OP- D Astrophysics Flashcards
apparent brightness
amount of energy received per second per unit area by an observer (Wm-2)
astronomical unit
the mean distance from the centre of the Earth to the centre of the Sun
(1.50 x 10^11)
binary stars
two stars orbiting their common centre of mass
three types of binary stars
- visual: can see two distinct stars
- eclipsing: periodic variation of brightness
- spectroscopic: change in wavelength of light receive from star (Doppler effect)
cepheid variable
a star that undergoes a periodic expansion of its outer layers that gives a periodic variation in its luminosity
Chandrasekhar limit
Maximum star remnant mass (1.4Ms) where electron degeneracy pressure prevent further gravitational collapse
constellation
a group of star that appears to make a pattern in the sky but they may not necessarily be close to each other in space.
cosmic microwave background (CMB) radiation
radiation emitted by the universe constituent with s temperature of 2.7K
cosmic scale factor (R)
gives a measure of the expansion that has taken place in the universe
dark energy
invisible energy source that my be accelerating the expansion of the universe
electron degeneracy pressure
where electron repulsion prevents further gravitational collapse of a star
galactic cluster
a group of galaxies bound together, orbiting around a common centre of gravity.
galaxy
a large scale collection of stars, gas, and dust held together by gravity.
globular stellar cluster
symmetrically arranged stellar cluster of 10^4 - 10^5 old stars
Hertzsprung-Russell diagram
graph plotting luminosity of stars against their temperature
Hubble’s Law
the speed at which galaxies are moving away from Earth (recession speed) is directly proportional to their distance from earth.