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Save the date: ESA’s Living Planet Symposium 2025
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By European Space Agency
Video: 00:10:27 In 1975, 10 European countries came together with a vision to collaborate on key space activities: science and astronomy, launch capabilities and space applications: the European Space Agency, ESA, was born.
In 2025, we mark half a century of joint European achievement – filled with firsts and breakthroughs in science, exploration and technology, and the space infrastructure and economy that power Europe today.
During the past five decades ESA has grown, developing ever bolder and bigger projects and adding more Member States, with Slovenia joining as the latest full Member State in January.
We’ll also celebrate the 50th anniversary of ESA’s Estrack network, 30 years of satellite navigation in Europe and 20 years since ESA launched the first demonstration satellite Giove-A which laid the foundation for the EU’s own satnav constellation Galileo. Other notable celebrations are the 20th anniversary of ESA’s Business Incubation Centres, or BICs, and the 30th year in space for SOHO, the joint ESA and NASA Solar and Heliospheric Observatory.
Sadly though, 2025 will mean end of science operations for Integral and Gaia. Integral, ESA's gamma-ray observatory has exotic objects in space since 2002 and Gaia concludes a decade of mapping the stars. But as some space telescopes retire, another one provides its first full data release. Launched in 2023, we expect Euclid’s data release early in the new year.
Launch-wise, we’re looking forward to Copernicus Sentinel-4 and -5 (Sentinel-4 will fly on an MTG-sounder satellite and Sentinel-5 on the MetOp-SG-A1 satellite), Copernicus Sentinel-1D, Sentinel-6B and Biomass. We’ll also launch the SMILE mission, or Solar wind Magnetosphere Ionosphere Link Explorer, a joint mission with the Chinese academy of science.
The most powerful version of Europe’s new heavy-lift rocket, Ariane 6, is set to fly operationally for the first time in 2025. With several European commercial launcher companies planning to conduct their first orbital launches in 2025 too, ESA is kicking off the European Launcher Challenge to support the further development of European space transportation industry.
In human spaceflight, Polish ESA project astronaut Sławosz Uznański will fly to the ISS on the commercial Axiom-4 mission. Artemis II will be launched with the second European Service Module, on the first crewed mission around the Moon since 1972.
The year that ESA looks back on a half century of European achievement will also be one of key decisions on our future. At the Ministerial Council towards the end of 2025, our Member States will convene to ensure that Europe's crucial needs, ambitions and the dreams that unite us in space become reality.
So, in 2025, we’ll celebrate the legacy of those who came before but also help establish a foundation for the next 50 years. Join us as we look forward to a year that honours ESA’s legacy and promises new milestones in space.
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By NASA
The NASA Ames Science Directorate recognizes the outstanding contributions of (pictured left to right) Maurice Valdez, Niki Parenteau, Dori Myer, and Judy Alfter. Their commitment to the NASA mission represents the entrepreneurial spirit, technical expertise, and collaborative disposition needed to explore this world and beyond.
Space Science and Astrobiology Star: Maurice Valdez
Maurice Valdez is a system administrator, supporting desktop systems and website development for the Space Science and Astrobiology Division. Maurice is recognized for his focus and commitment to supporting the division’s scientific productivity by keeping systems compliant and functioning. His can-do attitude makes him instrumental in the success of the team, whether he is finding new solutions for hybrid meetings, fixing equipment, patching systems, or troubleshooting issues.
Photo credit: Pacific Science Center Space Science and Astrobiology Star: Niki Parenteau
Niki Parenteau, a research scientist for the Exobiology Branch, embodies the true spirit of an interdisciplinary astrobiologist. She has applied her expertise to identify potential biosignatures of life on exoplanets and has taken a leading role in the project office for the development of the Habitable Worlds Observatory (HWO), where she facilitates collaborative efforts of Ames scientists across the division and shepherds the larger scientific community to enable observations of biosignatures with HWO.
