H
Helmut Wabnig
haha, another goodie for ya, Pom Totter,
http://www.esa.int/esaSC/SEM7I9R1VED_index_0.html
from that page, for the usenet archives:
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Relativity and the 1919 eclipse
Probably the most important eclipse in the history of science occurred
on 29 May 1919. Just six months after the end of World War I, British
astronomers used it to test a new idea that came from Germany in 1915.
The proposition was that gravity affected light, space and time
itself, and as a result the Sun would deflect starlight passing by it.
Changes in the apparent direction of stars in the sky, seen close to
the Sun during a total eclipse, could confirm the idea.
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 originator, a 40-year old Berliner called
Albert Einstein, at once became the most famous scientist in the
world.
Revolutionary theory
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, organised 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.
Illustration of gravitational bending
Illustration of gravitational bending
ESA's Hipparcos confirms Einstein
Even for stars almost in line with the Sun, the shift in apparent
position is less than two 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% 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.
Last update: 13 September 2004
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