Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

Magellan Telescopes

Coordinates:29°00′54″S70°41′30″W / 29.015°S 70.6917°W /-29.015; -70.6917
From Wikipedia, the free encyclopedia
Optical telescopes located at Las Campanas Observatory in Chile
Magellan Telescopes
Alternative namesWalter Baade Magellan 6.5-m telescope (LCO)Edit this at Wikidata
Location(s)Atacama Region, Chile
Coordinates29°00′54″S70°41′30″W / 29.015°S 70.6917°W /-29.015; -70.6917Edit this at Wikidata
Altitude2,516, 2,392 m (8,255, 7,848 ft)Edit this at Wikidata
Diameter6.5 m (21 ft 4 in)Edit this at Wikidata
Magellan Telescopes is located in Chile
Magellan Telescopes
Location of Magellan Telescopes
 Related media on Commons

TheMagellan Telescopes are a pair of 6.5-metre-diameter (21 ft) opticaltelescopes located atLas Campanas Observatory inChile. The two telescopes are named after the astronomerWalter Baade and thephilanthropistLandon T. Clay.First light for the telescopes was on September 15, 2000 for the Baade, and September 7, 2002 for the Clay. A consortium consisting of theCarnegie Institution for Science,University of Arizona,Harvard University, theUniversity of Michigan and theMassachusetts Institute of Technology built and operate the twin telescopes. The telescopes were named after the sixteenth-century Portuguese explorerFerdinand Magellan.

TheGiant Magellan Telescope (GMT) is anextremely large telescope under construction, as part of the US Extremely Large Telescope Program.[1]

Current instruments on the Magellan Telescopes

[edit]

Baade telescope:

  • Inamori Magellan Areal Camera and Spectrograph (IMACS)
  • FourStar
  • Folded port InfraRed Echellette (FIRE)
  • Magellan Echellete (MagE)

Clay telescope:

  • Magellan Inamori Kyocera Echelle (MIKE) spectrograph
  • Low-Dispersion Survey Spectrograph-3 (LDSS-3)
  • Megacam imager
  • MagAO-X
  • Michigan/Magellan Fiber System (M2FS)

Magellan Planet Search Program

[edit]
Main article:Magellan Planet Search Program

This program is a survey of stars searching for planets using the MIKE echelle spectrograph mounted on the 6.5 m Magellan II (Clay) telescope.[2][3]

MagAO Adaptive Optics System

[edit]

In 2013, Clay (Magellan II) was equipped with anadaptive secondary mirror called MagAO which allowed it to take the sharpest visible-light images to date, capable of resolving objects 0.02 arcseconds across—equivalent to adime (1.8 cm) seen from 100 miles (160 km) away.[4]

MagAO was originally intended for theLarge Binocular Telescope (LBT), but the secondary mirror was damaged before it could be installed. The project leader Laird Close and his team were able to repair and repurpose the broken mirror for use on Magellan II. As built for the LBT, the original MagAO mirror had a diameter of 36 inches (0.91 m). However, the edge of the mirror was broken. Technicians atSteward Observatory were able to cut the mirror to 33.5 inches (0.85 m) in diameter, thereby removing the broken edge.[5]

Gallery

[edit]
Comparison of nominal sizes of apertures of the Magellan Telescopes and some notable optical telescopes
  • Part of Las Campanas Observatory after snowfall, with the Magellan telescopes at the right.
    Part of Las Campanas Observatory after snowfall, with the Magellan telescopes at the right.
  • Telescopes at night
    Telescopes at night

See also

[edit]

References

[edit]
  1. ^Harvard & Smithsonian (6 February 2022)."Mission Critical: Giant Magellan Telescope Ranked a National Priority".SciTechDaily. Retrieved7 February 2022.
  2. ^Minniti, Dante; Butler, R. Paul; López-Morales, Mercedes; Shectman, Stephen A.; Adams, Fred C.; Arriagada, Pamela; Boss, Alan P.; Chambers, John E. (2009)."Low Mass Companions for Five Solar-Type Stars from the Magellan Planet Search Program".The Astrophysical Journal.693 (2):1424–1430.arXiv:0810.5348.Bibcode:2009ApJ...693.1424M.doi:10.1088/0004-637X/693/2/1424.S2CID 119224845.
  3. ^Arriagada, Pamela; Butler, R. Paul; Minniti, Dante; López-Morales, Mercedes; Shectman, Stephen A.; Adams, Fred C.; Boss, Alan P.; Chambers, John E. (2010)."Five Long-Period Extrasolar Planets in Eccentric Orbits from the Magellan Planet Search Program".The Astrophysical Journal.711 (2):1229–1235.arXiv:1001.4093.Bibcode:2010ApJ...711.1229A.doi:10.1088/0004-637X/711/2/1229.S2CID 118682009.
  4. ^Wall, Mike (21 August 2013)."New Telescope Tech Takes Sharpest Night Sky Photos Ever".Space.com. Retrieved29 July 2020.
  5. ^Beal, Tom (22 August 2013)."University of Arizona astronomers see more clearly than ever".Arizona Daily Star. Archived fromthe original on 25 August 2013. Retrieved29 July 2020.

External links

[edit]
Portals:
Retrieved from "https://en.wikipedia.org/w/index.php?title=Magellan_Telescopes&oldid=1303109781"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp