• Centripetal and centrifugal force

    From Luigi Fortunati@21:1/5 to All on Sun Jul 3 23:05:54 2022
    In my animation
    https://www.geogebra.org/m/uucnkfhy
    there is the chord OD which exerts a blue centripetal force on the
    rotating body A and there is an opposite red centrifugal force which is
    present only in the rotating reference (and not in the inertial one).

    Having specified this, is it correct to say that the point of
    application of the two opposing forces is point D?

    [[Mod. note -- No, not really.

    The *centrifugal* "force" acts on A's entire mass, so if we're going to
    model it as a force acting at a single point, it (the centrifugal "force")
    must have A's center of mass as its point of application.

    Where the *centripetal* force is applied depends on how A is teathered to
    the central point O. E.g. if A is attached to O by a string which connects
    to A at point D (the innermost point of A), then that point (D) is where
    the centripetal force would be applied. But if (e.g.) the string goes
    into a hole drilled into the body A and the string is actually only attached
    to A at the center of the body A, then the centripetal force would be applied to A there (the center of the body A). And if the centripetal force is supplied by the Newtonian gravity field of a spherical mass located at O,
    then the point of application is approximately the center of A.
    -- jt]]

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  • From Julio Di Egidio@21:1/5 to Luigi Fortunati on Wed Jul 6 23:10:14 2022
    On Monday, 4 July 2022 at 08:05:58 UTC+2, Luigi Fortunati wrote:
    In my animation
    https://www.geogebra.org/m/uucnkfhy
    there is the chord OD which exerts a blue centripetal force on the
    rotating body A and there is an opposite red centrifugal force which is present only in the rotating reference (and not in the inertial one).

    Having specified this, is it correct to say that the point of
    application of the two opposing forces is point D?

    [[Mod. note -- No, not really.

    The *centrifugal* "force" acts on A's entire mass, so if we're going to
    model it as a force acting at a single point, it (the centrifugal "force") must have A's center of mass as its point of application.

    Where the *centripetal* force is applied depends on how A is teathered to
    the central point O. E.g. if A is attached to O by a string which connects
    to A at point D (the innermost point of A), then that point (D) is where
    the centripetal force would be applied. But if (e.g.) the string goes
    into a hole drilled into the body A and the string is actually only attached to A at the center of the body A, then the centripetal force would be applied to A there (the center of the body A). And if the centripetal force is supplied by the Newtonian gravity field of a spherical mass located at O, then the point of application is approximately the center of A.
    -- jt]]

    Eventually, if there is no wobbling, the resultant centripetal force
    must be simply attached to the center of mass: in fact, always
    equal and opposite to the centrifugal one. (No?)

    Then I'd have a question: to the centripetal force, in accordance
    with Newton's third law, corresponds an equal and contrary force
    that the string exerts on the central pivot. But how does the
    centrifugal force satisfy that same law, if it does? (I understand
    the two forces really exist in the two distinct frames, but all the
    more so the question remains).

    Thanks in advance for any insights,

    Julio

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  • From J. J. Lodder@21:1/5 to Luigi Fortunati on Wed Jul 6 23:18:20 2022
    Luigi Fortunati <fortunati.luigi@gmail.com> wrote:

    In my animation
    https://www.geogebra.org/m/uucnkfhy
    there is the chord OD which exerts a blue centripetal force on the
    rotating body A and there is an opposite red centrifugal force which is present only in the rotating reference (and not in the inertial one).

    Having specified this, is it correct to say that the point of
    application of the two opposing forces is point D?

    [[Mod. note -- No, not really.

    The *centrifugal* "force" acts on A's entire mass, so if we're going to
    model it as a force acting at a single point, it (the centrifugal "force") must have A's center of mass as its point of application.

