Malargüe - DSA 3

The Malargüe station, Deep Space Antenna 3, is ESA's newest tracking station and is located 30 km south of the city of Malargüe, about 1200 km west of Buenos Aires, Argentina. DSA 3 hosts a 35 m-diameter antenna with transmission and reception in X-band and reception in Ka-band.

DSA 3 was inaugurated in December 2012 and entered full service in early 2013. Today, it provides daily support to missions such as Gaia, Mars Express, Rosetta and ExoMars.


The coordinates of the antenna are 35° 46' 33.63" S (35.776°S), 69° 23' 53.51" W (69.398°W), and the station is sited at 1550 m above sea level.

The station is a 45-km drive from Malargüe city, in Mendoza province. Malargüe has a population of some 23 000 and is also home to the southern site of the Pierre Auger Observatory, an international physics experiment searching for ultra-high-energy cosmic rays.

Facilities & technology

The Malargüe station incorporates state-of-the-art technology. Its technical facilities comprise Ka-band reception (31.8–32.3 GHz) and X-band transmission and reception. It is prepared to host Ka-band transmission (34.3–34.7 GHz) and K-band reception (25.5–27 GHz).

Its main functions are to receive telemetry, send telecommands and perform radiometric measurements (ranging, Doppler, Delta-DOR) on scientific and deep-space craft.

The dish is 35 m in diameter and the entire structure is 40 m high; its moving antenna weighs 610 tonnes. Engineers can move the antenna with a speed of up to 1 degree per second in all axes. The servo control system ensures the highest possible pointing accuracy under the site’s harsh environmental, wind and temperature conditions.

The station has a frequency and timing system based on atomic clocks using masers and crycooled sapphires. Communications are via the ESA Operations Network (OPSNET). The site is equipped with a no-break power plant.

The antenna’s radio-frequency (RF) system comprises a Cassegrain Beam Wave Guide operating with frequency-sensitive (dichroic) mirrors and X- and Ka-band feeds, helium-cooled X- and Ka-band low-noise amplifiers, a 400 W solid-state power amplifier, and 2 and 20 kW X-band transmitters.


The station provides routine spacecraft tracking support to ESA's deep-space missions such as Venus Express and Mars Express, and scientific missions such as Herschel and Planck, as well as to other agencies’ missions under resource-sharing agreements. Malargüe will also support future ESA scientific missions, including LISA Pathfinder, Gaia and BepiColombo.

For routine operations, the station is remotely controlled from ESOC, Darmstadt, Germany. Local maintenance and operation is provided by a team of five engineers.

Delta DOR, GPS-TDAF, radio science

The station is also equipped with delta-DOR receivers (Delta Differential One-Way Ranging), a new technology enabling highly precise spacecraft location and tracking.

A GPS-TDAF (GPS Tracking and Data Analysis Facility) dual-frequency receiver system with geodetic accuracy is installed, which delivers continuous measurements to the ESOC Navigation Facility.

The station also hosts facilities enabling scientists to analyse received signals to perform radio science experiments.


Construction of the station started in late 2009 and the huge dish reflector was hoisted into place on 7 December 2011. The station received the first test signals from Mars Express, at a distance of 193 million km, on 14 June 2012. It is set for formal inauguration on 18 December 2012, and will enter routine service early in 2013.

The site was chosen for ESA's third deep-space antenna for several reasons.

In order to obtain global coverage, DSA 3 had to be located about 120° in longitude from the existing DSA stations in Australia and Spain, which meant a location somewhere in the Americas. ESA’s DSA stations also use delta-DOR, which works best when the stations involved are as far apart as possible.

The choice between North and South America was also driven by the fact that NASA already has plenty of station capacity in North America, so it made sense to build in South America.

The final location was chosen after securing a long-term lease for the site and the requisite radio frequencies from Argentina.

The agreement to build and exploit the station was signed with Argentina on 16 November 2009, for a planned duration of 50 years. The agreement contains benefits, facilities and services to be provided by Argentina. In exchange, ESA will make available to Argentina 10% of the antenna time for their national scientific projects. Argentina's Comisión Nacional de Actividades Espaciales (CONAE) is responsible for coordinating the use of the 10% of antenna time as provided in the agreement. 

1972 Andes flight disaster

The foreboding beauty of the landscape near Malargüe, high in clear mountain air, is famous for the 1972 Andes flight disaster, dramatised in the 1993 film Alive: The Miracle of the Andes. The actual crash site in the mountains is 138 km, as the crow flies, from ESA’s station.

Access and contact

The ESOC point of contact is:
Head of Ground Facilities Operations Division (OPS-ON)
ESOC, Darmstadt
Tel: +49 6151 90 0

Local site contact is:
Diego Pazos
Maintenance & Operations Manager
Telespazio Argentina S.A.

European Space Agency
Malargüe Satellite Tracking Station
Ruta Provincial 186 km 20,5 (5613)
Malargüe, Provincia de Mendoza
Tel: +54 261 413 6330/67
Mobile: +54 911 4181 5763

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