David C Fernández-Remolar

Prof. David C Fernández-Remolar

orcid

Research Focus & Metrics

Academic Career Length

26Years (2001-Present)

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

Representative Publications

View All Publications
1 November 2005 in Earth and Planetary Science Letters
Verified
Journal Article
Closed access
DFDavid C Fernández-Remolar
David C Fernández-Remolar
RMRichard V. Morris
Richard V. Morris
JGJohn E. Gruener
John E. Gruener
RARicardo Amils
Ricardo Amils
AKAndrew H. Knoll
Andrew H. Knoll

1 February 2007 in Planetary and Space Science
Verified
Journal Article
Closed access
RARicardo Amils
Ricardo Amils
EGElena González-Toril
Elena González-Toril
DFDavid C Fernández-Remolar
David C Fernández-Remolar
Felipe GómezFelipe Gómez
Felipe Gómez
ÁAÁngeles Aguilera
Ángeles Aguilera
JSJosé Luis Sanz
José Luis Sanz

1 September 2004 in Nature
Verified
Journal Article
Closed access
AFAlberto G. Fairén
Alberto G. Fairén
DFDavid C Fernández-Remolar
David C Fernández-Remolar
JDJames M. Dohm
James M. Dohm
VBVictor R. Baker
Victor R. Baker
RARicardo Amils
Ricardo Amils

1 December 2011 in Astrobiology
Verified
Journal Article
Closed access
VPVictor Parro
Victor Parro
GDGraciela de Diego-Castilla
Graciela de Diego-Castilla
MMMercedes Moreno-Paz
Mercedes Moreno-Paz
YBYolanda Blanco
Yolanda Blanco
PCPatricia Cruz-Gil
Patricia Cruz-Gil
JGJavier Gómez-Elvira
Javier Gómez-Elvira
The Atacama Desert has long been considered a good Mars analogue for testing instrumentation for planetary exploration, but very few data (if any) have been reported about the geomicrobiology of its salt-rich subsurface. We performed a Mars analogue drilling campaign next to the Salar Grande (Atacama, Chile) in July 2009, and several cores and powder samples from up to 5 m deep were analyzed in situ with LDChip300 (a Life Detector Chip containing 300 antibodies). Here, we show the discovery of a hypersaline subsurface microbial habitat associated with halite-, nitrate-, and perchlorate-containing salts at 2 m deep. LDChip300 detected bacteria, archaea, and other biological material (DNA, exopolysaccharides, some peptides) from the analysis of less than 0.5 g of ground core sample. The results were supported by oligonucleotide microarray hybridization in the field and finally confirmed by molecular phylogenetic analysis and direct visualization of microbial cells bound to halite crystals in the laboratory. Geochemical analyses revealed a habitat with abundant hygroscopic salts like halite (up to 260 g kg−1) and perchlorate (41.13 μg g−1 maximum), which allow deliquescence events at low relative humidity. Thin liquid water films would permit microbes to proliferate by using detected organic acids like acetate (19.14 μg g−1) or formate (76.06 μg g−1) as electron donors, and sulfate (15875 μg g−1), nitrate (13490 μg g−1), or perchlorate as acceptors. Our results correlate with the discovery of similar hygroscopic salts and possible deliquescence processes on Mars, and open new search strategies for subsurface martian biota. The performance demonstrated by our LDChip300 validates this technology for planetary exploration, particularly for the search for life on Mars. Key Words: Atacama Desert—Life detection—Biosensor—Biopolymers—In situ measurement. Astrobiology 11, 969–996.

1 February 2011 in Chemical Geology
Verified
Journal Article
Closed access
MSMonica Sanchez-Roman
Monica Sanchez-Roman
CRChristopher S. Romanek
Christopher S. Romanek
DFDavid C Fernández-Remolar
David C Fernández-Remolar
ASAntonio Sánchez-Navas
Antonio Sánchez-Navas
JMJudith Ann McKenzie
Judith Ann McKenzie
CVCrisogono Vasconcelos
Crisogono Vasconcelos

1 January 2004 in Planetary and Space Science
Verified
Journal Article
Closed access
DFDavid C Fernández-Remolar
David C Fernández-Remolar
JGJ. Gómez-Elvira
J. Gómez-Elvira
Felipe GómezFelipe Gómez
Felipe Gómez
ESE. Sebastian
E. Sebastian
JMJ. Martı́in
J. Martı́in
RAR. Amils
R. Amils