The synchronous orbit is the orbit that allows a satellite to make a revolution around the planet while the planet makes one tour around itself. This means that if the orbit has an inclination and eccentricity equal to 0, then the satellite will appear from the ground of the planet, "immobile", still hanging in the sky at the same position above the equator. When the inclination of the plane of the satellite orbit is equatorial (inclination ≠ 0), the satellite appears to oscillate from north to south, above the equator of the planet. When the satellite's orbit is elliptical (eccentricity ≠ 0), the satellite appears to oscillate from East to West. When the inclination of the satellite orbit and the eccentricity are both different from 0, then the satellite moves across the sky producing a figure 8-shaped, called analemma. It does not exist in the solar system natural satellite, in synchronous orbit planet. On Earth, almost circular orbits are used by synchronous artificial communication satellites, these are the famous geostationary orbits. A satellite in a synchronous orbit is always in synchronous rotation (see note) because the satellite is blocked by tidal forces.
The geostationary orbit is a geosynchronous orbit, which has an inclination and a zero eccentricity. Above the geostationary orbit at 35,796 km altitude above the equator is a belt 230 km called "graveyard orbit" or "orbit trash" is the cemetery of satellites end of life.
Nota: be careful not to confuse the synchronous orbit of a satellite with a satellite synchronous rotation. The synchronous orbit is the orbit that allows a satellite to take a tour around the planet while the planet makes one revolution around itself. In the rotation synchronous satellite puts the same time to rotate about its axis for rotation about the planet. In the case of synchronous orbit, the satellite is always in the same place in the sky and in the case of synchronous rotation, the satellite always presents the same face to the planet. This is the case of the moon having a rotational period equal to the period of revolution (27.3217 days), it always presents the same face in the Earth but it moves in the air since it is not located on a synchronous orbit.
Video: observation satellites are typically positioned in synchronous orbit at 35,796 km altitude. These images are taken by geostationary EUMETSAT, NOAA satellites and AGC showing weather conditions in the world in 2013.
Where is the synchronous orbits of the planets?
How to calculate the synchronous orbits of the planets?
The synchronous orbit planets is calculated using the law of universal gravitation which boils down to: h=√3(G*M*T2/4π2)-R
h = Height of the artificial satellite G = Constant of gravitation (6.67*10-11) M = Mass of the planet T = Rotational period of the planet R = Radius of the planet The geosynchronous orbit (synchronous orbit of the Earth) is at an altitude of 35,796 km (≈ 36,000 km) and has a semi-major axis of 42,167 km. Excel formula used in this table to calculate the altitude of the satellite in synchronous orbit of the planet: =((((G*M*T^2)/(4*PI()^2))^(1/3))-R*1000)/1000 Excel formula used to calculate the semi-major axis of the synchronous orbit of the planet: =((((G*M*T^2)/(4*PI()^2))^(1/3)))/1000
Planets
Mass (1024 kg)
Volume (1012 km3)
Radius (km)
Rotation period (s)
Synchronous orbit altitude (km)
Synchronous orbit Semi-major axis (km)
Satellite speed (km/s)
Mercury
0.3302
0.06083
2439.74
5 053 137
240 025
242 464
0.30
Venus
4.8685
0.92843
6051.83
20 939 611
1 527 832
1 533 883
0.46
Earth
5.9736
1.08321
6371.01
86 163
35 796
42 167
3.07
Mars
0.64185
0.16318
3389.95
88 400
17 002
20 392
1.45
Jupiter
1898.6
1431.28
69910.97
35 629
89 811
159 722
28.17
Saturn
568.46
827.13
58232.00
38 256
53 811
112 043
18.40
Uranus
86.81
68.33
25361.46
61 894
57 173
82 534
8.38
Neptune
102.43
62.526
24622.04
57 837
58 739
83 361
9.06
Europa
0.048
0.01593
1560.90
306 822
18 134
19 694
0.40
Table: synchronous orbits of the planets and moons of planets.
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