Tectonics and Evolution of the Terrestrial Planets

Tectonics and Evolution of the Terrestrial Planets

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Tectonics and Evolution of the Terrestrial Planets

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Join to apply for the Tectonics and Evolution of the Terrestrial Planets role at ORAU

Organization

National Aeronautics and Space Administration (NASA)

Organization

National Aeronautics and Space Administration (NASA)

Reference Code

0039-NPP-NOV25-JPL-PlanetSci

How To Apply

All applications must be submitted in Zintellect

Please visit the NASA Postdoctoral Program website for application instructions and requirements : How to Apply | NASA Postdoctoral Program (orau.org)

A complete application to the NASA Postdoctoral Program includes :

• Research proposal
• Three letters of recommendation
• Official doctoral transcript documents

Application Deadline

11 / 1 / 2025 6 : 00 : 59 PM Eastern Time Zone

Description

About the NASA Postdoctoral Program

The NASA Postdoctoral Program (NPP) offers unique research opportunities to highly-talented scientists to engage in ongoing NASA research projects at a NASA Center, NASA Headquarters, or at a NASA-affiliated research institute. These one- to three-year fellowships are competitive and are designed to advance NASA’s missions in space science, Earth science, aeronautics, space operations, exploration systems, and astrobiology.

Description :

Earth-like planets, including exoplanets. This research will contribute to understanding planetary evolution and habitability by examining the links between interior, surface, and atmospheric evolution. Specific topics include modeling of the following processes :

factors that influence heat flow such as crustal and elastic thickness, volcanic history, and near surface thermal properties.

Interior thermal evolution and the role of mantle plumes on affecting surface geology and volatile evolution.

Tectonic processes that provides constraints on thermal evolution, such as rifting

Surface processes that provide constraints on the history of resurfacing on Venus, including possible signatures of climate change.

Modeling approaches include analytic and numerical methods. Model constraints come from data analysis of gravity, topography, radar, imaging, and surface temperature data.

Smrekar, S.E. and Sotin, C., Constraints on mantle plumes on Venus : Implications for volcanism and volatile history, Icarus, doi : 10.1016 / j.icarus.2011.09.011, 2012. Smrekar, S.E., E.R. Stofan, N. Mueller, A. Treiman, L. Elkins-Tanton, J. Helbert, G. Piccioni, and P. Drossart

Location :

Jet Propulsion Laboratory

Pasadena, California

Field of Science : Planetary Science

Advisors : Sue Smrekar

suzanne.e.smrekar@jpl.nasa.gov

818-354-4192

Applications with citizens from Designated Countries will not be accepted at this time, unless they are Legal Permanent Residents of the United States. A complete list of Designated Countries can be found at : https : / / www.nasa.gov / oiir / export-control.

Eligibility is currently open to :

Questions about this opportunity? Please email npp@orau.org

Point of Contact

Mikeala

Eligibility Requirements

Seniority level

Seniority level

Internship

Employment type

Employment type

Full-time

Job function

Job function

Other

Industries

Government Administration

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