Exam 12: Star Stuff

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The ultimate fate of our Sun is to ________.

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After a supernova explosion, the remains of the stellar core ________.

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What can we learn about a star from a life track on an H-R diagram?

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Why is a 1 solar-mass red giant more luminous than a 1 solar-mass main sequence star?

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Photographs of many young stars show long jets of material apparently being ejected from their poles.

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Which of the following types of data provide evidence that helps us understand the life tracks of low-mass stars?

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Consider a large molecular cloud that will give birth to a cluster of stars. Which of the following would you expect to be true?

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Which star spends the longest time in the protostellar phase of life?

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In order to predict whether a star will eventually fuse oxygen into a heavier element, you mainly want to know what fact about the star?

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Which event marks the beginning of a supernova?

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Which statement about this cluster is not true?

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What is the CNO cycle?

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Choose from the list below for the following questions. You may use a choice more than once. -Which one is used by a main-sequence star of spectral type B2?

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Which element is the dead end for cores of the most massive stars?

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This diagram represents the life track of a 1 solar mass star. Refer to the life stages labeled with roman numerals. Which stage lasts the longest?

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Compared to the star it evolved from, a red giant is

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After a supernova event occurring in a high-mass star, what is left behind?

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What is the CNO cycle?

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Which process is required to allow a gravitationally-collapsing gas cloud to continue to collapse?

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Do you think it is possible that a 1.5-solar-mass red giant could harbor an advanced civilization? Explain your reasoning.

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