Cosmology Flashcards
what is the cosmological principle
the universe is homogenous and isotropic
define homogoneous
uniform distribution of matter
define isotropic
physical property which is measured to be the same in all directions
what is 1AU (definition and value)
astronomical unit - average distance from the earth to the sun
1.5 x 10^11 m
define a light year
distance travelled by light in a vacuum in a year
define the parsec
the distance at which a radius of 1AU subtends an angle of one arcsecond
what is 1 degree in arcseconds
1 degree = 60 arcminutes = 3600 arcseconds
what is stellar parallax
a technique used to measure the distance of stars relatively close to us
what is parallax
the apparent shift in the position of a relatively close star against a backdrop of more distant stars
define the doppler effect
the apparent change in wavelength due to relative motion to an observer
what is red shifting
when a star/galaxy is moving away from an observer, the spectra lines will red shift (increased wavelength)
what is hubble’s law
recessional velocity of a galaxy is proportional to its distance from us
where can hubble’s law be applied
stars/galaxies outside of our own galaxy
why can hubble’s law not be used on very large or very short scales
short scale - gravitational attraction effects velocity
large scale - non-linear expansion rate may not be constant
what is evidence of the big bang
- in every direction, the universe is red-shifting
- in every direction, the temperature is about 2.7K
- EM radiation started as gamma, but as universe expanded and cooled, wavelength stretched to microwave radiation ( λmaxT = constant)