Palomar Observatory

Palomar Mountain Observatory

Alternative names	675 PA
Organization	California Institute of Technology
Observatory code	675
Location	San Diego County, California
Coordinates	33°21′23″N 116°51′54″W
Altitude	1,712 m (5,617 ft)
Established	1928
Website	www.astro.caltech.edu/palomar/
Telescopes	18-inch Schmidt camera Near-Earth Asteroid Tracking (NEAT) at Palomar observatory Palomar 60-inch telescope Palomar Mountain-DSS Hale Telescope Palomar Testbed Interferometer Samuel Oschin telescope
Location of Palomar Observatory
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Palomar Observatory is an astronomical observatory located in San Diego County, California, United States, 145 kilometers (90 mi) southeast of Los Angeles, California, in the Palomar Mountain Range. It is owned and operated by the California Institute of Technology (Caltech) located in Pasadena, California. Research time is granted to Caltech and its research partners, which include the Jet Propulsion Laboratory (JPL) and Cornell University.

The observatory operates several telescopes, including the 200-inch (5.1 m) Hale Telescope and the 48-inch (1.2 m) Samuel Oschin Telescope. In addition, other instruments and projects have been hosted at the observatory, such as the Palomar Testbed Interferometer and the historic 18-inch (0.46 m) Schmidt telescope, Palomar Observatory's first telescope, dating from 1936.

History

Hale's vision for large telescopes and Palomar Observatory

Astronomer George Ellery Hale, whose vision created the Palomar Observatory, built the world's largest telescope four times. He published an article in the April 1928 issue of Harper's Magazine called "The Possibilities of Large Telescopes". This article contained Hale's vision for building what was to become the 200-inch Palomar reflector; it was an invitation to the American public to learn about how large telescopes could help answer questions relating to the fundamental nature of the universe. Hale hoped that the American people would understand and support his project.

Hale followed this article with a letter to the International Education Board (later absorbed into the General Education Board) of the Rockefeller Foundation dated April 28, 1928, in which he requested funding for this project. In his letter, Hale stated:

"No method of advancing science is so productive as the development of new and more powerful instruments and methods of research. A larger telescope would not only furnish the necessary gain in light space-penetration and photographic resolving power, but permit the application of ideas and devices derived chiefly from the recent fundamental advances in physics and chemistry."

Hale Telescope

Main article: Hale telescope

The 200-inch telescope is named after astronomer George Hale. It was built by Caltech with a $6 million grant from the Rockefeller Foundation, using a Pyrex blank manufactured by Corning Glass Works. Dr. J.A. Anderson was the initial project manager assigned in the early 1940s. The telescope (the largest in the world at that time) saw first light January 26, 1949 targeting NGC 2261. The American astronomer Edwin Powell Hubble was the first astronomer to use the telescope.

The 200-inch telescope was the largest telescope in the world from 1949 until 1975, when the Russian BTA-6 telescope saw first light. Astronomers using the Hale Telescope have discovered distant objects at the edges of the known universe called quasars and have given us the first direct evidence of stars in distant galaxies. They have studied the structure and chemistry of intergalactic clouds, leading to an understanding of the synthesis of elements in the universe, and have discovered thousands of asteroids. A one-tenth-scale engineering model of the telescope at Corning Community College in Corning, New York, home of the Corning Glass Works (now Corning Incorporated) was used to discover at least one minor planet, (34419) Corning.†

Architecture and design

Hale Telescope Dome

According to the Observatory's Public Affairs Office, Russell W. Porter was primarily responsible for the Art Deco architecture of the Observatory's buildings, including the dome of the 200–inch Hale Telescope. Porter was also responsible for much of the technical design of the Hale Telescope and Schmidt Cameras, producing a series of cross-section engineering drawings that are considered among the finest examples of such work. Porter worked on the designs in collaboration with many engineers and Caltech committee members. The gleaming white building on Palomar Mountain that houses the 200–inch Hale Telescope is considered by many to be "The Cathedral of Astronomy".

Max Mason directed the construction and Theodore von Karman was involved in the engineering.

Directors

• Ira Sprague Bowen, 1948–1964
• Horace Welcome Babcock, 1964–1978
• Maarten Schmidt, 1978–1980
• Gerry Neugebauer, 1980–1994
• James Westphal, 1994–1997
• Wallace Leslie William Sargent, 1997–2000
• Richard Ellis, 2000–2006
• Shrinivas Kulkarni, 2006–

Palomar Observatory and light pollution

Much of the surrounding region of Southern California has adopted shielded lighting to reduce the light pollution that would potentially affect the observatory.

