Exam 8: The Deaths of Stars

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Theory predicts that neutron stars may not exceed 3 solar masses.

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What is the approximate size of the Schwarzschild radius of a one solar mass black hole?

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

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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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If neutron stars contain no nuclear fuel,why are they hot?

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  -The diagram shows a light curve from a supernova.How many days after maximum light did it take for the supernova to decrease in brightness by 5 magnitudes? -The diagram shows a light curve from a supernova.How many days after maximum light did it take for the supernova to decrease in brightness by 5 magnitudes?

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Why can't the lowest mass stars become giants?

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Which of the following offered support for the theory that the collapse of a massive star's iron core produces neutrinos?

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Suppose you discover a binary star system with a 0.7 solar mass giant star and a 2 solar mass main sequence star.Why is this surprising?

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Type II supernovae are believed to occur when the cores of massive stars collapse.

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Why can't pulsars be spinning white dwarfs?

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What is the term for a collection of 10⁵ to 10⁶ old stars in a region 30 to 100 light-years in diameter?

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Why does our theory predict that neutron stars will have strong magnetic fields?

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A three solar mass black hole has a Schwarzschild radius of about 9 km.How big would the Schrwarzschild radius of a 1000 solar mass black hole be?

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From what part of the H-R diagram have the giants in a star cluster evolved?

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If you had an extremely sensitive radio telescope,could you detect every pulsar in the Milky Way galaxy?

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Which of the following would be most likely to indicate the presence of an isolated black hole?

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How fast is the escape velocity at the event horizon around a black hole?

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  -What is the approximate age of the star cluster in the H-R diagram?  (Hint: Main sequence stars of spectral types O and B have a core supply of hydrogen that is sufficient to last about 250 million years;types A and F,about 2 billion years;type G about 10 billion years;types K and M about 30 billion years.The apparent magnitude scale means that larger numbers are toward the bottom of the vertical axis.) -What is the approximate age of the star cluster in the H-R diagram? (Hint: Main sequence stars of spectral types O and B have a core supply of hydrogen that is sufficient to last about 250 million years;types A and F,about 2 billion years;type G about 10 billion years;types K and M about 30 billion years.The apparent magnitude scale means that larger numbers are toward the bottom of the vertical axis.)

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What properties of degenerate matter are important to the structure of stars? Why?

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