2. Stars Flashcards

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1
Q

Units of Temperature

A

Kelvin

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2
Q

Celsius to Kelvin

A

+ 273

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3
Q

Black body

A

A perfect radiator and absorber, it emits and absorbs at the same rate

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4
Q

Stefan Boltzmann Law

A

Luminosity = Surface Area x SB constant x (Temperature)⁴

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5
Q

Stefan Boltzmann Constant

A

5.67 x 10(-8)

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6
Q

Wiens law

A

Peak wavelength = Weins constant / Temperature

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7
Q

Wiens constant

A

2.90 x10(-3)
Metre - kelvins

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8
Q

Wave characteristic graph

A

Y axis = Intensity
X axis = Wavelength

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9
Q

Visible light wavelength

A

400nm - 700nm

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10
Q

Inverse Square law

A

Intensity = Luminosity / 4(pi) x (Distance from earth to star)²

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11
Q

Multiwavelength astronomy

A

Helps to process images of different light
Taken using different parts of the EM spectrum

Eg. James Webb Telescope uses Infrared

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12
Q

Continuous spectrum

A

The stars emit all different gases from the surface at all frequencies - a no gaps spectrum

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13
Q

Absorption spectrum

A

When the light emitted from a star passes through the gases in its atmosphere some photons can be absorbed and scattered. This leaves absorption line and also jagged lines on a wave characteristic graph.

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14
Q

Binary solar system

A

The same solar system

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15
Q

What qualities are used to classify stars

A

Size
Luminosity
Temperature
Distance

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16
Q

What is multiwavelength astronomy

A

Using equipment that use other waves from the spectrum to observe stars that dont emit visible light

17
Q
A