From: Sam Wormley on
On 7/16/10 2:48 PM, JT wrote:
> On 16 Juli, 20:49, JT<jonas.thornv...(a)hotmail.com> wrote:
>> On 16 Juli, 20:40, Sam Wormley<sworml...(a)gmail.com> wrote:
>>
>>
>>
>>
>>
>>> On 7/16/10 12:53 PM, JT wrote:
>>
>>>> Well i can see an idiot ***trying*** to answer our rotation relative
>>>> the sun as RPM, but the idiot said he could give us the absolute
>>>> rotation of earth in RPM.
>>
>>>> But however i am still curious how you draw the conclusion.
>>
>>>> 360 / (24 * 60) = 0.25 degrees /min
>>
>>>> http://www.wolframalpha.com/input/?i=0.25+degrees+/min+to+RPM
>>
>>>> 6.94x10^-4 rpm (revolutions per minute)
>>
>>>> JT
>>
>>> The Earth's angular velocity = 0.72921158553 X 10**-4 Rad/s
>>> which comes out to be 86164.0905 seconds for a 2π (360°) rotation
>>> and 239.344696 seconds for every 1° or rotation.
>>
>> Is that angular velocity versus what sun fixed stars........ or what?
>> Is it also the absolute rotation?
>>
>> JT
>
> Sam?

> GRAVITATION AND INERTIA
> by Ignazio Ciufolini and John Archibald Wheeler
> Princeton University Press, Princeton, NJ 1995
> QC173.59.G44C58 1995 530.1'1--dc20 94-29874 CIP
> ISBN 0-691-03323-4
>
>
> In the first chapter Ciufolini and Wheeler introduce concepts and ideas
> of Einstein's General Theory of Relativity which are developed in the
> book. Part of the introductory material is reproduced here.
>
> "Gravity is not a foreign and physical force transmitted through space
> and time. It is a manifestation of the curvature of spacetime." That,
> in a nutshell, is Einstein's theory.
>
> What this theory is and what it means, we grasp more fully by looking
> at its intellectual antecedents. First, there was the idea of Riemann
> that space, telling mass how to move, must itself--by the principle of
> action and reaction--be affected by mass. It cannot be an ideal
> Euclidean perfection, standing in high mightiness above the battles of
> matter and energy. Space geometry must be a participant in the world of
> physics. Second, there was the contention of Ernst Mach that the
> "acceleration relative to absolute space" of Newton is only properly
> understood when it is viewed as acceleration relative to the sole
> significant mass there really is, the distant stars. According to this
> "Mach principle," inertia here arises from mass there. Third was that
> great insight of Einstein that we summarize in the phrase "free fall is
> free float": the equivalence principle, one of the best-tested
> principles in physics, from the inclined tables of Galilei and the
> pendulum experiments of Galilei, Huygens, and Newton to the highly
> accurate torsion balance measurements of the twentieth century, and the
> Lunar Laser Ranging experiment. With those three clues vibrating in his
> head, the magic of the mind opened to Einstein what remains one of
> mankind's most precious insights: gravity in manifestation of spacetime
> curvature.
>
> Euclid's (active around 300 B.C.) fifth postulate states that, given
> any straight line and any point not on it, we can draw through that
> point one and only one straight line parallel to the given line, that
> is, a line that will never meet the given one (this alternative
> formulation of the fifth postulate is essentially due to Proclos). This
> is the parallel postulate. In the early 1800s the discussion grew
> lively about whether the properties of parallel lines as presupposed in
> Euclidean geometry could be derived from the other postulate and
> axioms, or whether the parallel postulate had to be assumed
> independently. More than two thousand years after Euclid, Karl
> Friedrich Gauss, Jnos Bolyai, and Nikolai Ivanovich Lobacevskij
> discovered pencil-and paper geometric systems that satisfy all the
> axioms and postulates of Euclidean geometry except the parallel
> postulate. These geometries showed not only the parallel postulate must
> be assumed in order to obtain Euclidean geometry but, more important,
> that non-Euclidean geometries as mathematical abstractions can and do
> exist.