Space Biosciences Star: Dori Myer
Archivist Dori Myer has made an outstanding contribution in the Flight Systems Implementation Branch’s multi-year effort to digitize and preserve institutional knowledge. Under her guidance, the records management team digitized tens of thousands of historical records, preserving the branch’s institutional knowledge for years to come. Her exceptional initiative and dedication have transformed our record management processes, ensuring the accessibility of NASA’s rich institutional knowledge while streamlining its access in the modern age.
Earth Science Star: Judy Alfter
Judy Alfter, a Deputy Project Manager in the Earth Science Project Office (ESPO), has excelled in her multi-faceted role during the field campaign for the Plankton, Aerosol, Cloud, ocean Ecosystem Post-launch Airborne eXperiment (PACE-PAX). Judy launched the deployment phase of PACE-PAX, leading the effort to set up Twin Otter flight operations at Marina Municipal Airport in California. Following this phase, she transitioned to Santa Barbara in California to support the mobilization of PACE-PAX ship operations and concluded deployment activities at NASA Armstrong Flight Research Center’s main campus as ESPO site manager for ER-2 flight operations.
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By NASA
Photographers at NASA capture the sunset on Tuesday, Jan. 30, 2024, near the headquarters building of the agency’s Kennedy Space Center in Florida.NASA/Ben Smegelsky As NASA’s Kennedy Space Center in Florida wraps up a year that will see more than 90 government, commercial, and private missions launch from Florida’s Space Coast, a look to 2025 shows the missions, partnerships, projects, and programs at the agency’s main launch site will continue innovating, inspiring, and pushing the boundaries of exploration for the benefit of humanity.
“The next year promises to be another exciting one at Earth’s premier spaceport,” said Kennedy Center Director Janet Petro. “We have an amazing workforce, and when we join forces with industry and our other government partners, even the sky is no limit to what we can accomplish.”
New Year, New Missions to Space Station
NASA’s Commercial Crew Program (CCP), based out of Kennedy, and its commercial partner SpaceX plan two crew rotation missions to the International Space Station: NASA’s SpaceX Crew-10 and Crew-11. This also means the return of the Crew-9 mission and later Crew-10 during 2025. CCP continues working with Boeing toward NASA certification of the company’s Starliner system for future crew rotations to the orbiting laboratory.
NASA’s SpaceX Crew-10 members stand between Falcon 9 first-stage boosters at SpaceX’s HangarX facility at NASA’s Kennedy Space Center in Florida. From left are Mission Specialist Kirill Peskov of Roscosmos, Mission Specialist Takuya Onishi of JAXA (Japan Aerospace Exploration Agency), along with NASA astronauts Commander Anne McClain and Pilot Nichole Ayers. SpaceX “Operations in 2025 are a testament to NASA’s workforce carefully planning and preparing to safely execute a vital string of missions that the agency can depend on,” said Dana Hutcherson, CCP deputy program manager. “This is the 25th year of crewed operations for the space station, and we know that with every launch, we are sustaining a critical national asset and enabling groundbreaking research.”
NASA also plans several Commercial Resupply Services missions, utilizing SpaceX’s Dragon cargo spacecraft, Northrop Grumman’s Cygnus spacecraft, and the inaugural flight of Sierra Space’s cargo spaceplane, Dream Chaser. The missions will ferry thousands of pounds of supplies, equipment, and science investigations to the crew aboard the orbiting laboratory from NASA Kennedy and nearby Cape Canaveral Space Force Station.
The SpaceX Falcon 9 rocket carrying the Dragon spacecraft lifts off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida on Tuesday, Nov. 4, on the company’s 31st commercial resupply services mission for the agency to the International Space Station. Liftoff was at 9:29 p.m. EST. SpaceX In addition to the agency’s crewed flights, Axiom Space’s fourth crewed private spaceflight mission, Axiom Mission 4 – organized in collaboration with NASA through the International Space Station Program and operated by SpaceX – will launch to the orbital outpost.
