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Haystack Observatory

From Wikipedia, the free encyclopedia

Haystack Observatory
The Haystack Radio Telescope at Haystack Observatory
Alternative namesMIT Haystack Observatory Edit this at Wikidata
Organization
Observatory code 254 Edit this on Wikidata
LocationWestford, Massachusetts
Coordinates42°37′24″N 71°29′18″W / 42.6233°N 71.4882°W / 42.6233; -71.4882
Altitude131 m (430 ft) Edit this at Wikidata
Established1960 Edit this on Wikidata
Websitewww.haystack.mit.edu Edit this at Wikidata
Telescopes
Location of Haystack Observatory
 
 Related media on Commons
[edit on Wikidata]

Haystack Observatory is a multidisciplinary radio science center, ionospheric observatory, and astronomical microwave observatory owned by Massachusetts Institute of Technology (MIT).[1] It is in Westford, Massachusetts, in the United States, about 45 kilometers (28 mi) northwest of Boston. The observatory was built by MIT's Lincoln Laboratory for the United States Air Force and was called the Haystack Microwave Research Facility.[2] 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 other universities to operate the site as the Haystack Observatory. As of January 2012, a total of nine institutions participated in NEROC.[3]

The Haystack Observatory site is also the location of the Millstone Hill Geospace Facility, an atmospheric-sciences research center.[4] Lincoln Laboratory continues to use the site, which it calls the Lincoln Space Surveillance Complex (LSSC).[5] The George R. Wallace Astrophysical Observatory of MIT's Department of Earth, Atmospheric, and Planetary Sciences is south of the Haystack dome and east of the Westford dome.[6] The Amateur Telescope Makers of Boston has its clubhouse on the MIT property.[7]

Haystack Vallis on Mercury is named after this observatory.

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Transcription

The observatory started or activity on the hill where the observatory is located started more than 50 years ago back in the mid 1950s when Lincoln Laboratory needed to do work associated with radar. In particular radar for detecting inter- continental ballistic missiles and var- ious things associated with the Cold War. Now in those early days Haystack was built by the Air Force as a communications facility and I was around when it was first dedicated and somebody had a little TV dish and they said, "What are you going to use Haystack for, we can communicate using a communication satellite." And the Air Force at that time said, "Well maybe there's general research work that could be done with Haystack." And that's exactly what happened. A huge, powerful megawatt transmitter was built to do planetary radar; that is to bounce signals off of primarily Venus, Mercury, Mars; so that was the big thing back then and this was in the late 60s early 70s was planetary radar. So now we have multiple facilities. Some of them are Lincoln Laboratory facilities because they maintain a strong presence at the field site and some of them are Haystack Observatory facilities. Since its inception Haystack has been known for the 37-meter antenna: the iconic Haystack Radome but Haystack is a lot more than that. Scientists and engineers here are involved in a wide range of different types of radio science. We have two antennas used for atmospheric science; we also have another smaller radome that contains an 18-meter antenna that is used for geodetic science. Haystack also participates in radio science facilities located around the world, places like Chile and Australia for example. So when people normally thing of an observatory like Haystack Observatory they think of something that operates in wavelengths of light that you can see with because most people are born with a sensor that sees visible light. However here at Haystack we actually look at the universe through a number of different wavelengths that are far outside the range that human senses can directly measure. To do that we need theses things called antennas. They are very large pieces of metal and they act kind of like the lens on a normal telescope in that they focus radio waves in a particular direction down to a point where we can put a piece of electronics that can sense them. For the work we do here at Haystack the antennas have to be very large for two reasons; not only because we're trying to collect very faint radio waves and so we need a very large collecting surface, but also because those waves have a size or a wavelength that's much, much bigger than the normal optical waves that we see by and antennas get bigger or smaller as the wavelength or the size of those waves. So we actually have very large antennas here. One of them is about the size of a soccer field and we use those to sense very small waves that are either generated by the natural environment or that we make by bouncing a very large signal from the ground off the environment and recording the little, faint signal that comes back. At MIT Haystack we are advancing science in many ways. Even the average citizen is able to help us do science with tablets and mobile phones in everyones pocket. So how does it work? We are trying to get to the point where we can image the entire ionosphere of Earth in order to detect interesting phenomena that are either based in space or based on Earth like potentially monitoring tsunamis and earth- quakes. To do that we need people donating us bandwidths and transport data via mobile phones and different sensors. So imagine going from hundreds of sensors to billions of sensors. For myself I find Haystack Observatory to be a wonderfully exciting place to work and a tremendously rewarding place to work because of the people here and the consistant, sustained enthusiasm and sheer competence that exists here. I learned a tremendous amount within six months of walking in the door and that fact alone speaks volumes about what Haystack is and its really remarkable to see that community and the quality of people sharing their knowledge and integrating people into the Haystack culture sustained over decades. And one of the things I am committed to as Director going forward is to make sure that culture and that community continues to thrive because that's ultimately where excellence of the technical and scientific work at the observatory comes from.

