Stars as Black Bodies Flashcards

1
Q

What is a black body?

A

A perfect absorber and emitter
A body that absorbs and emits all wavelengths of EM radiation
Appears perfectly black when cold
When heated above absolute zero, it emits light across the whole EM spectrum

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2
Q

Objects hotter than absolute zero emit electromagnetic radiation due to what?

A

Their temperature.

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3
Q

What radiation is everyday temperature?

A

Infrared (which we can’t see)

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4
Q

Why do things glow (and emit visible light) if we heat them up?

A

The wavelengths of radiation emitted depend on the temperature of the object.
(High energy means shorter wavelength - visible shorter than infrared)

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5
Q

In what way does a pure black surface emit radiation?

A

strongly and well defined

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6
Q

The graph of intensity against wavelength varies with what?

A

TEMPERATURE

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7
Q

What does black body radiation produce?

A

A Continuous spectrum of EM radiation

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8
Q

What are the main two characteristics of a black body curve, with power output against wavelength?

A

peak on short wavelengths, so steeper on the curves left side

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9
Q

What does the peak in a black body curve give?

A

Temperature

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10
Q

What things are considered approximately black bodies?

A

Stars (and other astronomical sources)

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11
Q

The power output is what?

A

The luminosity

Total energy it emits per second

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12
Q

What is power output related to?

A

Temperature and surface area

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13
Q

What does Wein’s law say?

A

For a hot object, the wavelength of peak emission intensity is inversely proportional to the absolute temperature of the object.
(Higher surface temperature of a star = shorter peak wavelength)

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14
Q

What does a hotter black body mean?

A

Emit more radiation
Peak wavelength is a shorter wavelength
Higher total energy output (assuming surface area is the same)

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15
Q

Why may hotter stars not be as bright?

A

May mostly emit radiation that isn’t visible light.

If a cooler star emits more visible light radiation, it will appear brighter.

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16
Q

What is power output proportional and directly proportional to?

A

Power proportional to (stars surface Temperature)^4

Power directly proportional to surface area

17
Q
P = 
σ = 
A = 
T = 
What is each one?  What is it measured in? What is the equation?
A

Stefan’s Law:

Power output in watts
Stefan’s Constant
Surface area in meters squared
Temperature in Kelvin

18
Q

What law does intensity obey?

A

Inverse square law

19
Q

What’s the equation for inverse square law for intensity?

A

I = P / 4πd²

20
Q

What does the intensity equation show?

A

As radiation spreads out and becomes more diluted. Intensity decreases.

21
Q

What is assumed for inverse square law to apply

A

Star is spherical

22
Q

What is assumed that the stars act as for Wien’s, Stefan’s and Inverse Law to work?

A

Stars behave as black bodies