1We can use what to measure the speed of rotation of a star?
- Doppler Broadening
- Wien's Law
- Stefan-Boltsmann Law
- Planck's Broadening
2We can use what to measure the speed of stars toward or away from us according to this equation?
- Stefan-Boltzmann/ Δλ/λ=Δv/c
- Doppler Shift/ Δλ/λ=Δv/c
- Stefan-Boltzmann/ energy/sec/cm^2
- Doppler Shift/ energy/sec/cm^2
3Who was it who predicted that light would shift colour if the observer or the source was moving relative to each other. Thus a star rushing towards us shows its hydrogen spectrum as colour shiftsed towards the what end of the spectrum?
- Planck/Blue
- Doppler/Red
- Planck/Red
- Doppler/Blue
4When you have a blue star and a red star at the same distance away in space, which one would be brighter?
- Red
- Blue
- They're the same, duh
5If we observe a star's peak colour output we can determine its surface temperature using:
- Doppler Broadening
- Wien's Law
- Δλ/λ=Δv/c
- Stefan-Boltzmann Law
6If you knew the peak colour of a star, as well as its distance, it would be possible to calculate the star's "______"
- Physcial Diameter
- Hydrogen Levels
- Brightness
- Ultraviolet Levels
7It's possible to calculate a star's physical diameter using?
- Wien's Law and ISL
- Stefan-Boltzmann Law and ISL
- Stefan-Boltzmann Law and Δλ/λ=Δv/c
- Wien's Law and Δλ/λ=Δv/c
8What is it that tells us the total energy/sec/cm^2 is a function of temperature raised to the 4th power?
- Wien's Law
- Planck's Radiation Law
- Stefan-Boltzmann Law
- Doppler Effect
9If a star is twice as hot as another star, the hotter star is using its energy how much faster?
- 1^6 = 24x
- They use the same amount of energy, duh
- 2^6 = 14x
- 2^4 = 16x
10Which law is an inverse relationship such that when the temperature goes up by a factor of 10, the peak wavelength decreases by a factor of 10.
- Wien's Law
- Stefan-Boltzmann Law
- Stefan-Boltzmann Law
- Doppler's Law
11The inverse relationship where when the temperature goes up by a factor of 10, and the peak wavelength decreases by a factor of 10, means that the star gets?
12Increasing the temperature of an object causes it to radiate more photons in every colour, but the peak colour moves towards which end of the spectrum?
- Red
- Ultraviolet
- Blue
- Stays in the middle
13Which law is a relationship between colour and energy/sec/cm^2 for a given temperature?
- Doppler's Effect
- Wien's Law
- Stefan-Blotzmann Law
- Planck's Radiation Law
14As they heat, objects begin to glow, their colour changing goes thorugh what order?
- Dull red, red, white and then blue-white
- Blue-white, white, red then dull red
- White, dull red, red, then blue-white
- Red, blue, then to white
15As an object heats, and begins to glow and their colours change, this is caused by what in a dense medium moving into higher orbits and them falling down to emit what?
- Electrons/Energy
- Electrons/Light
- Energy/Light
- Light/Line Spectra
16What was observed in 1900 and which meant that physics theory did not correctly predict the energy output of a hot radiating object? It was a disaster because no one knew how to solve the problem.
- Doppler Effect
- Halley's Comet
- Ultraviolet Catastrophe
- Chormatic Abberation
17Who solved the Ultraviolet Catastrophe problem by assuming energy can only be absorbed or emitted in lumps we call quanta.
- Boltzmann
- Wien
- Stefan
- Planck