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ESA Top Multimedia

ESA Top Multimedia

The Exploration Company resonance igniter

Test-firing of a resonance igniter built by The Exploration Company in Bordeau France in November 2025. 

Building a working rocket engine is one thing, igniting the engine in a stable and repeatable way is an engineering feat in itself. Resonance ignition produces high‑frequency waves inside a shaped cavity. As the waves interact, they resonate and heat the propellants until they ignite. This type of ignition uses just the propellants themselves. 

Instead of relying on a spark, a pyrotechnic device or a plasma torch, the system creates self‑amplifying pressure waves that rapidly increase the temperature of propellant gases. 

Propellant mixtures are injected in gaseous form through a “resonance nozzle” into a cavity. If the shape of the nozzle and the cavity are exactly right, then the propellants bounce back and forth across the cavity and produce standing acoustic waves: one wave of gas moving in one direction meets the wave returning in the opposite direction. These waves break into each other at points called nodes, resulting in high pressure fluctuations and increasing the temperature of the gas.  

The Exploration Company is investigating this phenomenon as a novel technique to start their rocket engines, requiring no external ignition devices, just a resonance nozzle and cavity. An advantage of resonance igniters is that they can be used repeatedly, they use little electricity, there is no need for additional parts and they are therefore lightweight. Current technologies for rocket engines use spark plugs that require a high voltage, glow plugs that need time to warm up, or torch igniters. 

The first test campaign concluded in November and showed the technology works, allowing The Exploration Company to develop know-how on the device’s workings and better understand the geometry needed for successful, rapid and repeatable ignition.  

They tested different setups and analysed modes of ignition. The data from this test campaign will help develop another version of the device that will be included in the pre-combustors of The Exploration Company’s staged-combustion cycle high-thrust engine programme. 

The test was conducted within a €9 M contract from the European Space Agency as part of the Technologies for High-thrust Re-Usable Space Transportation initiative, THRUST! 

See you in March, Artemis II

The Artemis II rocket with the full Moon on its launchpad

ESA's sustainability ambition

Space activities are unlike any others. They interact not just with Earth, but with three interconnected environments: Earth, Earth’s orbit, and the Moon and deep space. On Earth, we aim to reduce the space sector’s environmental impacts while maximising the societal and environmental benefits of our missions. In orbit, we manage space debris and collision risks to maintain safe and secure operations. For the Moon and deep space, we are laying the foundations to minimise the impact of our missions on and around other celestial bodies.

Guided by our core values, ESA is committed to making its activities more sustainable, redefining how space activities are conceived, executed and shared with the world. Our objective is clear: to address the most pressing challenges and implement ambitious changes, both in our own practices and in close collaboration with our partners.

Looking ahead, in support of Strategy 2040, ESA is determined to lead through ambition, action and collaboration, building a future where space is not only a domain of opportunity but also a model of sustainability, responsibility and global unity.

εpsilon mission patch

ESA astronaut Sophie Adenot (FR) is scheduled to fly to the International Space Station in 2026. Her first mission to the International Space Station, εpsilon, is named after the fifth Greek letter and the fifth brightest star of the Leo constellation, following the French tradition to name human spaceflight missions after celestial bodies. It also pays tribute to the five career astronauts of ESA’s 2022 class. In mathematics, 'ε' represents something small. In the extensive collaborative effort of space exploration, involving thousands of participants, all roles, including the astronaut’s role, stay small, yet all are meaningful.

Just as the name reflects the power of small, yet impactful contributions and how multiple parts unite to create a whole, so does the idea behind the patch design. The hummingbird motif is central; though one of Earth’s smallest birds, it plays a crucial role in the jungle’s ecosystem, pollinating numerous plants. Around the edge is a ring of small dots, symbolising the many small contributions that together make great achievements possible. All these little actions that can be coordinated to form a circle and close the loop. At the top, three of these dots are coloured – blue, white and red – representing Sophie’s home country, France, and ESA’s exploration destinations: Earth, the Moon and Mars.

Three lines emerge from the 'i' of the εpsilon, shaping the tail of a shooting star, a poetic reminder that dreams keep us alive. Also featured are five stars, a tribute to the five career astronauts of ESA’s 2022 class. At the base of the patch is round blue shape, representing Earth’s surface and its natural beauty: mountains, forests and landscapes that Sophie enjoys exploring. It serves as a reminder of our motivation for spaceflight: to explore, learn and return with this knowledge to benefit life on Earth.

