Calculate Mass of Moon from Earth & Diameter

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Calculating the mass of the Moon involves understanding its orbital dynamics and gravitational interactions with Earth. The mass can be derived using the formula that relates the sum of the masses of Earth and the Moon to the orbital period and distance. Accurate measurements of the Moon's distance and orbital period are essential, as well as the gravitational constant. Satellites orbiting the Moon provide direct measurements of gravitational acceleration, aiding in mass calculations. Overall, determining the Moon's mass requires precise data and an understanding of celestial mechanics.
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hi, i can calculate the distance of moon from the Earth and its diameter - but i could't get the formula by which i can calculate the mass of the moon - although i can calculate the mass of the moon by assuming it has same average density that of Earth -
 
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The orbital period of the moon depends on its distance and the sum of masses of Earth and moon - if you can determine this sum with sufficient precision, you can subtract the mass of Earth and get the mass of moon.
Satellites orbiting the moon are a better way to determine its mass - they give direct access to the gravitational acceleration at a specific distance, together with the gravitational constant this can be used to calculate its mass.
 
but how do i calculate the sum of Earth and moon mass?
 
Measure distance, orbital period and the gravitational constant.

##M+m=\frac{4\pi^2a^3}{GT^2}## with the semi-major axis a (for a circular orbit, this would be the distance)
 
I'm curious as to how you calculated the distance between the Moon and Earth. That distance might not be the semi-major axis of the Moon's orbit. It might be the sum of the Moon's semi-major axis and the Earth's semi-major axis, as measured from their combined center of mass. (The 'a' in the previous equation is actually the sum of the semi-major axes, or the distance you most likely calculated.)

In practice, calculating the mass and the semi-major axis of planets was an almost impossible task even after Newton turned Kepler's Third Law into a formula. You had a formula containing three unknown variables (the universal gravitational constant, the mass, and the semi-major axis) and the only known was the orbital period.

In fact, that's why the Earth's semi-major axis for it's orbit around the Sun was measured in astronomical units, with one AU being the distance between the Sun and the Earth. You could measure Jupiter's semi-major axis in AU's, but had no way to convert that into a more traditional measure such as kilometers.
 
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