SPACE ADVENTURES
THALES
Discover
TRAVELING WAVE TUBES
Veuillez consulter sur
tablette en mode paysage ou
Smartphone en mode portrait
Mercury
1 mission
Venus
4 missions
Near Earth
1 mission
Earth
Mercury
1 mission
Mars
7 missions
Jupiter
3 missions
Dwarf
planets
1 mission
Small bodies
5 missions
Saturn
2 missions
Uranus
Neptune
Sun
4 missions
Universe
6 missions
DWARF
PLANETS
URANUS
EARTH
SMALL
BODIES
UNIVERSE
VENUS
SUN
MERCURY
NEPTUNE
JUPITER
MARS
SATURN
MICROWAVE & IMAGING SUB-SYSTEMS
Microwave & Imaging Sub-Systems
With over 60 years of expertise in aerospace, Thales MIS remains present in the long-term in all space solutions ranging from TWT technologies to new amplification solutions for very high throughput satellites (VHTS), flexible satellites as well as constellations.
Our portfolio continues to expand to include new solutions in development such as our newest Dual TWT as well as our SSPA or our HEMPT EV0 for electrical propulsion.
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH3609 (2 units)
RF Power: 20 Watts
Cumulated working time:
163,700 hours
Parker Solar Probe
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4704C (4 units)
RF Power: 71 Watts
Solar orbiter
Ulysses
Launch
February 2020
Arrival to destination
June 2020
End of mission
2027- 2030 (planned)
Outcome
By combining observations from Solar Orbiter’s instruments, scientists hope to find answers to some questions: What drives the Sun’s 11-year cycle of rising and subsiding magnetic activity? What heats up the upper layer of its atmosphere, the corona, to millions of degrees Celsius? What drives the generation of the solar wind? What accelerates the solar wind to speeds of hundreds of kilometres per second? And how does it all affect our planet?
Missions
Launch
October 2006
Arrival to destination
December 2006
End of mission
October 2014
Outcome
The objective of the mission is the study of coronal mass ejections by the Sun. It employs two twin satellites, one preceding the Earth in its revolution around the Sun and the other following it, which provide a three-dimensional image of the phenomenon from its genesis to its interactions with the interplanetary and space environment of the Earth.
Characteristics
The Sun is the star of the Solar System. Solar energy transmitted by solar radiation makes life on Earth possible by providing light energy and heat energy, allowing the presence of water in its liquid state and the photosynthesis of plants.
DistanceBetween Earth to the Sun: 150 million km
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4704C (3 units)
RF Power: 60 Watts
Cumulated working time:
225,500 hours
Stereo (Solar TErrestrial RElations Observatory)
Name Sun Diameter 1,392,000 km
Launch
August 2018
Arrival to destination
November 2018
End of mission
2025 (planned)
Outcome
Parker Solar Probe travels through the Sun’s atmosphere, closer to the surface than any spacecraft before it, facing brutal heat and radiation conditions to provide humanity with the closest-ever observations of a star.
Thales TWT
Band: X-band (7.25-8.50 GHz) and
32 GHz-band
Reference: TH4604C (3 units) and TH4606C (3 units)
RF Power: 11 Watts and 34 Watts
Launch
October 1990
Arrival to destination
June 1994
End of mission
June 2009
Outcome
Ulysses’ principal findings include data that showed that there is a weakening of the solar wind over time (which was at a 50-year low in 2008), that the solar magnetic field at the poles is much weaker than previously assumed, that the Sun’s magnetic field “reverses” in direction every 11 years, and that small dust particles coming from deep space into the solar system are 30 times more abundant than previously assumed.
Mission
BepiColombo
Launch
October 2018
Arrival to destination
December 2025 (planned)
End of mission
2026/2027 (planned)
Outcome
This mission is on a seven year journey to the smallest and least explored terrestrial planet in our Solar System. When it arrives at Mercury in late 2025, it will endure temperatures in excess of 350 °C and gather data during its one-year nominal mission, with a possible one-year extension.
Name MercuryDiameter 4,879 kmCharacteristicsMercury is the closest planet to the sun, one of the four telluric planets of the Solar System, and has a rocky structure like the Earth. It is also the smallest of the planets.
