Jump to content

Heinrich Hertz Submillimeter Telescope

Coordinates: 32°42′05.8″N 109°53′28.48″W / 32.701611°N 109.8912444°W / 32.701611; -109.8912444
From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Look2See1 (talk | contribs) at 09:59, 11 December 2015 (External links). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Heinrich Hertz Submillimeter Telescope
The SMT at night
Alternative namesSubmillimeter Telescope Edit this at Wikidata
Part ofEvent Horizon Telescope
Mount Graham International Observatory Edit this on Wikidata
Location(s)Arizona
Coordinates32°42′06″N 109°53′28″W / 32.701611°N 109.891244°W / 32.701611; -109.891244 Edit this at Wikidata
OrganizationArizona Radio Observatory
WavelengthSubmillimeter
Telescope styleradio telescope Edit this on Wikidata
Diameter10m
Secondary diameter0.69 m (2 ft 3 in) Edit this at Wikidata
Mass44.76 t (44,760 kg) Edit this at Wikidata
Collecting area~75m2
Focal lengthf/.35
MountingAltazimuth
Websitehttp://aro.as.arizona.edu/
Heinrich Hertz Submillimeter Telescope is located in the United States
Heinrich Hertz Submillimeter Telescope
Location of Heinrich Hertz Submillimeter Telescope
  Related media on Commons

The Submillimeter Telescope (SMT), formerly known as the Heinrich Hertz Submillimeter Telescope, is a submillimeter wavelength radio telescope located on Mount Graham, Arizona. It is a 10-meter-wide parabolic dish inside a building to protect it from bad weather. The building front doors and roof are opened when the telescope is in use. The telescope's construction was finished in 1993. Along with the 12 Meter Telescope on Kitt Peak, this telescope is maintained by the Arizona Radio Observatory, a division of Steward Observatory at the University of Arizona.

The dryness of the air around and above Mt. Graham is particularly vital for EHF (extremely short wavelength radio) and far-infrared observations - a region of the spectrum where the electromagnetic waves are strongly attenuated by any water vapor or clouds in the air.

This telescope is used nine-to-ten months of the year, and it is stowed only when there is too much water vapor in the atmosphere, primarily during the summertime. This telescope is one of the telescopes that makes up Mount Graham International Observatory.

Other MGIO Facilities

See also


32°42′05.8″N 109°53′28.48″W / 32.701611°N 109.8912444°W / 32.701611; -109.8912444{{#coordinates:}}: cannot have more than one primary tag per page