Deck 36: Other Planetary Systems

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Question
Dusty and gaseous material orbiting a star is called a(an) _____.

A) exoplanet
B) protoplanetary disk
C) Doppler disk
D) brown dwarf disk
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Question
Planets orbiting stars are called _____.

A) exoplanets
B) planetary disks
C) proper motion disks
D) transit disks
Question
A new theory about many planets orbiting other stars is they formed and then ______ to their present position.

A) migrated
B) transited
C) depleted
D) proper motioned
Question
The Doppler shift method of detecting exoplanets is possible because

A) a star spins faster as planets orbit it.
B) a star spins slower as planets orbit it.
C) a star wobbles as planets orbit it.
D) a star changes color as planets orbit it.
Question
Failed stars called _________ are too small to sustain nuclear fusion.
Question
It is now thought that many planets formed and then ____ to their present positions.
Question
The largest majority of planets found around other stars are earthlike in their masses.
Question
We use the Doppler Shift Method to detect exoplanets.
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Deck 36: Other Planetary Systems
1
Dusty and gaseous material orbiting a star is called a(an) _____.

A) exoplanet
B) protoplanetary disk
C) Doppler disk
D) brown dwarf disk
protoplanetary disk
2
Planets orbiting stars are called _____.

A) exoplanets
B) planetary disks
C) proper motion disks
D) transit disks
exoplanets
3
A new theory about many planets orbiting other stars is they formed and then ______ to their present position.

A) migrated
B) transited
C) depleted
D) proper motioned
migrated
4
The Doppler shift method of detecting exoplanets is possible because

A) a star spins faster as planets orbit it.
B) a star spins slower as planets orbit it.
C) a star wobbles as planets orbit it.
D) a star changes color as planets orbit it.
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5
Failed stars called _________ are too small to sustain nuclear fusion.
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6
It is now thought that many planets formed and then ____ to their present positions.
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7
The largest majority of planets found around other stars are earthlike in their masses.
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8
We use the Doppler Shift Method to detect exoplanets.
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