Deck 58: The Sizes of Stars
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Deck 58: The Sizes of Stars
1
If you know a star's temperature and use the Stefan-Boltzmann law you can find _____.
A) luminosity
B) distance
C) size
D) mass
A) luminosity
B) distance
C) size
D) mass
luminosity
2
A technique to find diameters of stars using short exposures is called
A) luminosity measurements.
B) speckle interferometry.
C) mass interferometry.
D) parallax.
A) luminosity measurements.
B) speckle interferometry.
C) mass interferometry.
D) parallax.
speckle interferometry.
3
Using the Stefan-Boltzman law to find luminosity requires _______.
A) radius and temperature
B) velocity and distance
C) brightness and radius
D) period and temperature
A) radius and temperature
B) velocity and distance
C) brightness and radius
D) period and temperature
radius and temperature
4
The technique of combining the light from two or more smaller telescopes to obtain an image that is equivalent to that of a much larger telescope is called
A) speckle imaging
B) adaptive optics
C) interferometry
D) angular resolution
A) speckle imaging
B) adaptive optics
C) interferometry
D) angular resolution
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5
________ create a light curve we can estimate the stars' sizes from.
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6
Using two or more telescopes to measure the angular sizes of stars is called ______.
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7
Eclipsing binaries cannot be used to measure masses of stars.
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8
New interferometry techniques have measured many sizes of stars far from Earth.
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