JWST Solar System PostDoc at Observatoire de Paris

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Current state: Approved and Notify DPS Secretary
Department: LESIA
City: Paris
Country: France
Contact Person: Emmanuel Lellouch
Contact Email: [email protected]
Institution: Observatoire de Paris
Application Due Date: Friday, October 01 2021
Web Link: https://jobregister.aas.org/ad/52b1806c

Applications are open for a Postdoctoral Research position within the planetary science group of LESIA at Observatoire de Paris, France. The position is in relation with the Early Release Science (ERS) Program on JWST “Observations of the Jovian System as a Demonstration of JWST’s Capabilities for Solar System Science’’, to which LESIA is associated through co-PI and co-I ships . JWST is expected to be launched in the fall of 2021, and a fraction of this ERS program will be devoted to the study of the tenuous atmo/exospheres of Io and Ganymede with MIRI and NIRSpec. In particular, Io’s atmosphere will be studied from observing of SO2 gas at 8.6 and 7.3 μm, and Ganymede’s exosphere will be targeted through fluorescent emissions from H2O (6.5 μm), CO (4.65 μm), and CO2 (4.25 μm). The analysis of the data will require the development of tailored non-LTE models for these molecular features, coupled with physical (temperature, densities) models of the two objects. The successful applicant will participate in the development of a versatile non-LTE code applicable to both objects. He/she will also be involved in data reduction, modelling, and interpretation, after data are acquired (nominally in June-August 2022). Experience in radiative transfer is required, and preference will be given to applicants with experience with non-LTE aspects.

The position is available for two years, starting anytime between Oct. 01, 2021 and February 01, 2022. Gross salary will be about 3200 Euros/months. Applications will be considered as they come and welcome until Oct. 01, 2021.

Planetary Astronomer

Posted on
Current state: Approved
Department: PDS Ring-Moon Systems Node
City: Mountain View
State/Province: CA
Country: USA
Contact Person: Armine Saroian
Contact Email: [email protected]
Institution: SETI Institute
Application Due Date: Friday, January 15 2021
Web Link: https://www.seti.org/jobs/planetary-astronomer

SETI INSTITUTE

POSITION DESCRIPTION

Position Title:                                      Planetary Astronomer

FLSA Status:                                        Full-Time, Exempt

Reports to:                                           NODE Manager

Location:                                              Mountain View, CA     

                                                                                                                                                                                                                                                                                                    

Position Summary:

The SETI Institute is seeking a Planetary Astronomer to support the work of the Ring-Moon Systems Node (RMS) of NASA’s Planetary Data System (PDS). The successful applicant will be an integral part of the RMS Node Team, which shares responsibility for archiving, augmenting, cataloging, and distributing key data sets from NASA’s missions to the outer planets. The PDS ensures that the entire community of planetary scientists has seamless access to NASA’s archive of planetary data. The RMS Node’s primary focus is on data sets relevant to planetary systems in the outer solar system, including the rings and moons of the outer planets, atmospheric research, and astrogeology.

The astronomer will focus primarily on ongoing efforts to enhance the scientific usability of RMS data sets, which include those from the Cassini, Voyager, Galileo, and New Horizons missions, as well as those from the Hubble Space Telescope and Earth-based observatories. We seek a curious and creative individual who is eager to work with data from diverse instruments and missions. The curation of planetary data requires someone who is able to understand the data’s scientific importance, assess the data’s validity, converse knowledgeably with fellow scientists, and confirm that documentation and descriptive metadata are sufficient for the needs of current and future scientists.

The astronomer will collaborate closely with the Node Manager, Dr Matt Tiscareno, on all aspects of RMS Node planning and task management. They will understudy with longtime RMS Deputy Manager, Dr Mitch Gordon, and prepare to carry on his work as he approaches retirement.

This is a full-time position with full benefits. However, the astronomer will be encouraged to seek additional research funding on any topic of their choosing including, but not limited to, topics related to the Node’s extensive data holdings. The position offers substantial growth potential for applicants who are able to demonstrate mastery of the key requirements.

Responsibilities:

  • Work with NASA’s planetary missions and other data providers on the design, preparation, submission, and peer review of archived data sets.
  • Design and maintain PDS “dictionaries”, which are used to capture the key information about astronomical observations.
  • Develop data processing pipelines to validate existing data and metadata, and convert it into the new, modern “PDS4” standard.
  • Generate and assemble supporting metadata so the data products can be integrated into OPUS, our online search engine (see https://opus.pds-rings.seti.org).
  • Work within the larger PDS community to develop and enhance archiving standards.
  • Represent the Node at PDS working groups, project meetings, scientific meetings, and to NASA.
  • Help with website content, hardware management, and research tool development.
  • Participate in team discussions about the latest results in planetary astronomy and related fields.

