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ESA Top Multimedia

ESA Top Multimedia

Annular solar eclipse over Antarctica

A 'ring of fire' solar eclipse seen from Concordia research station in Antarctica on 17 February 2026. 

Peaking at 19:47 local time (12:47 CET), the Moon passed directly in front of the Sun's centre, leaving only a thin, glowing annulus of sunlight visible. Astronomers call this moment annularity, and it lasted just two minutes, though the full partial eclipse spanned around two hours. 

Only a narrow path on Earth can witness an annular eclipse in its entirety, and today the crew at Concordia were among the very few located within that corridor. While a partial eclipse could be seen from other regions, only this small slice of Antarctica experienced the Sun transformed into a perfect ring of fire over the icy plateau.  

ESA's Proba-2 spacecraft also witnessed the eclipse from Earth orbit. Three upcoming solar eclipses - on 12 August 2026, 2 August 2027, and 26 January 2028 - will be visible from Europe. 

Operated by the French and Italian Antarctic research programmes, Concordia sits 1100 km inland at an altitude of 3200 m. It is currently summer at the station: today, the Sun stayed above the horizon for nearly 20 hours, with temperatures reaching a comparatively mild –29 °C. But soon the light will fade: from May to August, the Sun will not rise at all, plunging the station into four months of continuous darkness where temperatures can fall below –80 °C. During this polar winter, the crew must live in complete isolation and full autonomy. 

These extreme conditions make Concordia one of the best analogues on Earth for long-duration spaceflight, including future crewed missions to the Moon and Mars. For this reason, ESA sends a medical doctor every year to the station to study how humans adapt to disrupted daylight cycles, isolation and confinement. 

Despite the challenges, Concordia often rewards its crew with views found nowhere else on Earth.

You can find out more about the medical doctors who winter over at Concordia station on our blog.

Students kick off experiments on ESA’s flat floor

Students kick off experiments on ESA’s flat floor

Unfolding MetOp-SG-B1’s solar wing

Unfolding MetOp-SG-B1’s solar wing

Greta rocket engine first test-firing campaign

The Greta engine firing up on a new mobile test stand in Trauen, Germany. Greta was ignited multiple times from July to November 2025 and showed stable operations, including controlled shutdowns. During the test campaign the engine fired continuously for over 40 seconds at a time.

The Greta project, part of the European Space Agency’s Future Launchers Preparatory Programme is developing a 5 kN thrust class rocket engine that can be restarted reliably several times.

Greta uses hydrogen peroxide and ethanol as propellants, a more sustainable alternative with a lower carbon footprint compared to monomethyl hydrazine propellant used by most traditional rocket engines in this thrust range.

Greta was tested on a new, low-cost and versatile mobile test stand with instruments measuring data such as pressure and temperature, which will be used to further optimise the engine.

Greta’s 30-cm high combustion chamber is built up in layers by melting metal powders with a laser. This technique allows for complex shapes to be made that would be difficult to achieve with conventional metallurgy. For example, the Greta engine is cooled by passing fluid through complex channels built into the engine as close as possible to the inner wall of the chamber which is in contact with the hot – over 2000°C – combustion gases.

ArianeGroup in Ottobrunn, Germany is the prime contractor for Greta. This type of engine could be used on lunar landers or on kick stages, such as Astris that is being developed for Europe’s Ariane 6 rocket.

NGC 1637 (Hubble WFC3 and Webb NIRCam images)

NGC 1637 (Hubble WFC3 and Webb NIRCam images)

Meet ESA Astronaut Sophie Adenot

Born in France in 1982, Sophie Adenot is an engineer, helicopter test pilot and colonel in the French Air and Space Force. Selected as an ESA astronaut in 2022, she completed her basic training at the European Astronaut Centre in 2024 and launched to the International Space Station on 13 February 2026 for her first mission, εpsilon.

France hit by severe flooding

France hit by severe flooding

Smile orbit transfer and magnetometer boom deployment (artist impression)

The joint European-Chinese Smile mission will launch this spring from Europe’s Spaceport in French Guiana, on a Vega-C rocket.

The rocket will place Smile into an almost-circular orbit around Earth’s poles.

