Opposition to the Mauna Kea Observatories has existed since the first telescope was built in the late 1960s. Originally part of research begun by Gerard Kuiper of the University of Arizona, the site has expanded into the world's largest observatory for infrared and submillimeter telescopes. Opposition to the telescope from residents in the city of Hilo, Hawaii were concerned about the visual appearance of the mountain and Native Hawaiians voiced concerns over the site being sacred to the Hawaiian religion as the home of several deities. Environmental groups and activists have been expressing concern over endangered species habitat.
The Outrigger Telescopes Project, intended to build from four to six comparatively small telescopes for interferometry, was to surround the Keck telescopes. [1] It was cancelled in 2006, after a court found NASA's Environmental Impact Statement was improperly limited to just the telescope area. [2] [3]
An ongoing proposal for one of the world's largest optical telescopes, the Thirty Meter Telescope (TMT) was the focus of protests concerning the continued development of the mountain Hawaiians consider the most sacred peak in the island chain. On 30 October 2018, the Supreme Court of Hawaii approved the resumption of construction of the TMT. [4] [5]
After studying photos for NASA's Apollo program that contained greater detail than any ground-based telescope, Gerard Kuiper began seeking an arid site for infrared studies. [6] [7] While he first began looking in Chile, he also made the decision to perform tests in the Hawaiian Islands. Tests on Maui's Haleakalā were promising but the mountain was too low in the inversion layer and often covered by clouds. On the "Big Island" of Hawaii, Mauna Kea is considered the highest island mountain in the world. While the summit is often covered with snow the air itself is extremely dry. [6] Kuiper began looking into the possibility of an observatory on Mauna Kea. After testing, he discovered the low humidity was perfect for infrared signals. He persuaded then-Governor John A. Burns to bulldoze a dirt road to the summit where he built a small telescope on Puʻu Poliʻahu, a cinder cone peak. [6] [8] [9] The peak was the second highest on the mountain with the highest peak being holy ground, so Kuiper avoided it. [10] Next, Kuiper tried enlisting NASA to fund a larger facility with a large telescope, housing and other needed structures. NASA, in turn decided to make the project open to competition. Professor of physics, John Jefferies of the University of Hawaii placed a bid on behalf of the university. [6] [11] [12] Jefferies had gained his reputation through observations at Sacramento Peak Observatory. The proposal was for a two-meter telescope to serve both the needs of NASA and the university. While large telescopes are not ordinarily awarded to universities without well established astronomers, Jefferies and UH were awarded the NASA contract, infuriating Kuiper who felt that "his mountain" had been "stolen" from "him". [6] [13] Kuiper would abandon his site (the very first telescope on Mauna Kea) over the competition and begin work in Arizona on a different NASA project. After considerable testing by Jefferies' team, the best locations were determined to be near the summit at the top of the cinder cones. Testing also determined Mauna Kea to be superb for nighttime viewing due to many factors including the thin air, constant trade winds and being surrounded by sea. Jefferies would build a 2.24 meter telescope with the State of Hawaii agreeing to build a reliable, all weather roadway to the summit. Building began in 1967 and first light seen in 1970. [6]
Some of the people on the Big Island were concerned that the whole thing had got out of hand and the University of Hawaii was going to take over the top of the mountain, push all the skiers off and push all the hunters off, and essentially develop, in the worst sense, the side of the mountain. The Big Island is a rural community and there are a lot of people there who are not very sophisticated, as you know. They are nervous about changes in lifestyles, and they see those following on the development of the program of astronomy as just about as far removed from their daily pursuits as they possibly can be. And they do not trust the University, State, or Federal government worth a damn.
They feel—and in some cases I’ve had this said to me—that they are going to lose all access to the mountain because of these programs. The Federal government is going to come in and it's going to slowly move down the mountain, taking more and more of the mountain over as more and more programs go up there, and no-one will be able to get there. It is very hard to fight a fear of this kind—a formless, baseless concern—except through the same kind of backwoods interaction, at a grassroots level.
