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Lifting the canopy on Earth’s forests

ESA’s state-of-the-art Biomass mission has been designed to shed new light on the health and dynamics of the world’s forests, revealing how they are changing over time and, critically, enhancing our understanding of their role in the global carbon cycle. It is the first satellite to carry a fully polarimetric P-band synthetic aperture radar for interferometric imaging. Thanks to the long wavelength of P-band, around 70 cm, the radar signal can slice through the forest canopy and whole forest layer to measure the ‘biomass’, meaning the woody trunks, branches and stems, which is where trees store most of their carbon.
Biomass on the launch pad
Biomass in the launch tower
Biomass separates from Vega-C

ESA’s Biomass satellite is launched from Europe’s Spaceport in French Guiana on a Vega-C rocket. The satellite is released into orbit about one hour after liftoff, after which it opens its solar panel.
Once in orbit, this latest Earth Explorer mission will provide vital insights into the health and dynamics of the world’s forests, revealing how they are changing over time and, critically, enhancing our understanding of their role in the global carbon cycle.
Biomass on Vega-C

ESA’s Biomass satellite is launched from Europe’s Spaceport in French Guiana on a Vega-C rocket. The rocket fairing protects the satellite during liftoff but is jettisoned soon after.
Once in orbit, this latest Earth Explorer mission will provide vital insights into the health and dynamics of the world’s forests, revealing how they are changing over time and, critically, enhancing our understanding of their role in the global carbon cycle.
TerraMind, a next-generation AI model

TerraMind is a powerful new AI tool designed to help us better understand and protect our planet. By combining different types of Earth observation data, it can deliver accurate answers to questions about climate and nature. From spotting methane leaks to tracking changes in forests and land use, TerraMind is set to play a key role in tackling some of the current environmental challenges.
Read full story: ESA and IBM collaborate on TerraMind
ACES on its way to space

Today at 10:15 CEST, ESA’s Atomic Clock Ensemble in Space (ACES) began its journey to the International Space Station on a SpaceX Falcon 9 rocket launched from NASA’s Kennedy Space Center in Florida, United States.
ACES carries the most accurate clocks ever flown in space – PHARAO and the Space Hydrogen Maser – designed to keep time so precisely that they would lose just one second every 300 million years. Developed by the French space agency CNES and Safran Timing Technologies in Switzerland, these European-built clocks will work with a sophisticated time transfer time using microwave and laser links to synchronise the best clocks all over Earth.
Later this week, the Station’s Canadian robotic arm will install ACES on the exterior of ESA’s Columbus module. From its vantage point 400 km above Earth, ACES will link its ultra-precise clocks with the best timekeepers on the ground, enabling groundbreaking tests of fundamental physics, including Einstein’s theory of general relativity. Over its 30-month mission, it will carry out extended measurement sessions to investigate the very nature of time and enhance global time synchronisation.
ACES is a fully European mission led by ESA, with Airbus as a prime contractor, and will be operated from control centres in France and Germany (CADMOS and Col-CC).
“The launch of ACES marks a major milestone for European science and international cooperation in space. With this mission, we are placing the most precise timepiece ever sent to orbit aboard the International Space Station — opening new frontiers in fundamental physics, time transfer, and global synchronization. ACES is a shining example of what Europe can achieve when we unite cutting-edge technology, scientific ambition, and strong partnerships”, says Daniel Neuenschwander, Director of Human & Robotic Exploration at ESA.
Would you like to find out more? Here’s seven things you probably didn’t know about ACES.
Hubble spies a cosmic pillar in the Eagle Nebula

ESA School Days 2025 at ESRIN

English
From 7 to 11 April, ESA's Centre for Earth Observation in Frascati, ESRIN, hosted the 2025 edition of ESA School Days, welcoming almost 1400 young students.
The event kicked off with primary school students (4th and 5th grades) visiting during the first three days, followed by secondary school students on the final two days.
Throughout the week, 35 schools from across Italy engaged in presentations and laboratories, delving into the diverse space activities conducted at ESA’s establishment.
This initiative, which included contributions from ESERO Italia and the Italian Space Agency (ASI), aims to inspire and engage the next generation of STEM students by sharing knowledge about space and the European Space Agency.
Italian
Dal 7 all'11 aprile, ESRIN, il Centro per l'Osservazione della Terra dell'ESA a Frascati, ha ospitato l'edizione 2025 degli ESA School Days, accogliendo quasi1 400 giovani studenti. L'evento ha preso il via con la visita degli studenti delle scuole primarie (classi quarte e quinte) durante i primi tre giorni, seguiti dagli studenti delle scuole secondarie nei due giorni finali.
Per tutta la settimana, 35 scuole da tutta Italia si sono cimentate in presentazioni e laboratori, approfondendo la loro conoscenza delle diverse attività spaziali condotte presso lo stabilimento dell'ESA.
L'iniziativa, che ha visto il contributo di ESERO Italia e dell'Agenzia Spaziale Italiana (ASI), mira a ispirare e coinvolgere la prossima generazione di studenti STEM condividendo le conoscenze sullo spazio e sull'Agenzia Spaziale Europea.
The squid and the whale

