21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 17, Problem 16QP
To determine

The differences between the ways the hydrogen is converted into helium in a low-mass star and in a high-mass star, the catalyst in CNO cycle and the way in which it takes part in the reaction.

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Calculate the total energy output per second in watts (W) of a star that converts 900 million tonnes of hydrogen per second into helium, with a mass difference of 6.30 million tonnes per second due to nuclear fusion. Use E = Δmc2 and c = 3.0 × 108 m s-1.
What is the escape velocity (in km/s) from the surface of a 1.5 M neutron star? From a 3.0 M neutron star? (Hint: Use the formula for escape velocity,  Ve =    2GM r ;  make sure to express quantities in units of meters, kilograms, and seconds. Assume a neutron star has a radius of 11 km and assume the mass of the Sun is 1.99 ✕ 1030 kg.) 1.5 M neutron star km/s3.0 M neutron star km/s
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