1) Voyage 2050 ---- Long-term planning of the ESA Science Programme

The next planning cycle in ESA's Science Programme, Voyage 2050, is now underway. Ideas are solicited from the scientific community for the science themes that should be covered during the Voyage 2050 planning cycle, which covers the time period 2035-2050. Deadline for receipt of White Papers: 5 August 2019, 12:00 (noon) CEST.

 a) Membership of Topical Teams

     Scientists working in ESA Member States and with an interest in any topic in space science and in the
     relevant technologies are welcome to apply for membership of the Topical Teams. Space
     science is defined here in a broad sense, including the observation of the Universe, planetary
     science, solar science, study of the space environment, and scientific experiments that can
     carried out from a spacecraft.

    The Topical Teams will be appointed by the Director of Science after the evaluation and recommendations
    of the Senior Committee. It is intended to have a mix of experience represented in each Topical Team
     and early career scientists are specifically encouraged to apply.

    Full details, including information about Voyage 2050, the tasks of the Topical Team members, and
     information needed by applicants, can be found in the Call for Membership of Topical Teams document.

  b) White Papers

     By means of the present Call for White Papers, the Agency is soliciting ideas from the scientific
     community for the science themes that should be covered during the Voyage 2050 planning cycle.

     White Papers are not proposals for specific missions; they should rather argue why a specific scientific
     theme should have priority in the Voyage 2050 planning cycle. At the same time, and to ensure realism
     in the resulting Programme, applicants should briefly illustrate possible mission profiles.

     Any scientist or science team can submit a White Paper, with no limitation in terms of residence or
     nationality. All White Papers must be submitted in English. White Paper lead scientists cannot be members
     of the Topical Teams.

     Full details, including information about Voyage 2050, the requirements for White Papers, and the role these
     will play in formulating the future Science Programme, can be found in the Call for White Papers document.

    https://www.cosmos.esa.int/web/voyage-2050



2) TRAPPIST-1 | 11-14 June 2019 | Liège, Belgium

Dear colleague,

I'm happy to announce you that on June 11-14 will take place at Liege, Belgium, a multidisciplinary conference totally dedicated to the TRAPPIST-1 planetary system. It aims to cover all aspects of the study of TRAPPIST-1, notably:
* The host star TRAPPIST-1 (and other ultracool dwarf stars): structure, evolution, activity, etc.
* Formation, migration, and dynamics of the planets of TRAPPIST-1 (and around other ultracool dwarf stars)
* Exploring ultracool dwarfs (including brown dwarfs) for more TRAPPIST-1-like systems.
* The structure of TRAPPIST-1 planets: observations vs models, evolution, etc.
* The atmospheric properties of TRAPPIST-1 planets: models, evolution (erosion, outgassing, impacts, pre-main-sequence phase, etc.),
* Atmospheric characterization of the planets with JWST and other upcoming facilities, the prospects for liquid water, possible biosignatures and their detectability, etc.
* The possibility of life on TRAPPIST-1 planets: prebiotic chemistry and photosynthesis around ultracool dwarfs, the impact of high-energy radiation and cosmics, tidal locking, lessons from the solar system, etc.

Contributions from all horizons are welcome: stellar physics, exoplanetology, solar system planetology, observational and theoretical astrophysics, astrobiology, etc. The conference will be divided in different sessions, each composed of an invited review talk, several contributed talks, and short poster presentations.

The discovery of TRAPPIST-1 planets triggered the imagination of many artists that integrated them in their works (novels, music, poems, etc). This is why the conference will also include a special session on Thursday 13th called “TRAPPIST-1: between science and fiction”, during which some artists, writers, game developers, etc will present their works related to TRAPPIST-1 to the participating scientists, enabling the two communities to discuss their visions of a fascinating planetary system.

Registrations are opened up to May 15. The deadline for contributed talk propositions is Apr 1st (not a joke).

For more info, please visit the conference website: https://events.uliege.be/trappist-1

Don't hesitate to advertise the conference to any possibly interested colleague, and to display the conference poster on the walls of your institute!

