Palomar Observatory: Wikis

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Palomar Observatory
P200 Dome Open.jpg
Organization Caltech
Location San Diego County, California
Coordinates
Altitude 1,713 m (5,618 ft)
Website
Palomar at Caltech
Telescopes
Hale Telescope 200 inch (5.08 m) reflector
60 inch (1.52 m) Telescope 60 inch (1.52 m) reflector
Samuel Oschin Telescope 48 inch (1.22 m) Schmidt Reflector
JPL Palomar Testbed Interferometer Interferometer

Palomar Observatory [1], at approximately 5,570 ft elevation, is a privately owned observatory located in San Diego County, California, 90 miles (145 km) southeast of Pasadena's Mount Wilson Observatory, in the Palomar Mountain Range. It is owned and operated by the California Institute of Technology. Research time is granted to Caltech and its research partners which includes the Jet Propulsion Laboratory, and Cornell University.[1]. The observatory currently consists of three large telescopes: the 200 inch (5.08 m) Hale telescope, the 48 inch (1.22 m) Samuel Oschin telescope, and a 60 inch (1.52 m) reflecting telescope. In addition, the Palomar Testbed Interferometer and other instruments are located at this observatory. An 18 inch (457 millimeter) Schmidt telescope, Palomar Observatory's first telescope, dating from 1936, is no longer operational.

Contents

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 of what was to become the 200-inch Palomar reflector; it was an invitation to the American public 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. In fact the 200-inch telescope was the most important telescope in the world from 1949 until 1992 when the Keck I telescope (at approximately 10 meters - 387 inches) on Mauna Kea in Hawaii became the world's largest.

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."

Etymology

The word palomar is from the Spanish language, dating back from the time of Spanish California, and means pigeon house (in the same sense as henhouse). The name may be in reference to the large shoals of pigeons that can be seen during the spring and autumn months atop Palomar Mountain or reminiscent of an old pigeon-raising facility built there by the Spaniards.

The Hale Telescope

The 200-inch (5.08 m) telescope is named after astronomer George Ellery Hale. It was built by Caltech with a 6 million dollar grant from the Rockefeller Foundation, using a Pyrex blank manufactured by Corning Glass Works. The telescope (the largest in the world at that time) saw first light January 26, 1949 targeting NGC 2261.[2] The American astronomer Edwin Powell Hubble, perhaps the most important observer of the 20th century, was given the honor of being the first astronomer to use the telescope.

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 chemisty 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

Ronald Florence wrote a history of the instrument's construction, titled The Perfect Machine, ISBN 0-06-018205-9. Richard Preston wrote a critically acclaimed non-fiction book about the Hale telescope and the astronomers who have used it, called First Light.

Architecture and design

According to the Observatory's Public Affairs Office, Russell W. Porter was primarily responsible for the striking Art Deco architecture of the Observatory's buildings, most notably 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 remarkable 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 iconic, gleaming white building on Palomar Mountain that houses the 200 inch Hale Telescope is considered by many to be "The Cathedral of Astronomy".

Telescopes and instruments

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

Major instruments at the Palomar Observatory include:[3]

  • 200-inch Hale Telescope (Project started in 1928, and active since first light in 1948) (see above)
  • A 60" (1.5 m) f/8.75 telescope in the Oscar Mayer Building. It was dedicated in 1970 to take some of the load off of the Hale Telescope. This telescope discovered the first brown dwarf star.
  • The 48" (1.22 m) Samuel Oschin Telescope (Schmidt Camera). The dwarf planet Eris was discovered by Caltech astronomer Mike Brown using this instrument. It was this object that triggered the discussions in the international astronomy community that led to Pluto being re-classified as a dwarf planet.
  • A 24" robotic telescope completed in January 2006. It is used to monitor the weather on Saturn's largest moon, Titan, and to follow up on observations of moving objects in the solar system discovered with the Samuel Oschin telescope.
  • An 18" (0.4 m) Schmidt camera.[4] Now retired, in 1936 this became the first operational telescope at the Observatory. Comet Shoemaker-Levy 9 was discovered with this instrument in 1993. In the 1930s a Caltech astronomer named Fritz Zwicky discovered over 100 supernovae (exploding stars) in other galaxies with this telescope and gathered the first evidence for dark matter.
  • The Palomar Planet Search Telescope From 2003 - 2008 this small robotic telescope was dedicated to the search for planets around other stars using the transit method.[5]
  • The Palomar Testbed Interferometer a multi-telescope instrument that permits 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.

