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Our Ground Stations

Estrack Ground Stations

ESA’s tracking station network – Estrack – is a global system of ground stations providing links between satellites in orbit and ESOC, the European Space Operations Centre, Darmstadt, Germany. The core Estrack network comprises seven stations – some with multiple antennas – in seven countries.

The essential task of all ESA ground-based tracking stations is to communicate with spacecraft – to transmit commands and receive scientific data and spacecraft status information.

Our technically advanced stations can track spacecraft almost anywhere – circling Earth, watching the Sun, orbiting at the scientifically crucial Sun-Earth Lagrange points or voyaging deep into our Solar System.

Tracking is provided through all phases of a mission, from ‘LEOP’ – the critical Launch and Early Orbit Phase – through to routine operations, special manoeuvres or planetary flybys and ultimately through deorbiting and safe disposal.

Estrack core network

SMA

Santa Maria

The Santa Maria S-band station, also known as ‘Montes das Flores’ (Hill of Flowers), is located 5 km from the town of Vila do Porto on the Portuguese island of Santa Maria, in the Azores.

The station consists of a 5.5-m antenna hard-wired on a stable concrete platform and includes telecommunications equipment, a no-break power system, lightning protection and support infrastructure.

Santa Maria was one of the first Estrack stations with launcher tracking capability and is ideally located to acquire signals from launchers climbing up toward the North-East from ESA’s spaceport in Kourou, French Guiana.

RED

Redu

Redu station is located about 1 km from the village of Redu, in the Belgian province of Luxembourg. The station provides tracking capabilities in S- and Ka-band and hosts multiple tracking antennas operating in a variety of frequency bands to support in-orbit testing (IOT) of telecommunication satellites.

Redu station is equipped with its own emergency electrical power generator system and is connected to the Belgian communication network via fully redundant fibre-optic cables.

KIR-1

Kiruna

Kiruna station is located at Salmijärvi, 38 km east of Kiruna, in northern Sweden. It hosts a 15-m antenna, KIR-1, and a 13-m antenna, KIR-2. Both operate in S-band for uplink and downlink and in X-band for downlink.

KIR-1 features autotrack and program track capability in S-band.

Both antennas provide routine support for satellites in low-Earth orbits (LEO) during their routine phases, and specialised support during the Launch and Early Orbit Phase (LEOP).

The station provides facilities for tracking, telemetry, telecommand and radiometric measurements in S-band. X-band reception is used for high-rate payload data for Earth observation missions such as the Sentinel satellites of the European Copernicus Programme and scientific missions such as ESA’s Integral orbiting observatory.

KIR-2

Kiruna

Kiruna station is located at Salmijärvi, 38 km east of Kiruna, in northern Sweden. It hosts a 15-m antenna, KIR-1, and a 13-m antenna, KIR-2. Both operate in S-band for uplink and downlink and in X-band for downlink.

KIR-2 features autotrack and program track capability in both S- and X-band.

Both antennas provide routine support for satellites in low-Earth orbits (LEO) during their routine phases, and specialised support during the Launch and Early Orbit Phase (LEOP).

The site is equipped with a no-break power plant providing electrical power to all mission critical equipment. The station also hosts a Galileo Experimental Sensor Station (GESS) receiver and a Global Navigation Satellite System (GNSS) receiver, which deliver continuous data to ESOC.

KRU

Kourou

Kourou station, also known as ‘Kourou 93’, is located 27 km from the town of Kourou and 90 km from Cayenne, the capital of French Guiana, in South America.

The station site is 19 km from the Centre Spatiale Guyanais (CSG), Europe’s Spaceport. It is used to communicate with Earth-orbiting spacecraft such as XMM-Newton for routine operations, and for the Launch and Early Orbit Phase (LEOP) – or for backup – for other missions.

The station hosts a 15-m dish antenna that transmits and receives signals in S- and X-band wavelengths, plus facilities for tracking, telemetry, telecommand and radiometric measurements. There is also a 1.3-m dish mounted on the side of the 15-m dish as an X-band acquisition aid.

Kourou station also provides system validation testing for satellites during final checkout in the assembly building at CSG or just prior to launch when installed on their launcher at the CSG launch areas a few kilometres away.

CEB

Cebreros

Cebreros station, DSA 2 (Deep Space Antenna 2), is located 77 kms west of Madrid, Spain. It hosts a 35-metre deep-space communications antenna, CEB, with X-band transmission and X- and Ka-Band reception.

CEB provides daily routine operations or back-up support for a range of deep-space with facilities for tracking, telemetry, telecommand and radiometric measurements (ranging, Doppler, meteo)

Estrack 35-m antennas are also equipped with Delta-DOR (Delta Differential One-Way Ranging) capability, a technology used to locate and track distant spacecraft incredibly precisely. CEB also hosts facilities enabling scientists to analyse received signals to perform radio science experiments.

