![]() The observatory on the campus of the University of Arizona in Tucson | |||||||||||
Organization | University of Arizona | ||||||||||
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Observatory code | 692 ![]() | ||||||||||
Location | Tucson, Arizona | ||||||||||
Coordinates | 32°14′00″N110°56′56″W / 32.2333°N 110.9490°W | ||||||||||
Altitude | 792 meters (2,598 ft) | ||||||||||
Established | 1916 | ||||||||||
Website | Steward Observatory | ||||||||||
Telescopes | |||||||||||
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Steward Observatory is the research arm of the Department of Astronomy at the University of Arizona (UArizona). Its offices are located on the UArizona campus in Tucson, Arizona (US). Established in 1916, the first telescope and building were formally dedicated on April 23, 1923. It operates, or is a partner in telescopes at five mountain-top locations in Arizona, one in New Mexico, one in Hawaii, and one in Chile. It has provided instruments for three different space telescopes and numerous terrestrial ones. Steward has one of the few facilities in the world that can cast and figure the very large primary mirrors used in telescopes built in the early 21st century.
Steward Observatory owes its existence to the efforts of American astronomer and dendrochronologist Andrew Ellicott Douglass. In 1906, Douglass accepted a position as Assistant Professor of Physics and Geography at the University of Arizona in Tucson, Arizona. Almost immediately upon his arrival in Tucson, Douglass established astronomical research programs using an 8-inch refracting telescope on loan from the Harvard College Observatory and actively began to pursue funding to construct a large research-class telescope in Tucson. Over the next 10 years, all of Douglass’ efforts to secure funding from the University and the Arizona Territorial (and later State) Legislatures ended in failure. During this time period, Douglass served UArizona as Head of the Dept. of Physics and Astronomy, Interim President, and finally Dean of the College of Letters, Arts, & Sciences. [1]
Then on October 18, 1916, University President Rufus B. von KleinSmid announced that an anonymous donor had given the University $60,000 “…to be used to buy a telescope of huge size.” That donor was later revealed to be Mrs. Lavinia Steward of Oracle, Arizona. Mrs. Steward was a wealthy widow who had an interest in astronomy and a desire to memorialize her late husband, Mr. Henry Steward. [2] Douglass made plans to use the Steward gift to construct a 36-inch diameter Newtonian reflecting telescope. The Warner & Swasey Company of Cleveland, Ohio was contracted to build the telescope, but the United States entry into World War I delayed the contract since Warner & Swasey had war contracts that took priority. The situation was further delayed by the fact that up until this time, the expertise in large telescope mirror making was in Europe. The war made it impossible to contract with a European company. So Douglass had to find an American glass company that was willing to develop this expertise. After a couple of failed castings, the Spencer Lens Co. of Buffalo, New York ultimately produced a 36-inch mirror for the Steward Telescope. [1]
The telescope was finally installed in the observatory building in July 1922, and the Steward Observatory was officially dedicated on April 23, 1923. In his dedication address, Douglass recounted the trials and tribulations of establishing the observatory, then gave the following eloquent justification for the scientific endeavor: [3]
In concluding I wish to leave with you a more general view. This installation is to be devoted to scientific research. Scientific research is business foresight on a large scale. It is knowledge obtained before it is needed. Knowledge is power, but we cannot tell which fact in the domain of knowledge is the one which is going to give the power, and we therefore develop the idea of knowledge for its own sake, confident that some one fact or training will pay for all the effort. This I believe is the essence of education wherever such education is not strictly vocational. The student learns many facts and has much training. He can only dimly see which fact and which training will be of eminent use to him, but some special part of his education will take root in him and grow and pay for all of the effort which he and his friends have put into it. So it is with the research institutions. In this Observatory I sincerely hope and expect that the boundaries of human knowledge will be advanced along astronomical lines. Astronomy was the first science developed by our primitive ancestors thousands of years ago because it measured time. Performing that same function, it has played a vast part in human history, and today it is telling us facts, forever wonderful, about the size of our universe; perhaps tomorrow it will give us practical help in showing us how to predict climatic conditions in the future.
Steward Observatory manages three different observing locations in southern Arizona: Mount Graham International Observatory (MGIO), Mount Lemmon Station, and Catalina Station on Mount Bigelow. It also operates telescopes at two additional important observatories: Kitt Peak National Observatory (KPNO) and Fred Lawrence Whipple Observatory on Mount Hopkins. Steward is a partner in the Sloan Digital Sky Survey-III, which is located in New Mexico at Apache Point Observatory. Steward used to maintain a student observatory on Tumamoc Hill approximately 5 kilometers (3.1 mi) west of the campus, but that is no longer in operation. The original observatory dome in Tucson now houses the Ray White Jr. 21-inch telescope and is used for public outreach and undergraduate education.
