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Palomar Observatory

A Wisdom Archive on Palomar Observatory

Palomar Observatory

A selection of articles related to Palomar Observatory

Palomar Observatory

ARTICLES RELATED TO Palomar Observatory

Palomar Observatory: Encyclopedia II - Brown dwarf - In theory

Brown dwarf - Distinguishing heavy brown dwarfs from light stars. Lithium: Lithium is generally present in brown dwarfs and not in low-mass stars. Stars, which achieve the high temperature necessary for fusing hydrogen, rapidly deplete their lithium. This occurs by a collision of Lithium-7 and a proton producing two Helium-4 nuclei. The temperature necessary for this reaction is just below the temperature necessary for hydrogen fusion. Convection in stars ensures that lithium in the whole volume of the sta ...

See also:

Brown dwarf, Brown dwarf - History, Brown dwarf - In theory, Brown dwarf - Distinguishing heavy brown dwarfs from light stars, Brown dwarf - Distinguishing light brown dwarfs from large planets, Brown dwarf - In practice, Brown dwarf - Observational techniques, Brown dwarf - Milestones, Brown dwarf - Recent developments

Read more here: » Brown dwarf: Encyclopedia II - Brown dwarf - In theory

Palomar Observatory: Encyclopedia II - Reflecting telescope - Reflecting telescope designs

Reflecting telescope - Newtonian focus. The Newtonian usually has a paraboloid primary mirror but for small apertures, say 12cm or less, if the focal ratio is f/8 or longer a spherical primary mirror is sufficient for high visual resolution. A flat secondary mirror reflects the light to a focal plane at the side of the top of the telescope tube. It is one of the simplest and least expensive designs for a given size of primary, and is popular with amateurs as a home-build project. Since the light path is un ...

See also:

Reflecting telescope, Reflecting telescope - Technical considerations, Reflecting telescope - Reflecting telescope designs, Reflecting telescope - Newtonian focus, Reflecting telescope - Cassegrain focus, Reflecting telescope - Schmidt camera, Reflecting telescope - Focal planes, Reflecting telescope - Prime focus, Reflecting telescope - Coudé focus

Read more here: » Reflecting telescope: Encyclopedia II - Reflecting telescope - Reflecting telescope designs

Palomar Observatory: Encyclopedia II - Reflecting telescope - Technical considerations

A curved primary mirror is the reflector telescope's basic optical element and creates an image at the focal plane. The distance from the mirror to the focal plane is called the focal length. Film or a digital sensor may be located here to record the image, or an eyepiece for visual observation. Reflector mirrors eliminate chromatic aberration but still produce other types of aberrations. Expensive telescopes will have additional optical elements to correct some of these aberrations: spherical aberration when a non-parabolic mirror is used (the image plane is not flat ...

See also:

Reflecting telescope, Reflecting telescope - Technical considerations, Reflecting telescope - Reflecting telescope designs, Reflecting telescope - Newtonian focus, Reflecting telescope - Cassegrain focus, Reflecting telescope - Schmidt camera, Reflecting telescope - Focal planes, Reflecting telescope - Prime focus, Reflecting telescope - Coudé focus

Read more here: » Reflecting telescope: Encyclopedia II - Reflecting telescope - Technical considerations

Palomar Observatory: Encyclopedia II - Schmidt camera - Applications

The Schmidt camera is typically used as a survey instrument, for research programs in which a large amount of sky must be covered. These include astronomical surveys, comet and asteroid searches, and nova patrols. In addition, Schmidt cameras and derivative designs are frequently used for tracking artificial earth satellites. Starting in the early 1970s, Celestron marketed an 8-inch Schmidt Camera. The camera was focused in the factory and was made of materials with low expansion coefficients so it would never need to be focuse ...

See also:

Schmidt camera, Schmidt camera - Invention and Design, Schmidt camera - Applications, Schmidt camera - Derivative Designs

Read more here: » Schmidt camera: Encyclopedia II - Schmidt camera - Applications

Palomar Observatory: Encyclopedia II - 90377 Sedna - Orbital characteristics

Sedna has a highly elliptical orbit, with its aphelion estimated at 975 AU and its perihelion at about 76.16 AU. At its discovery it was approaching perihelion at about 90 AU from the Sun. It was the farthest from the Sun that any solar system object had up to then been observed, although some objects like long-period comets originally observed at closer distances were most likely further from the Sun than Sedna but too dim to be observed. 2003 UB313 was later detected at 97 AU. Sedna's orbit takes about ...