In Honolulu, the governor and legislature, enthusiastic about the development, set aside an even larger area for the observatory causing opposition in the main city of the Big Island, Hilo. Native Hawaiians believe the entire site to be sacred and that developing the mountain, even for science, would spoil the area. Environmentalists were concerned about rare native bird populations and other citizens of Hilo were concerned about the sight of the domes from the city. Using town hall meetings, Jefferies was able to overcome opposition by weighing the economic advantage and prestige the island would receive. [6]
There has been substantial opposition to the Mauna Kea observatories that continues to grow. [15] By 1977 Jefferies stated that the Mayor of Hawaii County had joined existing hunting and environmentalist opposition. [14] Over the years, the opposition to the observatories may have become the most visible example of the conflict western science has encountered over access and use of environmental and culturally significant sites. [16] Opposition to development grew shortly after expansion of the observatories commenced. Once access was opened up by the roadway to the summit, skiers began using it for recreation and objected when the road was closed as a precaution against vandalism when the telescopes were being built. Hunters voiced concerns, as did the Hawaiian Audubon Society, which was supported by Governor George Ariyoshi. [10]
The Audubon Society objected to further development on Mauna Kea over concerns to habitat of the endangered palila, an endemic species to only specific parts of this mountain. The bird is the last of the finch billed honeycreepers existing on the island. Over 50% of native bird species had been killed off due to loss of habitat from early western settlers, or the introduction of non-native species competing for resources. Hunters and sportsmen were concerned that the hunting of feral animals would be effected by the telescope operations. [17] A "Save Mauna Kea" movement was inspired by the proliferation of telescopes, with opposition believing development of the mountain to be sacrilegious. [18] Native Hawaiian non-profit groups, such as Kahea, (whose goals are the protection of cultural heritage and the environment), oppose development on Mauna Kea as a sacred space to the Hawaiian religion. [19] Today, Mauna Kea hosts the world's largest location for telescope observations in infrared and submillimeter astronomy. The land itself is protected by the U.S. Historical Preservation Act due to its significance to Hawaiian culture, but this still allowed development. [20]
Development of the Mauna Kea observatories is still opposed by environmental groups and Native Hawaiians. A 2006 proposal for the Outrigger Telescopes to become extensions of the Keck Observatory was canceled after a judge's determination that a full environmental impact statement must be prepared before any further development of the site. [21] The "outrigger" would have linked the Keck I and Keck II telescopes. Environmental groups and Native Hawaiian activists were much stronger in their opposition this time than they had been in the past, but NASA went ahead with the proposal for lack of an alternate site. The group Mauna Kea Anaina Hou made several arguments against the development, including that Mauna Kea was a sacred mountain to Native Hawaiians where many deities live, and that the cinder cone location being proposed was holy in Hawaiian tradition as a burial site for a demi-god. The group raised several other concerns, such as environmental, concern for the preservation of native insects, the question of Ceded lands, and an audit report critical of the mountain's management. [22]
The Thirty Meter Telescope (TMT) is a proposal for a large, segmented, mirror telescope, planned for the summit of Mauna Kea. The TMT has become a focal point for protests against further development of the observatory site, and a legal battle was fought through the Hawaii court system. The Supreme Court of Hawaii approved the resumption of construction of the telescope on 31 October 2018. [4]
The TMT project is a response to a recommendation in 2000 from the US National Academy of Sciences that a thirty-meter telescope be the top priority and be built within the decade. [23] Urgency in construction is due to the competitive nature of science with the European-Extremely Large Telescope also under construction. [24] Mauna Kea's summit is the most sacred of all the mountains in Hawaii to many, but not all, Native Hawaiian people. [25] Hawaiian cultural practitioners cite impacts to indigenous cultural practice, while recreational users have argued that construction harms the scenic view plane. Some environmentalists are concerned that irreparable ecological damage may be done by construction, although this has been disputed by other environmental advocates. [26] All three groups are represented among the petitioners opposing the TMT. [27] According to the State of Hawaii law HAR 13-5-30, the eight key criteria must be met before construction be allowed on conservation lands in Hawaii. Among other criteria, the development may not "cause substantial adverse impact to existing natural resources within the surrounding area, community, or region," and the "existing physical and environmental aspects of the land must be preserved or improved upon." [28]
Native Hawaiian activists such as Kealoha Pisciotta, a former employee of the Mauna Kea Observatories, have raised concerns over the telescopes on Mauna Kea desecrating what some Native Hawaiians consider to be their most sacred mountain. [29] Pisciotta, a former telescope systems specialist technician at James Clerk Maxwell Telescope, is one of several people suing to stop the construction, [30] and is also director of Mauna Kea Anaina Hou. [31] As of April 2015, two separate appeals were still pending. [32]
The 1998 study Mauna Kea Science Reserve and Hale Pohaku Complex Development Plan Update stated that "...nearly all the interviewees and all others who participated in the consultation process (Appendices B and C) called for a moratorium on any further development on the summit of Mauna Kea." [33]
The Hawaii Board of Land and Natural Resources gave final approval for the project in September 2017 after a protracted hearing process that included a six month long contested case hearing. [34] This decision was challenged in the Hawaii State Supreme Court the following year. The court ruled that the DLNR decision was valid and that construction may proceed. [35]
As of late 2021 construction of the Thirty Meter Telescope remains paused due to the controversy and ongoing effects of the COVID-19 pandemic. The 2020 Decadal report of the National Science Foundation has recommended federal investment in the TMT project. [36] The controversy surrounding construction of the Thirty Meter Telescope continues. Independent polls commissioned by local media organizations [37] [38] show consistent support for the project in the islands with over two thirds of local residents supporting the project. These same polls indicate Native Hawaiian community support remains split with about half of Hawaiian respondents supporting construction of the new telescope.
