http www ifa hawaii eduifamapsmapsummitc jpg 5 1

圖片來源：http: //www. ifa. hawaii. edu/ifa/maps/map_summitc. jpg

二、具有特色的5座天文台 1. 次毫米波陣列望遠鏡（Sub-Millimeter Array，簡稱SMA） 2. 雙子星天文台（Gemini Observatory） 3. 昴星團望遠鏡（Subaru Telescope） 4. 超長基線陣列（Very Long Baseline Array，簡寫：VLBA）接收機 5. 凱克天文台(Twin Keck Telescopes)

1. 次毫米波陣列望遠鏡（Sub. Millimeter Array，簡稱SMA） 圖片來源：http: //explore. pts. org. tw/img/1 -5. jpg

3. 昴星團望遠鏡（Subaru Telescope） 昴星團望遠鏡（左）以及凱克Ⅰ望遠鏡 圖片來源： http: //upload. wikimedia. org/wikipedia/commons/thumb/6/64/Subaru_keck_t els. jpg/300 px-Subaru_keck_tels. jpg

4. 超長基線陣列（Very Long Baseline Array，簡寫：VLBA）接收機 美屬維京群島聖克羅伊是超長基線位於最東邊的接受機。 圖片來源： http: //upload. wikimedia. org/wikipedia/commons/thumb/e/e 2/VLBA_St_Cr oix-04. jpg/280 px-VLBA_St_Croix-04. jpg

5. 凱克天文台(Twin Keck Telescopes) 圖片來源：http: //www. ifa. hawaii. edu/mko/images/keck_pair. jpg

三、不同波段的望遠鏡 1. Optical/Infrared (光學/紅外線望遠鏡) 2. Submillimeter (次毫米波望遠鏡) 3. Radio (無線電波望遠鏡) 資料來源： http: //www. ifa. hawaii. edu/mko/telescope_table. htm

Mirror sizes 主鏡大小 • The Hubble Space Telescope's mirror is similar in size to that of the UH 2. 2 meter telescope -- the second smallest telescope on the mountain. UH 2. 2 meter telescope 圖片來源：http: //www. ifa. hawaii. edu/mko/images/mr_mirror 2_small. jpg

Mauna Kea Telescopes毛納基山望遠鏡 –Optical/Infrared(光學望遠鏡 1) 種類 望遠鏡 主鏡大小 成立時間 UH 0. 6 m UH 0. 6 -m educational telescope 0. 6 m University of Hawaii at Hilo 1968 UH 2. 2 m UH 2. 2 -m telescope 2. 2 m UH Institute for Astronomy 1970 IRTF 3. 0 m NASA 1979 NASA Infrared Teles cope Facility 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

The UH Hilo 24" Educational Telescope (foreground) Aerial photograph of the University of Hawaii 2. 2 -meter telescope.

Mauna Kea Telescopes毛納基山望遠鏡 –Optical/Infrared(光學望遠鏡 2) 種類 望遠鏡 主鏡大小 成立時間 CFHT Canada-France. Hawaii Telescope 3. 6 m Canada / France / UH 1979 UKIRT United Kingdom Infrared Telescope 3. 8 m United Kingdom 1979 Keck I W. M. Keck Observatory 10 m Caltech / University of California 1992 資料來源： http: //www. ifa. hawaii. edu/mko/telescope_table. htm

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 4194 m above sea level.

Mauna Kea Telescopes毛納基山望遠鏡 –Optical/Infrared(光學望遠鏡 3) 種類 望遠鏡 主鏡大小 成立時間 Keck II W. M. 10 m Caltech / University Keck Observator of California 1996 y Subaru Telescope 8. 3 m Japan 1999 Gemini Northern 8. 1 m USA / UK / Canada / Telescope Argentina / Australia / Brazil / Chile 1999 資料來源： http: //www. ifa. hawaii. edu/mko/telescope_table. htm

圖片來源： http: //explore. pts. org. tw/img/1 -7. jpg 圖片來源： http: //www. gemini. edu/images/pio/telescope_images/2009060 4_gn_sunset_stars. jpg

Mauna Kea Telescopes毛納基山望遠鏡 –Submillimeter(次毫米波望遠鏡) 種類 望遠鏡 主鏡大小 成立時間 CSO Caltech Submillimeter Observatory James Clerk Maxwell Telescope 10. 4 m Caltech / NSF 1987 15 m UK / Canada / Netherlands 1987 Submillimeter Array 8 x 6 m Smithsonian Astrophysical Observatory / Taiwan 2002 JCMT SMA 資料來源： http: //www. ifa. hawaii. edu/mko/telescope_table. htm

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 15 m 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.

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 6 m dishes may be arranged into configurations with baselines as long as 509 m, 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.

Mauna Kea Telescopes毛納基山望遠 鏡 –Radio(無線電波望遠鏡) 種類 望遠鏡 主鏡大小 VLBA Very Long 25 m Baseline Array 成立時間 NRAO/AUI/NSF 1992 資料來源： http: //www. ifa. hawaii. edu/mko/telescope_table. htm