ESA Top Multimedia
Prospect mission animation
ESA’s Prospect mission is a key stepping stone on our journey back to the Moon and beyond.
Prospect has a suite of instruments that will drill beneath the surface of the Moon’s polar regions, extract samples, and analyse them to search for volatiles such as water ice. Volatiles are potential sources of water, oxygen, and fuel for future explorers.
The package combines a drilling and sampling system (ProSEED) with a miniaturised laboratory (ProSPA) to extract the cold-trapped volatiles and determine their origin and abundance.
The mini lab will also test in-situ resource utilisation, such as oxygen extraction from lunar regolith – the layer of loose dust and rock on the Moon's surface.
Prospect operations will take place during the course of one lunar day, over about 10 Earth days.
Prospect will reach the lunar surface with the Intuitive Machines’ Nova-C lunar lander on the IM-4 mission, as part of NASA’s Commercial Lunar Payload Services (CLPS) initiative, under an ESA–NASA agreement.
Prospect stands for Package for Resource Observation, in-Situ Prospecting for Exploration, Characterisation & Testing.
More information: www.esa.int/prospect
How Europe studies the Sun
English
How does Europe study the Sun? Discover the missions revealing the secrets of our closest star, from SOHO and Solar Orbiter to Proba-3, which is creating artificial solar eclipses in space to unlock new insights into the Sun's mysterious corona.
Featuring ESA Reserve Astronaut Sara García Alonso.
Spanish
¿Cómo se estudia el Sol desde Europa? Acompaña a Sara García Alonso en un recorrido por las misiones de la ESA que observan nuestra estrella, desde SOHO y Solar Orbiter hasta Proba-3, que está creando eclipses solares artificiales en el espacio para investigar la misteriosa corona solar.
Con Sara García Alonso, astronauta de reserva de la ESA.
Earth from Space: Baku, Azerbaijan
On World Environment Day, the Copernicus Sentinel-2 mission brings us an amazing view from space of Baku, capital of Azerbaijan, hosting this year’s celebration.Webb unveils young stars across every stage of formation
Webb unveils young stars across every stage of formationTessera’s ‘embedding’ view of Cambridge (split)
Mineralogy at Mawrth Vallis
Webb sniffs methane from interstellar Comet 3I/ATLAS
Webb's MIRI image of the interstellar Comet 3I/ATLAS in three different light wavelengthsSmile: cleanroom to space
Smile successfully launched from Europe’s Spaceport in French Guiana on 19 May 2026.
This timelapse captures the excitement and precision of launch operations as the spacecraft begins its journey to study the connection between the Sun and Earth.
Smile (the Solar wind Magnetosphere Ionosphere Link Explorer) is an international space science mission designed to investigate how the solar wind interacts with Earth's magnetosphere. By observing these dynamic processes from space, Smile will help scientists better understand space weather and its effects on our planet's magnetic environment.
Space science for your heart
SpaceX CRS-34 approach and docking
This timelapse was published by ESA astronaut Sophie Adenot on social media with the following caption:
Day 106, orbit 1644 — This timelapse shows the approach and docking of the SpaceX CRS‑34 resupply mission on 17 May. Isn’t it amazing to think that this docking manoeuvre takes place while flying at 28,000 km/h around the Earth?
The blurred dot in the middle of the picture is actually a micrometeoroid impact on the Cupola window… No worries, it’s been there for a long time !
--
Jour 106, orbite 1644 – Ce timelapse montre les phases d'approche et d’amarrage de la mission de ravitaillement SpaceX CRS‑34 le 17 mai. Incroyable de se dire que cette manœuvre d’amarrage s’effectue à 28 000 km/h autour de la Terre !
Le point flou au centre de l’image est un impact de micrométéoroïde sur le hublot de la Cupola… mais pas d’inquiétude, il n’est pas récent !
Maupiti, French Polynesia
ESA astronaut Sophie Adenot published this picture as part of a set on social media with the following caption:
Day 108, orbit 1675 — Our orbital path regularly takes us over countless breathtaking atolls, appearing like brilliant drops of turquoise scattered across the deep blue of both the Pacific and Indian oceans. These ecosystems, essential to a lot of marine and coastal species, face threats resulting from human activity, particularly the accelerating impacts of climate change, like ocean warming and rising sea levels.
From orbit, it becomes extremely clear that for life to continue thriving, all our planet’s ecosystems must be protected.
--
Jour 108, orbite 1675 – Notre trajectoire nous amène régulièrement à survoler d’innombrables atolls, de lumineuses gouttes d’un bleu turquoise dispersées sur le bleu profond des océans Pacifique et Indien. La vue est à couper le souffle. Ces écosystèmes, essentiels à de nombreuses espèces marines et côtières, sont menacés par les activités humaines, en particulier par l’accélération des effets du changement climatique, tels que le réchauffement des océans et l’élévation du niveau de la mer.
