Using Radiation to Investigate Stars (Unit 1) Flashcards
What does the stellar spectrum consist of?
-a star emits light as a continuous spectrum, from the dense gas of the surface of the star
Where do black lines of a line absorption spectrum come from?
- light must pass through the gasses in the star’s TENOUS atmosphere
-where the atoms in the gas absorb some wavelengths of light leaving absorption lines to be superimposed on the spectrum
Black bodies definition?
A body which absorbs all the incident radiation that falls upon it
What is a good example of a black body?
-stars are very good approximations to black bodies
When we look at light emitted from a star what do we see?
- a continuous spectrum (i.e. all colours, all wavelengths)
Features of black body spectrum?
-peak wavelength is inversely proportional to the absolute temperature
- higher temp, peak intensity happens at lower wavelength
How to work out luminosity per second of a star?
Using Stefan’s constant
-power = luminosity per second
-Unit = Watt
What does A equal in Stefan’s constant?
-Surface area
Relative Luminosity?
Power/Luminosity
Surface area of sphere?
4 pi r^2
Wein’s law? words
-The wavelength of peak emission from a black body is inversely proportional to the absolute temperature of the body
Use equation to define Stefan’s law?
-The power per unit area of a blackbody is directly proportional to it’s absolute temp to the power of 4
Intensity Units?
Pm^-2
Intensity equation?
Intensity = Power / 4 pi r^2
Compare intensity of two stars from same source? equation
i 1 x (r 1)^2 = i 2 x (r 2)^2