Reestablishing Humanity’s Lunar Presence
Preparations for NASA’s Artemis II test flight mission are ramping up, with all major components for the SLS (Space Launch System) hardware undergoing processing at Kennedy, including the twin solid rocket boosters and 212-foot-tall core stage. Teams with EGS (Exploration Ground Systems) will continue stacking the booster segments inside the spaceport’s VAB (Vehicle Assembly Building). Subsequent integration and testing of the rocket’s hardware and Orion spacecraft will continue not only for the Artemis II mission, but for Artemis III and IV. Technicians also continue building mobile launcher 2, which will serve as the launch and integration platform for the SLS Block 1B configuration starting with Artemis IV.
Teams with NASA’s Exploration Ground Systems transport the agency’s 212-foot-tall SLS (Space Launch System) core stage into High Bay 2 at the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida on Wednesday, Dec. 11, 2024. The one-of-a kind lifting beam is designed to lift the core stage from the transfer aisle to High Bay 2 where it will remain while teams stack the two solid rocket boosters on top of mobile launcher 1 for the SLS core stage.NASA/Kim Shiflett “Looking ahead to 2025, teams will embark on a transformative year as we integrate the flight hardware for Artemis II, while simultaneously developing the foundation for future Artemis missions that will reestablish humanity’s presence on the Moon,” said Shawn Quinn, EGS program manager.
A key part of the Artemis campaign, NASA’s CLPS (Commercial Lunar Payload Services) initiative will continue leveraging commercial partnerships to quickly land scientific instruments and technology demonstrations on the Moon. Firefly Aerospace’s first lunar CLPS flight, Blue Ghost Mission 1, will carry 10 NASA science and technology instruments to the lunar surface, including the Electrodynamic Dust Shield, a technology built by Kennedy engineers. Intuitive Machines, meanwhile, will embark on its second CLPS flight to the Moon. Providing the first in-situ resource utilization demonstration on the lunar surface, IM-2 will carry the Polar Resources Ice Mining Experiment-1 (PRIME-1), which features The Regolith and Ice Drill for Exploring New Terrain from Honeybee Robotics, as well as the Mass Spectrometer Observing Lunar Operations built by Kennedy. Both flights are targeted to lift off from Kennedy’s Launch Complex 39A during the first quarter of 2025.
As part of NASA’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign, Firefly Aerospace’s Blue Ghost Mission One lander will carry 10 NASA science and technology instruments to the Moon’s near side.Firefly Aerospace In development for Artemis IV and beyond, Gateway will be a critical platform for developing a sustained human presence beyond low Earth orbit. Deep Space Logistics (DSL) is the Gateway Program project office at Kennedy responsible for leading the development of a commercial supply chain in deep space. In 2025, DSL will continue developing the framework for the DSL-1 mission and working with commercial provider SpaceX to mature spacecraft design. Upcoming milestones include a system requirements review and preliminary design review to determine the program’s readiness to proceed with the detailed design phase supporting the agency’s Gateway Program and Artemis IV mission objectives.
Science Missions Studying Our Solar System and Beyond
NASA’s Launch Services Program (LSP), based at Kennedy, is working to launch three ambitious missions. Launching early in the year on a SpaceX Falcon 9 rocket from Vandenberg Space Force Base in California, SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer) is a space telescope to survey the universe using visible and near-infrared light, observing more colors than ever before and allowing astronomers to piece together a three-dimensional map of the universe with stunning accuracy. Launching with SPHEREx, NASA’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission will study how the mass and energy of the Sun’s corona transition into the solar wind.
