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As a main sequence star evolves off the main sequence, the helium core is contracting while the outer envelope is _______________.

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expanding

As a one-solar-mass star evolves off the main sequence, it will probably undergo a _____.


A) nova burnout
B) helium flash
C) hydrogen flash
D) helium bang
E) carbon flash

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Degenerate matter has two peculiar properties that can affect a star.  One is that the degenerate gas resists compression, and the other is that the degenerate gas ____.


A) is not density dependent
B) does depend on temperature
C) does not depend on temperature
D) is not pressure dependent.
E) does depend on the type of nuclei present

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C

List the two basic types of intrinsic variable stars.

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1 Cepheid ...

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Explain how one of the four laws of stellar structure works.

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1 Hydrostatic Equilibrium:  The weight o...

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Observing star clusters will give astronomers needed data for stellar evolution because all the stars in the cluster have the same ____.


A) masses
B) temperatures
C) ages
D) luminosities
E) apparent magnitudes

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Define nuclear fusion.

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Nuclear fusion is the combining of light...

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When a gas is so dense that most of its electrons are not free to change their energies, it is called _______________.

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Why is there an upper end in the main sequence of the H-R diagram?

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The upper end in the main sequence of th...

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Cepheid variable stars are classified as either ____.


A) Type A or Type B
B) Type I or Type II
C) Class A or Class B
D) Class I or Class II
E) Type C or Type R

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The period-luminosity relation for Cepheid and RR Lyrae variable stars can be used for ______________.

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distance m...

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If you observe a variable star with a period of 50 days as a yellow, supergiant star, then you most likely have seen a(n) ____.


A) degenerate star
B) RR Lyrae variable star
C) eclipsing binary star
D) Cepheid variable star
E) Type I Pulsar

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Giant and supergiant stars are rare because they do not form as often as main sequence stars.

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The age of a star cluster can be approximated by finding its turnoff point in the distribution of data points that represent stars on the H-R Diagram.

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Astronomers determine the internal structure of a star by using stellar models, since they cannot "see" into the interior of a star.

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What is degenerate matter?

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Degenerate matter is a gas tha...

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There is a mass-luminosity relationship because stars support their weight by generating energy, and more massive stars have more weight to support.

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Briefly explain why there is a main sequence on the H-R Diagram.

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Models of stars show that there is a mai...

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When the Sun moves off the main sequence, it will initially become a red supergiant.

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Astronomers can determine the interiors of main sequence stars by _____.


A) studying their atmospheres
B) creating stellar models
C) detailed observations of the Sun
D) using the Hertzsprung-Russell Stellar Model (HRSM)
E) satellite observations of the closest stars

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B

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