Telescopes and instruments

Astronomer Jean Mueller posing with the Samuel Oschin Telescope (Schmidt Camera)

• The 200-inch Hale Telescope was first proposed in 1928 and has been operational since 1948. It was the largest telescope in the world for 45 years.
• A 60-inch reflecting telescope is located in the Oscar Mayer Building. It was dedicated in 1970 to take some of the load off of the Hale Telescope. This telescope was used to discover the first brown dwarf star.
• The 48-inch Samuel Oschin Telescope (Schmidt Camera) was started in 1938 and installed in 1948. It was initially called the 48–inch Schmidt, and was dedicated to Samuel Oschin in 1986. The dwarf planet Eris was discovered using this instrument. The existence of Eris triggered the discussions in the international astronomy community that led to Pluto being re-classified as a dwarf planet.

Former instruments

• An 18-inch Schmidt camera became the first operational telescope at the Palomar in 1936. In the 1930s, Fritz Zwicky, a Caltech astronomer, discovered over 100 supernovae in other galaxies with this telescope and gathered the first evidence for dark matter. Comet Shoemaker-Levy 9 was discovered with this instrument in 1993. It has since been retired and is on display at the small museum/visitor center.
• The Palomar Testbed Interferometer was a multi-telescope instrument that permitted astronomers to make very high resolution measurements of the sizes and positions of objects in space. The shapes of some bright stars have been measured with the PTI. It operated from 1995 to 2008.
• The Palomar Planet Search Telescope (PPST), aka Sleuth, was a 0.1 m (3.9 in) robotic telescope that operated from 2003 until 2008. It was dedicated to the search for planets around other stars using the transit method. It operated in conjunction with telescopes at Lowell Observatory and in the Canary Islands as part of the Trans-atlantic Exoplanet Survey (TrES).

Research

The observatory has completed several astronomical surveys: the first in the 1950s, the second in the 1980s and 1990s, and a third in 2003.

POSS-I

The initial Palomar Observatory Sky Survey (POSS or POSS-I), sponsored by the National Geographic institute, was completed in 1958. The first plates were shot in November 1948 and the last in April 1958. This survey was performed using 14 inch² (6 degree²) or blue-sensitive (Kodak 103a-O) and red-sensitive (Kodak 103a-E) photographic plates on the 48-inch Samuel Oschin Schmidt reflecting telescope. The survey covered the sky from a declination of +90 degrees (celestial north pole) to -27 degrees and all right ascensions and had a sensitivity to +22 magnitudes (about 1 million times fainter than the limit of human vision). A southern extension extending the sky coverage of the POSS to -33 degrees declination was shot in 1957 - 1958. The final POSS I consisted of 937 plate pairs.

Fritz Zwicky was the first astronomer to observe on Mt. Palomar and was the father of the Sky Survey Technique.

Digitized Sky Survey (DSS) produced images which were based on the photographic data developed in the course of POSS-I.

J.B. Whiteoak, an Australian radio astronomer, used the same instrument to broaden this POSS-I data further. Whiteoaks observations extended south to about -45 degrees declination, using the same field centers as the corresponding northern declination zones. Unlike POSS-I, the Whiteoak extension consisted only of red-sensitive (Kodak 103a-E) photographic plates.

POSS-II

"Second Palomar Observatory Sky Survey" redirects here. For POSS I, see Palomar Sky Survey.

The Second Palomar Observatory Sky Survey (POSS II, sometimes Second Palomar Sky Survey) was performed in the 1980s and 1990s that made use of better, faster films and an upgraded telescope. The Oschin Schmidt was given an achromatic corrector and provisions for autoguiding. Images were recorded in three wavelengths: blue (IIIaJ), red (IIIaF) and near infrared (IVN) plates, respectively. Observers on POSS II included C. Brewer, D. Griffiths, W. McKinley, J. Dave Mendenhall, K. Rykoski, Jeffrey L. Phinney and Jean Mueller (who discovered over 100 supernovae by comparing the POSS I and POSS II plates). Mueller also discovered several comets and minor planets during the course of POSS II and the bright Comet Wilson 1986 was discovered by then graduate student C. Wilson early in the survey.

Until the completion of the Two Micron All Sky Survey (2MASS), POSS II was the most extensive wide-field sky survey ever. When completed, the Sloan Digital Sky Survey will surpass POSS I and POSS II in depth, although the POSS covers almost 2.5 times more area on the sky.

POSS II also exists in digitized form (i.e., the photographic plates were scanned), both in photographic form as the Digitized Sky Survey (DSS)

QUEST

The multi-year POSS projects were followed by the Palomar Quasar Equatorial Survey Team (QUEST) Variability survey. This survey yielded results that were used by several projects, including the Near-Earth Asteroid Tracking project. Another program that used the QUEST results discovered 90377 Sedna on 14 November 2003, and around 40 Kuiper belt objects. Other programs that share the camera are Shri Kulkarni's search for gamma-ray bursts (this takes advantage of the automated telescope's ability to react as soon as a burst is seen and take a series of snapshots of the fading burst), Richard Ellis' search for supernovae to test whether the universe's expansion is accelerating or not, and S. George Djorgovski's quasar search.

