This open workshop will bring together planetary scientists from multiple disciplines with a shared interest in future missions to the Ice Giants. We will review recent developments towards this goal, particularly within NASA and ESA, and discuss strategies for continued progress, including setting the scene for the Ice Giant Systems Workshop in London in January 2020.

Please note: We request to avoid any outer planet sessions, and to avoid any proposed meetings of the International Outer Planet Watch, to maximise attendance. Tuesday/Thursday slots, also 17:15+, are also suitable.

Public information:
This open workshop will bring together planetary scientists from multiple disciplines with a shared interest in future missions to the Ice Giants. We will review recent developments towards this goal, particularly within NASA and ESA, and discuss strategies for continued progress, including setting the scene for the Ice Giant Systems Workshop in London in January 2020. For further details, and to suggest brief contributions, please email leigh.fletcher@le.ac.uk.

SPICE is an information system that uses ancillary data to provide Solar System geometry information to scientists and engineers for planetary missions in order to plan and analyze scientific observations from space-born instruments. SPICE is developed and maintained by the Navigation and Ancillary Information Facility (NAIF) team of the Jet Propulsion Laboratory (NASA). NAIF and the ESA SPICE Service (ESS) provide SPICE Training Courses on a yearly basis, these are three-day courses which are hosted either nearby Pasadena (California, USA) or nearby Madrid (Spain).

ESS offers a training session on SPICE aimed at scientists and engineers who want to be introduced to SPICE or who might be considering attending a complete SPICE Training.

During this course a brief introduction to SPICE will be provided and it will be followed by a practical hands-on lesson of a SPICE application based on a remote sensing observation scenario. We will also go through WebGeocalc, SPICE-Enhanced Cosmographia 3D Visualization Software and some Python packages.

The envisaged agenda for the Seminar will be:

1-Introducing SPICE the cool way: Cosmographia.
2-Cosmographia & WebGeocalc demo
3-Brief introduction to ESS and SPICE Kernels 4-Questions & Answers 5-Remote Sensing Hands-on lesson 6-Questions & Answers and close-out

Training Material: All the training material will be provided with GitHub, using the ESS account: https://github.com/esaSPICEservice/ material will be provided as reference documents and with Jupyter Notebooks.

The aim of the splinter session is to make the attendees familiar with and as autonomous as possible with Rosetta archive data, so that they can quickly carry out their own cometary science studies. The target audience is cometary and small body scientists, as well as members of the broader planetary community to make them aware of the data products available in the Rosetta archive, to promote usage of that data. The workshop will begin with a short presentation of the ESA Planetary Science Archive as a whole and on the Rosetta archive in particular. This will be followed by presentations from a few select instrument teams who will give a brief overview of their archive data, to provide instrument level insights into data access. Following this, we aim to have a more interactive section which will focus on a published event which will allow attendees to gain experience in interacting with the archive data.
NOTE: We have selected Tuesday around lunchtime, but we would like to avoid running parallel with any small body session if possible, due to that limiting availability of Rosetta scientists to present their archive data access.

The Large Synoptic Survey Telescope (LSST; http://lsst.org) is an 8-meter, wide-field, ground-based survey program that will survey half the sky every few nights in six optical bands from 320 to 1050 nm. The LSST telescope is currently being constructed at Cerro Pachón, Chile, with first light expected in 2020 and start of survey operations in late 2022.

The LSST is slated to make a significant contribution to the study of the Solar System, delivering over a billion highly precise observations of millions of Solar System objects (5mmag photometry and 10mas astrometry, per observation, at the bright end). Current estimates show yields ranging from ~100,000 new discoveries of nearby NEOs, to 5.5 million for the main belt, and ~40,000 for KBO populations. The majority of these objects will receive hundreds of observations in multiple bandpasses.

This dataset presents tremendous opportunities for Solar System science. This meeting will overview the science possibilities, report on project status and expected data products, and discuss how to get involved in preparations for science with LSST.

We are looking forward to sharing our annual discussion of professional development topics with the EPSC/DPS community. All are welcome! The main topic will be announced on the registration page. Pre-registration at http://bit.ly/DPS_WIPS_2019 is recommended due to space limitations. Contact Kelsi.Singer@gmail.com with questions.

