Chapter 14: Problem 27
A reconnaissance spacecraft circles the Moon at very low altitude. Calculate (a) its speed and \((b)\) its period of revolution. Take needed data for the Moon from Appendix C.
Chapter 14: Problem 27
A reconnaissance spacecraft circles the Moon at very low altitude. Calculate (a) its speed and \((b)\) its period of revolution. Take needed data for the Moon from Appendix C.
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Get started for freeA comet moving in an orbit of eccentricity \(0.880\) has a speed of \(3.72 \mathrm{~km} / \mathrm{s}\) when it is most distant from the Sun. Find its speed when it is closest to the Sun.
A rocket is accelerated to a speed of \(v=2 \sqrt{g R_{\mathrm{E}}}\) near the Earth's surface and then coasts upward. (a) Show that it will escape from the Earth. ( \(b\) ) Show that very far from the Earth its speed is \(v=\sqrt{2 g R_{\mathrm{E}}}\).
The planet Mars has a satellite, Phobos, which travels in an orbit of radius \(9400 \mathrm{~km}\) with a period of 7 h 39 min. Calculate the mass of Mars from this information. (The mass of Phobos is negligible compared with that of Mars.)
It is conjectured that a "burned-out" star could collapse to a "gravitational radius," defined as the radius for which the work needed to remove an object of mass \(m\) from the star's surface to infinity equals the rest energy \(m c^{2}\) of the object. Show that the gravitational radius of the Sun is \(G M_{\mathrm{S}} / c^{2}\) and determine its value in terms of the Sun's present radius. (For a review of this phenomenon see "Black Holes: New Horizons in Gravitational Theory," by Philip C. Peters, American Scientist, September- October \(1974, \mathrm{p} .575 .)\)
Express the universal gravitational constant \(G\) that appears in Newton's law of gravity in terms of the astronomical unit \(\mathrm{AU}\) as a length unit, the solar mass \(M_{\mathrm{S}}\) as a mass unit, and the year as a time unit. \(\left(1 \mathrm{AU}=1.496 \times 10^{11} \mathrm{~m}, 1 \mathrm{M}_{\mathrm{S}}=1.99 \times\right.\) \(\left.10^{30} \mathrm{~kg}, 1 \mathrm{y}=3.156 \times 10^{7} \mathrm{~s} .\right)(b)\) What form does Kepler's third law (Eq. \(14-23\) ) take in these units?
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