21 Years of Europlanet

21 Years of Europlanet

New Year’s Day 2026 is Europlanet’s 21st birthday. To celebrate, we highlight 21 things that Europlanet has achieved since its foundation on 1 January 2005.

  1. The Europlanet Science Congress
Opening ceremony of EPSC-DPS2025. Credit: Europlanet.

First held in Berlin in 2006, the Europlanet Science Congress (EPSC) is the largest annual meeting on planetary science in Europe and regularly attracts over 1200 participants. Its interdisciplinary, interactive and adaptive format makes EPSC an ideal place for the global planetary community to share ideas and build new connections. Joint meetings with the American Astronomical Society’s Division of Planetary Sciences (DPS) and the European Astrobiology Network Association (EANA) have brought together even bigger international and cross-disciplinary audiences, with the recent EPSC-DPS2025 in Helskinki becoming the largest planetary meeting to date in Europe with 1800 participants.

  1. Research and Technology Infrastructure
The Laboratory of Electron Induced Fluorescence at Comenius University. Credit: Comenius University.

Europlanet provides access to state-of-the-art research and technology infrastructure (RTI) to support planetary science and space exploration. The distributed RTI includes facilities for the simulation of planetary environments, analysis of planetary samples, testing and development of space technologies, and support of interdisciplinary studies. Our Transnational Access (TA) programme is designed to allow researchers from anywhere in the world, and at all career stages, to have access to facilities to support scientific and technological excellence in planetary/space research and to foster international collaborations. To date, Europlanet has funded over 600 research visits, amounting to in excess of 5,500 days of access (15 years), involving over 800 individual researchers accessing 23 laboratories (with over 80 individual facilities), 12 planetary analogue field sites and 17 telescopes.

Applications for a new TA call will open later in January.

  1. Membership Organisation

Europlanet is a grass-roots organisation, supported by individual members since 2018 and organisational members since 2025. Membership benefits include discounted fees for EPSC, access to facilities, expert exchanges, webinars, training, workshops, funding schemes and much more. Join now to help us continue our mission to support the planetary community around the world.

Join Europlanet>>

  1. Europlanet Early Careers (EPEC) Network
Participants at EPEC Annual Week 2025. Credit: EPEC.

The Europlanet Early Career (EPEC) network is organised by early-career researchers for early-career researchers, and includes volunteers from across the Europlanet international community. The EPEC network is open to all students, doctoral candidates and early-career planetary scientists and space professionals whose last degree (e.g. MSc or PhD) was obtained a maximum of 7 years ago (excluding parental leave, serious illness and similar delays).

EPEC’s activities, including Annual Week and EPEC@EPSC, aim to form a strong network between young professionals by organising early-career-relevant events and by engaging in different projects amongst different focus areas (outreach, diversity, early career support). As early careers comprise over half Europlanet’s individual members and attendees at EPSC, EPEC ensures that the (scientifically) young members of our community have a clear voice within Europlanet to shape the future of planetary and space sciences and engineering.

Find out more>>

  1. Regional Hubs
The launch of the Europlanet Colombia Regional Hub in November 2025. Credit: Europlanet Colombia.

Europlanet’s Regional Hubs support the development of planetary science at a national and regional level, particularly in countries and areas that are currently under-represented within the community. Our Hub Committees organise networking events and workshops to support the research community, as well as to build links with amateur astronomers, industrial partners, policymakers, educators, the media and the wider public. In addition to 10 European Regional Hubs, a Colombian Regional Hub was established in 2025 to support the community in Colombia and Latin America.

  1. Projects
The launch of the European Planetology Network (EuroPlaNet) in 2005. Credit: Europlanet.

Europlanet was founded as a Coordination Action funded by the European Commission (EC) in 2005-2008 to promote networking, support the sharing of resources and overcome fragmentation in the European planetary science community. Through a series of further EC grants awarded between 2009 and 2024, Europlanet has subsequently developed into a global distributed research infrastructure that offers coordinated access to services and facilities spread over 5 continents, supporting a community of thousands of users in academia, industry and in the wider community. In total, the EC has invested €28 million in Europlanet to support the planetary community.

Europlanet has received funding from the European Commission under Grant Numbers 871149, 654208, 228319 and RICA-CT-2004-001637.

  1. VESPA
Superimposed olivine map from OMEGA / Mars-Express in N Syrtis Major area (Jezero crater is at the bottom), displayed in the Aladin service and accessed through VESPA.
Superimposed olivine map from OMEGA / Mars-Express in N Syrtis Major area (Jezero crater is at the bottom), displayed in the Aladin service and accessed through VESPA. Credit: Aladin.

VESPA (Virtual European Solar and Planetary Access) is a web-based search interface to identify and access planetary science and heliophysics data provided by the science community. Developed through EC-funded Europlanet projects, and hosted and maintained by the Observatory of Paris, VESPA is freely available to researchers and the general public. The VESPA portal supports user-friendly searching on metadata associated with generic observation conditions (such as target, instrument, time/space/spectral coverages, illumination conditions, etc) and metadata specific to each dataset (such as instrumental parameters) via the EPN-TAP protocol, which is now a standard of the International Virtual Observatory Alliance (IVOA) for Solar system data. Nearly 250 EPN-TAP data services of various size are declared in the IVOA registry, of which 94 are currently validated and accessible via the portal – including ESA’s Planetary Science Archive (PSA). VESPA also offers an easy solution for small teams to share newly-derived data from a publication or a research project.

  1. SPIDER

Europlanet’s SPIDER Planetary Space Weather Services provide contextual information on predictions and alerts for planetary space weather analysis and payload or spacecraft operations. SPIDER enables researchers to take advantage of data from a suite of missions at different points in the Solar System. Applications of SPIDER’s tools have led to several high-impact publications, and have been used to support planning of the BepiColombo and Juice missions. Opportunities identified through SPIDER for synergistic observations by BepiColombo during its cruise phase with the Solar Orbiter and Solar Parker Probe missions have also been implemented by ESA and JAXA. 

  1. GMAP and Winter School
GMAP Winter School Banner 2026.

The Geological Mapping (GMAP) activity provides a complete infrastructure for the geological mapping of planetary bodies. As well as everything needed to create planetary maps, GMAP provides guidelines and insights on how to produce effective mapping products for scientific exploitation, as well as information on how to display and archive results in a structured way. 

GMAP supports researchers who are interested in learning how to build their own mapping products, as well as mappers who want to learn how to incorporate other types of data analysis into their products.

