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Depth of the Martian cryosphere: Revised estimates and implications for the existence and detection of subpermafrost groundwater
DOI: 10.1029/2009JE003462 Bibcode: 2010JGRE..115.7001C

Heggy, Essam; Clifford, Stephen M.; Lasue, Jeremie +3 more

The Martian cryosphere is defined as that region of the crust where the temperature remains continuously below the freezing point of water. Previous estimates of its present thickness have ranged from ∼2.3-4.7 km at the equator to ∼6.5-12.5 km at the poles. Here we revisit these calculations, review some of the assumptions on which they were based…

2010 Journal of Geophysical Research (Planets)
MEx 163
Mineralogy and stratigraphy of phyllosilicate-bearing and dark mantling units in the greater Mawrth Vallis/west Arabia Terra area: Constraints on geological origin
DOI: 10.1029/2009JE003351 Bibcode: 2010JGRE..115.0D19N

Bibring, J. -P.; Poulet, F.; Bishop, J. L. +13 more

Analyses of MRO/CRISM images of the greater Mawrth Vallis region of Mars affirm the presence of two primary phyllosilicate assemblages throughout a region ∼1000 × 1000 km. These two units consist of an Fe/Mg-phyllosilicate assemblage overlain by an Al-phyllosilicate and hydrated silica assemblage. The lower unit contains Fe/Mg-smectites, sometimes…

2010 Journal of Geophysical Research (Planets)
MEx 96
Water ice at low to midlatitudes on Mars
DOI: 10.1029/2010JE003584 Bibcode: 2010JGRE..11510001V

Mustard, John; Forget, François; Vincendon, Mathieu

In this paper, we analyze water ice occurrences at the surface of Mars using near-infrared observations, and we study their distribution with a climate model. Latitudes between 45°S and 50°N are considered. Data from the Observatoire pour la Minéralogie, l'Eau, les Glaces et l'Actitité and the Compact Reconnaissance Imaging Spectrometer for Mars a…

2010 Journal of Geophysical Research (Planets)
MEx 76
Nightside ionosphere of Mars: Radar soundings by the Mars Express spacecraft
DOI: 10.1029/2010JE003663 Bibcode: 2010JGRE..11512009N

Gurnett, D. A.; Němec, F.; Morgan, D. D. +1 more

We present results of a survey of the nightside ionosphere of Mars as observed by Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) on board the Mars Express spacecraft. The occurrence rate of the nightside ionosphere is studied as a function of solar zenith angle (SZA), magnetic field magnitude, and magnetic field inclination. …

2010 Journal of Geophysical Research (Planets)
MEx 75
Spectral and stratigraphic mapping of hydrated sulfate and phyllosilicate-bearing deposits in northern Sinus Meridiani, Mars
DOI: 10.1029/2009JE003354 Bibcode: 2010JGRE..115.0D18W

Arvidson, R. E.; Morris, R. V.; Poulet, F. +7 more

We present detailed stratigraphic and spectral analyses that focus on a region in northern Sinus Meridiani located between 1°N to 5°N latitude and 3°W to 1°E longitude. Several stratigraphically distinct units are defined and mapped using morphologic expression, spectral properties, and superposition relationships. Previously unreported exposures …

2010 Journal of Geophysical Research (Planets)
MEx 61
Sinuous gullies on Mars: Frequency, distribution, and implications for flow properties
DOI: 10.1029/2009JE003540 Bibcode: 2010JGRE..11511001M

Mangold, N.; Ansan, V.; Mangeney, A. +4 more

Recent gullies on Mars are suspected to be the result of liquid-water-bearing flows. A formation from wet flows has been challenged by studies invoking granular (dry) flows. Our study focuses on the sinuous shapes observed for some of the recent Martian gullies. Sinuous gullies are found in locations and slopes (of 10°-15°) similar to straight gul…

2010 Journal of Geophysical Research (Planets)
MEx 50
Stratigraphy of hydrated sulfates in the sedimentary deposits of Aram Chaos, Mars
DOI: 10.1029/2009JE003353 Bibcode: 2010JGRE..115.0D17L

Murchie, Scott L.; Mustard, John F.; Arvidson, Raymond E. +8 more

Sedimentary deposits within the 280 km wide crater containing Aram Chaos (∼3°N, 339°E) have been differentially eroded by wind to expose a stratigraphic column 900-1000 m thick that unconformably overlies the chaos bedrock. A detailed stratigraphic and mineralogical description of the deposits is presented based on data from the Mars Reconnaissanc…

2010 Journal of Geophysical Research (Planets)
MEx 50
Late Noachian to Hesperian climate change on Mars: Evidence of episodic warming from transient crater lakes near Ares Vallis
DOI: 10.1029/2009JE003522 Bibcode: 2010JGRE..115.6013W

Muller, Jan-Peter; Gupta, Sanjeev; Kim, Jung-Rack +3 more

The Ares Vallis region is surrounded by highland terrain containing both degraded and pristine large impact craters that suggest a change in climate during the Late Noachian-Early Hesperian, from warmer, wetter conditions to colder, dryer conditions. However, the regional occurrence of Hesperian-age crater outlet channels indicates that this perio…

2010 Journal of Geophysical Research (Planets)
MEx 42
Internal structure of Planum Boreum, from Mars advanced radar for subsurface and ionospheric sounding data
DOI: 10.1029/2009JE003537 Bibcode: 2010JGRE..115.9003S

Plaut, J. J.; Safaeinili, A.; Aharonson, O. +1 more

An investigation of the internal structure of the ice-rich Planum Boreum (PB) deposit at the north pole of Mars is presented, using 178 orbits of Mars advanced radar for subsurface and ionospheric sounding data. For each radargram, bright, laterally extensive surface and subsurface reflectors are identified and the time delay between them is conve…

2010 Journal of Geophysical Research (Planets)
MEx 33
Rift zone volcanism and associated cinder cone field in Utopia Planitia, Mars
DOI: 10.1029/2010JE003578 Bibcode: 2010JGRE..11512019L

Neukum, G.; Wagner, R.; Lanz, J. K. +2 more

We analyzed a small cone field in SW Utopia Planitia that shows striking similarities to volcanic rift zones on Earth. This is of particular interest as the study area lies off any of the volcanic centers of Mars in the northern hemisphere lowlands and is surrounded by material of the Amazonian aged Vastitas Borealis Formation (VBF). We believe th…

2010 Journal of Geophysical Research (Planets)
MEx 26