Chapter 8: Problem 9
How should a satellite be launched so that its orbit takes it over every point on the (rotating) Earth?
Chapter 8: Problem 9
How should a satellite be launched so that its orbit takes it over every point on the (rotating) Earth?
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Get started for freeDetermine escape speeds from (a) Jupiter's moon Callisto and (b) a neutron star, with the Sun's mass crammed into a sphere of radius \(6.0 \mathrm{km} .\) See Appendix E for relevant data.
Tidal effects in the Earth-Moon system cause the Moon's orbital period to increase at a current rate of about 35 ms per century. Assuming the Moon's orbit is circular, to what rate of change in the Earth-Moon distance does this correspond? (Hint: Differentiate Kepler's third law, Equation 8.4, and consult Appendix E.)
To what radius would Earth have to shrink, with no change in mass, for escape speed at its surface to be \(30 \mathrm{km} / \mathrm{s} ?\)
What do Newton's apple and the Moon have in common?
Given the Moon's orbital radius of \(384,400 \mathrm{km}\) and period of 27.3 days, calculate its acceleration in its circular orbit, and compare with the acceleration of gravity at Earth's surface. Show that the Moon's acceleration is lower by the ratio of the square of Earth's radius to the square of the Moon's orbital radius, thus confirming the inverse-square law for the gravitational force.
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