Not exact matches
Such «dark matter
stars» could have been huge and, when their power source was
exhausted, might have collapsed to form
giant black holes.
Ness and her colleagues developed a computer program that analyzed the light emitted by red
giants — bright
stars that started out like the sun but
exhausted their hydrogen fuel — to determine the
stars» masses and ages.
Red
giants are dying
stars in the late stages of life that are
exhausting the nuclear fuel that makes them shine.
He has begun finding and studying worlds around red
giants, elderly
stars that have nearly
exhausted their nuclear fuel.
When
stars exhaust their hydrogen fuel the outer layers of the
star can expand greatly and the
star becomes a
giant.
As Vega is so much bigger and hotter than Sol, however, the
star will
exhaust its core hydrogen after only another 650 million years or so (for a total life of around a billion years) and turn into a red
giant or Cepheid variable before puffing away its outer layers to reveal a remnant core as a white dwarf.
When the core fuel is
exhausted, the internal structure of the
star changes rapidly; it quickly leaves the main sequence and moves toward the region of
giants and supergiants.
For a
star with at least 0.5 solar masses, once the hydrogen supply in its core is
exhausted and it expands to become a red
giant, it can start to fuse helium atoms to form carbon.
It may be only about 225 to 250 million years old (Liebert et al, 2005; and Ken Croswell, 2005), but being so much bigger and hotter than Sol, the
star will
exhaust its core hydrogen within only a billion years and turn into a red
giant or Cepheid variable before puffing away its outer layers to reveal a remnant core as a white dwarf.
Information about the ang... ▽ More When the core hydrogen is
exhausted during stellar evolution, the central region of a
star contracts and the outer envelope expands and cools, giving rise to a red
giant, in which convection occupies a large fraction of the
star.
Abstract: When the core hydrogen is
exhausted during stellar evolution, the central region of a
star contracts and the outer envelope expands and cools, giving rise to a red
giant, in which convection occupies a large fraction of the
star.
Red
giants are dying
stars in the late stages of life that are
exhausting their nuclear fuel that makes them shine.