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Gravity at play.


Astronomers are delighted to have found 19 galaxies that appear to be bent out of shape Bent Out of Shape is an LP issued by Rainbow in 1983. The first CD version to be released released featured several longer edits compared to the vinyl version. A remastered CD reissue was released in May 1999. . The distorted images are cosmic mirages, arcs or rings of light created when the gravity of a massive foreground object bends and magnifies the light from a galaxy lying behind it. Albert Einstein predicted the effect, known as gravitational lensing, in 1936, but telescopes at the time weren't powerful enough to discern it.

In the study, Adam Bolton of the Harvard-Smithsonian Center for Astrophysics The Harvard-Smithsonian Center for Astrophysics (CfA) is located in Cambridge, Massachusetts. It consists of the Harvard College Observatory and the Smithsonian Astrophysical Observatory. The Center is located at 60 Garden Street.  in Cambridge, Mass., and his colleagues combined the power of the Hubble Space Telescope Hubble Space Telescope (HST), the first large optical orbiting observatory. Built from 1978 to 1990 at a cost of $1.5 billion, the HST (named for astronomer E. P. Hubble) was expected to provide the clearest view yet obtained of the universe.  with the breadth of the Sloan Digital Sky Survey The Sloan Digital Sky Survey or SDSS is a major multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico. The project was named after the Alfred P. . That survey of one-fourth of the sky employs a ground-based telescope in Apache Point, N.M. Using Sloan data, the team picked out large, elliptical galaxies capable of acting as gravitational lenses. When they pointed Hubble at 28 of these lensing candidates, they found arcs and rings close to 19 of them, indicating that they were indeed distorting the images of more-distant galaxies.

Eight of the 19 lensed galaxies have had their light bent into a circle called an Einstein ring In observational astronomy a Chwolson ring or Einstein ring is the deformation of the light from a source (such as a galaxy or star) into a ring through gravitational deflection of the source's light by a lens (such as another galaxy, or a black hole). . This pattern arises when one galaxy is almost exactly aligned behind another, as seen from Earth. Astronomers had previously identified only three Einstein rings.

In addition to providing curious shapes, gravitational lensing is a powerful probe of dark matter, the invisible, exotic material that theorists say resides in massive halos around every elliptical galaxy. Although dark matter halos can't be directly seen, astronomers can deduce the presence of this material by the extent to which its mass bends the light of background galaxies.

Bolton and his colleagues describe their study in the February Astrophysical Journal The Astrophysical Journal, often abbreviated to ApJ, is a scientific journal covering astronomy and astrophysics. It was founded in 1895 by George Ellery Hale and James E. Keeler. It currently (October 2006) publishes three issues per month, with 500 pages per issue. .--R.C.
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Title Annotation:ASTRONOMY
Publication:Science News
Article Type:Brief Article
Geographic Code:1U1MA
Date:Jan 21, 2006
Words:281
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