MLG

Malargüe

Malargüe station, DSA 3 (Deep Space Antenna 3), is located 30 km south of the city of Malargüe, about 1200 km west of Buenos Aires, Argentina. It hosts a 35 m-diameter deep-space communications antenna, MLG with X-band transmission and X- and Ka-band reception.

CEB provides daily routine operations or back-up support for a range of deep-space with facilities for tracking, telemetry, telecommand and radiometric measurements (ranging, Doppler, Delta-DOR).

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.

NNO-1

New Norcia

New Norcia station, DSA 1 (Deep Space Antenna 1), is located 140 kilometres north of Perth, Western Australia, close to the town of New Norcia. It hosts a 35-metre deep-space communication antenna, NNO-1 with transmission and reception in both S- and X-band.

The NNO-1 antenna is one of the largest in the world for telemetry, tracking and command (TT&C) applications. This is essential for high-performance communications with distant spacecraft, such as Mars Express, and missions in highly elliptical orbits that take them far from Earth, such as Solar Orbiter.

The large antenna allows scientific data collected by deep-space missions such as the former comet explorer Rosetta to be reliably received on Earth, even from distances of up to 900 million kms – more than six times the distance from Earth to the Sun.

NNO-2

New Norcia

In 2015, a new 4.5-m radio dish was installed at New Norcia to replace the satellite acquisition capability previously provided by the station at Perth, which was retired. It is designated NNO-2.

NNO-2 offers a wider field of view than the NNO-1 antenna and can acquire signals from a newly launched spacecraft even when its position is not precisely known.

It can also be used to point the NNO-1 antenna. NNO-2 transmits and receives in X-band and can receive telemetry downloaded in S-band for launcher tracking.

NNO-3

New Norcia

A second 35-m deep space antenna is currently under construction at ESA’s New Norcia station. The new NNO-3 antenna will be very similar in design to NNO-1.

As ESA launches an increasing number of long-term space missions and supports the communication efforts of an increasing number of partners, the demand for ground station bandwidth is rising rapidly.

In order to meet this demand, ESA’s ground station experts are developing new technologies to make the existing Estrack stations more efficient than ever before. But as the stations reach the efficiency limits dictated by fundamental laws of physics, the only solution is to build more antennas.

Augmented network

The ESA-owned and operated core Estrack network is complemented by commercially operated stations provided through service contracts with organisations such as the Swedish Space Corporation (SSC), Spain’s National Institute of Aerospace Technology (INTA) and Kongsberg Satellite Services AS (KSAT, Norway).

These include tracking stations located at South Point, Hawaii (USA), Santiago (Chile), TrollSat, Antarctica, Svalbard (Norway) and Dongara (Australia).

These stations are used especially during the LEOP phase of a mission immediately following launch, when the flight control team needs continuous communication with their satellite, beyond what can be provided by ESA’s own station network.

International cooperation

ESA shares Estrack capacity with other space agencies, who in return provide tracking services to ESA missions under a number of resourcing-sharing agreements. These include networks and stations operated by ASI (Italy), CNES (France), DLR (Germany), NASA's Deep Space Network and Goddard Space Flight Centre and JAXA (Japan).

In recent years, Estrack has provided support to missions operated by China and Russia, as well as tracking the descent of NASA rovers to the surface of Mars.

This global cooperation allows all agencies to make use of a wide number of ground stations in geographically advantageous locations, maximising efficiency and enhancing scientific returns for all.

This cooperation is made possible, in part, through ESA's strong support for the development and adoption of internationally recognised technical standards for sharing tracking data.

Supporting European industry

Estrack station development, maintenance and upgrading are done by ESA at ESOC, in cooperation with European industry.

Recent highlights include ESA support to the industrial development of a made-in-Europe integrated chip that powers a new and highly sensitive amplifier that can operate at around –263ºC, just 10 degrees above absolute zero. The upgrade allows ESA’s 35 m-diameter antennas to receive an additional 40—80% scientific data in any given communication window with a spacecraft.

ESA has also supported European industry through the development of new technology – an array of eight small radio-frequency sensors around the rim of an existing dish antenna – that enables the quick acquisition of signals from satellites just after launch.

Explore ESA’s Ground Stations

ESTRACKnow

ESTRACKnow allows you to find out exactly which ground antenna is communicating with which spacecraft at any moment.

Explore the impressive dishes and antennas at ground stations across the globe, working every day to gather all of the vital information returned from space and sending commands direct from mission control.

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