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RUTHERFORD APPLETON LABORATORY
RALFacilities
Further reading

Site
Site plans and photographs
R1
R2
NIMROD
Britain Builds Proton Synchrotron
Excavating NIMROD
Nimrod operational Tannoy announcement
R3 building plans
ISIS
Neutron and muon source
Animated overview
Inauguration of ISIS
Space
NASA Ground Station
NASA 12m Antenna
James Clerk Maxwell Telescope (JCMT)
Lasers
R1 extension (1977)
Titania (1994-1999)

The James Clerk Maxwell Telescope at Maunakea, Hawaii

Work as part of the Harwell Heritage Project rediscovered a set of photographs and original artwork of the JCMT. Technical input from Malcolm Currie (RAL Space) and the loan of some wonderful little souvenirs of his time working on the telescope made an interesting display in the Library "airlock" April/May 2023.

The James Clerk Maxwell Telescope (JCMT) is named after the Scottish physicist renowned for developing the theory of light on which observational astronomy is based.

The telescope is situated on the volcanic peak of Maunakea* in Hawaii and is the world's most successful single-dish telescope for observing sub-millimetre wavelengths in the electromagnetic spectrum. Since it began operating in 1987 it has been associated with a number of major scientific discoveries, and continues to do world-class science as part of programmes such as the Event Horizon Telescope. Until February 2015 JCMT was funded by a partnership between the UK, Canada and the Netherlands. It was then taken over by the East Asian Observatory and is funded by various national astronomy institutes from China, Japan, South Korea and Taiwan.

* The name Maunakea means "white mountain" because of the snow on its peak.

Discovering the universe

Faint discs surround many stars suggesting the presence of larger unobservable bodies such as planets.  The SCUBA programme measured the low-level thermal emission from dust grains in such discs and discovered that peak flux occurred in two distinct regions much like an edge-on torus (doughnut-like) structure. The central "hole" contains significantly less dust which indicates that the region has been cleared of gas and dust by the formation of numerous small celestial bodies, or planetesimals.

Faint discs surround many stars suggesting the presence of larger unobservable bodies such as planets. The SCUBA programme measured the low-level thermal emission from dust grains in such discs and discovered that peak flux occurred in two distinct regions much like an edge-on torus (doughnut-like) structure. The central "hole" contains significantly less dust which indicates that the region has been cleared of gas and dust by the formation of numerous small celestial bodies, or planetesimals.
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The JCMT is part of the Event Horizon Telescope (EHT) which is a "virtual observatory" of eight radio receivers across the globe.  In April 2019 astronomers announced they had accomplished the seemingly impossible and had taken a picture of a black hole, a cosmic monster from which light itself cannot escape its clutches. Einstein predicted this in 1915 with his Theory of General Relativity.  The image shows the shadowy face of a 6.5-billion-solar-mass supermassive black hole at the core of Messier 87, a large elliptical galaxy 55 million light-years from Earth.

The JCMT is part of the Event Horizon Telescope (EHT) which is a "virtual observatory" of eight radio receivers across the globe. In April 2019 astronomers announced they had accomplished the seemingly impossible and had taken a picture of a black hole, a cosmic monster from which light itself cannot escape its clutches. Einstein predicted this in 1915 with his Theory of General Relativity. The image shows the shadowy face of a 6.5-billion-solar-mass supermassive black hole at the core of Messier 87, a large elliptical galaxy 55 million light-years from Earth.
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© UKRI Science and Technology Facilities Council

Finding a site

After a number of false starts, work on what was initially called the UK Millimetre-wave Telescope got underway in 1975. Detailed design work proceeded quite rapidly, but the issue of finding a site proved more difficult. Hawaii was the obvious choice but Maunakea is sacred land and the volcano is in a conservation area so the proposal to build a second telescope in addition to UKIRT (UK Infra Red Telescope) was controversial. Attention switched to La Palma in the Canary Islands and negotiations began. Then someone pointed out that if the telescope needed to get above the water vapour, La Palma simply wasn't high enough... but Maunakea was. Fortunately, circumstances in Hawaii had changed by this time so work recommenced on Maunakea.

The breaking ground ceremony was held in April 1983 and the Hawaiian fire goddess Pele was asked for her good favours.

The breaking ground ceremony was held in April 1983 and the Hawaiian fire goddess Pele was asked for her good favours.
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The dish

JCMT was designed at Appleton then Rutherford Appleton Laboratories. Its 15 metre diameter dish comprises 276 curved aluminium reflecting panels which were fabricated at RAL to an accuracy of 24 microns (about the thickness of a piece of tissue paper). The fabrication of the steel for the telescope took place at a factory in Ijmuiden near Amsterdam, followed by a test assembly and development of the various drives. It was then shipped to Hawaii and by late 1985 the main parts were on the mountain with an enthusiastic team ready to do the assembly.

Assembly in Holland.

Assembly in Holland.
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There were a few hairy moments lifting the reflector structure into the enclosure but by the end of 1986 the telescope was just about ready for first light.  The telescope and enclosure revolved together on a carousel.  Looking out of the dome the movement of the carousel is so smooth it feels as though you are sitting still and the whole world is revolving around you.

