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&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)
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Dr. Cristina A. Thomas (SOC chair)
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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)

1) post-doc position in computational astrophysics at Luth (Meudon)

Applications are invited for a postdoctoral position in the area of computational astrophysics and numerical cosmology at the Laboratoire Univers et Theories (LUTH). The laboratory is one of the departments of the Astronomical Observatory of Paris with expertise in the field of theoretical and numerical astrophysics. We are seeking candidates with a strong background in computational hydrodynamics, although candidates with expertise from all area of numerical astrophysics will be considered.
The succesful candidate will work in collaboration with the computer science group and other members of the laboratory to the development of a new Adaptive Mesh Refinement hydrodynamics code for applications in astrophysics and cosmology. Candidates are expected to have a solid experience in computational physics.

The position is jointly funded by the ERC-StG "EDECS" and LUTH. The appointment will be for two years starting in September 2018, though a later starting date is negotiable. Candidates must hold a PhD by the date of appointment.

Interested candidates should send applications consisting of a CV, publication list and a short statement of research interest should be sent to Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
Inquiries about the position can be sent to the same address. Applicants should arrange for a minimum of two letters of recommendation to be sent to the same address. Applications received by 20 January 2018 will receive full consideration, although later applications may be considered.


2) Final Cassini Science Symposium: Aug. 12-17, 2018, Boulder, Co.

The Cassini Project will host a five-day Cassini Science Symposium August 12-17, including a reception Sunday evening before the sessions. Poster attached.
The sessions will be held at the University of Colorado in Boulder.

Invited and contributed talks will include the latest Cassini findings on the Saturn system, including the interpretation and synthesis of results.  Sessions will cover the following disciplines:  Rings, Titan, Icy Satellites, Magnetospheres and Saturn. This Symposium can serve as a springboard for future studies and space missions. Future mission posters are possible.

The symposium website can be found at  http://lasp.colorado.edu/home/2018-cassini-science-symposium/
Details, including key dates, registration and hotel information, and abstract instructions  be added to the website as known and will be sent in future announcements. Abstracts will be due 16 April, 2018. But for now, please save the dates.

If this announcement was forwarded to you and you would like us to add your email address to the contact list for future information, please contact Laura Bloom (see below).

We hope to see you there.

Larry W. Esposito
Chair, Symposium Organizing Committee

3) post-doc position in planetary/spacecraft dynamics in the Sao Paolo region

The Group of Orbital Dynamics & Planetology invites applications
for post-doc positions. There are 5 positions that will be funded by
FAPESP (Fundação de Amparo à Pesquisa do Estado de São Paulo). The
candidates must have experience on Planetary Dynamics and/or Spacecraft
Dynamics. The projects to be developed are in the following subjects:
- Orbits of satellites and planetary rings derived from space missions data;
- Attitude and orbit analysis for a mission to a triple asteroid system;
- Spin-orbit coupling in solar system dynamics;
- Dynamics involving small bodies under gravitational close approaches;
- Planetary Formation.

The projects will be developed in one of the following institutions:
I) São Paulo State University – UNESP in Guaratinguetá;
II) National Institute for Space Research – INPE in São José dos Campos;

Applicants should send a statement of research interest and a
curriculum vitae with a list of publications to:

Prof. Silvia Giuliatti Winter (email: Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.) Deadline of Applications: March 3, 2018


4) Upcoming short courses and field schools in planetary science (US/Canada)

Cosmochemistry - Origin and formation of the Solar System and planets
When: February 20 – February 25, 2018 in class, and April 4th 2018 for presentations (in class or remote)
Where: University of Western Ontario, London, ON, Canada
Instructor: Dr. Audrey Bouvier (Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.)
Course webpage: http://cpsx.uwo.ca/training/graduate_student/courses/cosmochemistry_glps_9510.html

Planetary Surface Processes Field School
When: May 6 – 17, 2018
Where: Arizona and Utah, USA
Instructor: Dr. Gordon Osinski (Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.)
Course webpage: http://cpsx.uwo.ca/training/graduate_student/courses/planetary_surface_processes_field_school_planetsc_9605l.html

Remote Sensing and Image Analysis for Earth and Planetary Science
When: June 25 – 30, 2018
Where: University of Western Ontario, London, ON, Canada
Instructors: Dr. Catherine Neish Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.) and Dr. Livio Tornabene (Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.)
Course webpage: http://cpsx.uwo.ca/training/graduate_student/courses/remote_sensing_short_course.html


5) Online Courses in Astrobiology

Online Courses in Astrobiology is the first platform of online courses in astrobiology. It presents quality lectures in different disciplines related to
the search for the origin of life, and has been designed for upper level graduate students and recent postdocs, as well as interested and curious public. Lectures are presented by international experts and are available in French, English and Spanish (additional languages may be added later). Current courses can be found at  and are http://astrobiovideo.com/
and are continuously updated.

All lectures of the IAU Astrobiology 2017 conference held in Coyhaique in december, can be found there.


6) Summer School: Basics of Astrobiology: Vienna, Austria, 17-18 August 2018
Just before the IAU General Assembly 2018 in Vienna, a summer school on the topic of ”Basics of Astrobiology” will be organized at the Observatory of the University of Vienna. The school is associated with the IAU Symposium 345 ”ORIGINS: From the Protosun to the First Steps of Life” (scheduled for 20-23 August). The training school will cover the bascis of astrobiology, from the formation of stars and planetary systems to the early conditions of life on planets, including atmospheres and planetary interiors, and the formation and early evolution of life itself.

The school is open to all interested students and professionals, with an emphasis on graduate students, postdocs and young scientists. Registration is open and there is no registration fee for this Training School! To register, please send a short e-mail containing your name, institute/university affiliation, and dietary constraints to: Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.. Acceptance is on a ”first come first served basis”. Space is limited, so register soon to secure a seat. Lunch (including a vegetarian option) and coffee breaks will be offered free of charge at the venue.

