Investigation of diurnal variability of water vapor in Enceladus' plume by the Cassini ultraviolet imaging spectrograph. Issue 2 (21st January 2017)

• Record Type: Journal Article
• Authors: Hansen, C. J.; Esposito, L. W.; Aye, K.‐M.; Colwell, J. E.; Hendrix, A. R.; Portyankina, G.; Shemansky, D.
• Is Part Of: Geophysical research letters. Volume 44:Issue 2(2017)
• Page Start: 672
• Page End: 677
• Publication Date: 2017-01-21
• Subjects: Enceladus -- Enceladus plume -- Cassini UVIS -- stellar occultation; Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1002/2016GL071853
• Languages: English
• ISSNs: 0094-8276

Abstract

Abstract: An occultation of ε Orionis by Enceladus' plume was observed with Enceladus at an orbital longitude near apoapsis in order to investigate whether water vapor flow is modulated diurnally, similar to ice particles. The occultation showed that the bulk water vapor emanating from Enceladus changes little with orbital position. The amount of gas in at least one supersonic jet increased significantly, implying that the increase in the number of particles lofted at apoapsis could be due to more gas coming from the supersonic jets and not the overall gas flux from the tiger stripe fissures that cross Enceladus' south polar region. Key Points: Supersonic gas jets in Enceladus' water vapor plume loft more particles when Enceladus is at apoapsis The bulk quantity of gas from fissures across Enceladus' south pole is relatively unaffected by the position of Enceladus in its orbit