Astrophysics 1 Midterm 1

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10 Terms

1
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What is Kepler’s first law?

Every planet moves in an elliptical orbit, with the sun at one of the two foci. 

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What is Kepler’s third law?

P² is proportional to a³, aka the period squared is proportional to the semimajor axis cubed. Units are yrs and AU respectively.

3
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What is Wien’s law?

The peak wavelength emitted is inversely proportional to its temperature. The hotter an object gets, the shorter the wavelengths it emits.

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What is Stefan-Boltzmann law?

The total radiant heat energy emitted per unit surface area of a blackbody is directly proportional to T^4

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What is the physical mechanism that forms spectral lines?

The lines form when electrons transition between different energy states. This is done by absorbing or emitting photons.

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What is the energy of a photon?

E= h/f or E= hc/ lambda

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How do we identify elements in the sun?

Spectroscopy, because different atoms produce different spectral lines.

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What is the Doppler effect?

The change in perceived frequency because the source or observer is moving relative to the other.

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Why is a larger telescope better than a smaller telescope?

Larger telescopes have more area to collect light, thus resulting in a higher resolution image. Also allows for further, fainter objects to be seen.

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Which wavelength band yields the highest spatial resolution?

The panochromatic band, it captures a broad range of visible light.