Exam 16: Evolution of Low-Mass Stars

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Degenerate refers to a state of matter at:

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Describe the structure of a red giant star just before the helium flash takes place.How does this compare to the structure of a horizontal-branch star?

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What is the name of the nuclear reaction illustrated here? What is the name of the nuclear reaction illustrated here?

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The Ring Nebula is a planetary nebula that currently has a radius of 1.2 × 1013 km and an expansion velocity of 250 km/s.Approximately how long ago did its parent star die and eject its outer layers?

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When helium fusion begins in the core of a red giant star,the situation quickly gets out of control because electron-degeneracy pressure does not respond to changes in:

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In what two ways does temperature affect the rate of nuclear reactions?

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Why are novae thought to reoccur repeatedly?

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The Sun eventually could become a nova.

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Explain what the triple-alpha process is and when it takes place in evolving stars.

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A star's surface temperature during the horizontal branch phase is determined primarily by its:

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A 1M⨀ star in a binary system could create the following chemical element and eject it into the interstellar medium:

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A white dwarf star has a luminosity equal to 10−4 L⨀ and a temperature twice that of the Sun (i.e. ,T = 10,600 K).What is the radius of the white dwarf,expressed as a ratio to the solar radius?

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A low-mass main-sequence star's climb up the red giant branch is halted by:

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Why does the core of a main-sequence star have to be hotter to burn helium into carbon than hydrogen into helium?

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During which phase of the evolution of a low-mass star does it have two separate regions of nuclear burning occurring in its interior?

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A white dwarf with a temperature of 30,000 K would shine brightest at what wavelength?

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If a main-sequence star were gaining mass by being in an interacting binary system,what would happen to that star's luminosity and why?

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As a main-sequence star burns its core supply of hydrogen,what happens?

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When a spectral-type G2 star like the Sun leaves the main sequence:

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The gas in a planetary nebula is composed of:

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