14. Mauna Kea Telescopes 毛納基山望遠鏡 – Optical/Infrared( 光學望遠鏡 1) This chart shows all the mirrors of the optical and infrared telescopes on Mauna Kea to the same scale. 資料來源： http:// www.ifa.hawaii.edu/mko/telescope_table.htm NASA1979 3.0m NASA Infrared Telescope Facility IRTF UH Institute for Astronomy1970 2.2m UH 2.2-m telescope UH 2.2m University of Hawaii at Hilo1968 0.6m UH 0.6-m educational telescope UH 0.6m 成立時間 主鏡大小 望遠鏡 種類
15. The UH Hilo 24" Educational Telescope (foreground) Aerial photograph of the University of Hawaii 2.2-meter telescope.
16. Mauna Kea Telescopes 毛納基山望遠鏡 – Optical/Infrared( 光學望遠鏡 2) 資料來源： http:// www.ifa.hawaii.edu/mko/telescope_table.htm Caltech / University of California1992 10m W. M. Keck Observatory Keck I United Kingdom1979 3.8m United Kingdom Infrared Telescope UKIRT Canada / France / UH1979 3.6m Canada-France-Hawaii Telescope CFHT 成立時間 主鏡大小 望遠鏡 種類
17. The CFH observatory hosts a world-class, 3.6 meter optical/infrared telescope. The world's largest telescope dedicated solely to infrared astronomy, UKIRT is sited in Hawaii near the summit of Mauna Kea at an altitude of 4194m above sea level.
18. Mauna Kea Telescopes 毛納基山望遠鏡 – Optical/Infrared( 光學望遠鏡 3) 資料來源： http:// www.ifa.hawaii.edu/mko/telescope_table.htm USA / UK / Canada / Argentina / Australia / Brazil / Chile1999 8.1m Gemini Northern Telescope Gemini Japan1999 8.3m Subaru Telescope Subaru Caltech / University of California1996 10m W. M. Keck Observatory Keck II 成立時間 主鏡大小 望遠鏡 種類
22. The Caltech Submillimeter Observatory (CSO) is simultaneously one of the world's premier submillimeter telescopes and one of the easiest to use. With a diameter of 15m the James Clerk Maxwell Telescope (JCMT) is the largest astronomical telescope in the world designed specifically to operate in the submillimeter wavelength region of the spectrum. The JCMT is used to study our Solar System, interstellar dust and gas, and distant galaxies.
23. The Submillimeter Array (SMA) is an 8-element radio interferometer located atop Mauna Kea in Hawaii. Operating at frequencies from 180 GHz to 700 GHz, the 6m dishes may be arranged into configurations with baselines as long as 509m, producing a synthesized beam of sub-arcsecond width. Each element can observe with two receivers simultaneously, with 2 GHz bandwidth each. The digital correlator backend allows flexible allocation of thousands of spectral channels to each receiver.
24. Mauna Kea Telescopes 毛納基山望遠鏡 – Radio ( 無線電波望遠鏡 ) 資料來源： http:// www.ifa.hawaii.edu/mko/telescope_table.htm NRAO/AUI/NSF1992 25m Very Long Baseline Array VLBA 成立時間 主鏡大小 望遠鏡 種類
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