
ESA Top Multimedia
What plants can grow in space?

Do you know the difference between a vegetable, a fruit, and a seed? In this video, we explore the different components of plants, and their varying growth needs and yields, to consider which plants might be best suited for growing on a future space mission.
Second Ariane 6 in the spotlights
Webb visits a star-forming spiral

Earth from Space: Maha Kumbh Mela festival, India
Survey of Andromeda's satellite galaxies
Lifting the veil

Metal made in space lands on Earth

The first metal 3D part ever created on orbit has landed on Earth.
The sample was produced in ESA’s Metal 3D Printer on the International Space Station. Now, it’s on Earth for the first time, at ESA’s technical heart in the Netherlands (ESTEC).
The printer, developed by Airbus and its partners, was installed in the Columbus module by ESA astronaut Andreas Mogensen during his Huginn mission in January 2024. In June, the facility succeeded in making its first print, a curvy line in the shape of an 'S’. In summer, the printer produced its first full sample, and then a second sample in December.
This first sample will now be tested in the Materials and Electrical Components Laboratory at ESTEC and compared to samples printed on Earth to understand how microgravity affects the printing process.
The second sample will be handed over to the Technical University of Denmark (DTU).
While astronauts have operated plastic 3D printers on the International Space Station before, this marks the first successful metal printing on orbit. As missions venture farther from Earth, in-space manufacturing will be crucial for self-sufficiency, allowing astronauts to manufacture essential parts, repair equipment and create tools on demand, without relying on costly resupply missions.
Drilling into Mars

The ExoMars Rosalind Franklin rover will drill deeper than any other mission has ever attempted on the Red Planet.
The third episode in the series shows how the rover will extract, collect and analyse martian samples in a high-fidelity simulation.
Rosalind Franklin will be the first rover to reach a depth of up to two metres deep below the surface, acquiring samples that have been protected from harsh fsurface radiation and extreme temperatures.
The drill system combines multiple precission mechanisms in an intricate automated sequence. It uses three extension rods that connect tor form a two-metre “drill string”.
As the rover drills, it will simultaneously investigate the borehole using infrared spectroscopy to study mineral composition.
The ExoMars Rosalind Franklin mission is part of Europe’s ambitious exploration journey to search for past and present signs of life on Mars.
For the latest mission updates, visit ESA’s ExoMars website and our FAQ section.
Watch all the videos from the ExoMars Rosalind Frankin mission series.
Star field image taken by Proba-3's ASPIICS coronagraph

A spiral hiding an impostor

Earth from Space: Tokyo, Japan

MTG-S and Sentinel-4 in the cleanroom at Bremen
Revealed: glacier ice loss over two decades

As part of a community effort, the Glacier Mass Balance Intercomparison Exercise, Glambie, has compiled all major studies using observations from a wealth of different techniques to provide an estimate of the world’s glacier mass change over the last two decades. The results, published in the journal Nature, show that ice melting from glaciers around the world is depleting regional freshwater resources and driving global sea levels to rise at ever-faster rates. The animation here illustrates the different observation methods used in the research, and Vatnajökull in Iceland as an example.
Read full story: Glacier melt intensifying freshwater loss and accelerating sea-level rise
Sentinel-4: European air quality monitoring for Copernicus
The James Webb Space Telescope maps full picture of how Phoenix Galaxy Cluster forms stars

The pierogi challenge
Sentinel-4 scanner

The Copernicus Sentinel-4 mission, an ultraviolet, visible, near-infrared light spectrometer carried on the Meteosat Third Generation Sounder satellite in geostationary, provides hourly observations to monitor air quality over Europe. These hourly observations are set to make a breakthrough for air quality monitoring from space.
The animation shows how the mirror mechanism works to scan Earth’s atmosphere to provide critical data on the composition of the atmosphere at a spatial resolution of 8 km x 8 km.
Near-surface ozone over Europe, June 2018

