Literature DB >> 20735252

Hygroscopic salts and the potential for life on Mars.

Alfonso F Davila1, Luis Gago Duport, Riccardo Melchiorri, Jochen Jänchen, Sergio Valea, Asunción de Los Rios, Alberto G Fairén, Diedrich Möhlmann, Christopher P McKay, Carmen Ascaso, Jacek Wierzchos.   

Abstract

Hygroscopic salts have been detected in soils in the northern latitudes of Mars, and widespread chloride-bearing evaporitic deposits have been detected in the southern highlands. The deliquescence of hygroscopic minerals such as chloride salts could provide a local and transient source of liquid water that would be available for microorganisms on the surface. This is known to occur in the Atacama Desert, where massive halite evaporites have become a habitat for photosynthetic and heterotrophic microorganisms that take advantage of the deliquescence of the salt at certain relative humidity (RH) levels. We modeled the climate conditions (RH and temperature) in a region on Mars with chloride-bearing evaporites, and modeled the evolution of the water activity (a(w)) of the deliquescence solutions of three possible chloride salts (sodium chloride, calcium chloride, and magnesium chloride) as a function of temperature. We also studied the water absorption properties of the same salts as a function of RH. Our climate model results show that the RH in the region with chloride-bearing deposits on Mars often reaches the deliquescence points of all three salts, and the temperature reaches levels above their eutectic points seasonally, in the course of a martian year. The a(w) of the deliquescence solutions increases with decreasing temperature due mainly to the precipitation of unstable phases, which removes ions from the solution. The deliquescence of sodium chloride results in transient solutions with a(w) compatible with growth of terrestrial microorganisms down to 252 K, whereas for calcium chloride and magnesium chloride it results in solutions with a(w) below the known limits for growth at all temperatures. However, taking the limits of a(w) used to define special regions on Mars, the deliquescence of calcium chloride deposits would allow for the propagation of terrestrial microorganisms at temperatures between 265 and 253 K, and for metabolic activity (no growth) at temperatures between 253 and 233 K.

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Year:  2010        PMID: 20735252     DOI: 10.1089/ast.2009.0421

Source DB:  PubMed          Journal:  Astrobiology        ISSN: 1557-8070            Impact factor:   4.335


  30 in total

1.  A microbial oasis in the hypersaline Atacama subsurface discovered by a life detector chip: implications for the search for life on Mars.

Authors:  Victor Parro; Graciela de Diego-Castilla; Mercedes Moreno-Paz; Yolanda Blanco; Patricia Cruz-Gil; José A Rodríguez-Manfredi; David Fernández-Remolar; Felipe Gómez; Manuel J Gómez; Luis A Rivas; Cecilia Demergasso; Alex Echeverría; Viviana N Urtuvia; Marta Ruiz-Bermejo; Miriam García-Villadangos; Marina Postigo; Mónica Sánchez-Román; Guillermo Chong-Díaz; Javier Gómez-Elvira
Journal:  Astrobiology       Date:  2011-12-09       Impact factor: 4.335

2.  Prevalence of sucretolerant bacteria in common soils and their isolation and characterization.

Authors:  Casper Fredsgaard; Donald B Moore; Fei Chen; Benton C Clark; Mark A Schneegurt
Journal:  Antonie Van Leeuwenhoek       Date:  2017-04-13       Impact factor: 2.271

3.  DISTRIBUTION AND HABITABILITY OF (META)STABLE BRINES ON PRESENT-DAY MARS.

Authors:  Edgard G Rivera-Valentín; Vincent F Chevrier; Alejandro Soto; Germán Martínez
Journal:  Nat Astron       Date:  2020-05-11       Impact factor: 14.437

4.  Identification and Characterization of Early Mission Phase Microorganisms Residing on the Mars Science Laboratory and Assessment of Their Potential to Survive Mars-like Conditions.

Authors:  Stephanie A Smith; James N Benardini; David Anderl; Matt Ford; Emmaleen Wear; Michael Schrader; Wayne Schubert; Linda DeVeaux; Andrzej Paszczynski; Susan E Childers
Journal:  Astrobiology       Date:  2017-03-10       Impact factor: 4.335

Review 5.  Trajectories of martian habitability.

Authors:  Charles S Cockell
Journal:  Astrobiology       Date:  2014-02-07       Impact factor: 4.335

6.  Evidence of in situ microbial activity and sulphidogenesis in perennially sub-0 °C and hypersaline sediments of a high Arctic permafrost spring.

Authors:  Guillaume Lamarche-Gagnon; Raven Comery; Charles W Greer; Lyle G Whyte
Journal:  Extremophiles       Date:  2014-11-09       Impact factor: 2.395

7.  Perchlorate and halophilic prokaryotes: implications for possible halophilic life on Mars.

Authors:  Aharon Oren; Rahel Elevi Bardavid; Lily Mana
Journal:  Extremophiles       Date:  2013-10-23       Impact factor: 2.395

8.  Carbon monoxide as a metabolic energy source for extremely halophilic microbes: implications for microbial activity in Mars regolith.

Authors:  Gary M King
Journal:  Proc Natl Acad Sci U S A       Date:  2015-03-23       Impact factor: 11.205

9.  Widen the belt of habitability!

Authors:  D Möhlmann
Journal:  Orig Life Evol Biosph       Date:  2012-05-26       Impact factor: 1.950

10.  Bacterial Growth in Saturated and Eutectic Solutions of Magnesium Sulphate and Potassium Chlorate with Relevance to Mars and the Ocean Worlds.

Authors:  Jonathan M Wilks; Fei Chen; Benton C Clark; Mark A Schneegurt
Journal:  Int J Astrobiol       Date:  2019-01-28       Impact factor: 1.673

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