Meet Esther, our System Engineer currently working on the Proba-3 mission.
Proba-3 is scheduled to liftoff on Wednesday, 4 December, at 11:38 CET from the Satish Dhawan Space Centre in India, Proba-3 will use two satellites to create the perfect conditions for observing the Sun’s corona.
One satellite features a telescope, kept in the centre of the shadow cast by the other satellite around 150 m away, thanks to an occulter disc. Maintaining the correct position in the shadow requires a precise formation flying capability, down to a single millimetre of precision.
The double-satellite Proba-3 is the most ambitious member yet of ESA’s Proba family of experimental missions. Two spacecraft will fly together as one, maintaining precise formation down to a single millimetre. One will block out the fiery disc of the Sun for the other, to enable prolonged observations of the Sun’s surrounding atmosphere, or ‘corona’, the source of the solar wind and space weather. Usually, the corona can only be glimpsed for a few minutes during terrestrial total solar eclipses.
Proba-3 aims to reproduce such eclipses for up to six hours at a time, in a highly elliptical orbit taking it more than 60 000 km from Earth. The two spacecraft are being launched together by India’s PSLV-XL launcher from the Satish Dhawan Space Centre.
Radar allows us to see through what would otherwise be invisible. By sending out radio waves that bounce off objects and return as echoes, radar creates a detailed picture of our surrounding world.
This technology is everywhere: from guiding air traffic and enabling self-driving cars to tracking the movements of athletes. But its reach doesn’t stop there—radar is also transforming how we observe our Earth from space.
Satellites like the Copernicus Sentinel-1 mission use radar to see through clouds, darkness and any weather conditions. This capability is invaluable for detecting subtle changes on Earth’s surface—changes that are often hidden from the human eye. Discover how radar technology is helping us unlock these hidden insights about our planet.
Credit: ESA – European Space Agency
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
Thanks to the incredible precision of our Gaia mission, scientists have discovered potential moons orbiting over 350 asteroids! This nearly doubles the known number of ‘binary asteroids,’ revealing a whole new layer of complexity in our Solar System.
Meet Copernicus Sentinel-1 – this ground-breaking mission delivers continuous, all-weather, day-and-night imaging for land, ice and maritime monitoring.
Equipped with state-of-the-art C-band synthetic aperture radar (SAR), Sentinel-1 captures high-resolution data around the clock, in any weather, making it indispensable for detecting the subtle changes on Earth’s surface that remain hidden from the human eye.
Sentinel-1 data serves a multitude of critical applications: from ensuring the safety and efficiency of maritime traffic, tracking sea ice and icebergs, to monitoring structural integrity and natural hazards, such as earthquakes, landslides and volcanic activity.
Its enhanced radar technology provides precises precise information on ground movement, which is critical for urban planning, infrastructure resilience, subsidence risk assessment and geohazard monitoring.
Through consistent, long-term data collection, Sentinel-1 serves as a global asset, essential for environmental and safety monitoring worldwide. The mission is a beacon of innovation, advancing our understanding of our planet’s dynamic landscape.
This video features interviews with Mark Drinkwater, Head of Mission Sciences Division at ESA, Ramon Torres Cuesta, Sentinel-1 Project Manager at ESA and Julia Kubanek, Sentinel-1 Mission Scientist at ESA.
Credit: ESA – European Space Agency
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
Join us on a unique video tour of the Sun’s mesmerising surface. Thanks to its innovative instrumentation and a ‘daring’ trajectory passing close to the Sun, ESA’s Solar Orbiter spacecraft has obtained the highest-resolution full views of the Sun’s surface to date.
Watching the Sun in visible light, Solar Orbiter reveals a grainy surface and dark sunspots. On the same day, the spacecraft mapped the Sun’s magnetic field, tracked how fast and in which direction scorching hot material on the surface is moving, and snapped a hypnotising image in ultraviolet light of the Sun’s upper atmosphere, the corona. All taken on the same day, the four new images shown in this video let us peel away the Sun’s many layers.
