Newton's Law of Universal Gravitation:
F = -G(m1m2)/r^2
where
F is the magnitude of the (repulsive) gravitational force between the two point masses
G is the gravitational constant (6.67 × 10^−11 N m2 kg−2)
m1 is the mass of the first point mass (5kg)
m2 is the mass of the second point mass (5.9736 * 10^24 kg)
r is the distance between the two point masses (Radius of Earth + height = 6.37101 * 10^6m + 1 * 10^7 m)
Note: You have to include the radius of earth, because gravity is held to originate from the center point.
Plug it in:
F = 6.67 × 10^−11 N m2 kg−2 * (5kg * 5.9736 * 10^24 kg) / (6.37101 * 10^6m + 1 * 10^7 m)^2
F = 6.67 × 10^−11 N m2 kg−2 * (2.9868 *10^25 kg^2) / (1.637101 * 10^7m)^2
F = 6.67 × 10^−11 N m2 kg−2 * (2.9868 *10^25 kg^2) / (2.6801 * 10^14 m^2)
F = 6.67 × 10^−11 N m2 kg−2 * 1.1144 * 10^11 kg^2/m^2
F = 6.67 × 10^−11 N m2 kg−2 * 1.1144 * 10^11 kg^2/m^2
F = 7.433048 N
2006-08-29 01:25:31
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answer #1
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answered by ³√carthagebrujah 6
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2016-12-11 17:08:06
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answer #2
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answered by dricketts 4
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use newton's universal gravitational law ( Gravitational force = GMm/(r^2), M and m are the masses of which the gravitational force acts on each other. )
2006-08-29 01:19:42
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answer #3
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answered by vicks 2
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Why are you trying to be smart? Just ask a normal question will you. Are you an anorak???
2006-08-29 00:19:49
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answer #4
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answered by trog 3
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I know this, the answer is 42! lol
2006-08-29 00:31:08
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answer #5
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answered by Anonymous
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This website is ideal for you:
http://www.antonine-education.co.uk/Physics_A2/Module_4/Topic_8/topic_8.htm
2006-08-29 00:27:09
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answer #6
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answered by Allasse 5
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full tides at 6.15 pm
2006-08-29 00:10:47
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answer #7
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answered by Anonymous
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