>
> Consider the two-dimensional surface of a sphere, itself embedded in
> the three-dimensional space geometry of everyday existence. Euclid's
> system accurately describes the geometry of ordinary three-dimensional
> space, but not the geometry on the surface of a sphere. Let us consider
> two lines locally parallel on the surface of a sphere. They propagate
> on the surface as straight as any lines could possibly be, they bend in
> their courses one whit neither to left or right. Yet they meet and
> cross. Clearly, geodesic lines (on a surface, a geodesic is the
> shortest line between two nearby points) on the curved surface of a
> sphere do not obey Euclid's parallel postulate.
>
> The thoughts of the great mathematician Karl Friedrich Gauss about
> curvature stemmed not from theoretical spheres drawn on paper but from
> concrete, down-to-Earth measurements. Commissioned by the government in
> 1827 to make a survey map of the region for miles around Gttingen, he
> found that the sum of the angles in his largest survey triangle was
> different from 180. The deviation from 180 observed by Gauss--almost 15
> seconds of arc--was both inescapable evidence for and a measure of the
> curvature of the surface of Earth.
>
> To recognize that straight and initially parallel lines on the surface
> of a sphere can meet was the first step in exploring the idea of a
> curved space. Second came the discovery of Gauss that we do not need to
> consider a sphere or other two-dimensional surface to be embedded in a
> three-dimensional space to define its geometry. It is enough to
> consider measurements made entirely within that two-dimensional
> geometry, such as, would be made by an ant forever restricted to live
> on that surface. The ant would know that the surface is curved by
> measuring that the sum of the internal angles of a large triangle
> differs from 180, or by measuring that the ratio between a large
> circumference and its radius R differs from 2 pi.
>
> Gauss did not limit himself to thinking of a curved two-dimensional
> surface floating in a flat three-dimensional universe. In an 1824
> letter to Ferdinand Karl Schweikart, he dared to conceive that space
> itself is curved: "Indeed I have therefore from time to time in jest
> expressed the desire that Euclidean geometry would not be correct." He
> also wrote: "Although geometers have given much attention to general
> investigations of curved surfaces and their results cover a significant
> portion of the domain of higher geometry, this subject is still so far
> from being exhausted, that it can well be said that, up to this time,
> but a small portion of an exceedingly fruitful field has been
> cultivated" (Royal Society of Gttingen, 8 October 1827). The
> inspiration of these thoughts, dreams, and hopes passed from Gauss to
> his student, Bernhard Riemann.
>
> Bernhard Riemann went on to generalize the ideas of Gauss so that they
> could be used to describe curved spaces of three or more dimensions.
> Gauss had found that the curvature in the neighborhood of a given point
> of a specified two-dimensional space geometry is given by a single
> number: the Gaussian curvature. Riemann found that six numbers are
> needed to describe the curvature of a three-dimensional space at a
> given point, and that 20 numbers at each point are required for a
> four-dimensional geometry: the 20 independent components of the
> so-called Riemann curvature tensor.
>
> In a famous lecture he gave 10 June 1854, entitled On the Hypothesis
> That Lie at the Foundations of Geometry, Riemann emphasized that the
> truth about space is to be discovered not from perusal of the
> 2000-year-old books of Euclid but from physical experience. He pointed
> out that space could be highly irregular at very small distances and
> yet appear smooth at everyday distances. At very great distances, he
> also noted, large-scale curvature of space might show up, perhaps even
> bending the universe into a closed system like a gigantic ball. He
> wrote: "Space [in the large] if one ascribes to it a constant
> curvature, is necessarily finite, provided only that this curvature has
> a positive value, however small.... It is quite conceivable that the
> geometry of space in the very small does not satisfy the axioms of
> [Euclidean] geometry.... The curvature in the three directions can have
> arbitrary values if only the entire curvature for every sizable region
> of space does not differ greatly from zero.... The properties which
> distinguish space from other conceivable triply-extended magnitudes are
> only to be deduced from experience."
