Mars Bible — Organisations
CNES, the French space agency
Founded in 1961, CNES gave France Diamant, Kourou and Ariane. On Mars it has provided major instruments: OMEGA, ChemCam, the SEIS seismometer, SuperCam, and soon the Idefix rover on Phobos.
founded December 19, 1961 — Paris and Toulouse
- Founded
- December 19, 1961
- Centers
- Paris, Toulouse, Kourou (French Guiana)
- Instruments on Mars
- OMEGA, SPICAM (Mars Express), ChemCam (Curiosity), SEIS (InSight), SuperCam (Perseverance)
- First marsquake
- Detected by SEIS on April 7, 2019
- Project
- Idefix rover on Phobos (MMX), with DLR
4 chapters and 3 appendices: about 1,300 words, or about 5 minutes of reading. Every fact comes from verified sources, listed at the end of each chapter.
Part One
The agency
1961 – 2002
Chapter 1 · 1961 – 2002 France’s space agency
The Centre national d’études spatiales was born in 1961. In forty years it gave France a launcher, a base in French Guiana and a space industry, before putting its instruments to work exploring Mars.
De Gaulle and Asterix
On December 19, 1961, President Charles de Gaulle founded the Centre national d’études spatiales, CNES. On November 26, 1965, from the Hammaguir base in Algeria, the first French launcher, Diamant, put the first French satellite, Asterix, into orbit. The Guiana Space Centre at Kourou was established that same year; the Toulouse Space Centre in 1968.
Ariane and Europe
In 1973 the Ariane program got under way. In 1975, when the European Space Agency was created, CNES became its leading contributor. On December 24, 1979, Ariane 1 made its maiden flight. In 1986 SPOT-1 became, according to CNES, the first high-resolution civil Earth-imaging satellite. In 1995 came Helios, France’s first military observation satellite.
Sources: CNES, “History” (founded on December 19, 1961 by Charles de Gaulle, Diamant and Asterix on November 26, 1965 from Hammaguir, Guiana Space Centre in 1965, Toulouse Space Centre in 1968, Ariane in 1973, ESA in 1975 with CNES as leading contributor, Ariane 1 on December 24, 1979, SPOT-1 in 1986, Helios in 1995).
Part Two
France on Mars
2003 – 2031
Chapter 2 · 2003 – 2024 French instruments on Mars
Since 2003, French laboratories and CNES have provided several major Mars missions with a key instrument: a spectrometer, a laser, a seismometer, a microphone.
Mars Express
Launched on June 2, 2003, the European Mars Express probe carried three instruments with French contributions. OMEGA, a spectrometer mapping surface minerals in visible and infrared light, was conceived at the Institut d’astrophysique spatiale in Orsay and the LESIA laboratory in Meudon; SPICAM, an ultraviolet and infrared spectrometer for the atmosphere, at LATMOS. CNES funded and supported OMEGA and SPICAM, and built the ground segment for a third instrument, ASPERA. Over some ten years, the probe detected clays and hydrated sulfates, confirming that liquid water once flowed on Mars.
ChemCam
On the Curiosity rover, the ChemCam instrument was designed and developed in France and the United States. CNES is the project owner; the Institut de recherche en astrophysique et planétologie in Toulouse, IRAP, holds technical and scientific responsibility, with Los Alamos National Laboratory. More than three hundred people worked on it in France. Its laser heats a patch of rock smaller than a square millimeter to more than 10,000 degrees; the resulting spark reveals the rock’s composition. ChemCam was delivered to JPL in August 2010 and landed with Curiosity on August 6, 2012. From Toulouse, at CNES’s FOCSE operations center, French teams program the instrument one week in two and receive its data.
SEIS
On the InSight lander, which touched down on November 26, 2018, the SEIS seismometer was developed by France: CNES led its development with the Institut de physique du globe de Paris and other European and American partners, then ran its operations. SEIS entered service in early February 2019. On April 7, 2019, it detected the first quake ever recorded on Mars. By measuring the planet’s activity, it made it possible to infer its internal structure, such as the size of the core and the thickness of the mantle. InSight last communicated with Earth on December 15, 2022; after two attempts went unanswered, NASA declared the mission over on December 21.
SuperCam
On Perseverance, which landed on February 18, 2021, SuperCam combines three spectrometers, a camera and a microphone. Its upper part, the “head” at the top of the mast, is the French contribution: IRAP designed and coordinated it under CNES oversight, with several other French laboratories. Its laser reaches seven meters. The microphone listens to the noise of laser impacts to estimate the hardness and porosity of rocks, and is also used to study the atmosphere.
Sources: CNES, “Mars Express” (OMEGA, IAS and LESIA, SPICAM and LATMOS, ASPERA, CNES’s role, June 2 and December 25, 2003, clays and hydrated sulfates); CNES, “ChemCam” (project owner, IRAP and LANL, more than 300 people, more than 10,000 °C and less than a mm², delivery in August 2010, landing on August 6, 2012, FOCSE in Toulouse); CNES, “InSight” (SEIS, IPGP and partners, operations, landing on November 26, 2018, service from early February 2019, first quake on April 7, 2019, end of operations on December 21, 2022); NASA, “NASA Retires InSight Mars Lander Mission After Years of Science,” December 21, 2022 (last communication on December 15, two unanswered attempts, end of mission); CNES, “SuperCam” (IRAP’s Mast Unit under CNES oversight, French labs, three spectrometers, camera and microphone, 7 m range, landing on February 18, 2021); CNES, “Planète Mars” dossier (ChemCam of French design, SEIS developed by France).