Requirements:

  • A Ph.D. or equivalent career experience in planetary astronomy, astrophysics, physics, or a closely related field. 
  • Experience in scientific data analysis and in writing research papers for peer review.
  • A personal and demonstrable scientific interest in planetary systems is highly desirable.
  • Experience with computer programming for scientific applications is required. Proficiency with the Python programming language is highly desirable.
  • Excellent oral and written communication skills.
  • Must be detail oriented, pro-active, and flexible.
  • Should have the initiative to work independently and as a team player.
  • Ability to multi-task in a fast-paced environment.
  • Willing to accept major responsibilities and able to perform under pressure.

Diversity and Equity

All qualified applicants will receive consideration for employment without regard to race, color, religion, sex, sexual orientation, gender identity, or national origin.

The SETI Institute is an Affirmative Action Employer and members of underrepresented communities and demographics are particularly encouraged to apply, including women, people of color, LGBTQ and people with disabilities.

Employment Details:

Applicants should be prepared to establish residence in the San Francisco Bay Area by the end of Summer 2021, within a comfortable commuting distance of Mountain View, California.

 

 

JPL POSTDOC IN OCEAN WORLDS ICE SHELLS

Posted on
Current state: Approved
City: Pasadena
State/Province: California
Country: USA
Contact Person: Samuel Howell
Contact Email: [email protected]
Institution: Jet Propulsion Laboratory
Application Due Date: Thursday, December 31 2020
Web Link: https://jpl.jobs/jobs/2020-12443-Postdoctoral-Researcher-Ocean-Worlds-Ice-Shell-Modeling

In search of an enthusiastic researcher to join a wonderful group of
icy explorers at JPL! JPL is accepting applications for a postdoctoral
research position in geophysical modeling relevant to the icy layers of
Jupiter’s moon Europa, and potentially to other ocean worlds. This may
involve modeling of tectonic processes, constructing analytical or
first-principles arguments, describing ice shell evolution, melting,
freezing, and/or non-ice chemistry incorporation. These results will be
used to understand the potential for future measurements by robotic
spacecraft, and to derive environmental constraints on potential future
concepts for subsurface and ocean access. Dr. Samuel Howell, an ocean
worlds research scientist in the Planetary Interiors and Geophysics
group, will serve as the primary postdoctoral advisor. Please contact
samuel.m.howell at jpl.nasa.gov with any questions. Candidates should have
a recent Ph.D. in geology, planetary science, physics, or a related
field, with a strong background in analytical, numerical, and/or
statistical analysis as applied to geophysical research. Experience in
research relevant to the outer planet satellites and the impacts of
geophysical processes on habitability are highly desirable.

 

See full job details at link.

NASA Astrobiology Postdoctoral Opportunity at University of Hawaii

Posted on
Current state: Approved and Notify DPS Secretary
Department: Hawai'i Institute of Geophysics and Planetology
City: Honolulu
State/Province: HI
Country: USA
Contact Person: Sarah Fagents
Contact Email: [email protected]
Institution: University of Hawai'i
Application Due Date: Thursday, November 01 2018

Postdoctoral Research Opportunity at the University of Hawaii: Fluid migration in Titan’s ice shell

As part of the new NASA Astrobiology Institute (NAI) project “Habitability of Hydrocarbon Worlds: Titan and Beyond”, we are investigating the mechanisms and pathways by which biosignature-hosting materials might be transported from a habitable ocean environment to the surface, where they could be recognized by remote sensing instruments.  These mechanisms might include cryovolcanism, solid state convection in the ice shell, fracture/fault propagation, and the formation of subsurface fluid reservoirs that might facilitate fluid migration to the surface. See nai.nasa.gov/teams/can-8/jpl-titan/ for a more detailed description of the overall project.

An opportunity exists in this area for a postdoctoral researcher to develop a proposal for the NASA Astrobiology Postdoctoral Program, for a project to be pursued at the University of Hawaii.  The desired candidate will have a solid physics, math, or geology/geophysics background, and interests/expertise in numerical modeling, cryomagmatism, ice physics, Titan and/or other icy satellites.  The next deadlines for this program are November 1 and March 1.  If the proposal is selected for funding, the anticipated start dates would be spring/summer 2019 or fall 2019, respectively.  More details are available at nai.nasa.gov/funding/postdoctoral-fellowship-program

Please contact Sarah Fagents at [email protected] for more information.