Recent results ranging from the Pluto system, the Saturn system, other locations beyond ~5 AU, all the way to Mercury in the inner Solar System, and nearly all points in between, raise questions abut the state of carbon in the Solar System: how do carbonaceous compounds become weathered in response to thermal processes and irradiation? How do we recognize carbon compounds and their various weathering products? The synthesis of these results improves our scientific understanding of the role of carbon in the Solar System, how it evolves and how to recognize it. Analyses of samples from the carbonaceous near-Earth asteroids 162173 Ryugu and 101955 Bennu will provide context for the presence of carbon. In this workshop, please come prepared to discuss observational, laboratory and modeling work related to carbon and carbonaceous species on Solar System bodies.

The International Outer Planets Watch (IOPW) Atmospheres Node hosts an annual workshop to discuss on Jupiter Saturn and Icy Giants observations over the last year and plan further observations for the upcoming 2020. As usual the workshop will also host short presentations of scientific themes not accomodated on the oral and poster sessions. The list of topics includes: Jupiter observations and Juno observational support. Saturn observations from the ground. Observations of Uranus and Neptune. Model simulations of atmospheric dynamics of Jupiter/Saturn. If you are willing to provide some topics for presentations/discussions over the workshop please e-mail Ricardo Hueso (ricardo.hueso@ehu.eus) with a title and an estimation of time required for your presentation. Discussion on current amateur observations of the Giant planets from Jupiter to Neptune are also welcomed.

ARIEL, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was selected as the fourth medium-class mission in ESA’s Cosmic Vision programme. During its 4-year mission, ARIEL will study what exoplanets are made of, how they formed and how they evolve, by surveying a diverse sample of about 1000 extrasolar planets, simultaneously in visible and infrared wavelengths. It is the first mission dedicated to measuring the chemical composition and thermal structures of hundreds of transiting exoplanets, enabling planetary science far beyond the boundaries of the Solar System.

ARIEL has launched in April 2019 a global competition series to find innovative solutions for the interpretation and analysis of exoplanet data (https://ariel-datachallenge.azurewebsites.net).

The first ARIEL Data Challenge invites professional and amateur data scientists around the world to use Machine Learning (ML) to remove noise from exoplanet observations caused by star-spots and by instrumentation.
A second ARIEL Data Challenge that focuses on the retrieval of spectra from simulations of cloudy and cloud-free super-Earth and hot-Jupiter data was also launched in April. A further data analysis challenge to create pipelines for faster, more effective processing of the raw data gathered by the mission will be launched in June at the EWASS conference in Lyon.

Outcomes from all three ARIEL Data Challenges will be discussed in a dedicated splinter at the EPSC-DPS Joint Meeting 2019.

NEWTON is an international research project funded from EU H2020 programme funds. The project NEW portable multi-sensor scienTific instrument for non-invasive ON-site characterization of rock from planetary surface and sub-surfaces (NEWTON) is developing a new portable and compact multi-sensor instrument for ground breaking high resolution magnetic characterization of planetary surfaces and sub-surfaces through the combination of complex susceptibility and vector measurements, being the Moon and Mars the main scenarios of application of the instrument. This non-invasive technology provides unique scientific information on some of the main objectives related to the Solar System exploration roadmap as the intense magnetic crustal anomalies of Mars and the strongly discussed formation of its moons.
This workshop will look at latest state-of-the-art regarding in-situ instrumentation for planetary surface characterization, with particular focus on magnetometric devices and their application to planetary exploration. In addition to this, NEWTON multi-sensor instrument will be exhibited during the session as well as the results obtained from the field campaigns performed with NEWTON instrumentation.

Public information:
NEWTON is an international research Project funded from EU H2020 programme funds which aims at developing a new portable and compact multi-sensor instrument for high resolution magnetic characterisation of planetary surfaces, through the combination of complex susceptibility and vector measurements, being the Moon and Mars the main scenarios of application of the instrument. More information can be found in NEWTON web-page: http://www.h2020-newton.eu

NEWTON workshop will look at latest state-of-the-art regarding magnetic in-situ instrumentation for planetary surface characterization and their application to planetary exploration. During the session, NEWTON instrument, based on the combination of complex susceptibility and magnetic field vector measurement, will be presented, as well as the main technical innovations gained from it. In addition to this, the workshop will give the opportunity to examine the exploitation opportunities of magnetometric instrumentation and its application to the future space exploration programs. The results gained from the field campaigns performed with NEWTON instrumentation will be exposed and the innovations provided by this new technology for the exploration of the Moon and Martian System will be also discussed.