Please find additional info at:

Website: http://ninlil.elte.hu/boa/

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

We look forward to welcoming you in Vienna!

For the SOC:

M. Güdel, T. Lüftinger (Vienna)
M. Gargaud (Bordeaux)
B. Elmegreen (IBM, NY)
N. Haghighipour (Hawaii)
V. Toth (Budapest)


7) EPSC 2018 Berlin, Germany *** Call-for-sessions

Dear colleagues,

The 13th European Planetary Science Congress will take place at the
Technical University of Berlin, Berlin, Germany, from 16–21 September 2018.

We thank you for making last year's EPSC in Riga, Latvia, a great success.

As with the previous highly successful EPSC meetings, EPSC2018 provides
an attractive platform to exchange and present results, develop new
ideas and to network the planetary science community in Europe. A forum
you might say! It will have a distinctively interactive style, with a
mix of talks, workshops and posters, intended to provide a stimulating
environment for the community to meet.

The TU Berlin is located in the City West. Berlin is an attractive
capital city in the heart of Europe with lots of interesting historical
sites.

The success of EPSC is founded on the excellence of its sessions and
conveners. So we encourage you to make session or workshop proposals on
the conference website before 01 February 2018:

http://www.epsc2018.eu

The meeting will cover the whole scope of planetary science with
typically 50 sessions of different types.

We look forward to many proposals for exciting sessions and look forward
to seeing you in Berlin.

Best regards,

Maria Cristina De Sanctis
Scientific Organizing Committee Chair


8) Ph-D position in Louvain (Belgium) on « Evolution and Tracers of the Habitability Of Mars and Earth »


Thanks to a significant funding from the French-speaking and Dutch-speaking Communities, several universities in the North and South of the country have obtained funding to work on the project ET-HOME which is interested in understanding the habitability of the planets, and of the Earth and Mars in particular.

The contract for UCL is four years to carry out a doctoral thesis on the subject, and in particular, for the "Work Packages" which are the responsibility of UCL. For internal reasons, we first open the job for one year.

The scientist will have to work on the evolution of Mars' atmosphere, its greenhouse effect, transport in this atmosphere, meteorite impact erosion and the effects of volcanic degassing. The contract will start as soon as possible. Enthusiastic and motivated scientists are encouraged to apply.

The salary will follow the pay scales of UCL PhD students, which allows them to live comfortably.

WE ARE LOOKING FOR
The ideal candidate has a master's degree in science or engineering and combines many of the following characteristics:
-        Scientific curiosity
-        Strong interest in the field of space research and planetology
-        Learning fast, being creative, and having a pragmatic approach to problem solving
-        Experience in numerical modeling
-        Good knowledge of fluid mechanics, thermodynamics, transport phenomenon (diffusion, advection, convection, ...)
-        Experience in the use and development of GCM (General Circulation Model) of Mars’ atmosphere or of any other body in the solar system that has an atmosphere would be an advantage
-        Ability to work in English.
HOW TO APPLY
Send a CV (include the grades) with a letter of motivation (all in PDF format) and if possible two or three references before January 28, 2018 to Veronique Dehant, Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser., Professor at UCL, with copy to Özgur Karatekin, Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser., scientist at the Royal Observatory of Belgium.
Start of employment: February 1st or March 1st, 2018.


9) COSPAR 2018 Pasadena July 14-22.

Please consider submitting a paper for the 42nd Scientific Assembly of the Committee on Space Research (COSPAR), to be held in Pasadena,  on 14-22 July 2018.
The deadline for submitting abstracts is 9 February 2018.  Among a very rich COSPAR space research programme, we call in particular your attention and invite you to submit abstracts for sessions:

COSPAR-18-B3.1: LUNAR SCIENCE AND EXPLORATION
Lunar science and exploration are having a renaissance with as many as twelve missions (and 18 vehicles) sent to Moon during the last "International Lunar decade". This session is aimed at discussing new progress in lunar science from recent missions, latest science results, newer insights into our understanding of Moon, modelling and synthesis of different scientific data, future missions, and science questions. It will include invited, contributed, and poster papers. Papers on new lunar mission concepts, instrumentation for the future missions, the upcoming lunar decade of landers and lunar robotic village, and preparations for human lunar exploration are also welcome in this session.

Sub-sessions:
Results from Recent Lunar Missions
Upcoming missions towards lunar robotic village
Concepts, studies, technology and support research towards future lunar exploration
Exploration interactive workshop


COSPAR-18-PEX.2: "Human Exploration on the Moon, Mars and NEOs"
The session COSPAR-18-PEX.2: "Human Exploration on the Moon, Mars and NEOs", co-sponsored by COSPAR Exploration Panel and Commissions B, F will include solicited and contributed talks and poster/interactive presentations.  It will address various themes and COSPAR communities: Sciences (of, on, from) the Moon enabled by humans; Research from cislunar and libration points; From robotic villages to international lunar bases; Research from Mars & NEOs outposts; Humans to Phobos/Deimos, Mars and NEOs; Challenges and preparatory technologies, field research operations; Human and robotic partnerships and precursor missions; Resource utilisation, life support and sustainable exploration; Stakeholders for human exploration. One half-day session will be dedicated to a workshop format and meetings/reports of task groups: Science, Technology, Agencies, Robotic village, Human bases, Moon & Mars Villages, Society & Commerce, Outreach, Young Explorers. COSPAR has provided through Commissions, Panels and Working Groups (such as ILEWG, IMEWG) an international forum for supporting and promoting the robotic and human exploration of the Moon, Mars and NEOS.

Sub-sessions:
Sciences (of, on, from) the Moon, Mars & NEOs enabled by Humans
Technologies, field research operations; Human and robotic partnerships; Resource utilisation, life support
Stakeholders for sustainable MoonMars/Neos Villages: reports from task groups: Science, Technology, Agencies, Robotic village, Human bases, Habitats design, Society & Commerce, Outreach, Young Explorers

 COSPAR-18-B3.1 and COSPAR-18-PEX.2 will also serve as 13th International Conference on Exploration and Utilisation of the Moon (ICEUM13) from the ILEWG ICEUM series started in 1994.   

