Originally posted by toe21k
... from Gravity Probe B 'Official' Web Site:-
http://einstein.stanford.edu/content/story_of_gpb/gpbsty2.html
Any Comment(s) [?]
For the most part... very good article, 21toes
The basic idea, as Lurch said, is to test competing relativistic theories. In order to do so Gravity Prbe B is actually testing two different predicted GR effects:
One is called the
geodetic effect: At the proposed orbit the gyroscope axis is predicted by GR to precess (about 6.6 arcseconds/yr.) strictly due to its passage thru the static gravitational field of the earth; i.e., strictly as a result of passing thru the Earth's 'space-time curvature'. This is the same effect that produces the advance of the perihelion of Mercury, except in that case it is the solar 'geodetic' effect.
The 2nd effect is sometimes called the 'motional' GR effect, that is, due to the motion of mass (in this case, the
rotation of the earth) and is named after its discoverers Lense-Thirring. This effect is sometimes referred to as the 'gravitomagnetic field' since it is analogous to the magnetic field (in electromagnetics), which is due to the motion of electric charge.
The precession of the gyroscope due to the motional effect is quite a bit smaller than the geodetic, being about 42 milli arcseconds/year, and requires much greater precision and technology. However, in a polar orbit the two effects are predicted to be at right angles to each other, making discrimination somewhat easier.
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