Search Publications

Global investigation of olivine on Mars: Insights into crust and mantle compositions
DOI: 10.1029/2012JE004149 Bibcode: 2013JGRE..118..234O

Bibring, J. -P.; Gondet, B.; Langevin, Y. +4 more

present the distribution of olivine on Mars, derived from spectral parameters based on the 1 µm olivine absorption band. The olivine can be defined with respect to two spectral end-members: type 1 corresponds to olivine with low iron content and/or small grain size and/or small abundance, and type 2, which corresponds to olivine with higher iron c…

2013 Journal of Geophysical Research (Planets)
MEx 115
Three-dimensional Martian ionosphere model: I. The photochemical ionosphere below 180 km
DOI: 10.1002/jgre.20150 Bibcode: 2013JGRE..118.2105G

Forget, F.; Chaufray, J. -Y.; Leblanc, F. +6 more

We describe the Mars ionosphere with unprecedented detail in 3-D, as simulated by a Mars general circulation model (the Laboratoire de Météorologie Dynamique Mars GCM), and compare it with recent measurements. The model includes a number of recent extensions and improvements. Different simulations for a full Martian year have been performed. The e…

2013 Journal of Geophysical Research (Planets)
MEx 104
Rocket dust storms and detached dust layers in the Martian atmosphere
DOI: 10.1002/jgre.20046 Bibcode: 2013JGRE..118..746S

Määttänen, Anni; Forget, François; Spiga, Aymeric +2 more

Airborne dust is the main climatic agent in the Martian environment. Local dust storms play a key role in the dust cycle; yet their life cycle is poorly known. Here we use mesoscale modeling that includes the transport of radiatively active dust to predict the evolution of a local dust storm monitored by OMEGA on board Mars Express. We show that t…

2013 Journal of Geophysical Research (Planets)
MEx 95
Hydrovolcanic tuff rings and cones as indicators for phreatomagmatic explosive eruptions on Mars
DOI: 10.1002/jgre.20120 Bibcode: 2013JGRE..118.1656B

Hauber, E.; Brož, P.

is a common natural phenomenon on Earth and should be common on Mars, too, since its surface shows widespread evidence for volcanism and near-surface water. We investigate fields of pitted cones in the Nephentes/Amenthes region at the southern margin of the ancient impact basin, Utopia, which were previously interpreted as mud volcanoes. The cone …

2013 Journal of Geophysical Research (Planets)
MEx 77
Long-term variation in the cloud-tracked zonal velocities at the cloud top of Venus deduced from Venus Express VMC images
DOI: 10.1029/2011JE004013 Bibcode: 2013JGRE..118...37K

Futaana, Yoshifumi; Imamura, Takeshi; Kouyama, Toru +2 more

We present observational evidence of the variation of the cloud-tracked zonal velocity by ~20 m s-1 with a timescale of a few hundred days in the southern low latitude region based on an analysis of cloud images taken by the Venus Monitoring Camera on board Venus Express. A spectral analysis suggests that the variation has a periodicity…

2013 Journal of Geophysical Research (Planets)
VenusExpress 70
MAHLI at the Rocknest sand shadow: Science and science-enabling activities
DOI: 10.1002/2013JE004426 Bibcode: 2013JGRE..118.2338M

Kennedy, M. R.; Deen, R. G.; Schmidt, M. +29 more

Martian solar days 57-100, the Mars Science Laboratory Curiosity rover acquired and processed a solid (sediment) sample and analyzed its mineralogy and geochemistry with the Chemistry and Mineralogy and Sample Analysis at Mars instruments. An aeolian deposit—herein referred to as the Rocknest sand shadow—was inferred to represent a global average …

2013 Journal of Geophysical Research (Planets)
MEx 66
Asynchronous formation of Hesperian and Amazonian-aged deltas on Mars and implications for climate
DOI: 10.1002/jgre.20107 Bibcode: 2013JGRE..118.1529H

Hauber, E.; Platz, T.; Le Deit, L. +5 more

fluvial and lacustrine landforms on Mars are thought to be old and have formed more than ~3.8 Gyr ago, in the Noachian period. After a major climatic transition, surface liquid water became less abundant and finally disappeared almost completely. Recent work has shown that observational evidence for Hesperian and Amazonian aqueous processes is mor…

2013 Journal of Geophysical Research (Planets)
MEx 61
Mineralogy and morphology of geologic units at Libya Montes, Mars: Ancient aqueously derived outcrops, mafic flows, fluvial features, and impacts
DOI: 10.1029/2012JE004151 Bibcode: 2013JGRE..118..487B

Seelos, Frank P.; Murchie, Scott L.; Mustard, John F. +19 more

There is ample evidence of both ancient and long-lasting fluvial activity and chemical alteration in the Libya Montes region south of Isidis Basin. The region hosts Noachian to Amazonian aged surface rocks with extensive outcrops of olivine- and pyroxene-bearing material. Libya Montes also features surface outcrops and/or deposits hosting Fe/Mg-sm…

2013 Journal of Geophysical Research (Planets)
MEx 59
Gullies and landslides on the Moon: Evidence for dry-granular flows
DOI: 10.1002/jgre.20043 Bibcode: 2013JGRE..118..206S

Mustard, John; Ostrach, Lillian R.; Kiran Kumar, A. S. +7 more

High-resolution images from Chandrayaan-1 Terrain Mapping Camera and Lunar Reconnaissance Orbiter Camera reveal landslides and gully formation on the interior wall of a 7 km-diameter simple crater emplaced in Schrödinger basin on the farside of the Moon. These features occur on the steep upper crater wall, where the slope is ~35°. The gullies show…

2013 Journal of Geophysical Research (Planets)
Chandrayaan-1 58
The spiral troughs of Mars as cyclic steps
DOI: 10.1002/jgre.20142 Bibcode: 2013JGRE..118.1835S

Howard, Alan D.; Spiga, Aymeric; Holt, John W. +2 more

combine observations of stratigraphy, morphology, and atmospheric processes to relate the spiral troughs on Mars' polar layered deposits to a class of features known as cyclic steps. Cyclic steps are quasi-stable, repeating, and upstream-migrating bed forms that have been studied in terrestrial and submarine environments. The repeating pattern is …

2013 Journal of Geophysical Research (Planets)
MEx 56