Cosmology Flashcards
Nebulae
Clouds of dust, hydrogen, ice and helium.
Birthplace of new stars
Found in empty space between stars
Stars
Celestial bodies that create their own light and heat from nuclear fusion within their core. They are collected together in galaxies.
Solar system
refers to a star and all the objects that travel in orbit around it
All objects…
exert a force of gravity on all other objects in the universe
Galaxy
giant collection of gas, dust and stars held together by gravitational attraction
grouped in clusters
planets
as a natural object in space that is massive enough for gravity to make it approximately spherical
orbit stars
they do not create their own light
Black hole
region in space where gravity pulls so much that even light cant get out. The gravity is so strong because the matter in a black hole is extremely dense.
Created either when a massive star collapses or at the beginning of the Universe
1 astronomical unit (au)
approx 150 million km
1 light year (ly)
9.5 x 10(12) km
nuclear fusion
the source of energy in the stars
fuel of hydrogen cannot last forever
Structure and size of star depends on balance between
inward force of gravity pulling towards the stars centre
outward force of radiation pressure, the force caused by the heat from nuclear fusion
life cycle of a star (Sun)
nebula, protostar, main sequence star like our Sun, planetary nebula, white dwarf, black dwarf
life cycle of a star (bigger than Sun)
nebula, protostar, supergiant star, red giant, supernova, neutron star or black hole
star size
determined by the balance between the inward force of gravity which pulls matter towards he centre of the star, and the outward force of radiation pressure that results from the pressure caused by the heat radiated from nuclear fusion within the star
Neutron star
a dense celestial object that consists primarily of closely packed neutrons
resulted from the collapse of a supergiant stellar body
red giant
dying star in the final stages of stellar evolution
hydrogen in the core runs out, star burns helium to produce carbon, atmosphere of star expands up to 100 times its original diameter
white dwarf
stellar core remnant composed mostly out of electron degenerate matter
dense
no more nuclear fusion occurs and remaining core collapses due to gravity
black dwarf
stellar remnant, white dwarf that has cooled sufficiently to no longer emit significant heat or light
planetary nebula
regio fo cosmic gas and dust formed from the cast off outer layers of a dying star
protostar
a cloud of interstellar gas and dust that gradually collapses, forming a hot dense core, and evolves into a star once nuclear fusion can occur in the core
apparent magnitude
a measure of how bright a star appears to an observer on Earth
2 factors that determine a stars apparent magnitude
the amount of light it emits and the distance between the star and Earth
absolute magnitude
brightness of the star if it was 10 parsecs from Earth, where 1 parsec= 3.26 light years
2 factors that determine a star’s colour
surface temperature and which elements it contains
the age of the star and the ratio of hydrogen to helium changes the colour