2. Stars Flashcards
Units of Temperature
Kelvin
Celsius to Kelvin
+ 273
Black body
A perfect radiator and absorber, it emits and absorbs at the same rate
Stefan Boltzmann Law
Luminosity = Surface Area x SB constant x (Temperature)⁴
Stefan Boltzmann Constant
5.67 x 10(-8)
Wiens law
Peak wavelength = Weins constant / Temperature
Wiens constant
2.90 x10(-3)
Metre - kelvins
Wave characteristic graph
Y axis = Intensity
X axis = Wavelength
Visible light wavelength
400nm - 700nm
Inverse Square law
Intensity = Luminosity / 4(pi) x (Distance from earth to star)²
Multiwavelength astronomy
Helps to process images of different light
Taken using different parts of the EM spectrum
Eg. James Webb Telescope uses Infrared
Continuous spectrum
The stars emit all different gases from the surface at all frequencies - a no gaps spectrum
Absorption spectrum
When the light emitted from a star passes through the gases in its atmosphere some photons can be absorbed and scattered. This leaves absorption line and also jagged lines on a wave characteristic graph.
Binary solar system
The same solar system
What qualities are used to classify stars
Size
Luminosity
Temperature
Distance