M. A. Gordon
Last changed 5 October 1998
This chapter describes the characteristics of the four Chilean sites to be associated with the operation of the MMA and lists the construction items needed to make each site functional. These sites are the instrument site at Llano de Chajnantor at an elevation of 5,000 m (16,400 ft) in the Andes mountains near 23° S latitude, the principal support site near the village of San Pedro de Atacamaat an elevation of 2,425 m (7,960 ft), a business office near the sea port of Antofagasta, and a business office in the capital of Chile, Santiago. We also consider the NRAO support facilities in the United States.
Site development and operations (see
Chapter 18) are
closely linked. The
physical development of an observatory affects how it operates. Yet, we need to know how an
observatory will operate to build an effective physical plant. The plan for site development
described below is a consequence of our present ideas for operations in Chile. This plan will
surely evolve as we gain experience operating in Chile. Moreover, the Chilean custom of using
high-quality prefabricated buildings in remote areas will allow us to easily make substantive
changes in the physical plant as we discover what works and what does not.
Large, sophisticated optical observatories have operated in remote areas of
Chile for decades.
Indeed, perhaps the most sophisticated observatory of all, the Very Large Telescope (VLT) of
the European Southern Observatory (ESO) is now under construction at a remote site
approximately 96 km (60 miles) south of Antofagasta. Our development plan results from
inspections of these observatories, extensive discussions with their directors past and present,
and our own experience operating radio telescopes in the United States for forty years. To
succeed with the MMA, we will need to be flexible and creative.
A principal feature of the MMA operation will be remote or "service" observing. The local
operations staff will make observations for astronomers. During these observations, these
astronomers will be able to oversee the observing via an Internet connection and, when
necessary, modify the instructions. This mode is now common for the NRAO's VLA and 12-m
telescopes. This situation is similar at many other astronomical observatories. There will be
exceptions, of course, especially during the early years of operations. Data will be transported to
the astronomers probably in the form of magnetic tapes.
The MMA "site" in Chile will involve several locations. The observing site is the location of the
instrument itself, the Llano de Chajnantor in the Andes mountains. The nearby village of San
Pedro de Atacama will serve initially as the construction office and, with a scope that may
change with time, the local operations center. During construction and operations, the MMA
will need a business office near the port of Antofagasta. It will receive ocean, air, and overland
shipments, export material to and from the telescope and local operating site, make local
purchases, and interact with the regional authorities. The MMA will require an office in
Santiago because Chile's head Foreign Office is the only place to process shipping documents
associated with duty-free imports, no matter which Chilean port is used. Finally, the MMA will
rely heavily upon the sophisticated resources of the NRAO sites in the United States. Each of
these Chilean sites will need to be developed. Each of these sites will evolve differently because
of changing requirements as the MMA moves from construction through interim operations into
normal operations.
The telescope site lies at an elevation of 5,000 m (16,500 ft)
in Region II of Chile, at a latitude
of 23° S. Geologically, the site is a "bench" on the western side of the Andes range, with
excellent drainage and a line-of-sight to a nearby community.
Logistically, this site has three important advantages: easy access, proximity to developed
communities, and a gas pipeline. It lies near an international highway (Camino de Paso de
Jama or International Route 27) connecting Chile with Argentina and now being paved. It lies
within a 1-hour drive (approximately 55 km or 34 miles) east of the tourist village of San Pedro
de Atacama (population 1,000); within a 2-hour drive (approximately 180 km or 110 miles)
southeast of the mining support city of Calama (population 120,000) serviced daily by major
Chilean airlines; and within a 5-hour drive (approximately 390 km or 240 miles) east of the port
city of Antofagasta (population 300,000) also serviced daily by Chilean airlines. Finally, a new
high-pressure gas line will pass by the periphery of the site, providing reliable and inexpensive
energy to power gas-turbine electric generators.
Additionally, Chilean telephone companies are now installing broadband, fiber-optic cables and
modern switching systems to link Chilean cities to accommodate the rapidly expanding
economy. We can easily connect the MMA at Llano de Chajnantor into this network either by
fiber-optic cable or state-of-the-art microwave links.
To make this site viable for the MMA, we will need to improve an 18-km (11-mile) existing
mining road (with switchbacks) connecting the Paso de Jama highway with the site. It is likely
that we might also want to improve an existing, straighter, 32-km (20-mile) mining road
connecting the site to the Paso de Jama highway via the eastern side of the nearby hills Cerro
Toco, Cerro Chascon, and Cerro Chajnantor.