The images were taken when Solar Orbiter was less than 74 million kilometres from the Sun; being so close meant each high-resolution image only covers a small portion of the Sun. To obtain the full-disc views showcased in the video, 25 images were stitched together like a mosaic. The Sun has a diameter of around 8000 pixels in the full mosaics, revealing an extraordinary amount of detail.
Credit: ESA – European Space Agency Acknowledgements: Sun images: ESA & NASA/Solar Orbiter/PHI and EUI Teams; Solar Orbiter spacecraft animation: ESA/ATG medialab; Voiceover: Juliet Hannay
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
This video takes the viewer on a journey that zooms through space to reveal the Tarantula Nebula.
Thousands of never-before-seen young stars are spotted in the stellar nursery called 30 Doradus, captured by the NASA/ESA/CSA James Webb Space Telescope. It is nicknamed the Tarantula Nebula for the appearance of its dusty filaments in previous telescope images, the nebula has long been a favourite for astronomers studying star formation. In addition to young stars, Webb reveals distant background galaxies, as well as the detailed structure and composition of the nebula’s gas and dust.
Credit: NASA, ESA, CSA, STScI, ESO, E. Slawik, N. Risinger, D. De Martin, D. Lennon, E. Sabbi, N. Bartmann, M. Zamani Music: tonelabs – Happy Hubble
Smile is the Solar wind Magnetosphere Ionosphere Link Explorer, a brand-new space mission currently in the making. It will study space weather and the interaction between the solar wind and Earth’s environment.
Unique about Smile is that it will take the first X-ray images and videos of the solar wind slamming into Earth’s protective magnetic bubble, and its complementary ultraviolet images will provide the longest-ever continuous look at the northern lights.
In this first of several short videos, David Agnolon (Smile Project Manager) and Philippe Escoubet (Smile Project Scientist) talk about the why and the how of Smile. You’ll see scenes of the building and testing of the spacecraft’s payload module by Airbus in Madrid, including the installation of one of the European instruments, the Soft X-ray Imager from the University of Leicester.
Smile is a 50–50 collaboration between the European Space Agency (ESA) and the Chinese Academy of Sciences (CAS). ESA provides the payload module of the spacecraft, which carries three of the four science instruments, and the Vega-C rocket which will launch Smile to space. CAS provides the platform module hosting the fourth science instrument, as well as the service and propulsion modules.
Credit: ESA/Lightcurve Films
Acknowledgements: Direction, main camera, sound, editing, post-production by Lightcurve Films. Original music by William Zeitler. Artwork shown in the video is by Eryka Isaak and CAS.
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
On 12 November 2024, Mars kicks off a fresh New Year! While Earth and Mars both orbit the Sun, a Martian year is full of fascinating twists. Curious about how time flows differently on the Red Planet? Let’s dive into what makes a year on Mars unique—and what it shares with our own!
📹 ESA – European Space Agency 📸 ESA/DLR/Freie Universität Berlin
On 12 November 2014, after a ten-year journey through the Solar System and over 500 million kilometres from home, Rosetta’s lander Philae made space exploration history by touching down on a comet for the first time. On the occasion of the tenth anniversary of this extraordinary feat, we celebrate by taking a look back over the mission’s highlights.
Rosetta was an ESA mission with contributions from its Member States and NASA. It studied Comet 67P/Churyumov-Gerasimenko for over two years, including delivering lander Philae to the comet’s surface. Philae was provided by a consortium led by DLR, MPS, CNES and ASI.
Credits: ESA – European Space Agency
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
1️⃣ Space near Mercury is HOT. Sending a spacecraft there is a bit like asking a laptop to work inside a hot pizza oven! Some spacecraft have gotten close to Mercury but none have remained in this scorching heat continuously. This means we still don’t have high-resolution data covering Mercury’s entire surface.
2️⃣ It’s difficult to observe from Earth: Because Mercury is very close to the Sun, when we try to look at it from Earth, it’s often lost in the Sun’s glare.
3️⃣ It’s hard to reach: Mercury is not that far, but according to some estimates, it would take less energy to get to Pluto than to get to Mercury. The Sun’s strong gravitational pull means that spacecraft need to use a lot of energy to slow down enough to orbit Mercury.
