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Stellar Science

Stellar science involves the formation, evolution, explosions, death and remnants of stars.

AB
sun, Sol, Heliosour local small-mass, yellow dwarf, G2 class, main sequence star
starmost common, known astronomical object that produces energy/light by nuclear fusion
hydrogen fusionnuclear fusion found in ordinary stars, where 4 hydrogens are fused into 1 helium + energy
hydrogen/heliumbasic composition of stars, where hydrogen is the "fuel" and helium is the "byproduct"
core burningnuclear fusion in the core of a star
nucleosynthesisthe process of element creation in a stellar core due to fusion
Hertzsprung-Russell (H-R) diagrama classification plot of stars by spectral class (temperature) vs luminosity (energy output)
spectral classgrouping of stars by their spectral characteristics reflecting temperature variation
nebular theorystar formation theory starting with an interstellar nebula
nebulainterstellar cloud of gas and dust
protostarastronomical object that is forming and may become a star, if enough mass is available
gravity collapsethe accumulation of interstellar gas and dust into a protostar
failed stara protostar with not enough mass to start fusing H, a brown dwarf
brown dwarfa failed star, with a mass less than 8% of a solar mass, or less than 85x of Jupiter's mass
main sequence stara star located on the central band on a H-R diagram, considered stellar "adulthood" stage of evolution
stellar adulthoodevolutionary stage of stars that starts at H fusion in a star's core
small-mass stara star with a mass between .08 and a few solar masses
dwarf stara star similar in size to the sun or smaller
red dwarfmain sequence star that is small, cool, and faint
yellow dwarfa main sequence star with a mass of 1 solar mass
medium-mass stara star with a mass between several and 8 solar masses
subgiant stara star larger than the sun and up to 10x larger in size
large-mass stara star with a mass from 8 solar masses and higher
giant stara star between 10x and 100x larger than the sun in size
supergiant stara star greater than 100x the size of the sun
blue giantmain sequence star that is large, hot and bright
blue supergiantmain sequence star that is the largest, hottest and brightest
stellar old ageevolutionary stage of stars that starts at H fusion as a shell surrounding an ash core
shell burningfusion in a star's interior surrounding a nonfusing core
ash corethe nonfusing core during shell burning
red giant regionthe upper right area of an H-R diagram, where old-age, large, cool but bright stars plot
red subgiantan old-age, red giant region star less than 10x the size of the sun
red giantan old-age, red giant region star between 10x and 100x the size of the sun
helium flashthe point in small-mass, old-age, red giant region star when helium-core fusion starts
yellow gianta small-mass, old age, red giant region star with stable helium-core and hydrogen-shell fusion
red supergiantan old-age, red giant region star more than 100x the size of the sun
multiple shell burningheavy element fusion steps in a large-mass, old-age, red giant region star
stellar deaththe evolutionary end by explosion of an old-age, red giant region star
stellar remnantthe astronomical object that remains after an old-age star explodes
planetary nebulathe ejected outer layers of a small-mass, old-age, red giant region star as it dies
white dwarf regionthe lower left area of an H-R diagram, where stellar remnant that are small, hot but dim stars, plot
white dwarfthe small, hot but dim stellar remnant that remains after a medium- or small-mass red giant region star dies
helium white dwarfthe stellar remnant of a small-mass red giant
carbon white dwarfthe stellar remnant of a medium-mass red giant
black dwarfa cooled, solitary white dwarf stellar remnant
novathe sudden increase in brightness of a white dwarf, due to surface fusion explosions
supernovaa very large and bright, destructive explosion of a star
supernova Type Ithe catastrophic explosion of a carbon white dwarf star that gains mass to reach 1.4 solar masses
carbon detonation supernovaa supernova Type I that lacks a hydrogen signature
iron core collapsethe dying event of a large-mass, old-age red giant region star when it attains iron-core fusion
supernova Type IIthe catastrophic explosion of a large-mass, old age, red giant region star at iron core collapse
core collapse detonationa supernova Type II that has a hydrogen signature
supervova remnantthe ejected outer layers of a large-mass, old-age, red giant region star as it explodes
neutron starstellar remnant between 1.4 and 3 solar masses that forms during a supernova Type II
pulsara star with a "pulsating" appearance interpreted to be a rapidly rotation neutron star
black holean area in space in which gravity is so strong that no light or radiation is received
stellar black holea black hole that forms when a supernova Type II leaves a 3 solar mass or larger stellar remnant


Russell J. Wernlund

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