Stellar Evolution + Galaxies

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Created by:

Whitmoyer  on June 3, 2012

Subjects:

(H) Earth and Space Science

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Stellar Evolution + Galaxies

stellar evolution
stars change size and temperature due to the creation of new elements in the core by nuclear fusion
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stellar evolution stars change size and temperature due to the creation of new elements in the core by nuclear fusion
mass controls the life-cycle of all stars
sun g2
blue giants high mass, short contraction 10-20 solar masses
a,f,g and k medium mass, medium contraction 1-3 solar masses
red dwarf low mass, long contraction less than 1 solar mass
nebula cloud of gas and dust that contracts under gravity
4H-1He conversion in the main sequence
He-C conversion that makes a red giant
He-C, C-O, O-Si, Si-Fe conversion that makes a supergiant
pulsar 1.4-3 solar masses, "lighthouse in space", spins very fast
neutron star 1.4-3 solar masses, spins very fast, beam out of view
black hole greater than 3 solar masses
singularity black hole itself
event horizon point of no return
iron has the densest nucleus of all elements and is the densest element a star can produce in its core
supernova when a star tries to make an element heavier than iron in its core and the gravity and fusion pressure combine and tear apart the star
optical double two stars that appear to be double by chance line of sight, not related by gravity
visual binary two or more stars that can be "split" when viewed through a telescope, mass can be determined
eclipsing binary two stars that eclipse each other due to their orbit being in earth's line of sight, star changes in brightness due to eclipse
spectroscopic binary two or more stars that cannot be visually split but can be identified by the alternating red and blue shifting of their spectra
variable stars unstable stars that vary in brightness due to changes in size, period is related to true brightness therefore they can be used to determine distance
rr lyrae short period variable less than one day
cepheid medium period variable a few days to a couple months
if the period is bigger it gets brighter
mira variable long period variable months to years, red giants
nova white dwarf in a binary pair temporarily flares up when hydrogen stolen from the partner star builds on the white dwarf and finally fuses
galaxy large system of stars controlled by common gravity, also means "island universe"
elliptical galaxy egg-shaped galaxy
spiral galaxy bulge or nucleus, disc or spiral arms, comes in a barred type (galaxy)
irregular galaxy no basic shape (galaxy)
open cluster loosely formed group of stars of similar origin
globular cluster nearly spherical group of densely packed stars

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