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Will Gravity Probe B fulfill its promise?
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Everything I need to know I learned through Googling. |
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Can they re-run any tests now that they know about the charge patches to either get better data, or help reduce the noise?
CJSF
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Two years ago moved from my town I was looking up past the city lights But the city lights got in my way See the constellation ride across the sky No cigar, no lady on his arm Just a guy made of dots and lines -from "See The Constellation" by They Might Be Giants |
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All this may actually be a moot point since other recent reports from lunar ranging by Nordtvedt (using 35 years of lunar laser ranging data) have confirmed gravitomagnetism in the earth-moon system to 0.1 % of the GR prediction. See here: http://arxiv.org/PS_cache/gr-qc/pdf/0702/0702028v1.pdf Nordtvedt has been at the forefront for years in LLR, and (although not given the publicity of more media hyped GP-B) has previously shown that the solar geodetic effect (the so-called deSitter-Folker precession which rotates the plane of the earth-moon system), confirms GR predictions to about the same accuracy (0.1 %), ......and has also put tight constraints on competing theories, (as well as confirming the non-linear coupling of earth's gravity to itself, and the constancy of G to high precision). See here; http://www.springerlink.com/content/2gjffbwea99mrjxa/ Needless to say, Everitt was not too happy about the Nordtvedt report on Gravitomagnetism....but the same GR gravitomagnetic term that is used for the GP-B frame dragging is also responsible for the Gravitomagnetism of two rotating massive objects. So why not use the 'God given' gyroscopes that are already in place ? ....dang, Nordtvedt didn't even have to make the moon go superconducting or polish it to one billionth of a cm. ! ![]() G^2 ![]() Last edited by Gsquare; 02-May-2007 at 08:18 AM. |
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G^2,
If I read that .pdf right, the moon's orbit deviates no more than roughly 1cm from GR's predicted course. If that's correct, then that is darn-tootin' good. And from the Springerlink abstract, another thing I like is the earth and moon fall toward the sun at the same rate to within 10^-13. That is pretty good, too. -Richard -Richard |
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G^2 |
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Good point that 'any force' binding them will also require a vel. dependent term in the moving frame. Quote:
To the moving observer there is also Length contraction (in the direction of motion) by the same factor gamma; the shortened length between masses means greater gravitational mass. Also the charge density increases by a similar amount due to the same length contraction....so its possible mass-charge stays in equiibrium;(haven't done the math though). G^2 ![]() |
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Here is a paper that goes into detail on the mass-charge equilibrium: http://www.arxiv.org/abs/gr-qc/0304084 Note the interesting thing. If you add the requirement that inertial mass equal gravitational mass, you get only one factor of 2 (to first order, there are higher order terms apparently) on the gravitomagnetic force. The authors say the other factor of 2 can be seen as coming from "curvature". ![]() Note that Maxwellian gravity (without the factor of 4) would be completely Lorentz-kosher otherwise. It's only if you require the Equivalence Principle to absolutely hold that things have to get fancy........ ![]() -Richard |
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And thus it has become a 'nicht gedenken' experiment. Quote:
However, I unintentionally skipped over the section on justification of Gravitomagnetism using this thought exp.( ), since my intention was to focus on the implications of the Maxwellian gravity analogs involving spin, and not proving the necessity of gravitomagnetism, (However, the author does give a good formal presentation.). I really liked his approach since it uses the linear differential form of the gravitational field analogs which are heuristically simpler and more amenable to my limited cognitive resources. Nevertheless, as far as I am concerned there is enough 'real' physical evidence for gravitomagetism (GP-B not withstanding), that I need not resort to 'gedenken' type simplifications.That is what my 'Nordtvedt post' above was about. Gads; Nordtvedt even makes the case that gravitomagnetism is quite ubiquitous .... in the origin of inertia.... ![]() Here is a very interesting secondary source...referring to his comments .... http://physics.fullerton.edu/~jimw/g...ertia/nord.htm You are probably already familiar with it; if not, I recommend it considering the implications. Nevetheless, I really do want to get back to the issue of gravitomagnetism coupling to spin since that is where the experimental evidence is lacking. Maybe I will resurrect our last discussion in that regard when I have more time. G^2 ![]() Last edited by Gsquare; 09-May-2007 at 02:01 AM. |
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http://einstein.stanford.edu/
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jwj It's ok not to know. We should try harder to find out. |
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Testing for Lorentz Violation: Constraints on Standard-Model Extension Parameters via Lunar Laser Ranging
James B. R. Battat, John F. Chandler, Christopher W. Stubbs Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 http://arxiv.org/PS_cache/arxiv/pdf/...710.0702v1.pdf Quote:
After looking at some of the modifications they are making in the APOLLO experiment, such as measuring the effects of continental drift, it will be interesting to see how much the moon's orbital path is truly increasing. First round APOLLO science testing should be completed within a year.
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jwj It's ok not to know. We should try harder to find out. |
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Constraining Torsion with Gravity Probe B
Mao, Tegmark, Guth and Cabi http://arxiv.org/PS_cache/gr-qc/pdf/0608/0608121v4.pdf Quote:
We know the rotational moments of the Gravity B probes did change over time, and this unexpected change is thought to be due to electrostatic coupling and a time-dependent Polhode moment. If this unexpected momentum is due to torsion coupling; The coupling of each gyroscope should vary as a function of the angle of the gyroscope relative to the local 'torsion' moment. It would be interesting to see what the net Polhode correction would be if the torsion correction is first applied to each gyroscope.
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jwj It's ok not to know. We should try harder to find out. |
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http://einstein.stanford.edu/
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jwj It's ok not to know. We should try harder to find out. |
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Good question...probably you don't know. I really don't put much confidence in "tweaking" the gravitomagnetic data with new 'ad hoc' experimental models ....it seems too much like someone's trying to fit the data so as to resurrect a GR prediction from the GP-B ashes... If 30% error level is considered "reasonable" then the Lageos satellite detection by Ciulfolini beat them to the punch, at least for the gravitomagnetic part. Maybe we should go back and investigate other approaches....like the South Pole gravitomagnetic proposal by Braginsky and Kip Thorne. Rather than divert the OP I've put that idea on another thread here: South Pole Experimental Detection of Gravitomagnetism G^2 ![]() |
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Has Gravity Probe B been a Big Flop?
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Everything I need to know I learned through Googling. |
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I'm thinking that Gravity Probe C should be in a low orbit around Jupiter.
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Forming opinions as we speak |
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As I'm fond of saying, "if we knew what we were doing, it wouldn't be called research".
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