Giant Magellan Telescope

The University of Arizona, in collaboration with a number of top US universities and international partners, is in the process of constructing a telescope that is much size than any existing optical/infrared telescope. The gain in collecting area or "aperture" leads to unprecedented gains in sensitivity, and, with the application of adaptive optics, gains in resolution - allowing the Giant Magellan Telescope to see farther and smaller objects than ever before. Steward Observatory plays a critical role in the project both by fabricating the large primary mirror segments and having generated the initial concept study for the telescope. Additionally, we continue to be actively involved in the development of the adaptive optics and instrumentation plans.

Giant Magellan Telescope

The Giant Magellan Telescope (GMT) will be one of the next class of super giant earth-based telescopes. It will be located at the Las Campanas Observatory in Chile. The GMT project is the work of an international consortium of universities and science institutions - including the University of Arizona.

Location Specifications

Longtitude

-70.6922

Latitude

-29.0150

Elevation

8254 ft.

Telescope Specifications

Aperture

8.4 m per mirror

Focal Length  

18 m (M1), 202.745 m (M1+M2)

Mount

Altitude/Azimuth

Additional Information on telescope specifications

Additional information regarding optical specifications

Instruments

GMTNIRS

The High Resolution Near-IR Spectrograph for the Giant Magellan Telescope

MIISE

A Mid-Infrared Imaging Spectrograph for the GMT

NIRMOS

Near Infrared Multiple Object Spectrograph

GMACS

The GMT Wide-Field Optical Spectrograph

Additional information regarding science operations