Uranus from JWST: First Results
- 1University of Leicester, School of Physics and Astronomy, Leicester, LE1, United Kingdom
- 2Association of Universities for Research in Astronomy, Washington, DC, United States
- 3NASA Goddard Space Flight Center, Astrochemistry Laboratory, Greenbelt, MD, United States
- 4Jet Propulsion Laboratory, Pasadena, CA, United States
- 5University of Oxford, Oxford, United Kingdom
- 6Space Science Institute, Seabrook, TX, United States
- 7Univ California Berkeley, Berkeley, CA, United States
- 8LAM, Pythéas OU LESIA, Observatoire de Paris
We present first results from the James Webb Space Telescope (JWST) observations of Uranus, which provide the first spatially resolved, infrared spectra of the planet’s atmosphere spanning from 1.66 to 28.6 µm. We evaluate these unprecedented JWST NIRSpec (1.66–3.05 µm, 2.87–5.14 µm) and MIRI (4.9-28.6 μm) spectra in the context of existing observations and questions concerning Uranus’ stratospheric chemistry and thermal structure [1].
Owing to its frigid atmospheric temperatures, Uranus’ infrared spectrum is extremely weak. Much of the spectrum has never been spatially resolved before, while some had never been clearly observed at all.
From the ground, spatially resolved observations of Uranus’ mid-infrared emission are limited to imaging observations targeting the brighter regions of the infrared spectrum (i.e. ~13 µm emission from stratospheric acetylene, and 17-25 µm from the H2 continuum). Images from the Very Large Telescope VISIR instrument at 13 µm show a stratospheric structure distinct to Uranus, with elevated radiance at high latitudes. The physical nature of this structure–-whether produced by chemical or thermal gradients–-is unclear given previously available data [1]. From space, the Spitzer Space Telescope observed Uranus' mid-infrared spectrum between ~7 and 36 µm, but it lacked the spatial resolution necessary to resolve potential thermal and chemical structure across the disk [2].
Now, with its exceptional sensitivity and outstanding spatial and spectral resolution, JWST reveals Uranus’ stratospheric temperature and chemistry with exquisite new detail, placing new constraints on hydrocarbon abundances and temperature structure across the disk.
With a projected lifetime of over a decade, JWST promises to continue providing exciting new insights into the atmospheric structure, composition, and variability of the ice giants for years to come.
[1] Roman, M.T, et al. "Uranus in northern..." AJ 159.2 (2020): 45.
[2] Rowe-Gurney, N., et al. "Longitudinal variations..." Icarus 365 (2021): 114506.
How to cite: Roman, M., Fletcher, L., Hammel, H., Melin, H., Rowe-Gurney, N., Harkett, J., King, O., Milam, S., Orton, G., Irwin, P., Moses, J., De Pater, I., and Lamy, L.: Uranus from JWST: First Results, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-15491, https://doi.org/10.5194/egusphere-egu23-15491, 2023.
