Search Publications

Saturn's atmospheric response to the large influx of ring material inferred from Cassini INMS measurements
DOI: 10.1016/j.icarus.2022.115328 Bibcode: 2023Icar..39115328M

Fletcher, Leigh N.; Guerlet, Sandrine; Moses, Julianne I. +12 more

During the Grand Finale stage of the Cassini mission, organic-rich ring material was discovered to be flowing into Saturn's equatorial upper atmosphere at a surprisingly large rate. Through a series of photochemical models, we have examined the consequences of this ring material on the chemistry of Saturn's neutral and ionized atmosphere. We find …

2023 Icarus
Cassini 9
Microwaving Mimas, Enceladus, Tethys, Dione, Rhea, Iapetus and Phoebe: Insights into the regolith properties and geological history of Saturn's icy satellites
DOI: 10.1016/j.icarus.2023.115446 Bibcode: 2023Icar..39415446L

Lellouch, Emmanuel; Wall, Stephen; Le Gall, Alice A. +4 more

While Saturn's main airless moons are all composed largely of water ice, their respective thermal histories and near environments have led to different regolith compositions and structures. Part of this history is recorded in their subsurface which can be probed by microwaves. Using a combined thermal and radiative transfer model, we here investig…

2023 Icarus
Cassini 4
The Bolometric Bond Albedo of Enceladus
DOI: 10.1016/j.icarus.2023.115429 Bibcode: 2023Icar..39415429L

West, Robert A.; Nixon, Conor A.; Fry, Patrick M. +13 more

The bolometric Bond albedo is a fundamental parameter of planets and moons. Here, combined observations from the Cassini spacecraft and the Hubble Space Telescope are used to determine the bolometric Bond albedo of Enceladus. We provide the full-disk reflectance of Enceladus across all phase angles (0° -180°) from 150 nm to 5131 nm, a spectral ran…

2023 Icarus
Cassini eHST 2
The complex shape of the outer edge of Saturn's B ring, as observed in Cassini occultation data
DOI: 10.1016/j.icarus.2023.115678 Bibcode: 2023Icar..40515678F

Nicholson, Philip D.; French, Richard G.; Hedman, Matthew M. +9 more

We determine the time-variable shape of the outer edge of Saturn's B ring using the complete set of Cassini radio and stellar occultation data obtained between mid-2005 and the End-of-Mission in late 2017, considerably expanding the range and number of individual ring edge measurements used in previous analyses (Spitale and Porco, 2010; Nicholson …

2023 Icarus
Cassini 1