A July 2022, state law [39] responds to the protests by removing sole control over the master land lease from the University of Hawaii. After a joint transition period from 2023 to 2028, control will shift to the new Mauna Kea Stewardship and Oversight Authority, which will include representatives from the University, astronomers and native Hawaiians. [40]
Timeline of telescopes, observatories, and observing technology.
The United Kingdom Infra-Red Telescope (UKIRT) is a 3.8 metre (150 inch) infrared reflecting telescope, the second largest dedicated infrared telescope in the world. It is located on Mauna Kea, Hawai'i as part of Mauna Kea Observatory. Until 2014 it was operated by the Joint Astronomy Centre in Hilo. It was owned by the United Kingdom Science and Technology Facilities Council. UKIRT is currently being funded by NASA and operated under scientific cooperation between Lockheed Martin Advanced Technology Center, the University of Hawaii, and the U. S. Naval Observatory. The telescope is set to be decommissioned after completion of the Thirty Meter Telescope as part of the Mauna Kea Comprehensive Management Plan.
The W. M. Keck Observatory is an astronomical observatory with two telescopes at an elevation of 4,145 meters (13,600 ft) near the summit of Mauna Kea in the U.S. state of Hawaii. Both telescopes have 10 m (33 ft) aperture primary mirrors, and, when completed in 1993 and 1996, they were the largest optical reflecting telescopes in the world. They are currently the third and fourth largest.
Mauna Kea is dormant shield volcano on the island of Hawaiʻi. Its peak is 4,207.3 m (13,803 ft) above sea level, making it the highest point in Hawaii and the island with the second highest high point, behind New Guinea, the world's largest tropical island with multiple peaks that are higher. The peak is about 38 m (125 ft) higher than Mauna Loa, its more massive neighbor. Mauna Kea is unusually topographically prominent for its height: its prominence from sea level is fifteenth in the world among mountains, at 4,207.3 m (13,803 ft); its prominence from under the ocean is 9,330 m (30,610 ft), rivaled only by Mount Everest. This dry prominence is greater than Everest's height above sea level of 8,848.86 m (29,032 ft), and some authorities have labeled Mauna Kea the tallest mountain in the world, from its underwater base. Mauna Kea is ranked 8th by topographic isolation.
The Mauna Kea Observatories (MKO) are a group of independent astronomical research facilities and large telescope observatories that are located at the summit of Mauna Kea on the Big Island of Hawaiʻi, United States. The facilities are located in a 525-acre (212 ha) special land use zone known as the "Astronomy Precinct", which is located within the 11,228-acre (4,544 ha) Mauna Kea Science Reserve. The Astronomy Precinct was established in 1967 and is located on land protected by the Historical Preservation Act for its significance to Hawaiian culture. The presence and continued construction of telescopes is highly controversial due to Mauna Kea's centrality in native Hawaiian religion and culture, as well as for a variety of environmental reasons.
The Canada–France–Hawaii Telescope (CFHT) is located near the summit of Mauna Kea mountain on Hawaii's Big Island at an altitude of 4,204 meters, part of the Mauna Kea Observatory. Operational since 1979, the telescope is a Prime Focus/Cassegrain configuration with a usable aperture diameter of 3.58 metres (11.7 ft).
Roque de los Muchachos Observatory is an astronomical observatory located in the municipality of Garafía on the island of La Palma in the Canary Islands, Spain. The observatory site is operated by the Instituto de Astrofísica de Canarias, based on nearby Tenerife. ORM is part of the European Northern Observatory.
Hāmākua is a district on the northeast coast of Hawaiʻi's Big Island, administered by the County of Hawaiʻi in the state of Hawaiʻi. It is also the name given for the coastline in the region, the "Hāmākua Coast".
The Thirty Meter Telescope (TMT) is a planned extremely large telescope (ELT) proposed to be built on Mauna Kea, on the island of Hawai'i. The TMT would become the largest visible-light telescope on Mauna Kea.
A segmented mirror is an array of smaller mirrors designed to act as segments of a single large curved mirror. The segments can be either spherical or asymmetric. They are used as objectives for large reflecting telescopes. To function, all the mirror segments have to be polished to a precise shape and actively aligned by a computer-controlled active optics system using actuators built into the mirror support cell.
