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Peculiar rainbows in Saturn's E ring: Uncovering luminous bands near Enceladus

2025/02/25 by Niels Rubbrecht, Rubbrecht, Niels, Stéphanie Cazaux +11 · 1 voice
Physics and Astronomy · #Earth and Planetary Astrophysics (astro-ph.EP) #FOS: Physical sciences #astro-ph.EP

paper · pdf · doi:10.48550/arxiv.2502.18028

arxiv published 2025/02/25 · arxiv updated 2025/06/06

Abstract

We report observations of stripe-like features in Enceladus' plumes captured simultaneously by Cassini's VIMS-IR and ISS NAC instruments during flyby E17, with similar patterns seen in VIMS-IR data from flyby E13 and E19. These parallel stripes, inclined at approximately 16 to the ecliptic and 43 to Saturn's ring plane, appear continuous across images when projected in the J2000 frame. A bright stripe, most visible at wavelengths around 5 μm, acts as the zeroth-order diffraction peak of a reflection grating with an estimated groove spacing of 0.12-2.60 mm, while adjacent stripes are attributed to higher-order diffraction peaks. We suggest that this light-dispersing phenomenon originates from an inclined periodic structure within Saturn's E ring. This structure, constrained between Saturn's G ring and Rhea's orbit, likely consists of fresh ice particles supplied by Enceladus' plumes.

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