Stars as Black Bodies Flashcards

1
Q

What is a black body?

A

An object with a pure black surface that emits radiation strongly and in a well-defined way and absorbs all light incident on it.

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2
Q

Outline the graph of wavelength against power output.

A
  • Black body curves
  • Depends on temperature
  • Visible wavelengths between about 0.25 and 0.75 micro-metres
  • Peak shifts for different curves (shallower curves)
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3
Q

What is the generic definition of a black body?

A

A black body is a body that absorbs all electromagnetic radiation of all wavelengths and can emit all wavelengths of electromagnetic radiation.

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4
Q

What can we use black body radiation curves for?

A

Estimating an object’s temperature and other properties.

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5
Q

What is Wien’s displacement law?

A

All black body spectra have a peak intensity. The wavelength that this peak occurs at is called the peak wavelength. The higher the surface temperature, the shorter the peak wavelength.

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6
Q

What are the general findings of Wien’s law?

A

A hotter black body will emit more radiation than a cooler one, and it’s peak wavelength will be a shorter wavelength. Also has a higher power output.

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7
Q

What is Stefan’s law?

A

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

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8
Q

State an equation for intensity of a star in relation to it’s power output and distance.

A

I = P / 4πd^2

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9
Q

What is the relationship between distance and intensity of a star?

A

Inverse square law.

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10
Q

What are the assumptions about a star when using the inverse square law?

A

The star is spherical and gives out an even amount of power in every direction.

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