View more articles about

astrophysics

‘Lens’ zooms in on brightest, distant galaxy

U. CHICAGO (US) — A natural “zoom lens” in space offers a uniquely close-up look at the brightest gravitationally magnified galaxy yet discovered.

The imagery provides a visually striking example of gravitational lensing, in which one massive object’s gravitational field can magnify and distort the light coming from another object behind it. Such optical tricks stem from Einstein’s theory of general relativity, which describes how gravity can warp space and time, including bending the path that light travels.

In this case, gravity from the galaxy cluster RCS2 032727-132623 bent and amplified the light coming from a much more distant galaxy, 10 billion light-years from Earth. This “gravitational telescope” creates a vast arc of light, as if the distant galaxy had been reflected in a funhouse mirror. Researchers were able to reconstruct what the distant galaxy really looks like, using computational tools that reversed the effect of gravitational lensing.


This graphic shows a reconstruction (at lower left) of the brightest galaxy, whose image has been distorted by the gravity of a distant galaxy cluster. The small rectangle in the center shows the location of the background galaxy on the sky if the intervening galaxy cluster were not there. The rounded outlines show distinct, distorted images of the background galaxy resulting from lensing by the mass in the cluster. The image at lower left is a reconstruction of what the lensed galaxy would look like in the absence of the cluster, based on a model of the cluster’s mass distribution derived from studying the distorted galaxy images. (Credit: NASA; ESA; J. Rigby, NASA Goddard Space Flight Center; K. Sharon, Kavli Institute for Cosmological Physics; and M. Gladders and E. Wuyts, University of Chicago

[sources]

“What’s happening here is a manifestation of general relativity,” says Michael Gladders, assistant professor in astronomy & astrophysics at the University of Chicago. “Instead of seeing the normal, faint image of that distant source, you see highly distorted, highly magnified, and in this case, multiple images of the source caused by the intervening gravitational mass.”

The cosmic lens gave researchers the unusual opportunity to see what a galaxy looked like 10 billion years ago. The reconstructed image of the galaxy revealed regions of star formation glowing like bright points of light. These are much brighter than any star-formation region in Earth’s home galaxy, the Milky Way.

Looking at the nature of dark matter

In 2006 Chicago astronomers used the Very Large Telescope in Chile to measure the arc’s distance and calculated that the galaxy appears more than three times brighter than previously discovered lensed galaxies. Then last year, Jane Rigby of NASA’s Goddard Space Flight Center in Greenbelt, Md., and the Chicago team imaged the arc with the Hubble Space Telescope’s Wide Field Camera 3.

Using this gravitational lens as a telescope offers two major scientific opportunities, Gladders says. First, “It gives us a look at that very distant source with a precision and fidelity that we couldn’t otherwise achieve.”

And second, it provides an opportunity to learn something about the lens-forming mass, which is dominated by dark matter. “It’s really a way of looking at the nature of dark matter,” Gladders says. Dark matter accounts for nearly 90 percent of all matter in the universe, yet its identity remains one of the biggest mysteries of modern science.

Keren Sharon, a postdoctoral scholar at University of Chicago’s Kavli Institute for Cosmological Physics, led the effort to perform a detailed reconstruction of the lensed galaxy. She and her co-authors, including Gladders, NASA’s Rigby and UChicago graduate student Eva Wuyts, published their findings this month in the Astrophysical Journal.

Sharon painstakingly created a computer reconstruction of the gravitational lens, then reverse-engineered the distorted image to determine the distant galaxy’s actual appearance. “It’s a little bit of an art, but there’s a lot of physics in it. That’s the beauty of it,” Sharon says. “It was a fun puzzle to solve, especially when we had such great data.”

Gladders says Sharon is “one of the world experts on exactly how to do this. Combine that degree of finesse with this quality of data, and you get a very nice result. This object now becomes not only the brightest-lensed source known, but because of this analysis, it is also going to be one of the best-understood sources.”

Through spectroscopy, the spreading out of light into its constituent colors, the team plans to analyze the distant galaxy’s star-forming regions from the inside out to better understand why they are forming so many stars.

The team also has obtained data from one of the twin Magellan Telescopes to help them determine why the galaxy, which is 10 billion light years away, looks so irregular.

“It’s not like we have something to compare it to,” Sharon says. “We don’t know what other galaxies at the same distance look like at this level of detail.”

More news from University of Chicago: www-news.uchicago.edu

Related Articles