Space Telescope Imaging Spectrograph Observations of Europa’s Optical Aurora

Abstract We analyzed Hubble Space Telescope observations of Europa’s optical aurora, yielding further insight into the composition of its tenuous atmosphere and its plasma-interaction variability. We obtained these observations of auroral emissions while Europa was in solar eclipse behind Jupiter to avoid reflected sunlight as a background signal and source of noise. We analyzed oxygen 630.0 and 636.4 nm emission line brightness profiles across the disk to constrain O 2 abundances. Analyses of time-varying brightness ratios across different regions of Europa were compared with previous auroral studies in the ultraviolet and in the visible. We confirm a correlation with auroral brightness and relative distance from Jupiter’s plasma sheet crossing. We find that the decorrelated set of auroral brightnesses diminishes with longer eclipse duration, suggesting a possible partial collapse of Europa’s atmosphere when in eclipse.

Authors

Publication Details

Journal
Research Notes of the AAS
Published
2025-07-18
DOI
https://doi.org/10.3847/2515-5172/adf06e
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
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article

Space Telescope Imaging Spectrograph Observations of Europa’s Optical Aurora

Tracy M. Becker, K. D. Retherford, Michael Velez, Joshua A. Kammer et al.
Research Notes of the AAS
Astro and Planetary Science
article

Space Telescope Imaging Spectrograph Observations of Europa’s Optical Aurora

Tracy M. Becker, K. D. Retherford, Michael Velez, Joshua A. Kammer, Vincent Hue, Lorenz Roth
article en

Abstract

Abstract We analyzed Hubble Space Telescope observations of Europa’s optical aurora, yielding further insight into the composition of its tenuous atmosphere and its plasma-interaction variability. We obtained these observations of auroral emissions while Europa was in solar eclipse behind Jupiter to avoid reflected sunlight as a background signal and source of noise. We analyzed oxygen 630.0 and 636.4 nm emission line brightness profiles across the disk to constrain O 2 abundances. Analyses of time-varying brightness ratios across different regions of Europa were compared with previous auroral studies in the ultraviolet and in the visible. We confirm a correlation with auroral brightness and relative distance from Jupiter’s plasma sheet crossing. We find that the decorrelated set of auroral brightnesses diminishes with longer eclipse duration, suggesting a possible partial collapse of Europa’s atmosphere when in eclipse.

Research Notes of the AASVol. 9(7)
Openalex Percentile: Top 86%
Astro and Planetary Science
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