HelioWebJonathan J. Fortney
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A[Jonathan J. Fortney]
AC["Associated Concepts (19)"]
AW["Authored Works (17)"]
CA["Linked Co-Authors (3)"]
CI["Linked Collaborating Institutions (28)"]
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AW== author ==>CA
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click AW "#authored-works"
click CA "#co-authors"
click CI "#collaborating-institutions"
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- ORCiD
- https://orcid.org/0000-0002-9843-4354
- OpenAlex ID
- https://openalex.org/A5025584661 (API record)
Associated Concepts [?]
- Physics
- Astronomy
- Astrophysics
- Planet
- Computer science
- Computer vision
- Stars
- Exoplanet
- Biology
- Astrobiology
- Quantum mechanics
- Geography
- Optics
- Engineering
- Geology
- Meteorology
- Thermodynamics
- Planetary system
- Hot Jupiter
Authored Works
sorted by decreasing year, and then by display-name
- Saturn's Probable Interior: An Exploration of Saturn's Potential Interior Density Structures and What They Imply About the Planet's Composition
- Meteorite Outgassing Experiments to Inform Chemical Abundances of Super-Earth Atmospheres
- Evidence for a Dichotomy in the Interior Structures of Jupiter and Saturn from Helium Phase Separation
- The Mid-Infrared Search for Life on Nearby Transiting Exoplanets Using The Origins Space Telescope
- Mass Distribution in the Interiors of Saturn and Jupiter Inferred From Measured Gravity Fields With Minimal Assumptions
- Interior Models that Explain the Gravity Fields of Saturn and Jupiter
- Comparative Terrestrial Exoplanetology in an Era of Space-Based Infrared Spectroscopy
- Cassini Ring Seismology as a Probe of Saturn's Rotation
- Uranus and Neptune: internal heat flow
- The Linear Mixing Approximation for Planetary Ices
- The Bright Side of Saturn's Gravity
- Constraining Saturn's interior density profile from precision gravity field measurement obtained during Grand Finale
- Bayesian Thermal Evolution Models for Giant Planets: Helium rain and double-diffusive convection in Jupiter
- Double Diffusive Convection in Jupiter as a result of H/He demixing
- Atmospheric models for post- giant impact planets
- Atmospheric circulation modeling of super Earths and terrestrial extrasolar planets using the SPARC/MITgcm
- Exoplanet albedo spectra and colors as a function of orbital phase, separation, and metallicity
Linked Co-Authors
Linked Collaborating Institutions
- Arizona State University
- Cornell University, Department of Astronomy/Center for Radiophysics and Space Research
- Hampton University, Virginia
- Jet Propulsion Laboratory
- Johns Hopkins University, Applied Physics Laboratory
- Lawrence Livermore National Laboratory, California
- Los Alamos National Laboratory, New Mexico
- Massachusetts Institute of Technology
- NASA Ames Research Center
- NASA Goddard Space Flight Center, Maryland
- SETI Institute, California
- Sapienza University, Rome, Italy
- Space Telescope Science Institute, Baltimore, Maryland
- University of Arizona
- University of Arizona, Department of Planetary Sciences
- University of California, Berkeley
- University of California, Santa Cruz
- University of California, Santa Cruz, Department of Astronomy and Astrophysics
- University of California, Santa Cruz, Department of Earth and Planetary Sciences
- University of California, Santa Cruz, Department of Physics
- University of Idaho
- University of Iowa
- University of Iowa, Department of Physics and Astronomy
- University of Rostock, Germany
- University of Texas, Austin
- University of Texas, Austin, Department of Geological Sciences
- University of Zurich, Switzerland
- Washington University in Saint Louis, Missouri
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