sun, and up to eight times more massive, evolve into red giants towards the end of their lives. Their outer layers puff up and expand millions of kilometres, their dusty, gassy shells blown away from the central star in relatively slow winds up to few hundreds of km/s. That's all well and good but everybody knows anything that happens to our sun is the result of human activity on earth - it's settled science...
5 posted on
03/15/2018 5:08:08 AM PDT by
WayneS
(An appeaser is one who feeds a crocodile, hoping it will eat him last. - Winston Churchill.)
FreeRepublic.com is powered by software copyright 2000-2008 John Robinson