DistanceTo the Sun: 58 million km
To the Earth: varies between
80 million km to 220 million km
Thales TWT
Band: X-band (7.25-8.50 GHz) and
32 GHz-band
Reference: TH4604C (4 units) and TH4606C (4 units)
RF Power: 37 Watts and 37 Watts
Thales TWT
Band: 32 GHz-Band
Reference: THL32070C (3 units)
RF Power: 70 watts
Veritas
Magellan
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH 3609 (2 units)
RF Power: 20 Watts
Cumulated working time:
47,200 hours
Launch
2031/2032 (planned)
Arrival to destination
2034/2035 (planned)
End of mission
2038/2039 (planned)
Outcome
EnVision is designed to study volcanic gases in the atmosphere, atmosphere-surface interactions, surface composition, and the interior structure of Venus, and will return high-resolution radar images of the surface.
Thales TWT
Band: 32 GHz-Band
Reference: THL32150C (1 unit)
RF Power: 150 watts
Launch
May 1989
Arrival to destination
August 1990
End of mission
October 1994
Outcome
Complete radar mapping of Venus surface, allowing the study of its geological features. Magellan imagery of Venus is still the most complete and detailed available today, these are the most precise images we have to date.
Launch
November 2005
Arrival to destination
April 2006
End of mission
December 2014
Objectives/Results
- Study of atmospheric circulation: rotation speed, general circulation mechanisms
- Role of the greenhouse effect on the past evolution of the planet and its impact on its evolution
- Study of present tectonic and volcanic activity
- Origins of the divergence between the evolution of the Earth and that of Venus.
EnVision
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH 4704C (2 units)
RF Power: 67 Watts
Cumulated working time:
74,200 hours
Name VenusDiameter 12,104 kmCharacteristicsCovered of volcanoes and lava flows, Venus is considered to be a sister of Earth because of their similar size and composition.
DistanceTo the Sun: 108 million km
To the Earth: varies between
42 million km to 280 million km
Launch
2031 (planned)
Arrival to destination
2031/2032 (planned)
End of mission
2034/2035 (planned)
Outcome
VERITAS will study the planet's surface and interior with a powerful new generation of scientific tools. It will create incredibly detailed radar maps of Venus' surface, vastly improving the maps made by NASA’s Magellan mission in the 1990s.
Venus Express
Thales TWT
Band: X-band (7.25-8.50 GHz)
and 32 GHz-band
Reference: TH4300C (3 units)
and TH4606C (2 units)
RF Power: 100 Watts and 34 Watts
Exo Mars
Launch
November 1996
Arrival to destination
September 1997
End of mission
November 2006
Outcome
Mars Global Surveyor became the first successful mission to the red planet in two decades. The mission has studied the entire Martian surface, atmosphere, and interior. One of the most exciting observations of the spacecraft's wide-angle camera system is that the red planet has very repeatable weather patterns.
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH3908 (2 units)
RF Power: 20 Watts
Cumulated working time:
87,100 hours
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4704C (2 units)
RF Power: 66 Watts
Name MarsDiameter 6,779 kmCharacteristicsA telluric planet half the size of Earth. Like Earth, Mars has seasons due to the tilt of its axis of rotation.
DistanceTo the Sun: 228 million km
To the Earth: varies between 56 million km to 400 million km
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4300C (2 units)
RF Power: 102 Watts
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4704C (2 units)
RF Power: 50 Watts
Launch
August 2005
Arrival to destination
Mars 2006
End of mission
Not planned today
Outcome
NASA's Mars Reconnaissance Orbiter is on a search for evidence that water persisted on the surface of Mars for a long periods of time. While other Mars missions have shown that water flowed across the surface in Mars' history, it remains a mystery whether water was ever around long enough to provide a habitat for life.
MMX (Martian Moons eXploration)
Mars Global Surveyor
Launch
November 2011
Arrival to destination
Landed on August 2012
End of mission
2026 (planned)
Outcome
Early in its mission, Curiosity's scientific tools found chemical and mineral evidence of past habitable environments on Mars. It continues to explore the rock record from a time when Mars could have been home to microbial life.