All information concerning the scientific program may be found at:

http://cospar2018.org/assembly-information/general-assembly-information/
http://cospar2018.org/scientific-program/scientific-program-and-abstract-submission/


10) postdoctoral research position in planetary remote sensing in Beijing
The Planetary Remote Sensing Laboratory of Peking University (PKU) invites applicants for a postdoctoral research position in planetary remote sensing that is fully funded by the PKU Boya postdoc scheme.
 
The successful applicant will join a research group of planetary remote sensing that is led by Prof. Wenzhe Fa. Potential research topics include: 1) Near-surface properties of the Moon from radar observations. Radar scattering models from the lunar surface will be developed/updated and used to study polar craters for ice deposits, dark halo craters, and maria basalts thickness from recent lunar radar data (e.g., Earth-based Arecibo radar, Miniature Radio Frequency radar, Kaguya Lunar Radar Sounder, and Chang’E-3 Lunar Penetrating Radar). 2) Thermal properties of the lunar regolith. Using heat conduction equation and microwave radiative transfer equation, Chang’E-1/2 microwave radiometer and Diviner infrared radiometer data will be analyzed to investigate physical temperature and thermal properties of the lunar regolith. 3) Evolution of the lunar regolith. Using the recent high-resolution optical images of the Moon, thickness of regolith will be estimated based on crater morphology method and evolution of lunar regolith will be studied using a Monte Carlo simulation model. If the applicant has her/his own idea for any other project in the broad field of planetary remote sensing, I will be glad to support the application as well.  
 
Requirements
- Major in Remote Sensing, Geophysics, Geology, or a closely related field;
- Hold a doctoral degree for less than three years at the time of application;
- Strong programming skills with Matlab, C++/Fortran;
- Basic knowledge of remote sensing software;

- Good communication skills and ability to work in an interdisciplinary team.
The postdoc position is awarded for two years, and the annual salary is 270,000 RMB (1 RMB = 0.156$) including basic salary, housing allowance, and assurance. Travel expenses to international conferences will be provided by the lab. For details about this position and living in Beijing, please contact Prof. Wenzhe Fa.
 
To apply, please send a CV, publication list, and a 2-page statement of research interests by email to Prof. Wenzhe Fa (Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.) before February 20, 2018.  

11) 16th International Symposium on Experimental Mineralogy, Petrology and Geochemistry, Clermont-Ferrand, 17-21 june 2018
we are delighted to announce that the website is open for *Abstract **submission* and Registrationto the the Sixteenth International Symposium on Experimental Mineralogy, Petrology and Geochemistry (*EMPG 16*) that will be held at *Clermont-Ferrand *(France) on *17-21 june 2018*.

http://empg16.lmv.uca.fr/

Please mark the date and help us in advertising this meeting by informing your students and colleagues by displaying the attached poster.

*Dealdine for abstracts will be 1st of March 2018.*

Additional Information is attached in the second circular.

With kind regards,

Nathalie Bolfan-Casanova, on behalf of the Organizing Comittee.

PS: My apologies for the multiple posting.

_Organizing Comittee:_
Nathalie Bolfan-Casanova
Ali Bouhifd
Maud Boyet
Tahar Hammouda
Ken Koga
Didier Laporte
Muriel Laubier
Geeth Manthilake
Julien Monteux
Anne-Magali Seydoux-Guillaume

12) ESA Research Fellowship in In Situ Resource Utilisation

ESA have opened a Research Fellowship position to support preparations for the future utilisation of lunar resources.

https://career2.successfactors.eu/sfcareer/jobreqcareer?jobId=5121&company=esa&username=

 An emphasis is placed on the potential utilisation of cold trapped lunar volatiles, including water ice, and the chemical reduction of lunar minerals.  The research to be performed should be related to one or more of the following:
•             lunar resource prospecting through in-situ measurements and remote sensing
•             laboratory analysis of lunar materials
•             lunar regolith excavation, handling and beneficiation
•             handling and preservation of ices in the lunar environment
•             resource extraction or processing
 
The Research Fellow will be based at ESA ESTEC ( http://www.esa.int/About_Us/ESTEC ), and will work closely with the both Lunar Lander Team and Strategy and Innovation Team in the Directorate of Human and Robotic Exploration. The role of the Fellowship and research performed is to support In-Situ Resource Utilisation aspects of ESA’s exploration activities, including the PROSPECT resource analysis package on Luna-27 (http://exploration.esa.int/moon/59102-about-prospect/) and future mission studies and technology developments. The research will be targeted at work that supports the integration of these activities into an overall strategy for ISRU. This is likely to involve working closely with different groups within ESA, science and technology research communities in academia and the private sector.
 
Where needed, access to laboratories or research facilities, in particular those existing within ESA-ESTEC, and resources needed to support research activities may be agreed on a case by case basis.


13) Microscopy and Microanalysis Conference in Baltimore, MD from August 5-9, 2018
We invite you to submit an abstract to the upcoming session entitled “Planetary Building Blocks and the Techniques Needed to Analyze Them” at the Microscopy and Microanalysis Conference in Baltimore, MD from August 5-9, 2018. The abstract submission deadline is February 15, 2018.

Symposium Description:

After successful missions to collect solar wind (NASA Genesis), cometary dust (NASA Stardust), and asteroidal regolith (JAXA Hayabusa) and with the successful launches of the JAXA Hayabusa2 and NASA OSIRIS-REx missions, the planetary-materials community is firmly within the era of sample return. The proposed symposium solicits papers that use microscopy and related techniques to explore the origins of planetary materials. We welcome contributions that discuss a range of topics including but not limited to: current analytical approaches, developments in new characterization strategies, developments in spatial and spectral resolution for pushing spectroscopic detection sensitivity and precision, and new protocols for sample handling.

