LIRA, a pioneer in astrophysics and instrumentation, pushes back the frontiers of knowledge
LIRA
Laboratory for Instrumentation and Research in Astrophysics
The MIRS infrared imaging spectrometer aboard the MMX mission
16 February 2026The LIRA provided the Japan Aerospace Exploration Agency (JAXA) with the MIRS infrared imaging spectrometer (highlighted in red in the image), onboard the MMX (Mars Moons eXplorer) spacecraft. The instrument aims to map Mars’ two moons, Phobos and Deimos, and to analyze the atmosphere of the Red Planet. After successfully completing thermal vacuum tests in April 2025, the MMX spacecraft also passed its mechanical environment tests in September–October, followed by electromagnetic compatibility tests in November. The launch is scheduled for October 2026.
The MMX mission aims to return samples from Phobos to Earth in 2031, in order to characterize the surfaces of Mars’ moons and the composition of the planet’s atmosphere.
Credit: JAXA
Théminaires Planétologie Exploring Mercury’s Exosphere with BepiColombo/PHEBUS
Séminaires du pôle HPA Chemistry of the D-region during solar flares and HF absorption modelling
News
FIRST’s photonic lantern has just successfully completed the commissioning phase.
Johan Mazoyer has been awarded an ERC Consolidator Grant 2025 for his ECHOES project.
Presentation
LIRA, a CNRS joint research unit at Paris Observatory, is a laboratory of excellence in astrophysics and instrumentation. It studies astrophysical objects, from the Solar System to our Galaxy and beyond, through five thematic areas. Through international collaboration and instrumental innovation, it pushes back the frontiers of science and contributes to the training and dissemination of knowledge.
Our projects
MIRS on the JAXA MMX mission
The Martian Moons eXploration (MMX) mission of JAXA (Japan Aerospace Exploration Agency) is the first sample-return mission from the Phobos satellite. It also includes an exploration of the Martian system. The mission’s primary objective is to decipher the origin of Martian moons, which will provide important information on planet formation and the conditions for the emergence of water on Earth-like planets.
The MIRS (MMX InfraRed Spectrometer) instrument, developed under the leadership of LESIA (now LIRA), is an imaging spectrometer that will characterize the composition of the Martian system and help select candidate sites for sample collection.
GRAVITY+
The GRAVITY instrument, installed on the European Southern Observatory’s Very Large Telescope Interferometer (VLTI/ESO), has produced spectacular and transformative results on the supermassive black hole at the centre of the Milky Way, the active nuclei of other galaxies, proto-planetary disks around young stars and exoplanets. GRAVITY+ aims to modernise both VLTI and GRAVITY to make them ≈ 100 times more sensitive, while increasing sky coverage by a factor of ≈ 100, and contrast in the vicinity of bright objects by a factor of ≈ 10. These gains will benefit all the VLTI’s current and future instruments for the next 20 years, and will perpetuate it as a unique infrastructure in the world.
All projects
Projets en développement
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Projets passés
Contacts
Contacts
Postal address
Observatoire de Paris
5, place Jules Janssen
92195 Meudon
Phone
01 45 07 77 01
Meudon site
LIRA
Observatoire de Paris
5, place Jules Janssen
92195 MEUDON Cedex
Paris site
LIRA
Observatoire de Paris
77, Avenue Denfert-Rochereau
75014 Paris
Cergy site
LIRA - Site de Neuville II
UFR Sciences et Techniques - Département de physique
5, mail Gay Lussac
95000 Neuville-sur-Oise