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Abstract: The Temperature, Composition, and Haze Structure of Uranus' Atmosphere Determined from JWST (AGU25)

The Temperature, Composition, and Haze Structure of Uranus' Atmosphere Determined from JWST

Michael Thomas Roman1,2, Leigh N. Fletcher2, Heidi B Hammel3, Oliver King2, Patrick GJ Irwin4, Julianne I Moses5, Naomi Rowe-Gurney6, Glenn Orton7, Imke De Pater8, Henrik Melin9, Jake Harkett2 and Stefanie N Milam10, (1)Universidad Adolfo Ibåñez, Facultad de Ingeniería y Ciencias, Santiago, Chile, (2)University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, (3)Association of Universities for Research in Astronomy, Washington D.C., United States, (4)University of Oxford, Oxford, United Kingdom, (5)Space Science Institute, Boulder, United States, (6)Royal Astronomical Society, London, United Kingdom, (7)Jet Propulsion Laboratory/California Institute of Technology, Pasadena, United States, (8)Univ California Berkeley, Berkeley, United States, (9)Northumbria University, Mathematics, Physics and Electrical Engineering, Newcastle-Upon-Tyne, United Kingdom, (10)NASA Goddard Space Flight Center, Astrochemistry Laboratory, Greenbelt, United States
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