But our BepiColombo mission, will help us learn a lot more about Mercury when it enters into orbit in 2026! It’s the most advanced spacecraft ever sent to Mercury. It will help us answer many questions, such as: Why is there ice in the polar craters of the scorched planet? And what are the mysterious ‘hollows’ on its surface?
In this mosaic image stretching 340 light-years across, Webb’s Near-Infrared Camera (NIRCam) displays the Tarantula Nebula star-forming region in a new light, including tens of thousands of never-before-seen young stars that were previously shrouded in cosmic dust. The most active region appears to sparkle with massive young stars, appearing pale blue. Scattered among them are still-embedded stars, appearing red, yet to emerge from the dusty cocoon of the nebula. NIRCam is able to detect these dust-enshrouded stars thanks to its unprecedented resolution at near-infrared wavelengths.
📹 ESA – European Space Agency 📸 NASA, ESA, CSA, and STScI, N. Bartmann 🎶 Haunted House – Goosebumps
In mythology, centaurs are half-human, half-horse creatures, but in space, they’re celestial objects orbiting the Sun between Jupiter and Neptune.
Centaurs are “hybrid” objects in the sense that they share characteristics with trans-Neptunian objects from the Kuiper Belt reservoir and short-period comets. A team of scientists used the James Web Telescope to study Centaur 29P.
While data from previous observations of Centaur 29P showed a carbon monoxide (CO) gas jet pointed toward Earth, Webb parsed the jet’s composition in greater detail, and also detected multiple never-before-seen features of the centaur: two jets of carbon dioxide (CO2) emanating in the north and south directions, and another jet of CO pointing toward the north.
Centaur 29P’s different CO and CO2 abundances suggest that the body may be composed of different pieces that coalesced together during its formation. However, other scenarios to explain Centaur 29P’s outgassing activity are still being considered.
In 2022 NASA’s DART spacecraft made history, and changed the Solar System forever, by impacting the Dimorphos asteroid and measurably shifting its orbit around the larger Didymos asteroid. In the process a plume of debris was thrown out into space.
The latest modelling, available on the preprint server arXiv and accepted for publication in the September volume of The Planetary Science Journal, shows how small meteoroids from that debris could eventually reach both Mars and Earth – potentially in an observable (although quite safe) manner.
Aurelia works on VR experiences that recreate locations in space.
Sometimes, her work takes her beyond the office. Recently, Aurelia attended Gamescom , the world’s biggest video game event, where her team showcased MUSE, a VR project she helped design!
Fast’ solar wind moves with speeds above 500 km/s. Curiously, this wind exits the Sun’s corona with lower speeds, so something speeds it up as it moves farther away. The million-degree wind naturally cools down as it expands into a larger volume and becomes less dense, much like the air on Earth as you climb a mountain. And yet, it cools more slowly than expected from this effect alone.
So, what provides the necessary energy to accelerate and heat the fastest parts of the solar wind?
Data from our Solar Orbiter and NASA’s Parker Solar Probe have provided conclusive evidence that the answer is large-scale oscillations in the Sun’s magnetic field, known as Alfvén waves.
Data collected using the NASA/ESA/CSA James Webb Space Telescope, combined with earlier observations from the NASA/ESA Hubble Space Telescope, show surprisingly little methane (CH4) in the atmosphere of WASP-107 b, indicating that the interior of the planet must be significantly hotter and the core much more massive than previously estimated.
📹 ESA – European Space Agency 📸 NASA, ESA, CSA, R. Crawford
In 2013, our Herschel telescope solved the mystery of water in Jupiter’s upper atmosphere, tracing it back to the impact of comet Shoemaker-Levy 9 in July 1994.
This finding paved the way for our Juice mission, set to reach Jupiter in 2031. Juice’s observations will give us a better chance of understanding how Jupiter’s atmosphere responds to such events.
ESA’s Hera mission lifted off on a SpaceX Falcon 9 from Cape Canaveral Space Force Station in Florida, USA, on 7 October at 10:52 local time (16:52 CEST, 14:52 UTC).
Hera is ESA’s first planetary defence mission. It will fly to a unique target among the 1.3 million asteroids in our Solar System – the only body to have had its orbit shifted by human action – to solve lingering unknowns associated with its deflection.
