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Stars

Vocab

TermDefinition
Life Cycle of a star Infant -> youth -> middle age -> old age -> death
Interstellar Medium A thinly spread area of gas and dust
Nebula -Interstellar medium begins to collect into big clouds - Birthplace of stars
Protostar -Inside the nebula are regions with greater and lesser gravity, causing the gas and dust to pull together. -Not very stable phase
Equilibrium -A battle between gravity and gas pressure -Reached when both are even
Star An extremely hot ball of gas with hydrogen fussing into helium at its core
Main Sequence -Stars live out most of their lives in this stage -Stars have achieved nuclear fusion and stay at equilibrium
Red Giant -Phase after Main Sequence - Outer gas layers of the star expand but the core shrinks -Red in color, very high luminosity
Planetary Nebula -Occurs at the end of a low mass red giant's life -the outer layers of the star are expelled and the shell appears as brightly colored gas clouds - Core is very hot an luminous
White Dwarf -Forms when a low mass star runs out of fuel -Incredibly dense and will change color as it cools.
Black Dwarf -End product of white dwarf -the last stage of stellar evolution for low mass stars.
Red Super Giant -Same thing as a giant star but much bigger -As the star gets older it begins to sun out of fuel and expand
Supernova -Last stage of a massive stars life -Occurs as the star runs out of nuclear fuel and some of its mass flows into its core -Core collapses since it is so heavy and results in a giant explosion
Neutron Star -Core left behind after a supernova -Very very dense
Black Hole Forms when a very massive star collapses at the end of their life cycle - A large area in space with a very strong gravitational pull.
Hertzsprung–Russell diagram Plots each star on a graph and measures it magnitude (brightness) against its temperature(color)
Luminosity -The amount of energy (light) a star emits -Brightness
Brightness -The amount of energy (light) a star emits -Luminosity
Absolute Magnitude -The measure of a stars brightness as if it were at a standard distance of 10 parsecs from the observer
Created by: aliak_smsknights
 

 



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