The Space Studies Board (SSB) of the U.S. National Academy of Sciences, Engineering, and Medicine, and the Planetary Science Division (PSD) of NASA’s Science Mission Directorate invites participants in 2019 DPS/EPSC meeting to a discussion on the current state of planning for the next decadal survey in planetary science, scheduled to be initiated in the first quarter of 2020.

The decadal survey is the process through which the U.S. planetary science community identifies the key scientific issues ripe for progress in the coming decade and provides recommendations as to how these issues may be addressed by spacecraft missions, supporting ground based activities and other initiatives.

Lori S. Glaze (PSD) and David H. Smith (SSB) will provide an overview of the progress made towards preparing for and organizing the survey, along with an updated schedule for its implementation.

Community involvement is an essential feature of all phases of the decadal process and a critical component to the success of the survey. The SSB and PSD welcomes all community input on matters facing the next survey, which include (but are not limited to) the technical and programmatic scope, structure, the cost and technical evaluation process, the role of early-career scientists, and the international context.

The purpose of the Outer Planets Assessment Group (OPAG) Town Hall is to update the community on OPAG activities and get community input for upcoming activities, especially as they pertain to the run up for the next Decadal Survey.

MINERVA (see https://meetingorganizer.copernicus.org/EPSC-DPS2019/EPSC-DPS2019-496.pdf being presented in MIT9, Mon Sept 16th, 13:45-14:00 in Room Moon) provides a 3D data base, an interactive 3D viewer with GIS functionality and a visual analytics platform that helps find correlations between data coming from different instruments to discover new modes of scientific exploitation. We demonstrate the system with emphasis on data presentation and interaction of five instruments of the full MSL mission. You will see how to find out new correlations between instrument data, associate across instrument and telemetry data (spatially, temporally and in the multitemporal space of meta data), and find new and astonishing patterns in the data. All is visualized in real-time, based on the multiscale 3D vision data products from HiRISE and Mastcam.

Public information:
MINERVA (see https://meetingorganizer.copernicus.org/EPSC-DPS2019/EPSC-DPS2019-496.pdf being presented in MIT9, Mon Sept 16th, 13:45-14:00 in Room Moon) provides a 3D data base, an interactive 3D viewer with GIS functionality and a visual analytics platform that helps find correlations between data coming from different instruments to discover new modes of scientific exploitation. We demonstrate the system with emphasis on data presentation and interaction of five instruments of the full MSL mission. You will see how to find out new correlations between instrument data, associate across instrument and telemetry data (spatially, temporally and in the multitemporal space of meta data), and find new and astonishing patterns in the data. All is visualized in real-time, based on the multiscale 3D vision data products from HiRISE and Mastcam.

The splinter is intended to be a participative workshop with hackathons and collaborative planetary data handling and analysis components using state-of-the-art community-driven open source tools. Both junior and senior scientists willing to share expertise, tools, science use cases and issues are welcome.

Planets in a room is a DIY low-cost kit you can use to build a small spherical projector to easily see, show and teach planetary science. Planets in a room was developed by the italian association Speak Science in collaboration with INAF and Roma Tre University. The project was funded by Europlanet Outreach Funding Scheme and is now distributed online at www.planetsinaroom.net

Planets in a room is also a community of people who love space and science and who choose to build and use this system to make their passion grow, involving new generations. If you are a researcher, a teacher, an amateur astronomer, a student, and want to enter the community, in this workshop you will learn how to build, use and produce original content for Planets in a Room.

The James Webb Space Telescope (JWST) will have unprecedented sensitivity and angular resolution, and will be the next premier space-based facility for near- and mid-infrared astronomy (0.6-28.5 micron). The 6.5-meter telescope will be equipped with four state-of-the-art instruments which include imaging, spectroscopy, and coronagraphy capabilities. These instruments, along with the telescope’s moving target capabilities, will enable remarkable infrared studies of Solar System objects. JWST is scheduled for launch in March 2021 and is an international collaboration between NASA, the European Space Agency (ESA), and the Canadian Space Agency (CSA).
The first call for General Observer (GO) proposals will be released in January 2020, with a submission deadline on 1 May 2020. This will be the last proposal workshop prior to Cycle 1 offered at the annual DPS and EPSC meetings, so we encourage all future observers to participate.
In this workshop, we will provide a brief status update on the observatory as well as commissioning plans relevant to Solar System observations, will review the timeline for proposals, and will provide details about the Guaranteed Time Observer (GTO) and Early Release Science (ERS) programs for Solar System science. We will also give a detailed orientation to the proposal planning system, including demonstrations o f the Astronomer’s Proposal Tool (APT) and the Exposure Time Calculator (ETC) relevant for Solar System proposals.

