umm I need your help! =D
I Copied this right from my math book
Distance from the Earth to the Sun:
It follows from Kepler's Third Law of planetary motion that the average distance from a planet to the sun (in meters) is:
d = ((GM/(4pi^2))^(1^3) * T^(2/3)
where M = 1.99 * 10^30 kg is the mass of the sun, G = 6.67 * 10^(-11) N * m^2/kg^2 is the gravitational constant, and T is the period of the planet's orbit(in seconds) Use the fact that the period of the earth's orbit is about 365.25 days to find the distance from the earth to the sun
I know the equations seems confusing the way I typed it out, I did the best I could but the answer I got was D = 1.4956 * 10^14
I think this is close because I looked up stuff and found the number 1.495987 * 10^11 (I dont know if this is right)
So maybe there was some kind of problem with adding/subtracting exponents? AHHH
2007-01-10
18:15:41
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5 answers
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asked by
agill15806
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Science & Mathematics
➔ Mathematics