>
> But as Einstein was later to remark, "Physicists were still far removed
> from such a way of thinking: space was still, for them, a rigid,
> homogeneous something, susceptible of no change or conditions. Only the
> genius of Riemann, solitary and uncomprehended, had already won its way
> by the middle of the last century to a new conception of space, in
> which space was deprived of its rigidity, and in which its power to
> take part in physical events was recognized as possible."
>
> Even as the 39-year-old Riemann lay dying of tuberculosis at Selasca on
> Lake Maggiore in the summer of 1866, having already achieved his great
> mathematical description of space curvature, he was working on a
> unified description of electromagnetism and gravitation. Why then did
> he not, half a century before Einstein, arrive at a geometric account
> of gravity? No obstacle in his way was greater than this: he thought
> only of space and the curvature of space, whereas Einstein discovered
> that he had to deal with spacetime and the spacetime curvature.
>
> Einstein could not thank Riemann, who ought to have been still alive. A
> letter of warm thanks he did, however, write to Mach. In it he
> explained how mass there does indeed influence inertia here, through
> its influence on the enveloping spacetime geometry. Einstein's
> geometrodynamics had transmuted Mach's bit of philosophy into a bit of
> physics, susceptible to calculation, prediction, and test.
>
> Let us bring out the main idea in what we may call poor man's
> language. Inertia here, in the sense of local inertial frames, that is
> the grip of spacetime here on mass here, is fully defined by the
> geometry, the curvature, the structure of spacetime here. The geometry
> here, however, has to fit smoothly to the geometry of the immediate
> surroundings; those domains, onto their surroundings; and so on, all
> the way around the great curve of space. Moreover, the geometry in each
> local region responds in its curvature to the mass in that region.
> Therefore every bit of momentum-energy, wherever located, makes its
> influence felt on the geometry of space throughout the whole
> universe--and felt, thus, on inertia right here.
>
> The bumpy surface of a potato is easy to picture. It is the
> two-dimensional analogue of a bumpy three-sphere, the space geometry of
> a universe loaded irregularly here and there with concentrations and
> distributions of momentum-energy. If the spacetime has a Cauchy
> surface, that three-geometry once known--mathematical solutions as it
> is of the so-called initial-value problem of geometrodynamics--the
> future evolution of that geometry follows straightforwardly and
> deterministically.
>
> In other words, inertia (local inertial frames) everywhere and at all
> times is toally fixed, specified, determined, by the initial
> distribution of momentum-energy, of mass and mass-in-motion. The
> mathematics cries out with all the force at its command that mass there
> does determine inertia here.
>
> One exciting experiment to be performed by the turn of the century will
> be the measurement of frame-dragging by the Earth as it rotates. It is
> estimated that the gravitational effect of the rotating Earth on the
> local spacetime nearby is a measurable effect [330 milliarcsec per
> year]. The mass of the Earth has about 0.698 billionth total voting
> power as the rest of the universe on our local spacetime!
>

From: Sam Wormley on
On 7/16/10 1:25 PM, JT wrote:
> Well i did Sam it is the time it takes for the Earth to complete one
> rotation relative to the vernal equinox. And i guess that would be
> relative a fix star, so you say basicly that absolute rotation is
> relative fixed stars in the sky, i will buy that when you propose a
> force from those stars that is able to create the centripetal and
> centrifugal forces that a disc that spin relative them will produce.

While you wait for the "magical force" I assume you will ignore
the empirical evidence of pendulum, gyro, and direct observation?
