Space Flashcards
Evidence for big bang
Red shift - galaxies are moving away from us. This can either mean that we are at the centre of the universe, which disproves the cosmological principle SO it must mean that the universe is expanding at every point. More distant galaxies are more red shifted so are receding at a faster rate.
Cosmic background radiation- when the universe was first made it was very small, hot and dense. There was lots of gamma radiation and as it expanded the gamma radiation stretched out into microwaves. As it expanded the universe also cooled down drastically.
Keplers 1st Law
- The orbit of a planet is an ellipse with the sun at one focus
Keplers 2nd Law
- A line segment joining a planet and the sun sweeps out equal areas during intervals of equal time.
Keplers 3rd Law
Period^2 is directly proportional Radius^3
Cosmological Priniciple
The universe is isotropic and homogenous and the laws of physics apply everywhere in it.
Equation relating distance & parallax angle
d = 1/p
distance is in parsecs. only works for stars at max 100pc away.
Recessional velocity equation
recessional velocity = hubbles constant x distance
Hubbles constant
67.8 kms-1Mpc-1 but to find age of the universe have to use 2.2x10^-18 s-1
1/Hubbles constant = age of universe.
Emission line spectra
Every element has a unique one because of the unique set of energy levels associated with its electrons. It looks like coloured lines on a black background.
Continuous line spectra
All visible wavelengths of light are present, this is produced by a solid heated metal.
Absorption line spectra
Looks like black lines against a colourful (continuous spectra) background. Each black line corresponds to a wavelength of light used to excite atoms of that element. These wavelengths are the same for when those atoms are de-excited.
Isotropic
looks the same in every direction
Assumptions of kinetic theory of gases
- Forces are negligible except during collisions
- Collisions are perfectly elastic
- Particles occupy negligible volume compared to volume of gas
- Lots of particles move in random motion
Two conditions of SMH
acceleration is proportional to displacement
and acts in the opposite direction.
How to find Vmax in SMH
v max= w * A
which then can be used to find max KE (also equal to total energy