A short workshop with Q&A on the editorial and review processes in AGU journals by two Editors. We will discuss the scopes of the different journals, give a reminder on the requirements, present examples of best practices in preparing a manuscript and reviews, and answer any questions the audience might have.

Open meeting of the RMS Node's Advisory Council and user community. Discuss progress, solicit community inputs and priorities.

The James Webb Space Telescope (JWST) is an infrared-optimized telescope to be placed at the Earth-Sun Lagrange 2 point. It is scheduled for launch in 2021, and will have a robust suite of astronomical instrumentation (imaging and spectroscopy) operating from 0.6-28.5 microns. The first call for General Observer (GO) proposals will be released in January 2020 with a deadline of 1 May 2020. At this Town Hall, we will provide the community with an overview of the observatory, instrumentation, and specific details for solar system observations. Additionally, we will provide a timeline with upcoming deadlines, proposal workshops, updates on scattered light and brightness limits, and where to find more information and how to use the observatory tools/documentation. Our goal is to fully engage the Solar System community to provide them with the tools they need to begin planning their observations with JWST.

When should we start teaching astronomy to children? Is it useful to start in kindergarten or primary school? Do children make use of such knowledge later? Does this knowledge have an effect on children?
Are natural science hands-on sessions better than films on TV or cartoons? What happens if all children want to be astronomers or astronauts? Could we use astronomy as a motivation factor when teaching natural sciences?

We will have a lively discussion and a guest sharing her experiences with small children. FREE COPIES of a book about the topic will be distributed for those interested.
Pre-registration is recommended due to space limitations, at dosa.melinda@wigner.mta.hu.
All are welcome :)

As a speaker it is recommended to register before the start of EPSC, latest one day before the event. To do so please send an e-mail with your name, your institution, and the title of your presentation to noah.jaeggi@space.unibe.ch or get in touch with Noah (Jäggi) at the EPEC icebreaker event on Sunday or during the conference

Public information:
The Europlanet Early Career Network presents the 2019 EPEC Science Flash.

Present your work in a fun and original way! You have exactly 180 seconds of time supported by one slide and/or small additional equipment.
The three best presentations will receive a prize!

Everybody is welcome to join, listen and rate the entertaining presentations.
As a speaker it is recommended to register before the start of EPSC, latest one day before the event. To do so please send an e-mail with your name, your institution, and the title of your presentation to noah.jaeggi@space.unibe.ch or get in touch with Noah (Jäggi) at the EPEC icebreaker event on Sunday or during the conference.

This workshop will introduce the Python module sbpy, an astropy (http://astropy.org) affiliated package for small-body planetary astronomy. sbpy's functionality will include analysis tools and model implementations for photometry, spectroscopy, cometary activity, thermal emission from atmosphere-less bodies, and small-body light-curves; it furthermore provides tools for data archive access, comet coma image enhancement, and small-body observation planning. Information on the package and its installation can be found at http://sbpy.org. The workshop will introduce some of the currently available features and enable the discussion of future functionality. Everybody who is interested in contributing to, testing, or simply using sbpy is invited. sbpy is supported by NASA PDART Grant No. 80NSSC18K0987.

Public information:
This workshop will introduce the Python module sbpy, an astropy (http://astropy.org) affiliated package for small-body planetary astronomy. sbpy's functionality will include analysis tools and model implementations for photometry, spectroscopy, cometary activity, thermal emission from atmosphere-less bodies, and small-body light-curves; it furthermore provides tools for data archive access, comet coma image enhancement, and small-body observation planning. Information on the package and its installation can be found at http://sbpy.org. The workshop will introduce the currently available features and provide guidance in how to use these features in a short hackathon. Everybody who is interested in contributing to, testing, or simply using sbpy is invited. sbpy is supported by NASA PDART Grant No. 80NSSC18K0987.