Hera will carry out the first detailed survey of a ‘binary’ – or double-body – asteroid, 65803 Didymos, which is orbited by a smaller body, Dimorphos. Hera’s main focus will be Dimorphos, whose orbit around the main body was previously altered by NASA’s kinetic-impacting DART spacecraft.
By sharpening scientific understanding of this ‘kinetic impact’ technique of asteroid deflection, Hera should turn the experiment into a well-understood and repeatable technique for protecting Earth from an asteroid on a collision course.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
ESA’s Hera mission lifted off on a SpaceX Falcon 9 from Cape Canaveral Space Force Station in Florida, USA, on 7 October at 10:52 local time (16:52 CEST, 14:52 UTC).
Hera is ESA’s first planetary defence mission. It will fly to a unique target among the 1.3 million asteroids in our Solar System – the only body to have had its orbit shifted by human action – to solve lingering unknowns associated with its deflection.
Hera will carry out the first detailed survey of a ‘binary’ – or double-body – asteroid, 65803 Didymos, which is orbited by a smaller body, Dimorphos. Hera’s main focus will be Dimorphos, whose orbit around the main body was previously altered by NASA’s kinetic-impacting DART spacecraft.
By sharpening scientific understanding of this ‘kinetic impact’ technique of asteroid deflection, Hera should turn the experiment into a well-understood and repeatable technique for protecting Earth from an asteroid on a collision course.
————————————————— 📸 ESA – S. Corvaja Copyright: ESA/SpaceX —————————————————
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
Hera, ESA’s first planetary defence mission, is headed to space.
Hera will fly to a unique target among the 1.3 million known asteroids of our Solar System – the first body to have had its orbit shifted by human action – to probe lingering unknowns related to its deflection.
————————————————— Credits: ESA/SpaceX ————————————————— Chapters: 00:00 Start of ESA WebTV programme – live from ESA’s European Space Operations Centre in Darmstadt, Germany 18:30 SpaceX live broadcast begins 36:15 Hera lift-off 1:53:00 – Hera separates from Falcon 9 launcher: End of SpaceX live broadcast, ESA WebTV programme continues 1:57:20 Acquisition of the first signals from the Hera spacecraft 2:13:26 End of ESA WebTV programme
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
Hera, ESA’s first planetary defence mission, is headed to space.
Hera will fly to a unique target among the 1.3 million known asteroids of our Solar System – the first body to have had its orbit shifted by human action – to probe lingering unknowns related to its deflection.
Hera is scheduled for launch on a SpaceX Falcon 9 rocket from Cape Canaveral Space Force Station in Florida, USA, today, Monday 7 October, at 16:52 CEST / 15:52 BST.
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Credits: ESA – European Space Agency
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Chapters: 00:00 What is Hera? 01:07 Why do we need to protect our planet? 02:22 How did we pick this asteroid to explore? 03:36 What are we expecting to see on Dimorphos? 05:56 How do we get there? 07:48 What type of technology do we need to inspect an asteroid? 10:49 Conclusion
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
Live interviews and highlights from the ESA Open Day at ESTEC, featuring ESA astronauts Andreas Mogensen and André Kuipers, NASA astronaut Anna Fisher, The Expanse actor Steven Strait and more.
The ESA Open Day is an annual event where ESA opens the doors of the European Space Research and Technology Centre in the Netherlands to the public.
We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
This tiny satellite will study the surface of the asteroid Dimorphos up close, helping us learn more about asteroid deflection and space safety. With groundbreaking sensors and instruments, Milani is ready to explore this binary asteroid system alongside Hera and Juventas
Stay tuned for more on Hera’s thrilling mission!
📹 ESA – European Space Agency 📸 ESA/Science Office
Meet Ian Carnelli, project manager for Hera, our planetary defense mission that will very soon be launched into space.
Hera will be, along with NASA’s DART spacecraft, humankind’s first probe to rendezvous with a binary asteroid system, a little understood class making up around 15% of all known asteroids.
A shoebox-sized spacecraft from our Hera mission that’s about to explore the binary asteroid system of Didymos and its moon, Dimorphos – a space rock the size of the Great Pyramid!
