The Giant Magellan Telescope (GMT) just got a nice chunk of change to help develop and test the advanced technologies that will give the future observatory such sharp vision.
The U.S. National Science Foundation (NSF) has awarded a $17.5 million grant to the GMTO Corporation, which is developing the GMT and will operate the big scope once it gets up and running in the Chilean Andes in the late 2020s.
The money, the first awarded to the GMT project by the NSF, “signifies that the observatory will be important for the entire U.S. astronomy community,” GMTO president Robert Shelton told Space.com.
“This award really enables us to accelerate our progress on critical components,” Shelton said. “And I think that it allows us to kind of strut our stuff, to display a little bit the technical skills of the project team, which are manifest.”
The GMT will integrate seven 27.6-foot-wide (8.4 meters) primary mirrors into a single light-collecting surface 80 feet (24.5 m) across — three times wider than any optical telescope operating today. The big scope will also feature seven “adaptive secondary mirrors” (ASMs), each of which will be 3.3 feet (1 m) wide and just 2 millimeters thick, with hundreds of actuators affixed to its back.
“With those [actuators], we’re able to bend this thin glass surface at about 1,000 times every second,” GMTO project manager James Fanson told Space.com. “That is what we use to compensate for the distortion that’s introduced by Earth’s atmosphere. Millisecond by millisecond, we measure the distortion and correct it, so that we can essentially remove the atmosphere above the telescope and get very sharp images.”
These extreme optics will give the GMT 10 times the resolving power of NASA’s famous Hubble Space Telescope, GMT team members have said. Astronomers will use the GMT for a variety of high-impact projects, from hunting for signs of life in the atmospheres of nearby exoplanets to probing the nature of dark matter and dark energy, which dominate the universe but remain largely mysterious.
Making all this happen will be no walk in the park, however. For example, no other single-piece telescope mirror is larger than a GMT primary segment. And the surface of all seven GMT primaries must be shaped nearly to perfection: The margin of error is just 25 nanometers (1 millionth of an inch), about the width of a single glass molecule.
The seven segments must also be “phased” so that they align precisely and perform as a single piece of hardware. The newly awarded NSF money will help the GMT team demonstrate and practice doing just that at two custom-built phasing testbeds, one at the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, and the other at the University of Arizona in Tucson. The grant will…