Big Iron gets technology boost

Big Iron gets technology boost
Views of the 35m ESTRACK deep-space tracking station in Argentina, now supporting the Rosetta mission. Credit: ESA/D. Pazos - CC BY-SA IGO 3.0

ESA deploys 'big iron' to communicate with its deep-space missions: three 35 m-diameter dishes employing some of the world's most advanced tracking technology. And it's about to get a boost.

ESA's three Deep Space Antenna stations at New Norcia, Australia, Cebreros, Spain and Malargüe, Argentina, beam commands and receive data from spacecraft voyaging hundreds of millions of kilometres into our Solar System.

The trio form part of ESA's Estrack tracking network a global system of stations providing links between satellites in orbit and the European Space Operations Centre, Darmstadt, Germany. The core network comprises 10 stations in seven countries.

The huge dishes – whose moveable structures weigh in at 620 tonnes – can be rotated, elevated and aimed with pinpoint accuracy despite high winds and heat, and transmit radio signals with up to 20 kW of power – enough to run over 20 000 domestic coffee makers .

The stations' stellar performance, however, isn't just about big moving, mechanical things: they make use of advanced, made-in-Europe electronics, including cryogenically cooled low-noise amplifiers and exquisitely machined mirrors made of metal.

Exploiting the fundamental physics of radio waves and properties of geometric shapes, the stations use 'dichroic mirrors' made of metal, not glass, to reflect and separate the transmitted and received beams.

These mirrors are a metallic latticework comprising thousands of small shapes – either rectangles or crosses – and enable the stations to differentiate between radio signals ranging in frequency from 2 GHz to 40 GHz.

Using their original mirrors and frequencies, the stations, which entered service in 2001 (Australia), 2006 (Spain) and 2013 (Argentina), have provided flawless links with multiple ESA missions, including Gaia, Mars Express and Rosetta, as well as those of partner agencies such as NASA.

Big Iron gets technology boost
Factory acceptance test of the M6 S/X-band dichroic mirror installed at New Norcia station, Australia (DSA1). Credit: ESA/Telecom Italia

But they were designed to allow future upgrades, and with ESA's growing Solar System exploration plans, the future is here.

"Future exploration missions to destinations like Jupiter, Ganymede and Mercury will deliver much more scientific data from much further away, and this requires increasing the stations' transmit and receive capabilities," says Pier Mario Besso, an ESA antenna engineer.

Furthermore, spaceborne observatories like Herschel/Planck in the past and Gaia today traditionally use the 8 GHz band for beaming data back, while future missions such as Euclid will move to the 26 GHz band, which offers four times more data bandwidth.

This means upgrading the current fixed, solid dichroic mirrors with newer versions that can move between various mechanical positions, and cryogenically cooling microwave components to make them more sensitive.

As a measure of how much this will improve performance, consider that the stations typically offer a download rate of 228 kbit /s from Mars Express circling the Red Planet, and 7.6 Mbit/s from Gaia, some 1.5 million km from Earth.

When complete, the improvements will boost this to, typically, 2.2 Mbit/s for ExoMars, and a whopping 74 Mbit/s for Euclid at Gaia's distance – about four times faster than a typical home broadband Internet connection.

Big Iron gets technology boost
Juice, the JUpiter ICy moons Explorer mission, in the Jovian system. Credit: ESA/AOES

ESA is now upgrading the three sites to work at these new frequencies. 

"The work we're doing now to improve the design and performance will enable additional improvements as technology matures in the future," notes Pier Mario.

Plans already foresee improved cryogenic cooling for the microwave feed systems, and 80 kW power amplifiers are being developed, which would give ESA the invaluable ability of coping with emergency situations at interplanetary distances – only NASA's 70 m dishes can do that today.

ESA operates some of the world's most sophisticated deep-space tracking stations, enabling spacecraft to maintain contact with Earth while voyaging deep into our Solar System. The essential task of all ESA stations is to communicate with our missions, sending telecommands and receiving vital scientific data and spacecraft status information. The Agency's three Deep Space Antenna (DSA) stations are located in Australia, Spain and Argentina, and are centrally controlled from the ESOC Operations Centre in Germany. They are equipped with large, 35 m-diameter parabolic dish reflectors, weighing in at 610 tonnes, that can be rotated and pointed with extreme accuracy. Using signal data from the stations and an advanced navigational technique known as 'delta-DOR', engineers can pinpoint the orbit of a spacecraft exploring Mars or Venus - a distance of over 100 million kilometres from Earth - to an accuracy within 1 kilometre. Credit: ESA

Further into the future, ESA is exploring new possibilities for increasing data return, perhaps through arrays of deep-space antennas.

"The demand for data from deep space is only going to increase," says Pier Mario. "ESA operates, or will soon operate, spacecraft exploring increasingly farther away that deliver increasing amounts of information.

"They are travelling to the frontiers of human knowledge, and Estrack provides the link that brings their data down to Earth."


Explore further

Image: ESA's deep-space tracking station at New Norcia, Australia

Citation: Big Iron gets technology boost (2015, September 18) retrieved 29 May 2020 from https://phys.org/news/2015-09-big-iron-technology-boost.html
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only.
18 shares

Feedback to editors

User comments