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  2. Centrifugal force - Wikipedia

    en.wikipedia.org/wiki/Centrifugal_force

    The operations of numerous common rotating mechanical systems are most easily conceptualized in terms of centrifugal force. For example: A centrifugal governor regulates the speed of an engine by using spinning masses that move radially, adjusting the throttle, as the engine changes speed. In the reference frame of the spinning masses ...

  3. Polflucht - Wikipedia

    en.wikipedia.org/wiki/Polflucht

    Polflucht (from German, flight from the poles) is a geophysical concept invoked in 1922 by Alfred Wegener to explain his ideas of continental drift.. The pole-flight force is that component of the centrifugal force during the rotation of the Earth that acts tangentially to the Earth's surface.

  4. Rossby number - Wikipedia

    en.wikipedia.org/wiki/Rossby_number

    A small Rossby number signifies a system strongly affected by Coriolis forces, and a large Rossby number signifies a system in which inertial and centrifugal forces dominate. For example, in tornadoes, the Rossby number is large (≈ 10 3), in low-pressure systems it is low (≈ 0.1–1), and in oceanic systems it is of the order of unity, but ...

  5. Equatorial bulge - Wikipedia

    en.wikipedia.org/wiki/Equatorial_bulge

    The forces at play in the case of a planet with an equatorial bulge due to rotation. Red arrow: gravity Green arrow: the normal force Blue arrow: the resultant force The resultant force provides required centripetal force. Without this centripetal force frictionless objects would slide towards the equator.

  6. Tidal range - Wikipedia

    en.wikipedia.org/wiki/Tidal_range

    Tidal range is the difference in height between high tide and low tide. Tides are the rise and fall of sea levels caused by gravitational forces exerted by the Moon and Sun, by Earth's rotation and by centrifugal force caused by Earth's progression around the Earth-Moon barycenter.

  7. Clairaut's theorem (gravity) - Wikipedia

    en.wikipedia.org/wiki/Clairaut's_theorem_(gravity)

    The spheroidal shape of the Earth is the result of the interplay between gravity and centrifugal force caused by the Earth's rotation about its axis. [18] [19] In his Principia, Newton proposed the equilibrium shape of a homogeneous rotating Earth was a rotational ellipsoid with a flattening f given by 1/230.

  8. History of centrifugal and centripetal forces - Wikipedia

    en.wikipedia.org/wiki/History_of_centrifugal_and...

    Since the centrifugal force of the parts of the earth, arising from the earth's diurnal motion, which is to the force of gravity as 1 to 289, raises the waters under the equator to a height exceeding that under the poles by 85472 Paris feet, as above, in Prop. XIX., the force of the sun, which we have now shewed to be to the force of gravity as ...

  9. Sedimentation - Wikipedia

    en.wikipedia.org/wiki/Sedimentation

    Settling pond for iron particles at water works. Settling is the process by which particulates move towards the bottom of a liquid and form a sediment.Particles that experience a force, either due to gravity or due to centrifugal motion will tend to move in a uniform manner in the direction exerted by that force.