One of GMAP’s major successes has been the establishment of the annual Geology & Planetary Mapping Winter School. Now in its fifth iteration, the Winter School provides training for anyone interested in planetary mapping to build knowledge and skills in planetary mapping. Participants can follow synchronously or asynchronously to accommodate different time zones. The 2026 edition will run from 26-30 January 2026. 

Find out more or register now>>

  1. Europlanet Telescope Network
Amateur astronomer, Florence Libotte (centre) with astronomers Erika Pakštienė (left) and Gražina Tautvaišienė (right) at the Moletai Observatory, Lithuania.

The Europlanet Telescope Network brings together medium and small telescopes to facilitate and coordinate observations related to planetary science. Founded in 2020, the telescope network has awarded 256.5 observing nights and supported 44 projects on planetary topics from near Earth objects to exoplanets, as well as astrophysical subjects including black holes and binary star systems. As well as supporting the professional scientific community, the Europlanet telescope Network has provided access and training for amateur astronomers to enable them to contribute to planetary research. Since the end of the EC-funded project, the Europlanet Telescope Network has maintained a list of telescopes willing to offer observing time to the community. The Europlanet Telescope Network currently unites 21 observatories with 32 telescopes in 16 countries.

Find out more>>

  1. Webinars

Europlanet holds monthly webinars on a range of topics from science to policy, diversity and outreach. Quarterly webinars are also co-organised with the Science Team of the ESA Juice mission. 

The JUICE mission will explore Jupiter and its icy moons.
Europlanet webinars provide quarterly updates on the JUICE mission on its long journey to reach and explore Jupiter and its icy moons. Credit: ESA/ATG medialab/NASA/JPL/J Nichols/U Leicester/U Arizona/DLR.

Find out what’s coming up>>

  1. Meetings and Workshops
Group photo of in-person participants at ERIM 2023 in Bratislava, Slovakia.
Group photo of in-person participants at ERIM 2023 in Bratislava, Slovakia. Credit: Europlanet/J-D Bodénan.

In addition to EPSC and EPEC Annual Week, Europlanet organises a range of meetings, summer schools, workshops and training sessions to support the community. Our interactive online Teams Days, held 2-3 times per year, are an opportunity for the community to provide input and feedback into Europlanet’s strategy and operations. The Europlanet Research Infrastructure Meeting (ERIM) in 2023 comprised a series of interactive workshops with the aim of promoting collaboration across the Europlanet community. More recently, policy workshops organised in partnership with other research infrastructures have helped share information on upcoming opportunities and best practice for distributed RIs.

In total, over the past two decades, Europlanet has provided training for over 7,500 members of the planetary community, with a particular focus on early career researchers.

Find out more>>

  1. Discord

Join hundreds of other Europlanet members on our Discord server to keep up with news, events, job opportunities and to connect with colleagues around the world. The server is designed with a variety of channels to facilitate discussions and interactions, including text channels, discussion forums and voice channels. We also hold regular informal catch ups and science discussion ‘hangouts’.

Join Europlanet on Discord>>

  1. Diversity

Europlanet is committed to building a diverse, inclusive planetary science and ensuring that individuals within that community experience equal opportunity, regardless of gender, disability, ethnic origin, religion or belief, sexual orientation, marital status, age, nationality or socioeconomic background. The Europlanet Diversity Committee acts as a strategic task force to advise, coordinate and champion activities across Europlanet that further the association’s commitment to equality, diversity and inclusivity. As well as activities around EPSC, the Diversity Committee organises events to raise awareness of diversity, inclusivity and accessibility in the planetary community, such as through the Planetary Science Wiki Edit-a-thon.

  1. Outreach

Outreach and education have been a core part of Europlanet initiatives since its foundation the early 2000s. Our objective is to support the planetary science community at a grass roots level to do more public engagement and educational activities, and to share best practice, training and resources to increase the impact of those efforts. Over 20 public engagement and education projects have been supported with more than 135,000€ of seed funding by Europlanet.

The Outreach Working Group coordinates activities, such as EPSC Goes Live for Schools, funding programmes, sharing of best practice and the annual prize for Public Engagement.

  1. Policy and Industry
Europlanet exhibition in the European Parliament. Credit: Europlanet.

Europlanet engagement with policy makers and industry aim to build collaborations and create synergies between cutting-edge science and the technological challenges of planetary science and exploration.

Europlanet has organised and participated in briefings, events, conference sessions (e.g. at EPSC) and other opportunities to engage policy makers in the European Parliament and the European Commission with planetary science, as well as engage with high-level representatives of ESA, NASA and other national and international space agencies. Organising events within the European Parliament has proved an effective platform to develop relationships with MEPs and other stakeholders, enabling the community to feed into discussions on future funding and policies relevant to planetary science.

Industry engagement activities have included organising technology foresight workshops, collaborations with space industry trade associations, developing contacts and networks within industry, participating in industry conferences and events, and convening industry and policy sessions at EPSC.

Europlanet’s distributed infrastructure offers industrial partners access to simulation and testing facilities for a range of environments that planetary and space missions may encounter through launch to their destination in orbit or on a planetary surface. By accessing Europlanet facilities, companies and SMEs can increase the value of their technology by increasing the Technology Readiness Level (TRL), understanding how instrumentation operates under realistic planetary conditions, or by identifying potential issues. Several of our RTI facilities are operated by commercial organisations.

  1. Collaborations

Collaborations stimulated through Europlanet, and involving its beneficiaries, have led to several successful proposals for new projects funded through the European Commission and national agencies. From the development of Machine Learning tools to mobilising researchers in Africa, these external projects act as multipliers for the impact of Europlanet in many different communities. 

  1. Expert Exchanges
Expert exchange to observing the DART impact in Kenya. Credit: The Travelling Telescope.

Europlanet’s Expert Exchange Programme aims to support the mobilisation of the planetary community to share expertise and best practice and to prepare new facilities and services for integration into Europlanet’s research infrastructure. The programme provides funding for short visits (up to one week) and over the last two decades, more than 200 expert exchanges have been supported.

Topics for visits have included training on the use of instrumentation, short scientific projects, improvements to facilities and the development of outreach collaborations. Evaluation of the visits show that bringing individuals together to exchange expertise often leading to synergies that would not happen otherwise, particularly for researchers from under-represented countries. The programme has also supported the professional development of early career scientists, helping them to prepare for careers outside academia. 

Find out more>>

  1. Funding and Awards
Tactile Mars exhibit from the Planets in Your Hand exhibition funded by Europlanet in 2017. Credit: Kosmas Gazeas.

Europlanet offers funding and bursaries to support the community in various ways. Each year, we provide over 100 bursaries for early career and researchers from under-represented countries to attend EPSC. The Committee Funding Scheme offers grants of up to 5000 € to support the scientific, community-building and outreach activities of our members.

