• Neptune

    From Luigi Fortunati@21:1/5 to All on Sat Nov 12 13:48:52 2022
    Neptune is about 30 astronomical units (au) from Earth.

    If I look at the planet Neptune from Earth, I am not looking at a
    stationary object.

    In my reference, Neptune makes a full 360-degree turn in 24 hours.

    I was curious to check at what speed Neptune is moving with respect to
    my terrestrial frame of reference from which I am observing it and I
    have discovered that, incredibly, Neptune (with respect to me) is
    moving faster than the speed of light and exactly at 327,000 km per
    second.

    Obviously I am wrong in my calculations which are these.

    The space traveled by Neptune is a circumference that has its center in
    the Earth and a radius of 30 au.

    Thus, the circumference traveled (in my reference) by Neptune in the 24
    hours is 2*pi*r*30=2*3.14*30=188.4 au long.

    In one hour Neptune travels 188.4/24=7.85 au.

    In one minute Neptune travels 7.85/60=0.13 au.

    In a second Neptune travels 0.13/60=0.00218 au.

    Since an au corresponds to approximately 150,000,000 km, Neptune
    travels 0.00218*150,000.00=327,000 km per second, with respect to me.

    Can you tell me where is the conceptual or calculation error?

    [[Mod. note -- I see no conceptual or calculation error here.

    As a quick sanity check, https://en.wikipedia.org/wiki/Neptune
    gives the radius of Neptune's orbit about the sun as 4.5e9 km,
    so the apparent speed in the rotating-with-the-Earth reference frame
    is 2*pi*4.5e9 km / (24*3600 s) = 330,000 km/s.

    So, relative to your rotating-with-the-Earth reference frame, Neptune
    is moving a bit faster than the speed of light.

    There's no contradiction with relativity here -- this is just a
    (non-inertial) *coordinate* speed; there's no *physical object* in
    whose inertial reference frame another *physical object* is moving
    faster than the speed of light.

    In fact, we can carry your argument much farther: instead of considering
    a reference frame attached to the Earth (rotating about once per 24 hours),
    [Actually, you probably want the siderial rotation period,
    once per 23 hours 56 minutes.]
    let's consider a reference frame attached to the rotor of an ultracentifuge (sitting in a lab on the Earth's surface) rotating at 60,000 rpm = 1000 Hz. Relative to that (rapidly-rotating) reference frame, an object (stationary
    on the Earth's surface) about 50 km away would be moving slightly faster
    than the speed of light.

    Nature doesn't know about coordinates (which are solely a human construct),
    so (as a famous relativist once said in a slightly different context) coordinates can change "at the speed of thought".
    -- jt]]

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  • From Luigi Fortunati@21:1/5 to All on Tue Nov 15 08:45:58 2022
    uigi Fortunati sabato 12/11/2022 alle ore 06:48:52 ha scritto:
    Neptune is about 30 astronomical units (au) from Earth.

    If I look at the planet Neptune from Earth, I am not looking at a stationary object.

    In my reference, Neptune makes a full 360-degree turn in 24 hours.

    I was curious to check at what speed Neptune is moving with respect to my terrestrial frame of reference from which I am observing it and I have discovered that, incredibly, Neptune (with respect to me) is moving faster than the speed of light and
    exactly at 327,000 km per second.

    Obviously I am wrong in my calculations which are these.

    The space traveled by Neptune is a circumference that has its center in the Earth and a radius of 30 au.

    Thus, the circumference traveled (in my reference) by Neptune in the 24 hours is 2*pi*r*30=2*3.14*30=188.4 au long.

    In one hour Neptune travels 188.4/24=7.85 au.

    In one minute Neptune travels 7.85/60=0.13 au.

    In a second Neptune travels 0.13/60=0.00218 au.

    Since an au corresponds to approximately 150,000,000 km, Neptune travels 0.00218*150,000.00=327,000 km per second, with respect to me.

    Can you tell me where is the conceptual or calculation error?

    [[Mod. note -- I see no conceptual or calculation error here.

    Okay.

    In my animation
    https://www.geogebra.org/m/sn4eav7h
    I have highlighted on the left the point of view of the reference of the
    fixed stars where Neptune is (almost) stationary and the Earth rotates
    on itself by 360° in 24 hours.

    And on the right, the point of view of the terrestrial reference where
    the Earth stands still and Neptune rotates 360° around the Earth in 24
    hours.

    Speed ​​is relative and, therefore, from our point of view, we are observing a body moving at relativistic speed (with respect to us) and
    it is a condition that affects all planets and all stars eternally
    moving at different speeds.

    Some speeds (indeed most of them) are not such that they can be
    considered negligible compared to the speed of light.

    So, my question is this: Why with our telescopes do we always (and only)
    see perfectly spherical celestial bodies and have we never seen one
    contracted in the direction of motion like the one at the top right of
    my animation?

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  • From Phillip Helbig (undress to reply@21:1/5 to fortunati.luigi@gmail.com on Tue Nov 15 12:17:21 2022
    In article <tkvd81$aqr$1@gioia.aioe.org>, Luigi Fortunati <fortunati.luigi@gmail.com> writes:

    So, my question is this: Why with our telescopes do we always (and only)
    see perfectly spherical celestial bodies and have we never seen one contracted in the direction of motion like the one at the top right of
    my animation?

