Total Energy of a Geosynchronous Satellite

In summary, to calculate the total energy of a geosynchronous satellite with a mass of 1500kg orbiting Earth at a height of 325km, we use the formula ET=Ek+Ep where Ek=0.5mv^2 and Ep=mgh. The orbital velocity is not used in these calculations as it is used to keep the satellite stationary. Since we have not learned the formulas for calculating Ek and Ep in this lesson, we can use the simplified formula Et=mgh. However, it is possible to include the orbital energy in the calculation, which would result in the formula Et=(0.5mv^2)+(mgh).
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Homework Statement


Calculate the total energy of a geosynchronous satellite (one that orbits over a fixed spot) with a mass of 1500kg, orbiting Earth at a height of 325km with an orbital speed of 5000m/s

Homework Equations


ET=Ek+Ep
Ek=(0.5)(m)(v)^2
Ep=(m)(g)(h)

The Attempt at a Solution



Looking at the orbital velocity was confusing me, so I researched geosynchronous satellites. The orbital velocity is being used to keep it stationary, assuming the Earth is rotating at the same velocity. So it is not used in these calculations.

Now, in this lesson we have not learned the formulas of Ek= G(mp)(mo) /rp and
Ep= -G(mp)(mo)

Therefore, I bet the what the teacher wants is just Et=mgh . I would like to believe that it is not asking us to include the orbital energy.

But again Et is not a vectory quanitiy and orbital energy is possible.

Would the total energy in this case be

Et=(mo)(0.5)(5000m/s)^2 + (mo)(g)(h)
 
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  • #2
mgh applies near the Earth's surface where g is essentially constant. Way out where the satellite is, g ain't yer usual 'g' anymore! :wink:
 

What is the total energy of a satellite?

The total energy of a satellite is the sum of its kinetic energy and potential energy. It represents the amount of energy required to keep the satellite in orbit.

How is the total energy of a satellite calculated?

The total energy of a satellite can be calculated using the equation E = K + U, where E is the total energy, K is the kinetic energy, and U is the potential energy. Kinetic energy is calculated using the equation K = (1/2)mv^2, where m is the mass of the satellite and v is its velocity. Potential energy is calculated using the equation U = (-GmM)/r, where G is the gravitational constant, m and M are the masses of the satellite and the planet it is orbiting, and r is the distance between them.

What factors affect the total energy of a satellite?

The total energy of a satellite is affected by its mass, velocity, and the mass and distance of the planet it is orbiting. Additionally, the total energy can be altered by external forces such as atmospheric drag or gravitational perturbations from other objects.

Why is the total energy of a satellite important?

The total energy of a satellite is important because it determines its orbit and the amount of energy needed to maintain that orbit. If the total energy is too low, the satellite may crash into the planet. If it is too high, the satellite may escape the planet's gravitational pull and be lost in space.

Can the total energy of a satellite change?

Yes, the total energy of a satellite can change due to external forces or by altering its velocity through a maneuver. However, the total energy will remain constant if there are no external forces acting on the satellite.

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