Book contents
- Frontmatter
- Contents
- Preface
- Part 1 Optical Observatories
- 1 Palomar Mountain Observatory
- 2 The United States Optical Observatory
- 3 From the Next Generation Telescope to Gemini and SOAR
- 4 Competing Primary Mirror Designs
- 5 Active Optics, Adaptive Optics and Other Technical Innovations
- 6 European Northern Observatory and Calar Alto
- 7 European Southern Observatory
- 8 Mauna Kea Observatory
- 9 Australian Optical Observatories
- 10 Mount Hopkins' Whipple Observatory and the MMT
- 11 Apache Point Observatory
- 12 Carnegie Southern Observatory (Las Campanas)
- 13 Mount Graham International Optical Observatory
- 14 Modern Optical Interferometers
- 15 Solar Observatories
- Part 2 Radio Observatories
- Name Index
- Optical/ Infrared Observatory and Telescope Index
- Radio Observatory and Telescope Index
- General Index
- References
8 - Mauna Kea Observatory
from Part 1 - Optical Observatories
Published online by Cambridge University Press: 15 December 2016
- Frontmatter
- Contents
- Preface
- Part 1 Optical Observatories
- 1 Palomar Mountain Observatory
- 2 The United States Optical Observatory
- 3 From the Next Generation Telescope to Gemini and SOAR
- 4 Competing Primary Mirror Designs
- 5 Active Optics, Adaptive Optics and Other Technical Innovations
- 6 European Northern Observatory and Calar Alto
- 7 European Southern Observatory
- 8 Mauna Kea Observatory
- 9 Australian Optical Observatories
- 10 Mount Hopkins' Whipple Observatory and the MMT
- 11 Apache Point Observatory
- 12 Carnegie Southern Observatory (Las Campanas)
- 13 Mount Graham International Optical Observatory
- 14 Modern Optical Interferometers
- 15 Solar Observatories
- Part 2 Radio Observatories
- Name Index
- Optical/ Infrared Observatory and Telescope Index
- Radio Observatory and Telescope Index
- General Index
- References
Summary
Introduction
Hawaii was an important location for geophysical and astronomical observations during the International Geophysical Year (IGY) of 1957–58 because of its relative isolation in the middle of the Pacific Ocean. As a result, a number of such observations were planned but, unfortunately, there was not enough time nor money to establish all the facilities required. For example Walter Steiger of the University of Hawaiʻi (UH) had been hoping to establish a solar observatory in Hawaii, and in 1955 he had started site testing at the top of the 3,060 m (10,040 ft) high Haleakala, a virtually extinct volcano on the island of Maui. These tests indicated that Haleakala would be an ideal location for a solar observatory, but because of financial and timescale limitations Steiger had to settle, instead, for establishing a sea-level observatory on the island of Oahu.
Fred Whipple had also asked if the UH could build a satellite tracking station on Haleakala for the duration of the IGY. In this case he arranged for money to be provided in a rather round about way. He persuaded his old friend Kenneth Mees, a retired senior executive of Kodak and photographic scientist, to donate a number of Kodak plates to the UH so they could sell them and use the money to establish the tracking station. As a result the UH was able to acquire a plot of land on the summit not only for the satellite tracking station, which became operational in 1957, but, hopefully, to accommodate a future solar observatory there. At about the same time the United States Weather Bureau/National Bureau of Standards established an atmospheric research station at 11,120 ft (3,390 m) on the relatively stable northern slope of the active volcano Mauna Loa on the main island of Hawaii. Finally groundbreaking took place in February 1962 for the solar observatory on Haleakala. Dedicated two years later it was named the C.E. Kenneth Mees Solar Observatory in honour of the former Kodak senior executive.
Mitsuo Akiyama of the Hawaii Chamber of Commerce sent letters to many American and Japanese Universities in June 1963 suggesting that they consider the possibility of setting up an astronomical observatory on either of Hawaii's two large volcanoes, Mauna Kea and Mauna Loa.(1)
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- Observatories and Telescopes of Modern TimesGround-Based Optical and Radio Astronomy Facilities since 1945, pp. 175 - 188Publisher: Cambridge University PressPrint publication year: 2016