Through the Looking Glass
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A - HST 01248+0351 is a lensed pair on either side of the edge-on disk lensing galaxy.
A gravitational lens is created when the gravity of a massive foreground object, such as a galaxy or black hole, bends the light coming from a far more distant galaxy directly behind it. This focuses the light to give multiple or distorted images of the background object as seen by the observer.
A quick look at over 500 Hubble fields of sky has uncovered 10 interesting lens candidates in the deepest 100 fields. This is a significant increase in the number of known optical gravitational lenses. Hubble's sensitivity and high resolution allow it to see faint and distant lenses that cannot be detected with ground-based telescopes whose images are blurred by Earth's atmosphere. An analysis of this "Top Ten" list of Hubble gravitational lenses is published by Kavan Ratnatunga and Richard Griffiths of Carnegie Mellon University in the May issue of the Astronomical Journal.
The amount of gravitational lensing in the universe depends strongly on the cosmological constant, a hypothesized repulsive force that indicates the universe is older and larger than without this force. Therefore a large cosmological constant implies a larger number of more distant objects whose light can, by chance, pass close to a massive galaxy on its way to Earth and appear lensed.
The 100 Hubble fields cover a total area equal to that of the full Moon. Hubble's ability to see so many of these lenses in a small fraction of the sky takes them from being a scientific curiosity to serving as a potentially powerful tool for probing the universe's evolution and expansion.
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In 1936 Albert Einstein computed the gravitational deflection of light by massive objects and showed that an image can be highly magnified if the observer, source and the lensing object are well aligned. However, the lensed image separations were predicted to be so small in angular size, Einstein knew they were beyond the capabilities of ground-based optical telescopes. This made him remark that "there is no great chance of observing this phenomenon."
It wasn't for another 40 years since Einstein's conclusion that the first gravitational lens was discovered in 1979. Several bright and nearby lenses have been discovered since then from ground-based observations.
Further lens discoveries required Hubble's high resolution Wide Field Planetary Camera 2 (WFPC2) which allows the search extended to much fainter and farther objects. It is expected that the Advanced Camera for Surveys, to be installed on Hubble in the year 2000, will be able to discover many more gravitational lenses because of its sensitivity and relatively wide-angle coverage.
STScI press release - May 13, 1999
Hubble home page - at STScI
Gravitational Lensing Tutorial - from the Goddard Space Flight Center
Ring Around a Galaxy - Astronomy Picture of the Day, Dec. 23, 1998
Hubble Deep Field South - Astronomy Picture of the Day, Dec. 14, 1998
A Bulls-eye Einstein Ring - Astronomy Picture of the Day, Mar. 30, 1998
A Galaxy Cluster Lens - Astronomy Picture of the Day, Jan. 11, 1998
Chandra will target the age of the Universe -- Astronomers plan X-ray measurements of galaxy clusters for a new measurement of the Hubble Constant Apr. 23, 1999 NASA Science News
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