Tug of war (astronomy)
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]
Law of universal gravitation[]
According to Isaac Newton's law of universal gravitation
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
where the subscripts p and s represent the primary and the sun respectively, and m is the mass of the satellite.
The ratio of the two is
Example[]
Callisto is a satellite of Jupiter. The parameters in the equation are [2]
- Callisto–Jupiter distance (dp) is 1.883 · 106 km.
- Mass of Jupiter (Mp) is 1.9 · 1027 kg
- Jupiter–Sun distance (i.e. mean distance of Callisto from the Sun, ds) is 778.3 · 106 km.
- The solar mass (Ms) is 1.989 · 1030 kg
The ratio 163 shows that the solar attraction is much weaker than the planetary attraction.
The table of planets[]
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 |
The special case of the Moon[]
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]
References[]
- Moons
- Gravity
- Astronomical dynamical systems