The Arizona Radio Observatory, a part (sub-unit) of Steward Observatory, operates the SMT 10m diameter millimeter-wavelength radio telescope on Mount Graham and UArizona 12m diameter millimeter-wavelength radio telescope on Kitt Peak.
Steward Observatory participates in many partnered projects. It is a full member in the twin Magellan Telescopes located at Las Campanas Observatory in northern Chile. It is also a member in organizations that originated two projects planned for same region: the Large Synoptic Survey Telescope, now the Vera Rubin Observatory, and the Giant Magellan Telescope, a next generation extremely large telescope. The Richard F. Caris Mirror Laboratory completed the primary and tertiary mirrors for LSST and is fabricating the primary mirror segments, each 8.4m in diameter, for the GMT.
The Richard F. Caris Mirror Lab, located under the east side of Arizona Stadium, has pioneered new techniques of large mirror production, including spin-casting lightweight honeycomb mirrors in a rotating furnace, and stressed-lap polishing. The Mirror Laboratory completed the second mirror for the Large Binocular Telescope in September, 2005. The Mirror Lab also cast the 8.4 meter diameter primary/tertiary mirror for the Large Synoptic Survey Telescope, and has cast the central mirror and five of the seven off-axis primary mirrors for the Giant Magellan Telescope. [4] [5]
The Infrared Detector Laboratory built the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) instrument for the Hubble Space Telescope and the Multiband Imaging Photometer (MIPS) instrument for the Spitzer Space Telescope. For the James Webb Space Telescope, Steward built the Near-Infrared Camera (NIRCam) and helped build the Mid-IR Instrument (MIRI). [6]
Other groups include the Center for Astronomical Adaptive Optics (CAAO), the Imaging Technology Laboratory (ITL), the Steward Observatory Radio Astronomy Laboratory (SORAL), the Earths in Other Solar Systems (EOS) group, and the Astrochemistry/Spectroscopy Laboratory.
The Kitt Peak National Observatory (KPNO) is a United States astronomical observatory located on Kitt Peak of the Quinlan Mountains in the Arizona-Sonoran Desert on the Tohono Oʼodham Nation, 88 kilometers (55 mi) west-southwest of Tucson, Arizona. With more than twenty optical and two radio telescopes, it is one of the largest gatherings of astronomical instruments in the Earth's northern hemisphere.
Lowell Observatory is an astronomical observatory in Flagstaff, Arizona, United States. Lowell Observatory was established in 1894, placing it among the oldest observatories in the United States, and was designated a National Historic Landmark in 1965. In 2011, the Observatory was named one of "The World's 100 Most Important Places" by Time Magazine. It was at the Lowell Observatory that the dwarf planet Pluto was discovered in 1930 by Clyde Tombaugh.
The Large Binocular Telescope (LBT) is an optical telescope for astronomy located on 10,700-foot (3,300 m) Mount Graham, in the Pinaleno Mountains of southeastern Arizona, United States. It is a part of the Mount Graham International Observatory.
Yerkes Observatory is an astronomical observatory located in Williams Bay, Wisconsin, United States. The observatory was operated by the University of Chicago Department of Astronomy and Astrophysics from its founding in 1897 until 2018. Ownership was transferred to the non-profit Yerkes Future Foundation (YFF) in May 2020, which began millions of dollars of restoration and renovation of the historic building and grounds. Yerkes re-opened for public tours and programming in May 2022. The April 2024 issue of National Geographic magazine featured a story about the Observatory and ongoing work to restore it to relevance for astronomy, public science engagement and exploring big ideas through art, science, culture and landscape. The observatory offers tickets to programs and tours on its website.
The Mount Wilson Observatory (MWO) is an astronomical observatory in Los Angeles County, California, United States. The MWO is located on Mount Wilson, a 5,710-foot (1,740-meter) peak in the San Gabriel Mountains near Pasadena, northeast of Los Angeles.
The National Optical Astronomy Observatory (NOAO) was the United States national observatory for ground-based nighttime ultraviolet-optical-infrared (OUVIR) astronomy. The National Science Foundation (NSF) funded NOAO to provide forefront astronomical research facilities for US astronomers. Professional astronomers from any country in the world could apply to use the telescopes operated by NOAO under the NSF's "open skies" policy.
