21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 15.3, Problem 15.3CYU
To determine

The origin of required energy for the fusion in a protostars.

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The theory that the collapse of a massive star’s iron core produces neutrinos was supported by   a. the size and structure of the Crab nebula.   b. laboratory measurements of the mass of the neutrino.   c. the brightening of supernovae a few days after they are first visible.   d. underground counts from solar neutrinos.   e. the detection of neutrinos from the supernova of 1987.
Which of the following statements about various stages of core nuclear burning (hydrogen, helium, carbon, etc.) in a high- mass star is not true? A. As each stage ends, the core shrinks and heats further. B. Each successive stage creates an element with a higher atomic number and atomic mass number. C. As each stage ends, the reactions that occurred in previous stages continue in shells around the core. D.Each successive stage lasts for approximately the same amount of time.
The diagram below shows an H-R diagram with life track of a 1-solar-mass star, with various stages labeled A through E. Temperature What will happen to the star after stage E? A. It will gain mass until it collapses under its own weight. B. It will begin burning carbon in its core. C. It will explode in a supernova. D. It will collapse to make a neutron star. E. It will eject a planetary nebula. Luminosity →
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