Graduate Research Opportunity at the University of Hawaii: Fluid Migration in Titan’s Ice Shell

Posted on
Current state: Approved and Notify DPS Secretary
Department: Hawaii Institute of Geophysics and Planetology / Department of Earth Sciences
City: Honolulu
State/Province: HI
Country: USA
Contact Person: Sarah Fagents
Contact Email: [email protected]
Institution: University of Hawai'i
Application Due Date: Tuesday, January 15 2019

Graduate Research Opportunity at the University of Hawaii: Fluid Migration in Titan’s Ice Shell

As part of the new NASA Astrobiology Institute (NAI) project “Habitability of Hydrocarbon Worlds: Titan and Beyond”, we are investigating the mechanisms and pathways by which biosignature-hosting materials might be transported from a habitable ocean environment to the surface, where they could be recognized by remote sensing instruments.  These mechanisms might include cryovolcanism, solid state convection in the ice shell, fracture/fault propagation, and the formation of subsurface fluid reservoirs that might facilitate fluid migration to the surface. See nai.nasa.gov/teams/can-8/jpl-titan/ for a more detailed description of the overall project.

An opportunity exists in this area at the University of Hawaii (UH) for a graduate student to pursue their PhD, enrolled through the Department of Earth Sciences (formerly known as Geology and Geophysics; www.soest.hawaii.edu/GG/), but hosted within the Hawaii Institute of Geophysics and Planetology (HIGP; www.higp.hawaii.edu).  The deadline for applying to graduate school at UH is January 15 for Fall 2019 admission; more details at www.soest.hawaii.edu/GG/admissions/gg_admissions.html

The desired candidate will have a solid physics, math, or geology/geophysics background, and interests/expertise in numerical modeling, cryomagmatism, ice physics, Titan and/or other icy satellites.

Please contact Sarah Fagents at [email protected] for more information.

Physics and Chemistry of Outer Planetary Ice Analogs

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Current state: Approved and Notify DPS Secretary
Department: Planetary Sciences
City: Pasadena
State/Province: California
Country: USA
Contact Person: Murthy Gudipati
Contact Email: [email protected]
Institution: Jet Propulsion Laboratory
Application Due Date: Tuesday, May 01 2018
Web Link: https://postdocs-jpl.icims.com/jobs/

Physics and Chemistry of Outer Planetary (Europa) Ice Analogs

Apply at URL: https://postdocs-jpl.icims.com/jobs/

Job Locations US-CA-Pasadena

Requisition ID: 2018-9183; Relocation Eligibility: Yes; Hiring Organization: 3227 – PLANETARY ICES; Work Authorization: Ability to Obtain Work Authorization; Discipline: Planetary Science; Advisor Name: MURTHY GUDIPATI; Program (Postdoc): JPL

Overview

The Jet Propulsion Laboratory invites applications for a postdoctoral research position in the Planetary Ices Group. Drs. Murthy Gudipati and Bryana Henderson will serve as postdoctoral advisors to the selected candidate with Dr. Gudipati acting as primary. The appointee will carry out research in collaboration with the postdoctoral advisors, resulting in publications in the open literature. The postdoctoral position is available immediately.

Responsibilities

The research work will focus on the area of physics and chemistry of outer planetary ice analogs using laboratory simulations and spectroscopy. This position is aimed at understanding the evolution of organic matter in ices under high-radiation conditions such as on Europa. The successful candidate should have thorough hands-on experience in similar research activity and should be able to participate in multiple projects. In addition to the fundamental research mentioned above, the appointee will have an opportunity to participate in next-generation space instrumentation concepts, mission concepts, and observations.

Qualifications

Candidates should have a recent Ph.D. in chemistry, physics, astronomy or planetary sciences and a strong motivation to undertake this multidisciplinary research. Experience and expertise in the following techniques are highly desired: low-temperature techniques, laboratory ultraviolet and infrared spectroscopy, laser spectroscopy, ultra-high vacuum techniques, and mass-spectrometry. Candidates who have received their PhD within the past five years since the date of their application are eligible. Postdoctoral positions are awarded for a minimum of one-year period and may be renewed up to a maximum duration of three years.

 

The Jet Propulsion Laboratory is a federal facility. Due to rules imposed by NASA, JPL will not accept applications from citizens of designated countries unless they are Legal Permanent Residents of the U.S or have other protected status under 8 U.S.C. 1324b(a)(3). The Designated Countries List is available at http://oiir.hq.nasa.gov/nasaecp/.

