Search Publications

Global Mineralogical and Aqueous Mars History Derived from OMEGA/Mars Express Data
DOI: 10.1126/science.1122659 Bibcode: 2006Sci...312..400B

Drossart, Pierre; Korablev, Oleg; Forget, F. +43 more

Global mineralogical mapping of Mars by the Observatoire pour la Mineralogie, l'Eau, les Glaces et l'Activité (OMEGA) instrument on the European Space Agency's Mars Express spacecraft provides new information on Mars' geological and climatic history. Phyllosilicates formed by aqueous alteration very early in the planet's history (the ``phyllocian'…

2006 Science
MEx 1327
Formation of Glaciers on Mars by Atmospheric Precipitation at High Obliquity
DOI: 10.1126/science.1120335 Bibcode: 2006Sci...311..368F

Forget, F.; Montmessin, F.; Head, J. W. +2 more

Surface conditions on Mars are currently cold and dry, with water ice unstable on the surface except near the poles. However, geologically recent glacierlike landforms have been identified in the tropics and the midlatitudes of Mars. The ice has been proposed to originate from either a subsurface reservoir or the atmosphere. We present high-resolu…

2006 Science
MEx 361
The Analyzer of Space Plasmas and Energetic Atoms (ASPERA-3) for the Mars Express Mission
DOI: 10.1007/s11214-006-9124-8 Bibcode: 2006SSRv..126..113B

Coates, A. J.; Kallio, E.; Fedorov, A. +39 more

The general scientific objective of the ASPERA-3 experiment is to study the solar wind - atmosphere interaction and to characterize the plasma and neutral gas environment with within the space near Mars through the use of energetic neutral atom (ENA) imaging and measuring local ion and electron plasma. The ASPERA-3 instrument comprises four sensor…

2006 Space Science Reviews
MEx 253
Orientation and distribution of recent gullies in the southern hemisphere of Mars: Observations from High Resolution Stereo Camera/Mars Express (HRSC/MEX) and Mars Orbiter Camera/Mars Global Surveyor (MOC/MGS) data
DOI: 10.1029/2005JE002607 Bibcode: 2006JGRE..111.5001B

Mangold, Nicolas; Neukum, Gerhard; Balme, Matthew +5 more

Geologically recent small gullies on Mars display morphologies consistent with erosion by water or by debris flows. Suggested formation models are divided into two main categories: (1) groundwater or (2) melting of near-surface ice/snow sourced from the atmosphere. We have measured location and orientation and recorded the local contexts of gullie…

2006 Journal of Geophysical Research (Planets)
MEx 129
Nature and origin of the hematite-bearing plains of Terra Meridiani based on analyses of orbital and Mars Exploration rover data sets
DOI: 10.1029/2006JE002728 Bibcode: 2006JGRE..11112S08A

Bibring, J. -P.; Arvidson, R. E.; Gondet, B. +23 more

The ~5 km of traverses and observations completed by the Opportunity rover from Endurance crater to the Fruitbasket outcrop show that the Meridiani plains consist of sulfate-rich sedimentary rocks that are largely covered by poorly-sorted basaltic aeolian sands and a lag of granule-sized hematitic concretions. Orbital reflectance spectra obtained …

2006 Journal of Geophysical Research (Planets)
MEx 128
SPICAM on Mars Express: Observing modes and overview of UV spectrometer data and scientific results
DOI: 10.1029/2006JE002690 Bibcode: 2006JGRE..11110S90B

Montmessin, Franck; Bertaux, Jean-Loup; Perrier, Séverine +13 more

This paper is intended as an introduction to several companion papers describing the results obtained by the SPICAM instrument on board Mars Express orbiter. SPICAM is a lightweight (4.7 kg) UV-IR dual spectrometer dedicated primarily to the study of the atmosphere of Mars. The SPICAM IR spectrometer and its results are described in another compan…

2006 Journal of Geophysical Research (Planets)
MEx 116
Subvisible CO 2 ice clouds detected in the mesosphere of Mars
DOI: 10.1016/j.icarus.2006.03.015 Bibcode: 2006Icar..183..403M

Montmessin, Franck; Bertaux, Jean-Loup; Perrier, Séverine +8 more

The formation of CO 2 ice clouds in the upper atmosphere of Mars has been suggested in the past on the basis of a few temperature profiles exhibiting portions colder than CO 2 frost point. However, the corresponding clouds were never observed. In this paper, we discuss the detection of the highest clouds ever observed on Mars…

2006 Icarus
MEx 111
Plasma Morphology at Mars. Aspera-3 Observations
DOI: 10.1007/s11214-006-9039-4 Bibcode: 2006SSRv..126..209D

Barabash, S.; Lundin, R.; Winningham, J. D. +6 more

A total of about of 400 orbits during the first year of the ASPERA-3 operation onboard the Mars Express spacecraft were analyzed to obtain a statistical pattern of the main plasma domains in the Martian space environment. The environment is controlled by the direct interaction between the solar wind and the planetary exosphere/ionosphere which res…

2006 Space Science Reviews
MEx 109
Gusev crater: Wind-related features and processes observed by the Mars Exploration Rover Spirit
DOI: 10.1029/2005JE002491 Bibcode: 2006JGRE..111.2S09G

Arvidson, R. E.; Christensen, P. R.; Greeley, Ronald +19 more

Wind-related features observed by the rover Spirit in Gusev crater, Mars, include patches of soil on the surface, some of which are organized into bed forms. Windblown grains include dust (inferred to be <3 µm in diameter), sands (up to a few hundred µm in diameter), and granules (>2 mm in diameter). Microscopic Imager data show …

2006 Journal of Geophysical Research (Planets)
MEx 107
Plasma Acceleration Above Martian Magnetic Anomalies
DOI: 10.1126/science.1122071 Bibcode: 2006Sci...311..980L

Coates, A. J.; Kallio, E.; Fedorov, A. +20 more

Auroras are caused by accelerated charged particles precipitating along magnetic field lines into a planetary atmosphere, the auroral brightness being roughly proportional to the precipitating particle energy flux. The Analyzer of Space Plasma and Energetic Atoms experiment on the Mars Express spacecraft has made a detailed study of acceleration p…

2006 Science
MEx 104