ESA Top Multimedia
Star-forming region IC 348 (NIRCam image)
Star-forming region IC 348 (NIRCam image)Webb reveals stunning panorama of star formation
This video takes the viewer on a journey through space to a starry view of the nearby star-forming region IC 348. This one of the largest images from the NASA/ESA/CSA James Webb Space Telescope released to the public so far. Using Webb, astronomers searched IC 348 for brown dwarfs, which are less massive than the smallest stars. The researchers discovered brown dwarfs just twice the mass of Jupiter, bringing the study of these curious objects into a new mass range.
Learn more about this image here.
Read the article Webb reveals stunning panorama of star formation
Rendezvous tests in ESA's robotics lab
The video shows a rendezvous test performed at ESA’s Guidance, Navigation and Control Laboratory using GRALS, the lab’s duo of robotic arms mounted on 33-m long rails. One arm holds the navigation unit of an approaching spacecraft, the other holds a scale model of a spacecraft target or ‘client’. Both are suspended in the centre of a long dark room with only one lamp illuminating the scene, mimicking the Sun.
The European Space Agency (ESA) and industry are working together to develop and test interfaces that will allow satellites to approach in space, recognise each other and dock. The first hardware tests for this step took place at ESA’s testing facilities at ESTEC, the agency’s technical centre in the Netherlands, evaluating different interfaces and technologies developed by The Exploration Company with Sener, GMV, Almatech and CDS.
FLEX and Sentinel-3C launch highlights
ESA’s state-of-the-art FLEX Earth Explorer satellite and the Copernicus Sentinel-3C satellite have been launched together aboard a Vega-C rocket from Europe’s Spaceport in French Guiana, marking a new milestone in Europe’s Earth Observation Programmes. Flight VV30 lifted off on 15 September at 03:21 (14 September at 22:21 local time).
FLEX is designed to reveal a phenomenon invisible to the human eye: the faint fluorescence emitted by plants as they photosynthesise. Equipped with a Fluorescence Imaging Spectrometer, FLEX will detect and measure this incredibly weak signal from orbit. Because the fluorescence varies with plant health and environmental conditions, the measurements will provide scientists with new information about photosynthetic activity and vegetation stress on a global scale.
Sentinel-3C is the third in the Sentinel-3 series. Carrying a suite of cutting-edge instruments, Copernicus Sentinel-3C will continue the mission’s task of measuring systematically Earth’s oceans, land, ice and atmosphere to monitor and understand large-scale global dynamics. The mission also provides essential information in near-real time for ocean and weather forecasting.
Europe’s Vega-C rocket can launch 2300 kg into space, such as small scientific and Earth observation spacecraft. At 35 m tall, Vega-C weighs 210 tonnes on the launch pad and reaches orbit with three solid-propellant-powered stages before the fourth liquid-propellant stage takes over for precise placement of satellites into their desired orbit around Earth. This flight was a first dual launch for Vega-C, using a secondary payload adapter called Vespa. Sentinel-3C was placed on top of Vespa inside the main fairing and once deployed the Vespa adapter opened to reveal FLEX for its injection into orbit.
Relive the launch of FLEX and Sentinel-3C
Watch the full replay of the launch of ESA’s state-of-the-art FLEX Earth Explorer satellite and the Copernicus Sentinel-3C satellite. Both were launched together aboard a Vega-C rocket from Europe’s Spaceport in French Guiana, marking a new milestone in Europe’s Earth Observation Programmes. Flight VV30 lifted off on 15 September at 03:21 (14 September at 22:21 local time).
FLEX is designed to reveal a phenomenon invisible to the human eye: the faint fluorescence emitted by plants as they photosynthesise. Equipped with a Fluorescence Imaging Spectrometer, FLEX will detect and measure this incredibly weak signal from orbit. Because the fluorescence varies with plant health and environmental conditions, the measurements will provide scientists with new information about photosynthetic activity and vegetation stress on a global scale.
Sentinel-3C is the third in the Sentinel-3 series. Carrying a suite of cutting-edge instruments, Copernicus Sentinel-3C will continue the mission’s task of measuring systematically Earth’s oceans, land, ice and atmosphere to monitor and understand large-scale global dynamics. The mission also provides essential information in near-real time for ocean and weather forecasting.