From: Sam Wormley on
On 7/16/10 1:49 PM, JT wrote:
> On 16 Juli, 20:40, Sam Wormley<sworml...(a)gmail.com> wrote:
>> On 7/16/10 12:53 PM, JT wrote:
>>
>>> Well i can see an idiot ***trying*** to answer our rotation relative
>>> the sun as RPM, but the idiot said he could give us the absolute
>>> rotation of earth in RPM.
>>
>>> But however i am still curious how you draw the conclusion.
>>
>>> 360 / (24 * 60) = 0.25 degrees /min
>>
>>> http://www.wolframalpha.com/input/?i=0.25+degrees+/min+to+RPM
>>
>>> 6.94x10^-4 rpm (revolutions per minute)
>>
>>> JT
>>
>> The Earth's angular velocity = 0.72921158553 X 10**-4 Rad/s
>> which comes out to be 86164.0905 seconds for a 2π (360°) rotation
>> and 239.344696 seconds for every 1° or rotation.
>
> Is that angular velocity versus what sun fixed stars........ or what?
> Is it also the absolute rotation?
>
> JT

Rotation is absolute in this universe.

From: JT on
On 16 Juli, 22:17, NoEinstein <noeinst...(a)bellsouth.net> wrote:
> On Jul 16, 2:44 am, JT <jonas.thornv...(a)hotmail.com> wrote:
>
> JT:  Einstein was the only BAD genius, because his IQ was 85,
> maximum.  Ha, ha, HA!  — NE —
>
>
>
>
>
> > On 15 Juli, 22:53, PD <thedraperfam...(a)gmail.com> wrote:
>
> > > On Jul 14, 4:51 am,JT<jonas.thornv...(a)hotmail.com> wrote:
>
> > > > On 12 Juli, 01:27, "Socratis" <socra...(a)alice.it> wrote:
>
> > > > > "Androcles" <Headmas...(a)Hogwarts.physics_z> wrote in message
>
> > > > >news:WEq_n.205263$k15.183421(a)hurricane...
>
> > > > > > "Socratis" <socra...(a)alice.it> wrote in message
> > > > > >news:i1d9b3$ele$1(a)speranza.aioe.org...
> > > > > > | Out in space on a merry-go-round that's not moving.
> > > > > > | You toss the ball straight away from you - it goes directly
> > > > > > | to the person across from you.
> > > > > > |
> > > > > > | Out in space on a merry-go-round that's rotating.
> > > > > > | You toss the ball straight away from you (directly toward
> > > > > > | the person opposite) - it curves away toward someone else.
> > > > > > |
> > > > > > | Not trying to be a troll - I just don't understand the physics.
> > > > > > | It seems clear to me that this demonstrates that the merry-go-round
> > > > > > | is (absolutely) rotating in the second case.
> > > > > > |
> > > > > > You are already "out in space" riding the merry-go-round called "Earth".
> > > > > > There is a thin layer of air above you for 100 km (65 miles) straight up
> > > > > > and if you ride up in a balloon to that height you'd see the blackness of
> > > > > > space. The blue you see in daylight is scattered sunlight. It is scattered
> > > > > > by dust. At night you will be in the Earth's shadow, and if your view is
> > > > > > clear (no clouds) you'll see stars. As you turn, you'll see the stars
> > > > > > cross
> > > > > > the sky until you turn toward the Sun. Then it will be dawn, and as you
> > > > > > watch, you'll turn with the Earth and the Sun will appear to rise in the
> > > > > > sky
> > > > > > and then set in the west, but it is really not moving at all, you are as
> > > > > > you
> > > > > > ride the Earth. Thus the Sun crossing the sky is RELATIVE motion. There is
> > > > > > no absolute motion. Go outside and look up until you understand you are on
> > > > > > a
> > > > > > merry-go-round called Earth and the universe is standing still while *you*
> > > > > > are moving. Pick any star, then look where it is every hour of the night.