The University of Hawaiʻi 88-inch (2.24-meter) telescope—called UH88, UH2.2, or simply 88 by members of the local astronomical community—is situated at the Mauna Kea Observatories and operated by the University's Institute for Astronomy. It was constructed in 1968, and entered service in 1970, at which point it was known as "The Mauna Kea Observatory". It became one of the first professional telescopes to be controlled by a computer. The telescope was built with funding from NASA, to support Solar System missions, and is controlled by the University of Hawaiʻi. The success of the telescope helped demonstrate the value of Mauna Kea for astronomical observations.
Alexei Vladimir "Alex" Filippenko is an American astrophysicist and professor of astronomy at the University of California, Berkeley. Filippenko graduated from Dos Pueblos High School in Goleta, California. He received a Bachelor of Arts in physics from the University of California, Santa Barbara in 1979 and a Ph.D. in astronomy from the California Institute of Technology in 1984, where he was a Hertz Foundation Fellow. He was a postdoctoral Miller Fellow at Berkeley from 1984 to 1986 and was appointed to Berkeley's faculty in 1986. In 1996 and 2005, he was a Miller Research Professor, and he is currently a Senior Miller Fellow. His research focuses on supernovae and active galaxies at optical, ultraviolet, and near-infrared wavelengths, as well as on black holes, gamma-ray bursts, and the expansion of the Universe.
An extremely large telescope (ELT) is an astronomical observatory featuring an optical telescope with an aperture for its primary mirror from 20 metres up to 100 metres across, when discussing reflecting telescopes of optical wavelengths including ultraviolet (UV), visible, and near infrared wavelengths. Among many planned capabilities, extremely large telescopes are planned to increase the chance of finding Earth-like planets around other stars. Telescopes for radio wavelengths can be much bigger physically, such as the 300 metres aperture fixed focus radio telescope of the Arecibo Observatory. Freely steerable radio telescopes with diameters up to 100 metres have been in operation since the 1970s.
The Gordon and Betty Moore Foundation is an American foundation established by Intel co-founder Gordon E. Moore and his wife Betty I. Moore in September 2000 to support scientific discovery, environmental conservation, patient care improvements and preservation of the character of the San Francisco Bay Area.
The Onizuka Center for International Astronomy, also known as Hale Pōhaku, is a complex of support facilities for the telescopes and other instruments that comprise the Mauna Kea Observatory atop Mauna Kea, on Hawaiʻi island.
Charles Mattias ("Matt") Mountain is currently the President of the Association of Universities for Research in Astronomy (AURA) which designs, builds, and operates telescopes and observatories for the National Science Foundation (NSF) and the National Aeronautics and Space Administration (NASA). AURA's NASA center is the Space Telescope Science Institute (STScI), responsible for the science mission for the Hubble Space Telescope, the science and operations for the James Webb Space Telescope, and the MAST data archive. AURA's NSF centers are Gemini Observatory, the National Optical Astronomy Observatory (NOAO), and the National Solar Observatory (NSO). Dr. Mountain and AURA are also responsible for the NSF construction projects: the Daniel K. Inouye Solar Telescope (DKIST) on Haleakalā, Hawaii and the Large Synoptic Survey Telescope (LSST) on Cerro Pachón in Chile.
Puʻu Huluhulu is a volcanic cone located near the center of the Island of Hawaii in the State of Hawaii. It is located on the southern side of Hawaii Route 200, directly across from the highway's intersection with the Mauna Kea Access Road. Puʻu Huluhulu is Hawaiian for hairy hill.
The Thirty Meter Telescope (TMT) protests are a series of protests and demonstrations that began on the Island of Hawaii over the choosing of Mauna Kea for the site location of the Thirty Meter Telescope. Mauna Kea is the most sacred dormant volcano of Native Hawaiian religion and culture, and was known to natives as the home to Wākea, the sky god. Protests began locally within the state of Hawaii on October 7, 2014 but went global within weeks of the April 2, 2015 arrest of 31 people who had blockaded the roadway to keep construction crews off the summit.
Kapu aloha is an evolving, philosophical code of conduct that is culturally informed by Kanaka Maoli ontologies and epistemologies, being expressed politically through non-violent direct action, and ceremonially through behavioral conduct in alignment with Kanaka Maoli cultural practices and notions of the sacred. The term kapu aloha comes from the merging of two foundational Hawaiian language words kapu, and aloha. Kanaka Maoli cultural practitioners maintain that kapu aloha evolved from an unspoken cultural edict surrounding ceremony. As the practice of kapu aloha started to infiltrate the political realm, its ethos and praxis spread to include non-Kanaka Maoli settler-allies and those unfamiliar with Native Hawaiian culture.
Mauna Kea Anaina Hou and its sister group, Mauna Kea Hui, are indigenous, Native Hawaiian, cultural groups with environmental concerns located in the state of Hawaii.