Please find the template and submission instructions here:

https://www.microscopy.org/MandM/2018/program/submit.cfm

Thank you,

Tom Zega, University of Arizona

Michelle Thompson, NASA Johnson Space Center

Emma Bullock, Carnegie Institution for Science


14) workshop: "High Resolution Spectroscopy for Exoplanet atmospheres workshop - Nice, 1-5 October 2018"

Dear colleagues,

We are glad to annonce the "High Resolution Spectroscopy for Exoplanet atmospheres (HoRSE)” workshop that will
be held in Nice at the Observatoire de la Cote d’Azur from 1 to 5 October 2018.
Website: http://horse.sciencesconf.org

The registration is 120 euros and includes lunch and coffe breaks. The social dinner costs 36 euros: https://horse.sciencesconf.org/resource/page/id/5
We encourage everybody, and in particular PhD and Postdoc, to apply and to submit a contribution: https://horse.sciencesconf.org/submission/submit
We provide some financial support for young researchers, please apply before April 30th 2018: https://horse.sciencesconf.org/resource/page/id/1

IMPORTANT DATES
January, 2018: First announcement. Registration is OPEN
April 30th, 2018: Deadline for financial support request check here for information
June 30th, 2018: Deadline for registration and abstract submission
October 1st, 2018: The workshop starts

Looking forward to see you in Nice in October,
Andrea Chiavassa and Matteo Brogi on behalf of the SOC


15) Summer school on "sample return from small solar system bodies", Alpbach (Austria), July 17-26

This year, sixty European engineering and science students will be chosen to participate in the 42nd edition of the Summer School Alpbach, a ten-day learning opportunity held in the beautiful Austrian Alps. Participants will be engaged in an in-depth learning experience, attending stimulating lectures on various aspects of space science and engineering, and working intensely within smaller groups to define and design a space mission under the supervision of noted scientific and engineering experts within the field.

The topic of the Summer School Alpbach 2018 is “Sample return from small solar system bodies“. Students at the Alpbach Summer School 2018 will be informed about past achievements and current issues, and will be invited to propose ideas to study the solar system’s small bodies directly in situ with spacecraft and, ideally, returning samples to Earth in order to develop a much wider understanding of these small bodies, their properties, and what they can tell us about the evolution of the solar system.

Four student teams will define the scientific objectives of a space mission and will provide a preliminary end-to-end design of spacecraft, scientific instruments as well as mission and science operations that will meet their stated objectives. You and your team will be responsible for selecting and researching the problem to be addressed by your space mission, for cooperatively working with team members to meet difficult deadlines, and for developing your own working style.
For more info, visit https://www.summerschoolalpbach.at/

application deadline March 31, 2018

1) Post-doc positions in protoplanetary discs / planet formation, University of Leicester


Dear colleagues,

I'm writing to draw your attention to a new post-doctoral position (or positions) at the University of Leicester:
https://ig5.i-grasp.com/fe/tpl_UniversityOfLeicester01.asp?newms=jj&id=101425
https://jobregister.aas.org/ad/8f4ccfa9

Funding is available for three years from May 2018, but the starting date is negotiable; we can potentially consider dates as late as September/October.  We are ideally looking for applicants with experience of modelling protoplanetary discs and/or planet migration, but encourage applications from any candidates with a strong background in theoretical/computational astrophysics.  The deadline for applications is January 31st 2018.

I would appreciate it if you bring this message to the attention of any PhD students or post-docs who are currently on the job market. And please feel free to contact me with any questions about the job.

Best wishes for Christmas and the New Year,
Richard Alexander


2) EGU 2018 Last call for Abstracts: Outer planets Session and Cassini Symposium

please be informed of the following session and Union Symposium at the next EGU in Vienna, 8-13 April 2018.

https://www.egu2018.eu/

-------------------------------------------------------------------------------------------------
PS3.1 Outer Planets Systems

Please consider submitting an abstract to the session PS3.1 on Outer Planets Systems of the EGU General Assembly, to be held 8-13 April 2018, in Vienna, Austria, see:

https://meetingorganizer.copernicus.org/EGU2018/abstractsubmission/28491

The abstract submission deadline is 10 Jan 2018, 13:00 CET. Please note that this year late abstracts can only be accepted after approval by the Programme Committee; it also will entail a late abstract fee.

The PS3.1 EGU  session welcomes abstracts on the outer planets and Pluto systems, including their internal structures, atmospheres, magnetospheres, satellites and rings and coupling processes within those systems. A significant part of the session will be devoted to the Cassini-Huygens mission, including the Cassini Grand Finale Mission. Abstracts on observations from space and from the ground are also solicited. Supporting laboratory investigations and concepts for future space missions and Earth-based observations are also relevant to this session.

The Conveners: A. Coustenis, S. K. Atreya , O. Witasse , N. Altobelli , D. H. Atkinson , J-P. Lebreton , L. Spilker, C. Plainaki

————————————————————————————————————————————————

Also please note the Union Symposium : US3 celebrating the Cassini meeting with invited talks on different aspects of the mission :

US3: Cassini and future perspectives for the exploration of the outer solar system

The Cassini-Huygens Mission to Saturn has been an exemplary opportunity to the success expected from a large space mission built on international collaboration with ambitious goals. During 13 years, Cassini-Huygens has returned a huge amount of data that have been analysed and interpreted to enhance our understanding of the Saturnian system as a whole and not only (the investigations have bearing to our own planet and the formation of the Solar System as a whole). The mission ended in a dramatic plunge into Saturn’s atmosphere on September 15, 2017 sending back in-situ data as long as possible.  The final year of the mission included 20 “Ring-Grazing” orbits just outside the rings and a series of 22 highly inclined “Grand Finale” orbits with closest approach between the innermost D ring and Saturn’s upper atmosphere.   During the last half orbit, Cassini’s in-situ instruments were configured to collect atmospheric data until spacecraft signal was lost.  Both mission phases enabled the opportunity for unique science observations including: probing of gravitational and magnetic field moments to higher order and precision; determining the ring mass; in-situ sampling of the plasma environment, upper atmosphere and exosphere; and imaging both Saturn and rings at high resolution.  Already data obtained on these orbits have led to surprising initial results.  This Union Session will feature invited reports on the amazing discoveries that this mission brought and the new understanding we have gained of the Saturnian system.