NASA’s SPHEREx space observatory was photographed at BAE Systems in Boulder, Colorado, in November 2024 after completing environmental testing. The spacecraft’s three concentric cones help direct heat and light away from the telescope and other components, keeping them cool. BAE Systems IMAP (Interstellar Mapping and Acceleration Probe), scheduled to launch from Cape Canaveral in late 2025, will help map out thethe heliosphere – the magnetic environment surrounding and protecting our solar system. Carrying 10 instruments to make its observations, the IMAP mission is targeting the L1 Lagrange Point, an area between Earth and the Sun that is easy for spacecraft to maintain orbit, along with two Sun observing rideshare missions – NASA’s Carruthers Geocorona Observatory and the National Oceanic and Atmospheric Administration’s SWFO-L1 (Space Weather Follow-On at L1). Also launching in late 2025 on a Falcon 9 from Vandenberg is the second of two identical satellites, Sentinel-6B, which will monitor global sea levels with unprecedented precision. Its predecessor, Sentinel-6 Michael Freilich, has been delivering crucial data since it launched in 2020, and Sentinel-6B will ensure the continuation of this mission through 2030.
“Our missions launching next year will include groundbreaking technologies to help us learn more about the universe than ever before and provide new data for researchers that will have positive benefits here on Earth,” said LSP’s Deputy Program Manager Jenny Lyons.
NASA’s ESCAPADE (Escape and Plasma Acceleration and Dynamics Explorers) identical dual spacecraft are inspected and processed on dollies in a high bay of the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida on Thursday, Aug. 22, 2024. As the first multi-spacecraft orbital science mission to Mars, ESCAPADE’s twin orbiters will take simultaneous observations from different locations around the planet and reveal the real-time response to space weather and how the Martian magnetosphere changes over time.NASA/Kim Shiflett The program’s support for small satellite missions next year includes several missions to monitor the Sun, collect climate data, and more. NASA’s ESCAPADE (Escape and Plasma Acceleration and Dynamics Explorers) mission to explore Mars’ magnetosphere will lift off from Cape Canaveral’s Launch Complex 36 on NASA’s inaugural flight of Blue Origin’s New Glenn rocket. Some of these small satellite missions are part of NASA’s CubeSat Launch Initiative, which offers the next generation of scientists, engineers, and technologists a unique opportunity to conduct scientific research and develop and demonstrate novel technologies in space.
Building the Spaceport’s Future
Teams expect a busy year of construction projects to accommodate new missions, hardware, and milestones. In preparation for Artemis IV, mobile launcher 2 construction and modifications in the VAB’s High Bays 3 and 4 for the larger SLS Block 1B configuration will ramp up. Teams also will upgrade the spaceport’s Converter Compressor Facility (CCF) to meet the helium needs of its commercial launch partners and the Artemis campaign, increasing efficiency, reliability, and speed of pumping helium to rockets. Upgrades to the CCF’s internal infrastructure are also part of Kennedy’s plan to earn the U.S. Green Building Council’s Leadership in Energy and Environmental Design certification, joining nine other Kennedy facilities in achieving that rating.
Photographers at NASA capture the sunset on Tuesday, Jan. 30, 2024, near Vehicle Assembly Building at the agency’s Kennedy Space Center in Florida. The iconic Vehicle Assembly Building, currently used for assembly of NASA’s Space Launch System rocket for Artemis missions, remains the only building in which rockets were assembled that carried humans to the surface of another world. NASA/Ben Smegelsky “Kennedy’s spaceport will continue to see its launch cadence grow, and we have to meet our program and commercial partner needs in the most efficient way possible,” said Sasha Sims, deputy director of Kennedy’s Spaceport Integration and Services Directorate. “Process improvements and integrated approaches should improve the speed at which government and commercial construction takes place while also improving Kennedy’s infrastructure so that it’s robust, sustainable, and able to support America’s future in space.”
Driving down acquisition costs, increasing competition, and using innovative contracting mechanisms for construction are just some of the initiatives to maximize efficiency and reliability in 2025. The center’s “Critical Day” policy prohibits certain types of work during launches requiring full flight range support but will no longer apply to commercial launches where minimal flight range support is required, training events, static fires, exercises, tests, rehearsals, nor other activities leading up to or supporting launches. This policy change is expected to create more flexibility and free up over 150 days annually for construction, maintenance, and other essential work needed to keep the spaceport running smoothly.
