Astronomy and cosmology Flashcards
Luminosity
Total power of radiation emitted by a star
Standard candle
Astronomical object which has a known luminosity due to a characteristic quality possessed by that class of object
example of a standard candle
Capheid variable stars def
pulsating star which increases and decreases brightness over time
Example of a standard candle
Type 1a supernova
a supernova explosion involving a white dwarf
Inverse square law
Radiant flux density, F, is indirectly proportional to the square of distance
F=L/4πd²
How are standard candles used to determine distance
Standard candles luminosity can be compared to other objects to understand their distance from the Earth.
inverse square law can be used for calculation
Wien’s displacement law
wavelength of maximum intensity is inversely proportional to (thermodynamic) temperature
colour-frequency- wavelength is influenced by temperature
Stefan Boltzman law
Total energy emitted by a black body per unit area per second is proportional to the fourth power of the absolute temperature of the body
E/At = σ x T4
What can be used to find increase/ decrease in wavelength
Difference in lines of emission spectra
Red shift
when emission spectro lines move to the right
Explain why the red shift explains that the universe is expanding (3)
- receding stars or galaxies
- space between the earth and galaxies expand
- universe is expanding
Hubble’s law
the recession speed of the galaxies moving away from the Earth is directly proportional to their distance from the Earth
Big bang explained
- if the universe is expanding, at some point in time, it started as an extremely hot, dense, singular point which subsequently began expanding very quickly
SI unit of luminosity
Watts
Radiant flux intensity def
the observed amount of intensity of the radiant power per unit area of radiation measured on earth