Paper 1 - Astrophysics Flashcards
what is the universe
a large collection of billions of galaxies
what is a galaxy
a large collection of billions of stars
orbit of comet
around the sun
very elliptical
orbit of moons and planets
slightly elliptical but pretty much circular
orbital radius, orbital speed and time period equation
orbital speed = 2 x pi x orbital radius / time period
relationship between orbital radius and speed
big radius = big speed
colour gradient for temperature of stars
hottest -> coolest order: blue white yellow orange red
why are hotter stars blue but cooler stars red
hotter = emits higher frequency of light - short wavelength
colder = emits lower frequency of light - longer wavelength
life cycle of a star smaller than the sun
nebula protostar main sequence star red giant white dwarf
life cycle of star bigger than sun
nebula protostar main sequence star red supergiant supernova neutron star/black hole
describe the formation of a star
a cloud of dust and gas called a nebula forms
gravity pulls stuff together to form protostar
temperature rises as star gets denser and more particles collide
when temperature gets high enough, hydrogen nuclei undergo nuclear fusion to form helium nuclei, giving out huge amounts of energy
reaches stable period where thermal expansion balances force of gravity pulling it in
eventually hydrogen in core begins to run out, so thermal expansion becomes less than gravity force so the star compresses
keeps getting compressed until dense and hot enough so outer layers expand to form red giant or supergiant
red because surface cools