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)
what happened up to 1 second after the big bang
-started off as a hot, dense singularity
- time and space created
- inflation occurs
- expansion leads to cooling
- energy pair production - matter and antimatter elementary particles
- more matter than antimatter
- quarks combine to form protons and neutrons
what happened up to 100 seconds after the big bang
protons and neutrons fuse to form hydrogen nuclei and primordial helium
what happened up to 380,000 years after the big bang
- atoms form as electrons cool down and combine with nuclei
- universe becomes transparent - photons free to travel as gamma radiation
- expansion of universe - gamma radiation now microwave radiation
what happened up to 30 million years after the big bang
- first stars appear
- first heavier elements appear
what happens up to 200 million years after the big bang
our galaxy forms as gravitational forces pull clouds of hydrogen and existing stars together
what is dark matter and how was it discovered
- discovered that stars at the edge of galaxies are moving faster than they should given the distribution of stars
- this violates newton’s law
- we call this missing mass ‘dark matter’
- estimated 25% of the universe
what is dark energy and how was its presence theorised
- everything has gravity, therefore expansion of the universe should slow over time, or at least remain constant
- however, the universe is expanding at an ever increasing rate
scientists use dark energy to explain this, energy we do not know of which accelerates stars and galaxies - estimated 75% of the universe