Best wishes,
Michael


3) Call for 9th Paolo Farinella Prize
The call for the Farinella Prize 2019 has been announced. The ninth Paolo Farinella Prize will be awarded to a young scientist with outstanding contributions in the field of planetary science concerning “The Trans-Neptunian Population”. The prize is supported by the University of Pisa and by IAPS-INAF (Rome). The award ceremony will be hosted by the  European Planetary Science Congress (EPSC) – Division for Planetary Sciences (DPS) Joint Meeting in Geneva, Switzerland (15-20 September 2019).

For the 9th“Paolo Farinella” Prize the terms and rules are as follows:

A competition is announced to award the “Paolo Farinella” Prize for the year 2019. The prize consists of a plate, a certificate and the amount of 1500 €. The winner is expected to give a Prize lecture at the EPSC/DPS awards special session.
The winner will be selected on the basis of his/her overall research results in the field of “The Trans-Neptunian Population“.
Nominations must be sent by email not later than April 15 to the following addresses: Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.,Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser. Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser., using the downloadable form.
The nominations for the “Paolo Farinella” Prize can be made by any researcher that works in the field of planetary sciences following the indications in the attached form. Selfnominationsareacceptable. The candidates should have international and interdisciplinary collaborations and should be not older than 47 years, the age of Paolo when he passed away, at the date of April 15, 2019.
The winner of the prize will be selected before May 20 by the “Paolo Farinella” Prize Committee composed of outstanding scientists in planetary sciences, with specific experience in the field.
The Prize Committee will consider all the nominations, but will be entitled to autonomously consider other candidates.


4) EPSC-DPS Joint Meeting 2019 ---  Genève --- 15-20 septembre 2019

    Date limite pour la soumission des abstracts, le 8 mai: https://administrator.copernicus.org/authentication.php

     a) OPS1 - Ice Giant Systems
        Conveners: D. H. Atkinson
        This session welcomes abstracts addressing all aspects of ice-giants systems including the internal structure of the ice giants, the composition, structure, and processes of and within ice-giant atmospheres, ice-giant magnetospheres, satellites, and rings, and the relationship to exoplanetary systems. The session will comprise a combination of solicited and contributed oral and poster presentations on new and continuing studies of the ice-giant systems and the connection of the ice giants to our current understanding of exoplanetary system

We welcome papers that
Address the current understanding of ice-giant systems, including atmospheres, interiors, magnetospheres, rings, and satellites including Triton;
Advance our understanding of the ice-giant systems in preparation for future exploration, both remote sensing and in situ;
Discuss what the ice giants can tell us about solar system formation and evolution leading to a better understanding of the current structure of the solar system and its habitable zone
Address outstanding science questions requiring future investigations including from spacecraft, remote sensing, theoretical, and laboratory work necessary to improve our knowledge of the ice giants and their relationship to the gas giants and the solar system;
Present concepts for missions, instruments, and investigations to make appropriate and useful measurements.

b) OPS2 --- Saturn system and the Cassini-Huygens mission
Convener: Athena Coustenis
Results related to the Saturnian system from ground-based and Cassini-Huygens mission observations are welcome. All aspects of the system (planet, satellites and rings) will be presented with emphasis on recent results.


   c)  MIT6 -- Interstellar Probe: science, mission designs, opportunities and challenges
        Convener: Michel Blanc
An Interstellar Probe mission would be the first dedicated mission to venture into the unknown space between our star and other potentially habitable planetary systems. The idea was first discussed dating back to 1960 and the concept has been studied by multiple groups since then. The lack of propulsion technologies and launch vehicles have often presented a stumbling block for NASA and other space agencies to move further with these concepts. In 2016, a congressional report recommended NASA to take the enabling steps for an Interstellar scientific probe. A new NASA-funded study is under way to design a pragmatic Interstellar Probe mission with a goal of reaching 1000 AU within 50 years using available or near-term technology. The study objectives are to identify compelling science targets, develop realistic mission concepts and evaluate critical technologies. The cross-disciplinary science targets include exploration of the Very Local Interstellar Medium and its interaction with the heliosphere, characterization of the circum-solar dust disk, exploration of previously unexplored Kuiper Belt Objects, and observation of the extragalactic background light beyond the zodiacal cloud. A vantage point far away from the solar system, naturally enables these observations to be put in the context of other exoplanetary systems and astrospheres. At the same time, Chinese scientists are studying with their space agency CNSA a scenario in which two “Heliospheric Boundary Explorers” would be launched 6 years apart, one towards the “nose” of the Heliosphere, one in the direction of its putative tail, to address scientific objectives partly similar to the ones described in the NASA study. Not only will the synergies between these two missions be particularly valuable, but also both of them will offer unique opportunities for broad international collaborations, including European contributions.
This session will welcome reports on the unique science discoveries enabled by missions to the Interstellar Medium beyond heliospheric boundaries and will discuss their design concepts, enabling technologies and programmatic challenges.