See also:

90377 Sedna, 90377 Sedna - General information, 90377 Sedna - Orbital characteristics, 90377 Sedna - Physical characteristics, 90377 Sedna - Classification

Read more here: » 90377 Sedna: Encyclopedia II - 90377 Sedna - Orbital characteristics

Palomar Observatory: Encyclopedia II - 90377 Sedna - Physical characteristics

Sedna has an estimated diameter of between 1180 and 1800 kilometres (730 to 1120 miles). At the time of its discovery it was the largest object found in the solar system since Pluto was discovered in 1930. It is now generally believed to be the 4th largest known trans-Neptunian object after 2003 UB313, Pluto, and 2005 FY9. The planetoid is so far from the Sun that the temperatur ...

See also:

90377 Sedna, 90377 Sedna - General information, 90377 Sedna - Orbital characteristics, 90377 Sedna - Physical characteristics, 90377 Sedna - Classification

Read more here: » 90377 Sedna: Encyclopedia II - 90377 Sedna - Physical characteristics

Palomar Observatory: Encyclopedia II - Reflecting telescope - Focal planes

Reflecting telescope - Prime focus. In a prime focus design in large observatory telescopes, the observer sits inside the telescope, at the focal point of the reflected light. In the past this would be the astronomer himself, but nowadays CCD cameras are used. Radio telescopes often have a prime focus design. The mirror is replaced by a metal surface for reflecting radio waves, and the observer is an antenna. ...

See also:

Reflecting telescope, Reflecting telescope - Technical considerations, Reflecting telescope - Reflecting telescope designs, Reflecting telescope - Newtonian focus, Reflecting telescope - Cassegrain focus, Reflecting telescope - Schmidt camera, Reflecting telescope - Focal planes, Reflecting telescope - Prime focus, Reflecting telescope - Coudé focus

Read more here: » Reflecting telescope: Encyclopedia II - Reflecting telescope - Focal planes

Palomar Observatory: Encyclopedia II - San Diego County California - Sites of interest

San Diego County California - Observatories. Mount Laguna Observatory - owned and operated by San Diego State University (SDSU) Palomar Observatory - owned and primarily operated by California Institute of Technology (CalTech) San Diego County California - Wine regions. the Ramona Valley wine-producing ...

See also:

San Diego County California, San Diego County California - History, San Diego County California - Geography, San Diego County California - Adjacent Counties, San Diego County California - Sites of interest, San Diego County California - Observatories, San Diego County California - Wine regions, San Diego County California - Politics, San Diego County California - Demographics, San Diego County California - Current estimates, San Diego County California - Cities and towns in San Diego County, San Diego County California - Airports

Read more here: » San Diego County California: Encyclopedia II - San Diego County California - Sites of interest

Palomar Observatory: Encyclopedia II - San Diego County California - Cities and towns in San Diego County

Incorporated Cities Carlsbad (Aviara, La Costa) Chula Vista Coronado Del Mar El Cajon Encinitas (Cardiff-by-the-Sea, Leucadia, Olivenhain) Escondido Imperial Beach La Mesa Lemon Grove National City Poway Oceanside San Diego San Marcos Santee Solana Beach Vista Unincorporated Communities Agua Caliente Springs Alpine< ...

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San Diego County California, San Diego County California - History, San Diego County California - Geography, San Diego County California - Adjacent Counties, San Diego County California - Sites of interest, San Diego County California - Observatories, San Diego County California - Wine regions, San Diego County California - Politics, San Diego County California - Demographics, San Diego County California - Current estimates, San Diego County California - Cities and towns in San Diego County, San Diego County California - Airports

Read more here: » San Diego County California: Encyclopedia II - San Diego County California - Cities and towns in San Diego County

Palomar Observatory: Encyclopedia II - Reflecting telescope - Technical considerations

The primary mirror is the reflector telescope's basic optical element and creates an image at the focal plane. The distance from the mirror to the focal plane is called the focal length. Film or a digital sensor may be located here to record the image, or an eyepiece for visual observation. Reflector mirrors eliminate chromatic aberration but still contain other types of aberrations. Expensive telescopes will have additional optical elements to correct some of these aberrations; spherical aberration when a non-parabolic mirror is used (the image plane is not flat ...

See also:

Reflecting telescope, Reflecting telescope - Technical considerations, Reflecting telescope - Reflecting telescope designs, Reflecting telescope - Schmidt camera, Reflecting telescope - Newtonian focus, Reflecting telescope - Cassegrain focus, Reflecting telescope - Focal planes, Reflecting telescope - Prime focus, Reflecting telescope - Coudé focus

Read more here: » Reflecting telescope: Encyclopedia II - Reflecting telescope - Technical considerations

Palomar Observatory: Encyclopedia II - Reflecting telescope - Focal planes

Reflecting telescope - Prime focus. In a prime focus design, the observer sits inside the telescope, at the focal point of the reflected light. In the past this would be the astronomer himself, but nowadays CCD cameras are used. Radio telescopes often have a prime focus design. The mirror is replaced by a metal surface for reflecting radio waves, and the observer is an antenna. ...