USRA/LPI Postdoctoral Fellow in Planetary Surface Processes

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Current state: Approved and Notify DPS Secretary
Department: Lunar and Planetary Institute
City: Houston
State/Province: TX
Country: USA
Contact Person: Dr. Edgard G. Rivera-Valentín
Contact Email: [email protected]
Institution: Universities Space Research Association
Application Due Date: Wednesday, March 21 2018
Web Link: https://usra-openhire.silkroad.com/epostings/index.cfm?fuseaction=app.jobinfo&jobid=698&source=ONLINE&JobOwner=992390&company_id=16640&version=1&byBusinessUnit=NULL&bycountry=0&bystate=1&byRegion=US_US-TX&bylocation=NULL&keywords=&byCat=&proximityCountry=&postalCode=&radiusDistance=&isKilometers=&tosearch=yes&city=

USRA/LPI Postdoctoral Fellow in Planetary Surface Processes

The Universities Space Research Association’s Lunar and Planetary Institute invites applications for a postdoctoral fellow in modeling of planetary surface processes.

The successful candidate will join Dr. Edgard Rivera-Valentín in several projects related to simulating planetary surface process on Mars and the icy moons of Saturn. Projects are interdisciplinary in nature and involve numerical simulations of planetary surface processes and responsibilities in spacecraft data analysis and data management. Applicants should have a recent Ph.D. in planetary science, astronomy, physics, geosciences or a related field. Experience in numerical modeling and proficiency in programming languages is required; experience with MATLAB and IDL is desirable. Candidates with demonstrated experience in a wide array of subfields in planetary science are encouraged to apply. Candidates from underrepresented groups in STEM and those with a demonstrated history of efforts to improve diversity and inclusion in STEM are particularly encouraged.

Interested applicants should apply to the posting at https://usracareers.silkroad.com/ and must submit a cover letter, CV with list of publications, a statement of research interests and plans, and a list of at least three professional references. Review of candidates will begin on March 21, 2018.

PhD Positions in Solar System Science in Göttingen, Germany / Deadline 15 November 2017

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Current state: Approved and Notify DPS Secretary
Department: International Max Planck Research School for Solar System Science at the University of Göttingen
City: Göttingen
State/Province: Lower Saxony
Country: Germany
Contact Person: Dr. Sonja Schuh
Contact Email: [email protected]
Institution: Max Planck Institute for Solar System Research
Application Due Date: Wednesday, November 15 2017
Web Link: https://www.mps.mpg.de/phd/applynow

The International Max Planck Research School for Solar System Science at the University of Göttingen in Germany (Solar System School) offers a research-oriented doctoral program covering the physics of Solar system science. It is jointly run by the Max Planck Institute for Solar System Research (MPS) and the University of Göttingen. Read more at http://www.solar-system-school.de/

The science covered by the department Planets and Comets (one of three departments at the MPS) includes a wide spectrum of planetary research. We study the structure and composition of planets in our solar system as well as dynamic processes. The research includes the deep interior, surfaces, atmospheres and the plasma environment (thin hot charged particles in the environment) of the planets. The main focus lies in the research of the terrestrial planets (Mercury, Venus, Earth, Mars) and the gas giants (Jupiter and Saturn) as well as small bodies including comets and asteroids. We study similarities and differences among the various objects and compare them with each other to better understand the evolution of our solar system.

A list of open PhD projects in planetary sciences and cometary science is available at https://www.mps.mpg.de/phd/open-projects

Solar System School students collaborate with leading scientists in these fields and graduates are awarded a doctoral degree from the renowned University of Göttingen.

The Solar System School is open to students from all countries and offers an international three-year PhD program in an exceptional research environment with state-of-the-art facilities on the Göttingen Campus. Solar System Science is a key research area on Göttingen Campus, performed jointly with the nearby Institute of Astrophysics and the Institute of Geophysics of the Faculty of Physics, the Faculties of Chemistry, Mathematics, Geosciences, and the German Aerospace Center.

Applicants to the Solar System School should have a keen interest in Solar system science and a record of academic excellence. They must have, or must be about to obtain, an M.Sc. degree or equivalent in physics or a related field, including a written Masters thesis (or a scientific publication), and must document a good command of the English language.

Online applications should be submitted before the deadline of 15 November 2017 via https://www.mps.mpg.de/phd/applynow

Postdoctoral Fellowship in Planetary Hydrology

Posted on
Current state: Approved and Notify DPS Secretary
City: Houston
State/Province: TEXAS
Country: USA
Contact Person: Stephen Clifford
Institution: Lunar and Planetary Institute
Application Due Date: Monday, October 17 2016
Web Link: http://www.lpi.usra.edu/planetary_news/2016/08/01/job-opportunity-postdoctoral-fellowship-in-planetary-hydrology-lunar-and-planetary-institute/

The Universities Space Research Association’s Lunar and Planetary Institute (LPI), invites applications for a postdoctoral fellowship that will address a variety of investigations related to the hydrologic evolution of Mars. Applicants, with recent PHDs, should have a strong background in math, hydrology, groundwater modelling (MODFLOW), and computer programing (FORTRAN and/or Matlab). Additional experience in one or more of the following: planetary science, remote sensing, and/or Global Climate Modeling, is preferred but is not a prerequisite for selection.