Conveners: Stephanie C. Werner, Özgür Karatekin , Athena Coustenis , Linda Spilker , Scott Edgington


3) EGU 2018 Last call for Abstracts: PS1.11 Atmospheres of Terrestrial Planets

Dear colleagues,

Please consider submitting an abstract to the session PS1.11 on
Atmospheres of Terrestrial Planets of the EGU General Assembly to be held
8-13 April 2018, in Vienna, Austria:

http://meetingorganizer.copernicus.org/EGU2018/session/28542

The abstract submission deadline is 10 Jan 2018, 13:00 CET Please
note that this year late abstracts can only be accepted after approval by
the Programme Committee; it also will entail a late abstract fee.

This session focuses on the atmospheres of Venus, Mars and Titan, from
the boundary layer to their exospheres. Given the recent missions to
these bodies, the research on planetary atmospheres and their evolution
is blooming with new results. We welcome you to share your work with the
community as contributions discussing any aspect of the neutral
atmospheres of terrestrial planets. Contributions dealing with the
atmospheres of terrestrial-like extrasolar planets are also welcomed.

Please feel free to circulate this email.

Hope to see you in Vienna!

On behalf of the conveners
Francisco González-Galindo and Arnaud Beth


4) EGU 2018 Last call for Abstracts: PS4.2/BG8.2 Habitability and origin of life: From Early Earth to the Solar System and Beyond

We would like to draw your attention to the following two sessions to be held at the EGU General Assembly in Vienna, 8-13 April 2018:
 
PS4.2/BG8.2 Habitability and origin of life: From Early Earth to the Solar System and Beyond
convened by T. Spohn, V. Dehant, E. Javaux, L. Noack, and C. Szopa.

The aim of this session is to discuss the possible conditions and habitat for the origin and persistence of life in the solar system and beyond with emphasis on Earth, terrestrial planets, icy moons and exoplanets. We are interested in the conditions for habitability, the signatures of life, and the possible links between habitability and the evolution of planetary reservoirs (atmosphere, geosphere, hydrosphere, interior).

We invite contributions of relevance to the topic from all fields of Planetary Sciences and Biogeoscience including e.g., formation and structure of planetary bodies in the habitable zone, interior dynamics (convection, plate tectonics, and magnetic field), atmospheres, impacts and planetary evolution, geological evidence on Martian habitability, biogeochemical interactions, extremophiles and the limits of life, preservation and detection of biosignatures, mission concepts for exploration of planetary habitability.

http://meetingorganizer.copernicus.org/EGU2018/session/28524

PS4.1 Exoplanets: Observations and modeling
convened by Lena Noack, James Cho, Daniel Winterhalter, Yann Alibert and John Lee Grenfell.

A main goal of this session is to discuss the observations, formation and atmosphere/interior dynamics of exoplanets.
This includes recent observations of exoplanets from spacecraft and from ground-based observatories as well as papers discussing the status of, and/or plans for, future observations.
Further, theoretical and numerical models, in particular those that interpret or provide support for present and future observations, will be of strong interest.
Another topic of high interest pertains to the availability and observation of organic matter in planetary systems.

http://meetingorganizer.copernicus.org/EGU2018/session/28520

Abstract submission deadline: 10 Jan 2018

We would highly welcome your abstract in one of our sessions!

We look forward to seeing you in Vienna,
The conveners of PS4.1 and PS4.2/BG8.2


5) IAU general assembly: "recent advances in planetary astronomy", Aug. 24 & 27, Vienna

We would like to announce ​a two-day mini-conference on recent advances on planetary astronomy.

The conference is organized by the IAU Division F (Planetary Systems & Astrobiology)

in conjunction with the 30th General Assembly of the International Astronomical Union

that will be held in August 2018 in Vienna. The purpose of this program is to bring together

researchers from all fields of planetary astronomy (Solar system and extrasolar planets)

to present their new findings in form of oral and poster presentations, and discuss the current

state of research in our field. The website of the conference can be found at

 

http://www.ifa.hawaii.edu/planetsdays2018/


​The conference is held on August 24 & 27​, 2018 during the IAU General Assembly.

Registration is now open and abstracts are accepted from all fields of planetary astronomy for oral and

poster presentations. The deadline for early registration discount is January 31. Participants in this

workshop will receive admission to all scientific activities of the IAU General Assembly including the

Focus Meeting 1 on asteroid families, IAU Symposium 345 on the origin of life and planetary systems,

and a training school in Astrobiology held on August 17-18, 2018 by the University of Vienna.

 

We look forward to seeing you in Vienna.

Nader Haghighipour

President of the IAU Division F


6) Job opening at Australian National University Advanced Instrumentation and Technology Centre

 If you feel excited when the words “space” and “lasers” come together in the same sentence, this job announcement is for you!
An exciting opportunity has just come up for a motivated and talented Researcher or Engineer to join the Australian National University Advanced Instrumentation and Technology Centre (AITC) at Mount Stromlo Observatory near Canberra (http://rsaa.anu.edu.au/aitc).
The ANU AITC is leading the development and installation of the first adaptive optics-assisted ground-based telescope for laser tracking and manoeuvring of space debris. The system will be deployed on Mount Stromlo this year (2018) in the context of the Space Environment Management Cooperative Research Centre (SERC), also headquartered at Mount Stromlo Observatory.
More information on this and other projects undertaken by the ANU AITC to image satellites and space debris, and mitigate the threat of space missions and assets colliding with space debris can be found on the SERC web site at: http://www.serc.org.au
There are two 12-month fixed-term positions open to enable candidates with a preference for either an academic or a professional position to apply:
- A Postdoctoral Fellow (Level A) or Research Fellow (Level B) position - Please apply at: http://jobs.anu.edu.au/cw/en/job/519204/postdoctoral-fellowresearch-fellow
 
