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Variability of Callisto’s Optical Aurora in Eclipse

  • Authors: Zachariah Milby, Katherine de Kleer, Carl Schmidt

Zachariah Milby et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 5.

Change in Callisto’s 630.0 nm [O I] emission with distance from the plasma sheet centrifugal equator. Scatter points with error bars show the brightness and uncertainty calculated from individual 5 minute integrations on 2021 July 04 (gray) and 2025 November 29 (black). Scatter points with downward-pointing arrows (red) are the 2σ upper limits for nondetections. The solid gray line and shaded light gray region shows the best fit of Equation (1) to the 2025 November 29 data.

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