Exam 17: Evolution of High-Mass Stars

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Using the formula g =GMNS/R2NS, calculate the acceleration of gravity on a 2 MSUN neutron with a radius of 10 km, and express this in terms of the acceleration of gravity on the surface Of Earth (g = 9.8 m/s2).

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You observe three star clusters and construct their respective H-R diagrams.Cluster 1 has a main-sequence turnoff point at spectral type G, Cluster 2 has a turnoff point at spectral type A, and Cluster 3 has a turnoff point at spectral type B.Which cluster is the youngest and which is the oldest? Explain why.What is the approximate age of the oldest cluster?

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Which of the following is the correct order for elements fused (as fuel) in the core of late-stage high-mass stars?

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The nuclear fusion reactions involved in the CNO cycle require much higher temperatures than the reactions within the proton-proton chain because

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Short gamma-ray bursts (GRBs) are most likely caused by

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Why is the CNO cycle the primary fusion cycle in only high-mass stars?

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Where did the iron in your blood come from?

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If a 25 MSUN main-sequence star loses mass at an average rate of 10-6 MSUN/yr while on the main sequence, then how much mass will it lose in its lifetime of about 7 million years?

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We can identify only a fraction of all the radio pulsars that exist in our galaxy because

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As a high-mass main-sequence star evolves off the main sequence, it follows a ________ on the H-R diagram.

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Type Ia and Type II supernovae are respectively caused by what types of stars?

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Iron has 26 protons in its nucleus, and gold has 79 protons.Where did all the gold on Earth come from?

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A neutron star in a mass-transfer binary system is called

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The figure below shows the H-R diagram for the very young cluster NGC 6530.Notice that the main sequence is missing the low-luminosity red tail.At the same time, there are several reddish and yellowish objects to the right of the main sequence (clearly marked).What could these objects represent? The figure below shows the H-R diagram for the very young cluster NGC 6530.Notice that the main sequence is missing the low-luminosity red tail.At the same time, there are several reddish and yellowish objects to the right of the main sequence (clearly marked).What could these objects represent?

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The luminosity of a Cepheid star varies in time because

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Type I and Type II supernovae can be distinguished by what combination of observations?

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Explain why neutron stars are fast-spinning objects and why they have very strong magnetic fields.

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The main difference between classical Cepheids and RR Lyrae stars is

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Supernovae are very energetic events.Of the following events, which is the brightest that a supernova can outshine at their maximum?

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One reason why we think neutron stars were formed in supernova explosions is that

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