Chemistry of Planetary and Exoplanetary Atmospheres
The postdoctoral researcher will develop novel instrument techniques based on IR heterodyne remote sensing, nano-photonics, and photonic integrated circuits. Our objective is to enable new measurement capabilities for studying planetary chemistry, habitability, astrobiology, and climate evolution.
In addition, researchers in exoplanetary science are strongly encouraged to apply as well. We are developing a coupled ocean-rock-atmosphere chemistry model for extrasolar planets, and welcome applicants to conduct research in habitability evolution and biosignatures for exoplanets.
Location:
Jet Propulsion Laboratory
Pasadena, California
Field of Science:Planetary Science
Advisors:
Pin Chen
pin.chen@jpl.nasa.gov
818-393-0412
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:
- U.S. Citizens;
- U.S. Lawful Permanent Residents (LPR);
- Foreign Nationals eligible for an Exchange Visitor J-1 visa status; and,
- Applicants for LPR, asylees, or refugees in the U.S. at the time of application with 1) a valid EAD card and 2) I-485 or I-589 forms in pending status
- Degree: Doctoral Degree.
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