Europlanet recognises the contributions of the planetary science community through a range of medals, prizes and other awards. The Europlanet Medals, launched in 2025, honour outstanding contributions from individuals of three different scientific career-stages to the subjects covered by the Europlanet Science Congress (EPSC). The Europlanet Prize for Public Engagement with Planetary Science is also awarded to individuals or groups who have developed innovative and socially impactful practices in planetary science communication and education. The EPSC Outstanding Poster Competition recognises the work of early career researchers at EPSC.  

  1. Impact
Fernando Gomez from Argentina participated in a Transnational Access visit to facilities at the Korean Basic Science Institute (KBSI). Credit: F Gomez.

Europlanet activities are evaluated against a framework of core indicators for assessing scientific, technological, education and training, economic, and social and societal impacts. Evaluation shows that the impact of activities to date have been particularly strong in the scientific, technological, education and training areas. 

 The 197 Transnational Access projects supported through the most-recent Europlanet 2024 RI project are expected to lead to over 300 publications and 400 conference presentations. Interviews and follow-up surveys show that over 90% of visitors are planning future collaborations with their host facility. In particular, early career researchers and students report that the TA programme provides them with opportunities – including collaboration and network-building – that would not otherwise have been available to them, thus accelerating their career development. 

Upgrades to facilities have provided increasing support for local infrastructure and associated employment, and there has been at least one SME company that was developed as a result of the TA programme. 

The new Europlanet Evaluation Unit now offers evaluation support and consultancy for external organisations that would like to develop an evaluation framework or implement an impact evaluation of their activities.

  1. Teamwork

Europlanet’s existence and continued activities would not be possible without the support of many individuals and organisations. In particular, we would like to thank our Executive Board, Committees and Working Groups for their huge investment of time and energy in making Europlanet a thriving and vibrant community. We thank our individual and organisational members for supporting us and participating in our activities. We are also indebted to the European Commission for funding over the years, as well as our project officers at the EC for their support, guidance and advice.

Issue 7 of the Europlanet Magazine is out now!

Issue 7 of the Europlanet Magazine is out now!

In this issue:

In Focus

round up of news from Europlanet and the planetary community, including:

The cover of Issue 7 of the Europlanet Magazine shows a researcher at the Makgadikgadi salt pans in Botswana kneeling to examine a sample. She is wearing overalls with high-vis strips and a sun hat. The sky is blue and the foreground is pale grey and dusty.
Cover of Issue 7 of the Europlanet Magazine.

News from Europlanet
• Beyond the Europlanet 2024 Research Infrastructure
• Berlin Welcomes EPSC2024 
• Early Career Events at EPSC2024
• Inspired By Other Worlds Arts Contest 2024
• EPSC-DPS 2025
• Incoming Chair of EPSC
• Juice Science Webinar Series
• EPEC Annual Week 2024
• Launch of ESFRI Landscape Analysis 2024
• SPIDER Spies Atmospheric Escape at Venus

Community News
• Ariel Data Challenge 2024
• Workshop at ATOMKI
• Tatra Workshop
• 56th Conference On Variable Star Research
• Europlanet Early Career Prize for Best Iberian Thesis
• Incoming Chair of Germany Hub
• Inspiring Women
• Ireland-UK Hub Meeting
• PLANETOEXOBIO 2024

Field Notes from a Planetary Expedition

Niamh Shaw reports on her experiences participating in an expedition into the remote, Mars-like salt pans of Botswana to study the subsurface geology.

Planetary Perspectives: Meet the New Europlanet Society Board

This edition of Planetary Perspectives highlights opportunities within space industry for early careers in an interview with Yoga Barrathwaj Raman Mohan (Blue Skies Space Ltd/Europlanet Industry Team).

Europlanet Telescope Network: Small-Scale Facilities Lead to Large-Scale Successes

As the Europlanet Telescope Network celebrates its fourth birthday, Gražina Tautvaišienė (Vilnius University, Lithuania), Guenter Kargl (Austrian Academy of Sciences, Austria) and Anita Heward (University of Kent, UK) reflect on the achievements to date.

Engaging With Embassies

Nigel Mason (Coordinator of Europlanet 2024 RI) gives guidance on how to approach embassies and an example of the outcome of a collaboration between embassies in the UK and Hungary.

Little Venus in the Middle of the Atlantic

Uli Köhler (DLR, Germany) reports on an expedition to Iceland that is helping to prepare for NASA and ESA missions to Venus at the beginning of the next decade.

The Future of Sample Return

Peter McArdle, Hans Huybrighs, J D Prasanna Deshapriya and Ottaviano Rüsch of the Europlanet Early Careers (EPEC) Future Research Working Group interview Enrica Bonato, who developed the sample return lab at at the German Aerospace Center (DLR) in Berlin.

SPIDER: Supporting Space Weather Studies Through the Solar System

Nicolas André (Institut de Recherche en Astrophysique et Planétologie, France) and Andrea Opitz (HUN-REN Wigner Research Centre for Physics, Hungary) describe how Europlanet’s SPIDER services are supporting planetary space weather studies and Solar System missions.

Beautiful But Not Hospitable – A Sensory Tour of the Solar System’s Planets

Boyko Ranguelov (Bulgarian Academy of Science and Arts, Bulgaria) considers how human senses might respond to objects in the Solar System.

What Do You Think a Comet Smells Like?

Anita Heward (Europlanet/University of Kent, UK) and Thibaut Roger (University of Bern, Switzerland) report on reactions to an unusual scent at the Swiss Comic Con.

Workshops for Global Collaboration

Barbara Cavalazzi (University of Bologna, Italy) reviews a series of workshops organised by Europlanet in Africa and South America.

Stories of Planetary Mapping

Riccardo Pozzobon and Matteo Massironi (University of Padova, Italy) explains how Europlanet’s GMAP activity has created infrastructure to support geological mappers around the world.

Commkit – Should You Augment or Virtualise Your Reality?

Thibaut Roger (University of Bern/NCCR PlanetS, Switzerland) examines how to incorporate VR and AR in your outreach and communication.

The Last Word – Europlanet Beyond 2024

Ann Carine Vandaele, President of the Europlanet Society, and Nigel Mason, Coordinator of the Europlanet 2024 Research Infrastructure (RI) reveal a new phase for Europlanet.

BepiColombo Spies Escaping Oxygen and Carbon in Unexplored Region of Venus’s Magnetosphere

BepiColombo Spies Escaping Oxygen and Carbon in Unexplored Region of Venus’s Magnetosphere

A fleeting visit of the ESA/JAXA BepiColombo mission to Venus has revealed surprising insights into how gases are stripped away from the upper layers of the planet’s atmosphere. 

