ESA title
The Villafranca  VIL-1 15-m S-band antenna

ESA antennas in Spain

1310 views 1 likes
ESA / About Us / ESAC

Satellites stay in contact with the Earth by means of a ground-station network. Engineers send commands to correct their trajectories, manoeuvre them into different orbits, and operate their instruments. The satellite transmits back to Earth not only the scientific data that it is gathering, but also the ‘housekeeping’ information needed by the operators to check the satellite’s performance.

The scientific data from all astronomy and planetary ESA missions whose Science Operations Centres (SOCs) are housed at ESAC arrive here from the Agency’s European Space Operations Centre (ESOC) in Darmstadt, near Frankfurt.

For these purposes, ESA has a number of antennas located at ESAC in Villafranca, Madrid, with modern electronic telemetry, telecommand and ranging equipment that allows commands to be sent to control the satellites and their payloads, as well as the scientific data to be received on the ground.

The ESAC antennas at Villafranca currently support:

  • the Cluster flotilla, four satellites that are studying the Earth’s magnetic field
  • SMART-1, the ESA small-satellite mission to the Moon
  • Double Star (in support of China)
  • occasionally Integral, the gamma-ray telescope
  • and occasionally two of ESA’s Earth-observation satellites, Envisat and ERS-2.

ESA also has a deep space antenna located in Cebreros, Ávila. ESA’s next generation of astronomy and planetary missions are highly ambitious. Designed to open up new frontiers in space exploration, many of them will be placed very far away in space, not even orbiting Earth. To communicate with these deep-space missions, ESA is building-up a new network of deep-space antennas.

The new 35-metre deep space tracking station at Cebreros
The new 35-metre deep space tracking station at Cebreros

The powerful new 35-metre antenna at Cebreros is currently one of two ESA deep-space ground stations, the other being at New Norcia in Australia. Cebreros’s first task will be to support the Venus Express mission – the first ESA mission to our nearest neighbouring planet and the hottest in the Solar System – from October 2005. Other interplanetary missions will follow, including BepiColombo, as well as missions orbiting the second Lagrangian point – a point beyond the Moon, 1.5 million kilometres from Earth – such as Herschel, Planck and Gaia.

Related Links