Using its cutting-edge radar system, Juventas will reveal whether Dimorphos is a solid monolith or simply a loose pile of rubble. Plus, it’s going to gently land and measure the asteroid’s gravity—something never done before!
This tiny spacecraft is set to rewrite what we know about asteroids and could one day help protect our planet.
Stay tuned for more on Hera’s thrilling mission!
📸 ESA – European Space Agency 📹 ESA/Science Office
ESA’s Jupiter Icy Moons Explorer (Juice), is on an epic eight-year journey to Jupiter. This first episode of ‘The journey of Juice’ tells the story of Juice’s first months in space, from its launch on 14 April 2023 to its lunar-Earth gravity assist (LEGA for short) in August 2024. This flyby was not only the first double gravity assist manoeuvre of its kind, it was also a perfect opportunity to test out the spacecraft’s cameras and science instruments.
In this episode, Juice’s Mission Manager Nicolas Altobelli explains how the spacecraft will become the first ever human-made machine to orbit a moon of another planet, in this case Jupiter’s largest moon Ganymede.
You’ll also hear from Claire Vallat and Marc Costa at the European Space Astronomy Centre (ESAC) near Madrid, Spain. Juice will perform incredibly complex measurements once it reaches Jupiter, and the Science Operations team at ESAC is making sure we get the most out of every instrument.
Meanwhile, the Flight Control team at the European Space Operations Centre (ESOC) in Darmstadt, Germany, makes sure Juice is and stays on the right path. This episode shows what happened ‘behind the scenes’ before and during the lunar-Earth flyby, and stars Ignacio Tanco, Angela Dietz and members of the Juice Flight Control team as they do what they do best.
Finally, we highlight the ESA tracking station network (Estrack), another crucial component for Juice. Maintenance and Operations Engineer Belén Goméz gives a tour of the facility at Cebreros.
Following the very successful lunar-Earth flyby, Juice is now on its way to planet Venus for its next flyby. On 31 August 2025, this flyby will give Juice its second gravity boost. Tune back in next year for episode two of this series!
This series follows on from ‘The making of Juice’ series, which covered the planning, testing and launch of this once-in-a-generation mission.
Credit: ESA/Lightcurve Films, original music by William Zeitler
Acknowledgments: Direction, main camera, sound, editing, post-production: Maarten Roos. Camera at Cebreros during LEGA: Mikel Larequi. LEGA timelapse: Mark McCaughrean and Simeon Schmauß. Special thanks to Marc Costa (ESA – ESAC) and Jorge Fauste (ESA – Estrack)
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
Our Hera spacecraft will soon start its journey to the distant asteroid moon Dimorphos orbiting around its parent body Didymos.
One of the first features Hera will look for is the crater left on Dimorphos by its predecessor mission DART, which impacted the asteroid to deflect its orbit.
Yet, more recent impact simulations suggest no crater will be found. The DART impact is likely to have remodelled the entire body instead – a significant finding for both asteroid science and planetary defence.
Meet Codi, the cutting-edge rover being tested in the UK as it gears up for future Mars missions! This high-tech explorer navigates challenging landscapes and collects “lightsabre” samples with precision. And did you know? There’s a bit of fun on the side—Kevin the piglet, the team’s adorable mascot, is named after actor Kevin Bacon!
In this last episode of the Young Professional Satellite docu series, we follow the team’s last steps to make their dream come true: sending their satellite to space.
After securing the crucial final assembly and battery connection, we take you inside the thermal vacuum tests (TVAC) to see how YPSat is tested under the extreme temperatures of space; through vibration tests to ensure its structural integrity during launch; and electromagnetic compatibility (EMC) tests to prevent interference with the launcher’s systems.
As we approach the European Space Agency’s traditional Flight Acceptance Review, the satellite is officially certified for flight. With the integration complete and final battery charge applied, control is handed over to the rocket. The only task left for the teams on the ground is to analyse one last time the rocket’s trajectory and await the critical first signal.
As tension builds up on launch day, watch as the team retrieves YPSat’s data and decodes breathtaking images and videos from its mission.
