KEY TO INSTALLATIONS
- IAC Residencia
- 17m MAGIC
- 10.4m GTC
- 3.6m TNG
- 2.5m NOT
- 18cm CMT
- 4.2m WHT
- 45cm DOT
- 1m SST
- Super WASP
- 1m JKT
- 2.5m INT
- 1.2m MERCATOR
- 2m LIVERPOOL
The Isaac Newton Group of Telescopes forms but one part of the Observatorio del Roque de Los
Muchachos (ORM). So named after a volcanic rock formation on the highest point of La Palma. The
ORM is multi-national observatory with several European countries participating. These being: Belgium,
Germany, Italy, The Netherlands, Spain, the United Kingdom and the Nordic countries of Sweden, Norway,
Denmark, Finland and Iceland. The site is administered by the Instituto
de Astrofísica de Canarias (IAC). The installations at the ORM currently being:
Conventional Telescopes
Solar Telescopes
Specialised Telescopes
A TOUR AROUND THE ORM
View to the north showing the Residencia and the MAGIC telescopes
The helicopter pads were built for the Royal Inauguration of the observatory on the
29th June 1985 and are still used occasionally by visiting dignitaries or the emergency services. The
residencia provides accommodation for visiting astronomers and night staff as well as being the refectory
for the site.
View from the road just before entering the site showing the MAGIC, GranTecan and
TNG installations
William Herschel dome, the Swedish and Dutch Open solar telescopes and the enclosure
for the Carlsberg Meridian Telescope
MAGIC I showing the complex lattice work which supports the segmented mirrors
MAGIC II nearing completion (27th Dec 2005)
The dome and buildings of the 10.4m Gran Telescopio Canarias (GranTeCan)
This telescope is nearing completion and expected to see
First Light in 2006. Until more
grandiose projects are built, this telescope will become the largest 'single' telescope in the
world. Although based on the 10m 36 segmented mirror Keck design, the aperture is slightly larger.
Progress of the internal construction can be seen by clicking on this
WEBCAM link.
The 3.6m Telescopio Nazionale Galileo (TNG)
The enclosure is designed to optimise the air flow around the telescope to effectively reduce
the 'dome seeing' and improve image quality. This telescope with its active primary mirror support
system is very impressive. The Nasmyth image derotators mounted on the fork look into well ventilated
observing halls at each side of the telescope. The various imaging cameras and spectrographic
instruments are permanently attached to the rotators so eliminating the need for instrument changes.
The 2.5m Nordic Optical Telescope (NOT)
A unique feature is that the dome is fixed and entire structure rotates. A visiting NOT astronomer
once told me he would never know where the entrance/exit would end up after a nights observing and
was thankful for the walkway!
The domes of ING telescopes, the solar towers and the Liverpool and Mercator
telescopes
The Liverpool Telescope
The clam shell enclosure of the Liverpool Telescope provides an ideal housing. When open, the telescope
is totally exposed and free from the effects of air currents which circulate in conventional domes and
degrade image quality. The Liverpool telescope works remotely with the telescope and data acquisition
operations controlled via the Internet.
The 1.2m Mercator (Belgium) and 2m Liverpool (UK) telescopes as seen from the
roof of the INT
The 'Roll off Shed' enclosure of Super WASP with the JKT above
This is one of the latest installations at the ORM and came in operation in April 2004. The
instrument consists of a high quality equatorial mount with 8 CCD cameras (using 2k square
chips) each fitted with a Canon 200mm f/1.8 lens. It can image very large blocks of the sky
compared to a conventional telescope and the data taken each night is huge.
Site of the Polaris Trail Telescope (1972)
The structure made of cemented local rocks and blocks (to the left of the geographic trig point)
was made to support a special telescope pointed to the North Star (Polaris) and used to determine
the observing conditions of the site. Based on the observations, the island La Palma would eventually
be chosen to build what was then to be called 'The Northern Hemisphere Observatory'. Click
here for more information.
The JKT and INT buildings high above a sea of cloud
A photo from 1986 and was my first taken at the observatory. Seeing how perfect the sky is at this
altitude, its hardly surprising the RGO decided to move their operations from Herstmonceux to La Palma!
The Isaac Newton Telescope building in 1986
In those days, many RGO staff were on tours of duty for a few years. To make us feel not quite so
home sick, a bus stop sign (think it was 'borrowed' from from Hastings!) was fixed on the east side
of the building where the fleet cars pulled up on arrival... A nice touch! I too expected to return
to RGO after my 3 year tour in 1989, but I never did.
The Carlsberg Meridian Telescope (CMT)
This is the oldest telescope at the ORM and was made by Grubb Parsons in 1952. It was
originally used at the Copenhagen University Observatory (CUO) from 1964 to 1976, but
was then converted for automatic observations and renamed the Carlsberg Automatic
Meridian Circle when it came into operation on La Palma in 1984. Carlsberg of
"Probably the Best Lager in the World" fame were one of the main sponsors
at the time, hence the name. It has gone through many upgrades over the years and since
1997 works remotely.
I took this photo (in 1986) at twilight when the building had just opened up and the
telescope was doing its first calibration run. A precision divided glass setting circle
read by (I think) six optical reading heads around its circumference determines the angular
position of the telescope. The readings from the heads are averaged out and that value
taken at the time of observation.
The telescope is shown observing the nadir using a light source reflected back from a mercury
pool situated in a floor well between the piers. This calibrates the telescope in the vertical
plane. For horizontal calibration, collimator tubes utilising a light source are used. The
north collimator tube can seen in the foreground. From what I recall, the CMT does these
calibration checks at intervals throughout the night after its completed a number of
observations.