Cited by 384Planetary Science and ExplorationAstro and Planetary ScienceSpace Science and Extraterrestrial Life

Reanalysis of the Viking results suggests perchlorate and organics at midlatitudes on Mars

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Navarro‐González, Rafael, Vargas, Edgar, de la Rosa, José, Raga, Alejandro C., McKay, Christopher P.·2010·Journal of Geophysical Research: Planets

Abstract

The most comprehensive search for organics in the Martian soil was performed by the Viking Landers. Martian soil was subjected to a thermal volatilization process to vaporize and break organic molecules, and the resultant gases and volatiles were analyzed by gas chromatography‐mass spectrometry. Only water at 0.1–1.0 wt% was detected, with traces of chloromethane at 15 ppb, at Viking landing site 1, and water at 0.05–1.0 wt% and carbon dioxide at 50–700 ppm, with traces of dichloromethane at 0.04–40 ppb, at Viking landing site 2. These chlorohydrocarbons were considered to be terrestrial contaminants, although they had not been detected at those levels in the blank runs. Recently, perchlorate was discovered in the Martian Arctic soil by the Phoenix Lander. Here we show that when Mars‐like soils from the Atacama Desert containing 32 ± 6 ppm of organic carbon are mixed with 1 wt% magnesium perchlorate and heated, nearly all the organics present are decomposed to water and carbon dioxide, but a small amount is chlorinated, forming 1.6 ppm of chloromethane and 0.02 ppm of dichloromethane at 500°C. A chemical kinetics model was developed to predict the degree of oxidation and chlorination of organics in the Viking oven. Reinterpretation of the Viking results therefore suggests ≤0.1% perchlorate and 1.5–6.5 ppm organic carbon at landing site 1 and ≤0.1% perchlorate and 0.7–2.6 ppm organic carbon at landing site 2. The detection of organics on Mars is important to assess locations for future experiments to detect life itself.

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Crossref · 10.1029/2010je003599

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  • Phoenix detected perchlorates in the martian surface, which could explain the nondetection of organics even if present, because perchlorate is highly oxidizing at elevated temperatures and may have destroyed martian organics before detection.

    “More recently, the Phoenix lander detected perchlorates in the martian surface, which could explain the nondetection of organics even if present (Navarro-González et al., 2010). Perchlorate is highly oxidizing at the elevated temperatures of pyrolytic experiments and so may have destroyed martian organics before detection.”

    From The Astrobiology Primer v2.0 (2016) · cites this paper as Navarro-González et al., 2010

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Authors
Navarro‐González, R., Vargas, E., de la Rosa, J., Raga, A. C., & McKay, C. P.
Affiliations
  • Laboratorio de Química de Plasmas y Estudios Planetarios, Instituto de Ciencias Nucleares Universidad Nacional Autónoma de México, Circuito Exterior, Ciudad Universitaria Mexico City Mexico
  • Universidad Nacional Autónoma de México (MX)
  • Ames Research Center (US)
Venue
Journal of Geophysical Research: Planets
Published
2010-12
Volume
115
Issue
E12
ISSN
0148-0227 (ISSN-L)
OpenAlex
W1970425118
Cited by
384
References
51
Citations by year
2026: 15 · 2025: 18 · 2024: 17 · 2023: 24 · 2022: 22 · 2021: 24 · 2020: 27 · 2019: 28 · 2018: 36 · 2017: 20 · 2016: 24 · 2015: 23 · 2014: 31 · 2013: 26 · 2012: 25
FWCI
13.23
Type
journal article
Language
en
Open access
Locations
Journal of Geophysical Research Atmospheres (publishedVersion)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
Keywords
Viking landers, perchlorate, methyl chloride, dichloromethane, thermal volatilization, organic carbon, chemical kinetic modeling

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