(Submitted June 10, 1997)
What evidence is there that supports the theory of curved space?
What does General Relativity predict about the shape of
space-time near a large mass (eg, a star)?
There has been experimental evidence for the curvature
of spacetime by a massive object since the early part of this
century (1922), when observers set out to test the predictions of
general relativity. During a solar eclipse, they realized, the
light from stars in the same general area of the sky as the Sun
are visible during the day. If light from these stars is affected
by the curvature of spacetime due to the Sun's mass, then this would
be measurable as a deflection (or a change in location) of the star's
position on the sky. The stars closer to the position of the Sun in
the sky would suffer a larger deflection; in general the deflection
would be proportion to the stars distance from the Sun's location on
the sky. This effect was observed for 15 stars during the solar eclipse
of 1922 in Western Australia, and was interpreted as observational
verification of the predictions of general relativity. General relativity
predicts that spherical masses deform spacetime in much the same way a
lead ball would deform the surface of a rubber sheet. It is this deformation
that causes the planets to orbit the Sun, and the Moon to orbit the Earth.
In fact, all orbital motion is the result of bodies being affected by the
curvature of the spacetime in which they move.
Since that time, astronomers have observed other instances of the
curvature of spacetime near massive objects. One example is the deflection
of radio waves from quasars which are occulted by the Sun every year (such
as 3C 279). Another is the growing collection of gravitational lenses.
A gravitational lens occurs when the light from a very distant object
(often a quasar) is bent by a closer massive object (such as a galaxy) into
*multiple* images. Some very impressive images of gravitational lenses
have been taken. See, for example the Astronomy Picture of the Day:
Padi Boyd, for the Ask an Astrophysicist