d) EXO5 -- Aerosols and clouds in planetary atmospheres
Convener: P. Lavvas

Atmospheric aerosols and cloud particles are found in every atmosphere of the solar system, as well as, in exoplanets. Depending on their size, shape, chemical composition, latent heat, and distribution, their effect on the radiation budget varies drastically and is difficult to predict. When organic, aerosols also carry a strong prebiotic interest reinforced by the presence of heavy atoms such as nitrogen, oxygen or sulfur.

The aim of the session is to gather presentations on these complex objects for both terrestrial and giant planet atmospheres, including the special cases of Titan’s and Pluto's hazy atmospheres. All research aspects from their production and evolution processes, their observation/detection, to their fate and atmospheric impact are welcomed, including laboratory investigations and modeling.

e) EXO7 --- Planetary Aeronomy – Near and Afar
Convener: Antonio García Muñoz

Space missions, ground-based observations and theory allow for detailed characterization of planetary upper atmospheres in the solar system that provides novel insights into the physical mechanisms at play. At the same time, the detection of short-period extrasolar planets has inspired numerous studies of chemistry, dynamics, and escape of the upper atmospheres of these planets, at more extreme conditions than those found in the solar system. More than ever, it is critical to foster the communication between the communities working on the theoretical and observational aspects of both solar system and exoplanet upper atmospheres. This communication will secure a solid progress in the interpretation of new atmospheric observables and in the implications for e.g. planet demographics.

This session brings together researchers from the solar system and exoplanet communities in an attempt to exchange knowledge and ideas. We welcome papers on all aspects of planetary aeronomy i.e., the science of the upper atmosphere, either in the solar system or exoplanet systems. Suitable papers include results on photochemistry and ionization, magnetosphere-ionosphere coupling, energy balance and circulation, atmospheric escape and evolution as well as new observations and novel observational techniques.

5) Ninth International Conference on Mars ---- Caltech, Pasadena, California  ---- July 22-25

The Ninth International Conference on Mars will be held at the California Institute of Technology (Caltech) in
Pasadena, California, beginning the morning of Monday, July 22, and ending after a full day on Thursday, July 25.


The Mars Exploration Program Analysis Group (MEPAG) meeting is tentatively scheduled at Caltech on Friday, July 26,
following the Ninth International Conference on Mars. (These will be treated as two separate meetings for NASA
conference forecasting purposes. More information on the MEPAG meeting will be posted to the MEPAG website as it
becomes available.)

The Ninth International Mars Conference will be an ideal time to step back and summarize our current understanding
of Mars and the progress we have made so far. The aim of the meeting is to (1) synthesize changed paradigms in Mars
evolution and pull together the breadth of current Mars knowledge; (2) look forward toward the next decades of Mars
exploration; and (3) aid both individual community members’ and larger groups’/institutions’ planning for that next
decade.

Abstract Deadline: 7 mai

https://www.hou.usra.edu/meetings/ninthmars2019/


6) S-SAIL: Solar System Atmospheres’ Investigation and exopLanets  --- Lisbon, Portugal   --- 27-28 June 2019.

The Organizing Committee is pleased to inform that a Workshop on Planetary
Atmosphere Science entitled “S-SAIL: Solar System Atmospheres’ Investigation
and exopLanets“ will take place in Lisbon, Portugal, in the days 27-28 June
2019.  This workshop is supported by Europlanet 2020 RI NA1 –Innovation
through Science Networking, and Fundação para a Ciências e Tecnologia (FCT),
Portugal

+++ AIMS and TOPICS +++
The main goal of this 2-days workshop is to gather  researchers, post-docs and
students from all Europe, working on Planetary Science studies to discuss
about several topics related with Planetary Atmospheres (including
exoplanets), and promote collaborations on the basis of a interdisciplinary
approach.

