Star Life Cycles - Red Dwarfs

Stars and Nebulae

Index

Interstellar Clouds
Classes of Objects
Gas Giant Planets
Brown Dwarfs
Red Dwarfs
Sun-sized Stars
Large Stars
The Largest Stars
Impossible Stars
Star Clusters
Planetary Systems
Rocky Planets
An Endless Cycle


Questions
Credits
Links

Michael Gallagher
August 2002
July 2007

After Edward Martin et Al, American Scientist 1997

Red dwarfs have accumulated enough gas to sustain full nuclear fusion. The rate of fusion is slow - a Red Dwarf's hydrogen supply will last for trillions of years.

Red dwarfs are the most plentiful stars - they account for half the stellar mass of the galaxy. They are very dim - their detection requires a telescope. The closest star to the Sun, Proxima Centauri, is a Red Dwarf - although it is only 4.2 light years away, it is much too dim to be seen by the unaided eye.


Red Dwarf Details
Mass: 0.08 to 0.5 Suns (80 to 500 Jupiters)
Surface Temperature: 2,500° to 5,000° K
Lifetime: Trillions of years.
End point: Once fusion ceases, gradual loss of heat and slow fade to a dark body.