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  2. Orbit of the Moon - Wikipedia

    en.wikipedia.org/wiki/Orbit_of_the_Moon

    As the Earth rotates faster than the Moon travels around its orbit, this small angle produces a gravitational torque which slows the Earth and accelerates the Moon in its orbit. In the case of the ocean tides, the speed of tidal waves in the ocean [16] is far slower than the speed of the Moon's tidal forcing. As a result, the ocean is never in ...

  3. Moon - Wikipedia

    en.wikipedia.org/wiki/Moon

    The Moon is Earth's only natural satellite.It orbits at an average distance of 384,400 km (238,900 mi), about 30 times the diameter of Earth. Tidal forces between Earth and the Moon have synchronized the Moon's orbital period (lunar month) with its rotation period at 29.5 Earth days, causing the same side of the Moon to always face Earth.

  4. Lunar orbit - Wikipedia

    en.wikipedia.org/wiki/Lunar_orbit

    It passed within 6,000 kilometres (3,200 nmi; 3,700 mi) of the Moon's surface, but did not achieve lunar orbit. [11] Luna 3 , launched on October 4, 1959, was the first robotic spacecraft to complete a circumlunar free return trajectory , still not a lunar orbit, but a figure-8 trajectory which swung around the far side of the Moon and returned ...

  5. Orbital speed - Wikipedia

    en.wikipedia.org/wiki/Orbital_speed

    In gravitationally bound systems, the orbital speed of an astronomical body or object (e.g. planet, moon, artificial satellite, spacecraft, or star) is the speed at which it orbits around either the barycenter (the combined center of mass) or, if one body is much more massive than the other bodies of the system combined, its speed relative to the center of mass of the most massive body.

  6. Tidal acceleration - Wikipedia

    en.wikipedia.org/wiki/Tidal_acceleration

    It stays in orbit, and from Kepler's 3rd law it follows that its average angular velocity actually decreases, so the tidal action on the Moon actually causes an angular deceleration, i.e. a negative acceleration (−25.97±0.05"/century 2) of its rotation around Earth. [18] The actual speed of the Moon also decreases.

  7. Tidal locking - Wikipedia

    en.wikipedia.org/wiki/Tidal_locking

    Here, the ratio of the rotation period of a body to its own orbital period is some simple fraction different from 1:1. A well known case is the rotation of Mercury, which is locked to its own orbit around the Sun in a 3:2 resonance. [2] This results in the rotation speed roughly matching the orbital speed around perihelion. [14]

  8. Europa (moon) - Wikipedia

    en.wikipedia.org/wiki/Europa_(moon)

    Average orbital speed. 13 743.36 m/s [8] Inclination: ... The moon is the namesake of Europa, ... The Europa Clipper would not orbit Europa, ...

  9. Cassini's laws - Wikipedia

    en.wikipedia.org/wiki/Cassini's_laws

    Orbital inclination and rotation. When the Moon is 5.14° north of the ecliptic, its north pole is tilted 6.68° away from the Earth. The orientation of the plane containing the vectors normal to the orbits and the Moon's rotational axis rotates 360° with a period of about 18.6 years, whereas the Earth's axis precesses with a period of around 26,000 years, so the line-up of this illustration ...