Given these values, determine the mass of the Earth

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In summary: If so, then you can use this velocity to calculate the gravitational force and ultimately the mass of the Earth. In summary, to determine the mass of the Earth from the given information, you can use the formula F = mv^2/r and the fact that the moon's motion about the Earth is circular to calculate the velocity of the moon. Then, using this velocity and the formula F = G(Mm)/r^2, you can solve for the mass of the Earth.
  • #1
osakabosaka
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Homework Statement
The moon orbits the Earth at a distance of 3.84 x 10^8 m from the centre of Earth. The moon has a period of about 27.3 days. From these values, determine the mass of the Earth
Relevant Equations
F = G(Mm)/r^2
F = mv^2/r
Honestly at a loss. Don't know where to start, what formulas to use. Any help would be greatly appreciated!
 
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  • #2
osakabosaka said:
Homework Statement:: The moon orbits the Earth at a distance of 3.84 x 10^8 m from the centre of Earth. The moon has a period of about 27.3 days. From these values, determine the mass of the Earth
Relevant Equations:: F = G(Mm)/r^2
F = mv^2/r

Honestly at a loss. Don't know where to start, what formulas to use. Any help would be greatly appreciated!

What type of motion is the moon undergoing about the Earth? Does that help you to write down an ##F=ma## relation of some sort?

It might help to know that for two spherically symmetric masses, ##r## in Newton's law of gravitation is taken to be the distance between the centres.
 
  • #3
Gravitational force?
So is starting out with something like Fg=Fc alright?
 
  • #4
osakabosaka said:
Gravitational force?

##\vec{F_{g}}## is definitely the centripetal force.

osakabosaka said:
So is starting out with something like Fg=Fc alright?

Give it a shot and see what you get!
 
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  • #5
Fc = Fg
(mv^2)/r = (Gm1m2)/r^2

not sure what to do with velocity or if this is a dead end
 
  • #6
osakabosaka said:
Fc = Fg
(mv^2)/r = (Gm1m2)/r^2

not sure what to do with velocity or if this is a dead end

Well, the centripetal acceleration can be expressed in a few different ways. Most helpful in this context is ##a = r\omega^{2}##. That is, ##a = \frac{v^2}{r} = \frac{(r\omega)^{2}}{r} = r\omega^{2}##.
 
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  • #7
osakabosaka said:
Fc = Fg
(mv^2)/r = (Gm1m2)/r^2

not sure what to do with velocity or if this is a dead end
The question to ask yourself is: given the radius and period of circular motion, can you work out how fast the object is travelling?
 

Related to Given these values, determine the mass of the Earth

1. What are the values needed to determine the mass of the Earth?

The values needed to determine the mass of the Earth are the gravitational constant (G), the distance between the Earth and an object (r), and the object's orbital period (T).

2. How do you calculate the mass of the Earth using these values?

The mass of the Earth can be calculated using the formula M = (4π²r³)/GT², where M is the mass of the Earth, G is the gravitational constant, r is the distance between the Earth and an object, and T is the object's orbital period.

3. What is the gravitational constant and why is it important in determining the mass of the Earth?

The gravitational constant (G) is a fundamental constant in physics that represents the strength of the gravitational force between two objects. It is important in determining the mass of the Earth because it is used in the formula to calculate the mass of the Earth.

4. How accurate is the calculated mass of the Earth using this method?

The calculated mass of the Earth using this method is very accurate, with a margin of error of less than 0.1%. This is because the formula takes into account the effects of gravity and the object's orbital period, making it a reliable method for determining the mass of the Earth.

5. Can this method be used to determine the mass of other planets?

Yes, this method can be used to determine the mass of any planet as long as the values for the gravitational constant, distance, and orbital period are known. This formula is a universal law of gravitation and can be applied to any two objects in orbit around each other.

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