> > > > > > Do
> > > > > > this at least once in your life. I've done it many times, as do all
> > > > > > amateur
> > > > > > astronomers. If you get bored, do some night fishing. Be alone with Nature
> > > > > > for company, for just one night. You may get to like it,  I know I do. Get
> > > > > > away from city lights, get away from people anywhere and enjoy the
> > > > > > universe
> > > > > > you live in the way that people did before there was such a thing as
> > > > > > electricity to spoil the glory of the heavens. I can't do it for you, only
> > > > > > you can do it for yourself. If you have some impediment that prevents you,
> > > > > > overcome it. I don't know you or anything about you, I can only suggest
> > > > > > you
> > > > > > learn to live alone for one night without TV, radio or people telling you
> > > > > > what to do, how to think. Listen to the insects, look at the sky, catch a
> > > > > > fish. Do not light a fire, stay in the dark and *see*.
>
> > > > > Unfortunately, this is a typical answer that ignores the basic question.  It
> > > > > seems to me that rotation proves that absolute motion exists, and I
> > > > > can't seem to find a coherent explanation otherwise.  When something
> > > > > is rotating, objects on it and part of it are forced to the outside by
> > > > > something we typically call 'centrifugal force', a term I'm aware is
> > > > > controversial.  When something isn't rotating, objects on that
> > > > > something don't experience that 'force'.
>
> > > > > Please, if you know of a coherent way of explaining this, point me
> > > > > to it and I'll try to understand it, because I want to understand it.
> > > > > If you're tired of typing, just point me to a link.
> > > > > I and many others realize there are a lot of smart physicists who
> > > > > state there is no absolute motion, and many laymen who are
> > > > > directly aware that a rotating object is quite different from a
> > > > > non-rotating object.  Unlike the speed of light issues (which
> > > > > all make sense to me) the difference between rotating and
> > > > > non-rotating objects can be experienced by anyone, providing
> > > > > compelling and immediate evidence that absolute motion exists.- Dölj citerad text -
>
> > > > > - Visa citerad text -
>
> > > > I also find your questions interesting i do not know anything about
> > > > physic
>
> > > This seems to be a significant improvement in your self-assessment
> > > skills.- Dölj citerad text -
>
> > > - Visa citerad text -
>
> > It is all true but i am a bad genius on deductive reasoning.
>
> > JT- Hide quoted text -
>
> > - Show quoted text -

Put another +100 and -7 and you close in on reality.
From: JT on
On 16 Juli, 22:21, NoEinstein <noeinst...(a)bellsouth.net> wrote:
> On Jul 16, 3:10 am, JT <jonas.thornv...(a)hotmail.com> wrote:
>
> Ha, ha, HA!   — NE —
>
>
>
>
>
> > On 16 Juli, 04:55, NoEinstein <noeinst...(a)bellsouth.net> wrote:
>
> > > On Jul 15, 8:16 am,JT<jonas.thornv...(a)hotmail.com> wrote:
>
> > > DearJT:  Are you drunk?  Rotation much beyond 60 per minute would
> > > incapacitate everyone on board.  Get off the sauce, man!  — NoEinstein
> > > —
>
> > > > On 15 Juli, 01:46, NoEinstein <noeinst...(a)bellsouth.net> wrote:
>
> > > > > On Jul 14, 5:51 am,JT<jonas.thornv...(a)hotmail.com> wrote:
>
> > > > > DearJT:  You preface by saying that you know nothing about physics.
> > > > > Then, you claim that physical rotating a space ship 10,000 RPM won't
> > > > > impose stress on the occupants.  So, you prove your own point: You
> > > > > don't know anything about physics!  The laws of physics don't require
> > > > > closeness to mass for their existence.  In most likelihood, every
> > > > > person on your spaceship would be dead, from draining their blood from
> > > > > their brain, or stopping their heart because of the compressive forces
> > > > > put on the bodies.  The best way for you to learn physics is to
> > > > > observe what happens in real life.  Put a rat in a cage and spin it
> > > > > 10K rpm, and the rat dies.  Of course that same thing will happen
> > > > > halfway between galaxies.  — NoEinstein —
>
> > > > So what do you suppose the ship rotate relative (i said it rotate at
> > > > 100 000RPM relative earth but what make you say it is really rotating,
> > > > so tell me what is the real rotational RPM and versus what i guess you
> > > > do not hold our earth for the origo of nonerotation?)