Main topics:
- Atmosphere characterization I: chemical composition (Solar System planets)
- Clouds and Dynamics
- Atmospheric Waves
- Atmosphere Modeling
- Atmosphere characterization II: exoplanets
- Current and Future mission

Keynote speakers:
Alejandro Cardesin Moinelo (ESAC, Madrid, Spain)
Olivier Demangeon         (IA, Portugal)
Therese Encrenaz             (Obs. Paris, France)
Gabriella Gilli                  (IA, Portugal)
Pedro Machado                (IA, Portugal)
Jorge Martins                   (IA, Portugal)
Emmanuel Marcq            (LATMOS, Paris, France)
João Mendonça                (DTU Space, Denmark)
Pedro Miranda                  (IDL/FCUL, Univ. Lisboa, Portugal)
Santiago Perez Hoyos        (UPV/EHU, Bilbao, Spain)
Arianna Piccialli                (BIRA-IASP, Belgium)
Peter Read                        (Atm. Physics Clarendon Laboratory, Oxford,
UK)
Agustin Sanchez Lavega   (UPV/EHU, Bilbao, Spain)
Nuno Santos                     (IA, Portugal)
Aymeric Spiga                    (LMD/Sorbonne Univ., Paris, France)
Thomas Widemann              (Obs. Paris, France)

============ IMPORTANT INFORMATION ============

*REGISTRATION FEES*
The regular registration fees will be 100 euros for students and 130 euros for
others.
Late registration fees will be 140 euros for students and 170 euros for
others.

*Abstracts* (one page included figures and references, in pdf format) of
contributions should be sent by email to the organizing committee
Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.  until 15 May, 2019, indicating preferences (talk or poster).
The final decision will be taken by the SOC.

*FINANCIAL SUPPORT*
A limited amount of funding is available for PhD students and postdoc who
cannot fund their own travel. The grant is up to 400 euros and it includes
registration fees. To apply, please fill the form and send it by email to the
organizing commettee Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser. stating: an estimate of the amount of
funding required; status (student, postdoc etc.); and approx. 2 sentences on
how your research will benefit from attending this workshop.


Please find here attached the poster of the workshop
The details about registration, travel support and logistics may be found on
the workshop's website:

http://www.iastro.pt/research/conferences/s-sail/

Looking forward to see you in Lisbon,

Pedro Machado and Gabriella Gilli on behalf of the SOC


7) Two exoplanets postdoctoral research positions in Grenoble and Paris (France)

As part of a research project funded by the ANR (Agence Nationale de la Recherche), the SPIRou Legacy Survey team invites applications for two postdoctoral research positions in the field of exoplanets detections and characterization. The positions will be hosted respectively at the Institut de Planétologie et d'Astrophysique de Grenoble (IPAG) and at the Institut d’Astrophysique de Paris (IAP), France, with a preferred starting date between July and October 2019. Both postdocs will be expected to carry out original research in using SPIRou data of the Radial Velocity (RV) survey dedicated to search and characterize exoplanets. The postdoc at IPAG will have to play an important role in the organization and the exploitation of the systematic RV monitoring of nearby M-dwarfs (under the supervision of X. Delfosse); the postdoc at IAP will have to play an important role to exploit the SPIRou RV monitoring of transiting planet candidates (under the supervision of G. Hébrard).

Interested candidates should contact Xavier Delfosse (Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.) at IPAG and/or Guillaume Hébrard (Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.) at IAP, and send (in a singe pdf file) a CV, a publication list, a motivation letter, a short research statement describing past achievements and future projects, and arrange for up to two letters of recommendation to be sent before 15 th May 2019.

http://www.iap.fr/users/hebrard/postdocANR.pdf

8) POSTDOCTORAL position at ISTerre : X-ray analyses of Mars Returned Samples under quarantine

https://origin-life.univ-grenoble-alpes.fr/medias/fichier/postdoc-isterre-cool_1554215393430-pdf