Over the following month, Smile will gradually alter its orbit, firing its engines as it flies over Antarctica. Its final orbit will take it 121 000 km above the North Pole to collect information on Earth’s magnetic field and the northern lights, before flying close over the South Pole to deliver its data.

This special orbit will enable Smile to spend about 80% of its time at high altitude above the northern hemisphere, collecting continuous observations of the northern lights for 45 hours at a time.

After Smile has reached this final ‘science orbit’, it will deploy a three-metre-long boom that carries two magnetometer sensors at the end. These sensors will measure the strength and direction of magnetic fields around the spacecraft.

Known as ‘MAG’, data from this science instrument will be combined with data from Smile’s X-ray camera, ultraviolet camera, and particle detector to give humankind its first complete look at how Earth reacts to streams of particles and bursts of radiation from the Sun.

By improving our understanding of the solar wind, solar storms and space weather, Smile will fill a stark gap in our understanding of the Solar System and help keep our technology and astronauts safe in the future.

Watch Smile’s launch and solar panel deployment (artist impression) here.

Smile (the Solar wind Magnetosphere Ionosphere Link Explorer) is a joint mission between the European Space Agency and the Chinese Academy of Sciences.

Smile launch and solar panel deployment (artist impression)

3… 2… 1… lift off!

The joint European-Chinese Smile mission will launch this spring from Europe’s Spaceport in French Guiana, on a Vega-C rocket.

Following liftoff, the first, second and third stages of the rocket will be released one by one, before Smile finally separates from the fourth (upper) stage 57 minutes after launch.

Around 5–10 minutes later, Smile will deploy its solar arrays, stretching them out ready to collect the sunlight necessary to power its onboard systems and science instruments.

Using X-ray and ultraviolet cameras, as well as particle and magnetic field detectors, Smile will give humankind its first complete look at how Earth reacts to streams and bursts of particles and radiation from the Sun.

By improving our understanding of the solar wind, solar storms and space weather, Smile will fill a stark gap in our understanding of the Solar System and help keep our technology and astronauts safe in the future.

Watch Smile’s orbit transfer and magnetometer boom deployment (artist impression) here.

Smile (the Solar wind Magnetosphere Ionosphere Link Explorer) is a joint mission between the European Space Agency and the Chinese Academy of Sciences.

Sophie Adenot exercising on the CEVIS bike

ESA astronaut Sophie Adenot during one of her first workouts at the start of the εpsilon mission.

Uranus rotation in timelapse

This timelapse shows a full rotation of Uranus captured by NASA/ESA/CSA James Webb Space Telescope. Thanks to its orbit at L2, Webb was able to observe the planet for approximately 17 hours continuously. 

The video consists of over 1200 slices of multi-object spectroscopy data. By mapping distribution and temperature of hydrogen in its molecular and trihydrogen form, these observations provide the most detailed view to date of Uranus’ vertical upper atmosphere. The video shows where temperatures and densities of charged particles peak, and reveals clear auroral structures shaped by the planet’s unusual magnetic field.

Using Webb’s NIRSpec instrument, the team detected the faint glow from molecules high above the clouds. These unique data provide the most detailed portrait yet of where the planet’s auroras form, how they are influenced by its unusually tilted magnetic field, and how Uranus’s atmosphere has continued to cool over the past three decades. The results offer a new window into how ice-giant planets distribute energy in their upper layers.

Read more.

Space safety hazards: space weather

The Sun doesn't feel like a threat – until it does. 

Solar storms can put on beautiful light shows in the night sky, known as auroras. But they can also cause serious problems for the technology we rely on every day. Strong solar activity can interfere with communications, power grids and navigation systems on Earth and satellites in orbit.

Although we cannot stop such space weather from happening, we can limit its impact. The most effective protection comes from carefully monitoring the Sun and the effects of solar activity on the space environment around Earth. This information can be shared with system operators through services similar to weather reports and forecasts, so the operators can take protective action when needed.

Observing space weather and reducing its risks are activities of ESA’s Space Safety programme. ESA is building a wide range of space weather services, brought together in the ESA Space Weather Service Network, supported by data from ESA's own space weather sensors deployed in space. These services help industry and spacecraft operators respond quickly and effectively when space weather events occur. 