Please join us for discussion about harassment, bias, and what we can do to help change the culture. This meeting is specifically intended to help those who identify with privileged groups (e.g., men, straight, white, able-bodied, cis-gendered) to be more aware and proactive in support of equity, diversity, and inclusion. Everyone interested in this conversation is welcome to attend.

The European Astrobiology Institute (EAI) has been recently founded as virtual institute aiming to carry out research, training, outreach and dissemination activities in astrobiology in a comprehensive and coordinated manner and thereby securing a leading role for the European Research Area in the field. About 30 large space research organisations and leading research and higher education institutions have committed themselves to participate in it.

After a short introduction into the main features of the institute there will short presentations and ample room for the discussions on the scientific aims and the main activities of the institute. The focus will herein be on the formation of planetary systems and habitable environments on planets and satellites as well as on outreach activities of the Institute. Participants will also be informed about the different possibilities to participate in the institute.

Public information:
The programme of the session will be as follows:

15:30 - 15:45 General features of the EAI (Wolf Geppert, Stockholm University, SE)
15:45 - 15:55 Questions and Open Discussion
15:55 - 16:10 Presentation of the aims of the Working Group “Formation of Planetary systems and Habitable Environments” (Antonello Provenzale, INAF, IT)
16:10 - 16:20 Questions and Open Discussion
16:20 - 16:30 Presentation of the Working Group “Outreach, Media and Corporate Identity” (Caterina Boccato, INAF, IT)
16:30 - 16:40 Questions and Open Discussion
16:40 - 16:50 "Exoplanet Atmospheres: A new project team of the European Astrobiology Institute" (Kevin Heng, University of Bern, CH)
16:50 - 17:00 Questions and Open Discussion.

After the programme I invite you to a social dinner at Cafe Du Soleil (https://www.cafedusoleil.ch/site/fr/) at 19:30. The place is in walking distance (15 min) from the conference venue.

The place is a typical Genevan cafe-restaurant and still reasonably priced (at least for Geneva). If we are not too many we can eat a la carte. If you want to participate send a short e-mail to Wolf Geppert wgeppert(at)fysik.su.se.

The European SSHADE database on spectroscopy of solids (www.sshade.eu) provides on-line spectroscopic data (reflectance, optical constants, Raman, ...) on various types of solids, mostly covering the X, UV, Vis, Near/Mid/Far-IR and sub-mm ranges .

The measured samples include synthesized and natural ices, minerals, rocks, organic and carbonaceous materials, extraterrestrial samples ((micro-)meteorites, IDPs, Apollo, ...).

During this meeting we will make a live demonstration of the web interface of SSHADE and its search/visualization/export tools.

We will then let you play with SSHADE to try to found your favorite data (take your laptop), and ask questions.

The European SSHADE database on spectroscopy of solids (www.sshade.eu) provides on-line spectroscopic data (reflectance, optical constants, Raman, ...) on various types of solids, mostly covering the X, UV, Vis, Near/Mid/Far-IR and sub-mm ranges .

The measured samples include synthesized and natural ices, minerals, rocks, organic and carbonaceous materials, extraterrestrial samples ((micro-)meteorites, IDPs, Apollo, ...).

During this meeting we will make a live demonstration of the web interface of SSHADE and its search/visualization/export tools.

We will then let you play with SSHADE to try to found your favorite data (take your laptop), and ask questions.

EPSC Industry session

Public information:
EPSC Industry session

Taking the opportunity of the EPSC2019, we will hold progress meeting of the Euclid Solar System Science-Working-Group. This groups is developing the tools required to detect moving objects (inc. NEAs, asteroids, KBOs, comets) in the deep (V~26.5) visible and near-infrared images that the ESA Euclid space mission will acquire in the 2022-2028 time frame.

The JUICE and Clipper teams host a second workshop to discuss the status of both missions (including their trajectory updates), to share information on science plans and capability of both missions, and to identify synergistic investigations and collaborations. One key question is to understand how the science of interest if both missions are in the Jupiter system at the same time and how we can best leverage the science investigations if the missions are not in the Jupiter System at the same time. We expect specific talks and discussions to cover the following topics:
- Callisto science, including magnetic induction, gravity, and surface remote sensing;
- Complementary remote-sensing and in-situ observations of Europa’s surface, atmosphere, any plumes, and space environment;
- Spacecraft Impact at the end of either mission (e.g. one spacecraft monitoring the other as it impacts onto Ganymede);
- Improving the ephemerides of the Galilean satellites to constrain orbital evolution and tidal heating.
- Monitoring of Jupiter’s auroral activity by one spacecraft while the other makes remote-sensing and/or in-situ observations at one of the moons.
Other discussion topics are obviously possible.