>
> > > > The rotation of earth is measured against a fixed point origo, namely
> > > > our sun in euclidian space, using a Cartesian cordinate system if
> > > > earth never would change face relative the sun we would still have an
> > > > orbit but earth would be a nonerotating object by definition.
>
> > > > Do you propose that our sun is the origo of the nonerotating Euclidian
> > > > space we travel?
>
> > > > OR what is the nonerotating frame of the universe do you try to say
> > > > there is an absolute nonerotational frame in the the universe, i think
> > > > everyone is keen to now what you propose it is.
>
> > > > I say rotational forces is only present when something breaks out from
> > > > the ruling gravitational field.
> > > > In deepspace the body will not experience any g-forces, the only thing
> > > > that will let you know that you rotate is the background stars, If you
> > > > propose that there is a g-forces relative these foreign starts you
> > > > will have to invent a new longdistance gravitational force, i am all
> > > > pro that many have proposed such a force.
>
> > > > But your handwaving doesn't do it for me.
>
> > > >  JT
>
> > > > > > On 12 Juli, 01:27, "Socratis" <socra...(a)alice.it> wrote:
>
> > > > > > > "Androcles" <Headmas...(a)Hogwarts.physics_z> wrote in message
>
> > > > > > >news:WEq_n.205263$k15.183421(a)hurricane...
>
> > > > > > > > "Socratis" <socra...(a)alice.it> wrote in message
> > > > > > > >news:i1d9b3$ele$1(a)speranza.aioe.org...
> > > > > > > > | Out in space on a merry-go-round that's not moving.
> > > > > > > > | You toss the ball straight away from you - it goes directly
> > > > > > > > | to the person across from you.
> > > > > > > > |
> > > > > > > > | Out in space on a merry-go-round that's rotating.
> > > > > > > > | You toss the ball straight away from you (directly toward
> > > > > > > > | the person opposite) - it curves away toward someone else..
> > > > > > > > |
> > > > > > > > | Not trying to be a troll - I just don't understand the physics.
> > > > > > > > | It seems clear to me that this demonstrates that the merry-go-round
> > > > > > > > | is (absolutely) rotating in the second case.
> > > > > > > > |
> > > > > > > > You are already "out in space" riding the merry-go-round called "Earth".
> > > > > > > > There is a thin layer of air above you for 100 km (65 miles) straight up
> > > > > > > > and if you ride up in a balloon to that height you'd see the blackness of
> > > > > > > > space. The blue you see in daylight is scattered sunlight. It is scattered
> > > > > > > > by dust. At night you will be in the Earth's shadow, and if your view is
> > > > > > > > clear (no clouds) you'll see stars. As you turn, you'll see the stars
> > > > > > > > cross
> > > > > > > > the sky until you turn toward the Sun. Then it will be dawn, and as you
> > > > > > > > watch, you'll turn with the Earth and the Sun will appear to rise in the
> > > > > > > > sky
> > > > > > > > and then set in the west, but it is really not moving at all, you are as
> > > > > > > > you
> > > > > > > > ride the Earth. Thus the Sun crossing the sky is RELATIVE motion. There is
> > > > > > > > no absolute motion. Go outside and look up until you understand you are on
> > > > > > > > a
> > > > > > > > merry-go-round called Earth and the universe is standing still while *you*
> > > > > > > > are moving. Pick any star, then look where it is every hour of the night.
