1) Congrès du PNP

 

le site du colloque de bilan et prospective du PNP (du 5 au 7 Septembre 2018 à Nice) est désormais ouvert:

http://univ-cotedazur.fr/events/pnp

vous pouvez vous inscrire et soumettre votre titre et abstract. Les deadlines sont le 31 Mai pour les inscriptions avec abstract et le 25 Aout pour les inscriptions sans abstract.
Une participation aux frais de 30 euros est demandée

 

2) Session "Organic Matter in Space" @ EPSC 2018, 16–21 September 2018, Berlin - abstract deadline 16 mai

 

Dear colleagues,

We would like to invite the world-wide community of planetary scientists working on the organic matter to submit an abstract to our session "Organic Matter in Space" that is co-organized between the Small Bodies (SB) and Astrobiology (AB) programme groups.

Resume:

Organic matter was abundant in the protosolar nebula, as attested by the wide range of organic compounds in the primitive bodies of our solar system, such as comets and carbonaceous chondrites. These organic compounds were delivered to the early Earth and may have played a role in the emergence of life. However, the origin of this organic matter remains debated. Is it synthesized in the protosolar nebula and/or inherited from the interstellar medium?
 
This session focuses on the organic matter origin and evolution in astrophysical environments and on the connection that could exist between the organic matter of the interstellar medium and the compounds detected in primitive bodies of the solar system.  

This session invites communications on experimental, theoretical and observational studies related to the origin of organic matter in the primitive bodies, such as: a) detection and evolution of organic compounds in the interstellar medium, b) characterization and evolution of the organic matter in primitive bodies, c) distribution of organic matter in the protosolar disk, d) observation of organic matter in planetary surfaces.

The session will consist of Oral and Poster contributions.

You may see all deadlines & milestones of the conference at the following website:https://www.epsc2018.eu/information/deadlines_and_milestones.html

Please forward this message to colleagues who may be interested.

We look forward to seeing you in Berlin.

With best wishes,

Vassilissa Vinogradoff, Grégoire Danger, Laurent Remusat.


3) ESA Workshop: Towards the Use of Lunar Resources, ESTEC, 3-5 July 2018

In  order to support of preparations for the future utilisation of lunar resources ESA is hosting a workshop: Towards the Use of Lunar Resources.

Further information, registration and the opportunity to propose a presentation can be found at:

http://exploration.esa.int/moon/59878-workshop-towards-the-use-of-lunar-resources/

The workshop will be held at the European Space Research Technology Centre (ESTEC) in the Netherlands, on 3 to 5 July 2018. The meeting emphasises the role that lunar resources can play in supporting exploration goals and the synergies with the utilisation of resources on Earth, at Mars and from asteroids.

This meeting aims to bring together experts and stakeholders from sectors in space and on Earth to:
Identify:
Use cases and drivers for lunar resource utilisation
Relevant European strengths, heritage and expertise
Community aspirations for the future
Opportunities to engage in Space Resource and to create partnerships
Outcomes that should be delivered in the coming years
Raise awareness of:
ESA technology activities for lunar resources
ESA missions to prepare for lunar resource utilisation
Opportunities to partner with ESA
Contribute to:
The establishment of a European space resources community
The evolution of a space resources strategy
Preparations for future missions and technology development activities

 

1) post-doc position on planet formation at MPIA Heidelberg.

2 Postdoctoral Positions in the Planet and Star Formation Department at the
Max Planck Institute for Astronomy (MPIA), One in the group of Bertram Bitsch and
one in the Group of Hubert Klahr, Heidelberg (Reference number: 18_04)
The Max Planck Institute for Astronomy (MPIA) in Heidelberg invites applications for postdoctoral
research positions in the Planet and Star Formation Department.
The successful applicants will carry out research in the field of planet formation working in the groups
of Bertram Bitsch or Hubert Klahr. Prior experience and publications on radiation transfer, magneto
and radiation hydrodynamical simulations of protoplanetary discs, planet-disc interaction, physics and
chemistry of dusty and icy planet building material, and/or N-body simulations for planet formation is
highly appreciated.
We expect and foster collaborations and interaction within the PSF department, especially with the
other theory groups and the observational projects on planet and disc observations. A commitment to
student training and supervision will be appreciated.
Applicants should have a PhD in astronomy, astrophysics, physics or a closely related field. The
appointment will be for an initial period of three years, with the possibility of extension for another year.
Funds for publications travel and computer equipment will be provided.
The positions have a flexible starting date, with a preferred starting date after summer 2018. The
remuneration is based on the German collective wage agreement for the public sector (TVöD)
depending on qualification and experience in level E13/E14. Social benefits are granted according to
the regulations for public service. Interested candidates should send a curriculum vitae, publication list,
and a brief statement of research interests by March 31st. They should also arrange for three letters
of reference to be provided separately by the same date. All applications and reference letters need to be
submitted using our online application system at:
https://s-lotus.gwdg.de/mpg/mhas/psf_pd_18_04_in.nsf
Candidates should first register with our online system to generate a registration code, which must be
sent to referees for letter submission. Please concatenate CV, publication list, and research statement
into a single PDF file.
For scientific enquires and informal enquires please contact: Bertram Bitsch – Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser. or
Hubert Klahr – Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
For submission enquires please contact: Marina Gilke – Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
The Max Planck Society is an equal opportunity employer. Applications from women, disabled people
and minority groups are particularly welcome. The MPIA supports its employees in their search for
suitable child care institutions.


2) workshop "METEORITES – Understanding the origin of planetodiversity" Paris- 6-8 June 2018

An international workshop "METEORITES – Understanding the origin of planetodiversity" will be held at the Paris Museum- 6-8 June 2018

https://meteorites2018.sciencesconf.org/

This workshop will adress most of the recent issues in cosmochemistry and planetary formation. Invited speakers include Larry Nittler (Carnegie Institution), Sara Russell (NHM London), Thorsten Kleine (Münster University), Michael Zolensky (NASA), Anders Johansen (Lund University) and  Nathalie Carrasco (LATMOS).

It will be a unique occasion to visit the exhibit "Météorites, entre ciel et terre" at MNHN (expometeorites.fr)
Please submit your abstract by March 30th and send a declaration of interest at Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
The organizers - Prof. Gounelle & Roskosz


3) Goldschmidt conference. Boston, Aug. 12-17. Abstract deadline March 31

tout est dans le titre. Voir https://goldschmidt.info/2018/


4) quatrième réunion des utilisateurs du télescope T193 de l'OHP et du TBL: journées SF2, Bordeaux le 5 juillet

La quatrième réunion des utilisateurs du télescope T193 de l'OHP et du TBL (Télescope Bernard-Lyot) se tiendra le jeudi 5 juillet 2018 de 14h00 à 18h00 à Bordeaux, dans le cadre de la Semaine de l'Astrophysique Française de la SF2A.

