Haystack Observatory is an astronomical observatory owned by Massachusetts Institute of Technology (MIT). It is located in Westford, Massachusetts (US), approximately 45 kilometers (28 mi) northwest of Boston. Haystack was initially built by MIT's Lincoln Laboratory for the United States Air Force and was known as Haystack Microwave Research Facility. Construction began in 1960, and the antenna began operating in 1964. In 1970 the facility was transferred to MIT, which then formed the Northeast Radio Observatory Corporation (NEROC) with a number of other universities to operate the site as the Haystack Observatory. As of January 2012[update], a total of nine institutions participated in NEROC.
The Haystack Radio Telescope at Haystack Observatory
|Alternative names||MIT Haystack Observatory|
|Organization||Massachusetts Institute of Technology|
|Altitude||131 m (430 ft)|
|Telescopes||Haystack Radio Telescope|
Westford Radio Telescope
Millstone Hill Observatory
|Related media on Wikimedia Commons|
The Haystack Observatory site is also the location of the Millstone Hill Observatory, an atmospheric sciences research center. Lincoln Laboratory continues to use the site, which it calls the Lincoln Space Surveillance Complex (LSSC). The George R. Wallace Astrophysical Observatory of MIT's Department of Earth, Atmospheric, and Planetary Sciences is located south of the Haystack dome and east of the Westford dome. The Amateur Telescope Makers of Boston has its clubhouse on the MIT property.
Telescopes and radarsEdit
Haystack Radio TelescopeEdit
The 37 m (121 ft) Haystack Radio Telescope is a parabolic antenna protected by a 46 m (151 ft) metal-frame radome. It is known as the Haystack Long-Range Imaging Radar (LRIR) or Haystack Ultrawideband Satellite Imaging Radar (HUSIR) when used for the LSSC. It was constructed for use in space tracking and communication, but now is used primarily for astronomy. It was completed in 1964 and originally observed at 8 GHz on the radio spectrum. Since then it has been upgraded to listen to other frequency bands, though not simultaneously. When used for radar it broadcasts and listens in bands at either 10 GHz or 95 GHz. The main dish was upgraded in 2006, which allowed operation at frequencies up to 150 GHz. The secondary reflector of the Cassegrain design features an active surface.
Haystack Radar operationsEdit
The Long-Range Imaging Radar (LRIR) system was originally designed to function as an X-band long-range imaging radar. In wideband mode, LRIR runs at 10 GHz with a 1.024 GHz bandwidth. The system was capable of sensitivity of 25 cm resolution, allowing for tracking and imaging satellites out to geostationary orbit distances, as well as deep space objects out to 40,000 km (130,000,000 ft) range. The radar was upgraded with a completely new antenna capable of dual-band operations, called Haystack Ultrawideband Satellite Imaging Radar (HUSIR). The system is capable of simultaneous operations in X band and W-band, which allows it to better determine the size, shape, orientation, and motion of orbiting objects. The HUSIR design allows for tracking object with 0.5 millidegree accuracy. The W-band operates between 92 and 100 GHz, with a bandwidth of 8 GHz. The system contributes data to the United States Space Surveillance Network (SSN).
Haystack Auxiliary RadarEdit
The Haystack Auxiliary Radar (HAX) is Ku-band system with a 40 ft (12 m) dish antenna. It was constructed in 1993 to augment the LSSC imaging and data collections space debris. It contributes data to the SSN.
Westford Radio TelescopeEdit
The 18.3 m (60 ft) Westford Radio Telescope was built in 1961 by Lincoln Laboratory for Project West Ford as an X-band radar antenna. It is located approximately 1.2 kilometers (0.75 mi) south of the Haystack telescope along the same access road. The antenna is housed in a 28.4 m (93 ft) radome and has an elevation-azimuth mount. Since 1981, it has been used primarily for geodetic very long baseline interferometry (VLBI). By measuring the location of astronomical radio sources very accurately, geodetic VLBI techniques can be used to measure things such as changes in the axial tilt of the Earth.
Millstone Hill ObservatoryEdit
Millstone Hill Observatory is a Massachusetts Institute of Technology atmospheric sciences research centre in Westford, Massachusetts. It is part of Haystack Observatory, which focuses primarily on radio astronomy. Millstone Hill is the location for two of the most well-known incoherent scatter radars in the world. These include a fully steerable 46-meter antenna called Millstone Hill Steerable Antenna (MISA), and a 67-meter fixed-zenith antenna. These radars are capable of measuring a vast array of ionospheric components, including temperature, ion concentrations and solar wind data. Data from Millstone Hill is publicly available on the MADRIGAL database, an upper atmosphere data system managed by MIT Haystack.
Millstone Hill Steerable AntennaEdit
The Millstone Hill Steerable Antenna (MISA) is a 46 m (151 ft) fully steerable UHF antenna. Built in 1963, the system was initially installed at the Sagamore Hill Air Force facility in Hamilton, Massachusetts, relocated in Millstone Hill in 1978. It is primarily used as a space surveillance system using incoherent scatter radar techniques.
The 67 m (220 ft) Zenith antenna was constructed in 1963 to use with the UHF transmitter. The radar system has been previously connected to another steerable 84-foot antenna. When the steerable antenna that was converted to L-band, the Zenith system was dedicated exclusively to incoherent scatter observations.
Paul B. Sebring was the Haystack Observatory's director from 1970 to 1980. From 1980 to 1983 John V. Evans was the director. Joseph E. Salah was the director from 1983 to 2006, Alan R. Whitney was the interim director from 2006 to 2008, and Colin J. Lonsdale became the director on 1 September 2008.
The Sun Drawing ExhibitEdit
The Sun Drawing art exhibit at the Haystack Observatory was conceived and developed as part of the Global Sun Drawing Project by visual artist Janet Saad-Cook. "Sun Drawings" are projected images created by reflecting sunlight from a variety of materials that are strategically positioned to relate to their specific location on earth. The reflections change shape and color in relation to the position of the sun, creating a four-dimensional artwork of varying reflections throughout the day and year. Similar installations for the Global Sun Drawing Project have been planned at other astronomically significant locations worldwide, including an exhibit at the Karl G. Jansky Very Large Array in New Mexico.
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- Saad-Cook, Janet (25 May 2006). "Global Sun Drawing". www.janetsaadcook.com. Retrieved 28 February 2016.
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