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Life Cycle of A Star

Vocabulary for Life Cycle of a Star

TermDefinition
Life Cycle of a Star Stars go through a natural cycle, much like any living beings. This cycle begins with birth, expands through a lifespan characterized by change and growth, and ultimately leads to death.
Interstellar Medium the material which fills the space between the stars.
Nebula a cloud of gas and dust in outer space, visible in the night sky either as an indistinct bright patch or as a dark silhouette against other luminous matter.
Protostar a contracting mass of gas which represents an early stage in the formation of a star, before nucleosynthesis has begun
Equilibrium a state in which opposing forces or influences are balanced.
Star a fixed luminous point in the night sky which is a large, remote incandescent body like the sun.
Main Sequence a series of star types to which most stars belong, represented on a Hertzsprung–Russell diagram as a continuous band extending from the upper left (hot, bright stars) to the lower right (cool, dim stars).
Red Giant a very large star of high luminosity and low surface temperature. Red giants are thought to be in a late stage of evolution when no hydrogen remains in the core to fuel nuclear fusion.
Planetary Nebula a ring-shaped nebula formed by an expanding shell of gas around an aging star.
White Dwarf a small very dense star that is typically the size of a planet. A white dwarf is formed when a low-mass star has exhausted all its central nuclear fuel and lost its outer layers as a planetary nebula.
Black Dwarf a very small cooled remnant of white dwarf that emits no detectable light.
Red Super Giants An extremely large red giant star with a minimum of 15 solar masses.
Supernova a star that suddenly increases greatly in brightness because of a catastrophic explosion that ejects most of its mass.
Neutron Star any of a class of extremely dense, compact stars thought to be composed primarily of neutrons. Neutron stars are typically about 20 km (12 miles) in diameter.
Black Hole a region of space having a gravitational field so intense that no matter or radiation can escape.
Created by: klstorie
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