Europe’s Vega-C rocket can launch 2300 kg into space, such as small scientific and Earth observation spacecraft. At 35 m tall, Vega-C weighs 210 tonnes on the launch pad and reaches orbit with three solid-propellant-powered stages before the fourth liquid-propellant stage takes over for precise placement of satellites into their desired orbit around Earth. This flight was a first dual launch for Vega-C, using a secondary payload adapter called Vespa. Sentinel-3C was placed on top of Vespa inside the main fairing and once deployed the Vespa adapter opened to reveal FLEX for its injection into orbit.
FLEX and Sentinel-3C lofted into orbit
Vega-C gantry rolls back for FLEX and Sentinel-3C launch
Main Control Room at ESA's ESOC
Main Control Room at ESA's ESOCSentinel-3C and FLEX separate from Vega-C
The Earth Explorer FLEX satellite and the Copernicus Sentinel-3C satellite are launched together aboard a Vega-C rocket from Europe’s Spaceport in French Guiana.
A new launch adapter called Vespa allows both satellites to be stacked inside the Vega-C fairing for launch. Positioned on top of Vespa, Sentinel-3C is injected into orbit first, followed by FLEX approximately one hour later.
The animation shows the separation of the Sentinel-3C and FLEX satellites from the fairing and their solar panel deployments.
FLEX is designed to reveal a phenomenon invisible to the human eye: the faint fluorescence emitted by plants as they photosynthesise. Equipped with a Fluorescence Imaging Spectrometer, FLEX will detect and measure this incredibly weak signal from orbit. Because the fluorescence varies with plant health and environmental conditions, the measurements will provide scientists with new information about photosynthetic activity and vegetation stress on a global scale.
Sentinel-3C is the third satellite in the Copernicus Sentinel-3 series. Like its two older siblings in orbit, Sentinel-3C carries a suite of cutting-edge instruments that measure systematically Earth’s oceans, land, ice and atmosphere to monitor and understand large-scale global dynamics. It provides essential information in near-real time for ocean and weather forecasting.
Europe’s Vega-C rocket is an evolution of the Vega family, offering increased performance, greater payload capacity and improved competitiveness. With the capability to carry up to 3300 kg into orbit, Vega-C is well suited to launching scientific and Earth observation satellites into space.
Docking tests in ESA's robotics lab
In a docking test at ESA's Orbital Robotic Laboratory, a servicer and client spacecraft models are each attached to one platform hovering over an extremely flat and smooth floor.
Starting at four centimetres apart, the servicer’s docking mechanism first locks onto the client’s passive capture interface and then brings the two platforms closer and closer together until two ports – one for refilling and the other for power and data transfer – connect to their counterparts.
The European Space Agency (ESA) and industry are working together to develop and test interfaces that will allow satellites to approach in space, recognise each other and dock. The first hardware tests for this step took place at ESA’s testing facilities at ESTEC, the agency’s technical centre in the Netherlands, evaluating different interfaces and technologies developed by The Exploration Company with Sener, GMV, Almatech and CDS.
Meet our Hera Space Companion
Meet a key member of our Hera asteroid mission team: the Hera Space Companion, not just an AI chatbot but a dynamic mission-linked communication platform, designed to make one of humankind’s most important scientific endeavours accessible to everyone! https://hera.space/
ESA’s FLEX mission reveals the secret glow of plants
Plants may look still and silent, but every leaf is constantly responding to its environment.
As plants photosynthesise, they emit an incredibly faint glow called fluorescence. Invisible to our eyes, this signal can reveal how plants are using sunlight and how they respond to heat, drought, pests and other environmental stresses.
ESA’s Fluorescence Explorer, or FLEX, will detect this faint signal from space. Using its highly sensitive FLORIS instrument, FLEX will map plant fluorescence across Earth, giving scientists a new way to observe plant health and photosynthetic activity on a global scale.
These observations will help us better understand how vegetation responds to a changing climate, including the effects of drought, and improve our understanding of the global carbon and water cycles.
Every leaf tells a story. With FLEX, we’re learning how to read it.
How FLEX measures Earth’s secret glow from space
Nature is full of incredible light shows, like sea sparkles and fireflies, many of which we can see with the naked eye. In sunlight, however, there is a faint glow we do not see.
It is emitted by plants.
When plants absorb sunlight to photosynthesise, they also emit a very faint fluorescence signal. Invisible to the naked eye, this fluorescence varies with environmental conditions and the physiological state of the vegetation
Remarkably, this can be observed from space.
