Physics
Physics, 02.07.2019 21:30, madelyngv97

Let t be the period of a planet about the sun; that is, t is the time required for it to travel once are 2a and 2b. (a) use part (d) of problem 1 to show that t-2tab/h (b) show that_-ed=-. 2. lliptical orbit. su h2 gm b2 cl 4t2 gm (c) use parts (a) and (b) to show that ta this proves kepler's third law. [notice that the proportionality constant 4? 9(gm) is inde- pendent of the planet.]

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