Kathleen Campbell

Prof. Kathleen Campbell

Faculty of Science, The University of Auckland, Auckland 1010, New Zealand

Research Focus & Metrics

Academic Career Length

35Years (1992-Present)

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

Representative Publications

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1 March 2006 in Palaeogeography, Palaeoclimatology, Palaeoecology
Verified
Journal Article
Closed access
Kathleen CampbellKathleen Campbell
Kathleen Campbell

1 November 2015 in Astrobiology
Verified
Journal Article
Open access
FWFrances Westall
Frances Westall
FFFrédéric Foucher
Frédéric Foucher
NBNicolas Bost
Nicolas Bost
MBMarylène Bertrand
Marylène Bertrand
DLDamien Loizeau
Damien Loizeau
CCCharles S. Cockell
Charles S. Cockell
The search for traces of life is one of the principal objectives of Mars exploration. Central to this objective is the concept of habitability, the set of conditions that allows the appearance of life and successful establishment of microorganisms in any one location. While environmental conditions may have been conducive to the appearance of life early in martian history, habitable conditions were always heterogeneous on a spatial scale and in a geological time frame. This “punctuated” scenario of habitability would have had important consequences for the evolution of martian life, as well as for the presence and preservation of traces of life at a specific landing site. We hypothesize that, given the lack of long-term, continuous habitability, if martian life developed, it was (and may still be) chemotrophic and anaerobic. Obtaining nutrition from the same kinds of sources as early terrestrial chemotrophic life and living in the same kinds of environments, the fossilized traces of the latter serve as useful proxies for understanding the potential distribution of martian chemotrophs and their fossilized traces. Thus, comparison with analog, anaerobic, volcanic terrestrial environments (Early Archean >3.5–3.33 Ga) shows that the fossil remains of chemotrophs in such environments were common, although sparsely distributed, except in the vicinity of hydrothermal activity where nutrients were readily available. Moreover, the traces of these kinds of microorganisms can be well preserved, provided that they are rapidly mineralized and that the sediments in which they occur are rapidly cemented. We evaluate the biogenicity of these signatures by comparing them to possible abiotic features. Finally, we discuss the implications of different scenarios for life on Mars for detection by in situ exploration, ranging from its non-appearance, through preserved traces of life, to the presence of living microorganisms. Key Words: Mars—Early Earth—Anaerobic chemotrophs—Biosignatures—Astrobiology missions to Mars. Astrobiology 15, 998–1029.

7 May 2002 in Geofluids
Verified
Journal Article
Closed access
PDF file
Kathleen CampbellKathleen Campbell
Kathleen Campbell
JFJ. D. Farmer
J. D. Farmer
DMD. Des Marais
D. Des Marais

15 January 2000 in Mineralium Deposita
Verified
Journal Article
Closed access
PDF file
NHN. R. Herdianita
N. R. Herdianita
PBP. R. L. Browne
P. R. L. Browne
KRK. A. Rodgers
K. A. Rodgers
Kathleen CampbellKathleen Campbell
Kathleen Campbell

1 September 2007 in Sedimentary Geology
Verified
Journal Article
Closed access
RPRandall S. Perry
Randall S. Perry
NMNicola Mcloughlin
Nicola Mcloughlin
BLBridget Y. Lynne
Bridget Y. Lynne
MSMark A. Sephton
Mark A. Sephton
JOJoan D. Oliver
Joan D. Oliver
JSJames T. Staley
James T. Staley

1 January 1995 in Geology
Verified
Journal Article
Closed access
Kathleen CampbellKathleen Campbell
Kathleen Campbell
DBDavid J. Bottjer
David J. Bottjer