Palomar Observatory Sky Surveys

The Palomar Observatory Sky Survey (POSS), 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 or (6 degree)2 blue-sensitive (Kodak 103a-O) and red-sensitive (Kodak 103a-E) photographic plates on the 48 inch (1.22 m) 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 consisted of 937 plate pairs.

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

The Second Palomar Observatory Sky Survey (POSS II) 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, D. Mendenhall, K. Rykoski, J. Phinney and Jean Mueller (who discovered over 100 supernovae by comparing the POSS I and POSS II plates). Ms Mueller also discovered several comets during the course of POSS II and the bright Comet Wilson 1986 was discovered by then graduate student C. Wilson early in the survey.[6]

Until the completion of the Two Micron All Sky Survey (2MASS), POSS was the most extensive wide-field sky survey ever. When completed, the Sloan Digital Sky Survey will surpass the POSS in depth, although the POSS covers almost 2.5 times as much area on the sky. POSS also exists in digitized form (i.e., the photographic plates were scanned), both in photographic form as the Digitized Sky Survey (DSS)[7] and in catalog form as the Minnesota Automated Plate Scanner (MAPS) Catalog.[8]

POSS II was followed by the Palomar Quasar Equatorial Survey Team (QUEST) Variability survey[9]. 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.[10]. 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 [11], gamma-ray bursts, black holes, quasars and much more.[12]

The 48-inch Samuel Oschin Schmidt Telescope is actively working on a new sky survey, the Palomar Transient Factory.[13]

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 US and the UK 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 which sharpens pictures taken from the Palomar Observatory. The resolution attained exceeds that of the Hubble Space Telescope by a factor of two.[14] [15]

Directors

Public access

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 200-inch (5.08 m) telescope daily from 9 a.m. to 3 p.m. 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, http://palomar-observatory.org. There is a visitor's center and a gift shop on the grounds. Behind-the-scenes tours for the public are offered through the Friends of Palomar [2] support group and the Reuben H. Fleet Science Center.[16] 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 ).

In pop culture

The band Wellwater Conspiracy's 1997 debut album, Declaration of Conformity, contains a track entitled "Palomar Observatory." It is the last track on the album and completely instrumental. It is likely the track title was chosen by singer/drummer Matt Cameron, who grew up in San Diego near the observatory. Also, Canadian band The Rheostatics 11th track from their effort Whale Music is entitled Palomar. The song depicts a man named Palomar on the top of a mount, cleaning his lenses with saline waters. Palomar assembles his kaleidoscope in his lonely observatory. The song is an extremely visual characterization of a man on a mountain and his relationship with his best friend, a dog.

Italo Calvino's 1983 novel Mr. Palomar, which features a man reflecting on how he observes the world, is named after the observatory. Palomar is mentioned in the first episode of season 2 of The X-Files, "Little Green Men". Fox Mulder intimates that an ELF crawled through the window of Hale's billiard room and told him to build the observatory.

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.[17]

See also

References

  • Florence, Ronald (1995 September). The Perfect Machine: Building the Palomar Telescope. Harper Perennial. pp. 480. ISBN 0-06-092670-8.  
  • Crawford, David Livingstone, ed (1966). The Construction of large telescopes (International Astronomical Union. Symposium no. 27 ed.). London, New York: Academic Press. pp. 234.  

External links


Simple English

Palomar Observatory
Organization Caltech
Location San Diego County, California
Coordinates
Altitude 1,713 m (5,618 ft)
Website
Palomar at Caltech
Telescopes
Hale Telescope 200 inch (5.08 m) reflector
60 inch (1.52 m) Telescope 60 inch (1.52 m) reflector
Samuel Oschin Telescope 48 inch (1.22 m) Schmidt Reflector
JPL Palomar Testbed Interferometer Interferometer
Snoop All-Sky Camera

Palomar Observatory is a privately owned observatory in San Diego County, California, 90 miles (145 km) southeast of Mount Wilson Observatory, on Palomar Mountain in the Palomar Mountain Range. It is owned and run by the California Institute of Technology (Caltech). The observatory is made up of four main telescopes: the 200 inch (5.08 m) Hale telescope, the 48 inch (1.22 m) Samuel Oschin telescope, the 18 inch (457 millimeter) Schmidt telescope, and a 60 inch (1.52 m) reflecting telescope. Also, the Palomar Testbed Interferometer is located at this observatory.

Name

The word palomar is from the Spanish language, meaning pigeon house. The name may be because of the large amounts of pigeons that can be seen in the spring and autumn months on Palomar Mountain, or it may be because of an old pigeon-raising building built there by the Spaniards.



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