VLA at Sunrise
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VLA at Sunrise

July 13, 2010
The Very Large Array (VLA) radio telescope at sunrise. The VLA is a collection of 27 radio antennas located at the National Radio Astronomy Observatory site in Socorro, N.M. Each antenna in the array measures 25 meters (82 feet) in diameter and weighs about 230 tons. The Y-shaped array can be arranged into 4 different configurations: A, B, C, or D, depending on the distance between the antennas. The VLA is an interferometer, which means that the data from each antenna can be combined electronically so that the array effectively functions as one giant antenna. Dedicated in 1980, the VLA is used by astronomers from around the world to study everything from black holes to planetary nebulae. For more information, please visit the VLA Web site. More about this Image Astronomers recently used the NSF's Very Large Array (VLA) radio telescope (above) to help find the most distant water yet seen in the Universe, in a galaxy more than 11 billion light-years from Earth. Previously, the most distant water had been seen in a galaxy less than 7 billion light-years from Earth. The soggy galaxy is dubbed MG J0414+0534. In a region near its core, water molecules are acting as masers, the radio equivalent of lasers, to amplify radio waves at a specific frequency. The water molecules showed themselves with a tell-tale radio "fingerprint." The first indication came from the giant, 100-meter-diameter radio telescope in Effelsberg, Germany, and scientists confirmed the discovery using the VLA. The astronomers say their finding indicates that such giant, water masers were more common in the early Universe than they are today. MG J0414+0534 is seen as it was when the Universe was roughly one-sixth of its current age. At the galaxy's great distance, even the strengthening of the radio waves by the masers would not by itself have made them strong enough to detect with the radio telescopes. However, the scientists got help from nature in the form of another galaxy, nearly 8 billion light-years away, located directly in the line of sight from MG J0414+0534 to Earth. That foreground galaxy's gravity served as a lens to further brighten the more distant galaxy and make the emission from the water molecules visible to the radio telescopes. "We were only able to discover this distant water with the help of the gravitational lens," said Violette Impellizzeri, an astronomer with the Max-Planck Institute for Radio Astronomy (MPIfR) in Bonn, Germany. Water masers have been found in numerous galaxies at closer distances. Typically, they are thought to arise in disks of molecules closely orbiting a super-massive black hole at the galaxy's core. The amplified radio emission is more often observed when the orbiting disk is seen nearly edge-on. However, the astronomers said MG J0414+0534 is oriented with the disk almost face-on as seen from Earth. "This may mean that the water molecules in the masers we're seeing are not in the disk, but in the superfast jets of material being ejected by the gravitational power of the black hole," explained John McKean, also of MPIfR. [Story written for LiveScience by Dave Finley, NRAO/AUI/NSF] (Date of Image: 2008)

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