Earth from Space: Giza, Egypt
Sea surface warming acceleration

Between 1985 and 1989, a warming of 0.06 C in sea surface temperatures per decade was observed, while from 2019 to 2023, the increase was by 0.27 C per decade. The study suggests that sea surface temperatures are rising 4.5 times faster since 2019 than they were at the end of the 1980s.
Weather phenomena can cause short-term fluctuations in sea surface temperatures. El Niño, for example, has a temporary warming effect in certain years because it changes the distribution of heat in the tropics. Large volcanic eruptions – such as Mount Pinatubo in the Philippines in 1991 – release aerosols into the stratosphere, which reflect sunlight and can lead to a temporary cooling of the Earth's surface. However, this effect is short-term and does not significantly interrupt the long-term warming trend.
Read full story: Sea surface warming faster than expected
Explore spiral galaxy M83 through Webb’s infrared eyes

The barred spiral galaxy M83 is revealed in detail by the NASA/ESA/CSA James Webb Space Telescope. M83, which is also known as NGC 5236, was observed by Webb as part of a series of observations collectively titled Feedback in Emerging extrAgalactic Star clusTers, or FEAST.
MIRI, or the Mid-InfraRed Instrument, makes observations in the mid-infrared, which spans wavelengths of light very different from optical wavelengths. Optical wavelengths in astronomy roughly correspond to the range of light waves that human eyes are sensitive to, and extend from about 0.38 to 0.75 micron (a micron, is one thousandth of a millimetre). By contrast, MIRI detects light from 5 to 28 micron — however, when it makes observations, it does not typically observe across this entire wavelength range all at once. Instead, MIRI has a set of ten filters that allow very specific regions of light through. For example, one of MIRI’s filters (dubbed F770W), allows light with wavelengths of 6.581 to 8.687 micron to pass through it.
This image was compiled using data collected through just two of MIRI’s ten filters, near the short end of the instrument’s wavelength range. The result is this extraordinarily detailed image, with its creeping tendrils of gas, dust and stars. In this image, the bright blue shows the distribution of stars across the central part of the galaxy. The bright yellow regions that weave through the spiral arms indicate concentrations of active stellar nurseries, where new stars are forming. The orange-red areas indicate the distribution of a type of carbon-based compound known as polycyclic aromatic hydrocarbons (or PAHs) — the F770W filter, one of the two used here, is particularly suited to imaging these important molecules.
Hubble offers a new view of Sombrero galaxy

Hera's Mars flyby - Asteroid Framing Camera (colourised)

On 12 March 2025, ESA’s Hera spacecraft soared just 5000 km above Mars and passed within 300 km of its distant moon, Deimos. Captured by Hera’s 1020x1020 pixel Asteroid Framing Camera, this video sequence offers a rare view of the red planet and its enigmatic moon. The original greyscale images have been colour-enhanced based on known surface features.
Biomass on its launch adapter
Aleš Svoboda | Supersonic, Space Stuff & STEM | ESA Explores #14

Meet Aleš Svoboda— A skilled pilot with over 1500 flight hours, Aleš holds a PhD in aircraft and rocket technology and has commanded Quick Reaction Alerts. From flying high to training underwater, he’s always ready to take on new challenges—now including astronaut reserve training with ESA.
In this miniseries, we take you on a journey through the ESA Astronaut Reserve, diving into the first part of their Astronaut Reserve Training (ART) at the European Astronaut Centre (EAC) near Cologne, Germany. Our “ARTists” are immersing themselves in everything from ESA and the International Space Station programme to the European space industry and institutions. They’re gaining hands-on experience in technical skills like spacecraft systems and robotics, alongside human behaviour, scientific lessons, scuba diving, and survival training.
ESA’s Astronaut Reserve Training programme is all about building Europe’s next generation of space explorers—preparing them for the opportunities of future missions in Earth orbit and beyond.
This interview was recorded in November 2024.
You can listen to this episode on all major podcast platforms.
Keep exploring with ESA Explores!
Pangea’s methalox aerospike engine – first in the world!