The European Space Agency’s FLEX mission measures this unique signal to provide an unprecedented window into plant health, productivity and stress across the globe, enabling scientists to better understand how plants respond to environmental pressures such as drought, heat and climate change.
FLEX also delivers critical insights into the role of photosynthesis in the global carbon and water cycles, improving our understanding of Earth’s changing environment.
Biomass images mangrove degradation in the Niger Delta
MTM's selfie footage of BepiColombo's eight-year journey
Witness how over the last eight years, the ESA/JAXA BepiColombo mission has been travelling through the inner Solar System and aligning itself with Mercury's orbit. So far, it has travelled 9.9 billion km and completed nine 'planetary flybys' to help steer its way. In the video, you can see the spacecraft fly past Earth once, Venus twice, and Mercury six times.
Since launching on 20 October 2018, BepiColombo has been travelling as a composite spacecraft made up of ESA's Mercury Planetary Orbiter (MPO), JAXA's Mercury Magnetospheric Orbiter (Mio), and the Mercury Transfer Module (MTM) that carried the two orbiters to Mercury.
We've shared photos and videos before, taken by the spacecraft's three monitoring cameras (M-CAMs) on MTM. But this is the first time we've compiled them into a video of the mission's complete journey so far.
The monitoring cameras were designed to keep an eye on the spacecraft itself. In the foreground, you can see one of MTM's solar arrays (M-CAM 1, left), MPO's medium-gain antenna and magnetometer boom (M-CAM 2, middle), and MPO's high-gain antenna (M-CAM 3, right). The images have been positioned and oriented to approximately reflect the relative fields of view of the three M-CAMs.
As the M-CAMs have no shutter, many of the original images contain streaks due to light falling on the detectors during image read-out. These streaks have largely been removed for this video.
BepiColombo's arrival at Mercury began on 3 September 2026, with MTM separating from the spacecraft stack. The two stacked orbiters will enter orbit around Mercury in November, and separate from each other on 9–10 December 2026. From that moment on, BepiColombo will be the first mission with two spacecraft orbiting planet Mercury at the same time.
MTM has no computer to control itself, and lacks an antenna to communicate with Earth. Now that it has separated from the rest, it will circle the Sun indefinitely, letting the two science modules get to work. We expect MTM to pass by Mercury at a distance of around 130 000 km in late October. After that it will enter interplanetary space, and not get any closer to Mercury.
For more about BepiColombo, click here.
For the raw M-CAM images, click here.
Spectrum lifts off
Spectrum lifts offAnak Krakatau eruption by Sentinel-3
ESA’s High-Level Forum with Industry 2026
Round Table 4 – Strengthening Industry’s Capacity and Competitiveness, examining how Europe can scale industrial capacity, strengthen supply-chain resilience and remain globally competitive.BepiColombo begins its arrival at Mercury
A major milestone in BepiColombo’s journey to Mercury.
After almost eight years in space, the Mercury Transfer Module has completed its job. Following a carefully planned sequence of commands, it separated from the rest of the spacecraft and began drifting away at less than 40 cm per second.
ESA’s MPO and JAXA’s Mio will now continue their journey together towards Mercury, with the teams preparing for arrival over the next seven months.
Spectrum liftoff to orbit
Spectrum liftoff to orbitMedia briefing ahead of FLEX and Sentinel-3C launch
On 4 September 2026, media representatives joined an online briefing ahead of the launch of ESA’s FLEX and the Copernicus Sentinel-3C satellites.
The two satellites are scheduled to launch together aboard a Vega-C rocket from Europe’s Spaceport in French Guiana on 15 September at 03:21 CEST (14 September at 22:21 local time).
This video is a recording of the English briefing.
FLEX is equipped with the Fluorescence Imaging Spectrometer that will detect the faint fluorescence plants emit as they absorb sunlight during photosynthesis. Although invisible to the human eye, this subtle glow varies with plant health and environmental conditions.
In fact, the FLEX satellite will orbit in tandem with a Sentinel-3 satellite, which will be used to provide information on clouds, aerosols and water vapour as well as information about the land surface, such as the surface temperature, type of land cover and additional vegetation parameters. This integrated package of near-simultaneous measurements will provide an unprecedented view of global vegetation function and status.
