Gravitational pull with the earth and moon

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SUMMARY

The discussion focuses on calculating the location of the L1 point between the Earth and the Moon, where gravitational forces cancel each other out. The mass of the Moon is stated as 7.35x10^22 kg, and the distance between the Earth and the Moon is 3.84x10^5 km. The ratio of the masses of the Earth and Moon is established as 81, derived from the gravitational equations. The mass of the Earth is confirmed to be 5.9736x10^24 kg, providing a definitive basis for the calculations.

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alicia113
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Homework Statement



The mass of the moon is 7.35x10^22 kg. At some point between Earth and the Moon, the force of Earth's gravitational attraction on an object is canceled by the Moon's force of gravitational attraction. If the distance between the Earth and the moon (center to center) is 3.84x10^5 km, calculate where this will occur, relative to the Earth.

The Attempt at a Solution


ok now this is from another thread, and i completely understand how she got everyting but the 81! could someone please explain to me how she got the 81.. thts the only part I am lost in..

We assume an object is at the L1 point (the point where the gravitational fields of the two objects cancels out). We will call this object X

r is the radius between the Earth and the Moon
We will call
r1
the point from the center of the Earth to x and
r2
the point from x to the center of the moon
Therefore
(1)
r=r1+r2Using this assumption of the object X we get..

Fg=Gm1xr21
where
m1
is the mass of the earth, and x is the mass of object X
Fg=Gm2xr22
where
m2
is the mass of the moon, and x is the mass of object X

Since we know that, at the point where the object X is situated, the gravitiational pull from both the Earth and the Moon will be equal, we can equate the above two equations getting the following:
(2)
Gm1xr21=Gm2xr22Now, we obtain a ratio between
m1
and
m2
so we can express
m1
in terms of
m2m1m2=81
(Note: I rounded to 81 just to make typing it up here easier...)
Therefore,
m1=81m2Now, going back to equation (2), G and x will cancel out and we replace
r1
with
r−r2
(from equation (1)) leaving us with:
81m2(r−r2)2=m2r22m2
will cancel out:
81(r−r2)2=1r2281=(r−r2)2r22i take the square root of both sides, and put the denominator on the left side
9r2=r−r210r2=rr2=r/10r2=3.84∗104Since
r1=r−r2r1=3.84∗105−3.84∗104r1=3.456∗105
 
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alicia113 said:

Homework Statement



The mass of the moon is 7.35x10^22 kg. At some point between Earth and the Moon, the force of Earth's gravitational attraction on an object is canceled by the Moon's force of gravitational attraction. If the distance between the Earth and the moon (center to center) is 3.84x10^5 km, calculate where this will occur, relative to the Earth.

The Attempt at a Solution


ok now this is from another thread, and i completely understand how she got everyting but the 81! could someone please explain to me how she got the 81.. thts the only part I am lost in..

We assume an object is at the L1 point (the point where the gravitational fields of the two objects cancels out). We will call this object X

r is the radius between the Earth and the Moon
We will call
r1
the point from the center of the Earth to x and
r2
the point from x to the center of the moon
Therefore
(1)
r=r1+r2Using this assumption of the object X we get..

Fg=Gm1xr21
where
m1
is the mass of the earth, and x is the mass of object X
Fg=Gm2xr22
where
m2
is the mass of the moon, and x is the mass of object X

Since we know that, at the point where the object X is situated, the gravitiational pull from both the Earth and the Moon will be equal, we can equate the above two equations getting the following:
(2)
Gm1xr21=Gm2xr22Now, we obtain a ratio between
m1
and
m2
so we can express
m1
in terms of
m2m1m2=81
(Note: I rounded to 81 just to make typing it up here easier...)
Therefore,
m1=81m2Now, going back to equation (2), G and x will cancel out and we replace
r1
with
r−r2
(from equation (1)) leaving us with:
81m2(r−r2)2=m2r22m2
will cancel out:
81(r−r2)2=1r2281=(r−r2)2r22i take the square root of both sides, and put the denominator on the left side
9r2=r−r210r2=rr2=r/10r2=3.84∗104Since
r1=r−r2r1=3.84∗105−3.84∗104r1=3.456∗105

Alicia,

your post is very hard to read. Use the x2 button for a square and x2 for an index.

So distance between the Earth and the object at point L1 is r1, the distance between the Moon and the object is r2, the force from the Earth is Gm1x/r12, the force from the Moon is Gm2x/r22, they are equal, so m1r22=m2r12. You can find the mas of Earth in any table about Earth. Google "mass of Earth" if you do not have it on your Physics book. It is 5.9736˙1024 kg. You see that the ratio of the masses of Earth and Moon is about 81. ehild
 
ehild said:
Alicia,

your post is very hard to read. Use the x2 button for a square and x2 for an index.

So distance between the Earth and the object at point L1 is r1, the distance between the Moon and the object is r2, the force from the Earth is Gm1x/r12, the force from the Moon is Gm2x/r22, they are equal, so m1r22=m2r12.


You can find the mas of Earth in any table about Earth. Google "mass of Earth" if you do not have it on your Physics book. It is 5.9736˙1024 kg. You see that the ratio of the masses of Earth and Moon is about 81.


ehild


Thank you very much and sorry for my horrible computer skills! I'll try that next time !
 

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