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  2. Earth's orbit - Wikipedia

    en.wikipedia.org/wiki/Earth's_orbit

    [nb 1] Earth's orbital speed averages 29.78 km/s (19 mi/s; 107,208 km/h; 66,616 mph), which is fast enough to cover the planet's diameter in 7 minutes and the distance to the Moon in 4 hours. [3] 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".

  3. Earth's rotation - Wikipedia

    en.wikipedia.org/wiki/Earth's_rotation

    The tangential speed of Earth's rotation at a point on Earth can be approximated by multiplying the speed at the equator by the cosine of the latitude. [42] For example, the Kennedy Space Center is located at latitude 28.59° N, which yields a speed of: cos(28.59°) × 1,674.4 km/h = 1,470.2 km/h.

  4. Motion - Wikipedia

    en.wikipedia.org/wiki/Motion

    Motion is mathematically described in terms of displacement, distance, ... The Milky Way Galaxy is moving through space and many ... Light moves at a speed of ...

  5. Aberration (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Aberration_(astronomy)

    In the Earth's frame, the Sun moves, at a mean velocity v = 29.789 km/s, by a distance = ≈ 14,864.7 km in the time it takes light to reach Earth, = / ≈ 499 sec for the orbit of mean radius = 1 AU = 149,597,870.7 km.

  6. We Know How Fast Earth Spins ... Don’t We? - AOL

    www.aol.com/know-fast-earth-spins-don-175700545.html

    Earth rotates on its axis at about 1,000 miles per hour. That’s the short answer, but it’s not the whole story.

  7. Axial precession - Wikipedia

    en.wikipedia.org/wiki/Axial_precession

    In addition to the Moon and Sun, the other planets also cause a small movement of Earth's axis in inertial space, making the contrast in the terms lunisolar versus planetary misleading, so in 2006 the International Astronomical Union recommended that the dominant component be renamed the precession of the equator, and the minor component be ...

  8. Light-time correction - Wikipedia

    en.wikipedia.org/wiki/Light-time_correction

    An approximate light-time is calculated by dividing the object's geometric distance from Earth by the speed of light. Then the object's velocity is multiplied by this approximate light-time to determine its approximate displacement through space during that time. Its previous position is used to calculate a more precise light-time.

  9. Polar motion - Wikipedia

    en.wikipedia.org/wiki/Polar_motion

    Polar motion of the Earth is the motion of the Earth's rotational axis relative to its crust. [2]: 1 This is measured with respect to a reference frame in which the solid Earth is fixed (a so-called Earth-centered, Earth-fixed or ECEF reference frame). This variation is a few meters on the surface of the Earth.