"Einstein's Telescope": Zooming In On the Dark Side of the Universe

“Such stunning cosmic coincidences reveal so much about nature.”

~ Leonidas Moustakas, Jet Propulsion Laboratory

The 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. 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 and approximately 11 billion light-years.

“Such stunning cosmic coincidences reveal so much about nature.”

~ Leonidas Moustakas, Jet Propulsion Laboratory

The 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. 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 and approximately 11 billion light-years.

The discovery was made by an international team of astronomers led by Raphael Gavazzi and Tommaso Treu of the University of Californi, Santa Barbara. Treu says the odds of seeing such a special alignment are so small that they “hit the jackpot” with this discovery. “When I first saw it I said ‘wow, this is insane!’ I could not believe it!”

But this sight is more than just an incredible novelty. It’s also a very rare phenomenon that can offer insights into dark matter, dark energy, the nature of distant galaxies, and the curvature of the Universe itself. The discovery is part of the ongoing Sloan Lens Advanced Camera for Surveys (SLACS) program.

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 perfectly 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.

“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 Pasaden, California, USA. “The elegance of this lens is trumped only by the secrets of nature that it reveals.”

The dark matter distribution in the foreground galaxies that is warping space to create the Einstein's telescope, the gravitational lens, can be accurately 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.

A sample of several dozen double rings such as this one would offer a purely independent measure of the curvature of space by gravity. This would help in determining what the majority of the Universe is made of, and the properties of dark energy.

Original observations made in 1970 revealed that gravitational motions of gas clouds in the Andromeda galaxy were occurring at speeds far greater than the entire observed mass of that galaxy could account for. Similar problems detected in the 1930's involving motions of entire galaxies had long been disregarded. Later observations confirmed that so-called "ordinary matter" is insufficient to account for observed gravitational effects in the cosmos. Thus the universe must contain huge amounts of "dark matter," that we cannot observe and the composition of which we do not know. 

In 1998 reports of observations of distant supernovae revealed that the expansion of the universe was not slowing, as would be expected from long-term effects of gravity, but was instead accelerating. Something was overcoming the gravitational power of all of the matter in the universe. The acceleration, moreover, has not been present from the Big Bang on. For billions of years the speed of expansion slowed. Then, about 5 billion years ago, acceleration began. Obviously energy--a lot of it--- was required to explain these phenomena. This is "dark energy." We cannot detect it and currently know almost nothing about it. 

Today scientists believe that 5% of the universe consists of "ordinary" [observable] matter, 23% of "dark" matter and 72% of "dark energy."

Posted by Rebecca Sato with Casey Kazan.

Links:

http://imgsrc.hubblesite.org/hu/db/2005/32/images/a/formats/print.jpg
http://www.ia.ucsb.edu/pa/display.aspx?pkey=1708

The discovery was made by an international team of astronomers led by Raphael Gavazzi and Tommaso Treu of the University of Californi, Santa Barbara. Treu says the odds of seeing such a special alignment are so small that they “hit the jackpot” with this discovery. “When I first saw it I said ‘wow, this is insane!’ I could not believe it!”

But this sight is more than just an incredible novelty. It’s also a very rare phenomenon that can offer insights into dark matter, dark energy, the nature of distant galaxies, and the curvature of the Universe itself. The discovery is part of the ongoing Sloan Lens Advanced Camera for Surveys (SLACS) program.

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 perfectly 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.

“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 Pasaden, California, USA. “The elegance of this lens is trumped only by the secrets of nature that it reveals.”

The dark matter distribution in the foreground galaxies that is warping space to create the Einstein's telescope, the gravitational lens, can be accurately 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.

A sample of several dozen double rings such as this one would offer a purely independent measure of the curvature of space by gravity. This would help in determining what the majority of the Universe is made of, and the properties of dark energy.

Original observations made in 1970 revealed that gravitational motions of gas clouds in the Andromeda galaxy were occurring at speeds far greater than the entire observed mass of that galaxy could account for. Similar problems detected in the 1930's involving motions of entire galaxies had long been disregarded. Later observations confirmed that so-called "ordinary matter" is insufficient to account for observed gravitational effects in the cosmos. Thus the universe must contain huge amounts of "dark matter," that we cannot observe and the composition of which we do not know. 

In 1998 reports of observations of distant supernovae revealed that the expansion of the universe was not slowing, as would be expected from long-term effects of gravity, but was instead accelerating. Something was overcoming the gravitational power of all of the matter in the universe. The acceleration, moreover, has not been present from the Big Bang on. For billions of years the speed of expansion slowed. Then, about 5 billion years ago, acceleration began. Obviously energy--a lot of it--- was required to explain these phenomena. This is "dark energy." We cannot detect it and currently know almost nothing about it. 

Today scientists believe that 5% of the universe consists of "ordinary" [observable] matter, 23% of "dark" matter and 72% of "dark energy."

Posted by Rebecca Sato with Casey Kazan.

Links:

http://imgsrc.hubblesite.org/hu/db/2005/32/images/a/formats/print.jpg
http://www.ia.ucsb.edu/pa/display.aspx?pkey=1708

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[Jump Manual]

The only thing dark matter has in common with normal matter is that it behaves the same way with respect to gravity. Einstein's telescope is the bending of light by objects in space which helps scientist study dark matter.

[the jump manual]

In the cosmic scheme of things, the notion of dark energy is far more startling. Astronomers assumed for decades that our expanding universe was slowing down, only to find out that it's actually accelerating, somehow boosted by the presence of an odd, cosmos-wide pressure. As Gates writes so engagingly, its recent detection was "like finding an elephant on top of a table impeccably set with the finest china and silver . . . We stare in shock at the uninvited guest and demand to know where the elephant came from -- and how it got into [the] room." To find out, astronomers and physicists are exploring many avenues, from carrying out computer simulations to tracing dark energy's effects on the distribution of galaxies throughout the universe. Google is even getting involved, developing a Web portal that will allow astronomers, students and amateurs alike to assess data gathered by a special telescope, poised to regularly scan the entire hemisphere from the Chilean Andes in the next decade.

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Great share thanks for the post! This is good infomation. Now the real question is will be, is this for real?. I want to see this next year. Good post.