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4704C (2 units)
RF Power: 70 Watts
Launch
March 2016
Arrival to destination
October 2016
End of mission
2026 (planned)
Outcome
The program comprises two missions. The first launched in 2016 consists of the Trace Gas Orbiter (TGO) and Schiaparelli, an entry, descent and landing demonstrator module. The second is planned for launch in 2022 and comprises a rover and surface science platform. Together they will address the question of whether life has ever existed on Mars.
Launch
2024
Arrival to destination
2025
End of mission
2029
Outcome
Mars has two moons known as Phobos and Deimos. MMX is planning to perform a series of observations and collect surface material from Phobos and bring it back to the Earth (sample return).
Mars reconnaissance orbiter
Mars Express
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4300C (2 units)
RF Power: 102 Watts
MAVEN (Mars Atmosphere and Volatile EvolutioN)
Mars Science Laboratory (curiosity rover)
Launch
2013
Arrival to destination
September 2014
End of mission
2030 (planned)
Outcome
Scientists will use MAVEN data to determine the role that loss of volatiles from the Mars atmosphere to space has played through time, giving insight into the history of Mars' atmosphere and climate, liquid water, and planetary habitability.
Launch
June 2003
Arrival to destination
December 2003
End of mission
2022
Outcome
To study the martian atmosphere and climate, the planet’s structure, its mineralogy and its geology, and to search for traces of water.
Double Asteroid Redirection Test (DART)
Giotto
Psyche
Launch
November 2021
Arrival to destination
2022
Outcome
DART is a planetary defense-driven test of technologies for preventing an impact of Earth by an asteroid. DART was the first demonstration of the kinetic impactor technique to change the motion of an asteroid in space. The asteroid Didymos was the target for DART demonstration.
Launch
2023 (planned)
Arrival to destination
2029-2030 (planned)
End of mission
Not planned today
Outcome
The Psyche mission is a journey to a unique metal asteroid orbiting the Sun between Mars and Jupiter. What makes the asteroid Psyche unique is that it appears to be the exposed nickel-iron core of an early planet, one of the building blocks of our solar system.
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH3908A (4 units)
RF Power: 30 Watts
Cumulated working time:
329,300 hours
Launch
July 1985
Arrival to destination
March 1986
End of mission
July 1992
Outcome
Making encounters with comets Halley and Grigg–Skjellerup, Giotto was ESA’s first deep-space mission. It imaged a comet nucleus for the first time and found the first evidence of organic material on a comet.
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4704C (1 unit)
RF Power: 60 Watts
Name Small bodiesCharacteristics
The small bodies of the Solar System (asteroids, comets, Kuiper belt objects, icy moons, rings, and dust) represent archives of the state of the proto-solar disk at various times and places during the history of our Solar System’s formation.
Rosetta & Philae
Launch
March 2004
Arrival to destination
August 2014
End of mission
September 2016
Outcome
Rosetta's main objective was to rendezvous with and enter orbit around Comet 67P/Churyumov-Gerasimenko, performing observations of the comet's nucleus and coma.
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4300C (3 units)
RF Power: 102 Watts
Cumulated working time:
52,000 hours
OSIRIS-REx
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH3609 (2 units)
RF Power: 20 Watts
Cumulated working time:
61,400 hours
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4300 (2 units)
RF Power: 100 Watts
Launch
September 2016
Arrival to destination
December 2018
End of mission
September 2023 (planned)
Outcome
OSIRIS-REx will travel to a near-Earth asteroid called Bennu and bring a small sample back to Earth for study.
Launch
2023 (planned)
Arrival to destination
2031 (planned)
End of mission
2035 (planned)
Outcome
JUICE will perform detailed investigations of Jupiter and its system in all their inter-relations and complexity with particular emphasis on Ganymede as a planetary body and potential habitat. Investigations of Europa and Callisto would complete a comparative picture of the Galilean moons.
Launch
2024 (planned)
Arrival to destination
2034 (planned)
End of mission
Not planned today
Outcome
NASA's Europa Clipper spacecraft will conduct a detailed survey of Jupiter's moon Europa to determine whether the icy moon could harbor conditions suitable for life. The spacecraft, in orbit around Jupiter, will make about 45 close passes over Europa, shifting its flight path for each flyby to soar over a different location so that it eventually scans nearly the entire moon.