Depuis l’orbite, il est très clair que pour que la vie continue de prospérer, tous les écosystèmes de notre planète doivent être protégés.
Installing MatISS-4, designed to trap atmospheric contaminants
This timelapse was published by ESA astronaut Sophie Adenot on social media with the following caption:
Day 105, orbit 1629 — This accelerated video shows the installation of MatISS-4, a French experiment that aims to collect and study the biocontamination of the air inside the European Columbus module. Biocontamination – such as small skin cells, droplets from sneezes or saliva, and bacteria – is unavoidable, so we make sure to clean surfaces every week (I’ll publish a housekeeping timelapse soon!), but some areas are particularly hard to reach…
Over 10 years, MatISS has shown that the Station’s systems are very efficient; after several months of exposure, the contamination level inside the MatISS cases remains low. MatISS-4 features a new design, which will allow the contaminated membranes to be analysed at the European Synchrotron in Grenoble using an X-ray nano-imaging instrument. Go science!
MatISS has also enabled researchers to identify surfaces that are more resistant to biocontamination, opening up many applications on Earth: in public transportation, where thousands of people touch the same surfaces every day, in places where limiting contamination is key, such as hospitals, cruise ships, and submarines, and even in livestock farming. Less biocontamination = less cleaning with chemical products!
--
Jour 105, orbite 1629 – Cette vidéo accélérée montre l’installation de MatISS‑4, une expérience française qui vise à collecter et étudier la biocontamination de l’air à l’intérieur du module européen Columbus. La biocontamination – cellules de peau, éternuements, postillons, bactéries – est inévitable. Nous nettoyons les surfaces chaque semaine (je publierai bientôt un timelapse de ménage !), mais certaines zones sont particulièrement difficiles d’accès…
Depuis plus de 10 ans, MatISS démontre que les systèmes de la Station sont très efficaces ; après plusieurs mois d’exposition, le niveau de contamination à l’intérieur des boîtiers reste faible. MatISS‑4 présente un nouveau design, qui permettra d’analyser les membranes contaminées à l’aide d’un instrument de nano-imagerie X du synchrotron européen de Grenoble. Vive la science !
MatISS a également permis aux chercheurs d’identifier des surfaces plus résistantes à la biocontamination, ouvrant la voie à de nombreuses applications sur Terre : dans les transports publics, où des milliers de personnes touchent les mêmes surfaces chaque jour , dans les lieux où limiter la contamination est essentiel, tels que les hôpitaux, les navires de croisière et les sous‑marins, et même dans les élevages. Moins de biocontamination = moins de nettoyage avec des produits chimiques !
A new buzz at ESA’s astronaut centre
Launch of the ESA EAC beekeeping clubThis Month at ESA: May 2026
What did space deliver for Europe this month? From asteroid flybys to Mars landing tests, new discoveries from Webb and Hubble, and ESA astronaut Sophie Adenot capturing shooting stars from orbit, here’s your monthly roundup from the European Space Agency.
This month also saw ESA team up with DON’T NOD for Aphelion, a sci-fi adventure inspired by real space science and exploration.
Journey to the centre of a galaxy cluster
Journey to the centre of a galaxy clusterMount Vesuvius, Italy
This picture was published on social media as part of a set by ESA astronaut Sophie Adenot with the following caption:
Day 103, orbit 1598 — From orbit, volcanoes are some of the most beautiful natural sights… End of April, Etna caught me by surprise one morning as I opened the shutters. The whiteness of its slopes… and that elegant plume of smoke which is a gentle reminder that it’s only lightly, very lightly, asleep. I just had time to take a quick photo, but I kept an eye out for it the next day to capture a few more! A special thought for my fellow ESA astronaut Luca Parmitano, who is from Catania, at the foot of Etna.
Less than a minute later, and we’re flying over Vesuvius, instantly recognisable by the vast crater, the path winding up to the summit, and, most of all, Naples spread out all around it.
--
Jour 103, orbite 1598 – Les volcans sont parmi les plus beaux sites naturels à voir depuis l’orbite… Fin avril, l’Etna m’a prise par surprise un matin alors que j’ouvrais les volets… La blancheur des ses pentes, et surtout ce beau volute de fumée qui rappelle qu’il a le sommeil léger, très léger. J’ai juste eu le temps de prendre une photo, mais je l’ai guetté le lendemain pour en faire d’autres! Clin d’oeil à mon camarade Luca Parmitano, originaire de Catane, au pied de ce majestueux volcan…
Moins d’une minute plus tard, et nous sommes au-dessus du Vésuve, reconnaissable au premier coup d’oeil par son immense cratère, le sentier qui serpente vers le sommet, et surtout Naples qui l’entoure.
