Thales Alenia Space Secures ESA Deal for LISA Space Observatory Development

Thales Alenia Space Secures ESA Deal for LISA Space Observatory Development

Thales Alenia Space, the joint venture between Thales (67%) and Leonardo (33%), announces the signing of a €26.1 million phase 1 contract with the European Space Agency (ESA) related to the development of LISA’s telescopes. Made up of three satellites, the LISA (Laser Interferometer Space Antenna) mission will be the first European space observatory capable of detecting and studying gravitational waves generated by extreme cosmic events.

This latest announcement follows the signing of two other contracts related to the same mission. In June 2025, Thales Alenia Space announced a contract with prime contractor OHB System AG to provide several critical elements, including the spacecraft avionics and control software, the telecommunication system, and the drag-free and attitude control system (DFACS). In January 2026, the company was also selected by OHB System AG to provide the propulsion subsystem.

In France, Thales Alenia Space and Thales SESO®, which are responsible for developing the optical payload telescopes, will make a major contribution to the mission. 

Based on its globally renowned expertise in the design and manufacture of advanced optical technologies, Thales Alenia Space has been selected by the European Space Agency (ESA) to conduct Phase 1 for the development of the six telescopes, which is expected to proceed in three phases.

As prime contractor, Thales Alenia Space will be responsible for the development, design, assembly, and testing of the telescopes. The manufacture of the six telescopes, made entirely of Zerodur®, will present an unprecedented technological challenge.

It is only the combined expertise in design and manufacturing of Thales SESO® and Thales Alenia Space, along with Zerodur®’s extremely low thermal sensitivity, that will enable the picometer-level stability required by LISA mission.

For this initial development contract, Thales Alenia Space will be able to draw on the long-standing expertise of Thales SESO®, Europe’s leading supplier of ultra-lightweight Zerodur® mirrors.

Thales SESO® will be responsible for the procurement, machining, and polishing of the optics and structure. In addition, Thales Alenia Space and Thales SESO® will jointly be responsible for assembling the telescopes, aligning the optics, and conducting environmental and performance tests. With more than 200 Zerodur® Space mirrors manufactured and flying, Thales SESO® is among the world top leaders for optical surface precision achieved through polishing, with 0.2 nanometers reached over the 230-mm diameter surface of the mirrors made for Virgo (the European ground gravitational wave detector) —a level of precision that is priceless for the LISA mission.

LISA represents a pioneering initiative in astrophysics and space exploration that has not previously been attempted. Thales Alenia Space is responsible for several mission-critical components of the LISA project. I am pleased to expand our collaboration with Thales Alenia Space to include the first phase of the development of the telescopes, significantly mitigating the risk of this technological challenge. Thales Alenia Space will partner with Thales SESO®, a leading European supplier of ultra-lightweight Zerodur® mirrors. I am looking forward to seeing the first results of this development by year-end.” said Filippo Marliani, LISA Project Manager at ESA.

“We are extremely proud to be part of this exceptional mission dedicated to the study of gravitational waves from space, and we would like to thank ESA for its renewed trust,” said Bertrand Denis, Vice President Observation, Science, and Exploration at Thales Alenia Space in France. “The development of these telescopes is fully aligned with the core expertise of Thales Alenia Space and Thales SESO® in high-performance optical instrumentation. Our capability to produce instruments in series will also be a real asset in the project’s success.”

LISA (Laser Interferometer Space Antenna) is a unique space exploration mission by the European Space Agency (ESA) designed to detect gravitational waves directly from space. This space observatory will detect the tiniest distortions in spacetime caused by gravitational waves generated by the acceleration of massive objects, as predicted by Albert Einstein’s theory of general relativity in 1916, with a sensitivity and within a very low frequency range (between 0.1 mHz and 100 mHz), inaccessible to existing ground-based measurement facilities such as LIGO in the United States and VIRGO in Europe, due to their limited size and seismic interferences.

The LISA mission will provide a new opportunity to understand the early universe that existed before the formation of stars and galaxies, as well as celestial phenomena such as the interaction of compact stars or the merger of supermassive black holes at the centers of galaxies.

LISA consists of a constellation of three satellites, each spaced 2.5 million kilometers apart, forming an equilateral triangle and each carrying two test masses. These three satellites are linked by six laser beams, thus forming a massive optical interferometer. These inter-satellite laser beams will measure the displacement of these masses with an accuracy on the order of a picometer (smaller than an atom).

The LISA mission satellites benefit from the experience gained during the LISA Pathfinder program, launched in 2015, which successfully demonstrated the ability to maintain test masses in a state of “free fall” with exceptional precision. The same precision propulsion system, also used for ESA’s Gaia and Euclid missions, will ensure that each satellite keeps the laser interferometer beams pointed toward the other satellites with the utmost precision.

LISA will employ advanced laser interferometry measurement techniques to study astrophysical phenomena involving massive and distant systems, thereby offering unprecedented opportunities to explore and understand our universe. The three satellites are scheduled to launch in 2035 aboard an Ariane 6 rocket.