Finally, Kennedy will continue carrying Apollo’s legacy through Artemis. Seeds that traveled aboard the Orion spacecraft during the Artemis I mission will be planted at the spaceport, honoring the legacy of the original Moon Trees that grew from seeds flown on Apollo 14. The Florida spaceport will become one of the select locations across the country where the “new generation” of Moon Trees will take root and provide living testimony to the agency’s continuing legacy of lunar exploration.
“With so many missions and initiatives on the horizon, I’m looking forward to another banner year at Kennedy Space Center,” Petro said. “We truly are launching humanity’s future.”
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By European Space Agency
Our understanding of planet formation in the Universe’s early days is challenged by new data from the NASA/ESA/CSA James Webb Space Telescope. Webb solved a puzzle by proving a controversial finding made with the NASA/ESA Hubble Space Telescope more than 20 years ago.
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By NASA
Webb Webb News Latest News Latest Images Blog (offsite) Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Observatory Overview Launch Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning 7 Min Read NASA’s Webb Finds Planet-Forming Disks Lived Longer in Early Universe
This is a James Webb Space Telescope image of NGC 346, a massive star cluster in the Small Magellanic Cloud, a dwarf galaxy that is one of the Milky Way’s nearest neighbors. Credits:
NASA, ESA, CSA, STScI, Olivia C. Jones (UK ATC), Guido De Marchi (ESTEC), Margaret Meixner (USRA) NASA’s James Webb Space Telescope just solved a conundrum by proving a controversial finding made with the agency’s Hubble Space Telescope more than 20 years ago.
In 2003, Hubble provided evidence of a massive planet around a very old star, almost as old as the universe. Such stars possess only small amounts of heavier elements that are the building blocks of planets. This implied that some planet formation happened when our universe was very young, and those planets had time to form and grow big inside their primordial disks, even bigger than Jupiter. But how? This was puzzling.
To answer this question, researchers used Webb to study stars in a nearby galaxy that, much like the early universe, lacks large amounts of heavy elements. They found that not only do some stars there have planet-forming disks, but that those disks are longer-lived than those seen around young stars in our Milky Way galaxy.
“With Webb, we have a really strong confirmation of what we saw with Hubble, and we must rethink how we model planet formation and early evolution in the young universe,” said study leader Guido De Marchi of the European Space Research and Technology Centre in Noordwijk, Netherlands.
Image A: Protoplanetary Disks in NGC 346 (NIRCam Image)
This is a James Webb Space Telescope image of NGC 346, a massive star cluster in the Small Magellanic Cloud, a dwarf galaxy that is one of the Milky Way’s nearest neighbors. With its relative lack of elements heavier than hydrogen and helium, the NGC 346 cluster serves as a nearby proxy for studying stellar environments with similar conditions in the early, distant universe. Ten, small, yellow circles overlaid on the image indicate the positions of the ten stars surveyed in this study. NASA, ESA, CSA, STScI, Olivia C. Jones (UK ATC), Guido De Marchi (ESTEC), Margaret Meixner (USRA) A Different Environment in Early Times
In the early universe, stars formed from mostly hydrogen and helium, and very few heavier elements such as carbon and iron, which came later through supernova explosions.
“Current models predict that with so few heavier elements, the disks around stars have a short lifetime, so short in fact that planets cannot grow big,” said the Webb study’s co-investigator Elena Sabbi, chief scientist for Gemini Observatory at the National Science Foundation’s NOIRLab in Tucson. “But Hubble did see those planets, so what if the models were not correct and disks could live longer?”
To test this idea, scientists trained Webb on the Small Magellanic Cloud, a dwarf galaxy that is one of the Milky Way’s nearest neighbors. In particular, they examined the massive, star-forming cluster NGC 346, which also has a relative lack of heavier elements. The cluster served as a nearby proxy for studying stellar environments with similar conditions in the early, distant universe.
