How Do Planetary Orbits Reveal the Masses of Stars and Heights of Satellites?

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SUMMARY

The discussion centers on calculating the mass of the star HD 179949 and the height of the International Space Station (ISS) based on their respective orbital characteristics. The "hot Jupiter" planet discovered in 2004 orbits HD 179949 at a distance of 1/9 that of Mercury from the Sun, completing an orbit in 3.09 days. The mass of the star can be determined using Kepler's laws, while the ISS's altitude can be calculated from its orbital period of 15.65 revolutions per day.

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1) In 2004 astronomers reported the discovery of a large Jupiter-sized planet orbiting very close to the star HD 179949 (hence the term "hot Jupiter"). The orbit was just 1/9 the distance of Mercury from our sun, and it takes the planet only 3.09 days to make one orbit (assumed to be circular). What is the mass of the star? Express your answer (a)in kilograms and (b)as a multiple of our sun's mass.
How fast (in km/s) is this planet moving?

2) The International Space Station makes 15.65 revolutions per day in its orbit around the earth. Assuming a circular orbit, how high is this satellite above the surface of the earth?
 
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Please show some attempt at the solution. Once we see we're your trouble is, we'd be glad to help you.
 

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