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Credits: Directed and produced by Chilled Winston: https://chilledwinston.com/ and Emma de Cocker Powered by ESA – European Space Agency Soundtracks from Epidemic Sound
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Chapters: 00:00 – Introduction 01:30 – Final Assembly 02:49 – The Test Campaign 06:42 – Final Launch Preparations 10:01 – Ariane 6 Launch 11:38 – Gathering & Decoding the Footage 15:15 – Unveiling the Footage 17:08 – Watch at the End
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
The third Copernicus Sentinel-2 satellite, Sentinel-2C, has launched aboard the last Vega rocket, flight VV24, from Europe’s Spaceport in French Guiana. The rocket lifted off on 5 September at 03:50 CEST (4 September 22:50 local time).
Sentinel-2C was the last liftoff for the Vega rocket – after 12 years of service this was the final flight, the original Vega is being retired to make way for an upgraded Vega-C.
🎥 ESA – European Space Agency Credits: ESA/CNES/Arianespace
Watch the closest flyby of a planet ever, as the ESA/JAXA BepiColombo spacecraft sped past Mercury during its latest encounter on 4 September 2024.
This flyby marked BepiColombo’s closest approach to Mercury yet, and for the first time, the spacecraft had a clear view of Mercury’s south pole.
This timelapse is made up of 128 different images captured by all three of BepiColombo’s monitoring cameras, M-CAM 1, 2 and 3. We see the planet move in and out of the fields of view of M-CAM 2 and 3, before M-CAM 1 sees the planet receding into the distance at the end of the video. The first few images are taken in the days and weeks before the flyby. Mercury first appears in an image taken at 23:50 CEST (21:50 UTC) on 4 September, at a distance of 191 km. Closest approach was at 23:48 CEST at a distance of 165 km.
The sequence ends around 24 hours later, on 5 September 2024, when BepiColombo was about 243 000 km from Mercury.
During the flyby it was possible to identify various geological features that BepiColombo will study in more detail once in orbit around the planet. Four minutes after closest approach, a large ‘peak ring basin’ called Vivaldi came into view.
This crater was named after the famous Italian composer Antonio Vivaldi (1678–1741). The flyover of Vivaldi crater was the inspiration for using Antonio Vivaldi’s ‘Four Seasons’ as the soundtrack for this timelapse.
Peak ring basins are mysterious craters created by powerful asteroid or comet impacts, so-called because of the inner ring of peaks on an otherwise flattish floor.
A couple of minutes later, another peak ring basin came into view: newly named Stoddart. The name was recently assigned following a request from the M-CAM team, who realised that this crater would be visible in these images and decided it would be worth naming considering its potential interest for scientists in the future.
BepiColombo’s three monitoring cameras provided 1024 x 1024 pixel snapshots. Their main purpose is to monitor the spacecraft’s various booms and antennas, hence why we see parts of the spacecraft in the foreground. The photos that they capture of Mercury during the flybys are a bonus.
The 4 September gravity assist flyby was the fourth at Mercury and the seventh of nine planetary flybys overall. During its eight-year cruise to the smallest and innermost planet of the Solar System, BepiColombo makes one flyby at Earth, two at Venus and six at Mercury, to help steer itself on course for entering orbit around Mercury in 2026.
BepiColombo is an international collaboration between ESA and JAXA.
Processing notes: The BepiColombo monitoring cameras provide 1024 x 1024 pixel images. These raw images have been lightly processed. The M-CAM 1 images have been cropped to 995 x 995 pixels.
Credits: ESA/BepiColombo/MTM Acknowledgements: Image processing and video production by Mark McCaughrean
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
Watch the second episode of the ExoMars Rosalind Franklin rover mission – Europe’s ambitious exploration journey to search for past and present signs of life on Mars.
This episode starts with Rosalind searching for traces of life below the martian surface using a ground penetrating radar and a set of cameras.
The rover will dig, collect, and investigate the chemical composition of material collected by a drill. 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 surface radiation and extreme temperatures.