Hubble observations of NGC 346 from the mid 2000s revealed many stars about 20 to 30 million years old that seemed to still have planet-forming disks around them. This went against the conventional belief that such disks would dissipate after 2 or 3 million years.
“The Hubble findings were controversial, going against not only empirical evidence in our galaxy but also against the current models,” said De Marchi. “This was intriguing, but without a way to obtain spectra of those stars, we could not really establish whether we were witnessing genuine accretion and the presence of disks, or just some artificial effects.”
Now, thanks to Webb’s sensitivity and resolution, scientists have the first-ever spectra of forming, Sun-like stars and their immediate environments in a nearby galaxy.
“We see that these stars are indeed surrounded by disks and are still in the process of gobbling material, even at the relatively old age of 20 or 30 million years,” said De Marchi. “This also implies that planets have more time to form and grow around these stars than in nearby star-forming regions in our own galaxy.”
Image B: Protoplanetary Disks in NGC 346 Spectra (NIRSpec)
This graph shows, on the bottom left in yellow, a spectrum of one of the 10 target stars in this study (as well as accompanying light from the immediate background environment). Spectral fingerprints of hot atomic helium, cold molecular hydrogen, and hot atomic hydrogen are highlighted. On the top left in magenta is a spectrum slightly offset from the star that includes only light from the background environment. This second spectrum lacks a spectral line of cold molecular hydrogen.
On the right is the comparison of the top and bottom lines. This comparison shows a large peak in the cold molecular hydrogen coming from the star but not its nebular environment. Also, atomic hydrogen shows a larger peak from the star. This indicates the presence of a protoplanetary disk immediately surrounding the star. The data was taken with the microshutter array on the James Webb Space Telescope’s NIRSpec (Near-Infrared Spectrometer) instrument. Illustration: NASA, ESA, CSA, Joseph Olmsted (STScI) A New Way of Thinking
This finding refutes previous theoretical predictions that when there are very few heavier elements in the gas around the disk, the star would very quickly blow away the disk. So the disk’s life would be very short, even less than a million years. But if a disk doesn’t stay around the star long enough for the dust grains to stick together and pebbles to form and become the core of a planet, how can planets form?
The researchers explained that there could be two distinct mechanisms, or even a combination, for planet-forming disks to persist in environments scarce in heavier elements.
First, to be able to blow away the disk, the star applies radiation pressure. For this pressure to be effective, elements heavier than hydrogen and helium would have to reside in the gas. But the massive star cluster NGC 346 only has about ten percent of the heavier elements that are present in the chemical composition of our Sun. Perhaps it simply takes longer for a star in this cluster to disperse its disk.
The second possibility is that, for a Sun-like star to form when there are few heavier elements, it would have to start from a larger cloud of gas. A bigger gas cloud will produce a bigger disk. So there is more mass in the disk and therefore it would take longer to blow the disk away, even if the radiation pressure were working in the same way.
“With more matter around the stars, the accretion lasts for a longer time,” said Sabbi. “The disks take ten times longer to disappear. This has implications for how you form a planet, and the type of system architecture that you can have in these different environments. This is so exciting.”
The science team’s paper appears in the Dec. 16 issue of The Astrophysical Journal.
Image C: NGC 346: Hubble and Webb Observations
Image Before/After The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).
The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt manages the telescope and mission operations. Lockheed Martin Space, based in Denver also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.
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Media Contacts
Laura Betz – laura.e.betz@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Ann Jenkins – jenkins@stsci.edu, Christine Pulliam – cpulliam@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
Related Information
Past releases on NGC 346: Webb NIRCam image and MIRI image
Article: Highlighting other Webb Star Formation Discoveries
Simulation Video: Planetary Systems and Origins of Life
Animation Video: Exploring star and planet formation (English), and in Spanish
More Images of NGC 346 on AstroPix
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