Université Grenoble Alpes invites applications for a 2-year postdoc position in Earth and Planetary Sciences, devoted to search of life on Earth at the Archean, as well as preparing X-ray analyses protocols under quarantine for Mars Returned Samples. The position can start as early as September 2019, and will be hosted at the Institut de Sciences de la Terre (ISTerre)

The cross-disciplinary project « Origin of Life » (funded by Univ. Grenoble Alpes IDEX, https://origin-life.univ- grenoble-alpes.fr) brings together the expertise of astrophysicists, astrochemists, planetary scientists, prebiotic chemists, biologists, geologists and paleontologists. It aims to understand the chemical processes that have led to life on Earth, to define habitability conditions for both Solar System planets and exoplanets, and to detect the most favorable exoplanets where to search for a putative existence of life in a near future.

The search for traces of life, in situ on planetary bodies, in samples brought back to Earth, or in Archean rocks has become a scientific goal displayed by space missions in progress (ExoMars - ESA, Osiris Rex, Mars 2020 and MSR - NASA, Hayabusa II - Jaxa), or by Origin of Life projects. The scientific issues involve:

- reducing the risk of false positives in the analyses
- controlling the possible degradation of the biological traces during the first diagnostics.
- establishing the absolute elemental composition and chemical environment of the biological traces during the first diagnostics.

Imaging primordial fossil microorganisms on host minerals by advanced non-invasive/non-destructive X-ray imaging methods of high spatial resolution and sensitivity opens new capabilities for Sample Return missions.



9) Lectureship position at the Open University

   We are now recruiting to a lectureship position with a research specialism in analytical planetary sciences in the School of Physical Sciences at the Open University.  This Faculty position will provide the opportunity to join a large group of planetary scientists with an extensive range of excellent analytical and simulation facilities and involvement in many on-going and planned planetary missions, and to contribute to our distance learning curriculum.
   The deadline for applications is 23rd April 2019 - see Open University website for details (http://www.open.ac.uk/about/employment/vacancies/lecturer-planetary-science-15811).

Best Wishes,

    Mahesh Anand

10) Research Associate - Meteorite Curation And Analysis (University of Manchester)


The appointee will perform laboratory and database curation tasks, undertake preliminary characterisation and analysis of a new UK Antarctic meteorite collection, perform research studies, and publish and communicate project outcomes. The Lost Meteorites of Antarctica Project is funded by the Leverhulme Trust with support from the British Antarctic Survey (BAS) to explore new Meteorite Stranding Zones in Antarctica for meteorites that are encapsulated within ice. More details of the project can be found at https://ukantarcticmeteorites.com/. The first field season to Antarctica in December 2018-February 2019 recovered meteorites from the surface of blue ice fields in the Antarctic interior. These samples will arrive in Manchester in June 2019, where they will be preliminarily curated and classified to meet international standards. Another field season is planned for next Antarctic summer.
 

For more information on the position and how to apply please visit https://www.jobs.manchester.ac.uk/displayjob.aspx?jobid=17132.


11) PhD position at the Unité Matériaux et Transformation (UMET), Université de Lille
 
Water in chondrites: experimental investigation of water - silicate interactions
           Carbonaceous chondrites are fossilized remnants of the solar system formation. They contain hydrated silicates resulting from water-rock reactions, the nature of which remains puzzling. What was the state of water at the time of hydration - liquid or vapor? Where did it occur – in the protoplanetary disk or within the asteroids?
          This project aims at investigating experimentally the water/silicate interactions in order to understand the conditions of the alteration events (location, temperature, duration). We will focus on how fast water vapor might alter amorphous silicates, one of the major components accreted in chondrites. We will conduct experiments in an environmental cell, explore various conditions (temperature, fH2O, etc...) and a range of precursor compositions. The reaction products are expected to be nanometer-sized, and we will use state-of-the-art transmission electron microscopy (TEM) techniques to reveal their properties. The lab has recently acquired an advanced TEM with a configuration ideal to perform high resolution images, chemical analysis by EDS and electron energy loss spectroscopy (EELS). The environment also offers multiple and complementary analytical instruments. The results will be interpreted in the frame of the protoplanetary disk evolution and the alteration of asteroids.

Corentin Le Guillou, Hugues Leroux.
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