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The mineral diversity of Jezero crater: Evidence for possible lacustrine carbonates on Mars
DOI: 10.1016/j.icarus.2019.113526 Bibcode: 2020Icar..33913526H

Anderson, Ryan B.; Horgan, Briony H. N.; Dromart, Gilles +2 more

Noachian-aged Jezero crater is the only known location on Mars where clear orbital detections of carbonates are found in close proximity to clear fluvio-lacustrine features indicating the past presence of a paleolake; however, it is unclear whether or not the carbonates in Jezero are related to the lacustrine activity. This distinction is critical…

2020 Icarus
MEx 154
Refining the age, emplacement and alteration scenarios of the olivine-rich unit in the Nili Fossae region, Mars
DOI: 10.1016/j.icarus.2019.113436 Bibcode: 2020Icar..33613436M

Mangold, N.; Quantin-Nataf, C.; Millot, C. +8 more

The Nili Fossae region of Mars exhibits from remote sensing spectral data the largest exposures of olivine-rich materials on the planet. However, it is not clearly constrained how and when these terrains formed. Some of the proposed scenarios favor a mode of formation closely related to Isidis impact basin: either under intense effusive volcanism …

2020 Icarus
MEx 53
Climatology of SO2 and UV absorber at Venus' cloud top from SPICAV-UV nadir dataset
DOI: 10.1016/j.icarus.2019.07.002 Bibcode: 2020Icar..33513368M

Montmessin, Franck; Bertaux, Jean-Loup; Korablev, Oleg +6 more

Following our previous work (Marcq et al., 2013, 2011), we have updated our forward radiative transfer code and processed the whole SPICAV-UV/Venus Express nadir dataset (2006-2014) in order to retrieve SO2 abundance at cloud top - assuming a SO2 decreasing scale height of 3 km and a ratio SO/SO2 tied to 10% - as w…

2020 Icarus
VenusExpress eHST 42
The surface distributions of the production of the major volatile species, H2O, CO2, CO and O2, from the nucleus of comet 67P/Churyumov-Gerasimenko throughout the Rosetta Mission as measured by the ROSINA double focusing mass spectrometer
DOI: 10.1016/j.icarus.2019.113421 Bibcode: 2020Icar..33513421C

Hansen, Kenneth C.; Altwegg, Kathrin; Rubin, Martin +12 more

The Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) suite of instruments operated throughout the over two years of the Rosetta mission operations in the vicinity of comet 67P/Churyumov-Gerasimenko. It measured gas densities and composition throughout the comet's atmosphere, or coma. Here we present two-years' worth of measuremen…

2020 Icarus
Rosetta 38
The composition and structure of Enceladus' plume from the complete set of Cassini UVIS occultation observations
DOI: 10.1016/j.icarus.2019.113461 Bibcode: 2020Icar..34413461H

Hansen, C. J.; Hendrix, A. R.; West, R. A. +4 more

Observations acquired at ultraviolet wavelengths are uniquely well-suited to investigate the composition and structure of Enceladus' plume. This paper describes the observations, analysis techniques and results of all the Enceladus occultations observed by Cassini's Ultraviolet Imaging Spectrograph (UVIS) and other observations designed to study t…

2020 Icarus
Cassini 38
Crust stratigraphy and heterogeneities of the first kilometers at the dichotomy boundary in western Elysium Planitia and implications for InSight lander
DOI: 10.1016/j.icarus.2019.113511 Bibcode: 2020Icar..33813511P

Pan, Lu; Quantin-Nataf, Cathy; Tauzin, Benoit +9 more

InSight landed on Mars on November 26, 2018, in western Elysium Planitia. The Mars crust beneath the lander is subject to complex geologic history next to the great topographic and crustal dichotomy of Mars. Understanding this part of the Martian crust in the subsurface would aid future investigations of the internal structure of the planet based …

2020 Icarus
MEx 36
The landscape of Saturn's internal magnetic field from the Cassini Grand Finale
DOI: 10.1016/j.icarus.2019.113541 Bibcode: 2020Icar..34413541C

Cao, Hao; Dougherty, Michele K.; Hunt, Gregory J. +5 more

The Cassini mission entered the Grand Finale phase in April 2017 and executed 22.5 highly inclined, close-in orbits around Saturn before diving into the planet on September 15th 2017. Here we present our analysis of the Cassini Grand Finale magnetometer (MAG) dataset, focusing on Saturn's internal magnetic field. These measurements demonstrate tha…

2020 Icarus
Cassini 35
The gravity field and interior structure of Dione
DOI: 10.1016/j.icarus.2020.113713 Bibcode: 2020Icar..34513713Z

Tortora, Paolo; Zannoni, Marco; Hemingway, Douglas +1 more

During its mission in the Saturn system, Cassini performed five close flybys of Dione. During three of them, radio tracking data were collected during the closest approach, allowing estimation of the full degree-2 gravity field by precise spacecraft orbit determination.

The gravity field of Dione is dominated by J2 and C22

2020 Icarus
Cassini 28
Multiple mineral horizons in layered outcrops at Mawrth Vallis, Mars, signify changing geochemical environments on early Mars
DOI: 10.1016/j.icarus.2020.113634 Bibcode: 2020Icar..34113634B

Seelos, Frank P.; Murchie, Scott L.; Horgan, Briony +6 more

Refined calibrations of CRISM images are enabling identification of smaller deposits of unique aqueous materials on Mars that reveal changing environmental conditions at the region surrounding Mawrth Vallis. Through characterization of these clay-sulfate assemblages and their association with the layered, phyllosilicate units of this region, more …

2020 Icarus
MEx 26
Labyrinth terrain on Titan
DOI: 10.1016/j.icarus.2020.113764 Bibcode: 2020Icar..34413764M

Malaska, Michael J.; Lopes, Rosaly M. C.; Solomonidou, Anezina +14 more

The Cassini/Huygens mission revealed a terrain type on Saturn's moon Titan of dissected, elevated plateaux with a high density of valleys named labyrinth terrain. We define four subtypes of labyrinth terrains: valleyed, polygonal, finely-dissected, and the possible outlier Kronin Labyrinth. We mapped the locations of all labyrinths imaged by Cassi…

2020 Icarus
Cassini 25