Detections in a previously unexplored region of Venus’s magnetic environment show that carbon and oxygen are being accelerated to speeds where they can escape the planet’s gravitational pull.  The results have been published today in the journal Nature Astronomy.

Lina Hadid, CNRS researcher at the Plasma Physics Laboratory (LPP) and lead author of the study said: “This is the first time that positively charged carbon ions have been observed escaping from Venus’s atmosphere. These are heavy ions that are usually slow moving, so we are still trying to understand the mechanisms that are at play. It may be that an electrostatic ‘wind’ is lifting them away from the planet, or they could be accelerated through centrifugal processes.”

Unlike Earth, Venus does not generate an intrinsic magnetic field in its core. Nonetheless, a weak, comet-shaped ‘induced magnetosphere’ is created around the planet by the interaction of charged particles emitted by Sun (the solar wind) with electrically charged particles in Venus’s upper atmosphere. Draped around the magnetosphere is a region called the ‘magnetosheath’ where the solar wind is slowed and heated.

On 10 August 2021, BepiColombo passed by Venus to slow down and adjust course towards its final destination of Mercury. The spacecraft swooped up the long tail of Venus’s magnetosheath and emerged through the nose of the magnetic regions closest to the Sun. Over a 90-minute period of observations, BepiColombo’s instruments measured the number and mass of charged particles it encountered, capturing information about the chemical and physical processes driving atmospheric escape in the flank of the magnetosheath.

Early in its history, Venus had many similarities to Earth, including significant amounts of liquid water. Interactions with the solar wind have stripped away the water, leaving an atmosphere composed mainly of carbon dioxide and smaller amounts of nitrogen and other trace species. Previous missions, including NASA’s Pioneer Venus Orbiter and ESA’s Venus Express have made detailed studies of the type and quantity of molecules and charged particles that are lost into space. However, the missions’ orbital paths left some areas around Venus unexplored and many questions still unanswered.

Data for the study were obtained by BepiColombo’s Mass Spectrum Analyzer (MSA) and the Mercury Ion Analyzer (MIA) during the spacecraft’s second Venus flyby. The two sensors are part of the Mercury Plasma Particle Experiment (MPPE) instrument package, which is carried by Mio, the JAXA-led Mercury Magnetospheric Orbiter.

“Characterising the loss of heavy ions and understanding the escape mechanisms at Venus is crucial to understand how the planet’s atmosphere has evolved and how it has lost all its water,” said Dominique Delcourt, researcher at LPP and the Principal Investigator of the MSA instrument. 

Europlanet’s SPIDER space weather modelling tools enabled the researchers to track how the particles propagated through the Venusian magnetosheath.

“This result shows the unique results that can come out of measurements made during planetary flybys, where the spacecraft may move through regions generally unreachable by orbiting spacecraft,” said Nicolas André, of the Institut de Recherche en Astrophysique et Planétologie (IRAP) and lead of the SPIDER service.

A fleet of spacecraft will investigate Venus over the next decade, including ESA’s Envision mission, NASA’s VERITAS orbiter and DAVINCI probe, and India’s Shukrayaan orbiter. Collectively, these spacecraft will provide a comprehensive picture of the Venusian environment, from the magnetosheath, down through the atmosphere to the surface and interior.

“Recent results suggest that the atmospheric escape from Venus cannot fully explain the loss of its historical water content. This study is an important step to uncover the truth about the historical evolution of the Venusian atmosphere, and upcoming missions will help fill in many gaps,” added co-author, Moa Persson of the Swedish Institute of Space Physics.

Publication details:

Hadid et al. BepiColombo observations of oxygen and carbon ions in the flank of Venus induced magnetosphere. Nature Astronomy, 12 April 2024.

https://www.nature.com/articles/s41550-024-02247-2

DOI: 10.1038/s41550-024-02247-2

Images

Schematic view of planetary material escaping through Venus magnetosheath flank. The red line and arrow show the region and direction of observations by BepiColombo when the escaping ions (C+, O+, H+) were observed.
Schematic view of planetary material escaping through Venus magnetosheath flank. The red line and arrow show the region and direction of observations by BepiColombo when the escaping ions (C+, O+, H+) were observed. Credit: Thibaut Roger/Europlanet 2024 RI/Hadid et al.

Download image file as: JPG | PNG | PDF

Science Contacts

Dr Lina Hadid
Laboratoire de Physique des Plasmas (LPP)
Palaiseau
France
lina.hadid@lpp.polytechnique.fr

Dr Dominique Delcourt
Laboratoire de Physique des Plasmas (LPP)
Palaiseau
France
dominique.delcourt@lpp.polytechnique.fr

Dr Moa Persson
Institutet för Rymdfysik (IRF)
Swedish Institute of Space Physics
Uppsala
Sweden
moa.persson@irf.se

Dr Nicolas André
Institut de Recherche en Astrophysique et Planétologie (IRAP)
Toulouse
France
Nicolas.andre@irap.omp.eu

Media Contacts

Anita Heward
Press Officer
Europlanet 2024 Research Infrastructure (RI)
+44 7756 034243
aheward@europlanet-society.org

Thibaut Roger
Press Officer
Europlanet 2024 Research Infrastructure (RI)
thibaut.roger@science-elegance.com

Further Information

About ISAS/JAXA

In October 2003, the Japan Aerospace Exploration Agency (JAXA) was established as an independent administrative institution, integrating the Institute of Space and Astronautical Science (ISAS), the National Space Development Agency of Japan (NASDA) and the National Aerospace Laboratory of Japan (NAL). ISAS became one of four principal sections within the newly established organization. Its mission is to advance space science – scientific research conducted in outer space – in Japan, mainly by collaboration with universities. It also actively contributes to JAXA’s and Japan’s entire space development. 

ISAS’s new efforts and results in space science are published in Japan and shared with the international community, thus promoting JAXA’s status and enhancing Japan’s intellectual reputation in the world.

Web: https://www.isas.jaxa.jp/en/

Twitter: @ISAS_JAXA_EN

About Europlanet

Since 2005, Europlanet has provided Europe’s planetary science community with a platform to exchange ideas and personnel, share research tools, data and facilities, define key science goals for the future, and engage stakeholders, policy makers and European citizens with planetary science.

The Europlanet 2024 Research Infrastructure (RI) has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 871149 to provide access to state-of-the-art research facilities and a mechanism to coordinate Europe’s planetary science community. The project builds on a €2 million Framework 6 Coordination Action (EuroPlaNet), a €6 million Framework 7 Research Infrastructure (Europlanet RI) and a €10 million Horizon 2020 Research Infrastructure (Europlanet 2020 RI) funded by the European Commission. 

The Europlanet Society promotes the advancement of European planetary science and related fields for the benefit of the community and is open to individual and organisational members. The Society’s aims are:

  • To expand and support a diverse and inclusive planetary community across Europe through the activities of its 10 Regional Hubs
  • To build the profile of the sector through outreach, education and policy activities
  • To underpin the key role Europe plays in planetary science through developing links at a national and international level. 

Europlanet 2024 RI project website: www.europlanet-2024-ri.eu

Europlanet Society website: www.europlanet-society.org   

Follow on Twitter via @europlanetmedia

First BepiColombo Flyby of Mercury Finds Electron Rain Triggers X-Ray Auroras

First BepiColombo Flyby of Mercury Finds Electron Rain Triggers X-Ray Auroras

Europlanet 2024 Research Infrastructure (RI) Press Release

BepiColombo, the joint European Space Agency (ESA) and Japanese Aerospace Exploration Agency (JAXA) mission, has revealed how electrons raining down onto the surface of Mercury can trigger high-energy auroras. 

The mission, which has been enroute to the Solar System’s innermost planet since 2018, successfully carried out its first Mercury flyby on 1 October 2021. An international team of researchers analysed data from three of BepiColombo’s instruments during the encounter. The outcomes of this study have been published today in the scientific journal, Nature Communications.

Terrestrial auroras are generated by interactions between the solar wind, a stream of charged particles emitted by the Sun, and an electrically charged upper layer of Earth’s atmosphere, called the ionosphere. As Mercury only has a very thin atmosphere, called an exosphere, its auroras are generated by the solar wind interacting directly with the planet’s surface.

The BepiColombo mission consists of two spacecraft, the Mercury Planetary Orbiter (MPO) led by ESA, and the Mercury Magnetospheric Orbiter (MMO, named Mio after launch) led by JAXA, which are currently in a docked configuration for the seven-year cruise to the final orbit. During its first Mercury flyby, Bepicolombo swooped just 200 kilometres above the planet’s surface. The observations by plasma instruments onboard Mio enabled the first simultaneous observations of different kinds of charged particles from the solar wind in the vicinity of Mercury. 

Lead author, Sae Aizawa, of the Institut de Recherche en Astrophysique et Planétologie (IRAP), now at JAXA’s Institute of Space and Astronautical Science (ISAS) and University of Pisa, Italy, said: “For the first time, we have witnessed how electrons are accelerated in Mercury’s magnetosphere and precipitated onto the planet’s surface. While Mercury’s magnetosphere is much smaller than Earth’s and has a different structure and dynamics, we have confirmation that the mechanism that generates aurorae is the same throughout the Solar System.”

During the flyby, BepiColombo approached Mercury from the night side of the northern hemisphere and made its closest approach near the morning side of the southern hemisphere. It observed the magnetosphere on the daytime side of the southern hemisphere, and then passed out of the magnetosphere back into the solar wind. Its instruments successfully observed the structure and the boundaries of the magnetosphere, including the magnetopause and bow shock. The data also showed that the magnetosphere was in an unusually compressed state, most likely due to high pressure conditions in the solar wind. 

The acceleration of electrons appears to occur due to plasma processes in the dawn side of Mercury’s magnetosphere. The high energy electrons are transported from the tail region towards the planet, where they eventually rain down on the Mercury’s surface. Unimpeded by an atmosphere, they interact with material on the surface and cause X-rays to be emitted, resulting in an auroral glow. Although auroras had been observed before at Mercury by the NASA MESSENGER mission, the processes triggering the X-ray fluorescence by the surface had not been well understood and witnessed directly to date.

The study was carried out by a research team composed of the French Institut de Recherche en Astrophysique et Planétologie (IRAP), Kyoto University, ISAS, the Laboratoire de Physique des Plasmas (France), the Max Planck Institute for Solar System Research (Germany), the Swedish Institute of Space Physics, Osaka University, Kanazawa University, and Tokai University. The work was partially supported through Europlanet 2024 Research Infrastructure funding from the European Commission under grant agreement No 871149.

Publication Details

Aizawa et al. Direct evidence of substorm-related impulsive injections of electrons at Mercury. Nature Communications, 18 July, 2023.

DOI: 10.1038/s41467-023-39565-4

Link: https://www.nature.com/articles/s41467-023-39565-4

Image 

Artist’s representation of ESA/JAXA’s BepiColombo mission flying through precipitating electrons that can trigger X-rays auroras on the surface of Mercury.

Artist’s representation of the ESA/JAXA BepiColombo mission flying through precipitating electrons that can trigger X-ray auroras on the surface of Mercury. Credit: Creative Commons Attribution-ShareAlike 4.0 International (CC BY-SA 4.0) Thibaut Roger/Europlanet.

Science Contacts

Dr Sae Aizawa
Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS-UPS-CNES
Toulouse
France
also at ISAS, Japan and University of Pisa, Italy
sae.aizawa@irap.omp.eu

Dr Yuki Harada
Department of Geophysics, Graduate School of Science, Kyoto University
Kyoto
Japan
haraday@kugi.kyoto-u.ac.jp

Dr Moa Persson
Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS-UPS-CNES
Toulouse
France
also at University of Tokyo, Japan
moa.persson@irap.omp.eu

Dr Nicolas André
Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS-UPS-CNES
Toulouse
France
Nicolas.andre@irap.omp.eu

Dr Go Murakami
Institute of Space and Astronautical Science (ISAS)
Japan Aerospace Exploration Agency (JAXA)
Sagamihara
Japan
go@stp.isas.jaxa.jp

Media Contacts

Anita Heward
Press Officer
Europlanet 2024 Research Infrastructure (RI)
+44 7756 034243
aheward@europlanet-society.org

Further Information

The study used data mainly from Mio’s Mercury Electron Analyzer, MEA, complemented by data from the Mercury Ion Analyzer (MIA), and Energetic Neutral Atom (ENA) instruments, which are part of the Mercury Plasma Particle Experiment (MPPE). The MPPE consortium is led by the Principal Investigator, Yoshifumi Saito, from ISAS in Tokyo, Japan. https://mio.isas.jaxa.jp/en/mission/#mission_01

About ISAS/JAXA

In October 2003, the Japan Aerospace Exploration Agency (JAXA) was established as an independent administrative institution, integrating the Institute of Space and Astronautical Science (ISAS), the National Space Development Agency of Japan (NASDA) and the National Aerospace Laboratory of Japan (NAL). ISAS became one of four principal sections within the newly established organization. Its mission is to advance space science – scientific research conducted in outer space – in Japan, mainly by collaboration with universities. It also actively contributes to JAXA’s and Japan’s entire space development. 

