Calculate Speed & Time of Orbiting Satellite

  • Thread starter h_k331
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Janus has provided a summary of the conversation about determining the speed and time for a satellite in circular orbit above the Earth's surface. The satellite's speed was found to be 7580.897 m/s and the time required to complete one orbit was 5801.727 s. With the correct number of significant figures, the velocity would be 7.58e3 m/s and the time would be 5.80e3 s. Janus and hk have confirmed that the work is correct. In summary, the conversation was about determining the speed and time for a satellite in circular orbit 600 km above the Earth's surface, where the free-fall acceleration is 8.21 m/s^2, with the given radius
  • #1
h_k331
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I was hoping someone could check my work for me.

Question:
A satellite is in circular orbit 600 km above the Earth's surface, where the free-fall acceleration is 8.21 m/s^2. Take the radius of the Earth as 6400 km. Determine the speed of the satellite and the time required to complete one orbit around the earth.

Work:

Radius from to center of the Earth to the satellite is 600000 m + 6400000 m = 7000000 m.

For uniform circular motion a = v^2/r, so v = sqrt(ar).

v = sqrt(ar) = sqrt(8.21 m/s^2 * 7000000 m) = 7580.897 m/s

d = rt, so t = d/r.

t = d/r = (2pi * 7000000 m)/(7580.897 m/s) = 5801.727 s

So with the correct number of sig figs velocity would be 7.58e3 m/s and the time required to complete one orbit would be 5.80e3 s.

Thanks,
hk
 
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  • #2
Looks good.
 
  • #3
Thanks Janus.

hk
 

1. How do you calculate the speed of an orbiting satellite?

The speed of an orbiting satellite can be calculated using the formula v = √(GM/R), where v is the speed, G is the gravitational constant (6.67 x 10^-11 Nm^2/kg^2), M is the mass of the central body (in this case, the Earth), and R is the distance between the satellite and the center of the Earth.

2. What is the relationship between the speed and orbital radius of a satellite?

The speed of a satellite is directly proportional to its orbital radius. This means that the larger the orbital radius, the higher the speed of the satellite, and vice versa. This can be seen in the formula v = √(GM/R), where as R increases, v also increases.

3. How can you determine the time it takes for a satellite to complete one orbit?

The time it takes for a satellite to complete one orbit can be calculated using the formula T = 2π√(R^3/GM), where T is the orbital period, R is the orbital radius, and G and M have the same values as mentioned in the first question. This formula assumes that the satellite's orbit is circular.

4. Can the speed and time of orbiting satellites change?

Yes, the speed and time of orbiting satellites can change due to various factors such as atmospheric drag, gravitational pull from other celestial bodies, and adjustments made by ground controllers. In some cases, satellites may also intentionally change their speed and orbit to perform certain tasks or avoid collisions.

5. How do you take into account the Earth's rotation when calculating the speed and time of orbiting satellites?

When calculating the speed and time of orbiting satellites, the Earth's rotation is usually ignored as it does not have a significant impact on the calculations. However, in some cases, such as when dealing with geostationary satellites, the Earth's rotation may need to be taken into account to ensure accurate calculations.

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