21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 14, Problem 37QP

(a)

To determine

The amount of mass lost.

(b)

To determine

The fraction of current mass that has been converted into energy.

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5. The Sun radiates about 4.00 x1026 J of energy into space each second. a. How much mass does the Sun lose each second due to this radiation? b. If the mass of the Sun is 2.00 x1030 kg, how long can the Sun survive if the energy release continues at the present rate?
Energy in the sun is produced by the fusion of four hydrogen atoms into a helium atom. The process involves several steps, but the net reaction is simply 41H → 4He + energy. Given this, you can say thatA. One helium atom has more mass than four hydrogen atoms.B. One helium atom has less mass than four hydrogen atoms.C. One helium atom has the same mass as four hydrogen atoms.
The highest-energy cosmic ray ever detected had an energy of about 3.0 x 1020 eV. Assume that this cosmic ray was a proton.a. What was the proton’s speed as a fraction of c?b. If this proton started at the same time and place as a photon traveling at the speed of light, how far behind the photon would it be after traveling for 1 ly?
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