- An Instrumentation Engineer (ANUO7) position - Please apply at: http://jobs.anu.edu.au/cw/en/job/519205/instrumentation-engineer
 
This position will be open until filled, with a desirable starting date in early to mid-February 2018. The first round of applications will be reviewed on 10 January 2018. Interested applicants should apply as soon as possible.
For additional information, please contact: Associate Professor Celine d’Orgeville, by e-mail: Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser. or phone: +61 2 6125 6374.
The ANU AITC offers a supportive environment for parents and carers. Women are particularly encouraged to apply.
ANU values diversity and inclusion and is committed to providing equal employment opportunities to those of all backgrounds and identities. For more information about staff equity at ANU, visit https://services.anu.edu.au/human-resources/respect-inclusion
ANU also actively encourages applications from Aboriginal and Torres Strait Islander people. For more information on employment opportunities, contact our Indigenous Employment Consultant via: Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.

Dr. Marc Norman
Research School of Earth Sciences
The Australian National University
Canberra, ACT 0200 Australia
e-mail: Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.

7) Europlanet/VESPA open call
The 3rd annual Europlanet/VESPA call for Planetary Science Virtual Observatory data services is now open.

Our goal is to select 5 projects. The selected teams will be invited to a 1-week workshop to help them install and design their service, and to open it to the users community. These data services will be accessible from the VESPA portal (http://vespa.obspm.fr) and other VO tools.

The workshop will be held in Prague, Czech Republic, from April 16 to 20, 2018, at Institute of Atmospheric Physics of the Czech Academy of Science.
Details and application form are available here:  http://www.europlanet-vespa.eu/call2018.shtml
Deadline for application is 23 February 2018.

Teams which are beneficiaries of the Europlanet2020 contract are welcome to attend the workshop on their own funding - please contact us in advance so we can scale the venue correctly.

Best regards, and happy new year
Stéphane Erard and the VESPA team

 

1) 9th Workshop on Catastrophic Disruption in the Solar System. May 14 - 17, 2018, Kobe

9th Workshop on Catastrophic Disruption in the Solar System (CD9)

Date: May 14 - 17, 2018
Venue: Ikuta shrine (Ikuta Jinja Kaikan), Sannomiya, Kobe, Japan

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


IMPORTANT DATES:

Abstract submission and registration open: Jan. 9, 2018
Deadline for abstract submission and application for early registration: Feb. 28, 2018
Final deadline for application of registration, and excursion & banquet: April 9, 2018


PRELIMINARY PROGRAM:

CD9 will take place over 3 and 1/2 days, with both morning and afternoon sessions on May 14, 15 and 17, and a morning session on May 16. The program will include both invited and contributed talks divided across the following four research areas:

1- Observations and Missions
2- Experiments and Scaling Laws
3- Simulations/Modeling
4- Meteorites

Invited speakers are:
Jean-Baptiste Vincent (DLR, Germany)
Kevin Walsh (SwRI, USA)
Andy Cheng (APL/JHU, USA)
Desiree Cotto-Figueroa (Univ. Puerto Rico)
Masahiko Arakawa (Kobe Univ., Japan)
Angela Stickle (APL/JHU, USA)
Megan Burk-Syal (LLNL, USA)
Nicole Lunning (Smithsonian Inst., USA)
Guy Libourel (Obs. Cote d'Azur, France)

Since we want to leave enough time for discussions, there may be more abstracts submitted than can be accommodated as talks. For authors of abstracts which are accepted but not selected to give contributed talks, electronic posters (one page, PDF format) will be requested. These posters will be put on the workshop website during the workshop for discussion. In addition, there will be a time slot in the program for three-minute oral presentations for the presenters of these posters.


ABSTRACTS AND REGISTRATION:

Abstracts submission and registration will have to be done by the online tool linked from the meeting website. Upon submission, the participant should create an ID account, log in the registration site of the workshop, and fill the registration application form and abstract submission form on the web site. More details will be available on the web site (CD9 web > Abstracts & Registration) at the time of the opening of abstract submission and registration.

The SOC will make decisions on abstract acceptance and will notify the decision by March 9, 2018. The program will be available by the end of March.

If the number of participants exceeds the capacity of the workshop (about 75 participants) at or after the deadline of the early registration, we will close the registration before April 9.


PAYMENT:

No payment is required at the time of application for registration.
Participants should pay the registration fee by cash in Japanese yen at on-site registration. The LOC won’t accept credit card nor foreign currency.

Rates for professionals are:
Early registration rate: 12,000 JPY (until Feb 28, 2018, JST)
Late registration rate: 15,000 JPY (after Feb. 28 and until April 9, 2018, JST)

Rates for students are:
Early registration rate: 8,000 JPY (until Feb 28, 2018, JST)
Late registration fee will be 10,000 JPY (after Feb. 28 and until April 9, 2018, JST)

Registration for professionals & students includes admission to scientific sessions, meeting materials, beverage and refreshments during sessions and breaks, and admission to the Sunday ice breaker at Center for Planetary Science (CPS), Kobe University.
The registration fee DOES NOT include the fee of excursion & banquet.

The rate for excursion & banquet for registered professionals and students is 12,000 JPY.

The rate for accompanying person is 12,000 JPY for the three social events and admission to the venue.

On-site registration is available on the evening of Sunday, May 13 at CPS, and from Monday, May 14 to Thursday, May 17 at the venue.


SOCIAL EVENTS:

There will be an excursion and two evening social events for all CD9 Workshop participants and their registered accompanying persons.

Sunday evening, May 13: Ice breaker - at CPS located in the Port Island.