Learn more about Space Weather at ESA and the ESA Space Weather Service network.

Watch all Space safety hazards videos.

Rising ocean-surface temperatures in the Mediterranean Sea

Each year, the world’s leading climate scientists evaluate the most critical evidence on how our planet is changing. Their assessments draw heavily on data from Earth-observing satellites – and the latest 10 New Insights in Climate Science report 10 New Insights in Climate Science report delivers a stark warning: the planet’s energy balance is drifting further out of alignment, oceans are warming at unprecedented rates, and the land’s capacity to absorb carbon is declining, along with other troubling trends.
Insight number two highlights that marine heatwaves are becoming more intense and prolonged. These changes are causing severe ecosystem damage, undermining coastal livelihoods, increasing extreme weather risks and weakening the ocean’s capacity to absorb carbon.

The image depicts sea-surface temperature anomalies in the Mediterranean Sea for August 2023 relative to 1985–2005, and highlights two cases of biodiversity loss.

Read full story: Revealed: 10 new insights in climate science

Moving space debris out of the way with OMLET

The team explores the technical complexities of laser-based collision avoidance, an approach to safely redirect space junk away from the path of active satellites.

With space getting increasingly crowded, space debris represents a major problem to future missions. Vital services like communications, navigation and weather forecasting are severely limited without functioning satellites.

The European Space Agency is already making use of laser technology to detect and monitor space debris with the Izaña laser ranging station complex. But what if we could also use laser technology to actually prevent collisions?

ESA, from its European Space Operations Centre (ESOC), began exploring this concept with a general feasibility study funded by its Space Safety Programme. This effort has since progressed: meet OMLET (Orbit Maintenance via Laser MomEntum Transfer), a ground-based solution being advanced to mitigate collision risk into low Earth orbit.

Based on a high-power laser platform integrated with precision pointing systems and adaptive optics, this concept will enable the application of small, controlled velocity changes to space debris objects. Through the interaction between the laser beam and the illuminated object, a slight trajectory adjustment could reduce the probability of conjunction or even prevent collisions.

OMLET is currently transitioning from requirement definition stage to design and implementation. The current Phase A/B1 is carried out by an international consortiumconsortium led by the Institute of Technical Physics at the German Aerospace Centre (DLR).

Celeste

The world runs on invisible satellite navigation signals: they fuel our society, generate economic growth and are integral to our security. But they can fade or vanish.

A pivotal step for more robust navigation is expanding to a system including a fleet of satellites in low Earth orbit, operating in a range of signals and frequencies.

ESA’s Celeste demonstrator mission will test the potential of such a system in providing significant augmentation and diversity to Galileo and other existing systems, increasing resilience and enabling new services to places where today’s satnav systems cannot reach.

Learn more about Celeste.

Dragon approaching the International Space Station for docking

The SpaceX Dragon carrying four Crew-12 members, including ESA astronaut Sophie Adenot, nears the International Space Station for a docking to the Harmony module’s space-facing port.

Docking of Crew-12 to the International Space Station

Watch the replay of the Crew-12 docking operations at the International Space Station (ISS).

On 14 February, a SpaceX Falcon 9 rocket lifted off from Space Launch Complex 40 at NASA’s Kennedy Space Center at 10:15 UTC (11:15 CET). Following this, the SpaceX Dragon spacecraft docked at the orbiting lab at 20:15 UTC (21:15 CET).

ESA astronaut Sophie Adenot is flying as mission specialist for the εpsilon mission. The other Crew-12 members are NASA astronauts Jessica Meir (commander) and Jack Hathaway (pilot), and Roscosmos cosmonaut Andrei Fedyaev (mission specialist).

Crew-12: Docking, hatch opening and welcome remarks

Watch the docking operations of Crew-12 to the International Space Station (ISS), which took place on 14 February 2026 at 21:15 CET. The docking is followed by the hatch opening and the welcome remarks by the astronauts already present in the ISS.                                        

ESA astronaut Sophie Adenot flies as mission specialist. The other Crew-12 members are NASA astronauts Jessica Meir and Jack Hathaway, respectively commander and pilot of the mission, and Roscosmos cosmonaut Andrei Fedyaev, mission specialist.

