Search Publications

Local topography effects on the surface temperatures on Mars - Application to the case of Recurring Slope Lineae (RSL)
DOI: 10.1016/j.icarus.2020.114136 Bibcode: 2021Icar..35514136M

Quantin-Nataf, Cathy; Leyrat, Cédric; Millot, Cédric +1 more

Recurring Slope Lineae (RSL) are dark linear recurrent features which incrementally lengthen and fade each year on Martian slopes. Their activity during warmest seasons rises the question of modern martian water related process. To investigate this question, this study focuses on the thermal context of slopes hosting RSL. The paper presents a nume…

2021 Icarus
MEx 11
The Eris/Dysnomia system I: The orbit of Dysnomia
DOI: 10.1016/j.icarus.2020.114130 Bibcode: 2021Icar..35514130H

Buie, M. W.; Grundy, W. M.; Holler, B. J. +1 more

We present new results on the Eris/Dysnomia system including analysis of new images from the WFC3 instrument on the Hubble Space Telescope (HST). Seven HST orbits were awarded to program 15171 in January and February 2018, with the intervals between observations selected to sample Dysnomia over a full orbital period. Using relative astrometry of E…

2021 Icarus
eHST 10
Spectrophotometric properties of materials observed by Pancam on the Mars Exploration Rovers: 4. Final mission observations
DOI: 10.1016/j.icarus.2020.114261 Bibcode: 2021Icar..35714261J

Johnson, Jeffrey R.; Grundy, William M.; Lemmon, Mark T. +4 more

The last sets of Panoramic Camera (Pancam) visible/near-infrared (432-1009 nm) multispectral observations made under varying viewing and illumination geometries by the Mars Exploration Rovers Spirit and Opportunity were examined using radiative transfer models to study the surface scattering and microphysical nature of rock and soil units at both …

2021 Icarus
MEx 10
Ice-rich landforms of the southern mid-latitudes of Mars: A case study in Nereidum Montes
DOI: 10.1016/j.icarus.2020.114170 Bibcode: 2021Icar..35514170B

Crown, David A.; Berman, Daniel C.; Smith, Isaac B. +1 more

Mapping of Viscous Flow Features (VFFs), a general grouping of ice-rich flow features that includes Lobate Debris Aprons (LDA), Concentric Crater Fill (CCF), Lineated Valley Flow (LVF), small lobate flows (i.e., glacier-like flows, or GLFs), and arcuate ridges, in the southern hemisphere of Mars shows a dense concentration in Nereidum Montes, alon…

2021 Icarus
MEx 9
Evidence of mud volcanism due to the rapid compaction of Martian tsunami deposits in southeastern Acidalia Planitia, Mars
DOI: 10.1016/j.icarus.2020.114096 Bibcode: 2021Icar..35414096D

Costard, François; Séjourné, Antoine; Di Pietro, Ilaria +2 more

Thumbprint terrain was first recognized in Viking Orbiter data and described as sets of alternating continuous parallel ridges and depressions up to several tens of kilometres in length, with high and low albedo respectively. We performed a geomorphological analysis of these features using both Context Camera and High Resolution Imaging Science Ex…

2021 Icarus
MEx 9
Spectral properties of lunar impact melt deposits from Moon Mineralogy Mapper (M3) data
DOI: 10.1016/j.icarus.2021.114392 Bibcode: 2021Icar..36114392N

Tornabene, L. L.; Neish, C. D.; Cannon, K. M. +3 more

Lunar impact melt deposits have unusual surface properties, unlike any measured terrestrial lava flow. Radar observations suggest that they are incredibly rough at decimeter scales, but they appear smooth in high-resolution, meter-scale optical images. The cause of their unusual surface roughness is unknown. In this work, we investigate the proper…

2021 Icarus
Chandrayaan-1 9
Landforms indicative of regional warm based glaciation, Phlegra Montes, Mars
DOI: 10.1016/j.icarus.2020.114173 Bibcode: 2021Icar..35514173G

Butcher, Frances E. G.; Gallagher, Colman; Balme, Matt +2 more

Viscous flow features (VFF) occur in the mid-latitudes of Mars and have characteristics consistent with being glaciers. Climate models suggest that martian glaciers are cold-based systems in which meltwater has never been widely produced. VFF are common in Phlegra Montes, a mountain range in the mid-latitudes of the northern hemisphere of Mars. Ho…

2021 Icarus
MEx 9
Daily dust variation from the PFS MEx observations
DOI: 10.1016/j.icarus.2020.113823 Bibcode: 2021Icar..35313823W

Giuranna, Marco; Wolkenberg, Paulina

We collected over 7 Martian years (MY) of data observed by the Planetary Fourier Spectrometer (PFS) to present a daily variation of dust content in the Martian atmosphere. We found three typical behaviors of dust opacities with LT (local time). The most peculiar variation was observed when global dust storms (MYs 28 and 34) or particularly strong …

2021 Icarus
MEx 9
Monitoring the negative polarization in Comet 29P/Schwassmann-Wachmann during quiescence
DOI: 10.1016/j.icarus.2021.114536 Bibcode: 2021Icar..36614536K

Kim, Sungsoo S.; Videen, Gorden; Zubko, Evgenij +4 more

During five nights between February 3 and 10, 2021, we monitored the degree of linear polarization in Comet 29P/Schwassmann-Wachmann with the broadband R filter. It is the first polarimetric investigation of this comet measured during a period of quiescent activity. We found a nearly constant negative polarization PQ ≈ -2.1% at α ≈ 9.5°…

2021 Icarus
Rosetta 8
Impact of gradients at the martian terminator on the retrieval of ozone from SPICAM/MEx
DOI: 10.1016/j.icarus.2019.113598 Bibcode: 2021Icar..35313598P

Aoki, S.; Vandaele, A. C.; Daerden, F. +11 more

Rapid variations of pressure, temperature and illumination at the day-night terminator have the potential to cause asymmetries in the abundance distribution of the atmosphere constituents along the line of sight (LOS) of a solar occultation experiment. Ozone, in particular, displays steep density gradients across the terminator of Mars due to phot…

2021 Icarus
MEx 8