Cette réunion se veut avant tout un moment d'échange et de partage d'expériences. Les télescopes, leur fonctionnement, leur instrumentation et leurs perspectives y seront présentés et discutés. Une grande partie sera également consacrée à la présentation de résultats scientifiques obtenus récemment sur ces deux télescopes, sur la base des contributions proposées par les participants.

Les utilisateurs du T193 et du TBL sont invités à participer à cette réunion et à y proposer des contributions d'ici au 3 juin 2018 sur le site de la SF2A : http://sf2a.eu/semaine-sf2a/2018

http://sf2a.eu/semaine-sf2a/2018/workshop_page.php?lang=fr&workshop=Quatrième%20réunion%20des%20utilisateurs%20des%20télescopes%20français%20(TBL/OHP193)&workshop_code=S13


5) post-doc position on formation and evolution of complex organic matter at IPAG Grenoble (deadline April 15)

The Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) in Univ. Grenoble Alpes,
France invites applications for a postdoctoral research position in Laboratory Astrophysics. The
appointment is initially for one year and may be extended to two more years, is funded by the
French Scientific Research Center (CNRS) and is paid according to the French public service scale.
15 k€/year will be allocated to the successful candidate to carry his/her research project. IPAG is
located in Grenoble (France), a lively and scenic university town.
The postdoc will carry out original research related to the formation and evolution of complex
organic matter in the solar system (and beyond) through the analysis by very high-resolution mass
spectrometry of laboratory analogues and/or extraterrestrial samples. The postdoc will be joining
the mass spectrometry group of the “planeto” team (∼20 faculties, technicians, postdocs and
students) and will closely work with Dr. Véronique Vuitton (PI of the research project) and with
other colleagues at IPAG (F.-R. Orthous-Daunay, L. Bonal, E. Quirico), as well as in the Paris area
and the United States. The mass spectrometry group has a solid experience in Titan’s atmospheric
chemistry as well as in the evolution of the organic matter present in small bodies (comets,
meteorites) and is currently expanding its interests to Pluto and extrasolar planets. It has also
significantly contributed to several space missions (e.g. Cassini-Huygens and Rosetta).
Applicants must hold a Ph.D. with a solid background in analytical chemistry and/or laboratory
astrophysics and have strong interest in planetary sciences and/or geochemistry and/or
astrobiology. Experience in mass spectrometry and/or liquid chromatography and/or scientific
programming is an asset.
Applicants should send a curriculum vitae, a list of publications, a summary of previous research
(2 pages max.), research interests (1 page max.), and the names of at least two persons who can
be contacted for letters of references. Applications can be sent in electronic form or regular post
(documents will not be returned) to the address below by April 15, 2018. Applications will be
considered until the position is filled. The preferred starting date is June 1, 2018.
Applications should be sent to:
Dr. Véronique Vuitton
Institut de Planétologie et d’Astrophysique de Grenoble
Université Grenoble Alpes - Bât OSUG A
CS 40700 38058 Grenoble Cedex 9 France
E-mail: Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.


6) Planet Formation and Evolution, Rostock, 27.02.-01.03.2019 (1st announcement)

the 12th Workshop in the series "Planet Formation and Evolution
(PFE-12)" will be held at the Institute of Physics, University of
Rostock, Feb 27 - March 1, 2019. All information about the Workshop,
deadlines, the program, travel to Rostock, accommodation etc. will be
given via the PFE-12 web pages which will be updated regularly.

Registration to the Workshop and abstract submission will be possible
online from July 1 to October 31, 2018. We plan to circulate the final
program in early January 2019. Summary:

Workshop PFE-12
Date:       Feb 27 - March 1, 2019
Location: Institute of Physics, University of Rostock, Germany
www:       http://pfe2019.stat.physik.uni-rostock.de/

Please forward this information to the members of your groups and all
potentially interested colleagues. We are looking forward to see you at
the PFE-12 Workshop in Rostock in 2019.

On behalf of the LOC, Ronald Redmer


7) offre de Thèse: "irradiation des glaces et formation de matière organique", PIIM, Marseille

Intitulé du Projet :
Etudes préliminaires à l’analyse de données des futures missions d’exploration du système solaire: irradiation des glaces et formation de matière organique

Nom et Prénom du Directeur de thèse principal : Danger Grégoire (PIIM)
Adresse email : Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
Ecole doctorale principale : ED 250 – Sciences Chimiques

Nom et Prénom du co-Directeur de thèse : Mousis Olivier (LAM)
Adresse email : Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
Ecole doctorale partenaire : ED 352 – Physique et sciences de la matière
Le sujet de thèse s'intéresse à déterminer le lien qui peut exister entre la glace initiale, les composés organiques volatils qui subliment lors du réchauffement de cette même glace préalablement irradiée (photons UV, électrons, ions), et les résidus organiques qui se forment après désorption de ces composés volatils. Lier ces trois phases est un élément essentiel pour comprendre les processus chimiques qui se déroulent lors de l'évolution de ces glaces. Par ailleurs, la compréhension de l'interaction glace/gaz/matière organique réfractaire permettra de définir à terme les méthodologies analytiques nécessaires qui pourront être proposées pour de futures missions spatiales ayant pour objectifs l'analyse de la matière organique présente dans l'environnement de ces objets interplanétaires. Nous pourrons déterminer par exemple en quoi une analyse de la phase gazeuse peut amener des informations sur la composition de la surface d’objets astrophysiques et quelle pourrait en être les limites.

Nous appuierons de plus nos recherches sur quatre outils analytiques déjà développés pour le spatial (spectroscopie infrarouge et  GC-MS), ou en cours de développement (orbitrap et HPLC). La caractérisation de l'altération des glaces par des irradiations VUV, d’ions ou d’électrons, suivie d'un réchauffement se fait in situ par spectrométrie infrarouge. L'analyse des composés organiques volatils se fait par GC-orbitrap à partir d'un dispositif spécialement développé à cet effet. L'analyse des résidus se fait par spectrométrie de masse très haute résolution (orbitrap) et par UHPLC-orbitrap. Ainsi à la fin de cette thèse nous déterminerons la faisabilité d’unifier ces quatre outils au sein d’une mission spatiale ayant pour objectif scientifique l’analyse de la matière organique au sein d’objets interplanétaires ou à la surface de satellites glacés. Ces informations seront essentielles pour le design de futures missions spatiales proposées par la LAM, et pour venir enrichir les modèles d’évolution de la matière au sein des corps du système solaire.


