Two University of Arizona research and development groups were selected to develop and manufacture key technology for the first major undertaking to investigate the mystery of dark energy in the universe.
UA's Imaging Technology Laboratory, a research group within Steward Observatory, and the Optical Fabrication and Engineering Facility at the College of Optical Sciences will provide image recording devices and the heart of the optical system used for imaging, respectively, for the Hobby-Eberly Telescope at the McDonald Observatory, which is operated by the University of Texas, Austin.
The additions are part of outfitting the world's fourth largest optical telescope with an array of new instruments to analyze the light from distant galaxies in an effort to understand the nature of dark energy. Scientists have known for a while that dark energy exists, but so far, nobody has been able to come up with an explanation of what it is.
During the Hobby-Eberly Telescope Dark Energy Experiment, or HETDEX, the telescope will search a large area of the sky that encompasses most of the Big Dipper constellation. This region is far above the plane of the Milky Way galaxy, which is filled with clouds of gas and dust that block the view of distant galaxies. During three years of observations, UA's imaging sensors will collect the faint light from at least one million galaxies that are between nine billion and eleven billion light-years away. The data about their movement, size and precise locations with respect to one another will then be computed into the largest three-dimensional map of the universe ever produced.
The Optical Fabrication and Engineering Facility at the College of Optical Sciences was awarded a $4 million contract to devise and build an extremely complex optical device known as a wide field corrector.
"The wide field corrector broadens the telescope's view into space," explained Martin Valente, who directs the facility, "enabling it to survey vast swaths of the sky in a relatively short amount of time."
Ever since the Big Bang, the universe has been expanding and galaxies are moving away from each other. Galaxies attract each other through their immense gravitational forces, which should slow down the expansion of the universe. Instead, the expansion of the universe has sped up over time. This acceleration is attributed to some unknown force – dark energy – counteracting the galaxies' gravitational pull, causing them to spread out deeper into space.
The map of galaxies produced by the HETDEX survey will allow astronomers to measure how fast the universe was expanding at different times in its history. Changes in the expansion rate will reveal the role of dark energy at different epochs. Various explanations for dark energy predict different changes in the expansion rate, so by providing exact measurements of the expansion, the HETDEX map will eliminate some of the competing ideas.
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