Public information:
The JUICE and Europa Clipper science teams host a second workshop to discuss the status of both missions (including their trajectory updates), to share information on science plans and capability of both missions, and to identify synergistic investigations and collaborations. Key questions are to understand how the science of interest if both missions are in the Jupiter system at the same time and how we can best leverage the science investigations if the missions are not in the Jupiter system at the same time.
Workshop topics:
• Introduction, JUICE and Europa Clipper projects status reports, updated Europa Clipper trajectory, discussion
• Improving the ephemerides of Jupiter moons, JUICE-Clipper synergies
• Spacecraft impact at the end of either mission: potential science
• Potential joint JUICE-Europa Clipper Callisto science
• Discussion, wrap-up

The workshop is open to all JUICE and Europa Clipper science team members.

The JUICE and Clipper teams host a second workshop to discuss the status of both missions (including their trajectory updates), to share information on science plans and capability of both missions, and to identify synergistic investigations and collaborations. One key question is to understand how the science of interest if both missions are in the Jupiter system at the same time and how we can best leverage the science investigations if the missions are not in the Jupiter System at the same time. We expect specific talks and discussions to cover the following topics:
- Callisto science, including magnetic induction, gravity, and surface remote sensing;
- Complementary remote-sensing and in-situ observations of Europa’s surface, atmosphere, any plumes, and space environment;
- Spacecraft Impact at the end of either mission (e.g. one spacecraft monitoring the other as it impacts onto Ganymede);
- Improving the ephemerides of the Galilean satellites to constrain orbital evolution and tidal heating.
- Monitoring of Jupiter’s auroral activity by one spacecraft while the other makes remote-sensing and/or in-situ observations at one of the moons.
Other discussion topics are obviously possible.

Public information:
The JUICE and Europa Clipper science teams host a second workshop to discuss the status of both missions (including their trajectory updates), to share information on science plans and capability of both missions, and to identify synergistic investigations and collaborations. Key questions are to understand how the science of interest if both missions are in the Jupiter system at the same time and how we can best leverage the science investigations if the missions are not in the Jupiter system at the same time.
Workshop topics:
• Introduction, JUICE and Europa Clipper projects status reports, updated Europa Clipper trajectory, discussion
• Improving the ephemerides of Jupiter moons, JUICE-Clipper synergies
• Spacecraft impact at the end of either mission: potential science
• Potential joint JUICE-Europa Clipper Callisto science
• Discussion, wrap-up

The workshop is open to all JUICE and Europa Clipper science team members.

Comet Interceptor is a mission proposed to ESA, with contributions from Japan and the USA, in response to the agency's F-class call. The mission would involve a spacecraft and two sub-spacecraft being targeted at either a comet approaching the Sun for the first time, or an interstellar object passing through our solar system. ESA will announce the selected mission in July 2019, and, if our proposal is successful, EPSC provides a perfect and invaluable opportunity to hold a short team meeting post-selection, and to inform the wider planetary science community of our plans for the mission.

Public information:
An invitation-only meeting for members of the ESA Comet Interceptor mission team.

Dawn mission splinter reserved for science team members of the mission. To exchange ideas and works among the team.

This is a team meeting to discuss and plan progress, timing, logistics and deliverables of our accepted JWST-ERS proposal.

The annual editorial board meeting held to discuss journal statistics, forthcoming initiatives and past challenges relevant to Icarus.

Meeting of the IAU Working Group Planetary System Nomenclature and its supporting Task Groups

This is an annual event, which the PDS SBN always has during the DPS meeting. It is a meeting of the SBN personnel with the science advisors to report the progress in data archiving and discuss the future plans. We always offer food (lunch) for our attendees.

Meeting of the MMX rover team

Public information:
Meeting of the JAXA MMX CNES-DLR rover team (by invitation only)

We would like to take advantage of the EPSC/DPS conference to organise the annual meeting of the thesis committee for Cecily SUNDAY. Thesis title: "Rolling in milligravity: feasibility and performance of a wheel on the surface of a small body"

Short meeting (one hour) for the organization of the Horizon 2061 session next Friday.