Stars as Black Bodies Flashcards

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1
Q

What is a black body?

A

A body that absorbs all EM radiation of all wavelengths and can emit all wavelengths of EM radiation

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2
Q

What can stars be approximated to?

A

As black bodies

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3
Q

What is a black body radiator?

A

A perfect emitter and absorber of all possible wavelengths of radiation.

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4
Q

What does Wien’s law show?

A

as the black body gets hotter, the peak wavelength decreases, the frequency increases and the energy of the wave increases.

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5
Q

What is Wien’s law used for?

A

To estimate the temperature of black-body sources.

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6
Q

What does the intensity of light emitted by a star follow?

A

the inverse square law, meaning intensity is inversely proportional to the distance between the star and the observer.

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7
Q

What is Stefan’s law?

A

The power output of a star is the total power of the star’s surface temperature and is directly proportional to the surface area.

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8
Q

From Earth, we can measure the intensity of a star. What is the intensity of a star?

A

the power of radiation per square metre, so as the radiation spreads out and becomes diluted, the intensity decreases.

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9
Q

what do need to assume to use the inverse square law?

A

you need to assume that the star is spherical, and it gives you out an even amount of power in every direction

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10
Q

How do you use all the 3 laws to work out all sorts of things about stars?

A

you assume that stars behave as black bodies.

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11
Q

What objects emit EM radiation?

A

All objects that are hotter than absolute zero emit EM radiation due to their temperature.

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