> > > > > > > > Do
> > > > > > > > this at least once in your life. I've done it many times, as do all
> > > > > > > > amateur
> > > > > > > > astronomers. If you get bored, do some night fishing. Be alone with Nature
> > > > > > > > for company, for just one night. You may get to like it,  I know I do. Get
> > > > > > > > away from city lights, get away from people anywhere and enjoy the
> > > > > > > > universe
> > > > > > > > you live in the way that people did before there was such a thing as
> > > > > > > > electricity to spoil the glory of the heavens. I can't do it for you, only
> > > > > > > > you can do it for yourself. If you have some impediment that prevents you,
> > > > > > > > overcome it. I don't know you or anything about you, I can only suggest
> > > > > > > > you
> > > > > > > > learn to live alone for one night without TV, radio or people telling you
> > > > > > > > what to do, how to think. Listen to the insects, look at the sky, catch a
> > > > > > > > fish. Do not light a fire, stay in the dark and *see*.
>
> > > > > > > Unfortunately, this is a typical answer that ignores the basic question.  It
> > > > > > > seems to me that rotation proves that absolute motion exists, and I
> > > > > > > can't seem to find a coherent explanation otherwise.  When something
> > > > > > > is rotating, objects on it and part of it are forced to the outside by
> > > > > > > something we typically call 'centrifugal force', a term I'm aware is
> > > > > > > controversial.  When something isn't rotating, objects on that
> > > > > > > something don't experience that 'force'.
>
> > > > > > > Please, if you know of a coherent way of explaining this, point me
> > > > > > > to it and I'll try to understand it, because I want to understand it.
> > > > > > > If you're tired of typing, just point me to a link.
> > > > > > > I and many others realize there are a lot of smart physicists who
> > > > > > > state there is no absolute motion, and many laymen who are
> > > > > > > directly aware that a rotating object is quite different from a
> > > > > > > non-rotating object.  Unlike the speed of light issues (which
> > > > > > > all make sense to me) the difference between rotating and
> > > > > > > non-rotating objects can be experienced by anyone, providing
> > > > > > > compelling and immediate evidence that absolute motion exists..- Dölj citerad text -
>
> > > > > > > - Visa citerad text -
>
> > > > > > I also find your questions interesting i do not know anything about
> > > > > > physic but to me it seem like the centrifugal and centripetal force
> > > > > > only is adjacent when you have rotation within a gravitational field.
> > > > > > So rotational forces is the result of a body trying to break out from
> > > > > > the ruling gravitational field.
>
> > > > > > A ship in deepspace rotating at a 100 000 RPM versus earth will put no
> > > > > > strain or forces upon the inhabitants nor the ship..........
> > > > > > It is only when the ship get close to a big gravitational body the g-
> > > > > > forces will start to act upon both ship and its inhabitants.
>
> > > > > > This could all be wrong, but then there probably is a centra of
> > > > > > gravity in the universe so absolute rotation can be measured even in
> > > > > > deep space far away from gravitational attractors.
>
> > > > > >JT- Hide quoted text -
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> > > > > - Visa citerad text -- Hide quoted text -
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> > Bullshit you have no clue about what rotation is, rotation is not
> > measured RPM an objects absolute rotation is measured by tension and
> > stress forces within the material.
>
> > And as i told you there will not be any on an object rotating in deep
> > space, unless you invent some new type of gravitational force working
> > over vast distances.
>
> > Centrifugal and centripetal forces is created when an object moving
> > within a gravitational field, so when you spinn it is trying to break
> > lose from the stronger gravitational field.
>
> > But what is this force you seem to think exist that work over deep
> > space and still manage to hold your object from not rotating, and will
> > create the centripetal force, centrifugal force when it start rotate.
>
> > And what create that force do you suggest it is mass, it can not be
> > inertia because that only work during the acceleration face.
>
> > What is your suggestion for none rotation and creation of the
> > ****absolute rotational forces**** that you seem to imply exist?
>
> > JT- Hide quoted text -
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> > - Show quoted text -

Well i will beat any monkey bot named NoEinstein in any IQ test.