Gravitational perturbations = tidal forces?

In summary, the book explains that gravitational perturbations on satellites due to celestial bodies are caused by the difference in forces between the body and the satellite. To calculate the perturbations caused by the Moon, the formula used is 2GM/r_m^3a_{sat}, where M is the mass of the Moon, r_m is the distance from the Moon to Earth, and a_{sat} is the distance from the center of the Earth to the satellite. This is different from using the formula GM/d^2, as the satellite's distance from the Moon is not the only factor in calculating the perturbations. Additionally, this formula is still valid for satellites beyond the Moon's orbital radius, as the Moon's gravity still
  • #1
Deadstar
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Hey folks I'm learning about graviational perturbations on satellites due to planets and, mainly for now, the Moon. In the book I'm reading on this, they say that gravitational perturbations due to celestial bodies are not casued by the full gravitational attraction of them but only by the corresponding tidal terms (i.e. by the difference between forces on the Earth and that on the satellite).

Can anyone elaborate on this? Say if we wanted to know the perturbations due to the Moon on a satellite, the book says to use the formula...
[tex]2 \frac{GM}{r_m^3}a_{sat}[/tex]
where M is mass on the Moon, [itex]r_m[/itex] the distance from the Moon to Earth and [itex]a_{sat}[/itex] the distance from the centre of the Earth to the satellite. I would have just gone and used
[tex]\frac{GM}{d^2}[/tex]
with d being the distance from Moon to satellite but why is this wrong?

The satellites they use this formula on are all 'close' to the Earth (i.e. with the Moons orbital radius). Would the formula they used still be valid for a satellite beyond the Moons orbital radius..?
 
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  • #2
The thing to remember is that that moon pulls on the Earth too. If the Earth and satellite were an equal distance from the the Moon, then their accleration towards the Moon would be equal and there would be no influence acting to pull them apart.

As it is, there is a small difference between the distances so the Earth and Satellite have different accelerations due ot he Moon's gravity and this tends to pull the satellite and Earth apart. Note that his happens even if the Satellite is further from the Moon than the Earth is, as when the satellite is on the opposite side of the Earth from the Moon.
 

1. What are gravitational perturbations and tidal forces?

Gravitational perturbations refer to the changes in the gravitational field of an object caused by the presence of another object or external force. Tidal forces, on the other hand, are the differential gravitational forces exerted on an object by another object due to their difference in distance from the source of gravity.

2. How do gravitational perturbations and tidal forces affect objects?

Gravitational perturbations and tidal forces can cause objects to experience changes in their orbits or rotation. They can also cause objects to deform or stretch due to the differential gravitational forces acting on them.

3. What causes gravitational perturbations and tidal forces?

Gravitational perturbations are caused by the presence of other objects or external forces that disrupt the gravitational field of an object. Tidal forces are mainly caused by the difference in the strength of the gravitational pull from a nearby massive object on different parts of an object.

4. How do scientists study and measure gravitational perturbations and tidal forces?

Scientists use mathematical models and simulations, as well as observational data, to study and measure gravitational perturbations and tidal forces. They also use instruments such as gravimeters and tidal gauges to directly measure the effects of these forces on objects.

5. Can gravitational perturbations and tidal forces have any practical applications?

Yes, gravitational perturbations and tidal forces have several practical applications in fields such as astronomy and geophysics. They can help scientists understand the dynamics of celestial bodies and the Earth's tides, and they also play a crucial role in the design of satellites and spacecraft for accurate navigation and orbit determination.

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