Wednesday afternoon, May 16: Excursion - Bus tour to Himeji Castle. Himeji castle is an old beautiful castle. It is one of the first UNESCO World Heritage Sites in Japan.

Wednesday evening, May 16: Banquet - A dinner cruise to enjoy the illumination of Kobe city and a long suspension bridge, Akashi Kaikyo Bridge.

TRAVEL:

There are direct flights to Kansai Airport (KIX) from abroad. If you land on Tokyo/Narita first, you can fly to either Kobe Airport (UKB), Osaka Airport (ITM), or Kansai Airport (KIX). You can also come by trains; a local train to the Tokyo Station and a super-express train (Shinkansen) from Tokyo to the Shin-Kobe Station. The expected time from the airports and the Shin-Kobe station to downtown Kobe (Sannomiya) are:

From KIX terminal 1: 65 min. by Airport Limousine (1,950 JPY)
From UKB: 30 min. by Port Liner (330 JPY)
From ITM: 40 min. by Airport Limousine (1,050 JPY)
From Shin-Kobe Sta.: 20 min. by walk (subway, taxi, and local bus are also available)


ACCOMODATION AND OTHER INFORMATION:

Available in the 1st circular.
http://www.impact-res.org/CD2018/Catastrophic_Disruption_2018/Welcome_files/1st_announcement.html

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

SOC:
Neyda Abreu (Pen State University, USA) and
Patrick Michel (Observatoire de la Cote d'Azur, Nice, France), co-Chairs
Erik Asphaug (University of Arizona, USA)
Bobby Bus (University of Hawaii, USA)
Adriano Campo Bagatin (Universidad de Alicante, Spain)
Dan Durda (Southwest Research Institute, Boulder CO, USA)
Kevin Housen (University of Washington, USA)
Akiko Nakamura (Kobe University, Japan)

LOC :
Akiko Nakamura (Kobe University), Chair
Masahiko Arakawa (Kobe University)
Naoyuki Hirata (Kobe University)
Keiji Ohtsuki (Kobe University)
Fumihiko Usui (Kobe University)
Minami Yasui (Kobe University)

This workshop is supported by Japan Society for the Promotion of Science (JSPS) Core-to-Core Program "International Network of Planetary Sciences”, and CPS of Kobe University.


2) poste de DR2 en section 4, avec possibilité  de recrutement externe, pour le GSMA, Reims

(http://www.univ-reims.fr/gsma/).

La thématique de la section 4 - Atomes et molécules, optique et lasers,
plasmas chauds - inclut explicitement la spectroscopie atomique et
moléculaire appliquée à l'astrophysique. Ce concours peut donc concerner
des candidats produisant une recherche à l'intersection des thématiques
de la section 4 et des activités de planétologie du GSMA (atmosphères
planétaires et exoplanètes).

Pour information:
* Site de la section 4:
  http://www.cnrs.fr/comitenational/sections/section.php?sec=04
* Site du concours :
  http://gestionoffres.dsi.cnrs.fr/fo/offres/detail-fr.php?&offre_id=9
* Site du GSMA :
  http://www.univ-reims.fr/gsma
* Equipe planétologie du GSMA:
  https://planeto.univ-reims.fr/

Contacts :
Directeur du GSMA / Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
Groupe planétologie / Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.


3) EGU 2018 Extraterrestrial Seismology Session - 8-13 April 2018, in Vienna

This session discusses advances in seismic instrumentation and seismological methodology aimed at investigating terrestrial planets, icy moons, and small bodies.

We welcome contributions presenting (1) robust and low-power seismic instrumentation adequate for space, including new deployment and sensor concepts: miniaturization, rotational sensors, or sensors for atmospheric recordings of seismic waves; (2) seismological methods adaptable to cases of limited data availability or harsh conditions on extraterrestrial bodies: dealing with single-station setups, scarce networks, strong background noise, lack of meta-deta etc.; (3) insights obtained from previous and recent missions such as Apollo and Rosetta, preparations for seismic data processing of the InSight mission to Mars, as well as simulations of seismic experiments on asteroids, comets, icy moons etc.

We especially invite contributions presenting seismological experiments in challenging, i.e. analogue terrestrial environments, e.g. experiments on (floating) ice, in the oceans, or in deserts.

Please consider submitting an abstract to the session PS5.3/SM1.03
https://meetingorganizer.copernicus.org/EGU2018/session/28537
The abstract submission deadline is 10 Jan 2018, 13:00 CET.

Best regards,
Stefanie Hempel, Brigitte Knapmeyer-Endrun, Martin Knapmeyer, Savas Ceylan, Simon C. Stähler


4) Research Associate in Planetary Physics, Imperial College London, deadline 10 January 2018

please find below an opportunity at ICL:

Research Associate in Planetary Physics, Imperial College London.
Closes: 10th January 2018
http://www.jobs.ac.uk/job/BGJ963/research-associate-in-planetary-physics


5) ESLAB-52 Symposium "Comparative aeronomy and plasma environment of terrestrial planets", 14-18 May, 2018, ESTEC

we would like to remind you about the ESLAB 52 symposium
Comparative aeronomy and plasma environment of terrestrial planets
to be held on 14-18 May 2018 at ESTEC/ ESA in Noordwijk, the Netherlands.

Below you can find description of the symposium.
In the beginning of January we will open the web site and call for abstracts
with submission deadline in the beginning of February. We will inform you accordingly.

We would like to strongly encourage you to participate in the symposium.
Please distribute this message among your colleagues working in the field.
Merry Christmas and Happy New Year !

Dima Titov and Bruce Jakosky
Convenors of the Symposium
_____________________________________________

ESLAB-52 Symposium
Comparative aeronomy and plasma environment of terrestrial planets
14-18 May 2018, ESTEC/ ESA, Noordwijk, the Netherlands.