8) Research Scientist position at ELSI (Tokyo). 14 April Deadline

I would like to bring to your attention an upcoming recruitment for “Research Scientist” with an application deadline of 14 April. Contract durations are presently offered up to 3 years. We are seeking ambitious and adventurous young scientists from a large variety of fields who are interested in very broad inter-disciplinary collaboration (ranging from galaxy formation/evolution to planet formation theory, planet evolution, pre-biotic chemistry, micro-biology, and everything between, above, and below).

Here is a link to the detailed recruitment information and application instructions: https://goo.gl/ow5MBb
Best Regards,
John Hernlund
ELSI Vice Director

1) Permanent PLATO position at the University of Warwick

Applications are invited for a full time and permanent Research Fellow position at the University of Warwick, UK. Closing date for applications is 23rd March 2018.

The position is in support of ESA’s PLATO Mission, and is based in the Science Management Office. It is funded by the UK Space Agency and the University of Warwick.

The successful candidate will hold a PhD degree, a proven research track record, and preferably experience of working in an (international) project environment.

Duties include organisational support of the PLATO Science consortium, and there will be other opportunities to become involved with the PLATO mission, both technically and scientifically. Opportunities are also available to become scientifically involved in CHEOPS, and in ground based experiments in which Warwick has significant roles (e.g. NGTS and SuperWASP). We expect that some of the post holder’s time will be available for research, preferably in the area of extra-solar planets with the Astronomy and Astrophysics Group at Warwick.

Informal enquiries about this post can be made to Prof. D. L. Pollacco (d.pollacco[at]warwick.ac.uk)

Full details about the post, and information on how to apply: https://atsv7.wcn.co.uk/search_engine/jobs.cgi?owner=5062452&ownertype=fair&jcode=1713193&vt_template=1457&adminview=1

Information about the PLATO Science consortium: https://warwick.ac.uk/plato-science/

Information about the Astronomy & Astrophysics Group: https://warwick.ac.uk/fac/sci/physics/research/astro/


2) NASA Exploration Science Forum - JUNE 26-28, 2018 at NASA Ames Research Center
The Solar System Exploration Research Institute (SSERVI) is pleased to announce the 5th annual NASA Exploration Science Forum (ESF), to be held in person JUNE 26-28, 2018 at NASA Ames Research Center, Moffett Field, CA.  This year's Forum will feature scientific discussions of human exploration targets of interest (the Moon, near-Earth asteroids, and the moons of Mars).  Science sessions will focus on recent mission results and in-depth analyses of science and exploration studies.  Dedicated side-conferences for graduate students and young professionals will coincide with the ESF.  Public engagement discussions will be interwoven among science topics as well.   

Abstracts are currently open and will be accepted through 11:59 p.m. PDT March 30, 2018 at
https://nesf2018.arc.nasa.gov/

Foreign national participants MUST register at the above url by May 25, 2018.  US citizens may register until June 22, 2018.  Hotel room reservation blocks at per diem


3) Joint ARES/JSC-LPI Gordon A. McKay Fellowship

Direct link: https://usra-openhire.silkroad.com/epostings/index.cfm?fuseaction=app.jobInfo&version=1&jobid=723

 

The Astromaterials Research and Exploration Science (ARES) Division at NASA Johnson Space Center and the Universities Space Research Association’s Lunar and Planetary Institute (LPI), both in Houston, Texas, are proud to announce a new, prestigious Gordon A. McKay Postdoctoral Fellowship, honoring the accomplishments of Dr. Gordon A. McKay. Dr. McKay was a world-recognized authority on planetary igneous petrology and geochemistry, and was the leader of the ARES Research Office at JSC for over 20 years. The McKay Fellowship recognizes and promotes excellence in research for scientists within five years of their doctorate and is intended to encourage the development of young scientists in the field of astromaterials research that involves the study of the origin, composition, structure, and evolution of the bodies of the Solar System, including the planets and their satellites, the Earth and Moon, meteorites, asteroids, comets, and dust. McKay Fellows are expected to be self-motivated and to define their own research direction and foci within the planetary sciences (defined inclusively). The McKay Fellow will be in residence at JSC while also being an employee of USRA and active at the LPI, and be expected to interact with scientists of both organizations (see www.lpi.usra.edu and https://ares.jsc.nasa.gov/). Fellows will also enjoy access to all of JSC’s laboratories and analytical instruments on the same basis as scientific staff.

Applicants for this position should have a Ph.D. in a planetary and space sciences-related field before taking up the position. McKay Fellows will be provided highly competitive levels of salary, research support, and travel support for two years, with possible extension for another year. The candidate must be able to pass a detailed government background investigation. And due to security issues, citizens of U.S. State Department Designated Countries (see link under "ECP Notices" at http://oiir.hq.nasa.gov/nasaecp/) are not eligible.

Questions can be addressed to Dr. Louise Prockter (Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.). Interested applicants should apply to the posting at https://usracareers.silkroad.com/ and must submit a curriculum vita with list of publications, a two to three page statement of research interests, and a list of three professional references. Further information on current research and facilities at the LPI and at JSC can be found through the websites given above.

USRA is an independent, nonprofit research corporation where the combined efforts of in-house talent and university-based expertise merge to advance space science and technology. USRA works across disciplines including biomedicine, planetary science, astrophysics, and engineering and integrates those competencies into applications ranging from fundamental research to facility management and operations.

USRA is an Equal Opportunity Employer: Minorities / Females / Protected Veterans / Disabled / Sexual Orientation / Gender Identity.


4) School: "Stable and Chaotic Motions in the Planetary Problem" - Asiago (Italy) June 10-15 2018

The aim of this school is to study in depth the dynamics of planetary
systems from  the underlying mathematical theories coming from perturbation
theories and going back to A. N. Kolmogorov,  V.I. Arnold and J. Moser, up to the recent astronomical observations of comets, asteroids and exoplanets from ground and space.