Rosalind Franklin uses the WISDOM radar to help scientists on Earth decide where to drill. Besides identifying the most promising targets for sampling, WISDOM will help the rover avoid potential hazards, such as the presence of buried rocks that could damage the drill. The scientific eyes of the rover are set on the Panoramic Camera suite known as PanCam. The Close-UP Imager (CLUPI) sits on the side of the drill box, a camera designed to acquire high-resolution, colour, close-up images of outcrops, rocks and soils. PanCam and CLUPI will help scientists find the most promising spots to drill. These instruments can also investigate very fine outcrop details and image drill samples before they are sent into the rover’s laboratory. After the rover retracts its drill, the sample is in a special chamber at the tip. Under the reduced martian gravity (38% of Earth’s), the material drops onto a special “hand” that the rover can extend to the front to collect drill samples. The mission will serve to demonstrate key technologies that Europe needs to master for future planetary exploration missions.
The ExoMars rover series show the rover and martian landscapes as true to reality as possible for a simulation.
Check ESA’s ExoMars website and our frequently asked questions for the latest updates.
Credits: ESA – European Space Production: Mlabspace for ESA 3D animation: ESA/Mlabspace Video footage: ESA/NASA, Shutterstock Music composed by Valentin Joudrier
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
On 26 September 2022, NASA’s approximately half-tonne Double Asteroid Redirect Test (DART) spacecraft impacted the Dimorphos asteroid at an approximate speed of 6.1 km/s, shortening its orbit around Didymos by more than half an hour.
Our Hera spacecraft will be launched this October to reach Dimorphos and perform a close-up ‘crash scene investigation’, gathering data on the asteroid’s mass, structure and make-up to turn this kinetic impact method of planetary defence into a well understood and repeatable technique.
Today, Salsa, the first of four satellites that make up our Cluster mission, will reenter Earth’s atmosphere over the South Pacific Ocean Uninhabited Area.
This marks the end of the historic mission, over 24 years after it was sent into space to measure Earth’s magnetic environment. Though the remaining three satellites will also stop making scientific observations, discoveries using existing mission data are expected for years to come.
This ‘targeted reentry’ is the first of its kind. ESA’s efforts to ensure a clean end to the Cluster mission go beyond international standards, making the agency a world-leader in sustainable space exploration.
The first of four satellites that make up ESA’s Cluster mission is coming safely back down to Earth, marking a brilliant end to this remarkable mission.
The satellite’s orbit was tweaked back in January to target a region as far as possible from populated regions. This ensures that any spacecraft parts that survive the reentry will fall over open ocean.
During 24 years in space, Cluster has sent back precious data on how the Sun interacts with Earth’s magnetic field, helping us better understand and forecast potentially dangerous space weather.
With this first ever targeted reentry, Cluster goes down in history for a different reason, taking ESA well beyond international space safety standards and helping ensure the long-term sustainability of space activities.
Credits: ESA – European Space Agency
Chapters: 00:00 Introduction to the Cluster Mission 02:17 How do we deorbit a satellite? 05:05 Why does Cluster’s reentry matter so much? 06:15 Conclusion
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
The Copernicus Sentinel-2C satellite lifted off on 5 September at 03:50 CEST (4 September 22:50 local time) aboard the last Vega rocket, flight VV24, from Europe’s Spaceport in French Guiana.
Sentinel-2C will continue the legacy of delivering high-resolution data that are essential to Copernicus – the Earth observation component of the EU Space Programme. Developed, built and operated by ESA, the Copernicus Sentinel-2 mission provides high-resolution optical imagery for a wide range of applications including land, water and atmospheric monitoring.
Sentinel-2C was the last liftoff for the Vega rocket – after 12 years of service this was the final flight, the original Vega is being retired to make way for an upgraded Vega-C.
Credits: ESA/CNES/Arianespace
Chapters: 00:00 Waiting for liftoff 01:10 Liftoff 04:25 Second stage separation 06:18 Sentinel-2C separation 06:46 Acquisition of signal 07:23 Statements
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We are Europe’s gateway to space. Our mission is to shape the development of Europe’s space capability and ensure that investment in space continues to deliver benefits to the citizens of Europe and the world. Check out https://www.esa.int/ to get up to speed on everything space related.
