Gemini South 

 

The International Gemini Observatory consists of twin 8.1-meter diameter optical/infrared telescopes located on two of the best observing sites on the planet. The Gemini South telescope is located on a mountain in the Chilean Andes called Cerro Pachón, where very dry air and negligible cloud cover make this another prime telescope location. Both of the Gemini telescopes have been designed to excel in a wide variety of optical and infrared capabilities. By incorporating technologies such as laser guide star adaptive optics and multi-object spectroscopy, astronomers in the Gemini partnership explore the universe in unprecedented depth and detail. The Gemini Observatory’s international headquarters is located in Hilo, Hawai‘i at the University of Hawaii Hilo's University Park.

Gemini’s twin telescopes are optimized for observing in the mid-infrared with silver-coated mirrors, an extremely light structure for the secondary, and a light baffle (used when observing in the optical) which can be closed for observing in the infrared.

The Gemini telescopes have a suite of 4 optical and infrared, imagers and spectrographs, mounted on the back of the telescopes at the same time (as well as the acquisition and guidance instruments). This means that switching from one instrument to another takes a matter of minutes to complete before being capable of taking data on the next science target.

Gemini is also unique among other 8-10 meter class observatories in that the telescopes can be operated fully remotely from our base facilities.

For scientists: More details can be found on the science pages.

 

Gemini South

Name(s) Gemini South
Status Operational
Broad Science Goals
  • Twin telescopes in both hemispheres provide participant members with access to the entire sky
  • To provide the best image quality possible from the ground for telescopes of their size.
  • To provide the cleanest possible (i.e., lowest possible emissivity) telescopes, for optimal infrared observing from the ground.

The Gemini Observatory is a world-leader in wide-field adaptive optics assisted infrared imaging, and supports research in almost all areas of astronomy.

Site Cerro Pachón, Chile
Location Coordinates 30º14.5’S
70º44.8’W
Altitude 2737 meters (8980 feet)
Enclosure 46-meter rotating dome
Type Optical/Infrared telescope
Optical Design Ritchey-Chretien Cassegrain
Field of View Maximum 10 arcmin diameter on the bottom port, and 7 arcmin diameter on the side ports due to science fold mirror size. 
Diameter: Primary M1 8.1 meters
Material: Primary M1 Corning Ultra-Low Expansion (ULE) Glass
Diameter: Secondary M2 1.0 meter
Material: Secondary M2  
Mount Alt-azimuth 
First Light Date 2000
Adaptive Optics Gemini Multi-Conjugate Adaptive Optics System (GeMS) with FLAMINGOS-2 and the Gemini South Adaptive Optics Imager (GSAOI) provides uniform, diffraction-limited image quality to arcminute-scale fields of view
Images taken with the Gemini South Link
Images of the Gemini South Link
Videos of the Gemini South Link
Press Releases with the Gemini South  Link

Please help us to complete this page by emailing information and corrections to info@noirlab.edu.