We foresee 18 hourly mathematical and 10 astronomical lectures.


a) The Mathematical Lectures:

-Alessandra Celletti, Univ. Tor Vergata, Roma (lectures on KAM Theorem);

-Vadim Kaloshin, University of Maryland & ETH, Zurigo (Arnold diffusion);

-Richard Moeckel, University of Minnesota (the N-Body problem);

-Tere Seara, UPC, Barcellona (Arnold diffusion);

b) The Astronomical Lectures (10 hours):

-Alessandro Morbidelli, Observatoire de la Coste d’Azure, Nice (evolution of planetary systems)

-Ivano Bertini, University of Padova (space missions, comets);

-Foriangela La Forgia, University of Padova (comets);

-Francesco Marzari, University of Padova (extrasolar planets dynamics)

The precise titles and abstracts will be soon announced.

The lectures will be held at the Astrophysical Observatory in Asiago.

If you are interested to participate, please register
by sending an e-mail to Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser., by includig also
a short CV, before 30 April.

The participation to the school is open to Phd students, Post doc researchers
and researchers. We strongly encourage the participation of Phd and
Post-Doc researchers. We will be able to cover the local expenses for a limited number of young participants: to apply for financial support please mention
it in the registration e-mail.

The selection of the participants and of the financial support will
be confirmed by e-mail.

Accomodation: a limited number of rooms (cheap, from 10 to 15 euros per day, but comfortable; with kithchen facility) are available in the guest rooms at the
Observatory. Further information on other possible accomodations will be soon available.


5) Rencontres "Connexions en Physique Solaire et Stellaire », 14-18 Mai 2018, Observatoire de Banyuls


Site web: https://sunstars.sciencesconf.org
Contact: Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.

Chers collègues,

nous vous invitons à participer aux rencontres "Connexions en Physique Solaire et Stellaire », qui visent à une revue croisée des méthodes et connaissances actuelles sur plusieurs aspects de la physique stellaire et solaire. Les principaux thèmes abordés seront les suivants:

    - Signature observationnelle de l'activité
    - Héliosismologie et astérosismologie
    - Champ magnétique solaire et stellaire
    - Dynamique des fluides astrophysiques
    - Environnement solaire et stellaire

Ces rencontres regrouperont participants et intervenants sur une semaine et se veulent un lieu d'échange et de débat stimulés par des cours. Elles sont ouvertes aux chercheurs, doctorants et post-doctorants.

Plus d’informations sont disponible sur le site.

Cloture des inscriptions le 16 mars (attention, nombre de participants limité)


6) Atélier: "Existe-t-il un lien entre la chimie du milieu interstellaire et celle des comètes ? " - CNES, Paris, le 24 mai 2018

Bonjour à tous,
Comme chaque année nous organisons le 24 mai 2018 Salle de l’Espace au CNES Paris un atelier dont le thème sera  "Existe-t-il un lien entre la chimie du milieu interstellaire et celle des comètes ? ". Nous tenterons de répondre à certaines de ces questions en comparant la composition de ces milieux, en rappelant les méthodes d’identification des molécules et les limites associées, en montrant ce qui peut être issu d’une transformation photochimique ou d’une autre source énergétique (chocs, hydrogène radicalaire, …) et en rappelant que chimie radicalaire et chimie ionique peuvent chacune jouer un rôle dans cette évolution chimique. Observations et simulations en laboratoire de ces milieux seront présentées.

Vous pourrez trouver toutes les informations nécessaires pour assister à cet atelier sur l'adresse suivante: https://ateliercnes2018.sciencesconf.org/

Bien cordialement.

Grégoire Danger, Jean-Claude Guillemin, Yann Trolez et Fabien Borget


7) Post-doc position: "Probing Saturn’s magnetosphere with auroral observations of Cassini and Hubble" au LESIA

The research project primarily aims at investigating the auroral processes and the dynamics at
various timescales of Saturn’s magnetosphere, through the analysis of remote ultraviolet (UV)
auroral observations recently acquired by the Cassini/UVIS spectro-imager and the Hubble
Space Telescope (HST), complemented by in situ radio and plasma measurements of the
Cassini spacecraft. The main objective of this project is to build and exploit a high level
database of Cassini/UVIS auroral observations in the frame of the APIS service, and to take
advantage of multi-platform measurements to disentangle and characterize the different
components of kronian aurorae (e.g. energy budget, dynamics from short-term scales to
solar/seasonal variations) and constrain the underlying acceleration processes. The Cassini
‘Grand Finale’, made of a series of high-inclination orbits, provided unprecedented vantage
views on both the northern and southern UV aurorae together with unique in situ
measurements along the auroral field lines. These observations were supported by coordinated
HST instantaneous observations of the northern UV aurorae near solstice, precisely scheduled
during the Cassini traversal of auroral field lines. Coincidentally, HST similarly observed the
UV aurorae of other giant planets which offer an extended frame for comparative planetology.

Requirements for the candidate:
The applicant should master the basics of magnetospheric and auroral physics, have a
documented past experience with space-based plasma observations and skills in massive data
processing.

Location and starting date:
The project will ideally start in Sept. 2018 (or before) at LESIA-Observatoire de Paris, 5
place Jules Janssen, 92190 Meudon, France.
Salary: in the range 3000-3200€/month (gross), according to experience.
Duration: 18 months.

Apply:
Application deadline is fixed on April 30th 2018.
Applications with CV, copies of degree diplomas and grades, two reference letters, and copies
of any previous research-related work statement of motivation.
The application should be sent preferably by e-mail to: Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.


8) session "interaction fluide/roche : des météorites à la terre", RST conference, du 22 au 26 Octobre à Lille Grand Palais

En Octobre prochain, les laboratoires Lillois du domaine des géosciences organisent, en partenariat avec la Société Géologique de France, la 26e réunion des Sciences de la Terre. Cet évènement se déroulera du 22 au 26 Octobre à Lille Grand Palais. Voici le lien du site sur lequel vous trouverez toutes les informations : https://rst2018-lille.sciencesconf.org

Parmi les nombreuses sessions que nous proposons, j'attire votre attention sur la session 9.2. Interactions fluide-roche : des météorites à la Terre. Cette session comprend plusieurs sous-sessions qui pourraient vous intéresser :
1/ Altération hydrothermale dans les contextes extraterrestre et terrestre : étude des interactions fluide – minéraux, front de réactions, mécanismes et cinétiques réactionnels dans des contextes extraterrestres (chondrites, astéroïdes, surface de Mars, etc...), ou des contextes terrestres de sub-surface (altération de la croûte océanique et des surfaces continentales).
2/ Interactions fluide-roche en contexte de stockage : étude de l’évolution minéralogique et géochimique d’un matériel géologique naturel subissant des contraintes externes (comme la mise en place en son sein d’une barrière ouvragée) en conditions hydrothermales. Ceci concerne aussi bien les études in situ que les approches expérimentales, pour des contextes de stockage géologique profond de déchets radioactifs, ou encore de stockage géologique du CO2.