See also:

Reflecting telescope, Reflecting telescope - Technical considerations, Reflecting telescope - Reflecting telescope designs, Reflecting telescope - Schmidt camera, Reflecting telescope - Newtonian focus, Reflecting telescope - Cassegrain focus, Reflecting telescope - Focal planes, Reflecting telescope - Prime focus, Reflecting telescope - Coudé focus

Read more here: » Reflecting telescope: Encyclopedia II - Reflecting telescope - Focal planes

Palomar Observatory: Encyclopedia II - San Diego County California - Demographics

As of the census2 of 2000, there are 2,813,833 people, 994,677 households, and 663,449 families residing in the county. The population density is 259/km² (670/mi²). There are 1,040,149 housing units at an average density of 96/km² (248/mi²). The racial makeup of the county is 66.52% White, 5.74% Black or African American, 0.86% Native American, 8.88% Asian, 0.48% Pacific Islander, 12.82% from other races, and 4.69% from two or more races. ...

See also:

San Diego County California, San Diego County California - History, San Diego County California - Geography, San Diego County California - Adjacent Counties, San Diego County California - Sites of interest, San Diego County California - Observatories, San Diego County California - Wine regions, San Diego County California - Politics, San Diego County California - Demographics, San Diego County California - Current estimates, San Diego County California - Cities and towns in San Diego County, San Diego County California - Airports

Read more here: » San Diego County California: Encyclopedia II - San Diego County California - Demographics

Palomar Observatory: Encyclopedia II - Mount Wilson Observatory - 100 inch 2.5 m Hooker telescope

Hale immediately set about creating a larger telescope. John D. Hooker provided crucial funding for it, along with Carnegie. The Saint Gobain factory was again chosen to cast a blank in 1906, which it completed in 1908, After considerable trouble over the blank (and potential replacements), the 100 inch (2.5 m) telescope was completed and saw "first light" on November 1, 1917. The mechanism incorporates a mercury float to provide smooth operation. The Hooker telescope was equipped in 1919 with a special attachment, an optical interfer ...

See also:

Mount Wilson Observatory, Mount Wilson Observatory - 60 inch 1.5 m Hale telescope, Mount Wilson Observatory - 100 inch 2.5 m Hooker telescope, Mount Wilson Observatory - Solar telescopes, Mount Wilson Observatory - Interferometry

Read more here: » Mount Wilson Observatory: Encyclopedia II - Mount Wilson Observatory - 100 inch 2.5 m Hooker telescope

Palomar Observatory: Encyclopedia II - Brown dwarf - History

Brown dwarfs were originally called black dwarfs, a classification for dark substellar objects floating freely in space which were too low in mass to sustain stable hydrogen fusion (black dwarfs currently refer to something different). Early stellar models suggested that a true star requires a mass at least 80 times that of Jupiter to support such fusion. Dense star-like objects with smaller masses, or "brown dwarfs," were hypothesized by the early 1960s -- formed much the way stars are formed, they would however be hard to fin ...

See also:

Brown dwarf, Brown dwarf - History, Brown dwarf - In theory, Brown dwarf - Distinguishing heavy brown dwarfs from light stars, Brown dwarf - Distinguishing light brown dwarfs from large planets, Brown dwarf - In practice, Brown dwarf - Observational techniques, Brown dwarf - Milestones, Brown dwarf - Recent developments

Read more here: » Brown dwarf: Encyclopedia II - Brown dwarf - History

Palomar Observatory: Encyclopedia II - Brown dwarf - In practice

Typical atmospheres of known brown dwarfs range in temperature from 300 to over 3000 K, in comparison with stars, which cool to minimum temperatures of around 4000 K. Compared to stars, which warm themselves with steady internal fusion, brown dwarfs cool quickly over time; more massive dwarfs cool slower than less massive ones. Brown dwarf - Observational techniques. Coronographs have recently been used to detect faint objects orbiting bright visible stars, including Gliese 229B. Sensitive ...

See also:

Brown dwarf, Brown dwarf - History, Brown dwarf - In theory, Brown dwarf - Distinguishing heavy brown dwarfs from light stars, Brown dwarf - Distinguishing light brown dwarfs from large planets, Brown dwarf - In practice, Brown dwarf - Observational techniques, Brown dwarf - Milestones, Brown dwarf - Recent developments

Read more here: » Brown dwarf: Encyclopedia II - Brown dwarf - In practice

Palomar Observatory: Encyclopedia II - 90377 Sedna - Classification

The discoverers have argued that Sedna is actually the first observed body belonging to the Oort cloud, saying that it is too far out to be considered a Kuiper belt object. Because it is a great deal closer to the Sun than was expected for an Oort cloud object, and has an inclination roughly in line with the planets and the Kuiper belt, they describe the planetoid as being an inner Oort cloud object, situated in the disc reaching from the K ...