Spanish company Pangea Aerospace developed and tested the first aerospike engine in the world to run on liquid methane and oxygen. This video shows scenes of the engine being tested at the German aerospace center, DLR, test centre in Lampoldshausen Germany in 2021.
Unlike almost all rocket engines in operation, aerospike engines don’t have bell-shaped nozzles but plugs to eject their exhaust. This allows the engine to be more efficient at different altitudes, offering up to 15% more efficiency – and in rocket launches efficiency is everything as you try to escape Earth’s gravity. Aerospike engines have stayed theoretical for decades. Although a few were built in the 1980’s, new 3D-printing techniques have made them more economically viable
These scenes were taken from four test runs with the engine firing for around a minute during each test. Liquid methane and liquid oxygen – often abbreviated to methalox – is cooled down to around –170°C before being mixed and burnt in the engine, where the mixture then heats up to temperatures above 3000°C. To prevent the engine from melting, Pangea Aerospace’s design runs both the cryogenic methane and oxygen fluids around the engine to cool it. The test firing delivered up to 20 kilonewtons of thrust.
This engine development was supported in part by ESA’s Future Launchers Preparatory Programme, and Pangea Aerospace is also working with ESA to identify how to design and build a very high thrust rocket engine for future launchers – offering over 2 meganewtons of thrust.
Spectrum first flight

European commercial rocket Spectrum, developed and operated by Isar Aerospace, took flight from Andøya Spaceport in Norway on 30 March 2025 and flew for 30 seconds, clearing the launch pad and proving the launch vehicle could achieve one of the hardest parts of space transportation: liftoff.
Isar Aerospace’s two-stage launch vehicle Spectrum is 28 m tall, 2 m in diameter and, with its ten engines, it is targeting to launch payloads of up to 1000 kg to low Earth orbit.
The flight allows Isar Aerospace engineers to analyse all the data they need to tweak their Spectrum launcher for a next flight. “Our first test flight met all our expectations, achieving a great success”, said Isar Aerospace CEO Daniel Metzler, “We had a clean liftoff, 30 seconds of flight and even got to validate our flight termination System.”
Isar Aerospace is a German-based company, building their Spectrum launch vehicle in state-of-the-art production facilities relying on in-house manufacturing.
Initially supported by ESA’s Business Incubation Centre, the company is supported by three rounds of co-funding from ESA so far, as part of the Boost! programme that helps commercial initiatives offering transportation services to space, in space, and returning from space. ESA's support will follow steps preparing the second test flight of the Spectrum rocket and scaling-up of production facilities at the company’s new headquarters in Vaterstetten, Germany.
Exciting news from Paxi!

Paxi has some news to share!
Amelie Schoenenwald | Science, Exploration, Training | ESA Explores #13

Meet Amelie Schoenenwald— biotechnologist, business expert, and PhD in structural biology. Whether in the lab or the great outdoors, she thrives in extreme environments, ready to embrace the adventure of ESA’s Astronaut Reserve.
In this miniseries, we take you on a journey through the ESA Astronaut Reserve, diving into the first part of their Astronaut Reserve Training (ART) at the European Astronaut Centre (EAC) near Cologne, Germany. Our “ARTists” are immersing themselves in everything from ESA and the International Space Station programme to the European space industry and institutions. They’re gaining hands-on experience in technical skills like spacecraft systems and robotics, alongside human behaviour, scientific lessons, scuba diving, and survival training.
ESA’s Astronaut Reserve Training programme is all about building Europe’s next generation of space explorers—preparing them for the opportunities of future missions in Earth orbit and beyond.
This interview was recorded in November 2024.
Learn more about Amelie’s favourite space mission.
You can listen to this episode on all major podcast platforms.
Keep exploring with ESA Explores!
Strong gravitational lenses captured by Euclid

Euclid Deep Field North – preview

Euclid’s view of the Cat’s Eye Nebula

Location of Euclid Deep Fields on Gaia and Planck sky map

Euclid Deep Field South, 70x zoom

Galaxies in different shapes captured by Euclid

Euclid Deep Field Fornax – preview

Euclid Deep Field South – preview

Euclid Deep Field South, 16x zoom

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