The tug of war in astronomy is the ratio of planetary and solar attractions on a natural satellite. The term was coined by Isaac Asimov in The Magazine of Fantasy and Science Fiction in 1963.[1]
According to Isaac Newton's law of universal gravitation
F=G ⋅
m1 ⋅ m2 | |
d2 |
In this equation
F is the force of attraction
G is the gravitational constant
m1 and m2 are the masses of two bodies
d is the distance between the two bodies
The two main attraction forces on a satellite are the attraction of the Sun and the satellite's primary (the planet the satellite orbits). Therefore, the two forces are
Fp=
G ⋅ m ⋅ Mp | ||||||
|
Fs=
G ⋅ m ⋅ Ms | ||||||
|
The ratio of the two is
Fp | |
Fs |
=
| |||||||||||||
|
Callisto is a satellite of Jupiter. The parameters in the equation are [2]
Fp | |
Fs |
=
1.9 ⋅ 1027 ⋅ (778.3)2 | |
1.989 ⋅ 1030 ⋅ (1.883)2 |
≈ 163
The ratio 163 shows that the solar attraction is much weaker than the planetary attraction.
Asimov lists tug-of-war ratio for 32 satellites (then known in 1963) of the Solar System. The list below shows one example from each planet.
Primary | Satellite | Tug-of-war ratio | |
---|---|---|---|
Neptune | Triton | 8400 | |
Uranus | Titania | 1750 | |
Saturn | Titan | 380 | |
Jupiter | Ganymede | 490 | |
Mars | Phobos | 195 | |
Earth | Moon | 0.46 |
Unlike other satellites of the solar system, the solar attraction on the Moon is more than that of its primary. According to Asimov, the Moon is a planet moving around the Sun in careful step with the Earth.[1]