Search Publications

Sedimentological evidence for a deltaic origin of the western fan deposit in Jezero crater, Mars and implications for future exploration
DOI: 10.1016/j.epsl.2016.10.056 Bibcode: 2017E&PSL.458..357G

Mustard, John F.; Goudge, Timothy A.; Head, James W. +2 more

We examine the stratigraphic architecture and mineralogy of the western fan deposit in the Jezero crater paleolake on Mars to reassess whether this fan formed as a delta in a standing body of water, as opposed to by alluvial or debris flow processes. Analysis of topography and images reveals that the stratigraphically lowest layers within the fan …

2017 Earth and Planetary Science Letters
MEx 132
Detection of Mg-spinel bearing central peaks using M3 images: Implications for the petrogenesis of Mg-spinel
DOI: 10.1016/j.epsl.2017.01.019 Bibcode: 2017E&PSL.465...48S

Li, Lin; Sun, Ying; Zhang, Yuanzhi

Mg-spinel bearing lithologies, lacking abundant mafic materials, have been discovered with images acquired by the Moon Mineralogy Mapper (M3) aboard Chandrayaan-1. We conducted a systematic screening of lunar crater central peaks for the presence of Mg-spinel to address its distribution and petrogenesis. 38 Mg-spinel bearing crater cent…

2017 Earth and Planetary Science Letters
Chandrayaan-1 30
Recurrence rate and magma effusion rate for the latest volcanism on Arsia Mons, Mars
DOI: 10.1016/j.epsl.2016.10.040 Bibcode: 2017E&PSL.458..170R

Richardson, Jacob A.; Wilson, James A.; Connor, Charles B. +2 more

Magmatism and volcanism have evolved the Martian lithosphere, surface, and climate throughout the history of Mars. Constraining the rates of magma generation and timing of volcanism on the surface clarifies the ways in which magma and volcanic activity have shaped these Martian systems. The ages of lava flows on other planets are often estimated u…

2017 Earth and Planetary Science Letters
MEx 28
Surface roughness of Titan's hydrocarbon seas
DOI: 10.1016/j.epsl.2017.06.007 Bibcode: 2017E&PSL.474...20G

Lorenz, Ralph D.; Cassini Radar Team; Elachi, Charles +6 more

We derive fields of solutions for the surface properties (roughness and permittivity) of the liquid hydrocarbon bodies Ligeia, Kraken and Punga Mare on Titan by applying the Radar Statistical Reconnaissance (RSR) technique to the Cassini RADAR observations in altimeter mode during the northern early summer. At the time of observation, Kraken and L…

2017 Earth and Planetary Science Letters
Cassini 25
Global permittivity mapping of the Martian surface from SHARAD
DOI: 10.1016/j.epsl.2017.01.012 Bibcode: 2017E&PSL.462...55C

Mège, Daniel; Gurgurewicz, Joanna; Castaldo, Luigi +2 more

SHARAD is a subsurface sounding radar aboard NASA's Mars Reconnaissance Orbiter, capable of detecting dielectric discontinuities in the subsurface caused by compositional and/or structural changes. Echoes coming from the surface contain information on geometric properties at metre scale and on the permittivity of the upper layers of the Martian cr…

2017 Earth and Planetary Science Letters
MEx 20
The Acheron Dorsum on Mars: A novel interpretation of its linear depressions and a model for its evolution
DOI: 10.1016/j.epsl.2017.02.019 Bibcode: 2017E&PSL.465...92D

Martino, Salvatore; De Blasio, Fabio Vittorio

The Acheron Dorsum north of Olympus Mons on Mars is a unique 800 km-long arcuate ridge apparently unrelated to other adjacent morphologies. Acheron Dorsum is crossed by deep and wide fractures ("fossae", here referred to also as Linear Depressions or "LDs"), commonly interpreted as grabens formed by local lithosphere stress in response to endogeno…

2017 Earth and Planetary Science Letters
MEx 4