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Kepler's 3rd Law - Advanced The above equation might seem intimidating but you may notice the familiar t² = r³ embedded in the formula. The 'G' is the Universal Constant of Gravitation and the 'm' represents the sum of the masses of 2 orbital bodies. 't' is the time of one orbital period and 'r' is the average orbital radius. By taking the value of 4 π² as 39.730 and using the C.G.S. value of 'G' = 6.6739 x 10-8, the formula becomes:
where 'm' is stated in grams, 't' in seconds and 'r' in centimeters. The
formula might still seem unwieldly but don't worry - this calculator does
all the work for you !!!
Click on the 'RADIUS' button, enter the time and mass, click on 'CALCULATE' and the answer is 4.226 x109 centimeters or 4.226 x107 meters or 42,260 kilometers or 26,260 miles. (This is the distance as measured from the Earth's center).
2) The Moon orbits the Earth at a center-to-center distance of
3.86 x1010 centimeters (3.86 x108 meters). As for determining the mass to use, scroll
to the top of the page. You will see that the 'M' in the formula stands
for the mass of both orbital bodies. Usually, the mass of one is
insignificant compared to the other. However, since the Moon's mass is about
1/81 that of the Earth's, it is importatnt to use the sum of their
masses. Since the Moon's mass= .0735 X1027 grams and the Earth's
mass = 5.979 x1027 grams, then their sum = 6.0525 x1027
grams (6.0525 x1024 kilograms).
Now that you have this information, how long does it take the Moon to
make one revolution around the Earth?
3) Every 151,200 seconds, Io orbits Jupiter at an orbital radius of
4.218 x 1010 centimeters (4.218 x 108 meters). What is Jupiter's Mass?
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