Mars surface diversity as revealed by the OMEGA/Mars express observations

Jean Pierre Bibring; Yves Langevin; Aline Gendrin; Brigitte Gondet; François Poulet; Michel Berthé; Alain Soufflot; Ray Arvidson; Nicolas Mangold; John Mustard; P. Drossart; Stéphane Erard; Olivier Fomi; Michel Combes; Thérèse Encrenaz; Thierry Fouchet; Riccardo Merchiorri; Gian Carlo Belluci; Francesca Altieri; Vittorio Formisano; Guillaume Bonello; Fabricio Capaccioni; Pricilla Cerroni; Angioletta Coradini; Sergio Fonti; Volodia Kottsov; Nikolai Ignatiev; Vassili Moroz; Dimitri Titov; Ludmilla Zasova; Patrick Pinet; Sylvain Douté; Bernard Schmitt; Christophe Sotin; Ernst Hauber; Harald Hoffmann; Ralf Jaumann; Uwe Keller; Tom Duxbury; François Forget

doi:10.1126/science.1108806

Mars surface diversity as revealed by the OMEGA/Mars express observations

Jean Pierre Bibring
, Yves Langevin
, Aline Gendrin
, Brigitte Gondet
, François Poulet
, Michel Berthé
, Alain Soufflot
, Ray Arvidson
, Nicolas Mangold
, John Mustard
, P. Drossart
, Stéphane Erard
, Olivier Fomi
, Michel Combes
, Thérèse Encrenaz
, Thierry Fouchet
, Riccardo Merchiorri
, Gian Carlo Belluci
, Francesca Altieri
, Vittorio Formisano

Guillaume Bonello, Fabricio Capaccioni, Pricilla Cerroni, Angioletta Coradini, Sergio Fonti, Volodia Kottsov, Nikolai Ignatiev, Vassili Moroz, Dimitri Titov, Ludmilla Zasova, Patrick Pinet, Sylvain Douté, Bernard Schmitt, Christophe Sotin, Ernst Hauber, Harald Hoffmann, Ralf Jaumann, Uwe Keller, Tom Duxbury, François Forget

Institut d'Astrophysique Spatiale
Washington University in St. Louis
Bâtiment 509
Women and Infants Hospital of Rhode Island-Warren Alpert Medical School of Brown University
Sorbonne Univ.
INAF-IFSI
INAF-IASF
University of Salento
Space Research Institute (IKI)
Observatoire Midi-Pyrénées
Laboratoire de Planétologie
Université de Nantes
Deutschen Zentrum F. Luft-and R.
Max Planck Inst. F. S.
Science Division

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) investigation, on board the European Space Agency Mars Express mission, is mapping the surface composition of Mars at a 0.3- to 5-kilometer resolution by means of visible - near-infrared hyperspectral reflectance imagery. The data acquired during the first 9 months of the mission already reveal a diverse and complex surface mineralogy, offering key insights into the evolution of Mars. OMEGA has identified and mapped mafic iron-bearing silicates of both the northern and southern crust, localized concentrations of hydrated phyllosilicates and sulfates but no carbonates, and ices and frosts with a water-ice composition of the north polar perennial cap, as for the south cap, covered by a thin carbon dioxide-ice veneer.

langue originale	Anglais
Pages (de - à)	1576-1581
Nombre de pages	6
journal	Science
Volume	307
Numéro de publication	5715
Les DOIs	https://doi.org/10.1126/science.1108806
état	Publié - 11 mars 2005

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10.1126/science.1108806

Contient cette citation

Bibring, J. P., Langevin, Y., Gendrin, A., Gondet, B., Poulet, F., Berthé, M., Soufflot, A., Arvidson, R., Mangold, N., Mustard, J., Drossart, P., Erard, S., Fomi, O., Combes, M., Encrenaz, T., Fouchet, T., Merchiorri, R., Belluci, G. C., Altieri, F., ... Forget, F. (2005). Mars surface diversity as revealed by the OMEGA/Mars express observations. Science, 307(5715), 1576-1581. https://doi.org/10.1126/science.1108806

@article{a1bbfe59d0894cc5978452f226e072c7,

title = "Mars surface diversity as revealed by the OMEGA/Mars express observations",

abstract = "The Observatoire pour la Min{\'e}ralogie, l'Eau, les Glaces, et l'Activit{\'e} (OMEGA) investigation, on board the European Space Agency Mars Express mission, is mapping the surface composition of Mars at a 0.3- to 5-kilometer resolution by means of visible - near-infrared hyperspectral reflectance imagery. The data acquired during the first 9 months of the mission already reveal a diverse and complex surface mineralogy, offering key insights into the evolution of Mars. OMEGA has identified and mapped mafic iron-bearing silicates of both the northern and southern crust, localized concentrations of hydrated phyllosilicates and sulfates but no carbonates, and ices and frosts with a water-ice composition of the north polar perennial cap, as for the south cap, covered by a thin carbon dioxide-ice veneer.",