Aden B. Meinel was an American astronomer. He retired in 1993 as a distinguished scientist at the Jet Propulsion Laboratory. He also held the rank of professor emeritus at the University of Arizona College of Optical Sciences. His research interests have included upper atmospheric physics, glass technology, optical design, instrumentation and space systems.
The MDM Observatory is an optical astronomical observatory located adjacent to Kitt Peak National Observatory on Kitt Peak, west of Tucson, Arizona, in the United States. It is owned and operated by the University of Michigan, Dartmouth College, Ohio State University, Columbia University, and Ohio University. The Massachusetts Institute of Technology (MIT) was also part of the operating consortium in the past.
Perkins Observatory is an astronomical observatory in Delaware, Ohio. It is owned and operated by Ohio Wesleyan University.
The Giant Magellan Telescope (GMT) is a ground-based, extremely large telescope currently under construction at Las Campanas Observatory in Chile's Atacama Desert. With a primary mirror diameter of 25.4 meters, it is expected to be the largest Gregorian telescope ever built, observing in optical and mid-infrared wavelengths. Commissioning of the telescope is anticipated in the early 2030s.
The Alice P. Lennon Telescope and its Thomas J. Bannan Astrophysics Facility, known together as the Vatican Advanced Technology Telescope (VATT), is a Gregorian telescope observing in the optical and infrared situated on Mount Graham in southeast Arizona, United States. Measuring 1.83 m wide, the telescope achieved its first light in 1993.
The MMT Observatory (MMTO) is an astronomical observatory on the site of Fred Lawrence Whipple Observatory. The Whipple observatory complex is located on Mount Hopkins, Arizona, US in the Santa Rita Mountains. The observatory is operated by the University of Arizona and the Smithsonian Institution, and has a visitor center in nearby Amado, Arizona. The MMTO is the home of the MMT, which has a primary mirror 6.5 m in diameter. The name comes from the six smaller mirrors originally used before the single primary mirror was installed in 1998. The primary mirror has a special lightweight honeycomb design made by the University of Arizona's Steward Observatory Mirror Laboratory. The MMT is housed in a building which allows the walls and roof around the telescope to be completely rolled back, allowing it to cool down very quickly in order to improve observation.
The Warner and Swasey Observatory is the astronomical observatory of Case Western Reserve University. Named after Worcester R. Warner and Ambrose Swasey, who built it at the beginning of the 20th century, it was initially located on Taylor Road in East Cleveland, Ohio, USA. The observatory, which at that time housed a 9.5-inch (24 cm) refractor, was donated in 1919 to the Case School of Applied Science. The newer 24-inch (61 cm) Burrell Schmidt telescope was built in 1939.
Mount Lemmon Observatory (MLO), also known as the Mount Lemmon Infrared Observatory, is an astronomical observatory located on Mount Lemmon in the Santa Catalina Mountains approximately 28 kilometers (17 mi) northeast of Tucson, Arizona (US). The site in the Coronado National Forest is used with special permission from the U.S. Forest Service by the University of Arizona's Steward Observatory, and contains a number of independently managed telescopes.
The ARO 12m Radio Telescope is a 12-meter dish located on Kitt Peak, approximately 60 mi (97 km) from Tucson in Arizona at an elevation of 6,215.8 ft (1,894.6 m).
Astronomy Camp is a science summer camp hosted by the University of Arizona's Alumni Association, and run by astronomer Don McCarthy. Many of the early camps took place at the Mount Lemmon Station Observatory atop Mount Lemmon, near Tucson, Arizona. On Mount Lemmon, the campers have access to a 12-inch (30 cm), 20-inch, 40-inch and 60-inch telescope, and on the nearby Mount Bigelow site, a 61-inch (150 cm) telescope.
A. E. Douglass was an American astronomer. He discovered a correlation between tree rings and the sunspot cycle, and founded the discipline of dendrochronology, which is a method of dating wood by analyzing the growth ring pattern. He started his discoveries in this field in 1894 when he was working at the Lowell Observatory. During this time he was an assistant to Percival Lowell, but fell out with him when his experiments made him doubt the existence of artificial "canals" on Mars and visible spokes on Venus.
Catalina Station (CS), also known as Steward Observatory Catalina Station, is an astronomical observing facility located on Mount Bigelow in the Santa Catalina Mountains approximately 29 kilometers (18 mi) northeast of Tucson, Arizona. The site in the Coronado National Forest is used with special permission from the United States Forest Service (USFS) by the Steward Observatory of the University of Arizona.
Richard Frederick Green is an American astronomer, former director of the Kitt Peak National Observatory, UKIRT and the Large Binocular Telescope Observatory.