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Detection of methane in the atmosphere of Mars

Author
FORMISANO, Vittorio1 ; ATREYA, Sushil2 ; ENCRENAZ, Thérèse3 ; IGNATIEV, Nikolai1 4 ; GIURANNA, Marco1
[1] Istituto di Fisica dello Spazio Interplanetario INAF-IFSI, Via del Fosso del Cavaliere 100, 00133 Rome, Italy
[2] Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI 48109-2143, United States
[3] Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique (LESIA), Observatoire de Paris, 5 Place Janssen, 92195 Meudon, France
[4] Space Research Institute of Russian Academy of Sciences (IKI) Profsojuznaja 84/32, 117810 Moscow, Russian Federation
Source

Science (Washington, D.C.). 2004, Vol 306, Num 5702, pp 1758-1761, 4 p

CODEN
SCIEAS
ISSN
0036-8075
Scientific domain
Multidisciplinary
Publisher
American Association for the Advancement of Science, Washington, DC
Publication country
United States
Document type
Article
Language
Russian
Keyword (fr)
Atmosphère planétaire Composition chimique Méthane Observation par sonde spatiale Planète Mars Rapport mélange Spectre IR
Keyword (en)
Planetary atmospheres Chemical composition Methane Space probe observation Mars planet Mixing ratio Infrared spectra
Keyword (es)
Observación por sonda espacial
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B30 Planets, their satellites and rings. Asteroids / 001E03B30G Mars

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B35 Planetary, asteroid, and satellite characteristics and properties / 001E03B35E Chemical composition

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16341340

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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