ISAS’s new efforts and results in space science are published in Japan and shared with the international community, thus promoting JAXA’s status and enhancing Japan’s intellectual reputation in the world.

Web: https://www.isas.jaxa.jp/en/

Twitter: @ISAS_JAXA_EN

About Europlanet

Since 2005, Europlanet has provided Europe’s planetary science community with a platform to exchange ideas and personnel, share research tools, data and facilities, define key science goals for the future, and engage stakeholders, policy makers and European citizens with planetary science.

The Europlanet 2024 Research Infrastructure (RI) has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 871149 to provide access to state-of-the-art research facilities and a mechanism to coordinate Europe’s planetary science community. The project builds on a €2 million Framework 6 Coordination Action (EuroPlaNet), a €6 million Framework 7 Research Infrastructure (Europlanet RI) and a €10 million Horizon 2020 Research Infrastructure (Europlanet 2020 RI) funded by the European Commission. 

The Europlanet Society promotes the advancement of European planetary science and related fields for the benefit of the community and is open to individual and organisational members. The Society’s aims are:

  • To expand and support a diverse and inclusive planetary community across Europe through the activities of its 10 Regional Hubs
  • To build the profile of the sector through outreach, education and policy activities
  • To underpin the key role Europe plays in planetary science through developing links at a national and international level. 

Europlanet 2024 RI project website: www.europlanet-2024-ri.eu

Europlanet Society website: www.europlanet-society.org   

Follow on Twitter via @europlanetmedia

ERIM / EPEC Annual Week 2023 – Registration Now Open

Europlanet Research Infrastructure Meeting (ERIM)/Europlanet Early Career (EPEC) Annual Week 2023 – Registration Now Open

The first Europlanet Research Infrastructure Meeting (ERIM), co-hosted with the fifth Europlanet Early Career (EPEC) Annual Week, will take place from 19-23 June 2023 in hybrid format at the Hotel Sorea / Comenius University, Bratislava, Slovakia and online. 

Registration is free and accommodation and travel support is available for participants. 

Registration is now open.

Deadline for on-site registration: 19 May 2023

Deadline for virtual registration: 16 June 2023

About ERIM

ERIM is a new kind of meeting to support European planetary science and associated communities. The format of ERIM 2023 is a series of interactive workshops related to the activities of the Europlanet 2024 Research Infrastructure (RI) project, research infrastructures in general, and the Europlanet Society. The meeting will be co-hosted with EPEC Annual Week 2023, the training school for the Europlanet Early Career Network. 

How will it Work?

Workshops will be organised under a series of programme tracks. You can dip in and out of programme tracks, workshops and even sessions during the week. The aim is to make new connections, brainstorm ideas, develop synergies, increase opportunities for collaboration and help us build a strong, thriving, sustainable community for planetary science in Europe.

You don’t have to be a member of the Europlanet Society or the Europlanet 2024 RI project to participate in ERIM. We are looking for new people to engage with Europlanet, so everyone is welcome. However, we will be offering free accommodation and travel grants to a limited number (~150) of participants. If we are over-subscribed in requests for support, priority will be given to Europlanet Society members. (Find out about other benefits of joining the Europlanet Society).

Programme 

Many different topics will be covered within the ERIM programme tracks and workshops, including:

For full details of the meeting and registration, see: https://www.europlanet.org/erim2023/

If you have any questions, contact us.

We hope to see you in Bratislava!

The ERIM 2023 Organising Committee

SPIDER in the News

Europlanet 2024 RI logo

SPIDER in the News

Europlanet’s SPIDER (Sun Planet Interactions Digital Environment on Request) virtual access service has been in the news recently in two studies using data from ESA missions at Venus and Mars.

SPIDER provides services and databases to support researchers modelling planetary environments and solar wind interactions.

A paper published in Nature Communications, led by Dr Moa Persson of the University of Tokyo describes how the convergence of BepiColombo and Solar Orbiter at Venus in August 2021 has given a unique insight into how the planet is able to retain its thick atmosphere without the protection of a global magnetic field. 

In this video, Moa explains how SPIDER has been used to support observations by BepiColombo and Solar Orbiter of Venus’s induced magnetosphere and magnetosheath. 

Co-author of the study, Sae Aizawa of ISAS/JAXA, explains how the solar wind interacts with magnetic fields and atmospheres at different planets in our Solar System.

Back in December, a second paper led by Yoshifumi Futaana of the Swedish Institute of Space Physics, showed how background radiation counts detected by ESA’s long-serving twin missions, Mars Express and Venus Express, revealed the relationship between intensity of high-energy cosmic rays and the influence of the Sun’s activity across our inner Solar System. The databases of the background radiation counts extracted for the study ere published and can be accessed through SPIDER. In this video, he explains more about his approach to his reasearch.

BepiColombo and Solar Orbiter compare notes at Venus

BepiColombo and Solar Orbiter compare notes at Venus 

Europlanet 2024 RI/ISAS/JAXA Press Release
Thursday, 26 January 2023

The convergence of two spacecraft at Venus in August 2021 has given a unique insight into how the planet is able to retain its thick atmosphere without the protection of a global magnetic field. 

The ESA/JAXA BepiColombo mission, enroute to study Mercury, and the ESA/NASA Solar Orbiter, which is observing the Sun from different perspectives, are both using a number of gravity-assists from Venus to change their trajectories and guide them on their way.  On 9-10 August 2021, the missions flew past Venus within a day of each other, sending back observations synergistically captured from eight sensors and two vantage points in space. The results have been published in Nature Communications.

Unlike Earth, Venus does not generate an intrinsic magnetic field in its core. Nonetheless, a weak, comet-shaped ‘induced magnetosphere’ is created around the planet by the interaction of the solar wind – a stream of charged particles emitted by the Sun – with electrically charged particles in Venus’s upper atmosphere. Around this magnetic bubble, the solar wind is slowed, heated and deflected like the wake of a boat in a region called ‘magnetosheath’.

During the flyby, BepiColombo swooped along the long tail of the magnetosheath and emerged through the blunt nose of the magnetic regions closest to the Sun. Meanwhile, Solar Orbiter captured a peaceful solar wind from its location upfront of Venus.

“These dual sets of observations are particularly valuable because the solar wind conditions experienced by Solar Orbiter were very stable. This meant that BepiColombo had a perfect view of the different regions within the magnetosheath and magnetosphere, undisturbed by fluctuations from solar activity,” said lead-author Moa Persson of the University of Tokyo in Kashiwa, Japan, who was funded to carry out the study by the European Commission through the Europlanet 2024 Research Infrastructure (RI) project.

