Gravity Lenses

Gravity Lens

Gravitational fields are only homogeneous over small volumes of space and show different degrees and fluctuations of intensity over large cosmological distances. The curvature of space is increasingly effected by the mass and consequent gravitational intensity of larger astrophysical bodies and as light propagates along this spacial curvature, the apparent position and actual position of objects in space differs. Planets, stars, galaxies and galactic clusters all have an effect on curving light that either emanates from them, or that passes through their gravitational influence in a line of sight propagation from the original source to the observer.

Gravitational effects not only determine the apparent position of objects but also their appearance as far as apparent shape and size are concerned. These effects were first predicted by Einstein's relativity theory and proven by the inadequacy of the earlier Newtonian theory in the observation of the planet Mercury's perihelion (closest point in its orbit to the Sun) also in the now proven bending of starlight as it passes close to the limb of the Sun and displaces the starfield's apparent position more, the closer to the limb this light passes.

We are also used to seeing objects reduce in apparent size with the effects of perspective - this phenomenon may actually be reversed at very large cosmological distances, predicted to occur at about 5000 MPc (one Parsec = 3,26 Light Years, one LY = 9,4605e+12 km, therefore about 4.7e+22 km). Past these distances further objects may actually begin to appear larger depending on the actual curvature of space about which there is still some conjecture.

When a distant light emitting source lies in exact line of sight with a sufficiently large gravitational body such as a galaxy, the closer object's field may cause a gravitational lens to be formed which can split the further object's image into multiple images - this is the effect seen above.
The first actual gravitational lens was discovered in 1979 by the British astronomer Dennis Walsh. This lens is a giant elliptical galaxy which produces a double image of a vastly more distant quasar (quasi-stellar object - some of the most energetic and bright objects, all lying at vast distances.)

An even stranger phenomenon is the "Einstein Lens" which causes the further object's image to be projected as a perfect ring, this first observed in 1988.

The actual curvature of the Universe depends solely on the matter-density per cubic volume of space. Einstein and De Sitter worked extensively on models of future cosmic evolution and universes that were respectively open, closed, bounded and unbounded were postulated. In a universe where the density factor is exactly Unity, the universe will have a Euclidean geometry. A density factor of more than unity will cause the universe to reach an equilibrium phase in the far future after which it will gravitationally collapse in on itself, a "Big Crunch" which in itself might be a cyclically transitional phase for another Big Bang creative phase.

If the density factor is less than unity the universe will essentially continue to expand forever. The density factor can empirically be determined by measuring the distribution of matter in the visible universe. When this is done by advanced astrophysical measurement techniques, the amount of visible matter in the universe falls far short of a unity distribution. It is however strongly suspected that so-called "dark matter", interstellar gas and dust clouds that consist of non-emitting material, contributes vastly more matter than attributed only to the visible component, thereby making up for the "missing matter". The latest observational evidence places the density distribution extremely close to a unity factor, a stable everlasting universe. The evidence for a Euclidean universe comes mainly from observations of the cosmic microwave background radiation at a telescope in Saskatoon, Canada, although this has also been exmined by NASA's Cosmic Background Explorer (COBE). Gravitational lenses are however regarded as counter-evidence for the Euclidean geometry of space as it is argued that such lensing effects should be common in such a universe whereas in reality they are rare.

Another type of gravitational light distortion, sweeping arcs of light, such as seen here in the nebula Abell 2218, should be infrequently observed whereas they are far more common. This image was photographed by the Hubble Space Telescope, HST's wide field planetary camera. Abell 2218 Gravity Lensing

The case for the open or closed universe is therefore not yet solidly resolved and the intriguing mystery continues...