Orbital velocity and radius for satellite

In summary, the problem asks for the distance and velocity at which a satellite should be placed in order to maintain a geostationary orbit to view the far side of the moon. The calculated distance of the center of gravity from the earth is 4,669,513.807 m. However, it is not possible for a satellite to be geostationary and view the far side of the moon simultaneously. A solution using the Earth-Moon L2 point may provide a simplified solution.
  • #1
joemmonster
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Homework Statement


A geostationary satellite is to be placed to view the far side of the moon. How far away should it be placed from the center of the Earth and what velocity should it travel in order to maintain its orbit? (Considering the moon and Earth as one entity and solve for the center of gravity, then determine the distance the satellite should be)

Mass of Earth: 5.97x10^24kg
Mass of moon: 7.349x10^22kg
Distance of moon to earth: 384,000,000 m
Center of gravity from earth: 4,669,513.807 m

Homework Equations


http://media.wiley.com/Lux/78/331278.image0.png
u6l4b5.gif

http://media.wiley.com/Lux/83/331283.image5.png

The Attempt at a Solution


I calculated the orbital radius and it seems that it's not going to be on the far side of the moon (42,399,473.46 m)
 
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  • #2
when you saying the far side of the moon you mean the so called "dark-side" of the moon? That is the side that we can't observe by no means with an observatory in the surface of the earth?

The center of the orbit of the sattelite will be the center of earth, the center of the moon, or the center of the system earth+moon?
 
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  • #3
Frankly it doesn't sound like this is possible. A satellite can stay stationary over a specific point on earth by orbiting with a specific velocity and distance from the earth, ignoring the influence of the moon. Similarly a satellite can stay stationary over a specific point on the moon with a specific velocity and distance ignoring the influence of the Earth (which would be a greater error) and a satellite can even orbit at a specific velocity and distance from the joint center of mass of the Earth and moon but such a satellite would NOT stay stationary over a point on the moon.
 
  • #4
yeah, the moon goes round the Earth once per month. So if we had a satellite that stayed exactly on the other side of the moon to us, the satellite would need to also go round the Earth once per month. And on the other hand, if we wanted the satellite to be geostationary, it would need to go round the Earth once per day (since the Earth takes one day to rotate). So it's not possible to have both.
 
  • #5
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  • #6
joemmonster said:

Homework Statement


A geostationary satellite is to be placed to view the far side of the moon. How far away should it be placed from the center of the Earth and what velocity should it travel in order to maintain its orbit? (Considering the moon and Earth as one entity and solve for the center of gravity, then determine the distance the satellite should be)

Mass of Earth: 5.97x10^24kg
Mass of moon: 7.349x10^22kg
Distance of moon to earth: 384,000,000 m
Center of gravity from earth: 4,669,513.807 m

Homework Equations


331278.image0.png

u6l4b5.gif

[PLAIN]http://media.wiley.com/Lux/83/331283.image5.png

The Attempt at a Solution


I calculated the orbital radius and it seems that it's not going to be on the far side of the moon (42,399,473.46 m)
It's not at all clear what you have done, except find the location of the c.o.m. of the earth-moon system.

Please provide all of your calculations.
 
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Related to Orbital velocity and radius for satellite

What is orbital velocity and how is it calculated?

Orbital velocity is the speed at which an object orbits around another object in space. It is calculated using the equation v = √(GM/r), where G is the gravitational constant, M is the mass of the central object, and r is the distance between the two objects.

How does the radius of a satellite's orbit affect its orbital velocity?

The radius of a satellite's orbit directly affects its orbital velocity. As the radius increases, the orbital velocity decreases and vice versa. This is because the force of gravity decreases as the distance between two objects increases, resulting in a slower orbital velocity.

What factors can influence the orbital velocity of a satellite?

The orbital velocity of a satellite can be influenced by several factors, including the mass of the central object, the distance between the two objects, and the altitude of the satellite's orbit. Other factors such as atmospheric drag, solar wind, and gravitational forces from other celestial bodies may also affect the orbital velocity.

Can a satellite have a circular orbit with a non-zero orbital velocity?

Yes, a satellite can have a circular orbit with a non-zero orbital velocity. This occurs when the velocity of the satellite is perpendicular to the radius vector, resulting in a constant distance between the satellite and the central object. This type of orbit is known as a circular or circular-equatorial orbit.

How does the mass of a satellite affect its orbital velocity?

The mass of a satellite does not affect its orbital velocity as long as it is significantly smaller than the mass of the central object. This is because the mass of the satellite is negligible compared to the mass of the central object in the equation for orbital velocity. However, a larger mass may require a higher velocity to maintain a stable orbit at a certain radius.

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