Sentinel-3C is the third satellite in the Copernicus Sentinel-3 series. Like its two older siblings in orbit, Sentinel-3C carries a suite of cutting-edge instruments that measure systematically Earth’s oceans, land, ice and atmosphere to monitor and understand large-scale global dynamics. It provides essential information in near-real time for ocean and weather forecasting.
Europe’s Vega-C rocket is an evolution of the Vega rocket family, offering greater performance, larger payload capacity and improved competitiveness. It can launch up to 3300 kg into space, ideal for carrying small scientific and Earth observation satellites into orbit.
Guided relaxation sessions in orbit
This video was published on social media by ESA astronaut Sophie Adenot with the following caption:
Day 203 orbit 3146 — Floating upside down (from your point of view!), eyes closed, listening to a guided relaxation session...
Staying at your best in space isn't just about good hygiene, plenty of exercise and precise nutrition. Life in orbit is demanding, with busy schedules, occasional disrupted sleep and the challenges of microgravity, and for decades, astronauts have developed their own relaxation and meditation routines.
As part of the European RelaxPro study, we’re now officially testing techniques designed to help astronauts manage stress and improve sleep. By combining our feedback with physiological measurements, including saliva and hair samples, researchers hope to better understand how simple practices can support astronaut’s health and well-being on future long-duration missions.
In space as on Earth, staying at your best is sometimes also knowing when to slow down and breathe!
Jour 203, orbite 3146 – Suspendue la tête en bas (de votre point de vue !), les yeux fermés, avec dans les oreilles une séance de relaxation guidée...
Rester à 100% de ses capacités dans l’espace, ce n’est pas seulement une question d’hygiène, d’exercice physique ou de nutrition adaptée. La vie en orbite est exigeante: l’emploi du temps est chargé, le sommeil peut être perturbé, et la micropesanteur est un défi constant ! Du coup, cela fait des décennies que les astronautes emploient leurs propres routines de relaxation et de méditation.
L’étude européenne RelaxPro vise à tester scientifiquement des techniques destinées à aider les astronautes à mieux gérer leur stress et à améliorer leur sommeil. En combinant notre ressenti avec des mesures physiologiques, notamment à partir d’échantillons de salive et de cheveux, les chercheurs espèrent mieux comprendre comment de simples pratiques pourront contribuer à préserver la santé et le bien-être des astronautes lors des futures missions de longue durée.
Dans l’espace comme sur Terre, être au meilleur de sa forme, c’est parfois aussi savoir ralentir et prendre le temps de respirer profondément.
Third EVA highlights
This video was published on social media by ESA astronaut Sophie Adenot with the following caption:
Day 202 orbit 3131 — And that's three! Who remembers Jack standing at the bow of the Titanic , gazing out at the endless blue ocean ahead? That image popped into my mind as I reached the forward end of the Station to replace a retroreflector crucial for Dragon spacecraft dockings.
Definitely one of the most beautiful views in the world, and at the same time a bit intimidating from inside my spacesuit, with 400 km of emptiness beneath my feet. Ahead of me, nothing but the hypnotic blue of Earth , contrasting with the infinitely deep black of space. I arrived there during orbital night, my way lit only by my helmet lights, and then the Sun peeked over the horizon, illuminating our magnificent planet as it rotated beneath me. Just... wow!
They say that the journey matters more than the destination Reaching this part of the Station requires carefully making your way through dozens of structures and items that you absolutely must not touch, neither with the bulky rigid spacesuit nor with the tethers and straps that accompany every movement. Add to that handrails crowded with cables, and tools that seem to have a natural tendency to snag on anything they can... Imagine moving slowly, methodically and precisely through a cactus forest, doing everything you can to avoid the spines! I had been warned: "It's complicated, but it's doable." Of all the tasks I was entrusted with, this is probably the one I'm happiest to have completed successfully.
What an adventure these three spacewalks have been! But it will be good to catch my breath and recover physically before our return to Earth, which is also quite a challenge for the human body.
The teams were incredible. A huge thank you to everyone who worked so hard to make these EVAs a success.
Jour 202, orbite 3131 – Et de 3 !Qui se souvient de Jack à la proue du Titanic , visualisant devant lui l’infini océan bleu... C’est exactement ce qui m’est passé par la tête lorsque j’ai rejoint le point le plus en avant de la station pour remplacer un rétroréflecteur indispensable à l’amarrage de la capsule Dragon.
