This article has multiple issues. Please helpimprove it or discuss these issues on thetalk page.(Learn how and when to remove these messages) (Learn how and when to remove this message)
|
Entrance to the Fred Lawrence Whipple Observatory | |||||||||||||||
| Alternative names | The Mount Hopkins Observatory | ||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Named after | Fred Lawrence Whipple | ||||||||||||||
| Observatory code | G91, 696 | ||||||||||||||
| Location | Mount Hopkins,Amado,Mount Hopkins, United States | ||||||||||||||
| Coordinates | 31°40′52″N110°52′41″W / 31.6811°N 110.878°W /31.6811; -110.878 | ||||||||||||||
| Altitude | 2,606 m (8,550 ft) | ||||||||||||||
| Established | 1968 | ||||||||||||||
| Website | linmax | ||||||||||||||
| Telescopes | |||||||||||||||
| |||||||||||||||
![]() | |||||||||||||||
| | |||||||||||||||
TheFred Lawrence Whipple Observatory is an Americanastronomicalobservatory owned and operated by theSmithsonian Astrophysical Observatory (SAO); it is their largest field installation outside of their main site inCambridge, Massachusetts. It is located nearAmado, Arizona on the summit ofMount Hopkins.
Research activities include imaging and spectroscopy of extragalactic, stellar, solar system and extra-solar bodies, as well asgamma-ray andcosmic-ray astronomy.
In 1966, roadwork began at the site with funding granted for theSmithsonian Mt. Hopkins Observatory. The Whipple 10-meter gamma-ray telescope was constructed in 1968.
Formerly known as the Mount Hopkins Observatory, the observatory was renamed in late 1981 in honor ofFred Lawrence Whipple, a planetary expert, space science pioneer, and director emeritus of SAO, under whose leadership the Arizona facility was established.[1]

Whipple observatory hosts theMMT Observatory, which is jointly run by SAO and theUniversity of Arizona and houses a 6.5-meter telescope. The observatory also has 1.5- and 1.2-meter reflectors and a second 1.3-meter reflector named PAIRITEL (Peters Automated IR Imaging Telescope, ex-2MASS ). Also on site is theHATNet (Hungarian-made Automated Telescope) network, theMEarth Project, and four 0.7-meter telescopes of the automatedMiniature Exoplanet Radial Velocity Array (MINERVA).
The observatory is known for its pioneering work in ground-based gamma-ray astronomy through the development of theImaging Atmospheric Cherenkov Technique (IACT) with the Whipple 10-meter Telescope during the early 1980s. The Whipple 10-meter is currently preparing to be decommissioned after forty years of service.
In April 2007,VERITAS (a system of 4 IACT telescopes with 12-meter reflectors) started full operations at the FLWO basecamp. Subsequently, in September 2009, after a 4-month effort, one of the telescopes was moved to a new position, making the array symmetric and increasing its sensitivity.