    It is a misconception that spheres look contracted when moving at
    relativistic speeds:

    A. Lampa, _Z. f. Physik_, 27, 138, 1924.
    J. Terrell, _Phys. Rev._, 116, 1041, 1959.
    R. Penrose, _Proc. Camb. Phil. Soc._, 55, 137, 1959.

    I can turn around in a second but the relative motion of the Moon, much
    faster than the speed of light, doesn't correspond to the notion of
    relative motion normally discussed in SR.

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  • From Luigi Fortunati@21:1/5 to All on Wed Nov 16 17:28:17 2022
    Phillip Helbigundress to reply martedì 15/11/2022 alle ore 13:17:21 ha
    scritto:
    In article <tkvd81$aqr$1@gioia.aioe.org>, Luigi Fortunati <fortunati.luigi@gmail.com> writes:

    So, my question is this: Why with our telescopes do we always (and only)
    see perfectly spherical celestial bodies and have we never seen one
    contracted in the direction of motion like the one at the top right of
    my animation?

    It is a misconception that spheres look contracted when moving at relativistic speeds:

    A. Lampa, _Z. f. Physik_, 27, 138, 1924.
    J. Terrell, _Phys. Rev._, 116, 1041, 1959.
    R. Penrose, _Proc. Camb. Phil. Soc._, 55, 137, 1959.

    I can turn around in a second but the relative motion of the Moon, much faster than the speed of light, doesn't correspond to the notion of
    relative motion normally discussed in SR.

    In my animation
    https://www.geogebra.org/m/pxcxznqz
    I added a light clock on Neptune, where the photon (in the reference of
    the inhabitant of neptune) moves vertically (up and down) along the red
    line.

    Instead, for the terrestrial observer, the same photon follows a zigzag
    path.

    Thus, Neptune's space *must* be contracted (in the direction of motion)
    for the terrestrial observer.

    This is the correct notion of relative motion normally discussed in SR.

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  • From Jonathan Thornburg [remove -color t@21:1/5 to Phillip Helbig on Thu Nov 17 09:04:44 2022
    Phillip Helbig wrote:
    It is a misconception that spheres look contracted when moving at
    relativistic speeds:

    A. Lampa, _Z. f. Physik_, 27, 138, 1924.
    J. Terrell, _Phys. Rev._, 116, 1041, 1959.
    R. Penrose, _Proc. Camb. Phil. Soc._, 55, 137, 1959.

    I can turn around in a second but the relative motion of the Moon, much
    faster than the speed of light, doesn't correspond to the notion of
    relative motion normally discussed in SR.

    Luigi Fortunati <fortunati.luigi@gmail.com> wrote:
    [[question about an apparent paradox involving special relativity
    and a rotating reference frame]]

    I think the underlying cause of Luigi's apparent paradox may be that
    special relativity implicitly assues that the geometry of space is
    Euclidean... but the geometry of a rotating reference frame is non-Euclidean. (The non-Euclidean nature of rotating reference frames results in things
    like the Sagnac effect, the Ehrenfest paradox, etc.)

    There are interesting and relevant discussions in
    https://en.wikipedia.org/wiki/Sagnac_effect
    https://en.wikipedia.org/wiki/Ehrenfest_paradox
    https://en.wikipedia.org/wiki/Born_coordinates

    --
    -- "Jonathan Thornburg [remove -color to reply]" <dr.j.thornburg@gmail-pink.com>
    currently on the west coast of Canada
    "!07/11 PDP a ni deppart m'I !pleH" -- slashdot.org page footer, 2022-10-16
    "eHpl !'I mrtpaep dnia P PD1 /107" -- slightly more plausible message
    given PDP-11 little-endian byte order

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  • From Jonathan Thornburg [remove -color t@21:1/5 to All on Thu Nov 17 21:53:43 2022
    I wrote:
    Luigi Fortunati <fortunati.luigi@gmail.com> wrote:
    [[question about an apparent paradox involving special relativity
    and a rotating reference frame]]

    I think the underlying cause of Luigi's apparent paradox may be that
    special relativity implicitly assues that the geometry of space is Euclidean... but the geometry of a rotating reference frame is non-Euclidean. (The non-Euclidean nature of rotating reference frames results in things
    like the Sagnac effect, the Ehrenfest paradox, etc.)