Telescopes and radars

Haystack Radio Telescope

Haystack radio telescope at the MIT Haystack Observatory, Westford, MA
Westford Radio Telescope
Millstone Hill Radar

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.[5] 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.[8] 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.[9] The secondary reflector of the Cassegrain design features an active surface.

Haystack Radar operations

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.[10] 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.[11] The HUSIR design allows for tracking object with 0.5 millidegree accuracy.[12] 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).[13]

Haystack Auxiliary Radar

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.[14] It contributes data to the SSN.[10]

Westford Radio Telescope

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.[15] 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).[16] 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.

Event Horizon Telescope

Haystack serves as a computational hub for the Event Horizon Telescope, an assemblage of radio telescopes around Earth that combine data for very-long-baseline interferometry (VLBI) to achieve angular resolution capable of imaging a supermassive black hole's event horizon. Data are transported on large hard drives from the observing telescopes to Haystack, where a cluster of about 800 CPUs run algorithms to produce black hole imagery. The computation has been termed a "silicon lens", as each the data from each telescope is useless by itself and must be computationally combined to produce an image.[17]

Former telescopes

  • The Deuterium Array was a 25-element radio telescope array optimized to observe at 327 MHz, which is one of the emission lines of deuterium. Each element, or station, was itself a 25-element array of dipoles. The array operated from 2004 to 2006.[18]

Millstone Hill Geospace Facility

The Lincoln Laboratory Millstone Hill Radar Observatory, ca. 1958.

Millstone Hill Geospace Facility is a Massachusetts Institute of Technology atmospheric sciences research centre in Westford, Massachusetts, under primary support from the US National Science Foundation's Geospace Facilities section. It is part of Haystack Observatory, a multidisciplinary radio science observatory. 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 68-meter fixed zenith antenna. These radars are capable of measuring a vast array of ionospheric state variables, including electron density, plasma temperature, ion velocity, and ion composition. Data from Millstone Hill is publicly available on the MADRIGAL distributed database, an upper atmosphere data system managed by MIT Haystack.

Millstone Hill Steerable Antenna

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, and was relocated as part of Millstone Hill at the Haystack Observatory complex in 1978. It is primarily used as an upper atmospheric radar observatory using incoherent scatter radar techniques.[19]

Zenith Antenna

The 67 m (220 ft) Zenith antenna was constructed in 1963 to use with the UHF transmitter. The radar transmitter was previously connected to a steerable 84-foot antenna with a UHF horn feed. When the steerable 84' antenna was converted to a higher L-band frequency, the Zenith antenna was connected to the UHF transmitter and was dedicated exclusively to incoherent scatter radar observations of the mid-latitude ionosphere.[20]

Directors

Paul B. Sebring was the Haystack Observatory's director from 1970 to 1980.[21] 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. Colin J. Lonsdale was the director from 1 September 2008 to 31 December 2023. Philip J. Erickson became the new director on 1 January 2024.[22]

See also

Exhibits

The Sun Drawing Exhibit

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.[23][24] "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.[25][26]