There were a few hairy moments lifting the reflector structure into the enclosure but by the end of 1986 the telescope was just about ready for first light. The telescope and enclosure revolved together on a carousel. Looking out of the dome the movement of the carousel is so smooth it feels as though you are sitting still and the whole world is revolving around you.
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© UKRI Science and Technology Facilities Council

Many institutes contributed to the JCMT including the Netherlands Science Foundation (ZWO), the UK's SRC Appleton and Rutherford Laboratories, and the National Research Council, Canada.

The Joint Astronomy Centre (JAC)

The Joint Astronomy Centre (JAC) in Hilo is about 42 miles from the JCMT and was built in 1980 as a base for visiting astronomers from around the world.

The Joint Astronomy Centre (JAC) in Hilo is about 42 miles from the JCMT and was built in 1980 as a base for visiting astronomers from around the world.
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© UKRI Science and Technology Facilities Council

To get to the telescope you drove about an hour from the JAC to Hale Pohaku then acclimate over-night to the 9300 feet (2800 metres) altitude. For the last half hour of your journey you wind your way through several switchbacks before emerging onto what looks very much like a lunar landscape. You were not allowed to stay long however -- for safety reasons there was a limit of 14 hours per night at the summit.

Malcolm Currie, the technical consultant for this display, worked for some years in the Scientific Computing Group at the JAC.  He says that the occasional nights at the telescope was always a thrill, seeing new data as it arrived, and at the end driving across the lunar landscape you could sometimes see the red glow from Kilauea volcano... when there wasn't a sea of cloud beneath you.

Malcolm Currie, the technical consultant for this display, worked for some years in the Scientific Computing Group at the JAC. He says that the occasional nights at the telescope was always a thrill, seeing new data as it arrived, and at the end driving across the lunar landscape you could sometimes see the red glow from Kilauea volcano... when there wasn't a sea of cloud beneath you.
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© UKRI Science and Technology Facilities Council

A remote-control centre (JROC) was established in 2013 to avoid the drive, have more time for observations and so make the telescope more productive. It is also much easier to think clearly at sea level than at 13400 feet (4000 metres).

Opening ceremony

The telescope was opened on Monday 27th April 1987 by HRH Prince Philip who unveiled a plaque and looked to be enjoying himself at the celebrations afterwards. The opening was mostly memorable for the fact that when the traditional "lever to start the first observation" was pressed, nothing happened because one of the VIP guests was leaning on the emergency stop button.

Plaque.

Plaque.
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© UKRI Science and Technology Facilities Council

In the photo are:
Roy Tolcher (Head of Council Works Unit, SERC), Dr Don Hall (University of Hawaii), 
Sir John Clerk (descendant of James Clerk Maxwell), HRH Prince Philip, Duke of Edinburgh, 
Mrs Lynne Waihee (deputising for her husband, the Governor of Hawaii), Dante Carpenter (Mayor of Hawaii County), 
Professor Bill Mitchell (Chairman, SERC), Dr Bernard Gingras (NRC, Canada), Dr Paul Williams (Director of RAL), 
Dr Albert Mulder (ZWO, Netherlands), Professor Richard Hills (Project Scientist), Brian Edwards (Project Engineer).

In the photo are: Roy Tolcher (Head of Council Works Unit, SERC), Dr Don Hall (University of Hawaii), Sir John Clerk (descendant of James Clerk Maxwell), HRH Prince Philip, Duke of Edinburgh, Mrs Lynne Waihee (deputising for her husband, the Governor of Hawaii), Dante Carpenter (Mayor of Hawaii County), Professor Bill Mitchell (Chairman, SERC), Dr Bernard Gingras (NRC, Canada), Dr Paul Williams (Director of RAL), Dr Albert Mulder (ZWO, Netherlands), Professor Richard Hills (Project Scientist), Brian Edwards (Project Engineer).
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© UKRI Science and Technology Facilities Council

The voyage of the enclosure

The telescope sits inside an enclosure which incorporates a blind to protect it from wind and solar heat during daytime observations.

The telescope sits inside an enclosure which incorporates a blind to protect it from wind and solar heat during daytime observations.
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© UKRI Science and Technology Facilities Council

The steel-work for the enclosure was made in Bolton. The plan was to ship it to Hawaii using a large boat but that broke down so the shipping company subcontracted to a small freighter which set off on its voyage barely visible under the large pile of steel lashed to its deck. It all went quiet for several weeks then information was received that the freighter had not gone directly to Hawaii as planned, but rather to Holland where it loaded up with a second cargo... of high explosives. There was an additional delay before it could get through the Panama Canal whereupon it vanished again, probably to off-load the explosives in Ecuador.

By the time the freighter reached Hawaii the penalty clauses for late delivery were nearly equal to the total fee for the charter. The captain stopped outside the territorial waters and demanded full payment of the original price or he would off-load the steel into the sea. Fortunately JCMT staff were able to obtain a writ for piracy on the high seas so the US Coastguard went out, arrested the captain (at gunpoint!), took possession of the boat and towed it safely into Hilo.

Mahalo!

Mahalo!
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© UKRI Science and Technology Facilities Council

Display.

Display.
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© UKRI Science and Technology Facilities Council

Display.

Display.
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See also:

The James Clerk Maxwell Telescope / A guide for the propective user (1991)

The James Clerk Maxwell Telescope / A guide for the propective user (1991)
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© UKRI Science and Technology Facilities Council
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