Calculate Mass of Moon from Earth & Diameter

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SUMMARY

The mass of the Moon can be calculated using the formula M+m=\frac{4\pi^2a^3}{GT^2}, where M is the mass of the Moon, m is the mass of the Earth, a is the semi-major axis, G is the gravitational constant, and T is the orbital period. To determine the mass of the Moon accurately, one must measure the distance (semi-major axis) and the orbital period of satellites orbiting the Moon. This method provides direct access to gravitational acceleration, which, when combined with the gravitational constant, allows for precise mass calculations. The discussion highlights the challenges faced in calculating celestial masses, particularly before the advancements in gravitational theory.

PREREQUISITES
  • Understanding of Kepler's Third Law of planetary motion
  • Familiarity with gravitational constant (G)
  • Knowledge of orbital mechanics and satellite dynamics
  • Basic mathematical skills for manipulating equations
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  • Research the application of Kepler's Third Law in celestial mechanics
  • Study the methods for measuring gravitational acceleration of celestial bodies
  • Learn about the gravitational constant and its significance in astrophysics
  • Explore techniques for calculating the semi-major axis of orbits
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Astronomers, astrophysicists, students studying celestial mechanics, and anyone interested in calculating the mass of celestial bodies like the Moon.

wasi-uz-zaman
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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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