Geosynchronous Orbit and Radius Calculation for Satellite | 8 Earth Radii

  • Thread starter Thread starter UrbanXrisis
  • Start date Start date
  • Tags Tags
    Orbit
Click For Summary
SUMMARY

A satellite in geosynchronous orbit has an average radius of approximately 42,164 km, or 8 Earth radii, measured from the Earth's center. The calculation for the radius involves understanding gravitational forces and centripetal motion, specifically using Kepler's Third Law. The orbital period for a geosynchronous satellite matches the Earth's rotation period of 86,164 seconds. Additionally, the time taken for a radio signal to travel between a transmitter and receiver near the North Pole can be calculated using the formula d/v=t, where d is the distance and v is the speed of light.

PREREQUISITES
  • Understanding of gravitational forces and centripetal motion
  • Familiarity with Kepler's Laws, particularly Kepler's Third Law
  • Basic knowledge of orbital mechanics
  • Ability to perform calculations involving speed, distance, and time
NEXT STEPS
  • Study the derivation of Kepler's Third Law for satellite motion
  • Learn about gravitational force equations and their applications in orbital mechanics
  • Explore the concept of signal propagation time in telecommunications
  • Investigate the relationship between orbital radius and satellite velocity
USEFUL FOR

Aerospace engineers, astrophysicists, telecommunications professionals, and students studying orbital mechanics will benefit from this discussion.

UrbanXrisis
Messages
1,192
Reaction score
1
A satellite in geosynchronous orbit remains above the Earth's equator as the planet rotates on its axis.

a) calculate the radius of its orbit.

does this mean from the center of the earth?
I looked online and the distance is about 7 Earth radii, which would make the radius of the orbit 8 Earth radii. Earth's radius is 6.37x10^6m.. makeing the radius 5.096x10^7m.

what does it mean by calculate the orbit?

b) the satellite relays a radio signal from a transmitter near the noth pole to a receiver, also near the north pole. Traveling at the speed of light, how long is the radio wave in trasit?

d/v=t
d=\frac{\sqrt{r_{earth}^2+r_{satellite}^2}}{c}
 
Physics news on Phys.org
UrbanXrisis said:
A satellite in geosynchronous orbit remains above the Earth's equator as the planet rotates on its axis.

a) calculate the radius of its orbit.

does this mean from the center of the earth?
I looked online and the distance is about 7 Earth radii, which would make the radius of the orbit 8 Earth radii. Earth's radius is 6.37x10^6m.. makeing the radius 5.096x10^7m.

what does it mean by calculate the orbit?

b) the satellite relays a radio signal from a transmitter near the noth pole to a receiver, also near the north pole. Traveling at the speed of light, how long is the radio wave in trasit?



d/v=t
d=\frac{\sqrt{r_{earth}^2+r_{satellite}^2}}{c}
a) For use in formulas relating to gravitational forces and geosynchronous orbits, the orbit radius is that measured from the Earth's CENTER.
Hint: At what orbit radius will the gravitational force between Earth and satellite provide the exact centripetal force required for the satellite's rotational velocity "ω" (in radians/sec) to equal Earth's rotational "ω" (in radians/sec)??

b) Remember that the radio signal path is 2-way ("uplink" and "downlink").


~~
 
Last edited:
UrbanXrisis said:
A satellite in geosynchronous orbit remains above the Earth's equator as the planet rotates on its axis.

a) calculate the radius of its orbit.

does this mean from the center of the earth?
I looked online and the distance is about 7 Earth radii, which would make the radius of the orbit 8 Earth radii. Earth's radius is 6.37x10^6m.. makeing the radius 5.096x10^7m.

what does it mean by calculate the orbit?

b) the satellite relays a radio signal from a transmitter near the noth pole to a receiver, also near the north pole. Traveling at the speed of light, how long is the radio wave in trasit?

d/v=t
d=\frac{\sqrt{r_{earth}^2+r_{satellite}^2}}{c}
You may have misunderstood what they meant by the 'distance' for a geosynchronous satellite. A geosynchronous satellite has an average radius of 42,164 km, or approximately 7 times the Earth's radius. In other words, they didn't mean for you to add that distance to the Earth's radius.

For your problem, multiplying the Earth's radius by 7 gets you an approximate answer, provided that's the way they want you to calculate the radius.

However, I'm not sure that's the way they wanted you to calculate the radius. Since you have thread about Kepler's Second Law, does that mean you learned Kepler's Third Law, as well? If so, in order for a satellite to stay over the same spot on the Earth, it must complete one orbit in the same amount of time the Earth completes one complete rotation (86164 seconds). The orbital period is known, so you can rearrange the equation for orbital period to solve for the radius, instead, and will come much closer to an accurate answer than the rough approximation you found online.
 
thx with the help...
\frac{GM}{r^2}=\frac{4r \pi^2}{T^2}

that's the equation I was trying to figure out
 

Similar threads

Replies
1
Views
2K
  • · Replies 11 ·
Replies
11
Views
2K
Replies
6
Views
3K
Replies
2
Views
2K
Replies
5
Views
3K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 15 ·
Replies
15
Views
4K
Replies
3
Views
5K
  • · Replies 18 ·
Replies
18
Views
3K
  • · Replies 12 ·
Replies
12
Views
12K