    Actually calculating it for an extended body can be simplified
    by noting that the centrifugal force can be derived from a potential.
    (equal to - 1/2 \Omega^2 r^2,
    with r the distance from the axis of rotation)

    Where the *centripetal* force is applied depends on how A is teathered to
    the central point O. E.g. if A is attached to O by a string which connects to A at point D (the innermost point of A), then that point (D) is where
    the centripetal force would be applied. But if (e.g.) the string goes
    into a hole drilled into the body A and the string is actually only attached to A at the center of the body A, then the centripetal force would be applied to A there (the center of the body A). And if the centripetal force is supplied by the Newtonian gravity field of a spherical mass located at O, then the point of application is approximately the center of A.

    For the Earth/Moon system it isn't.
    The simplest way to derive the tides (Earth/Moon only)
    is to calculate the combined potential in co-rotating coordinates.
    (gravity from Earth and Moon, and centrifugal potential
    from the rotation around their common centre of mass)

    It is the shortest way to seeing that there must be two tidal bulges,

    Jan

    [[Mod. note -- You're right. I was thinking of the case where the
    central mass O is fixed in position in an inertial reference frame.
    That's a bit unrealistic... :)
    -- jt]]

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  • From Luigi Fortunati@21:1/5 to All on Wed Jul 6 23:16:24 2022
    Luigi Fortunati alle ore 18:05:54 del giorno domenica ha scritto:
    In my animation
    https://www.geogebra.org/m/uucnkfhy
    there is the chord OD which exerts a blue centripetal force on the
    rotating body A and there is an opposite red centrifugal force which is present only in the rotating reference (and not in the inertial one).

    Having specified this, is it correct to say that the point of
    application of the two opposing forces is point D?

    [[Mod. note -- No, not really.

    Where the *centripetal* force is applied depends on how A is teathered to
    the central point O. E.g. if A is attached to O by a string which connects to A at point D (the innermost point of A), then that point (D) is where
    the centripetal force would be applied.
    -- jt]]

    This is the case of my animation and, therefore, the point of
    application of the centripetal force (of the string on body A) is,
    without a doubt, point D.

    But at point D, in addition to the centripetal action of the string on
    body A, there must also be an opposite (and, therefore, centrifugal)
    reaction force of body A on the string (third principle).

    I would like to know if there is any other point (of the string or of
    the body A) where the third principle is not valid, that is where the
    action of the centripetal force is not opposed by any type of opposite
    reaction (ie directed in the centrifugal direction).

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  • From Luigi Fortunati@21:1/5 to All on Fri Jul 8 08:22:20 2022
    J. J. Lodder alle ore 18:18:20 del giorno mercoled=EC ha scritto:
    The simplest way to derive the tides (Earth/Moon only)
    is to calculate the combined potential in co-rotating coordinates.
    (gravity from Earth and Moon, and centrifugal potential
    from the rotation around their common centre of mass)

    It is the shortest way to seeing that there must be two tidal bulges,

    Why does centrifugal force that "appear" ONLY in accelerated references=20 generate bulges that ALSO appear in inertial references?

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  • From J. J. Lodder@21:1/5 to Luigi Fortunati on Thu Jul 14 12:12:14 2022
    Luigi Fortunati <fortunati.luigi@gmail.com> wrote:

    J. J. Lodder alle ore 18:18:20 del giorno mercoledì ha scritto:
    The simplest way to derive the tides (Earth/Moon only)
    is to calculate the combined potential in co-rotating coordinates.
    (gravity from Earth and Moon, and centrifugal potential
    from the rotation around their common centre of mass)

    It is the shortest way to seeing that there must be two tidal bulges,

    Why does centrifugal force that "appear" ONLY in accelerated references generate bulges that ALSO appear in inertial references?

    It is a physical effect,
    so it cannot depend on any particular reference frame.
    It is just that the derivation is simpler in one frame than in another.

    In non-rotating coordinates you have a dynamic problem
    rather than a static one, so you have to derive the motions.

    The bulge then comes about because the solid bulk of the Earth
    falls faster towards the Moon than the water on the far side,

    Jan

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