From an emotional perspective, the same message is conveyed. In life’s intricate tapestry, small threads contribute to create the most beautiful patterns. A kind word, a gentle smile, a moment of patience – these seemingly insignificant actions can transform lives and shape destinies. This patch invites each of us to embrace the potential of our smallest actions as they ripple outward, touching hearts and inspiring souls.

Animation of Ariane 6 with four boosters

Spinning Ariane 6 rocket showing four boosters it can use to rocket to space.

Ariane 6 is a three-stage launch vehicle with the boosters, main stage and then upper stage expending their propellant to reach orbit. The number of boosters and length of the tip of the rocket, called the fairing, can be adapted per mission.

Ariane 6 in its four-booster configuration doubles the rocket’s performance compared to the two-booster version that flew first in 2024. The P120C boosters used by Ariane 6 are one of the most powerful one-piece motors in production in the world. Flying with four boosters takes Ariane 6 to a whole new class of rockets. With the extra thrust from two more boosters Ariane 6 can take around 21.6 tonnes to low Earth orbit, more than double the 10.3 tonnes it could bring to orbit with just two boosters. 

Jammertest: strengthening satellite navigation

Satellite navigation is essential to everyday life, from tracking your morning jog to landing air ambulances. But as reliance on satellite navigation grows, so do the risks associated with its interruption, natural or intentional. To strengthen European resilience in navigation, the European Space Agency (ESA) takes part annually in Jammertest.

Organised on the remote island of Andøya, Norway, Jammertest is the world’s largest open air testing campaign for jamming and spoofing resilience. In September 2025, ESA engineers attended Jammertest with ESA’s mobile navigation lab to test how different systems respond to interference. After this, the data are analysed to check which technologies perform the best against jamming and spoofing. 

By bringing together academia, industry and governmental organisations, Jammertest helps make satellite navigation better for everyone and protects European assets. 

More on Jammertest: ESA - Navigating through interference at Jammertest

Technicians prepare Ariane 6 for flight VA267

Technicians prepare Ariane 6 for flight VA267

Eurasian and Indian tectonic plates collision zone

Eurasian and Indian tectonic plates collision zone

Dark rings and new light

Dark rings and new light

Earth from Space: Rudong coast, China

The Copernicus Sentinel-2 mission takes us over part of the coastal area of Rudong County on China’s eastern seaboard.

Dentist remotely controlling a robotic arm

A dentist at ESA’s European Centre for Space Applications and Telecommunications (ECSAT) in the UK controlling a robotic arm at the University of Glasgow’s SCENE facility at Loch Lomond.

This is Crew-12

From left to right: Roscosmos cosmonaut Andrei Fedyaev, NASA astronauts Jack Hathaway and Jessica Meir, and ESA astronaut Sophie Adenot from France.

Hayli Gubbi eruption in Ethiopia, by MTG-Sounder

This animation uses data from the MTG-Sounder satellite’s Infrared Sounder instrument. It tracks the eruption of Ethiopia's Hayli Gubbi volcano on 23 November 2025.

The background imagery shows surface temperature changes while infrared channels highlight the developing ash plume. The satellite's timely observations enable tracking of the evolving ash plume over time.

Artemis II rollout

On 17 January, the Artemis II Space Launch System rocket and Orion spacecraft were rolled out from the Vehicle Assembly Building at NASA's Kennedy Space Center in Florida, to Launch Pad 39B. The 6.5-km journey took around 12 hours and was carried out using NASA's crawler-transporter, which has been moving rockets to launch pads for over 50 years.

At the top of the rocket sits the Orion spacecraft, bearing the ESA and NASA logo and designed to carry four astronauts on a 10-day lunar flyby mission. Artemis II will be the first crewed flight of the Artemis programme and the first time humans have ventured towards the Moon in over 50 years.

Their journey depends on our European Service Module, built by industry from more than 10 countries across Europe. This powerhouse will take over once Orion separates from the rocket, supplying electricity from tis four seven-metre-long solar arrays, providing air and water for the crew, and performing key propulsion burns during the mission, including the critical trans-lunar injection that sends the spacecraft and its crew on their trajectory towards the Moon.