See also:

90377 Sedna, 90377 Sedna - General information, 90377 Sedna - Orbital characteristics, 90377 Sedna - Physical characteristics, 90377 Sedna - Classification

Read more here: » 90377 Sedna: Encyclopedia II - 90377 Sedna - Classification

Palomar Observatory: Encyclopedia II - 90377 Sedna - Physical characteristics

Sedna has an estimated diameter of between 1180 and 1800 kilometres (730 to 1120 miles). At the time of its discovery it was the largest object found in the solar system since Pluto was discovered in 1930. It is now generally believed to be the 5th largest known trans-Neptunian object after 2003 UB313, Pluto, 2005 FY9, and 2003 EL61. The planetoid is so far from the Sun that the temperatur ...

See also:

90377 Sedna, 90377 Sedna - General information, 90377 Sedna - Orbital characteristics, 90377 Sedna - Physical characteristics, 90377 Sedna - Classification

Read more here: » 90377 Sedna: Encyclopedia II - 90377 Sedna - Physical characteristics

Palomar Observatory: Encyclopedia II - 1948 - Births

1948 - January-February. January 2 - Mary Archer, British scientist January 2 - Deborah Watling, British actress January 7 - Kenny Loggins, American singer January 10 - Donald Fagen, American keyboardist January 10 - Mischa Maisky, Latvian cellist January 14 - Carl Weathers, American football player and actor January 14 - T-Bone Burnett, American record producer and musician January 15 - Ronnie Van Zant, American musician (d. 1977) Janu ...

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1948, 1948 - Events, 1948 - January-February, 1948 - March-April, 1948 - May, 1948 - June-July, 1948 - August-December, 1948 - Undated, 1948 - Unknown date, 1948 - Births, 1948 - January-February, 1948 - March-April, 1948 - May-July, 1948 - August-December, 1948 - Unknown date, 1948 - Deaths, 1948 - Nobel Prizes

Read more here: » 1948: Encyclopedia II - 1948 - Births

Palomar Observatory: Encyclopedia II - 90377 Sedna - Orbital characteristics

Sedna has a highly elliptical orbit, with its aphelion estimated at 942 AU and its perihelion at about 76.1 AU. At its discovery it was approaching perihelion at about 90 AU from the Sun. It was the farthest from the Sun that any solar system object had up to then been observed, although some objects like long-period comets originally observed at closer distances were most likely further from the Sun than Sedna but too dim to be observed. 2003 UB313 was later detected at 97 AU. Sedna's orbit takes about ...

See also:

90377 Sedna, 90377 Sedna - General information, 90377 Sedna - Orbital characteristics, 90377 Sedna - Physical characteristics, 90377 Sedna - Classification

Read more here: » 90377 Sedna: Encyclopedia II - 90377 Sedna - Orbital characteristics

Palomar Observatory: Encyclopedia II - California Institute of Technology - Academics

Academics at Caltech are famously hard, and the analogy of drinking water from a firehose is often applied. Life is sometimes described by the aphorism, "Work, sleep, social life: pick two," pointing to the great amount of academic work. While Caltech is most famous for its physics department, under the leadership of David Baltimore, it has strived particularly to improve its facilities in the life sciences. Caltech is also known for interdisciplinary programs such as the Computation and Neural Systems (CNS) program. C ...

See also:

California Institute of Technology, California Institute of Technology - History, California Institute of Technology - Academics, California Institute of Technology - Academic departments, California Institute of Technology - Undergraduate program, California Institute of Technology - Student life, California Institute of Technology - House system, California Institute of Technology - Traditions

Read more here: » California Institute of Technology: Encyclopedia II - California Institute of Technology - Academics

Palomar Observatory: Encyclopedia II - California Institute of Technology - Student life

California Institute of Technology - House system. See main article: House System at Caltech During the early 20th century, a Caltech committee visited several universities and decided to transform the undergraduate housing system from regular fraternities to a House System, similar to the residential college system of Oxford and Cambridge. Four (south) houses (or hovses, so named for the inscription on the gates thereof) were built: Blacker House, Dabney House, Fleming House, and Ricketts Ho ...

See also:

California Institute of Technology, California Institute of Technology - History, California Institute of Technology - Academics, California Institute of Technology - Academic departments, California Institute of Technology - Undergraduate program, California Institute of Technology - Student life, California Institute of Technology - House system, California Institute of Technology - Traditions

Read more here: » California Institute of Technology: Encyclopedia II - California Institute of Technology - Student life

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