The Ground-Based BIOMEX Experiment Verification Tests for Life Detection on Mars

The success of an astrobiological search for life campaign on Mars, or other planetary bodies in the Solar System, relies on the detectability of past or present microbial life traces, namely, biosignatures. Spectroscopic methods require little or no sample preparation, can be repeated almost endles...

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Autores principales: Claudia Pacelli, Alessia Cassaro, Ilaria Catanzaro, Mickael Baqué, Alessandro Maturilli, Ute Böttger, Elke Rabbow, Jean-Pierre Paul de Vera, Silvano Onofri
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Publicado: MDPI AG 2021
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Acceso en línea:https://doaj.org/article/a8ddd93b691f45fb8fc3c4afa2667714
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spelling oai:doaj.org-article:a8ddd93b691f45fb8fc3c4afa26677142021-11-25T18:11:15ZThe Ground-Based BIOMEX Experiment Verification Tests for Life Detection on Mars10.3390/life111112122075-1729https://doaj.org/article/a8ddd93b691f45fb8fc3c4afa26677142021-11-01T00:00:00Zhttps://www.mdpi.com/2075-1729/11/11/1212https://doaj.org/toc/2075-1729The success of an astrobiological search for life campaign on Mars, or other planetary bodies in the Solar System, relies on the detectability of past or present microbial life traces, namely, biosignatures. Spectroscopic methods require little or no sample preparation, can be repeated almost endlessly, and can be performed in contact or even remotely. Such methods are therefore ideally suited to use for the detection of biosignatures, which can be confirmed with supporting instrumentation. Here, we discuss the use of Raman and Fourier Transform Infrared (FT-IR) spectroscopies for the detection and characterization of biosignatures from colonies of the fungus Cryomyces antarcticus, grown on Martian analogues and exposed to increasing doses of UV irradiation under dried conditions. The results report significant UV-induced DNA damage, but the non-exceeding of thresholds for allowing DNA amplification and detection, while the spectral properties of the fungal melanin remained unaltered, and pigment detection and identification was achieved via complementary analytical techniques. Finally, this work found that fungal cell wall compounds, likely chitin, were not degraded, and were still detectable even after high UV irradiation doses. The implications for the preservation and detection of biosignatures in extraterrestrial environments are discussed.Claudia PacelliAlessia CassaroIlaria CatanzaroMickael BaquéAlessandro MaturilliUte BöttgerElke RabbowJean-Pierre Paul de VeraSilvano OnofriMDPI AGarticlebiosignaturedark pigmentspolysaccharidespolychromatic radiationsimulated conditionsMarsScienceQENLife, Vol 11, Iss 1212, p 1212 (2021)
institution DOAJ
collection DOAJ
language EN
topic biosignature
dark pigments
polysaccharides
polychromatic radiation
simulated conditions
Mars
Science
Q
spellingShingle biosignature
dark pigments
polysaccharides
polychromatic radiation
simulated conditions
Mars
Science
Q
Claudia Pacelli
Alessia Cassaro
Ilaria Catanzaro
Mickael Baqué
Alessandro Maturilli
Ute Böttger
Elke Rabbow
Jean-Pierre Paul de Vera
Silvano Onofri
The Ground-Based BIOMEX Experiment Verification Tests for Life Detection on Mars
description The success of an astrobiological search for life campaign on Mars, or other planetary bodies in the Solar System, relies on the detectability of past or present microbial life traces, namely, biosignatures. Spectroscopic methods require little or no sample preparation, can be repeated almost endlessly, and can be performed in contact or even remotely. Such methods are therefore ideally suited to use for the detection of biosignatures, which can be confirmed with supporting instrumentation. Here, we discuss the use of Raman and Fourier Transform Infrared (FT-IR) spectroscopies for the detection and characterization of biosignatures from colonies of the fungus Cryomyces antarcticus, grown on Martian analogues and exposed to increasing doses of UV irradiation under dried conditions. The results report significant UV-induced DNA damage, but the non-exceeding of thresholds for allowing DNA amplification and detection, while the spectral properties of the fungal melanin remained unaltered, and pigment detection and identification was achieved via complementary analytical techniques. Finally, this work found that fungal cell wall compounds, likely chitin, were not degraded, and were still detectable even after high UV irradiation doses. The implications for the preservation and detection of biosignatures in extraterrestrial environments are discussed.
format article
author Claudia Pacelli
Alessia Cassaro
Ilaria Catanzaro
Mickael Baqué
Alessandro Maturilli
Ute Böttger
Elke Rabbow
Jean-Pierre Paul de Vera
Silvano Onofri
author_facet Claudia Pacelli
Alessia Cassaro
Ilaria Catanzaro
Mickael Baqué
Alessandro Maturilli
Ute Böttger
Elke Rabbow
Jean-Pierre Paul de Vera
Silvano Onofri
author_sort Claudia Pacelli
title The Ground-Based BIOMEX Experiment Verification Tests for Life Detection on Mars
title_short The Ground-Based BIOMEX Experiment Verification Tests for Life Detection on Mars
title_full The Ground-Based BIOMEX Experiment Verification Tests for Life Detection on Mars
title_fullStr The Ground-Based BIOMEX Experiment Verification Tests for Life Detection on Mars
title_full_unstemmed The Ground-Based BIOMEX Experiment Verification Tests for Life Detection on Mars
title_sort ground-based biomex experiment verification tests for life detection on mars
publisher MDPI AG
publishDate 2021
url https://doaj.org/article/a8ddd93b691f45fb8fc3c4afa2667714
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