Jonathan J Fortney
· Chair and ProfessorUniversity of California, Santa Cruz · Physics and Astronomy
Active 2000–2026
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About
Jonathan J Fortney is a Professor and Chair in the Department of Astronomy & Astrophysics within the Division of Physical & Biological Sciences. His expertise encompasses astrophysics and astronomy, with a focus on planetary atmospheres, planetary interiors, and exoplanets. Fortney's research aims to understand different kinds of planets as classes of astrophysical objects by characterizing their composition and evolution over time. He primarily functions as a modeler and theorist, working closely with observers to study the atmosphere, interior, and thermal evolution of planets both within the solar system and around other stars, at various distances from their parent stars. His work involves studying planets at different ages, from young to old, and across different environments, to better understand their physical properties and developmental processes.
Research topics
- Physics
- Astronomy
- Astrobiology
- Astrophysics
- Meteorology
- Chemistry
- Biology
- Environmental science
- Geology
- Computer Science
Selected publications
Photochemically produced SO2 in the atmosphere of WASP-39b
Nature · 2023 · 236 citations
also shows observable features at ultraviolet and thermal infrared wavelengths not available from the existing observations.
Early Release Science of the exoplanet WASP-39b with JWST NIRISS
Nature · 2023 · 210 citations
. Here we present the transmission spectrum of WASP-39b obtained using the Single-Object Slitless Spectroscopy (SOSS) mode of the Near Infrared Imager and Slitless Spectrograph (NIRISS) instrument on the JWST. This spectrum spans 0.6-2.8 μm in wavelength and shows several water-absorption bands, the potassium resonance doublet and signatures of clouds. The precision and broad wavelength coverage of NIRISS/SOSS allows us to break model degeneracies between cloud properties and the atmospheric com…
Identification of carbon dioxide in an exoplanet atmosphere
Nature · 2022 · 184 citations
, but little methane. Furthermore, we also tentatively detect a small absorption feature near 4.0 micrometres that is not reproduced by these models.
Early Release Science of the exoplanet WASP-39b with JWST NIRCam
Nature · 2023 · 180 citations
).
The Astrophysical Journal Letters · 2023 · 160 citations
Abstract We present the highest fidelity spectrum to date of a planetary-mass object. VHS 1256 b is a <20 M Jup widely separated (∼8″, a = 150 au), young, planetary-mass companion that shares photometric colors and spectroscopic features with the directly imaged exoplanets HR 8799c, d, and e. As an L-to-T transition object, VHS 1256 b exists along the region of the color–magnitude diagram where substellar atmospheres transition from cloudy to clear. We observed VHS 1256 b with JWST's NIRSpec…
Recent grants
Towards a Comprehensive Understanding of Brown Dwarf Atmospheres
NSF · $245k · 2015–2018
Evolutionary Models of Young Jupiters and Hot Jupiters
NSF · $165k · 2008–2010
Collaborative Research: Characterizing Cloudy Exoplanet Atmospheres
NSF · $335k · 2013–2016
Frequent coauthors
- 304 shared
Mark S. Marley
University of Arizona
- 211 shared
Caroline Morley
- 211 shared
Jean-Michel Désert
- 178 shared
Kevin B. Stevenson
Johns Hopkins University Applied Physics Laboratory
- 157 shared
Heather A. Knutson
California Institute of Technology
- 157 shared
Nikole K. Lewis
- 151 shared
Michael R. Line
- 144 shared
Adam P. Showman
Labs
Education
- 2003
Ph.D., Astronomy
California Institute of Technology
- 1999
M.S., Astronomy
California Institute of Technology
- 1997
B.S., Physics
Harvard University
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