Lunar orbit question (calculating the mass ratio of earth and moon)

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SUMMARY

The discussion focuses on calculating the mass ratio of the Earth and Moon, as well as the acceleration of free fall on the Moon's surface. The center of the Earth-Moon system is located 4.7x10^3 km from the Earth's center, with the distance between their centers being 3.8x10^5 km. The centripetal force equation is applied to relate the gravitational force to the masses and distances involved. The participants clarify that both the Earth and Moon orbit a common center of mass, and their angular velocities must be equal.

PREREQUISITES
  • Understanding of gravitational force and centripetal force equations
  • Familiarity with the concept of center of mass (COM)
  • Basic knowledge of angular velocity and tangential velocity
  • Proficiency in using constants such as G (gravitational constant) and distances between celestial bodies
NEXT STEPS
  • Calculate the mass ratio of Earth to Moon using the provided distances and gravitational equations
  • Determine the acceleration due to gravity on the Moon's surface using the formula g = G*m/r^2
  • Explore the concept of angular momentum in the Earth-Moon system
  • Investigate the effects of the Earth-Moon distance on their gravitational interaction
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Astronomy students, physics enthusiasts, and anyone interested in celestial mechanics and gravitational interactions between the Earth and Moon.

jkena04
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The problem I am struggling with is this . .

The centre of the Earth-Moon system is 4.7x10^3 km from the centre of the earth. Calculate;

i.the ratio of the mass of the Earth with the mass of the moon.
ii.The acceleration of free fall on the Moon's surface.

Constants
Distance between centre of mass of the Earth and centre of mass of moon - 3.8x10^5 km
Radius of Earth - 6.4x10^3 km
radius of moon - 1.7x10^3 km

Im a bit confused over how the moon actually orbits the earth. Do both planets orbit a centre point? If this is the case then for the Earth is in circular motion about a centre point, hence;

F(centripetal)=(m(earth)*v^2)/r = Gravitational force = (G*m(earth)*m(moon))/R^2

where R=distance between Earth and moon
r=radius of circular orbit

is this correct? also do the Earth and the moon also have the same tangential or angular speed?

Thank you in advance for your help!
 
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You could go the route of balancing the centripetal forces as you began to do. If so, you might want to cast it in terms of angular velocity rather than tangential velocity, since the angular velocities of the Earth and Moon about their mutual center of gravity must be equal (and independent of their orbital radii about the center of mass).

Alternatively, suppose you were asked to find the center of mass (COM) of two stationary objects sitting in front of you. You're given their masses, m1 and m2, and the total distance between them, d, and you need to find the distance of the COM from the center of m1 in terms of the masses and distances given. How would you proceed?
 

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