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About La Silla |
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La Silla is a 2400-m mountain, bordering the southern extremity of the Atacama desert in Chile. It is located about 160 Km north of La Serena. Its geographical coordinates are: Latitude 29º 15' south & Longitude 70º 44' west. Originally known as Cinchado, the mountain was renamed La Silla (the saddle) after its shape. It rises quite isolated and remote from any artificial light and dust sources (astronomy's worst enemies). La Silla was the first ESO observatory built in Chile. Its history is full of optimism and disappointments, ups and downs, since its beginnings in the 50's until the middle of the 70's when the observatory became a reality.
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La
Silla air view
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The Idea of
a European Southern Observatory is Born
The Idea of a European Southern Observatory is Born
The
idea of establishing a common large observatory that joined the European
astronomers was born in the spring of 1953, in the mind of the renowned
astronomer Walter Baade. This suggestion was then discussed, for the first
time, by a group of astronomers at Leiden on June 21, 1953, after which
they were invited to discuss it with their colleagues at home. Some months
later, on January 26, 1954, twelve leading astronomers from six European
countries: Belgium, United Kingdom, France, Germany,
the Netherlands and Sweden gathered in the Senate Room of
Leiden University to discuss the idea of the recently suggested joint European
observatory. Here, they issued a historical statement, which expressed the
wish that the scientific organizations in their respective home countries
recommended the establishment of a joint observatory in South Africa, equipped
with a 3-m aperture telescope and a Schmidt telescope of 1.2 m aperture.
The project was conceived to be completed over the next ten years and would
need a convention between learned societies or between governments. In order
to develop this project, an ESO Committee (EC) was formed.
The ESO Convention
A first proposal for the convention between organizations
was drafted in November 1954. Some of the most important features in that
draft described the fact that financial contributions had to be proportional
to the national income but only up to a fixed limit. Besides, the draft
stated that the observatory should be located in the southern hemisphere
and should have a large optical telescope and a Schmidt telescope as "Initial
program", considering a future extension with any kind of other instrumentation.
The southern hemisphere was the ideal choice, since most interesting objects
of research could be reached from this hemisphere. In 1962, after years
of meetings and struggles, the ESO Convention was finally signed, but the
required ratifications were only completed early in 1964. Hence, ESO was
finally on solid grounds to begin its long-term building project.
South Africa: The first choice to settle the observatory
Over more than seven years -until the middle of
1963- many European astronomers and their assistants were engaged in the
search for a site in Southern Africa, where many European communities had
observing facilities. South Africa -in particular- was chosen because it
had the best astronomical climate known at that time. However, by the end
of 1963, it was clear that the observatory could not be built in this continent,
mainly because of the deterioration of the atmospheric seeing in the course
of the night, as a result of the decrease in the temperature.
The Andes Versus South Africa
The first explorations in the Andes had been already
performed in March 1959 by G. P. Kuiper, followed in April 1959, by the
astronomer Jürgen Stock, whose site survey for an AURA project grew in importance
when outstanding conditions appeared to be found to the north of Santiago.
During 1962, towards the end of the site testing in South Africa, ESO became
more interested in the possibilities offered by the Andes Range in South
America. By June 1963, a small group of members of the EC was sent to Chile
to carry out further investigations. Thus, in June 6, two groups formed
by members of ESO and AURA visited Santiago and La Serena areas, where they
worked on two mountains on the AURA territory: Tololo and a mountain named
Morado. This last mountain was suggested -by AURA- as a suitable location
for the ESO observatory because of its large surface and well-tested favorable
observing conditions. At this point, a principal subject of discussion was
the possible relation between the AURA and the ESO projects in case ESO
should decide to settle in Morado. In a new meeting of the EC in November
15, 1963, a report was prepared on behalf of the Site Selection Committee,
which showed a comparison of the data collected in South Africa and Tololo.
Finally, the EC decided unanimously to choose the South American site over
South Africa for the location of the ESO observatory, based on the superiority
of the climatic and observing conditions.
ESO Signs the Contract to Purchase La Silla
In October 30, 1964 a contract was signed in Santiago
between ESO and the Government of Chile, for the purchase of an area of
627 km2 including the mountain La Silla. The relatively low price paid by
ESO, showed the interest on the part of the Chilean Government in having
the observatory established in Chile.