Europa Clipper
Juice (JUpiter ICy moons Explorer)
Name JupiterDiameter 139,822 km
Juno
Thales TWT
Band: X-band (7.25-8.50 GHz) and
32 GHz-band
Reference: TH4704C (4 units) and TH4606C (4 units)
RF Power: 53 Watts and 29 Watts
Characteristics
Fifth in line from the Sun, Jupiter is, by far, the largest planet in the solar system – more than twice as massive as all the other planets combined. As on other gaseous planets, violent winds of nearly 600 km/h run through the upper layers of the planet.
DistanceTo the Sun: 778 million km
To the Earth: varies between
591 million km to 960 million km
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4604C (3 units)
RF Power: 26 Watts
Cumulated working time:
141,700 hours
Thales TWT
Band: X-band (7.25-8.50 GHz) and
32 GHz-band
Reference: TH4604C (3 units) and TH4606C (3 units)
RF Power: 20 Watts and 35 Watts
Launch
August 2011
Arrival to destination
July 2016
End of mission
July 2025 (planned)
Outcome
Juno's principal goal is to understand the origin and evolution of Jupiter. Underneath its dense cloud cover, Jupiter safeguards secrets to the fundamental processes and conditions that governed our solar system during its formation. As our primary example of a giant planet, Jupiter can also provide critical knowledge for understanding the planetary systems being discovered around other stars.
Name SaturnDiameter 116,460 km
Characteristics
The most famous feature of the planet is its prominent ring system. Saturn is the second most massive planet in the Solar System. Saturn is classified as a gas giant because it is mainly composed of hydrogen and helium.
DistanceTo the Sun: 1.4 billion km
To the Earth: varies between
1.4 billion km to 1.6 billion km
Launch
2026 (planned)
Arrival to destination
2034 (planned)
End of mission
2036/2037 (planned)
Outcome
Dragonfly, a rotorcraft-lander expedition to Saturn’s large, exotic moon Titan, will explore dozens of locations across Titan, sampling and measuring the composition of Titan’s organic surface materials to characterize the habitability of Titan’s environment and investigate the progression of prebiotic chemistry.
Launch
October 1997
Arrival to destination
February 2004
End of mission
September 2017
Outcome
Orbiting the ringed planet Saturn and its numerous moons, the Cassini spacecraft and Huygens probe had been a keystone of exploration of the Saturnian system and the properties of gaseous planets in our solar system.
Thales TWT
Band: X-band
Thales TWT
Band: X-band (8.393-8.45 GHz)
Reference: TH4300C (4 units)
RF Power: 103 watts
Cassini-Huygens
Dragonfly
New Horizons
Name Ceres, Pluto, Eris, Makemake, HaumeaCharacteristics
According to the International Astronomical Union, which sets definitions for planetary science, a dwarf planet is a celestial body that orbits the sun, has enough mass to assume a nearly round shape, has not cleared the neighborhood around its orbit and is not a moon. Ceres is located in the asteroid belt. Pluto, Eris, Makemake and Haumea are in the outdoor solar system.
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4604C (2 units)
RF Power: 15 Watts
Cumulated working time:
119,500 hours
Launch
January 2006
Arrival to destination
July 2015
End of mission
2026 (planned)
Outcome
The New Horizons mission is helping us understand worlds at the edge of our solar system by making the first reconnaissance of the dwarf planet Pluto and by venturing deeper into the distant, mysterious Kuiper Belt – a relic of solar system formation.
Ulysses
› see mission
Solar orbiter
› see mission
Parker Solar Probe
› see mission
STEREO (Solar TErrestrial RElations Observatory)
› see mission
BepiColombo
› see mission
Magellan
› see mission
Venus Express
› see mission
Juno
› see mission
JUICE (JUpiter ICy moons Explorer)
› see mission
Europa Clipper
› see mission
Cassini-Huygens
› see mission
New Horizons
› see mission
Herschel
› see mission
Planck
› see mission
TESS (Transiting Exoplanet
Survey Satellite)
› see mission
Euclid
› see mission
JWST (James Webb Space Telescope)
› see mission
Nancy Grace Roman Space Telescope
› see mission
Launch
2027 (planned)
Arrival to destination (Lagrange L2)
2027 (planned)
End of mission
2032/2037 (planned)
Outcome
The Roman Space Telescope is a NASA observatory designed to settle essential questions in the areas of dark energy, exoplanets, and infrared astrophysics.
