Module 8: Modelling the universe Flashcards
Olber’s paradox
For an infinite, uniform and static universe, the night sky should be bright because of light received in all directions from stars.
Hubble’s law
Speed of recession of galaxy is proportional to distance of galaxy.
The cosmological principle
The universe is:
Isotropic: on a large scale the universe looks the same in all directions.
Homogeneous: on a large scale, the matter is spread out evenly in the universe.
Universal: all physical laws that apply on the Earth are equally valid in the rest of the universe.
Critical density
The density of the universe that will give rise to a flat universe.
Astronomical unit
The mean distance between the Earth and the Sun. 1.49x1011 m
Parsec
The distance that gives a parallax angle of 1 arc second. 3.1x1016 m
Light year
Distance travelled by light (in a vacuum) in a time of 1 year. 3.0x108 m