Processes in the upper atmospheres, ionospheres and magnetospheres of terrestrial
planets and their interactions with the solar wind are of great importance for our understanding
of atmospheric losses to space and evolution of climates. Spacecraft observations
at Mars, Venus, Earth and Titan, as well as Moon, Mercury and other atmosphere-less bodies
provided a wealth of data that allow characterization of  the processes in all their diversity
and in a comparative manner. The wide range of boundary conditions found in the Solar System
provides tremendous input into understanding evolution of the atmospheres of exoplanets
as driven by aeronomy processes.

The symposium will address the processes in the upper atmospheres and plasma envelopes
of all terrestrial planets, including escape and atmospheric evolution.
The experimental results from MAVEN, Mars Express, Venus Express, Pioneer-Venus, Cluster, Swarm, Messenger
and other space missions will form the basis of the symposium programme.
They will be complemented by results from theoretical investigations and numerical modelling.
The symposium will be organized with 5 days of sessions that will include invited summary talks,
oral presentations, poster sessions and discussions.


6) Virginia Initiative on Cosmic Origins (VICO): Postdoc positions

We are pleased to announce the new Virginia Initiative on Cosmic Origins (VICO) that, with Eric Herbst and others, we are helping to set up at the University of Virginia. Please see

http://cosmicorigins.space/

for more information.

There are three or more Cosmic Origins postdoctoral fellowships (Jan. 15th deadline) being advertised as part of this initiative, including fellowships in partnership with Chalmers and MPE:

https://jobregister.aas.org/ad/c0b0a45b

We expect there will be workshops and conferences hosted by VICO in the coming years and we look forward to welcoming you to Charlottesville in the near future!

Best regards,

Jonathan Tan


7) Call for abstracts at the AOGS 2018, 3-8 June, Hawaii

we invite you to submit abstracts to the following sessions taking place at the upcoming AOGS 2018 (June 3-8, 2018) in Hawaii.


The abstract submission deadline is 19 January 2018.

More information can be found on the AOGS website:
http://www.asiaoceania.org/aogs2018/public.asp?page=home.htm


PS6: Magnetospheres, Atmospheres, Exospheres of Outer Planets and Their Satellites

This session welcomes papers about magnetospheres, atmospheres, exospheres of outer planets and their satellites with special emphasis on observations (both from space and from the ground), modelling, and theoretical interpretation. Abstracts on satellite interactions with their neutral and charged environments, supporting laboratory investigations and concepts for future spacecraft missions and investigations are also relevant to this session. We especially welcome papers about the Cassini mission Grand Finale time period as well as results from the most recent Juno data.

Conveners:
Dr. Norbert Krupp (Max Planck Institute for Solar System Research, Germany), Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.

Dr. Linda Spilker (Jet Propulsion Laboratory, United States), Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
Dr. Scott Bolton (Southwest Research Institute, United States), Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser. 

Prof. Sushil Atreya (University of Michigan, United States),Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.

PS16 : Cassini’s Grand Finale Science Highlights and Discoveries

Session Description The Cassini-Huygens Mission to Saturn ended in a dramatic plunge into Saturn’s atmosphere on September 15, 2017 sending back in-situ data as long as possible.  The final year of the mission included 20 Ring-Grazing orbits just outside the rings and a series of 22 highly inclined “Grand Finale” orbits with closest approach between the innermost D ring and Saturn’s upper atmosphere.  The final 22 orbits enabled the opportunity for unique science observations including: probing of gravitational and magnetic field moments to higher order and precision; determining the ring mass; in-situ sampling of the plasma environment, upper atmosphere and exosphere; and imaging both Saturn and rings at high resolution. Already data obtained on these orbits have led to surprising initial results. We propose a multi-disciplinary session to report on analysis and modeling of data collected during this once-in-a-lifetime opportunity to explore Saturn up close and personal.

Conveners:
Dr. Scott Edgington (Jet Propulsion Lab / California Institute of Technology, United States), Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
Prof. Sushil Atreya (University of Michigan, United States), Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser. 

Dr. Athena Coustenis (Paris Observatory, France), Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
Dr. Wing-Huen Ip (National Central University, Taiwan), Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.

 

PS18 : Understanding Icy Worlds, Ocean Worlds, and Habitability

This session will be devoted to understanding icy worlds in the outer solar system, including those containing subsurface oceans, their possible analogues around other stars, and their associated processes and geochemistry that might enable them to support life. The session will include solicited and contributed presentations addressing observational, laboratory, and theoretical studies relevant to past, ongoing, and future missions.

Relevant subtopics include:
(1) interior structure, composition, and thermal evolution,
(2) surface geology and composition,
(3) orbital dynamics and tidal interactions

Conveners:
Dr. Steven Vance (Jet Propulsion Laboratory, California Institute of Technology, United States) Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.

Dr. Frank Sohl (German Aerospace Center (DLR), Germany) Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser. 

Dr. Athena Coustenis (Paris Observatory, France), Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
Dr. Mathieu Choukroun (Jet Propulsion Laboratory, California Institute of Technology, United States) Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.
Dr. Jun Kimura (Osaka University, Japan) Cette adresse e-mail est protégée contre les robots spammeurs. Vous devez activer le JavaScript pour la visualiser.

PS22: Field and Laboratory Studies in Support of Planetary Infrared Remote Sensing
This session will highlight the importance of comprehensive analog studies towards understanding planetary remote sensing datasets, with a focus on the near infrared and thermal infrared. Contributions that probe the links between the small-scale of laboratory (microns to millimeters) and ground/airborne field (centimeters to meters) measurement to the large-scale (10s meters to kilometers) in remote sensing observations to better interpret the dynamics, chemistry, composition, thermophysics, and physical properties of surfaces and atmospheres are encouraged. This session is open to a diverse range of planetary bodies, including Mercury, Venus, Moon, NEOs, Mars, Martian Moons, MBOs, Trojans, Gas Giants, Ice Giants, Icy Satellites, Irregular Satellites, and Plutoids. New developments of instrumentation and techniques used in field and laboratory studies are also welcome.

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