The French ESA astronaut is the first of her class, the Hoppers, to fly. Sophie has chosen the name εpsilon for her mission, which may last up to nine months. On board the Station, she will conduct a wide range of tasks, including European-led scientific experiments and medical research, support Earth observation activities, and contribute to operations and maintenance on the Station.

Crew-12 Walkout with ESA astronaut Sophie Adenot

Crew-12 Walkout with ESA astronaut Sophie Adenot

Full replay: Launch of Crew-12 with Sophie Adenot | εpsilon mission

Watch the launch of ESA astronaut Sophie Adenot to the International Space Station (ISS), aboard a SpaceX Falcon 9 rocket from Space Launch Complex 40 at NASA’s Kennedy Space Centre. Sophie flies as mission specialist. The other Crew-12 members are NASA astronauts Jessica Meir and Jack Hathaway, respectively commander and pilot of the mission, and Roscosmos cosmonaut Andrei Fedyaev, mission specialist.

Highlights of Sophie Adenot’s launch to the ISS

Watch the highlights of the launch of ESA astronaut Sophie Adenot to the International Space Station (ISS) on Crew-12. A SpaceX Falcon 9 rocket lifted off from Space Launch Complex 40 at NASA’s Kennedy Space Centre in Florida, USA, on Friday 13 February 2026 at 10:15 GMT/11:15 CET (5:15 local time).

Sophie flies as mission specialist. The other Crew-12 members are NASA astronauts Jessica Meir and Jack Hathaway, respectively commander and pilot of the mission, and Roscosmos cosmonaut Andrei Fedyaev, mission specialist.

The French ESA astronaut is the first of her class, the Hoppers, to fly. Sophie has chosen the name εpsilon for her mission, which may last up to nine months. On board the Station, she will conduct a wide range of tasks, including European-led scientific experiments and medical research, support Earth observation activities, and contribute to operations and maintenance on the Station.

Watch the full launch replay

Launch of Crew-12 to the ISS

Watch the liftoff of ESA astronaut Sophie Adenot to the International Space Station (ISS), aboard a SpaceX Falcon 9 rocket from Space Launch Complex 40 at NASA’s Kennedy Space Centre. Sophie flies as mission specialist. The other Crew-12 members are NASA astronauts Jessica Meir and Jack Hathaway, respectively commander and pilot of the mission, and Roscosmos cosmonaut Andrei Fedyaev, mission specialist.

Watch the full launch replay

εpsilon launch

εpsilon launch

Highlights of first launch of Ariane 6 with four boosters

At 16:45 GMT/17:45 CET the first Ariane 6 rocket with four boosters lifted off from Europe’s Spaceport in French Guiana on 12 February, taking 32 Amazon Leo satellites to orbit.

This is Ariane 6’s most powerful version yet. The new three-stage European rocket can be adapted according to each mission with either two or four boosters as well as the length of the fairing – the nosecone that splits vertically in two. This launch was the sixth Ariane 6 flight, the first to fly with four boosters and also the first with the long fairing.

Ariane 6 in its four-booster configuration, known as Ariane 64, doubles the rocket’s performance compared to the two-booster version that has flown five times including the inaugural flight 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.

Crew-12 upon their arrival at the Kennedy Space Center

Crew-12 upon their arrival at the Kennedy Space Center

Crew-12 in front of a SpaceX booster

Crew-12 in front of a SpaceX booster

Sophie Adenot ready for first space mission

ESA astronaut Sophie Adenot is preparing to launch to the International Space Station for her first space mission: εpsilon.

After years of intensive training — from emergency procedures to spacewalk simulations — the countdown has begun. Flying alongside astronauts from NASA and Roscosmos, Sophie will join an international crew living and working together in space.

Aboard the ISS, Sophie will live and work in microgravity, conducting scientific research and performing a range of European- and French-led experiments that advance knowledge for life on Earth and in space.

Join us live on YouTube to watch the launch of Sophie Adenot.

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.

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