    There are interesting and relevant discussions in
    https://en.wikipedia.org/wiki/Sagnac_effect
    https://en.wikipedia.org/wiki/Ehrenfest_paradox
    https://en.wikipedia.org/wiki/Born_coordinates

    Two other excellent discussions which directly address the complexities
    of rotating reference frames in relativity are physics FAQ entries:
    https://math.ucr.edu/home/baez/physics/Relativity/SR/rotatingCoordinates.html
    https://math.ucr.edu/home/baez/physics/Relativity/SR/rigid_disk.html

    ciao,
    --
    -- "Jonathan Thornburg [remove -color to reply]" <dr.j.thornburg@gmail-pink.com>
    currently on the west coast of Canada
    "!07/11 PDP a ni deppart m'I !pleH" -- slashdot.org page footer, 2022-10-16
    "eHpl !'I mrtpaep dnia P PD1 /107" -- slightly more plausible message
    given PDP-11 little-endian byte order

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  • From Richard Livingston@21:1/5 to All on Thu Nov 17 21:54:13 2022
    On Thursday, November 17, 2022 at 3:04:47 AM UTC-6, Jonathan Thornburg [remove -color to reply] wrote:
    Phillip Helbig wrote:
    It is a misconception that spheres look contracted when moving at
    relativistic speeds:

    A. Lampa, _Z. f. Physik_, 27, 138, 1924.
    J. Terrell, _Phys. Rev._, 116, 1041, 1959.
    R. Penrose, _Proc. Camb. Phil. Soc._, 55, 137, 1959.

    I can turn around in a second but the relative motion of the Moon, much
    faster than the speed of light, doesn't correspond to the notion of
    relative motion normally discussed in SR.
    Luigi Fortunati <fortuna...@gmail.com> wrote:
    [[question about an apparent paradox involving special relativity
    and a rotating reference frame]]

    I think the underlying cause of Luigi's apparent paradox may be that
    special relativity implicitly assues that the geometry of space is Euclidean... but the geometry of a rotating reference frame is non-Euclidean. (The non-Euclidean nature of rotating reference frames results in things
    like the Sagnac effect, the Ehrenfest paradox, etc.)

    There are interesting and relevant discussions in https://en.wikipedia.org/wiki/Sagnac_effect https://en.wikipedia.org/wiki/Ehrenfest_paradox https://en.wikipedia.org/wiki/Born_coordinates

    --
    -- "Jonathan Thornburg [remove -color to reply]" <dr.j.th...@gmail-pink.com> currently on the west coast of Canada
    "!07/11 PDP a ni deppart m'I !pleH" -- slashdot.org page footer, 2022-10-16 "eHpl !'I mrtpaep dnia P PD1 /107" -- slightly more plausible message
    given PDP-11 little-endian byte order

    The misunderstanding is that the rotating coordinate frame is not an
    inertial reference frame. SR only applies in inertial frames.
    Velocities in a rotating frame are not real and you can't use SR with
    these coordinates.

    Rich L.

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  • From Jonathan Thornburg [remove -color t@21:1/5 to All on Thu Nov 17 21:54:43 2022
    I wrote:

    Luigi Fortunati <fortunati.luigi@gmail.com> wrote:
    [[question about an apparent paradox involving special relativity
    and a rotating reference frame]]

    I think the underlying cause of Luigi's apparent paradox may be that
    special relativity implicitly assues that the geometry of space is Euclidean... but the geometry of a rotating reference frame is non-Euclidean.

    There are interesting and relevant discussions in
    [[references]]

    On further thought, I think the questions Luigi raised don't actually
    involve the rotating-coordinate issues discussed in those references.
    Instead, Luigi's questions are "just" about what we see if we observe
    something (Neptune) in a reference frame which is moving *faster*
    than the speed of light.

    As Phillip Helbig noted, it's easy to see observationally that the
    answer is "nothing special" -- if you spin your body around at an
    angular frequency of faster than about 1 revolution per 8 seconds,
    your body reference frame will have the Moon moving faster than the
    speed of light, and empirically the Moon looks pretty ordinary
    when you do this.

    --
    -- "Jonathan Thornburg [remove -color to reply]" <dr.j.thornburg@gmail-pink.com>
    currently on the west coast of Canada
    "!07/11 PDP a ni deppart m'I !pleH" -- slashdot.org page footer, 2022-10-16
    "eHpl !'I mrtpaep dnia P PD1 /107" -- slightly more plausible message
    given PDP-11 little-endian byte order

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  • From Tom Roberts@21:1/5 to Richard Livingston on Fri Nov 18 18:14:08 2022
    On 11/17/22 3:54 PM, Richard Livingston wrote:
    [...] the rotating coordinate frame is not an inertial reference
    frame.

    True.

    A minor point: in SR all possible frames are inertial, because "frame"
    implies the coordinate axes are mutually orthogonal, and that only
    happens for Minkowski coordinates at rest in an inertial frame. Rotating
    and otherwise-accelerated coordinates do not have mutually orthogonal coordinate axes.

    SR only applies in inertial frames.

    False. SR applies in any coordinates if the physical situation is within
    its domain of applicability. That domain is restricted to flat manifolds
    with the topology of R^4, which means that gravitation is absent (or at
    least negligible).

    Note, however, that standard presentations of SR give equations only in inertial coordinates (within its domain). To determine what equations
    apply in rotating or otherwise-accelerated coordinates, one starts with
    the usual equations in inertial coordinates and applies the appropriate coordinate transform to the desired coordinates.

    Velocities in a rotating frame are not real and you can't use SR
    with these coordinates.

    That is merely repeating the above mistake.

    Tom Roberts

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