Gas Atacama, an international consortium planning the gas pipeline between gas-rich northern
Argentina and energy-thirsty northern Chile, has agreed to route the pipeline near but not
across the MMA site. They will provide a gas tap at a place of our choosing, to allow us to site a
gas turbine electric generating plant to power the MMA itself and the site support facilities.
Energy provided to the site in this form should be reliable, inexpensive, and visually unobtrusive
compared with the option of a high-voltage transmission line between Calama and the Llano de
Chajnantor.
Potable water is a more difficult but solvable problem for the site. The Atacama desert receives
little moisture, although the Andes mountains receive more because of the cooler temperatures
associated with their altitude and their proximity to the wetter, eastern side of the range. The
small, known accumulations of water on the western slopes of the Andes have already been
committed to providing water for desert communities. For example, Antofagasta's water is
piped about 320 km (200 miles) from the Andes to the coast. However, Andes water also
collects into underground aquifers in the valley (Salar de Atacama) where San Pedro de Atacama
lies. The town manager (and, independently, a well driller familiar with the area) has told us that
good water adequate for MMA operations lies approximately 30 m(98 ft) below the surface,
accessible through a well. The simplest way to supply the MMA site would be to process this
water through a treatment plant near San Pedro de Atacama and truck the water to the site as
needed. Alternatively, it may be possible to drill a well at the MMA site itself.
Environmentally, it would be prudent to use this water sparingly at the site by installing low-water toilets and reprocessing grey water, if any. In effect, European Southern Observatory now
does this to supply their VLT site at Cerro Paranal, approximately 96 km (60 miles) south of
Antofagasta.
The remaining locations in Chile will serve to support operation of the
MMA. Their functional
aspects will change as the MMA moves from construction into operations and, correspondingly,
so will the site characteristics. Largely, these changes will depend upon the individual
preferences of the first few Chilean hires, on the Chilean economy at the time of their hiring, on
the cash flow from the funding agencies, and what we learn is necessary to support the array.
Initially, this village will surely be the center of construction operations. It is the closest
community to the MMA site. Built to support its tourist industry, its few modern hotels could
house temporary visitors to the construction operations. The highway connecting it with Calama
is excellent. The runway of its small airport has just been paved and, possibly, commercial
feeder flights may begin to use it in support of the tourist trade.
Land needed for the operations center and for off-center private housing may have limited
availability. San Pedro de Atacama is a village of privately-owned land surrounded by
government or "fiscal" land. Chilean law prevents foreign nationals from owning land within
100 km of an international border. The MMA should plan to lease fiscal land directly from
the government or through an intermediary like the University of Chile or the Catholic
University. Discussions so far indicate there will be no insurmountable problems in this regard.
The extent of the MMA development in San Pedro de Atacama will depend upon how
construction proceeds. We are planning to send antennas to Antofagasta, Chile, by ship and to
San Pedro de Atacama by road in the largest practical modules, so that a minimum of assembly
will be required. If possible, we will assemble the antennas at the 2,425 m (7,960 ft) altitude of
San Pedro, equip the antennas with cabling and electronics, and truck the completed antennas to
the much higher-altitude MMA site. Such an operation would require a 2-storey assembly
building, a machine shop, an electronics workshop, offices, a library, dormitories, a dining
facility, a water treatment plant, and some recreational facilities such as tennis courts and
swimming pool. The extent of these facilities will depend upon how quickly we procure the
antennas, that is, ultimately upon the cash flow from the funding agencies.
The MMA should plan to generate its own electric power in San Pedro de Atacama. At this time,
the village provides electric power by a generator operated only during the early evening
hours. There is no electric power during the day. The better hotels generate their own electricity.
The GasAtacama pipeline will run a few kilometers east of the village. They have agreed
to install a separate side tap to provide natural gas to the MMA operations support
facility (OSF) near the village. Still to be decided is whether to generate electric power
at the tap and bring it to the OSF by high voltage lines, or to install approximately
3 kilometers of 6 inch gas pipe between the tap and the OSF to allow electric power
to be generated at the MMA support facilities. Economic and aesthetic considerations will
influence this decision.
