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Sergei Kopeikin, other scientists measure the speed of gravity
Kopeikin worked with Ed Fomalont, a radio astronomer with the National Science Foundation’s National Radio Astronomy Observatory (NRAO) in Charlottesville, Va. On Sept. 8, the scientists measured the shift of a quasar, a celestial object that resembles a star. Jupiter’s gravitational force caused the radio waves from the quasar to shift as Jupiter passed by it closely.
The scientists presented their findings to the American Astronomical Society's meeting in Seattle, Wash. The landmark measurement is important to physicists working on field theories that attempt to combine particle physics with Einstein's general theory of relativity and electromagnetic theory. To conduct the experiment, the scientists used the National Science Foundation's Very Long Baseline Array (VLBA), a continent-wide, radio-telescope system, and a 100-meter radio telescope in Effelsberg, Germany, to make an extremely precise observation when Jupiter passed in front of the quasar. The observation recorded a slight "bending" of the radio waves coming from the quasar because of the gravitational effect of Jupiter. The bending resulted in a small change in the quasar’s apparent position in the sky in addition to the deflection of light calculated by Einstein in 1915.
In 1999, Kopeikin extended Einstein’s theory for light propagation to include the gravitational effects of a moving body on light and radio waves. Prior to this study, no one had tried to measure the speed of gravity because most physicists had assumed that the only way to do so was to detect gravitational waves, Kopeikin said. The MU scientist realized that if Jupiter moved closely in front of a star or radio source, he could test his theory. The VBLA system is a result of a general radio technique known as Very Long Baseline Interferometry (VLBI). January 2003 Additional links: |
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