9) Researcher position in Mathematical Physics at the University of Roma Tor Vergata

The Department of Mathematics of the University of Rome "Tor Vergata"
invites applications from talented individuals for a 3-years position of
     "ricercatore a tempo determinato di tipo B [RTD-B]"
a sort of tenure track position according to the Italian law n. 240/2010.
The position will be addressed to a very highly qualified researcher
working in the scientific field of
     MATHEMATICAL PHYSICS.
The application deadline is March 15, 2018.

For more information, see the job advertisement at
http://web.uniroma2.it/module/name/Content/newlang/italiano/action/showpage/navpath/CON/content_id/51738/section_id/6206

More information about the RTD-B position are available at "Art. 24"
of the Italian law n. 240/2010:
http://www.camera.it/parlam/leggi/10240l.htm

The Department of Mathematics - Univ. of Rome Tor Vergata is Italian Excellence Department 2018-2022.


10) Technologies and Infrastructures Workshop for Planetary Exploration, Horizon 2061, Lausanne, April 23-25, 2018

This is the second announcement of the *Technologies and Infrastructures Workshop for Planetary Exploration, Horizon 2061*, which will take place on *April 23-25, 2018*, in the *SwissTech Convention center on the campus of EPFL, Lausanne, Switzerland.*

*To ensure a great meeting the deadline of paper submission (Talks/Posters) has been extended to March 6, 2018 at:*

https://cmt3.research.microsoft.com/PE2018/

Alternatively, as some people had apparently some difficulties, you can submit your abstract (Including title and list of co-authors) to

Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser. <mailto:Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.>

*You can register to this event by connecting directly to:*

https://meeting.artegis.com/lw/lp/Participants/Participants?EVENT_ID=12704

*All information can be found at:*https://planetaryexploration2061.epfl.ch/

In particular, *a consolidated list of the keynotes is:*

• Dave Beaty (JPL, USA): Sample return and curation

• Michel Blanc (IRAP+ISSI): Planetary vision, a European view

• Fabienne Casoli (CNES, France): The CNES Vision

• Steve Chien (JPL, USA): Autonomy and on board processing

• Rachel Cross (Aberystwyth, UK): Hyperspectral cameras for planetary exploration

• David Ehrenreich (U. Geneva, CH): Current and future of exoplanets

• Sabrina Feldman (JPL, USA): New Sensors and science instruments

• Antonella Ferri (Thales Alenia Space): Current and future sample return missions

• Enrico Flamini (ASI, Italy): ASI Vision of Planetary Exploration and technological challenges

• Tony Freeman (JPL, USA): Disruptive technologies

• Masaki Fujimoto (ISAS/JAXA, Japan): Japanese Vision of Planetary Exploration and technological challenges

• Manuel Grande (Aberystwyth, UK): Technology foresight for Planetary Exploration

• Linli Guo (CAST, China): The Key Technologies for Lunar Base

• Brook Lakew (Goddard, USA) Planetary Science’s Vision 2050: Technology Challenges

• Joseph Lazio (JPL, USA): Communication and radio science

• Stephen Mackwell (USRA): Lessons learned from Planetary Science Vision 2050: Science Questions and Implementation Strategy

• Heike Rauer (DLR, Germany): Space technology developments for planetary exploration

Looking forward to prepare the future of Planetary Exploration with your participation.


Michel Blanc, Manuel Grande, Jean-Paul Kneib & Anton Ivanov

(on behalf of the SOC and LOC)

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
11) Poste de Maître de Conférences en Planétologie, Université de Besançon

Un concours pour un poste de Maître de Conférences en planétologie à l'Université de Besançon (laboratoire UTINAM), pour la rentrée 2018,
est ouvert.

Voir le profil sur

https://www.galaxie.enseignementsup-recherche.gouv.fr/ensup/ListesPostesPublies/ANTEE/2018_1/0251215K/FOPC_0251215K_4451.pdf
 
Date de fermeture des candidatures : 29 mars 2018.


12) Cosmic Cycle of Dust and Gas in the Galaxy: from Old to Young Stars -July 9th to July 13th, 2018- Quy Nhon, Vietnam

The registration for the conference Cosmic Cycle of Dust and Gas in the Galaxy: from Old to Young Stars -July 9th to July 13th, 2018- is now open. The conference will take place at the International Center for Interdisciplinary Science and Education (ICISE) which is located in the beautiful coastal city of Quy Nhon, Vietnam. You are invited to register and submit contributed talks and posters.

https://cosmiccycle2018.sciencesconf.org/

Organized in the framework of the "Rencontres du Vietnam", the conference focuses on the evolution of dust and gas from evolved to young stars. The aim of the conference is to bring astronomers working on the circumstellar environment of evolved stars and star forming regions and planetologists working on the origin of the solar system together to discuss about science in a friendly and relaxed environment at ICISE. In July 2016, in the same cycle of conferences, “Blowing In the Wind” addressed issues of dynamics of gas and dust in the Galaxy. In July 2017, another conference “Star Formation in Different Environments” focused on how stars form. This year's conference will be dedicated to the physico-chemistry and evolution of gas and dust. It will review state-of-the-art knowledge of the molecular and dust components of envelopes and shells surrounding AGB stars, planetary nebulae, diffuse giant molecular clouds as well as Supernovae. Special sessions will be dedicated to the origin and evolution of matter in the solar system: meteorites, comets, etc. Recent observations, in particular with ALMA, are the source of major progress in the study of the cosmic cycle of gas and dust in the Galaxy making such a conference very timely.

The list of invited speakers can be found at: https://cosmiccycle2018.sciencesconf.org/resource/page/id/6

There is some funding from the Rencontres du Vietnam to pay the hotel for a few participants. Grants will be given in priority to those giving a talk at the conference. If you need support, please fill in a form in the following link (Financial Support section):

https://cosmiccycle2018.sciencesconf.org/resource/page/id/2):

Bootcamp:

During the weekend before the conference, we organize a series of tutorials and lectures introducing the topics of the conference to senior undergraduates, PhD students and young postdocs. If you are interested in attending it, please contact Tuan-Anh Pham (Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.).

Anne Dutrey and Diep Ngoc Pham, on behalf of the SOC


13) Ph.D. position(s) in Galaxy, Star and/or Planet formation at Chalmers University, Gothenburg, Sweden

We are advertising one or more Ph.D. positions in Galaxy, Star and/or Planet formation (~4-year positions, post Masters) at Chalmers University of Technology, Gothenburg, Sweden. Please advertise to any students that you think may be suitable and have an interest in such opportunities.

