Relativity and the 1919 eclipse
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Figure 1. Principe Island, 29 May 1919. Marked on a negative photo of the 1919 solar eclipse are the positions of stars examined in the historic test of Einstein's theory of gravity (from Memoirs of the Royal Astronomical Society LXII, Appendix Plate 1). Enquiries about reproducing this and related totality images should be addressed to the Library of the Royal Astronomical Society, London. Image courtesy of the Royal Astronomical Society |
The announcement of favourable results in London on 8 November 1919 signalled the replacement of Newton's theory of gravity by the theory of general relativity. Its inventor, a 40-year-old Berliner called Albert Einstein, at once became the most famous scientist in the world. Expeditions of astronomers photographed the eclipse in difficult tropical conditions in Brazil and on the African island of Principe. At the time, the Sun was in front of a useful cluster of stars, the Hyades. The astronomers compared the relative positions in the sky near the Sun with the positions of the same stars as previously photographed in the night sky. The expeditions and analyses, organized by the Royal Society and the Royal Astronomical Society, were masterminded by Arthur Eddington of Cambridge. He was one of the very few experts who immediately understood Einstein's theory and appreciated its revolutionary importance, if it was correct.
Even for stars almost in line with the Sun, the shift in apparent position is less than 2 seconds of arc, or a few ten-thousandths of a degree. The 1919 measurements confirmed that the Sun bent the light rays by roughly the right extent - less than predicted in Principe, more than predicted in Brazil. After half a century of similar eclipse observations of the shifting stars, critics still said that there could be a 20 per cent error in the results. They were not accurate enough to rule out newer theories of gravity that challenged Einstein's version. Radio astronomers did somewhat better, with Quasar 3C279 which passes behind the Sun on 8 October every year. ESA's Hipparcos satellite (1989-93) provided the emphatic confirmation of Einstein's prediction. Hipparcos charted the positions of stars so accurately that no eclipse was needed to see the effect of the Sun's gravity. Where previous observations of the shifts had been confined to objects seen within a degree or two of the edge of the Sun, where the effect is strongest, the European satellite sensed the bending of light-rays even from stars in the night sky, at right angles to the Sun. According to the Hipparcos scientists, Einstein's prediction is correct to within one part in a thousand.
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Figure 2. Illustration of gravitational bending - light from a star is bent by the strong gravitational field of the Sun. The effect of this is that the star appears to be in a different position. |