BepiColombo’s flyby was a rare opportunity to investigate the ‘stagnation region’, an area at the nose of the magnetosphere where some of the largest effects of the interaction between Venus and the solar wind are observed. The data gathered gave the first experimental evidence that charged particles in this region are slowed significantly by the interactions between the solar wind and Venus, and that the zone extends to an unexpectedly large distance of 1,900 kilometres above the planet’s surface.

The observations also showed that the induced magnetosphere provides a stable barrier that protects the atmosphere of Venus from being eroded by the solar wind. This protection remains robust even during solar minimum, when lower ultraviolet emissions from the Sun reduce the strength of the currents that generate the induced magnetosphere. The finding, which is contrary to previous predictions, sheds new light on the connection between magnetic fields and atmospheric loss due to the solar wind.

‘The effectiveness of an induced magnetosphere in helping a planet retain its atmosphere has implications for understanding the habitability of exoplanets without internally-generated magnetic fields,” said co-author Sae Aizawa of JAXA’s Institute of Space and Astronautical Science (ISAS).

BepiColombo comprises a pair of spacecraft, Mio, the JAXA-led Mercury Magnetospheric Orbiter, and MPO, the ESA-led Mercury Planetary Orbiter, which have been stacked together for the journey to Mercury. The study combined data from Mio’s four particle sensors, the magnetometer and another particle instrument on MPO, and the magnetometer and solar wind analyser on Solar Orbiter. Europlanet’s SPIDER space weather modelling tools enabled the researchers to track in detail how features in the solar wind observed by Solar Orbiter were affected as they propagated towards BepiColombo through the venusian magnetosheath.

“The important results of this study demonstrate how turning sensors on during planetary flybys and cruise phases can lead to unique science,” said co-author Nicolas Andre, the coordinator of the Europlanet SPIDER service at the Institut de Recherche en Astrophysique et Planétologie (IRAP) in Toulouse, France.

Publication details:

Persson et al. BepiColombo mission confirms stagnation region of Venus and reveals its large extent. Nature Communications vol 13, 7743 (2022). https://doi.org/10.1038/s41467-022-35061-3 

Further information

Science and Housekeeping data for the study were obtained from eight sensors on three spacecraft:

  • Mio
    • Mercury Electron Analyzer (MEA)
    • Mercury Ion Analyzer (MIA)
    • Mass Spectrum Analyzer (MSA) 
    • Energetic Neutral Atom (ENA)
  • MPO 
    • Magnetometer (MAG)
    • Miniature Ion Precipitation Analyzer (MIPA) 
  • Solar Orbiter 
    • Magnetometer (MAG)
    • Proton Alpha Spectrometer (PAS)

Image

The convergence of BepiColombo and Solar Orbiter spacecraft at Venus in August 2021 was a rare opportunity to investigate the ‘stagnation region’, an area of the venusian magnetosphere where some of the largest effects of the interaction between Venus and the solar wind are observed. Credit: CC BY-Nc-SA 4.0 – Thibaut Roger/Europlanet 2024 RI

The convergence of BepiColombo and Solar Orbiter spacecraft at Venus in August 2021 was a rare opportunity to investigate the ‘stagnation region’, an area of the venusian magnetosphere where some of the largest effects of the interaction between Venus and the solar wind are observed.

Download full resolution image as JPG, PNG or PDF.

Video

Dr Moa Persson describes the observations by BepiColombo and Solar Orbiter of Venus’s induced magnetosphere and magnetosheath.

Dr Sae Aizawa explains how the solar wind interacts with magnetic fields and atmospheres at different planets in our Solar System.

Science Contacts

Dr Moa Persson
The University of Tokyo
Kashiwa
Japan
moa.persson@irap.omp.eu

Dr Sae Aizawa
Institute of Space and Astronautical Science (ISAS)
Japan Aerospace Exploration Agency (JAXA)
Sagamihara
Japan
sae.aizawa@irap.omp.eu

Dr Go Murakami
Institute of Space and Astronautical Science (ISAS)
Japan Aerospace Exploration Agency (JAXA)
Sagamihara
Japan
go@stp.isas.jaxa.jp

Dr Nicolas André
Institut de Recherche en Astrophysique et Planétologie (IRAP)
Toulouse
France
Nicolas.andre@irap.omp.eu

Media Contacts

Anita Heward
Press Officer
Europlanet 2024 Research Infrastructure (RI)
+44 7756 034243
aheward@europlanet-society.org

Further Information

About ISAS/JAXA

In October 2003, the Japan Aerospace Exploration Agency (JAXA) was established as an independent administrative institution, integrating the Institute of Space and Astronautical Science (ISAS), the National Space Development Agency of Japan (NASDA) and the National Aerospace Laboratory of Japan (NAL). ISAS became one of four principal sections within the newly established organization. Its mission is to advance space science – scientific research conducted in outer space – in Japan, mainly by collaboration with universities. It also actively contributes to JAXA’s and Japan’s entire space development. 

ISAS’s new efforts and results in space science are published in Japan and shared with the international community, thus promoting JAXA’s status and enhancing Japan’s intellectual reputation in the world.

Web: https://www.isas.jaxa.jp/en/

Twitter: @ISAS_JAXA_EN

About Europlanet

Since 2005, Europlanet has provided Europe’s planetary science community with a platform to exchange ideas and personnel, share research tools, data and facilities, define key science goals for the future, and engage stakeholders, policy makers and European citizens with planetary science.

The Europlanet 2024 Research Infrastructure (RI) has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 871149 to provide access to state-of-the-art research facilities and a mechanism to coordinate Europe’s planetary science community. The project builds on a €2 million Framework 6 Coordination Action (EuroPlaNet), a €6 million Framework 7 Research Infrastructure (Europlanet RI) and a €10 million Horizon 2020 Research Infrastructure (Europlanet 2020 RI) funded by the European Commission. 

The Europlanet Society promotes the advancement of European planetary science and related fields for the benefit of the community and is open to individual and organisational members. The Society’s aims are:

  • To expand and support a diverse and inclusive planetary community across Europe through the activities of its 10 Regional Hubs
  • To build the profile of the sector through outreach, education and policy activities
  • To underpin the key role Europe plays in planetary science through developing links at a national and international level. 

