Chapter 8: Problem 3
When you stand on Earth, the distance between you and Earth is zero. So why isn't the gravitational force infinite?
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Chapter 8: Problem 3
When you stand on Earth, the distance between you and Earth is zero. So why isn't the gravitational force infinite?
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Determine escape speeds from (a) Jupiter's moon Callisto and (b) a neutron star, with the Sun's mass crammed into a sphere of radius \(5.7 \mathrm{~km}\). See Appendix E for relevant data.
As a member of the 2040 Olympic committee, you're considering a new sport: asteroid jumping. On Earth, world-class high jumpers routinely clear \(2 \mathrm{~m}\). Your job is to make sure athletes jumping from asteroids will return to the asteroid. Make the simplifying assumption that asteroids are spherical, with average density \(1700 \mathrm{~kg} / \mathrm{m}^{3}\). For safety, make sure even a jumper capable of \(2.8 \mathrm{~m}\) on Earth will return to the surface. What do you report for the minimum asteroid diameter?
What's the approximate value of the gravitational force between a \(69-\mathrm{kg}\) astronaut and a \(77,000-\mathrm{kg}\) spacecraft when they're \(80 \mathrm{~m}\) apart?
Though the Sun's gravitational pull is much stronger than that of the Moon, the ocean tides on the Earth are caused principally by the Moon. Why?
Exact solutions for gravitational problems involving more than two bodies are notoriously difficult. One solvable problem involves a configuration of three equal-mass objects spaced in an equilateral triangle. Forces due to their mutual gravitation cause the configuration to rotate. Suppose three identical stars, each of mass \(M\), form a triangle of side \(L\) Find an expression for the period of their orbital motion.
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