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  2. Orbit of the Moon - Wikipedia

    en.wikipedia.org/wiki/Orbit_of_the_Moon

    There are no rearward loops in the Moon's solar orbit. Considering the EarthMoon system as a binary planet, its centre of gravity is within Earth, about 4,671 km (2,902 miles) [25] or 73.3% of the Earth's radius from the centre of the Earth. This centre of gravity remains on the line between the centres of the Earth and Moon as the Earth ...

  3. Tidal locking - Wikipedia

    en.wikipedia.org/wiki/Tidal_locking

    Earth's sidereal day would eventually have the same length as the Moon's orbital period, about 47 times the length of the Earth day at present. However, Earth is not expected to become tidally locked to the Moon before the Sun becomes a red giant and engulfs Earth and the Moon. [10] [11] For bodies of similar size the effect may be of ...

  4. 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.

  5. Lunar distance - Wikipedia

    en.wikipedia.org/wiki/Lunar_distance

    Variation of the distance between the centers of the Moon and the Earth over 700 days Distribution of perigee and apogee between 3000 BC and AD 3000. Because of the influence of the Sun and other perturbations, the Moon's orbit around the Earth is not a precise ellipse. Nevertheless, different methods have been used to define a semi-major axis.

  6. Why scientists say we need to send clocks to the moon - AOL

    www.aol.com/news/no-one-knows-time-moon...

    For 50 years, scientists have also been able to observe atomic clocks that are tucked aboard GPS satellites, which orbit Earth about 12,550 miles (20,200 kilometers) away — or about one ...

  7. Tidal acceleration - Wikipedia

    en.wikipedia.org/wiki/Tidal_acceleration

    The net tide raised on Earth by the Moon is dragged ahead of the Moon by Earth's much faster rotation. Tidal friction is required to drag and maintain the bulge ahead of the Moon, and it dissipates the excess energy of the exchange of rotational and orbital energy between Earth and the Moon as heat. If the friction and heat dissipation were not ...

  8. Why the moon shines so bright overhead in winter | The Sky Guy

    www.aol.com/why-moon-shines-bright-overhead...

    Curveball: the moon’s orbit around the Earth is tilted about 5 degrees so (83.5 + 5 = 88.5 degrees). Morning sky: Very bright Venus rises in the east around 5 a.m. in early January and around 6 ...

  9. Claimed moons of Earth - Wikipedia

    en.wikipedia.org/wiki/Claimed_moons_of_Earth

    This asteroid's orbit keeps it near the Earth, but not orbiting it in the usual sense. When analyzing its orbit from the perspective of different bodies, the presumed quasi-satellite does seem to have a more stable location near the Earth The orbit of 2020 CD 3 around the Earth. The white band is the orbit of the Moon.