Ignis mission timelapses: Earth and Moon views from the International Space Station

ESA project astronaut Sławosz Uznański-Wiśniewski captured these stunning timelapse videos during his 20-day stay aboard the International Space Station as part of Axiom Mission 4, known as Ignis. Filmed from the Cupola – the Space Station’s iconic seven-windowed observation module – the footage showcases breathtaking views of Earth and the Moon from orbit.

Launched on 25 June 2025 aboard a SpaceX Dragon spacecraft, Sławosz conducted 13 experiments proposed by Polish institutions in collaboration with ESA, plus three ESA-led investigations. These spanned human research, materials science, biology, biotechnology and technology demonstrations.

The Ax-4 mission marks the second commercial human spaceflight for an ESA project astronaut. Ignis was sponsored by the Polish government and supported by ESA, the Polish Ministry of Economic Development and Technology (MRiT) and the Polish Space Agency (POLSA).   

Access the related broadcast quality footage

ESA Academy Experiments teams at the Orbital Robotics Laboratory

After being selected to join the ESA Academy Experiments programme, three student teams from universities across Europe were invited to carry out the experimental part of their research projects in ESA’s test facilities with support and guidance from experts.

For their experiments, the student teams made use of ESA’s ORBIT facility – a part of the Orbital Robotic Laboratory (ORL) located at ESTEC, the agency’s technical heart in the Netherlands. ORBIT consists of a 43 m2 ultra-flat floor – the height difference between its lowest and highest points is less than a millimetre.

The Skywalker team from Aalborg University, Denmark, used the simulated two-dimensional microgravity environment to test the reinforcement learning algorithms they have developed for their robotic arm. Their project aims to demonstrate the concept of autonomous crawling in microgravity.

In the very first ORBIT facility experiment involving human participants, the V-STARS team from Birkbeck, University of London, and the University of Kent, UK, investigated the relationship between the human vestibular system (region of the inner ear responsible for body balance) and the perception of verticality in a microgravity environment.

The GRASP team from Sapienza University of Rome, Italy, explored an innovative approach to performing manoeuvres with non-cooperative objects in space. The robotic arm they have developed themselves is sporting an adhesive gripper inspired by geckos.

Read more

Magnetic avalanche in action

Solar Orbiter’s most detailed view yet of a large solar flare, observed during its 30 September 2024 close approach to the Sun. 

The imagery was published in 2025, but now scientists have focused in on the details to uncover an exciting and surprising result: individual solar flares are triggered by initially weak disturbances that quickly become more violent – much like an avalanche on a snowy mountain. This rapidly evolving process creates a ‘sky’ of raining plasma blobs that continue to fall even after the flare subsides.

For the first time, this process is revealed in the video shown here, along with the supplementary videos featured in the full story.

When Solar Orbiter’s Extreme Ultraviolet Imager (EUI) first started observing the region at about 23:06 Universal Time (UT), a dark arch-like ‘filament’ of twisted magnetic fields and plasma was already present, connected to a cross-shaped structure of progressively brightening magnetic field lines.

Zooming in to this feature shows that new magnetic field strands are appearing in every image frame – equivalent to every two seconds or less. Each strand is magnetically contained, and they become twisted, like ropes. Then, just like in a typical avalanche, the region becomes unstable. The twisted strands begin to break and reconnect, rapidly triggering a cascade of further destabilisations in the area. This creates progressively stronger reconnection events and outflows of energy, seen as increasing brightness in the imagery.

A sudden brightening begins at 23:29 UT, followed by the dark filament disconnecting from one side, launching into space and at the same time violently unrolling at high speed. The unwinding closest to the footprint is recorded at 250 km/s, increasing to 400 km/s at the site of disconnection. Bright sparks of reconnection are seen all along the filament in stunning high resolution as the flare erupts at 23:47 UT.

At the same time, ribbon-like features are seen moving extremely quickly down through the Sun’s atmosphere. These streams of ‘raining plasma blobs’ are signatures of energy deposition from the reconnection events, which get stronger and stronger as the flare progresses. Even after the flare subsides, the rain continues for some time.

While EUI captured this high-resolution imagery, Solar Orbiter’s SPICE and STIX instruments monitored the temperatures and particle emissions at different layers in the Sun’s atmosphere. They revealed the slow rise of ultraviolet to x-ray emission prior to the flare, followed by a dramatic increase in x-ray emission during the main phase of the flare – signifying that particles were accelerated to 40-50% the speed of light equivalent to about 431–540 million km/h. This was recorded close to the base of the filament connection point as it unfurled into space.

