2006/03/09 by C. J. Hansen, L. W. Esposito, A. I. F. Stewart +5 · 10 citations
Physics and Astronomy · #Astro and Planetary Science #Planetary Science and Exploration #Astrophysics and Star Formation Studies #Enceladus #Plume #Saturn #Astrobiology #Water vapor #Spectrograph #Polar #Icy moon #Spacecraft #Astronomy #Physics #Environmental science #Planet #Meteorology #Spectral line
paper · doi:10.1126/science.1121254
openalex publication_date 2006/03/09 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/02
The Cassini spacecraft flew close to Saturn's small moon Enceladus three times in 2005. Cassini's UltraViolet Imaging Spectrograph observed stellar occultations on two flybys and confirmed the existence, composition, and regionally confined nature of a water vapor plume in the south polar region of Enceladus. This plume provides an adequate amount of water to resupply losses from Saturn's E ring and to be the dominant source of the neutral OH and atomic oxygen that fill the Saturnian system.