JWST (James Webb Space Telescope)
Thales TWT
Band: X-band (7.25-8.50 GHz) and
32 GHz-band
Reference: TH4604C (4 units) and TH4626C (4 units)
RF Power: 23 Watts and 52 Watts
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4604C (6 units)
RF Power: 35 Watts
Cumulated working time:
451,900 hours
Herschel
TESS (Transiting Exoplanet Survey Satellite)
Launch
April 2018
Arrival to destination
July 2018
End of mission
End of 2020 (planned)
Outcome
TESS will survey 200,000 of the brightest stars near the sun to search for transiting exoplanets.
Thales TWT
Band: 32 GHz-band
Reference: TH4626C (3 units)
RF Power: 76 Watts
Launch
2023 (planned)
Arrival to destination (Lagrange L2)
2023 (planned)
End of mission
2028 (planned)
Outcome
Euclid is designed to give us important new insights into the "dark side" of the universe -- namely dark matter and dark energy, both thought to be key components of our cosmos.
Thales TWT
Band: 32 GHz-band
Reference: TH4626C (1 unit)
RF Power: 11 Watts
Cumulated working time:
9,700 hours
Launch
May 2009
Arrival to destination
July 2009
End of mission (Lagrange L2)
April 2013
Outcome
The Herschel Space Observatory's large telescope and state-of-the-art infrared detectors provide the first confirmed finding of oxygen molecules in space discovered in the Orion star-forming complex.
Planck
Nancy Grace Roman Space Telescope (formerly WFIRST)
Euclid
Launch
May 2009
Arrival to destination (Lagrange L2)
July 2009
End of mission
April 2013
Outcome
Planck produced its first all-sky image in 2010. Analysis has already highlighted numerous star-forming clouds across the Milky Way galaxy as well as a previously invisible population of galaxies covered in dust billions of years old.
Thales TWT
Band: 26 GHz-band
Reference: TH4626C (2 units)
RF Power: 52 Watts
Launch
December 2021
Arrival to destination (Lagrange L2)
2022
End of mission
2027/2032 (planned)
Outcome
JWST is an orbiting infrared observatory that will complement and extend the discoveries of the Hubble Space Telescope. The longer wavelengths enable JWST to look much closer to the beginning of time and to hunt for the unobserved formation of the first galaxies, as well as to look inside dust clouds where stars and planetary systems are forming today.
Name UniverseCharacteristics
The universe is all of space and time and their contents, including planets, stars, galaxies, and all other forms of matter and energy. While the spatial size of the entire universe is unknown, it is possible to measure the size of the observable universe, which is currently estimated to be 93 billion light-years in diameter.
Rosetta & Philae
› see mission
Giotto
› see mission
Psyche
› see mission
DART
› see mission
OSIRIS-REx
› see mission
MAVEN
› see mission
Mars Science Laboratory (curiosity rover)
› see mission
Mars reconnaissance orbiter
› see mission
Mars Express
› see mission
Exo Mars
› see mission
Mars Global Surveyor
› see mission
MMX (Martian Moons eXploration)
› see mission
The 1980s sparked a revolution of knowledge in astrophysics and cosmology. Funded by ESA, NASA, JAXA, CNES and other National Space Agencies, over fifty deep space missions have been decided, starting with Mars (MARS OBSERVER), Jupiter (GALILEO) or Saturn (CASSINI). They have now targeted almost all of the major planets in our solar system, except Uranus and Neptune but including Pluto through the NEW HORIZONS mission. Besides, multiple probes such as ROSETTA have been sent to study comets and asteroids. To embrace cosmologic scales, advanced telescopes have been embarked on helio-synchronous satellites (HUBBLE for example) and since the 2000s, they are located at L2 Lagrange orbital point to improve their stability, in particular PLANCK, GAIA and tomorrow JAMES WEBB SPACE TELESCOPE. Satellites and probes collect data and images and download them to Earth using a microwave link. To deal with huge distances, millions to billions of kilometers, large receiving antennas have been built, up to 35 meters wide. At the other end, space amplifiers usually integrate high efficiency Travelling Wave Tubes (TWT). 20 years ago, communications were done in X-band but the high level of interference and the limited bandwidth now affected the efficiency. Millimeter wave links were therefore preferred, starting with Jupiter, Mercury and Sun missions, at 26 GHz and even 32 GHz despite higher atmospheric attenuation. Up to 1.5 GHz bandwidth is now available to increase data link throughputs and resilience. TWT amplifiers are also used to implement the satellite telemetry for platform maneuvers and scientific instruments management, and for deep space missions it is usually in X-band.