The successful candidate will work with Dr. Stephen Clifford at the Lunar and Planetary Institute in Houston, Texas. The position is for two years, with a possible extension to a third year. The candidate is expected to work half-time in support of Dr. Clifford’s NASA-funded research and half-time on their own individual research projects, which may utilize the computational and analytical resources at LPI and the nearby NASA Johnson Space Center. The candidate will be encouraged to propose for external funding, participate in grant review panels and analysis groups, and become further involved with spacecraft missions.

At the LPI, the successful candidate will interact with scientists with a broad range specialties and backgrounds, including Astromaterials, lunar science and exploration, Mars, Venus, and icy/ocean worlds. LPI scientists maintain active collaborations with the Astromaterials Research and Exploration Science (ARES) group at Johnson Space Center and with faculty in the geosciences departments of Rice University and the University of Houston.

The candidate must be able to pass a detailed government background investigation. Applicants should apply to the posting at https://usracareers.silkroad.com/  and include a letter of interest, a curriculum vita with a list of publications, a brief (maximum three pages) statement of research interests, and a list of three references. Review of candidates will begin on October 17, 2016, with a hiring decision as soon as possible thereafter. Additional information on current research and facilities at the LPI and at JSC can be found through our website www.lpi.usra.edu and www.usra.edu.

USRA is an independent, non-profit 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 engages the creativity and authoritative expertise of the research community to develop and deliver sophisticated, forward-looking solutions to Federal agencies and other customers – on schedule and within budget.

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

Two Faculty Positions in Astrophysics at Instituto de Astrofisica de Atacama, Copiapo (Chile)

Posted on
Current state: Review
Department: Instituto de Astrofisica de Atacama
City: Copiapo
State/Province: Atacama
Country: Chile
Contact Person: Mauro Barbieri
Contact Email: [email protected]
Institution: Universidad de Atacama
Application Due Date: Friday, March 18 2016
Web Link: http://eas.unige.ch/jobs.jsp?id=671

The Instituto de Astrofisica de Atacama (IAA) at the Universidad De Atacama (UDA) in Copiapo (Chile) invites applications for two faculty positions to join the IAA team.
The successful candidates will join a group of five faculty working on a broad range of research topics and will have access to the Chilean Time in a broad array of facilities, including ALMA, VLT, Gemini, Magellan, LSST, GMT and the E-ELT. 

We are particularly interested in candidates with strong experience in one or more of these fields: 

-Origin, structure and evolution of planets, satellites, and minor bodies in the Solar System; 
-Extrasolar Planets; 
-Formation, structure and evolution of stars; 
-Milky Way: stellar populations, star clusters, variable stars, galactic structure; 
-Terrestrial Mars analogs; 
-Astrobiology. 

The positions carry teaching duties in astronomy at the undergraduate level, with a load of 6h per week. The working language is English. While knowledge of Spanish is not required (teaching can be done in English), the successful candidates are expected to teach in Spanish within two years. 
The appointment at UDA will be for three years, with a first probation year, and the position is further extendable subject to performance. 

Applicants should have a PhD in astronomy or physics or related sciences completed at least 3 years prior to the starting day of the contract. 

To receive full consideration, applications must be sent by Friday 18 of March 2016, although the positions will remain open until filled. Start date is expected to be October 2016. 

Applications must be submitted by e-mail to Mauro Barbieri (mauro.barbieri @ uda.cl), and they should include: 
1) Cover letter, 
2) Curriculum Vitae, 
3) List of publications, 
4) Statement of recent research achievements (max. 2 pages), 
5) An outline of future research (min. 2 pages, max. 10 pages), 
6) The contact details of three referees (one needs to be the last employer, the others needs to be aware of the recent work of the candidate). 

Questions may be addressed to the previous e-mail address. 

Relevant links: 

Universidad de Atacama 
http://www.uda.cl 

Instituto de Astrofisica de Atacama 
https://sites.google.com/site/grupoastrouda 

Convocatoria Programa de Insercion de Investigadores en la UDA 
http://www.vrip.uda.cl/frontend/noticia_completa/104