Transcript

Cloud of Stellar Dust and Gas

Protostar

Brown Dwarf

Sun-Like Star

Red Giant

Planetary Nebula

White Dwarf

Type 1aSupernova

BlackHole

NeutronStar

Type II Supernova

Blue Supergiant

Red Supergiant

Blue Giant

Red Dwarf

The dust and gas collapse and heat up

Much smaller than the Sun

Much larger than the Sun

Same size as the Sun

Somewhat smaller than

the Sun

Nuclear fusion consumes all the hydrogen

Material is ejected, creating a Filamentary shell surrounding a hot small star

A Star with the mass about 150 times

the mass of the Sun

Nuclear fuel is used up

Nuclear fuel is used up

Core Collapses

Core Collapses

Outer layers of the star are ejected

A Star with the mass about 100 times the mass of the Sun

The central star collapses

IF it is pushed over a limit of about 1.4 times the mass of

the Sun, it explodes

A Star more massive than ~10 Suns

STELLAR EVOLUTIONThe rate of evolution and the ultimate fate of a star depends on its mass.

National Aeronautics and Space Administration

www.nasa.gov

CHANDRA.SI.EDU/LEARN_SNR.HTML

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