Forcément l’une des plus belles vues au monde, et en même temps, tellement impressionnante depuis mon scaphandre, avec 400 km de vide sous les pieds. Et comme seul paysage devant moi, le bleu hypnotisant de la Terre en contraste avec le noir infiniment dense de l’espace. Je suis arrivée de nuit, sans autre éclairage que celui de mon casque, et quand le soleil a pointé son nez sur l’horizon, notre magnifique planète qui défilait sous mes yeux. Juste... waouh !
On dit souvent que l’important, c’est le chemin, pas la destination Pour rejoindre cette zone de la Station, il faut progresser avec précaution au milieu de dizaines d’éléments qu’il ne faut surtout pas toucher, ni avec l’imposant scaphandre rigide, ni avec les longes et les sangles qui accompagnent nos mouvements. Ajoutez à cela les mains courantes encombrées de câbles, et les outils qui semblent avoir une attirance naturelle pour tous les endroits où ils peuvent se coincer... Visualisez une forêt de cactus dans laquelle vous avancez lentement, avec précision et méthode, pour éviter tout contact avec les épines ! J’étais prévenue : « C’est compliqué, mais faisable » et je suis particulièrement heureuse d’avoir mené à bien cette mission qui m’avait été confiée.
Quelle belle aventure que ces trois sorties extravéhiculaires ! Mais je l’avoue, cela va faire du bien de souffler un peu et de récupérer physiquement avant notre retour sur Terre, qui représente lui aussi un sacré défi pour l’organisme.
Les équipes ont été formidables. Un grand merci à tous qui avez travaillé dur pour faire de ces EVAs un succès.
BepiColombo’s Mercury arrival begins - full replay
Watch the replay of the livestream originally broadcast on 3 September as ESA/JAXA's BepiColombo mission took the first critical step towards arriving at Mercury.
After travelling through the inner Solar System together for eight years, BepiColombo's Mercury Transfer Module (MTM) will separate from the rest of the stacked spacecraft on 3 September 2026. This marks the beginning of one of the most complex planetary arrival sequences ever attempted by ESA.
Broadcast live from ESA's European Space Operations Centre (ESOC) in Darmstadt, Germany, the programme includes live views from the iconic Main Control Room, expert analysis, behind-the-scenes insights, and the first signal from the spacecraft following separation.
Livestream schedule (CEST):
13:45 – Livestream begins
14:00 – MTM separation
14:30 – Livestream pause
15:30 – Livestream resumes
15:53 – Earliest possible acquisition of signal and spacecraft status check
16:00-16:45 – End of livestream
EVA-99: NASA astronaut Jessica Meir riding Canadarm2
ESA astronaut Sophie Adenot and NASA astronaut Jessica Meir successfully completed US EVA-99 at 21:29 CEST on Tuesday 1 September. It was Sophie’s third spacewalk, and the 33rd conducted by a European astronaut.
During the 6-hour, 49-minute spacewalk, Sophie and Jessica completed several maintenance tasks, including replacing a spacecraft navigational aid, preparing a cosmic particle detector for future upgrades, installing jumper cables to enhance data relay capabilities, and collecting samples for the MicroOrganisms experiment.
EVA-99: Sophie Adenot working in the vacuum of space
ESA astronaut Sophie Adenot and NASA astronaut Jessica Meir successfully completed US EVA-99 at 21:29 CEST on Tuesday 1 September. It was Sophie’s third spacewalk, and the 33rd conducted by a European astronaut.
During the 6-hour, 49-minute spacewalk, Sophie and Jessica completed several maintenance tasks, including replacing a spacecraft navigational aid, preparing a cosmic particle detector for future upgrades, installing jumper cables to enhance data relay capabilities, and collecting samples for the MicroOrganisms experiment.
EVA-99: Sophie Adenot working in the vacuum of space
ESA astronaut Sophie Adenot and NASA astronaut Jessica Meir successfully completed US EVA-99 at 21:29 CEST on Tuesday 1 September. It was Sophie’s third spacewalk, and the 33rd conducted by a European astronaut.
During the 6-hour, 49-minute spacewalk, Sophie and Jessica completed several maintenance tasks, including replacing a spacecraft navigational aid, preparing a cosmic particle detector for future upgrades, installing jumper cables to enhance data relay capabilities, and collecting samples for the MicroOrganisms experiment.
EVA-99: Sophie Adenot working in the vacuum of space
ESA astronaut Sophie Adenot and NASA astronaut Jessica Meir successfully completed US EVA-99 at 21:29 CEST on Tuesday 1 September. It was Sophie’s third spacewalk, and the 33rd conducted by a European astronaut.