The application deadline is 31st March 2018, with a start date expected around Sept. 2018 (but is flexible).

More information is here:

https://jobregister.aas.org/ad/aec9c1d5


14) Postdoc position on Geomagnetic field analysis and Earth’s core dynamics, IPGP

The Geological Fluid Dynamics and Geomagnetism groups of IPG Paris (http://www.ipgp.fr)  are seeking applicants for a postdoctoral fellowship on Earth’s core dynamics and geomagnetic observations. The successful fellow will take part in a current project on explaining and modelling Earth’s core dynamics and the geomagnetic field, from the rapid to historical secular variations.

Good knowledge in one or several of these fields is preferred: numerical simulations of the geodynamo, acquisition of geomagnetic data, techniques for data assimilation in Earth sciences. Please write to Julien Aubert, Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser., for general enquiries about the position. Applications should include a CV and short description of the research record and activities. The appointment is for 1 year.

Applications should be received by May 1 2018 but can be considered after this date if the position is not filled. The position start date is flexible.

 

1) atelier international sur la Spectrométrie de Masse Spatiale, Orléans, du 16 au 18 mai

Deadline for registration : Tuesday 27th of March

In recent decades, the search for signs of extraterrestrial life has been a prime topic in scientific space exploration. This international conference, organized by LE STUDIUM Loire Valley Institute for Advanced Studies, aims at presenting the current state of knowledge acquired so far in the field of mass spectrometry by the activities of the world's scientific organizations and the most active space agencies pursuing this fundamental research field.

International experts will present the results on mass spectrometry of on-going and recently-completed in situ space missions (review talks on Cassini-Huygens, Rosetta, MSL-Curiosity, etc….) as well as the results of the return sample missions (Stardust, Hayabusa, etc..) and experimental laboratory and relevant modelling results.

Several space missions under development that address the research field will be presented by representatives of Space Agencies (NASA, ESA, JAXA, RSA, CNES,..)

A part of the workshop will be devoted to the presentations of new High Resolution Mass Spectrometry (HRMS) space instruments under development that are required to advance in our capability to address the ambitious science objectives laid down for the future missions under study.

Main topics: Mass Spectrometry, Space Missions, Spatial Instrumentation, Planetology, Exobiology, Habitability.

pour plus d'infos:
http://www.lestudium-ias.com/fr/event/advances-space-mass-spectrometry-search-extraterrestrial-signs-life-0



2) Two Job Openings in planetary science at Goddard Space Flight Center

JOB OPENING 1: Planetary Scientist with expertise in exospheres at Goddard Space Flight Center
The Planetary Magnetospheres Laboratory of the Solar System Exploration Division (SSED) at NASA Goddard Space Flight Center (GSFC) located in Greenbelt, Maryland has a U.S. civil service position open for a Planetary Scientist, with expertise in exospheres, at the GS-13 (Junior) level. The Solar System Exploration Division conducts theoretical and experimental research to explore the solar system and understand the formation and evolution of planetary systems. For more information about the duties of this position and requirements or to apply please see

http://www.usajobs.gov/GetJob/ViewDetails/489402400

 More Information about the SSED can be found at science.gsfc.nasa.gov/solarsystem. The job opening closes on 9 February. Specific questions about the SSED and this position can be directed to Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser..

JOB OPENING 2: Planetary Scientist with expertise in magnetometry at Goddard Space Flight Center

The Planetary Magnetospheres Laboratory of the Solar System Exploration Division (SSED) at NASA Goddard Space Flight Center (GSFC) located in Greenbelt, Maryland has a civil service position open for a Magnetometry Scientist, at either the Junior or mid-career levels. The Solar System Exploration Division conducts theoretical and experimental research to explore the solar system and understand the formation and evolution of planetary systems. For more information about the duties of this position and requirements or to apply please see: www.usajobs.gov/GetJob/ViewDetails/487865100 (GS-13 position) and www.usajobs.gov/GetJob/ViewDetails/487885200 (GS-15 position)
We will be hiring a single individual, at either a junior or mid-career level, to fill this position. More Information about the SSED can be found at science.gsfc.nasa.gov/solarsystem. These job openings close on 5 February. Specific questions about the SSED and this position can be directed to Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.


3) allocation de temps d'observation sur les télescopes aux Canaries

NB: The deadline for the 2018 call for proposals is
midnight, February 28, 2018.
The International Scientific Committee (CCI) of the Roque de los Muchachos
(ORM, La Palma) and Teide (OT, Tenerife) observatories invites applications
for International Time Programmes (ITP) on telescopes installed at these
Observatories.
The ITP offers up to 5% of the observing time, evenly spread throughout the year and
the lunar cycle, at the telescopes listed on the ITP web page:
www.iac.es/eno.php?op1=5&op2=13&op3=26&lang=en
A proposal can request up to 15 nights/year (80 hours on GTC & STELLA) of
observing time. A proposal can cover a period of up to two consecutive years, i.e. in
this case, up to a maximum of 30 nights / 160 hours per telescope can be requested.
Proposals must include a justification of the time requested on each telescope.

Links:
------
[1] http://www.iac.es/eno.php?op1=5&amp;lang=en
[2] http://www.iac.es/disclaimer.php
[3] http://www.iac.es/disclaimer.php?lang=en


4) ISSS Course on “The Polar Upper Atmosphere: from Science to Operational Issues”, L'Aquila (It), 17-21/9

The International School of Space Science of the Consorzio Interuniversitario per la Fisica Spaziale organizes a Course on “The Polar Upper Atmosphere: from Science to Operational Issues”, to be held in L’Aquila, Italy, 17-21 September 2018, directed by G. De Franceschi, M. Mendillo, C. Mitchell.  
The goal of the school is to foster excitement and encourage involvement of the next generation of space researchers in studies of the geospace environment of Polar Regions.  The importance of these regions is rapidly growing due to modern society’s dependence on Global Navigation Satellite Systems (GNSS) services and products, strongly affected by ionospheric variability at high latitudes. Topics will focus on the infrastructures for multi-instrument monitoring, data management from sub auroral to polar latitudes, the need for specialized models of the upper atmosphere, and the development of mitigation algorithms to improve GNSS services and products. The school is mainly addressed to graduate and post-graduate students with enthusiastic interest on this topic. Students-teams will be organized through an “inside team building” activity scheduled on the first day of the school.  This initial activity will formulate, under the supervision of experts, the “first iteration” of student-led project proposals. The establishment of the student-teams aims to both stimulate the interaction among the new generation of scientists from different countries and furnish the preliminary tools to build successful project proposals.  On the final day the students-teams will present their project results and participate in their evaluation by the School Program and Organization Committees.

