Paulo De Souza

Paulo De Souza

orcid

Research Focus & Metrics

Academic Career Length

30Years (1997-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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3 December 2004 in Science
Verified
Journal Article
Closed access
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GKG. Klingelhöfer
G. Klingelhöfer
RMR. V. Morris
R. V. Morris
BBB. Bernhardt
B. Bernhardt
CSC. Schröder
C. Schröder
DRD. S. Rodionov
D. S. Rodionov
RAR. E. Arvidson
R. E. Arvidson
Mössbauer spectra measured by the Opportunity rover revealed four mineralogical components in Meridiani Planum at Eagle crater: jarosite- and hematite-rich outcrop, hematite-rich soil, olivine-bearing basaltic soil, and a pyroxene-bearing basaltic rock (Bounce rock). Spherules, interpreted to be concretions, are hematite-rich and dispersed throughout the outcrop. Hematitic soils both within and outside Eagle crater are dominated by spherules and their fragments. Olivine-bearing basaltic soil is present throughout the region. Bounce rock is probably an impact erratic. Because jarosite is a hydroxide sulfate mineral, its presence at Meridiani Planum is mineralogical evidence for aqueous processes on Mars, probably under acid-sulfate conditions.

1 November 2005 in Earth and Planetary Science Letters
Verified
Journal Article
Closed access
SMS.M. McLennan
S.M. McLennan
JBJ.F. Bell
J.F. Bell
WCWendy Calvin
Wendy Calvin
PCP.R. Christensen
P.R. Christensen
BCB.C. Clark
B.C. Clark
AYA. Yen
A. Yen

23 May 2008 in Science
Verified
Journal Article
Closed access
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SSS. W. Squyres
S. W. Squyres
RAR. E. Arvidson
R. E. Arvidson
SRS. Ruff
S. Ruff
RGR. Gellert
R. Gellert
RMR. V. Morris
R. V. Morris
PSPaulo De Souza
Paulo De Souza
Mineral deposits on the martian surface can elucidate ancient environmental conditions on the planet. Opaline silica deposits (as much as 91 weight percent SiO 2 ) have been found in association with volcanic materials by the Mars rover Spirit. The deposits are present both as light-toned soils and as bedrock. We interpret these materials to have formed under hydrothermal conditions and therefore to be strong indicators of a former aqueous environment. This discovery is important for understanding the past habitability of Mars because hydrothermal environments on Earth support thriving microbial ecosystems.

7 July 2005 in Nature
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Journal Article
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AYAlbert S. Yen
Albert S. Yen
RGRalf Gellert
Ralf Gellert
CSChristian Schröder
Christian Schröder
RMRichard V. Morris
Richard V. Morris
JBJames F. Bell
James F. Bell
JZJutta Zipfel
Jutta Zipfel

22 February 2006 in Journal of Geophysical Research
Verified
Journal Article
Closed access
PDF file
RMRichard V Morris
Richard V Morris
GKG. Klingelhöfer
G. Klingelhöfer
CSChristian Schröder
Christian Schröder
DRD. S. Rodionov
D. S. Rodionov
AYA. Yen
A. Yen
RAR. E. Arvidson
R. E. Arvidson

6 August 2004 in Science
Verified
Journal Article
Closed access
PDF file
RMRichard V Morris
Richard V Morris
GKG. Klingelhöfer
G. Klingelhöfer
BBB. Bernhardt
B. Bernhardt
CSC. Schröder
C. Schröder
DRD. S. Rodionov
D. S. Rodionov
RAR. E. Arvidson
R. E. Arvidson
Mössbauer spectra measured on Mars by the Spirit rover during the primary mission are characterized by two ferrous iron doublets (olivine and probably pyroxene) and a ferric iron doublet (tentatively associated to nanophase ferric iron oxide). Two sextets resulting from nonstoichiometric magnetite are also present, except for a coating on the rock Mazatzal, where a hematite-like sextet is present. Greater proportions of ferric-bearing phases are associated with undisturbed soils and rock surfaces as compared to fresh rock surfaces exposed by grinding. The ubiquitous presence of olivine in soil suggests that physical rather than chemical weathering processes currently dominate at Gusev crater.