MTG-I2 embarks on journey to Europe’s Spaceport
100 days in space
This picture was published by ESA astronaut Sophie Adenot on social media with the following caption:
Day 101, orbit 1567 — 100 days in space already… Living and working aboard the International Space Station is becoming second nature, but each morning, as I open the Cupola shutters, I’m reminded of how extraordinary it really is.
Over these past weeks, I’ve been constantly challenged, amazed, and inspired – by the work, by the views, and by the incredible teams on the ground who make all of this possible.
Looking forward to the next 100 days!
--
Jour 101, orbite 1567 – Déjà 100 jours dans l’espace… Vivre et travailler à bord de la Station spatiale internationale est presque devenu la routine. Et pourtant, chaque matin, en ouvrant les volets de la Cupola, la vue me rappelle à quel point cette aventure est extraordinaire.
Ces dernières semaines m’ont challengée, émerveillée et inspirée à travers le travail, les vues à couper le souffle et les équipes formidables au sol qui rendent tout cela possible.
Hâte de découvrir ce que les 100 prochains jours me réservent !
Little Red Dot Abell2744-QSO1 (NIRCam Image)
Little Red Dot Abell2744-QSO1 (NIRCam Image)Hot surfaces during Europe's heatwave 'seen' by Sentinel-3
European Service Module at the (space) disco
European Service Module for Artemis III during acoustic testing, May 2026.Change in Earth’s molten core flow 1997–2025
The molten core, which swirls about 2200 km beneath our feet, generates Earth’s geomagnetic field as it moves. By measuring small changes in the magnetic field, scientists have historically observed the core flowing mainly westwards. But in 2010, it unexpectedly changed direction deep beneath the Pacific Ocean and started moving strongly eastwards. The reasons for this unexplained reversal in the flow of molten material are still a mystery but satellites, including ESA’s Swarm and CryoSat, provided data that has now been analysed and published.
The study, published in the Journal Studies of Earth’s Deep Interior, analyses both ground observations and satellite data between 1997 and 2025. The video shows the large scale of flow in the molten core between 1997 and 2025. The overturn of the flow below the Pacific and the main stable structures of the flow have been isolated. Each arrow indicates the movement of the core liquid horizontal to Earth’s surface.
Read full story: Insights into Earth’s molten outer core from space
Group photo of ESA’s astronaut reserve
Group photo with the members of ESA's astronaut reserve in the training hall of ESA’s European Astronaut Centre .From orbit: a tapestry of cities and fleets
A view from the Cupola window in mid‑April, as brightly lit cities and shipping fleets drift beneath the orbiting path of the International Space Station in this nighttime timelapse captured by ESA astronaut Sophie Adenot.
DNA Nano Therapeutics‑3 experiment timelapse
In this timelapse, ESA astronaut Sophie Adenot processes blood stem cell samples to help scientists understand how larger quantities of clinical‑grade stem cells could be produced in microgravity. This research aims to improve stem cell quality, with potential applications in treating blood diseases and cancer, while also opening new avenues for commercial research in orbit.
The Life Science Glovebox, located in the Kibo module, allows biological samples to be handled in a fully sealed workspace designed to ensure strict containment. Preventing contamination is critical on the ISS – both to protect the crew and to maintain the integrity of the research.
Inflight call with ESA astronaut Sophie Adenot
On 20 May, ESA astronaut Sophie Adenot conducted an in-flight call with selected media representatives live aboard the International Space Station. During the discussion, Sophie shared insights into life and research in orbit, including scientific experiments supporting human health, climate science and future space exploration.
Hyguane signature ceremony in the Jupiter Room at Europe’s Spaceport in French Guiana
Smile launch highlights
ESA’s Smile satellite launched aboard a Vega-C rocket from Europe’s Spaceport in French Guiana. The rocket lifted off on at 04:52 BST / 05:52 CEST (00:52 local time) on 19 May 2026.
Smile flew to space on Vega-C flight VV29. At 35 m tall, a Vega-C weighs 210 tonnes on the launch pad and the rocket used three solid-propellant-powered stages to take Smile to orbit before the fourth liquid-propellant stage took over for a precise drop-off around Earth.Smile (the Solar wind Magnetosphere Ionosphere Link Explorer) is a joint mission between the European Space Agency (ESA) and the Chinese Academy of Sciences (CAS).
Smile will use four science instruments to study how Earth responds to the solar wind from the Sun. In doing so, Smile will improve our understanding of solar storms, geomagnetic storms and the science of space weather.
Vega-C liftoff with Smile up close
Wide view of Vega-C liftoff with Smile
Page 1 de 3
- 1
- 2
- 3
- Suivante
- Dernière »