Applications are due before May 6, 2018.

For more information visit http://www.cifs-isss.org/ or send an e-mail to Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.


5) Two theoretical astrophysics postdoc positions at Lund Observatory

Two postdoc positions in Theoretical Astrophysics at Lund Observatory are available. Theoretical astrophysics at Lund Observatory encompasses planet formation and dynamics, high-energy astrophysics, binary stellar evolution, stellar and Galactic dynamics, and galaxy formation. We have strong observational links, including involvement in the ESA missions Gaia, CHEOPS, PLATO and LISA.

We are seeking postdocs having a background within a broad range of astronomy and astrophysics, both observational and theoretical.

The postdocs will be free to define their own research in collaboration with the theoretical astrophysics researchers in Lund but will be required to work on two specific projects. One postdoc will work with Alexander Mustill on modelling the post-main sequence fate of planetary systems and the pollution of white dwarfs by accreted asteroids. The second postdoc will work with Ross Church on the early lives of binary stars that go on to form gravitational wave sources.

Research at Lund Observatory also includes work on stellar populations, stellar and laboratory spectroscopy, and research related to Gaia (particularly the astrometric solution).

The applicants should, at the start of the contract, hold a PhD in astronomy, astrophysics or a related field. The PhD should have been obtained no earlier than three years prior to the deadline.

Both positions are available for two years with the potential for a third year. The positions are available from Spring 2018, but starting dates as late as Autumn 2018 are possible.

The application should include a CV, publication list, and a statement of research interests. The statement of research interests should include your own research to be carried out in Lund as well as an indication of specific interests related to the post-main sequence evolution of planetary systems and/or gravitational wave progenitors. Names and contact information of three persons willing to give references should be supplied.

Included Benefits:
All employees in Sweden and at Lund University enjoy full access to the national health care system. The position includes 5 weeks paid annual leave. For employees with small children there are extra possibilities of leave and there are state provided day-care facilities for all employees.

Related URLs:
Lund Observatory
Application Deadline:
Thursday, February 22, 2018

See instructions following link to application system
URL:
Full advert and link to application system
Institution/Company Job ID or Reference Code:
PA2018/94


6) workshop  "Inverse problems and approximation techniques in planetary sciences", 16-18 May 2018, Sophia Antipolis

Dates: 16-18 May 2018.
Location: INRIA, Centre de Recherche Sophia Antipolis Méditerranée.

Organizers: Laurent Baratchart, Sylvain Chevillard, Juliette Leblond, Marie-Line Merinho.

The organization is supported by C4PO (UCA Jedi), INRIA Sophia Antipolis, and the team APICS-FACTAS.

Presentation:
A workshop and a school will be held for 3 days on inverse problems in harmonic electromagnetism and approximation, with applications mainly dedicated to geomagnetism and paleomagnetism. They will more precisely concern direct and inverse potential problems of source detection and non-destructive control, data extension, conductivity or permittivity estimation from boundary data, together with resolution algorithms. The techniques pertain to harmonic analysis, e.g. expansions in spherical harmonics or other families of special functions, Hodge decomposition principles, approximation theory and constrained optimization, Fourier analysis, ...

Applications to geosciences and planetary sciences concern in particular geomagnetism, subsoil prospection, paleomagnetism, gravimetry, source imaging, processing of stellar signals, measures protocols and steering of instruments.

The school and the workshop are open to Master or PhD students and of course to post-doctoral researchers, researchers, professors, engineers.

Talks and lectures will be given by the following speakers (preliminary list, to be confirmed):

Christian Gerhards (Computational Science Center, Univ. Vienna, Austria),
Eduardo A. Lima (Dep. Earth, Atmospheric Planetary Sciences, MIT, Cambridge, MA, USA),
Dmitry Ponomarev (Laboratory POEMS, ENSTA-INRIA, Saclay, France),
Yoann Quesnel (CEREGE-CNRS, Univ. Aix-Marseille, Aix-en Provence, France),
Doug Hardin (Department of Mathematics, Vanderbilt Univ., Nashville, TN, USA),
Mark Wieczorek (Observatoire de la Côte d'Azur, Nice, France).

7) Rosetta workshop on comets and their role in Solar System formation, 28 May to 1 June 2018 in Rhodes

The Rosetta spacecraft completed its observations of Comet 67P/Churyumov-
Gerasimenko in September 2016, but analysis and interpretation of the data are continuing.  The Rosetta Project is holding one of its last Science Working Team meetings from 28 May to 1 June 2018 in Rhodes, Greece, and invites the scientific community to participate.  The discussions/presentations will focus on three themes:  
1) Where and how did comets form, how are they put together, and what is their role in solar system and planetary formation scenarios?
2) What are comets made of?
3) How do comets work?
Additional information is available at the workshop website:
     https://www.cosmos.esa.int/web/rosetta-swt-49
Note that attendees must register in advance via the website prior to 26 March 2018.
March 26th is also the deadline for obtaining a special room rate at the conference hotel.
A registration fee of approximately 300 Euros will be collected on-site, and must
be paid in cash (Euros).  The exact fee will be determined by the number of registrants.


8) Didymos observer workshop, June 19-21, Prague

The binary near-Earth asteroid (65803) Didymos is the planned target for the
Asteroid Impact & Deflection Assessment  (AIDA, https://www-n.oca.eu/michel/AIDA/) mission. AIDA will be the first space experiment to demonstrate asteroid impact hazard mitigation by using a kinetic impactor to deflect an asteroid.  It is an international cooperation, consisting of two mission elements: the NASA Double Asteroid Redirection Test (DART, http://dart.jhuapl.edu/) mission and the ESA Hera (previously known as AIM) rendezvous mission
Remote (mostly Earth-based) observations of Didymos are an important part of
the mission. In this workshop, we will discuss observations for the 2019, 2020-2021, and 2022 apparitions of Didymos. We will discuss detailed plans and expected outcomes for 2019 observations and preliminary observing plans for the subsequent apparitions.
Additional meeting information is available at:
http://didymos2018-mtg.asu.cas.cz/
The full first announcement is available at:
http://didymos2018-mtg.asu.cas.cz/didymosprague2018_firstannouncement.txt
Dr. Petr Pravec (LOC chair)
Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
Dr. Cristina A. Thomas (SOC chair)
Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.