After three antennas have been delivered to the site, limited observing can and should begin to
test the array and to produce astronomical data. Such operations will require high-level support
staff like computer programmers, electronics engineers, and support scientists generally
unavailable locally. These employees, although temporary, may insist upon bringing their
families to Chile and require the MMA project to provide family housing as well, some of which
will surely be in San Pedro de Atacama.
As operations increases and construction wanes, the character of the work and of the support
staff in San Pedro will change. Those remaining will tend to be "permanent" MMA employees,
largely Chilean nationals, who will operate and maintain the array. Buildings suitable for
construction will become unnecessary, and they should be removed. On the other hand,
additional office and laboratory space will be required. Given the widespread use of high-quality
prefabricated buildings in the Chilean mining industry, the MMA should also use such buildings
in San Pedro de Atacama. Prefabricated buildings make it easy to change the physical plant to
adapt to its changing function.
Eventually, MMA operations should become routine, very much like those of NRAO's VLA.
Only a small staff may be required in San Pedro de Atacama, and most of the support staff could
be moved to a Chilean city with more amenities such as Antofagasta where employee recruitment
and retention will be easier. At this stage, the physical plant in San Pedro could be further
reduced if prefabricated buildings are used.
Whatever the evolution of MMA operations based in San Pedro de Atacama, the MMA
management needs to be sensitive to the character of the village. It is an international tourist
destination because of its 16th century architecture, its geothermal areas, its pre-Columbian
archeological sites, its indigenous Atacamañan residents, and its unique charisma. The village
itself has strict architectural codes. Our location with respect to the village and the architecture
of our buildings will affect our being accepted as desirable members of the community.
In Region II, Antofagasta is the important city. It is the economic and administrative capital of
the region. It is an international port. It has several commercial flights each day. It has at least
one English-language international school. It has two small universities, and it is the largest city
in Region II. The MMA organization will need to have a small office there to receive and ship
goods, to buy supplies unavailable in Calama or San Pedro de Atacama, and on occasion to
represent the interests of the MMA to the regional government.
As the MMA moves from construction into full operations, the role of the Antofagasta office
could expand substantially. Because of the limited amenities in San Pedro de Atacama itself,
most long-term MMA families will choose to live elsewhere. To support this expanded
presence, the Antofagasta office would need to grow considerably.
Chile is a country of about 14 million inhabitants. About 50% live in the Santiago-Valparaiso
area, and five million live in Santiago itself. Santiago's environs while smog-impaired during
part of the year are exceedingly pleasant. It is an international city with lots of amenities. It has
foreign-language schools that can prepare students adequately for admission to foreign
universities, such as scoring well on the US SAT and achievement examinations, or the
German Arbitur exam, or the French Baccalauréat exam. Two of its universities, the University
of Chile and the Catholic University are among the best in South
America. Most substantive Chilean companies maintain offices there. It is the entry point for
most international flights. It is where you have to be to make and maintain important political
and economic connections. Chileans and foreigners enjoy living there. Simply put, it is the
capital of Chile.
The MMA operations will need a representative in Santiago. Shipping documents for duty-free
imports can be processed only by the Foreign Office in Santiago. Specific goods are more
available in Santiago than elsewhere in Chile. Visitors to the MMA will arrive first in Santiago.
What is in question is the extent to which the MMA will need facilities in Santiago. Unlike the
Cerro Tololo International Observatory (CTIO), Carnegie Southern Observatory (CARSO), and
the European Southern Observatory (ESO), the MMA is expected to operate primarily as a
service telescope. Like the VLA, astronomers need not travel to the telescope to make excellent
observations. Accordingly, no reception center will be required, no guest house will be required.
When MMA staff and other visitors do come to Santiago, the large range of commercial hotels
and restaurants in the city will suffice.
I believe that the MMA will need a small business office in the Vitacura or Providencia districts,
staffed with one or two people. This staff will process customs documents, purchase and ship
items unavailable in Region II, represent the MMA in governmental matters, and coordinate
their activities with the CTIO and ESO offices now located there.
The sophisticated support resources of the NRAO in the USA will be impossible to duplicate in Chile, owing principally to the diversity of the instrumentation maintained in the USA. While the MMA management will maintain its equipment as much as possible in Chile, the ultimate support will be the NRAO facilities in the United States. I would expect technical development of new sophisticated equipment and software to occur in the United States, as well as the identification and correction of subtle flaws in hardware and software, and support of MMA users located in the US.