Europlanet 2024 RI project website: www.europlanet-2024-ri.eu

Europlanet Society website: www.europlanet-society.org   

Follow on Twitter via @europlanetmedia

Cosmic Ray Counts Hidden in Spacecraft Data Highlight Influence of Solar Cycle at Mars and Venus

Cosmic Ray Counts Hidden in Spacecraft Data Highlight Influence of Solar Cycle at Mars and Venus

Europlanet and Swedish Institute of Space Physics Joint Press Release

EMBARGOED for 11:00 UTC / noon CET on Monday, 5 December 2022

Measurements by ESA’s long-serving twin missions, Mars Express and Venus Express, have captured the dance between the intensity of high-energy cosmic rays and the influence of the Sun’s activity across our inner Solar System. 

A comparison of data from the ASPERA plasma sensor, an instrument carried by both spacecraft, with the number of sunspots visible on the surface of the Sun shows how cosmic ray counts are suppressed during peaks of activity in the 11-year solar cycle. The international study, led by Dr Yoshifumi Futaana of the Swedish Institute of Space Physics, has been published today in the Astrophysical Journal.

Cosmic rays are particles travelling at almost the speed of light that originate outside our Solar System. They are a dangerous form of high energy radiation that can cause electronic failures in spacecraft and damage the DNA of humans in space.

As well as the decadal-long relationship with the solar cycle, the researchers also looked at how cosmic ray detections varied over the short timescales of an orbit. Surprisingly, they found that the area protected from cosmic rays behind Mars is more than 100 kilometres wider than the planet’s actual radius. The cause of why this blocked area should be so large is not yet clear.

“The study shows the range of valuable insights that can be derived from what is actually background count information collected by the ASPERA instruments. Understanding the various relationships between cosmic rays and the solar cycle, the atmospheres of planets and the performance of spacecraft instrumentation is very important for future robotic missions and human exploration,” said Dr Futaana.

Launched in 2003, Mars Express remains in service around the Red Planet, while Venus Express operated from 2006 until 2014. The researchers compared the 17-year dataset from Mars and eight-year dataset from Venus with Earth-based cosmic ray measurements from the Thule neutron monitor in Greenland. Scientists took median value of cosmic ray counts over three-month periods to minimise the influence of sporadic solar activity, such as flares or coronal mass ejections. The databases of background radiation counts extracted for the study have been published and can be accessed through the Europlanet SPIDER planetary space weather service (http://spider-europlanet.irap.omp.eu/).

All the datasets showed a decrease in the number of cosmic ray detections as the peak in activity for Solar Cycle 24 was reached. In particular, the Mars Express data and the observations from Earth showed very similar features. However, there was an apparent lag of around nine months between the maximum number of sunspots and the minimum in cosmic ray detections at Mars.

“Previous studies have suggested that there is a delay of several months between solar activity and the behaviour of cosmic rays at the Earth and at Mars. Our results appear to confirm this and also provide further evidence that Solar Cycle 24 was a bit unusual, perhaps due to the long solar minimum between Cycle 23 and 24, or the relatively low activity during Cycle 24,” said Dr Futaana.

The analysis of the Venus Express data has been complicated by changes in the way onboard processing was carried out from 2010 onwards. In addition, while the ASPERA instruments carried by Mars Express and Venus Express were based on a common design, they were each tailored to the very different planetary environments in which they operated. This means that a direct comparison of cosmic ray fluxes at Mars and Venus is not possible using the available datasets. 

“The use of background counts to study the interaction of cosmic rays and high energy particles with planetary missions is relatively new. However, obtaining this information shows potential as a powerful tool, for example, in protecting the upcoming JUpiter Icy moon Explorer (JUICE) mission of the European Space Agency, which will explore the harsh environment around Jupiter’s icy moons,” said Nicolas Andre of the Institut de Recherche en Astrophysique et Planétologie (IRAP) in Toulouse, France, coordinator of the Europlanet SPIDER service and co-author of this study.

Publication details

Futaana et al. Galactic Cosmic Rays at Mars and Venus: Temporal Variations from Hours to Decades Measured as the Background Signal of Onboard Micro-Channel Plates. The Astrophysical Journal. 2022. DOI: 10.3847/1538-4357/ac9a49

Images

Artists’ impressions of Mars Express (left) and Venus Express (right). Credit: ESA/D Ducros/AOES Medialab.

Artists' impressions of Mars Express (left) and Venus Express (right).
Artists’ impressions of Mars Express (left) and Venus Express (right). Credit: ESA/D Ducros/AOES Medialab.

Artistic representation of galactic cosmic rays. Credit: M Eriksson/IRF.

Artistic representation of galactic cosmic rays.
Artistic representation of galactic cosmic rays. Credit: M Eriksson/IRF

Video

Interview with Dr Yoshifumi Futaana. https://youtu.be/5ZdwAEivOtY

Science Contacts

Dr Yoshifumi Futaana
Swedish Institute of Space Physics
Kiruna
Sweden
futaana@irf.se

Dr Nicolas André
Institut de Recherche en Astrophysique et Planétologie (IRAP)/OMP
Toulouse
France
nicolas.andre@irap.omp.eu

Media Contacts

Martin Eriksson
Information officer
Swedish Institute of Space Physics
Kiruna
+46 72 581 33 33
martin.eriksson@irf.se

Anita Heward
Press Officer
Europlanet 2024 Research Infrastructure (RI)
+44 7756 034243
aheward@europlanet-society.org

Further Information

About IRF

The Swedish Institute of Space Physics (IRF) is a governmental research institute under the Ministry of Education. IRF conducts basic research and postgraduate education in space physics, space technology, and atmospheric physics.

IRF has over 60 years of experience in developing instruments for space research projects and participates in several major international collaborative projects using satellites and ground-based equipment.

About Europlanet

Since 2005, Europlanet has provided Europe’s planetary science community with a platform to exchange ideas and personnel, share research tools, data and facilities, define key science goals for the future, and engage stakeholders, policy makers and European citizens with planetary science.

The Europlanet 2024 Research Infrastructure (RI) has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 871149 to provide access to state-of-the-art research facilities and a mechanism to coordinate Europe’s planetary science community. The project builds on a €2 million Framework 6 Coordination Action (EuroPlaNet), a €6 million Framework 7 Research Infrastructure (Europlanet RI) and a €10 million Horizon 2020 Research Infrastructure (Europlanet 2020 RI) funded by the European Commission. 

The Europlanet Society promotes the advancement of European planetary science and related fields for the benefit of the community and is open to individual and organisational members. The Society’s aims are:

  • To expand and support a diverse and inclusive planetary community across Europe through the activities of its 10 Regional Hubs
  • To build the profile of the sector through outreach, education and policy activities
  • To underpin the key role Europe plays in planetary science through developing links at a national and international level. 

Europlanet 2024 RI project website: www.europlanet-2024-ri.eu

Europlanet Society website: www.europlanet-society.org   

Follow on Twitter via @europlanetmedia