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UChicago Commits $50M to GMT

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CHICAGO, July 23, 2010 — The University of Chicago will provide millions of dollars to the Giant Magellan Telescope (GMT) project, joining an effort to build the world’s largest telescope. The GMT, to be built in Chile, is set to eclipse the image quality of even the Hubble Space Telescope, as the quest continues for answers to some of the deepest mysteries of modern cosmology. The ground-based optical telescope will produce images of objects 100 times fainter than the Hubble can detect.

“The University of Chicago’s department of astronomy and astrophysics is among the best astronomy and astrophysics departments in the country and worldwide,” said Wendy Freedman, director of the Carnegie Observatories and chairperson of the GMT Organization. “This is exactly the kind of partner we need to make this ambitious telescope project a success.”

(Image: Giant Magellan Telescope - GMTO Corp.)

The other founding GMT partners are the Carnegie Institution for Science, University of Texas at Austin, Harvard University, Australian National University, Smithsonian Astrophysical Observatory, University of Arizona, Texas A&M University, Astronomy Australia Ltd., and the Korea Astronomy and Space Science Institute. Construction of the GMT will begin at Las Campanas Observatory, Chile, in 2012 and will take approximately seven years to complete.

“Chicago has a great tradition in exploring the universe,” said Robert Kirshner, Harvard’s Clowes Professor of Science. “At the founding of the university, Chicago built the world’s largest telescope at Yerkes; Chicago trained Edwin Hubble, the leading astronomer of the 20th century; and now they’re looking to be leaders in the field for the 21st century.”

The University of Chicago also has committed $14 million to joining the related consortium that currently operates the twin 6.5-m Magellan telescopes at Las Campanas. These arrangements guarantee that university scientists will receive a share of observing time on the telescopes, a critical component of pioneering cosmological research.

“The twin Magellan telescopes give our astronomers immediate access to some of the best optical telescopes in the world,” said Edward Kolb, chairman of the University of Chicago’s department of astronomy and astrophysics. “We’re looking to make great discoveries with the Magellan telescopes. They will be the workhorses of the department in optical astronomy for the next 10 years.”

These telescopes are necessary tools for prying loose answers to the mysteries of dark energy and dark matter, two of the biggest questions confronting modern cosmologists, Kolb said. Dark energy is a repulsive force of unknown origin that is accelerating the expansion of the universe. Dark matter is a material of unknown composition that is far more plentiful in the universe than the ordinary matter of everyday life. Theories and observations have convinced most cosmologists that dark energy and dark matter exist in huge amounts, but their precise nature has remained elusive.

The Magellan telescopes will complement University of Chicago research at the South Pole Telescope and in the Dark Energy Survey.

“Even now, the South Pole Telescope is discovering sources that are being followed up by observations at the Magellan telescopes,” Kolb said. “The important thing for the department is to have not just one facility, but an array of these different facilities to do the science that we want to do.”

Beyond the next decade, University of Chicago astronomers will turn to the next-generation GMT to make their optical observations. In addition to carrying out research on dark energy and dark matter, the GMT will be able to search for planets around stars other than the sun. “This is part of the goal of looking for Earthlike planets around other stars that could be the sites for life,” Kolb said. “This is one of the new avenues that the Giant Magellan Telescope will open, in addition to being able to look at the sky with unprecedented resolution and light-gathering power.”

The $700 million GMT will combine seven 8.4-m primary mirror segments into the equivalent of a 24.5-m telescope. The first mirror, now under development at the Steward Observatory Mirror Lab at the University of Arizona, will be completed later this year.

The University of Chicago has a deep historical link to the Carnegie Observatories through its founder, George Ellery Hale (1868-1938). Hale founded the university’s department of astronomy and astrophysics in the 1890s and became the founding director of Yerkes Observatory in Williams Bay, Wis., in 1897. A Chicago native, Hale later founded the Mount Wilson and Palomar observatories, today known as the Carnegie Observatories, in Southern California.

“Hale spent a great part of his life and career building the biggest telescopes in the world at that time,” Freedman said. “He started out at Chicago doing just that, and he ended up at Carnegie continuing to do that. So the idea that both institutions would come together in the future, I suspect, would really please him.”

For more information, visit:
Jul 2010
The scientific observation of celestial radiation that has reached the vicinity of Earth, and the interpretation of these observations to determine the characteristics of the extraterrestrial bodies and phenomena that have emitted the radiation.
AmericasAsia-PacificastronomyAstronomy Australia Ltd.astrophysicsAustralian National UniversityBasic ScienceBusinessCarnegie Institution for ScienceCarnegie ObservatoriesChiledark energyDark Energy Surveydark matterEdward KolbGeorge Ellery HaleGiant Magellan TelescopeGMTHarvard UniversityHubble Space TelescopeIllinoisimagingKorea Astronomy and Space Science InstituteLas Campanas ObservatoryMagellan TelescopesMassachusettsmirrorsopticsResearch & TechnologyRobert KirshnerSmithsonian Astrophysical ObservatorySouth Pole telescopeSteward Observatory Mirror LabTexas A&M UniversityUniversity of ArizonaUniversity of ChicagoUniversity of Texas at AustinWendy FreedmanYerkes Observatory

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