The Growth of La Silla During 1964-1966
At the end of 1964, ESO had an office in La Serena
functioning with five people, and had already a road project from Pelícano
camp to the top of La Silla. The year 1965 saw much more progress, since
apart from the road construction, Pelícano camp began to take its more definite
shape. Similarly, a small temporary camp was constructed at La Silla, which
included a storage room, some living quarters, a powerhouse and a temporary
workshop. A year later, in 1966 a second, and more definite camp, was constructed
near the top of La Silla. In January of that same year, the road connection
to La Silla was completed; then, on March 24, 1966, the dedication of the
road took place with the presence of many authorities and guests, such as
the Archbishop of La Serena and the ESO’s President G. W. Funke.
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*
May 1967: The building for the 1.5-m Telescope. On the left, part
of the provisional dome for the 1-m telescope.
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* December 1967: La Silla's earliest Residential Quarters, Office Buildings, Catering Facilities for nigth and day workers, etc. |
The Inauguration
Three years after the dedication of the road,
the first stage of the constructions had been finally completed, the middle-size
telescopes had become operational while the hotel, the dormitories, a workshop,
a storage space -among other facilities- had been completed as well. Thus,
in March 25 1969, La Silla Observatory was inaugurated, with an audience
of more than 300 people among Government officials, representatives of AURA
and CARSO (Carnegie Southern Observatory, at las Campanas), besides staff
members of ESO, and other guests. After two decades of growth, since the
first initiatives towards La Silla creation in June 1953, the dream had
become a reality.
The Telescopes
In 1958 the EC appointed an Instrumentation Committee
(IC), which should be in charge of the future instrumentation in La Silla.
The IC was given two main tasks: preparing all technical and financial aspects
of the instrumentation so as to enable the EC to take the necessary decisions,
and making all necessary technical and instrumental decisions within the
frame of the budget. Hence, one of the IC’s first assignments was the specification
of the telescopes in La Silla; thus in 1961, they recommended the construction
of the middle-size telescopes: 1 m and 1.5 m, both
erected only in the second half of the 1960s. In 1968, the GPO (Grand
Prism Objectif) was installed in La Silla to resume its work after eight
years of service in the site testing activities in South Africa. In 1971,
the 1.2-m Schmidt was finally installed in La Silla, as was the ESO
50 cm -a duplicate of the Copenhagen 50 cm-. Then, in November 1976,
the largest telescope foreseen in the "initial program" the 3.6 m
saw "first light". Subsequently, a 1.4-m CAT (Coude Auxiliary Telescope)
would feed a high-resolution spectrograph within the 3.6-m telescope
building. In 1984, the 2.2 m began its operations, while in March
1989, the 3.5-m New Technology Telescope (NTT) saw "first light".
Last, but not least, the SEST (Swedish ESO Submillimetre Telescope)
is the only large submillimetre telescope (15-m diameter) in the southern
hemisphere. It was built in 1987 on behalf of the Swedish Natural Science
Research Council (NFR) and the European Southern Observatory.
National Telescopes
An extension of the telescope park not foreseen in the
early days constituted the so-called National Telescopes. These are "telescopes
which are property of one of the member states -or of an institute in
one of these states- which are placed on La Silla and, as compensation
for ESO services, ESO obtains a fraction of the observing time". The first
telescope built under this category was the Bochum 61cm, installed
in September 1968. The second one was the Danish 50 cm (or SAT,
for Strömgren Automatic Telescope) from the Copenhagen University Observatory
in Denmark, whose operation began in 1971. A third one, the Danish
1.5 m, became operational in October 1979. The 90-cm Dutch Telescope
–the "Light Collector", property of the Leiden Observatory in the
Netherlands- was removed from its site at the Leiden Southern Station
in South Africa, and re-erected at La Silla during 1978 and 1979. Lastly,
ESO has granted full operational night to a number of projects run by
their patronizing institutes. These are: Marly 1 m (Marseille Observatory),
the Geneva 1.2 m (Geneva Observatory) and the DENIS (Côte
d’Azur and Paris observatories). Nowadays, roughly nine telescopes are under operation
of which four are national. Others, such as the ESO 50 cm, Schmidt, CAT
1.4 m and Bochum 61 cm, have been decommissioned. The table below lists
all the telescopes in the history of a Silla, including the ones that
are currently active (in blue characters).
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LA
SILLA TELESCOPES
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ESO
Operated Telescopes
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National
Telescopes
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3.6
m
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DENIS
1 m
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2.2
m
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MARLY
1 m (EROS project)
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ESO
1.5 m
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Geneva
1.2 m
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Danish
1.5 m
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Danish
50 cm
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NTT
3.5 m
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Dutch
90 cm
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SEST
15 m
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Marseille
40 cm
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ESO
50 cm
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Bochum
61 cm
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CAT
1.4 m
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IRIS
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Schmidt
1 m
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GPO
(replaced by Marly 1 m)
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