References

  1. ^ Whitney, Alan R.; Lonsdale, Colin J.; Fish, Vincent L. (2014). "Insights into the Universe: Astronomy with Haystack's Radio Telescope" (PDF). Lincoln Laboratory Journal. 21 (1): 1–14.
  2. ^ "MIT Haystack Observatory: History". MIT Haystack Observatory. Retrieved 31 January 2012.
  3. ^ "MIT Haystack Observatory: NEROC". MIT Haystack Observatory. Retrieved 31 January 2012.
  4. ^ "MIT Haystack Observatory: Atmospheric Sciences Millstone Hill Observatory". MIT Haystack Observatory. Retrieved 31 January 2012.
  5. ^ a b "MIT Lincoln Laboratory: Facilities". MIT Lincoln Laboratory. Retrieved 31 January 2012.
  6. ^ "Wallace Astrophysical Observatory". MIT Department of Earth, Atmospheric, and Planetary Sciences. Retrieved 31 January 2012.
  7. ^ "ATMoB Clubhouse". Amateur Telescope Makers of Boston. Retrieved 9 May 2017.
  8. ^ Sebring, P. B. (January 1972). "Haystack Observatory, Northeast Radio Observatory Corporation, Westford, Massachusetts. Observatory report covering the period from 1 July 1970 through 30 June 1971". Bulletin of the Astronomical Society. 4: 51. Bibcode:1972BAAS....4...51S.
  9. ^ "MIT Haystack Observatory: Haystack Radio Telescope". MIT Haystack Observatory. Retrieved 31 January 2012.
  10. ^ a b "Millstone-Haystack". FAS. Retrieved 7 May 2015.
  11. ^ Staff (October 2014). "Range-independent Radar". R&D Magazine (Paper). 56 (5): 16. Retrieved 3 June 2016.
  12. ^ "TechNotes - Haystack Ultrawideband Satellite Imaging Radar" (PDF). MIT. Retrieved 7 May 2015.
  13. ^ Czerwinski, Mark G.; Usoff, Joseph M. (2014). "Development of the Haystack Ultrawideband Satellite Imaging Radar" (PDF). Lincoln Laboratory Journal. 21 (1). MIT.
  14. ^ "MIT Lincoln Laboratory: Facilities". MIT Lincoln Laboratory. Retrieved 7 May 2015.
  15. ^ "MIT Haystack Observatory: Westford Radio Telescope". MIT Haystack Observatory. Retrieved 31 January 2012.
  16. ^ "Network Station Configuration File". International VLBI Service. Retrieved 31 January 2012.[permanent dead link]
  17. ^ Mearian, Lucas (18 August 2015). "Massive telescope array aims for black hole, gets gusher of data". Computerworld. Retrieved 29 April 2020.
  18. ^ "MIT Haystack Observatory: Deuterium Array". MIT Haystack Observatory. Retrieved 31 January 2012.
  19. ^ "MIT Haystack Observatory: Millstone Hill Radar MISA Antenna". MIT Haystack Observatory. Retrieved 7 May 2015.
  20. ^ "MIT Haystack Observatory: Millstone Hill Radar Zenith Antenna". MIT Haystack Observatory. Retrieved 7 May 2015.
  21. ^ Sebring, P. B.; Leslie, B. G. (1980). "Haystack Observatory". Bulletin of the American Astronomical Society. 12: 126–128. Bibcode:1980BAAS...12..126S.
  22. ^ "Philip Erickson named director of MIT Haystack Observatory". MIT News. 15 December 2023.
  23. ^ Saad-Cook, Janet (25 May 2006). "Global Sun Drawing". www.janetsaadcook.com. Archived from the original on 28 January 2016. Retrieved 28 February 2016.
  24. ^ Saad-Cook, Janet (1995). "Sun Art - Sun Drawings". www.haystack.mit.edu. Retrieved 28 February 2016.
  25. ^ "Sun Drawings". www.haystack.mit.edu. MIT Haystack Observatory. Retrieved 28 February 2016.
  26. ^ Star Dust, Vol II #11 (June 1991). "Janet Saad-Cook to Discuss VLA Sun Drawing Project" (PDF). www.capitalastronomers.org. National Capital Astronomers, Inc. Retrieved 28 February 2016.{{cite web}}: CS1 maint: numeric names: authors list (link)

External links

This page was last edited on 31 January 2024, at 18:49
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