author = "Bibring, \{Jean Pierre\} and Yves Langevin and Aline Gendrin and Brigitte Gondet and Fran{\c c}ois Poulet and Michel Berth{\'e} and Alain Soufflot and Ray Arvidson and Nicolas Mangold and John Mustard and P. Drossart and St{\'e}phane Erard and Olivier Fomi and Michel Combes and Th{\'e}r{\`e}se Encrenaz and Thierry Fouchet and Riccardo Merchiorri and Belluci, \{Gian Carlo\} and Francesca Altieri and Vittorio Formisano and Guillaume Bonello and Fabricio Capaccioni and Pricilla Cerroni and Angioletta Coradini and Sergio Fonti and Volodia Kottsov and Nikolai Ignatiev and Vassili Moroz and Dimitri Titov and Ludmilla Zasova and Patrick Pinet and Sylvain Dout{\'e} and Bernard Schmitt and Christophe Sotin and Ernst Hauber and Harald Hoffmann and Ralf Jaumann and Uwe Keller and Tom Duxbury and Fran{\c c}ois Forget",

year = "2005",

month = mar,

day = "11",

doi = "10.1126/science.1108806",

language = "English",

volume = "307",

pages = "1576--1581",

journal = "Science",

issn = "0036-8075",

number = "5715",

}

Bibring, JP, Langevin, Y, Gendrin, A, Gondet, B, Poulet, F, Berthé, M, Soufflot, A, Arvidson, R, Mangold, N, Mustard, J, Drossart, P, Erard, S, Fomi, O, Combes, M, Encrenaz, T, Fouchet, T, Merchiorri, R, Belluci, GC, Altieri, F, Formisano, V, Bonello, G, Capaccioni, F, Cerroni, P, Coradini, A, Fonti, S, Kottsov, V, Ignatiev, N, Moroz, V, Titov, D, Zasova, L, Pinet, P, Douté, S, Schmitt, B, Sotin, C, Hauber, E, Hoffmann, H, Jaumann, R, Keller, U, Duxbury, T & Forget, F 2005, 'Mars surface diversity as revealed by the OMEGA/Mars express observations', Science, VOL. 307, Numéro 5715, p. 1576-1581. https://doi.org/10.1126/science.1108806

TY - JOUR

T1 - Mars surface diversity as revealed by the OMEGA/Mars express observations

AU - Bibring, Jean Pierre

AU - Langevin, Yves

AU - Gendrin, Aline

AU - Gondet, Brigitte

AU - Poulet, François

AU - Berthé, Michel

AU - Soufflot, Alain

AU - Arvidson, Ray

AU - Mangold, Nicolas

AU - Mustard, John

AU - Drossart, P.

AU - Erard, Stéphane

AU - Fomi, Olivier

AU - Combes, Michel

AU - Encrenaz, Thérèse

AU - Fouchet, Thierry

AU - Merchiorri, Riccardo

AU - Belluci, Gian Carlo

AU - Altieri, Francesca

AU - Formisano, Vittorio

AU - Bonello, Guillaume

AU - Capaccioni, Fabricio

AU - Cerroni, Pricilla

AU - Coradini, Angioletta

AU - Fonti, Sergio

AU - Kottsov, Volodia

AU - Ignatiev, Nikolai

AU - Moroz, Vassili

AU - Titov, Dimitri

AU - Zasova, Ludmilla

AU - Pinet, Patrick

AU - Douté, Sylvain

AU - Schmitt, Bernard

AU - Sotin, Christophe

AU - Hauber, Ernst

AU - Hoffmann, Harald

AU - Jaumann, Ralf

AU - Keller, Uwe

AU - Duxbury, Tom

AU - Forget, François

PY - 2005/3/11

Y1 - 2005/3/11

N2 - The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) investigation, on board the European Space Agency Mars Express mission, is mapping the surface composition of Mars at a 0.3- to 5-kilometer resolution by means of visible - near-infrared hyperspectral reflectance imagery. The data acquired during the first 9 months of the mission already reveal a diverse and complex surface mineralogy, offering key insights into the evolution of Mars. OMEGA has identified and mapped mafic iron-bearing silicates of both the northern and southern crust, localized concentrations of hydrated phyllosilicates and sulfates but no carbonates, and ices and frosts with a water-ice composition of the north polar perennial cap, as for the south cap, covered by a thin carbon dioxide-ice veneer.

AB - The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) investigation, on board the European Space Agency Mars Express mission, is mapping the surface composition of Mars at a 0.3- to 5-kilometer resolution by means of visible - near-infrared hyperspectral reflectance imagery. The data acquired during the first 9 months of the mission already reveal a diverse and complex surface mineralogy, offering key insights into the evolution of Mars. OMEGA has identified and mapped mafic iron-bearing silicates of both the northern and southern crust, localized concentrations of hydrated phyllosilicates and sulfates but no carbonates, and ices and frosts with a water-ice composition of the north polar perennial cap, as for the south cap, covered by a thin carbon dioxide-ice veneer.

U2 - 10.1126/science.1108806

DO - 10.1126/science.1108806

M3 - Article

C2 - 15718430

AN - SCOPUS:20144365375

SN - 0036-8075

VL - 307

SP - 1576

EP - 1581

JO - Science

JF - Science

IS - 5715

ER -

Mars surface diversity as revealed by the OMEGA/Mars express observations

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