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Hubble Finds Double Einstein Ring
ScienceDaily (Jan. 12, 2008) - The NASA/ESA Hubble Space Telescope has revealed 
a never-before-seen optical alignment in space: a pair of glowing rings, one 
nestled inside the other like a bull's-eye pattern. The double-ring pattern is 
caused by the complex bending of light from two distant galaxies strung 
directly behind a foreground massive galaxy, like three beads on a string.


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See also: 
Space & Time
  a.. Astrophysics
  b.. Astronomy
  c.. Galaxies
  d.. Dark Matter
  e.. NASA
  f.. Space Telescopes
Reference
  a.. Barred spiral galaxy
  b.. Hubble Deep Field
  c.. Galaxy formation and evolution
  d.. Local Group
More than just a novelty, a very rare phenomenon found with the Hubble Space 
Telescope can offer insight into dark matter, dark energy, the nature of 
distant galaxies, and even the curvature of the Universe. A double Einstein 
ring has been found by an international team of astronomers led by Raphael 
Gavazzi and Tommaso Treu of the University of California, Santa Barbara. The 
discovery is part of the ongoing Sloan Lens Advanced Camera for Surveys (SLACS) 
program. They are reporting their results at the 211th meeting of the American 
Astronomical Society in Austin, Texas, USA. A paper has been submitted to The 
Astrophysical Journal.

The phenomenon, called gravitational lensing, occurs when a massive galaxy in 
the foreground bends the light rays from a distant galaxy behind it, in much 
the same way as a magnifying glass would. When both galaxies are exactly lined 
up, the light forms a circle, called an "Einstein ring", around the foreground 
galaxy. If another more distant galaxy lies precisely on the same sightline, a 
second, larger ring will appear.

The odds of seeing such a special alignment are so small that Tommaso says that 
they "hit the jackpot" with this discovery.

"Such stunning cosmic coincidences reveal so much about nature. Dark matter is 
not hidden to lensing," added Leonidas Moustakas of the Jet Propulsion 
Laboratory in Pasadena, California, USA. "The elegance of this lens is trumped 
only by the secrets of nature that it reveals."

The massive foreground galaxy is almost perfectly aligned in the sky with two 
background galaxies at different distances. The foreground galaxy is 3 billion 
light-years away. The inner ring and outer ring are comprised of multiple 
images of two galaxies at a distance of 6 billion and approximately 11 billion 
light-years.

SLACS team member Adam Bolton of the University of Hawaii's Institute for 
Astronomy in Honolulu first identified the lens in the Sloan Digital Sky Survey 
(SDSS). "The original signature that led us to this discovery was a mere 500 
photons (particles of light) hidden among 500,000 other photons in the SDSS 
spectrum of the foreground galaxy," commented Bolton.

"The twin rings were clearly visible in the Hubble image", added Tommaso. "When 
I first saw it I said 'wow, this is insane!' I could not believe it!"

The distribution of dark matter in the foreground galaxies that is warping 
space to create the gravitational lens can be precisely mapped. In addition, 
the geometry of the two Einstein rings allowed the team to measure the mass of 
the middle galaxy precisely to be a value of 1 billion solar masses. The team 
reports that this is the first measurement of the mass of a dwarf galaxy at 
cosmological distance (redshift of z=0.6).

A sample of several dozen double rings such as this one would offer a purely 
independent measure. The comparative radius of the rings could also be used to 
provide an independent measure of the curvature of space by gravity.

Observations of the cosmic microwave background (a relic from the Big Bang) 
favour flat geometry. A sample of 50 suitable double Einstein rings would be 
sufficient to measure the dark matter content of the Universe and the equation 
of state of the dark energy (a measure of its pressure) to 10 percent 
precision. Other double Einstein rings could be found with wide-field space 
telescope sky surveys that are being proposed for the Joint Dark Energy Mission 
(JDEM) and recently recommended by the National Research Council.

Adapted from materials provided by ESA/Hubble Information Centre.

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