After the main phase of the flare, the original cross-shape of magnetic field lines relaxes and the instruments see the plasma cool down to ‘normal’ levels. Bundles of looped magnetic field lines and suspended plasma – ‘arcades’ – hang over the flare site for some time.

Read more 

Solar Orbiter is a space mission of international collaboration between ESA and NASA. The EUI instrument is led by the Royal Observatory of Belgium (ROB).

Legs made for a Mars landing

To land on the right foot on the Red Planet, European engineers have been dropping a skeleton of the four-legged ExoMars descent module at various speeds and heights on simulated martian surfaces.

Watch a quick sequence of some of the drops from different angles. For over a month, Thales Alenia Space and Airbus teams ran dozens of vertical drops using a full-scale model of the landing platform at the ALTEC facilities in Turin, Italy. 

This first series of tests involved dropping the model onto both hard and soft surfaces, the latter filled with powdery, Mars-like soil.  The team changed the speed and height of the falls by a few centimetres. 

During the test campaign, the four legs replicated the structure and dimensions of those that will fly to Mars. The lightweight, deployable legs are interconnected and equipped with shock absorbers to withstand the impact.

Another goal of the campaign was to verify the performance of the touchdown sensors. A system installed in all four legs detects when the spacecraft approaches the surface and triggers the shutdown of the descent engines after a soft landing.  

The landing legs are crucial gear for the safe touchdown of the ExoMars Rosalind Franklin rover mission in 2030, alongside parachutes and engines that will slow the spacecraft’s descent onto Mars. 

While Thales Alenia Space is the industrial lead of the mission, Airbus provides the landing platform and ALTEC offers technical support.

ESA preview 2026

As a new year begins, let’s take a look at what’s ahead for the European Space Agency in 2026. From Earth to the farthest reaches of the Solar System, 2026 marks a year of firsts that continue to shape the future of space.

Press conference with ESA astronaut Sophie Adenot

Media representatives joined French ESA astronaut Sophie Adenot, on Monday 5 January, for a hybrid press conference to learn more about her first mission to space.

This event, held at the European Astronaut Centre (EAC) in Germany, was the final media event in Europe ahead of her launch to the International Space Station.

Sophie selected the name ‘εpsilon’ for her first mission, currently planned no earlier than 15 February, reflecting the power of small, yet impactful contributions, and how many parts come together to make a whole.

During εpsilon, Sophie will conduct a wide range of tasks on the International Space Station, including European-led scientific experiments, medical research, supporting Earth observation and contributing to operations and maintenance on the Station.

The European Space Agency explained

We are the European Space Agency, committed to peacefully exploring and using space to benefit everyone. Since our creation as an intergovernmental organisation in 1975, we've been championing European scientific and industrial interests in space.

What does ESA do?

In short, ESA’s job is to draw up the European space programme and carry it through. ESA's programmes are designed to find out more about Earth, its immediate space environment, our Solar System and the Universe, as well as to develop satellite-based technologies and services, and to promote European industries. ESA also works closely with space organisations outside Europe.

Who belongs to ESA?

Austria, Belgium, Czech Republic, Denmark, Estonia, Finland, France, Germany, Greece, Hungary, Ireland, Italy, Luxembourg, the Netherlands, Norway, Poland, Portugal, Romania, Slovenia, Spain, Sweden, Switzerland and the United Kingdom. Slovakia, Latvia and Lithuania are Associate Members. Canada takes part in some projects under a cooperation agreement. Bulgaria, Croatia, Cyprus and Malta have cooperation agreements with ESA.

Where do ESA’s funds come from?

ESA’s mandatory activities (space science programmes and the general budget) are funded by a financial contribution from all the Agency’s Member States, calculated in accordance with each country’s gross national product. In addition, ESA conducts a number of optional programmes. Each Member State decides in which optional programme they wish to participate and the amount they wish to contribute.

How big is ESA’s budget?

ESA's budget for 2025 is €7.68 billion. ESA operates on the basis of geographical return, i.e. it invests in each Member State, through industrial contracts for space programmes, an amount more or less equivalent to each country’s contribution. 

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