Detection of the infrared aurora at Uranus with Keck-NIRSPEC

Emma M. Thomas*, Henrik Melin, Tom S. Stallard, Mohammad N. Chowdhury, Ruoyan Wang, Katie Knowles, Steve Miller

*Corresponding author for this work

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Abstract

Near-infrared (NIR)-wavelength observations of Uranus have been unable to locate any infrared aurorae, despite many attempts to do so since the 1990s. While at Jupiter and Saturn, NIR investigations have redefined our understanding of magnetosphere–ionosphere–thermosphere coupling, the lack of NIR auroral detection at Uranus means that we have lacked a window through which to study these processes at Uranus. Here we present NIR Uranian observations with the Keck II telescope taken on the 5 September 2006 and detect enhanced H3+ emissions. Analysing temperatures and column densities, we identify an 88% increase in localized H3+ column density, with no significant temperature increases, consistent with auroral activity generating increased ionization. By comparing these structures against the Q3mp magnetic-field model and the Voyager 2 ultraviolet observations, we suggest that these regions make up sections of the northern aurora.
Original languageEnglish
Pages (from-to)1473-1480
Number of pages10
JournalNature Astronomy
Volume7
Issue number12
Early online date23 Oct 2023
DOIs
Publication statusPublished - 1 Dec 2023

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