Understanding radiation effects in dust and icy regolith on airless bodies

About the role

The Planetary Magnetospheres Lab (695) in the Solar System Exploration Division (690) at NASA’s Goddard Space Flight Center seeks a qualified postdoctoral applicant to carry out experimental studies on a newly built ultra-high vacuum radiation simulation chamber in the SpaceREDI (Radiation Effects in Dust and Ice) laboratory.

Responsibilities

This position is strictly laboratory based and the applicant is invited to propose a project using neutral and ion mass spectrometry combined with infra-red spectroscopy to understand the effects of ionizing radiation (i.e., solar wind plasma and photons, magnetospheric plasmas, and cosmic ray particles) in icy regolith analogs representative of comets, polar cold traps at the Moon and Mercury, or icy moons.

Requirements

• A Ph.D. or the equivalent degree in Planetary Science, Physics, Geology, Astrophysics, or a related field.
• Desired laboratory skills include experience with apparatus design and construction of experimental systems, fast ion and electron beams, continuous and pulsed photon sources, ultra-high vacuum techniques, visible and near infrared spectral reflectance measurements, quadrupole mass spectrometers, and associated electronics.
• Desired computer skills include programming, multidimensional data analysis, LabView, Python, Autodesk Inventor, Solidworks, SIMION, Linux/Mac OS, and Windows OS.
• A strong background in at least some of the areas listed above, a proven research ability, and evidence of future research potential.
• Ability to work well independently and cooperatively with a team and to communicate the results of his/her research both orally and in writing.

Qualifications

The successful candidate will have a strong background in at least some of the areas listed above, a proven research ability, and evidence of future research potential. The candidate is expected to be able to work well independently and cooperatively with a team and to communicate the results of his/her research both orally and in writing. Demonstrated written and oral communication skills are highly desirable.

Skills

None specified in the job posting.

Benefits

None specified in the job posting.

Pay

Not specified in the job posting.

Schedule

Not specified in the job posting.

Additional Information

The Planetary Magnetospheres Lab (695) in the Solar System Exploration Division (690) at NASA’s Goddard Space Flight Center seeks a qualified postdoctoral applicant to carry out experimental studies on a newly built ultra-high vacuum radiation simulation chamber in the SpaceREDI (Radiation Effects in Dust and Ice) laboratory. This position is strictly laboratory based, and the applicant is invited to propose a project using neutral and ion mass spectrometry combined with infra-red spectroscopy to understand the effects of ionizing radiation (i.e., solar wind plasma and photons, magnetospheric plasmas, and cosmic ray particles) in icy regolith analogs representative of comets, polar cold traps at the Moon and Mercury, or icy moons.

Radiation is responsible for numerous observed physical and chemical processes on airless bodies, such as implantation of exogenous species and the formation of new molecules through radiolysis (radiation-induced bond rearrangement), stimulated desorption of surface species and production of a surface-bound exosphere (collisionless atmosphere around airless bodies), and molecular migration and radiation-enhanced diffusion into the subsurface that can create local reservoirs of important species. Studies using mass spectrometry and infrared spectroscopy can determine how the physical properties of icy regolith change when exposed to radiation, and the results can provide critical information for the interpretation of observations and development of high-fidelity computational models.

Granular morphology, compositional heterogeneity, and thermal gradients have all been shown to strongly influence radiation, and experiments must be performed to understand of radiation effects in mixed, granular materials that are representative of the composition and structure of airless body regolith. Thus, a major focus of this NPP will the in situ production and characterization of high fidelity icy regolith analogs.

The successful candidate will have a Ph.D. or the equivalent degree in Planetary Science, Physics, Geology, Astrophysics, or a related field. Desired laboratory skills include experience with apparatus design and construction of experimental systems, fast ion and electron beams, continuous and pulsed photon sources, ultra-high vacuum techniques, visible and near infrared spectral reflectance measurements, quadrupole mass spectrometers, and associated electronics. Desired computer skills include programming, multidimensional data analysis, LabView, Python, Autodesk Inventor, Solidworks, SIMION, Linux/Mac OS, and Windows OS.

The successful candidate will have a strong background in at least some of the areas listed above, a proven research ability, and evidence of future research potential. The candidate is expected to be able to work well independently and cooperatively with a team and to communicate the results of his/her research both orally and in writing. Demonstrated written and oral communication skills are highly desirable.

The Planetary Magnetospheres Lab (695) in the Solar System Exploration Division (690) at NASA’s Goddard Space Flight Center seeks a qualified postdoctoral applicant to carry out experimental studies on a newly built ultra-high vacuum radiation simulation chamber in the SpaceREDI (Radiation Effects in Dust and Ice) laboratory. This position is strictly laboratory based, and the applicant is invited to propose a project using neutral and ion mass spectrometry combined with infra-red spectroscopy to understand the effects of ionizing radiation (i.e., solar wind plasma and photons, magnetospheric plasmas, and cosmic ray particles) in icy regolith analogs representative of comets, polar cold traps at the Moon and Mercury, or icy moons.

