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help with orbitals... |
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| Apr27-05, 01:57 PM | #1 |
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help with orbitals...
I have no idea where to start on this:
A satellite is in a circular orbit very close to the surface of a spherical planet. The period of the orbit is 1.69 hours. What is density of the planet? Assume that the planet has a uniform density. Perhaps someone could point me in the right direction? Thanks. |
| Apr27-05, 02:23 PM | #2 |
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Hint: Kepler's Third Law of Planetary Motion
and the fact that the satellite is near the planet's surface. http://scienceworld.wolfram.com/phys...sThirdLaw.html http://scienceworld.wolfram.com/physics/MeanMotion.html |
| Apr27-05, 02:24 PM | #3 |
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1. You should know that the centripetal force causing the satellite to be in the circular orbit is due to the gravitational force, so equate the two, i.e. [tex]\frac{GmM}{R^2} = \frac{mv^2}{R}[/tex] 2. But you also know that [tex]v = r\omega[/tex] [tex]\omega =2\pi/T[/tex] [tex]\rho = \frac{M}{4/3 \pi R^3}[/tex] 3. A bunch of things cancel out and you should be able to do the simple algebra to find the density. Zz. |
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