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The Complex Molecules Detector (CMOLD): A Fluidic-Based Instrument Suite to Search for (Bio)chemical Complexity on Mars and Icy Moons

Authors :
R. L. Heredero
Victor Parro
Olga Prieto-Ballesteros
Javier Gómez-Elvira
Tomás Belenguer
Mercedes Moreno-Paz
Andoni Moral
José Antonio Rodríguez-Manfredi
Carlos Briones
Alberto G. Fairén
Unidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737
Briones, C. [0000-0003-2213-8353]
Prieto Ballesteros, O. [0000-0002-2278-1210]
López Heredero, R. [0000-0002-2197-8388]
European Research Council (ERC)
Agencia Estatal de Investigación (AEI)
European Commission (EC)
Source :
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial, Universitat Pompeu Fabra, Digital.CSIC. Repositorio Institucional del CSIC, instname, Astrobiology, Instituto Nacional de Técnica Aeroespacial (INTA), Universidad de Alicante (UA)
Publication Year :
2020
Publisher :
Mary Ann Liebert Publishers, 2020.

Abstract

Organic chemistry is ubiquitous in the Solar System, and both Mars and a number of icy satellites of the outer Solar System show substantial promise for having hosted or hosting life. Here, we propose a novel astrobiologically focused instrument suite that could be included as scientific payload in future missions to Mars or the icy moons: the Complex Molecules Detector, or CMOLD. CMOLD is devoted to determining different levels of prebiotic/biotic chemical and structural targets following a chemically general approach (i.e., valid for both terrestrial and nonterrestrial life), as well as their compatibility with terrestrial life. CMOLD is based on a microfluidic block that distributes a liquid suspension sample to three instruments by using complementary technologies: (1) novel microscopic techniques for identifying ultrastructures and cell-like morphologies, (2) Raman spectroscopy for detecting universal intramolecular complexity that leads to biochemical functionality, and (3) bioaffinity-based systems (including antibodies and aptamers as capture probes) for finding life-related and nonlife-related molecular structures. We highlight our current developments to make this type of instruments flight-ready for upcoming Mars missions: the Raman spectrometer included in the science payload of the ESAs Rosalind Franklin rover (Raman Laser Spectrometer instrument) to be launched in 2022, and the biomarker detector that was included as payload in the NASA Icebreaker lander mission proposal (SOLID instrument). CMOLD is a robust solution that builds on the combination of three complementary, existing techniques to cover a wide spectrum of targets in the search for (bio)chemical complexity in the Solar System.<br />This work has been funded by the project “MarsFirstWater,” European Research Council Consolidator grant number 818602 to Alberto G. Fairén; the Spanish Ministry of Economy and Competitiveness (MINECO) and EU FEDER program projects no. ESP2015-69540-R, RTI2018-094368-B-I00, BIO2016-79618-R, and ESP2017-89053-C2-1-P; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737)

Details

Database :
OpenAIRE
Journal :
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial, Universitat Pompeu Fabra, Digital.CSIC. Repositorio Institucional del CSIC, instname, Astrobiology, Instituto Nacional de Técnica Aeroespacial (INTA), Universidad de Alicante (UA)
Accession number :
edsair.doi.dedup.....231f4ecb7cc24c0d0605de40a2c0aeee