Exam 10: The Deaths of Stars

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The helium flash is the cause of some supernovae.

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As a main-sequence star exhausts hydrogen in its core, its surface becomes___ and its energy output per second (luminosity) becomes ____

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Because more massive stars have more gravitational energy, they can fuse heavier nuclear fuels.

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The theory that the collapse of a massive star's iron core produces neutrinos was supported by

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Synchrotron radiation is produced

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A planetary nebula is

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The average size of a white dwarf is about the same size as the Earth.

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A main-sequence star of 8.5 solar masses can become a white dwarf by

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Explain how we can find the age of a star cluster.

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Helium fusion does not begin until the star has entered the giant region of the H-R diagram.

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The image shows the Crab Nebula. The Crab Nebula is The image shows the Crab Nebula. The Crab Nebula is

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Giant and supergiant stars are rare because that stage of stellar evolution is short.

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Why can't a massive star generate energy through iron fusion?

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Even the youngest star clusters have no stars still contracting toward the main sequence.

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After what evolutionary stage does a star become a white dwarf?

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Star clusters are important to our study of stars because

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A Type II supernova produces a planetary nebula.

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Planetary nebulae are sites of planet formation.

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Stars in a star cluster

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An accretion disk can grow hot enough to radiate X-rays.

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