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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. Earth's rotation - Wikipedia

    en.wikipedia.org/wiki/Earth's_rotation

    The South Pole is the other point where Earth's axis of rotation intersects its surface, in Antarctica. Earth rotates once in about 24 hours with respect to the Sun, but once every 23 hours, 56 minutes and 4 seconds with respect to other distant stars . Earth's rotation is slowing slightly with time; thus, a day was shorter in the past.

  4. Earth's orbit - Wikipedia

    en.wikipedia.org/wiki/Earth's_orbit

    The point towards which the Earth in its solar orbit is directed at any given instant is known as the "apex of the Earth's way". [ 4 ] [ 5 ] From a vantage point above the north pole of either the Sun or Earth, Earth would appear to revolve in a counterclockwise direction around the Sun.

  5. Tidal locking - Wikipedia

    en.wikipedia.org/wiki/Tidal_locking

    If the Moon were not rotating at all, it would alternately show its near and far sides to Earth, while moving around Earth in orbit, as shown in the right figure. The Moon is shown in polar view, and is not drawn to scale. A side view of the Pluto–Charon system. Pluto and Charon are tidally locked to each other.

  6. List of orbits - Wikipedia

    en.wikipedia.org/wiki/List_of_orbits

    Comparison of geostationary Earth orbit with GPS, GLONASS, Galileo and Compass (medium Earth orbit) satellite navigation system orbits with the International Space Station, Hubble Space Telescope and Iridium constellation orbits, and the nominal size of the Earth. [a] The Moon's orbit is around 9 times larger (in radius and length) than ...

  7. Moon - Wikipedia

    en.wikipedia.org/wiki/Moon

    The Moon makes a complete orbit around Earth with respect to the fixed stars, its sidereal period, about once every 27.3 days. [h] However, because the EarthMoon system moves at the same time in its orbit around the Sun, it takes slightly longer, 29.5 days, [i] [72] to return to the same lunar phase, completing a full cycle, as seen from Earth.

  8. Lunar precession - Wikipedia

    en.wikipedia.org/wiki/Lunar_precession

    Since the Moon's axial tilt is only 1.5° with respect to the ecliptic (the plane of Earth's orbit around the Sun), this effect is small. Once every 18.6 years, [ 1 ] the lunar north pole describes a small circle around a point in the constellation Draco , while correspondingly, the lunar south pole describes a small circle around a point in ...

  9. Lunar node - Wikipedia

    en.wikipedia.org/wiki/Lunar_node

    Around this time, the Moon's declination will vary from −28°36′ to +28°36′. Conversely, 9.3 years later, the angle between the Moon's orbit and Earth's equator reaches its minimum of 18°20′. This is called a minor lunar standstill. The last lunar standstill was a minor standstill in October 2015.