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Llano de Chajnantor

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Llano de Chajnantor
NameLlano de Chajnantor
CountryChile
RegionAntofagasta Region
Coordinates23°1′S 67°45′W
Elevation5,000 m
RangeAndes
TypeHigh-altitude plateau

Llano de Chajnantor Llano de Chajnantor is a high-altitude plateau on the Altiplano in the Antofagasta Region of Chile, notable for hosting a cluster of international astronomical observatories and scientific installations. Situated near the Atacama Desert and adjacent to the Chajnantor Plateau, the site lies within a landscape influenced by the Andes and proximal to the Salar de Atacama, offering exceptional atmospheric conditions for millimeter and submillimeter astronomy. The plateau's strategic location has attracted projects involving institutions such as the National Radio Astronomy Observatory, European Southern Observatory, National Science Foundation and universities including Massachusetts Institute of Technology and University of Tokyo.

Geography and Climate

The plateau occupies part of the Altiplano, bordered by features like the Salar de Atacama, the Licancabur volcanic chain, and the Puna de Atacama, and lies within the administrative boundaries of the Antofagasta Region and near the municipality of San Pedro de Atacama. Its elevation (approximately 5,000 metres) places it above many Andes passes and influences ties to meteorological stations run by agencies such as the National Oceanic and Atmospheric Administration and observatories linked to the Institute of Astrophysics. Climatic conditions include extremely low precipitable water vapor, low atmospheric pressure comparable to conditions studied by NASA for high-altitude physiology, and large diurnal temperature ranges similar to sites evaluated by the European Space Agency and the Japan Aerospace Exploration Agency. The plateau's aridity and clear skies are comparable to other premier sites like Mauna Kea and Paranal Observatory, factors assessed in site surveys by collaborations involving the Max Planck Society and the Kavli Foundation.

Astronomical Facilities

Llano de Chajnantor hosts an array of facilities, including arrays and single-dish telescopes developed by consortia such as the Atacama Large Millimeter Array partnership of the European Southern Observatory, the National Radio Astronomy Observatory, and the National Astronomical Observatory of Japan. Other projects on or near the plateau involve the Atacama Pathfinder Experiment run by the Max Planck Institute for Radio Astronomy and the Atacama Submillimeter Telescope Experiment affiliated with the Nobeyama Radio Observatory. Facility planning has included proposals from organizations like the Square Kilometre Array consortium and collaborations with universities such as Harvard University, California Institute of Technology, and University of Cambridge. Instrumentation on site benefits from collaborations with laboratories like Jet Propulsion Laboratory and funding agencies including the National Science Foundation and the European Research Council.

Infrastructure and Access

Access to the plateau is typically from San Pedro de Atacama via roads connected to the Pan-American Highway and regional routes used by logistics teams from institutions such as the European Southern Observatory and the National Radio Astronomy Observatory. Infrastructure supporting operations includes antenna maintenance facilities, power supplied through agreements involving the Chilean Ministry of Energy and private utilities, and communications links coordinated with satellite providers like Intelsat and research networks affiliated with the Square Kilometre Array and the Global Grid Forum. High-altitude medical support protocols on site reference standards from World Health Organization and techniques developed at Cerro Tololo Inter-American Observatory, with personnel trained in conjunction with universities such as University of Chile and Pontifical Catholic University of Chile.

Scientific Research and Discoveries

Research conducted at the plateau has contributed to breakthroughs in millimeter and submillimeter astronomy, cosmology, and planetary studies, with teams from institutions like Massachusetts Institute of Technology, European Southern Observatory, National Radio Astronomy Observatory, Max Planck Society, and National Astronomical Observatory of Japan. Observations from facilities on the plateau have informed studies of the cosmic microwave background by collaborations including the South Pole Telescope and have supported discoveries relating to molecular clouds, star formation in regions compared to Orion Nebula, and high-redshift galaxies discussed in papers by researchers at Harvard–Smithsonian Center for Astrophysics and California Institute of Technology. Data pipelines and analysis tools developed by groups at National Center for Supercomputing Applications and CERN-associated teams have enabled joint publications with the European Southern Observatory and the Max Planck Institute for Astronomy.

Environmental Protection and Cultural Significance

The plateau lies within a broader region that intersects protected landscapes and indigenous territories, including areas associated with the Atacameño people and cultural heritage sites near San Pedro de Atacama and the Tatio Geysers. Environmental oversight involves Chilean agencies such as the Consejo de Monumentos Nacionales and environmental assessments aligned with standards from the International Union for Conservation of Nature and the United Nations Educational, Scientific and Cultural Organization. Collaborative initiatives include sustainability practices promoted by the European Southern Observatory and community engagement programs with local institutions like the Municipality of San Pedro de Atacama and universities such as Universidad de Antofagasta, aiming to balance scientific development with conservation of archaeological sites celebrated by ICOMOS and recognized in studies by the Smithsonian Institution.

Category:Landforms of Antofagasta Region Category:High plateaus of Chile