112... Astronomy In a little more than 5 billion years, our Sun will collapse to white dwarf approximately 16,000 km in diameter. (Ignore the fact that the Sun will lose mass as it ages.) (a) What will our Sun's angular momentum and rotation rate be as a white dwarf? (Express your answers as multiples of its present-day values.) (b) Compared to its present value, will the Sun's rotational kinetic energy increase, decrease, or stay the same when it becomes a white dwarf? If it does change, by what factor will it change? The radius of the Sun is presently 6.96 × 108 m. Example 9-14

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112... Astronomy In a little more than 5 billion years, our Sun will collapse to
white dwarf approximately 16,000 km in diameter. (Ignore the fact that the Sun
will lose mass as it ages.) (a) What will our Sun's angular momentum and
rotation rate be as a white dwarf? (Express your answers as multiples of its
present-day values.) (b) Compared to its present value, will the Sun's rotational
kinetic energy increase, decrease, or stay the same when it becomes a white
dwarf? If it does change, by what factor will it change? The radius of the Sun is
presently 6.96 × 108 m. Example 9-14
Transcribed Image Text:112... Astronomy In a little more than 5 billion years, our Sun will collapse to white dwarf approximately 16,000 km in diameter. (Ignore the fact that the Sun will lose mass as it ages.) (a) What will our Sun's angular momentum and rotation rate be as a white dwarf? (Express your answers as multiples of its present-day values.) (b) Compared to its present value, will the Sun's rotational kinetic energy increase, decrease, or stay the same when it becomes a white dwarf? If it does change, by what factor will it change? The radius of the Sun is presently 6.96 × 108 m. Example 9-14
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