During the 6-hour, 49-minute spacewalk, Sophie and Jessica completed several maintenance tasks, including replacing a spacecraft navigational aid, preparing a cosmic particle detector for future upgrades, installing jumper cables to enhance data relay capabilities, and collecting samples for the MicroOrganisms experiment.
Separation for Mars
The slow-motion footage shows the separation of the ExoMars landing platform from the backshell during a test. A backshell is the cone-shaped rear section of a spacecraft’s protective aeroshell, which shields it from extreme heat and pressure during atmospheric entry.
Engineers are recreating the moment the lander breaks away from the backshell to head towards the martian surface. Anactuator with springs physically releases the lander at the right time and altitude.
It all happens when the landing platform is less than a kilometre in altitude from the ground, approaching it at 125 km per hour. At that moment, the parachutes are slowing down the module, which has already jettisoned its front shield and deployed its four legs.
Only after checking the spacecraft’s altitude and speed, and the readiness of the braking engines, does the onboard computer trigger the separation.
The test campaign at the Thales Alenia Space facilities in Turin, Italy, and used a full-scale model that replicates the structure and dimensions of the ExoMars landing platform and backshell.
The successful campaign takes ESA’s ExoMars Rosalind Franklin rover mission one step closer to a safe touchdown on Mars launch in 2028.
Hubble's superbubble scene
This sprawling cosmic vista and subject of today’s ESA/Hubble Picture of the Month comes from the Large Magellanic Cloud (LMC). The LMC is the largest of the small galaxies that orbit our Milky Way galaxy. At just 160 000 light-years away, the LMC offers a close look at highly active stellar birthsites like the nebula shown here. This nebula is named LHA 120-N44, or N44 for short, and it’s located in the constellation Dorado.
The appearance of this photogenic nebula is dominated by two features: a vast central void and a shell of dense, dusty gas. The central void is a ‘superbubble’ spanning roughly 210 by 140 light-years. The glittering stars at the centre of the void are responsible for its creation; through their powerful stellar winds and explosive supernovae, these stars have expelled much of the gas from which they were born.
When the stars of N44’s central star cluster swept away this gas, the expelled gas formed a shell around the superbubble. New stars are forming in this compressed gas shell, making N44 an interesting target for researchers studying the process of star formation. In particular, astronomers have turned to this nebula as an ideal place to time this process from start to finish. Their goal is to understand how long it takes from the collapse of cold gas clouds into dense knots to the moment nuclear fusion ignites in the heart of a newborn star.
Researchers used Hubble to survey N44 and take a census of its stars, cataloguing nearly half a million stars within the cluster as well as interlopers drifting in front of it. Of the stars surveyed, nearly 30 000 are what astronomers call pre-main-sequence stars, which have yet to begin fusing hydrogen into helium in their cores. This treasure trove of baby stars was discoverable thanks to the high sensitivity and fine spatial resolution of Hubble’s instruments that can pick out faint objects in crowded clusters.
The gas shell surrounding the superbubble is energised by ultraviolet radiation from massive stars, causing it to glow and highlighting several distinct features. Each feature within the broader N44 star-forming complex was catalogued by astronomer Karl Henize in the 1950s. One feature is a smaller bubble, catalogued as N44F, that is located near the upper-right corner of this image. N44F is an interstellar bubble blown by the intense stellar winds of a single hot and massive star. As this previously released Hubble closeup shows, the star’s furious winds and radiation have sculpted the surrounding bubble and created pillars of dusty gas.
The data used to create this image come from an observing programme (#14689; PI: Gouliermis) that aimed to probe stars in the N44 complex that have not yet begun fusing hydrogen into heavier elements in their cores. These data help to determine how long the process of star formation takes, as well as what masses newborn stars typically have. Hubble's sensitive observations of the lowest-mass stars in this region open a new window onto star formation in regions that, like the LMC or the galaxies of the early Universe, are poor in elements heavier than helium.
[Image Description: A dense field of stars fills the image, surrounded by wispy clouds of gas and dust. Pale blue and grey nebulosity forms an intricate web across the scene, with darker clouds of dust concentrated towards the lower right. Numerous bright stars appear in shades of blue, white and orange.]
Page 1 de 3
- 1
- 2
- 3
- Suivante
- Dernière »
