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Tug of war (astronomy)

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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.

Contents

Law of universal gravitation

According to Isaac Newton's law of universal gravitation

F = G m 1 m 2 d 2

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

F p = G m M p d p 2 F s = G m M s d s 2

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

F p F s = M p d s 2 M s d p 2

Example

Callisto is a satellite of Jupiter. The parameters in the equation are

  • 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
  • F p F s = 1.9 10 27 ( 778.3 ) 2 1.989 10 30 ( 1.883 ) 2 163

    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.

    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.

    References

    Tug of war (astronomy) Wikipedia