Thales Alenia Space will provide prime contractor OHB System AG with several mission-critical elements, including the spacecraft avionics and control software, the telecommunication system, and the drag-free and attitude control system (DFACS). The joint venture will be responsible for the design, manufacture, assembly, integration, and testing of the propulsion subsystem for the LISA mission. Thales Alenia Space is also responsible for ensuring the exceptional electromagnetic, radiation, and self-gravity operational environment for the payload, essential to mission performance, for which Thales Alenia Space is also managing the budgets.

Thales Alenia Space in Turin, Italy, as member of the LISA Core Team makes use of the experience and design solutions inherited from the five-year study phase led by Thales Alenia Space as the prime contractor. Our facility, in Gorgonzola, Italy, will develop the On-Board Computer and the Mass Memory in the same integrated unit. In the United Kingdom, the company is supplying the propulsion system, while France is responsible for developing the telescopes in collaboration with Thales SESO®. Our teams in Switzerland are involved in developing part of the instrument's electronics and of the Constellation Acquisition System for LISA.

Leonardo is also contributing with its technologies to the LISA mission with some key equipment, such as the micro propulsion assemblies, a highly precise system of thrusters used to control the satellite’s attitude with extreme accuracy. Other company sites will also have the opportunity to contribute to the LISA mission, supplying spacecraft subsystems or equipment.

Click here to know more about LISA

Publisher: SatNow
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GNSS Constellations - A list of all GNSS satellites by constellations

beidou

Satellite NameOrbit Date
BeiDou-3 G4Geostationary Orbit (GEO)17 May, 2023
BeiDou-3 G2Geostationary Orbit (GEO)09 Mar, 2020
Compass-IGSO7Inclined Geosynchronous Orbit (IGSO)09 Feb, 2020
BeiDou-3 M19Medium Earth Orbit (MEO)16 Dec, 2019
BeiDou-3 M20Medium Earth Orbit (MEO)16 Dec, 2019
BeiDou-3 M21Medium Earth Orbit (MEO)23 Nov, 2019
BeiDou-3 M22Medium Earth Orbit (MEO)23 Nov, 2019
BeiDou-3 I3Inclined Geosynchronous Orbit (IGSO)04 Nov, 2019
BeiDou-3 M23Medium Earth Orbit (MEO)22 Sep, 2019
BeiDou-3 M24Medium Earth Orbit (MEO)22 Sep, 2019

galileo

Satellite NameOrbit Date
GSAT0223MEO - Near-Circular05 Dec, 2021
GSAT0224MEO - Near-Circular05 Dec, 2021
GSAT0219MEO - Near-Circular25 Jul, 2018
GSAT0220MEO - Near-Circular25 Jul, 2018
GSAT0221MEO - Near-Circular25 Jul, 2018
GSAT0222MEO - Near-Circular25 Jul, 2018
GSAT0215MEO - Near-Circular12 Dec, 2017
GSAT0216MEO - Near-Circular12 Dec, 2017
GSAT0217MEO - Near-Circular12 Dec, 2017
GSAT0218MEO - Near-Circular12 Dec, 2017

glonass

Satellite NameOrbit Date
Kosmos 2569--07 Aug, 2023
Kosmos 2564--28 Nov, 2022
Kosmos 2559--10 Oct, 2022
Kosmos 2557--07 Jul, 2022
Kosmos 2547--25 Oct, 2020
Kosmos 2545--16 Mar, 2020
Kosmos 2544--11 Dec, 2019
Kosmos 2534--27 May, 2019
Kosmos 2529--03 Nov, 2018
Kosmos 2527--16 Jun, 2018

gps

Satellite NameOrbit Date
Navstar 82Medium Earth Orbit19 Jan, 2023
Navstar 81Medium Earth Orbit17 Jun, 2021
Navstar 78Medium Earth Orbit22 Aug, 2019
Navstar 77Medium Earth Orbit23 Dec, 2018
Navstar 76Medium Earth Orbit05 Feb, 2016
Navstar 75Medium Earth Orbit31 Oct, 2015
Navstar 74Medium Earth Orbit15 Jul, 2015
Navstar 73Medium Earth Orbit25 Mar, 2015
Navstar 72Medium Earth Orbit29 Oct, 2014
Navstar 71Medium Earth Orbit02 Aug, 2014

irnss

Satellite NameOrbit Date
NVS-01Geostationary Orbit (GEO)29 May, 2023
IRNSS-1IInclined Geosynchronous Orbit (IGSO)12 Apr, 2018
IRNSS-1HSub Geosynchronous Transfer Orbit (Sub-GTO)31 Aug, 2017
IRNSS-1GGeostationary Orbit (GEO)28 Apr, 2016
IRNSS-1FGeostationary Orbit (GEO)10 Mar, 2016
IRNSS-1EGeosynchronous Orbit (IGSO)20 Jan, 2016
IRNSS-1DInclined Geosynchronous Orbit (IGSO)28 Mar, 2015
IRNSS-1CGeostationary Orbit (GEO)16 Oct, 2014
IRNSS-1BInclined Geosynchronous Orbit (IGSO)04 Apr, 2014
IRNSS-1AInclined Geosynchronous Orbit (IGSO)01 Jul, 2013
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