The camera for the Palomar QUEST Survey was a mosaic of 112 Charge-coupled devices (CCDs) covering the whole (4 degree by 4 degree) field of view of the Schmidt telescope, the largest CCD mosaic used in an astronomical camera when built. This instrument was used to produce The Big Picture, the largest astronomical photograph ever produced. The Big Picture is on display at Griffith Observatory.

Current research

Current research programs on the 200-inch Hale Telescope cover the range of the observable universe including studies on near-Earth asteroids, outer solar system planets, Kuiper Belt Objects, star formation, exoplanets, gamma-ray bursts, black holes, quasars and much more.

The 48-inch Samuel Oschin Schmidt Telescope is actively working on a new sky survey, the Palomar Transient Factory (PTF).

The 60-inch telescope is used for a variety of projects including follow-up observations for the Palomar Transient Factory and is a rapid response telescope for gamma-ray bursts.

Clearest images

In September 2007, a team of astronomers from the United States and Britain released some of the clearest pictures ever taken of outer space. The pictures were obtained through the use of a new hybrid "Lucky imaging" and "adaptive optics" system that sharpens pictures taken from the Palomar Observatory. The resolution attained exceeds that of the Hubble Space Telescope by a factor of two.

Visiting

The Palomar Observatory is an active research facility. However, parts of it are open to the public during the day. Visitors can take self-guided tours of the 200-inch telescope daily from 9 a.m. to 3 p.m. The observatory is open 7 days a week, year round, except for December 24 and 25 and during times of inclement weather. Guided tours of the 200-inch Hale Telescope dome and observing area are available Saturdays and Sundays from April through October. Details are available at the Observatory's web site. There is a visitor's center and a gift shop on the grounds. Behind-the-scenes tours for the public are offered through the community support group, Friends of Palomar support group. Periodic tours are also organized by the Reuben H. Fleet Science Center in San Diego. The observatory is located off State Route 76 in northern San Diego County, California, is two hours' drive from downtown San Diego, and three hours' drive from central Los Angeles ( UCLA, LAX airport ). Those staying at nearby Palomar Campground can visit Palomar Observatory by hiking 2.2 miles (3.5 km) up Observatory Trail.

In popular culture

In the October 11 and 12, 1989, Calvin and Hobbes comic strips, Calvin has a dream where Stupendous Man takes the lens from the Palomar Observatory telescope (though really the telescope has a mirror and not a lens) and uses it to destroy his school.

Canadian band The Rheostatics' 1992 release Whale Music features a track entitled "Palomar." The song depicts a man named Palomar on the top of a mount, cleaning his lenses with saline waters, and assembling his kaleidoscope in his lonely observatory. The song presents a visual characterization of a man on a mountain and his relationship with his best friend, a dog.

In 1994, Palomar is mentioned in the first episode of season 2 of The X-Files, "Little Green Men". Fox Mulder refers to Hale's suggestion that an elf crawled through his window and told him to build the observatory.

The band Wellwater Conspiracy's 1997 debut album, Declaration of Conformity, contains an instrumental track entitled "Palomar Observatory." Wellwater Conspiracy singer/drummer Matt Cameron grew up in San Diego near the observatory.

Selected books

This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by adding missing items with reliable sources.

• 1983 — Calvino, Italo. Mr. Palomar. Torino: G. Einaudi. ISBN 9788806056797; OCLC 461880054 Template:It
• 1987 — Preston, Richard. First Light. New York: Atlantic Monthly Press. ISBN 9780871132000; OCLC 16004290
• 1994 — Florence, Ronald. The Perfect Machine. New York: HarperCollins. ISBN 9780060182052; OCLC 611549937
• 2010 — Brown, Michael E.. How I Killed Pluto and Why It Had It Coming. Spiegel & Grau. ISBN 0-385-53108-7; OCLC 495271396

See also

• National Geographic Society – Palomar Observatory Sky Survey
• Mount Laguna Observatory
• Jet Propulsion Laboratory
• California Institute of Technology
• Digitized Sky Survey

Further reading

• Crawford, David Livingston (1966). The Construction of large telescopes. London, New York: Academic Press. OCLC 1093049
• Mollise, Rod (2006). The Urban Astronomer's Guide: a Walking Tour of the Cosmos for City Sky Watchers. Berlin: Springer. ISBN 9781846282171; ISBN 9781846282164 OCLC 299995003
• Watterson, T.V. (1941). Palomar Observatory. San Diego, California: Frye & Smith.OCLC 6327013

External links

• Caltech Astronomy: Palomar Observatory
• Palomar Skies, news and history written by Palomar public affairs coordinator Scott Kardel
• The SBO Palomar Sky Survey Prints
• Palomar Observatory Clear Sky Clock Forecast of observing conditions.