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Titolo:
The Martian surface composition
Autore:
Bibring, JP; Erard, S;
Indirizzi:
Inst Astrophys Spatiale, F-91405 Orsay, France Inst Astrophys Spatiale Orsay France F-91405 iale, F-91405 Orsay, France
Titolo Testata:
SPACE SCIENCE REVIEWS
fascicolo: 1-4, volume: 96, anno: 2001,
pagine: 293 - 316
SICI:
0038-6308(200104)96:1-4<293:TMSC>2.0.ZU;2-P
Fonte:
ISI
Lingua:
ENG
Soggetto:
THERMAL EMISSION SPECTROMETER; SOIL ANALOG MATERIALS; MU-M; SNC METEORITES; REFLECTANCE SPECTROSCOPY; CHEMICAL-COMPOSITION; LOW-TEMPERATURE; ISM EXPERIMENT; IRON-OXIDES; MARS;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Physical, Chemical & Earth Sciences
Citazioni:
68
Recensione:
Indirizzi per estratti:
Indirizzo: Bibring, JP Inst Astrophys Spatiale, Batiment 121, F-91405 Orsay, France Inst Astrophys Spatiale Batiment 121 Orsay France F-91405 nce
Citazione:
J.P. Bibring e S. Erard, "The Martian surface composition", SPACE SCI R, 96(1-4), 2001, pp. 293-316

Abstract

Mars is unique to have undergone all planetary evolutionary steps, withoutglobal resets, till its geological death: this is reflected in the varietyof its surface features. The determination of Mars surface composition hasthus the potential to identify the processes responsible for the entire Mars evolution, from geological timescales to seasonal variations. Due to technical challenges, only few investigations have been performed so far. Theyare summarized in this paper, and their interpretation is discussed in terms of surface materials (minerals, ices and frosts).

ASDD Area Sistemi Dipartimentali e Documentali, Università di Bologna, Catalogo delle riviste ed altri periodici
Documento generato il 28/03/20 alle ore 10:06:16