DE
Thales heritage :
from Deep Space to Earth
FR
Microwave & Imaging
Sub-Systems
Sun
4 missions
Mercury
1 mission
Venus
4 missions
Mars
7 missions
Small
bodies
5 missions
Jupiter
3 missions
Saturn
2 missions
Dwarf
planets
1 mission
Universe
6 missions
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4704C (4 units)
RF Power: 71 Watts
Name MercuryDiameter 4,879 kmCharacteristicsMercury is the closest planet to the sun, one of the four telluric planets of the Solar System, and has a rocky structure like the Earth. It is also the smallest of the planets.
DistanceTo the Sun: 58 million km
To the Earth: varies between 80 million km
to 220 million km
Name VenusDiameter 12,104 kmCharacteristicsCovered of volcanoes and lava flows, Venus is considered to be a sister of Earth because of their similar size and composition.
DistanceTo the Sun: 108 million km
To the Earth: varies between 42 million km to
280 million km
Name MarsDiameter 6,779 kmCharacteristicsA telluric planet half the size of Earth. Like Earth, Mars has seasons due to the tilt of its axis of rotation.
DistanceTo the Sun: 228 million km
To the Earth: varies between 56 million km to 400 million km
Thales TWT
Band: X-band (7.25-8.50 GHz)
Reference: TH4300C (3 units)
RF Power: 102 Watts
Cumulated working time:
52,000 hours
Characteristics
Fifth in line from the Sun, Jupiter is, by far, the largest planet in the solar system – more than twice as massive as all the other planets combined. As on other gaseous planets, violent winds of nearly 600 km/h run through the upper layers of the planet.
DistanceTo the Sun: 778 million km
To the Earth: varies between 591 million km to 960 million km
Characteristics
The most famous feature of the planet is its prominent ring system. Saturn is the second most massive planet in the Solar System. Saturn is classified as a gas giant because it is mainly composed of hydrogen and helium.
DistanceTo the Sun: 1.4 billion km
To the Earth: varies between 1.4 billion km to
1.6 billion km
Launch
May 2009
Arrival to destination (Lagrange L2)
July 2009
End of mission
April 2013
Outcome
The Herschel Space Observatory's large telescope and state-of-the-art infrared detectors provide the first confirmed finding of oxygen molecules in space discovered in the Orion star-forming complex.
Thales TWT
Band: 32 GHz-band
Reference: TH4626C (3 units)
RF Power: 76 Watts
mis.sales-contact@thalesgroup.com
Contact
www.thalesgroup.com
PLANÈTES
NAINES
PETITS
CORPS
SATURNE
SOLEIL
MERCURE
UNIVERS
TERRE
Planck
› voir mission
JWST (James Webb Space Telescope)
› voir mission
Avec plus de 60 ans d’expertise dans l’Aérospatial, Thales MIS est un acteur incontournable des solutions d’amplification spatiale, allant de la technologie des Tube à Ondes Progressives (TOP) aux nouvelles solutions d’amplification pour les satellites à haut débit, les satellites flexibles ainsi que les constellations.
Notre portefeuille produit continue de s'étendre pour inclure de nouvelles solutions en cours de développement, notamment notre dernier Dual-TWT, le SSPA et notre HEMPT EV0 pour la propulsion électrique
Nancy Grace Roman Space Telescope
› voir mission
Herschel
› voir mission
Euclid
› voir mission
TESS (Transiting Exoplanet
Survey Satellite)
› voir mission
Thales heritage : from Deep Space to Earth
Privacy notice
Veritas
› see mission
EnVision
› see mission
Dragonfly
› see mission