Chapter 4: Problem 26
Suppose that the Earth were moved to a distance of \(3.0 \mathrm{AU}\) from the Sun. How much stronger or weaker would the Sun's gravitational pull be on the Earth? Explain.
Chapter 4: Problem 26
Suppose that the Earth were moved to a distance of \(3.0 \mathrm{AU}\) from the Sun. How much stronger or weaker would the Sun's gravitational pull be on the Earth? Explain.
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(a) In what direction does a planet move relative to the horizon over the course of one night? (b) The answer to (a) is the same whether the planet is in direct motion or retrograde motion. What does this tell you about the speed at which planets move on the celestial sphere?
In what direction does a planet move relative to the stars when it is in direct motion? When it is in retrograde motion? How do these compare with the direction in which we see the Sun move relative to the stars?
Explain why the semimajor axis of a planet's orbit is equal to the average of the distance from the Sun to the planet at perihelion (the perihelion distance) and the distance from the Sun to the planet at aphelion (the aphelion distance).
Figure 4-21 shows the lunar module Eagle in orbit around the Moon after completing the first successful lunar landing in July 1969. (The photograph was taken from the command module Columbia, in which the astronauts returned to Earth.) The spacecraft orbited \(111 \mathrm{~km}\) above the surface of the Moon. Calculate the period of the spacecraft's orbit. See Appendix 3 for relevant data about the Moon.
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