Chapter 3 · 2017 – 2031 Idefix, a rover on Phobos
With the Japanese MMX mission, a vehicle designed in France and Germany is to drive, for the first time, on a moon of Mars.
The rover
For MMX, the Japanese Phobos sample-return mission, CNES is building with the German space agency, DLR, the small Idefix rover and its four instruments. It is to attempt to drive on Phobos, where gravity is about 1,800 times weaker than on Earth, during a hundred-day mission. CNES also provides the MIRS near-infrared imaging spectrometer, built by the LIRA laboratory (formerly LESIA), which will identify the moons’ minerals, study Mars’s atmosphere and help choose landing sites; and it studies the cruise trajectories.
The schedule
Launch is planned for October 20, 2026, from Tanegashima, Japan. Between 2027 and 2030 the spacecraft is to enter orbit around Phobos, land, collect at least ten grams of material from two centimeters down and set the rover on the surface. The samples are to return to Earth in 2031, in the Australian desert.
Sources: CNES, “MMX” (Idefix with DLR and its four instruments, gravity 1,800 times weaker, hundred-day mission, MIRS and the LIRA lab, flight dynamics, launch on October 20, 2026, 2027-2030, at least 10 g from 2 cm, return in 2031 in Australia). The book on JAXA tells the mission in more detail. The CNES page counts twelve instruments aboard in one place and thirteen in another; we do not give the number.
Epilogue
CNES and Mars
Chapter 4 · The lesson What CNES brings to Mars
France has no Mars ship. Yet its instruments have read the minerals, analyzed the rocks, and listened to the quakes and atmosphere of Mars. Three lessons emerge.
Excellence in an instrument
Providing a first-rank instrument for a partner’s mission means taking part in exploration without bearing its full cost. A future international Martian base will need such national specialties.
Operating from home
From Toulouse, French teams program instruments sitting on Mars every week. Martian work will also be done from Earth, in centers spread over several continents.
Listening to Mars
A seismometer and a microphone opened new senses on Mars. Those who live there will also have to monitor an active planet: its quakes, its atmosphere, its dust.
This lesson is a reflection by the author of this book, based on the facts reported in the preceding chapters, where their sources are given.
Appendices
Further reading
Appendix Understanding CNES’s role
A few ideas, explained simply, to follow this book.
The project owner
The body that commissions and funds an instrument and guarantees it gets built, entrusting its design and manufacture to laboratories and companies.
Laser-induced breakdown spectroscopy
A technique that vaporizes a spot of rock with a very powerful laser, then analyzes the light of the resulting spark to find out which chemical elements it contains. It is the principle of ChemCam and part of SuperCam.
A seismometer
An instrument that records ground vibrations. Quake waves travel through the planet and carry information about what they met: crust, mantle, core.
The operations center
A place on Earth where teams prepare the commands sent to an instrument and receive its data. CNES’s FOCSE in Toulouse plays this role for French instruments on Mars.
These explanations are general notions. ChemCam’s principle follows CNES’s page on the instrument.
Appendix Timeline
CNES and Mars.
December 19, 1961. CNES founded.
November 26, 1965. Diamant puts Asterix into orbit.
December 24, 1979. Ariane 1’s maiden flight.
June 2, 2003. Mars Express launches, with OMEGA and SPICAM.
August 2010. ChemCam delivered to JPL.
August 6, 2012. Curiosity and ChemCam land on Mars.
November 26, 2018. InSight and SEIS land on Mars.
April 7, 2019. First marsquake detected.
February 18, 2021. Perseverance and SuperCam land on Mars.
December 15, 2022. InSight’s last communication.
December 21, 2022. NASA declares the InSight mission over.
March 2024. Idefix rover handed over to Japan.
October 20, 2026. Planned MMX launch.
2031. Planned return of Phobos samples.
Sources: those of the chapters; ISAS/JAXA, MMX page (rover handover in March 2024).
Appendix Sources and method
This book tells CNES’s role in exploring Mars from the agency’s official pages. This appendix shows where the facts come from and what does not agree.
The main sources
This book replaces an earlier page of about 17,000 words that covered the whole French space program; here we keep to Mars. It draws on CNES’s pages on its history, the “Planète Mars” dossier, Mars Express, ChemCam, InSight, SuperCam and MMX.
What does not agree
CNES dates the end of InSight operations to December 21, 2022; JPL reports a last communication on December 15. NASA’s release of December 21, 2022 explains the gap: these are two distinct events, the last contact and the declaration of the end of the mission, and we give both. The ChemCam page gives Curiosity’s launch as November 26, 2011 in one place and the 25th in another; NASA dates it to November 26, 2011, the date we keep. The MMX page counts twelve and then thirteen instruments.
Length
This book runs to about one thousand four hundred words. The goal set for this collection was one hundred thousand. We did not reach it, and we prefer to say so. The French instruments are told in more detail in this collection’s biographies devoted to the missions that carry them.
The illustration
The image at the top of this book is an illustration whose exact provenance we were unable to verify.
Online sources
- CNES, “History”
- CNES, “Planète Mars” dossier
- CNES, “Mars Express”
- CNES, “ChemCam”
- CNES, “InSight”
- CNES, “SuperCam”
- CNES, “MMX”
- NASA, end of the InSight mission (December 21, 2022)
Facts checked against these sources on October 11, 2026.
Go further
Mars Library
This book extends the page with a complete settlement architecture. The dossier above remains deliberately self-contained: Arcadia is optional further reading, not a prerequisite for understanding it.
Arcadia — Master Plan of the First Martian City