Using data from satellite sensors such as Tropomi on Sentinel-5P and GOME-2 on MetOp along with forecast models, this animation shows concentrations of near-surface ozone every hour over Europe throughout June 2018. It shows a typical summer month with several instances of heavy pollution, for example over the Netherlands and Germany on 7 June. Concentrations often exceed 120 μg/m3, which exceeds the eight-hourly mean limit of European air-quality standards.
The Copernicus Sentinel-4 mission, an ultraviolet, visible, near-infrared light spectrometer carried on the Meteosat Third Generation Sounder satellite in geostationary, provides hourly observations to monitor air quality over Europe. These hourly observations are set to make a breakthrough for air quality monitoring from space.
Near-surface nitrogen dioxide over Europe, November 2018

Using data from satellite sensors such as Tropomi on Sentinel-5P and GOME-2 on MetOp along with forecast models, this animation shows concentrations of near-surface nitrogen dioxide every hour over Europe throughout November 2018. Urban and industrial areas are particularly polluted – concentrations over the Randstad area in the Netherlands often reaches 40 μg/m3, exceeding European air-quality standards. High values can also be seen in valleys near sources of pollution where there is little wind.
The Copernicus Sentinel-4 mission, an ultraviolet, visible, near-infrared light spectrometer carried on the Meteosat Third Generation Sounder satellite in geostationary, provides hourly observations to monitor air quality over Europe. These hourly observations are set to make a breakthrough for air quality monitoring from space.
Fly! Project media briefing

Watch the latest updates on ESA’s Fly! Feasibility Study with Daniel Neuenschwander, ESA Director of Human and Robotic Exploration, John McFall, Member of the ESA Astronaut Reserve & Fly! Subject Matter Expert, Jerome Reineix, Fly! Study Manager, and Alessandro Alcibiade, Fly! Flight Surgeon.
Announced in November 2022 during the Ministerial Council held in Paris, France, this unique and groundbreaking study is aimed at understanding and challenging the limitations posed by physical disabilities to human spaceflight. Concluded in late 2024, the Fly! Feasibility Study successfully demonstrated it is technically feasible to fly someone with a physical disability, like John’s, on a six-month mission to the International Space Station as a fully integrated crew member. It underpinned the desire to ensure that space exploration is not limited by physical constraints and that every individual can contribute to our collective understanding of the cosmos and of the benefits of spaceflight for life on Earth.
The end of the feasibility study marks the start of the next phase: Fly! Mission Ready . This is an essential step to carry out the first long-term mission for an astronaut with a physical disability.
Cosmic cloudscape

Earth from Space: Heart of Mount St Helens

Sentinel-1C interferogram of northern Chile
Pierogi space packaging
Biomass standing proud
Meet Biomass

Meet Biomass – ESA’s next Earth Explorer mission to launch. Carrying the first P-band synthetic aperture radar in space, this new mission is set to deliver crucial information about the state of our forests and how they are changing, and to further our knowledge of the role forests play in the carbon cycle.
A lab with a view
Euclid image of a bright Einstein ring around galaxy NGC 6505

Biomass counts biomass

ESA’s Earth Explorer Biomass is the first satellite to carry a P-band synthetic aperture radar in space to measure forest biomass and height, consistently across the globe and across different forest types. Thanks to the long 70 cm wavelength of P-band, the signal can penetrate through the forest canopy, allowing it to collect information on amounts of different parts of the forest, namely, tree trunks, branches and stems – which is where trees store most of their carbon.
Since carbon makes up roughly half the weight of wood, the mission is extremely important in the quest to reduce uncertainties about the role forests play in the global carbon cycle and in our climate system.
Forests in focus

ESA’s Earth Explorer Biomass is the first satellite to carry a P-band synthetic aperture radar in space to measure forest biomass and height, consistently across the globe and across different forest types. Thanks to the long 70 cm wavelength of P-band, the signal can penetrate through the forest canopy, allowing it to collect information on amounts of different parts of the forest, namely, tree trunks, branches and stems – which is where trees store most of their carbon.
Since carbon makes up roughly half the weight of wood, the mission is extremely important in the quest to reduce uncertainties about the role forests play in the global carbon cycle and in our climate system.
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