Radiation is responsible for numerous observed physical and chemical processes on airless bodies, such as implantation of exogenous species and the formation of new molecules through radiolysis (radiation-induced bond rearrangement), stimulated desorption of surface species and production of a surface-bound exosphere (collisionless atmosphere around airless bodies), and molecular migration and radiation-enhanced diffusion into the subsurface that can create local reservoirs of important species. Studies using mass spectrometry and infrared spectroscopy can determine how the physical properties of icy regolith change when exposed to radiation, and the results can provide critical information for the interpretation of observations and development of high-fidelity computational models.

Granular morphology, compositional heterogeneity, and thermal gradients have all been shown to strongly influence radiation, and experiments must be performed to understand of radiation effects in mixed, granular materials that are representative of the composition and structure of airless body regolith. Thus, a major focus of this NPP will the in situ production and characterization of high fidelity icy regolith analogs.

The successful candidate will have a Ph.D. or the equivalent degree in Planetary Science, Physics, Geology, Astrophysics, or a related field. Desired laboratory skills include experience with apparatus design and construction of experimental systems, fast ion and electron beams, continuous and pulsed photon sources, ultra-high vacuum techniques, visible and near infrared spectral reflectance measurements, quadrupole mass spectrometers, and associated electronics. Desired computer skills include programming, multidimensional data analysis, LabView, Python, Autodesk Inventor, Solidworks, SIMION, Linux/Mac OS, and Windows OS.

The successful candidate will have a strong background in at least some of the areas listed above, a proven research ability, and evidence of future research potential. The candidate is expected to be able to work well independently and cooperatively with a team and to communicate the results of his/her research both orally and in writing. Demonstrated written and oral communication skills are highly desirable.

The Planetary Magnetospheres Lab (695) in the Solar System Exploration Division (690) at NASA’s Goddard Space Flight Center seeks a qualified postdoctoral applicant to carry out experimental studies on a newly built ultra-high vacuum radiation simulation chamber in the SpaceREDI (Radiation Effects in Dust and Ice) laboratory. This position is strictly laboratory based, and the applicant is invited to propose a project using neutral and ion mass spectrometry combined with infra-red spectroscopy to understand the effects of ionizing radiation (i.e., solar wind plasma and photons, magnetospheric plasmas, and cosmic ray particles) in icy regolith analogs representative of comets, polar cold traps at the Moon and Mercury, or icy moons.

Radiation is responsible for numerous observed physical and chemical processes on airless bodies, such as implantation of exogenous species and the formation of new molecules through radiolysis (radiation-induced bond rearrangement), stimulated desorption of surface species and production of a surface-bound exosphere (collisionless atmosphere around airless bodies), and molecular migration and radiation-enhanced diffusion into the subsurface that can create local reservoirs of important species. Studies using mass spectrometry and infrared spectroscopy can determine how the physical properties of icy regolith change when exposed to radiation, and the results can provide critical information for the interpretation of observations and development of high-fidelity computational models.

Granular morphology, compositional heterogeneity, and thermal gradients have all been shown to strongly influence radiation, and experiments must be performed to understand of radiation effects in mixed, granular materials that are representative of the composition and structure of airless body regolith. Thus, a major focus of this NPP will the in situ production and characterization of high fidelity icy regolith analogs.

The successful candidate will have a Ph.D. or the equivalent degree in Planetary Science, Physics, Geology, Astrophysics, or a related field. Desired laboratory skills include experience with apparatus design and construction of experimental systems, fast ion and electron beams, continuous and pulsed photon sources, ultra-high vacuum techniques, visible and near infrared spectral reflectance measurements, quadrupole mass spectrometers, and associated electronics. Desired computer skills include programming, multidimensional data analysis, LabView, Python, Autodesk Inventor, Solidworks, SIMION, Linux/Mac OS, and Windows OS.

The successful candidate will have a strong background in at least some of the areas listed above, a proven research ability, and evidence of future research potential. The candidate is expected to be able to work well independently and cooperatively with a team and to communicate the results of his/her research both orally and in writing. Demonstrated written and oral communication skills are highly desirable.

The Planetary Magnetospheres Lab (695) in the Solar System Exploration Division (690) at NASA’s Goddard Space Flight Center seeks a qualified postdoctoral applicant to carry out experimental studies on a newly built ultra-high vacuum radiation simulation chamber in the SpaceREDI (Radiation Effects in Dust and Ice) laboratory. This position is strictly laboratory based, and the applicant is invited to propose a project using neutral and ion mass spectrometry combined with infra-red spectroscopy to understand the effects of ionizing radiation (i.e., solar wind plasma and photons, magnetospheric plasmas, and cosmic ray particles) in icy regolith analogs representative of comets, polar cold traps at the Moon and Mercury, or icy moons.

Radiation is responsible for numerous observed physical and chemical processes on airless bodies, such as implantation of exogenous species and the formation of new molecules through radiolysis (radiation-induced bond rearrangement), stimulated desorption of surface species and production of a surface-bound exosphere (collisionless atmosphere around airless bodies), and molecular migration and radiation-enhanced diffusion into the subsurface that can create local reservoirs of important species. Studies using mass spectrometry and infrared spectroscopy can determine how the physical properties of icy regolith change when exposed to radiation, and the results can provide critical information for the interpretation of observations and development of high-fidelity computational models.

Granular morphology, compositional heterogeneity, and thermal gradients have all been shown to strongly influence radiation, and experiments must be performed to understand of radiation effects in mixed, granular