9) 9th Workshop on Catastrophic Disruption in the Solar System, May 14 - 17, 2018 Ikuta shrine (Japan)

Venue: Ikuta shrine (Ikuta Jinja Kaikan), Sannomiya, Kobe, Japan

http://www.impact-res.org/CD2018/Catastrophic_Disruption_2018/Welcome.html


ABSTRACT and REGISTRATION:

The site for abstract submission and registration is now open.
The deadline for abstract submission and application for early registration is Feb. 28 (JST).


TRAVEL GRANTS:

Partial travel support is available to encourage those with limited sources of funding to attend the meeting. Applicants must be the sole or senior author of an accepted abstract to qualify, and must be the presenter of the contribution. The deadline to submit an application for a travel grant is Feb. 28 (JST).

The maximum amount of the support will be 100, 000 JPY per person, which includes partial support for the expenses for transportation and accommodation. LOC will review the applications and decide the amount of the support, depending on the availability of funding. Priority will be given to Ph.D. students and recent PhDs. Grant applicants will be notified of the decision after the SOC’s decision of abstract acceptance is finalized (March 9, 2018). Successful applicants will be given the grant in cash at the registration desk.

Applicants must complete the "Grant Application Form" and send it to Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser. with a recommendation letter of supervisor (in case of Ph.D. student) or a publication list (Postdoc/Other).


10) workshop "Asteroid Science Intersections with Mine Engineering 2018" in Belval, Luxembourg, April 16-17,

As part of the Luxembourg government's in-space utilisation initiative (1), we have developed a two-day workshop on April 16-17, 2018 titled:

"Asteroid Science Intersections with Mine Engineering 2018" in Belval, Luxembourg at the University of Luxembourg https://asime.uni.lu/

Abstracts due: March 9, 2018

ASIME 2018 focuses on the 'asteroid composition' theme of the science knowledge gaps (SKGs) (2) that emerged from the previous  ASIME in 2016 (3) and goes deeper.

What do we know about asteroid composition from remote-sensing observations? What are the potential caveats in the interpretation of Earth-based spectral observations? What are the next steps to improve our knowledge on asteroid composition by means of ground-based and space-based observations and asteroid rendez-vous and sample return missions?  How can this knowledge be used by asteroid mining companies?

The ASIME 2018 program is roughly these topics with these key speakers  for each:

1st Day Spectroscopic Observations from the  Ground  classic spectroscopy

                                Julia de Leon, Instituto de Astrofísica de Canarias – IAC spectroscopy  near-IR  

                                Antonella Barucci, Observatoire Paris-Site de Meudon mineralogy and water

                                Humberto Campins, University of Central Florida

                               Andy Rivkin,  John Hopkins, University asteroid shape linking taxonomy to dynamical asteroid class

                                Benoît Carry, Observatoire de la Côte d'Azur      

                Round table lead at the end of the first day

                                Alan Fitzsimmons, Queen's University Belfast Astrophysics Research Centre      

                           
                Workshop Dinner (provided)            

2nd Day Lab measurements then Space missions

                Laboratory Measurements (Meteorites)

                                Lydie Bonal, University of Grenoble

                Composition, mineralogy

                                Pierre Beck, University of Grenoble       

                Space Missions
                NEOWise

                                Amy Mainzer, JPL

                Hayabusa 2

                                Tomoki Nakamura, Tohoku University

                Osiris Rex

                                Dante Lauretta, University of Arizona

                Hera (was AIM2)

                                Patrick Michel ,Observatoire de la Côte d'Azur

                Dawn Review of instruments to access composition, from gamma-ray to TIR

                                Carol Raymond JPL         

                Wrap-up: How to Improve Our Knowledge

                                Simon Green, Open University             

                Workshop Dinner (provided)              

End of Workshop

We are aiming for 30 workshop participants plus n number of 'listeners'. The format will be long presentations and discussions.

Outcomes: The Outcomes will produce conclusions, as best we know today to asteroid mining company questions regarding asteroid composition.

The asteroid composition questions will be asked to the asteroid mining companies and posted to the conference web site at least one month before the workshop starts. The questions will also be available in a Google Doc document for those experts who cannot make the workshop. The participants can think about those questions and have the topic in their minds when they present their own work.

The questions/answers will then form either the next ASIME White Paper Reference document and/or a published journal article. We hope to see you there!
Amara Graps Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser., Patrick Michel Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.


11) COSPAR session B1.3 "Growing Up: the Long Journey of Planetary Systems .....", Pasadena, 14-22 July

We wish to remind you of the approaching deadline for the submission of abstracts to the 42nd COSPAR Scientific Assembly (https://www.cospar-assembly.org) that will be held in Pasadena, California, USA, on 14-22 July 2018, and to invite you to attend event B1.3:

"Growing Up: the Long Journey of Planetary Systems from Interstellar Volatiles and Refractories to Asteroids, Comets, and Planets",

jointly organized by Commission B "Space Studies of the Earth-Moon System, Planets, and Small Bodies of the Solar System" and Commission E "Research in Astrophysics from Space".

ABSTRACT SUBMISSION DEADLINE is 9 FEBRUARY 2018

Scientific Rationale:

The path starting from interstellar materials and leading to the formation of planetary systems is complex and still not completely understood. To advance our understanding, the history of the different planetary bodies needs to be studied together with their evolving surroundings. The initial interstellar volatile composition, its chemical evolution and the growth of refractory particles into the primordial planetesimals are tightly coupled to the emergence of a star-disc system from a prestellar core. The evolution of the star-disc system, in turn, deeply affects the growth of the planetesimals into planets and the composition of their cores and atmospheres. Finally, the physical and compositional characteristics of the different planetary bodies are influenced by the evolution of the planetary system as a whole. The aim of this COSPAR event, co-organized by Commissions B and E, is to provide researchers studying prestellar cores and protoplanetary discs, small bodies and meteorites, the Solar System and exoplanets with an interdisciplinary venue for presenting and comparatively discussing new data and results to advance our understanding of the long journey interstellar materials undertake to form the rich variety of planetary systems orbiting the Sun and other stars. This scientific event is sponsored by the Center for Space and Habitability of the University of Bern (www.csh.unibe.ch).


Main Scientific Organizers:
Diego Turrini (INAF-IAPS; Italy) & Maria Drozdovskaya (University of Bern; Switzerland)

Deputy Organizers:
Martin Rubin (University of Bern; Switzerland) & Sho Sasaki (Osaka University; Japan)

Sous-catégories