Image Details

Choose export citation format:

Callisto from JWST: CO2-rich Terrain on the Leading Hemisphere and Global Patterns of H2O Ice

  • Authors: Maria Camarca, Katherine de Kleer, Richard J. Cartwright, Geronimo L. Villanueva, Bryan J. Holler, Zachariah Milby, Kevin P. Hand, Lorenz Roth

Maria Camarca et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 4.

The band depths and centers of Callisto’s CO2 as measured at 4.25 µm for three viewing geometries. The trailing hemisphere and Asgard-centered data were previously published by R. J. Cartwright et al. (2024). The following geologic units are marked with symbols: Valhalla, ⋆; Asgard, ∘; Lofn/Heimdall, △. The subobserver longitude of the observation is indicated in the panels. The projected angular size of Callisto varies slightly between each observation, so the spaxel scale is slightly different in each panel. The typical uncertainty in the band depth is ±0.4%, while the band center is ±0.0006 µm

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse