(Submitted October 16, 1997)
Can you please tell me in plain language what a Red Giant is?
I'll give you a short answer and a longer one. The short answer is that
towards the end of a star's life, the temperature near the core rises and
this causes the size of the star to expand. This is the fate of the Sun in
about 5 billion years. You might want to mark your calendar!
The long answer is that stars convert hydrogen to helium to produce light
(and other radiation). As time progresses, the heavier helium sinks to the
center of the star, with a shell of hydrogen around this helium center
core. The hydrogen is depleted so it no longer generates enough energy
and pressure to support the outer layers of the star. As the star
collapses, the pressure and temperature rise until it is high enough for
helium to fuse into carbon, i.e. helium burning begins. To radiate the
energy produced by the helium burning, the star expands into a Red Giant.
For Ask an Astrophysicist