Literature DB >> 24552233

Science applications of a multispectral microscopic imager for the astrobiological exploration of Mars.

Jorge I Núñez1, Jack D Farmer, R Glenn Sellar, Gregg A Swayze, Diana L Blaney.   

Abstract

Future astrobiological missions to Mars are likely to emphasize the use of rovers with in situ petrologic capabilities for selecting the best samples at a site for in situ analysis with onboard lab instruments or for caching for potential return to Earth. Such observations are central to an understanding of the potential for past habitable conditions at a site and for identifying samples most likely to harbor fossil biosignatures. The Multispectral Microscopic Imager (MMI) provides multispectral reflectance images of geological samples at the microscale, where each image pixel is composed of a visible/shortwave infrared spectrum ranging from 0.46 to 1.73 μm. This spectral range enables the discrimination of a wide variety of rock-forming minerals, especially Fe-bearing phases, and the detection of hydrated minerals. The MMI advances beyond the capabilities of current microimagers on Mars by extending the spectral range into the infrared and increasing the number of spectral bands. The design employs multispectral light-emitting diodes and an uncooled indium gallium arsenide focal plane array to achieve a very low mass and high reliability. To better understand and demonstrate the capabilities of the MMI for future surface missions to Mars, we analyzed samples from Mars-relevant analog environments with the MMI. Results indicate that the MMI images faithfully resolve the fine-scale microtextural features of samples and provide important information to help constrain mineral composition. The use of spectral endmember mapping reveals the distribution of Fe-bearing minerals (including silicates and oxides) with high fidelity, along with the presence of hydrated minerals. MMI-based petrogenetic interpretations compare favorably with laboratory-based analyses, revealing the value of the MMI for future in situ rover-mediated astrobiological exploration of Mars. Mars-Microscopic imager-Multispectral imaging-Spectroscopy-Habitability-Arm instrument.

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Year:  2014        PMID: 24552233      PMCID: PMC3929460          DOI: 10.1089/ast.2013.1079

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


  17 in total

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Journal:  J Geophys Res       Date:  1999-11-25

2.  Spectral and other physicochemical properties of submicron powders of hematite (alpha-Fe2O3), maghemite (gamma-Fe2O3), magnetite (Fe3O4), goethite (alpha-FeOOH), and lepidocrocite (gamma-FeOOH).

Authors:  R V Morris; H V Lauer; C A Lawson; E K Gibson; G A Nace; C Stewart
Journal:  J Geophys Res       Date:  1985-03-10

3.  Sulfates in the north polar region of Mars detected by OMEGA/Mars Express.

Authors:  Yves Langevin; François Poulet; Jean-Pierre Bibring; Brigitte Gondet
Journal:  Science       Date:  2005-02-17       Impact factor: 47.728

4.  The Mars Astrobiology Explorer-Cacher (MAX-C): a potential rover mission for 2018. Final report of the Mars Mid-Range Rover Science Analysis Group (MRR-SAG) October 14, 2009.

Authors: 
Journal:  Astrobiology       Date:  2010-03       Impact factor: 4.335

5.  Subglacial hydrothermal alteration minerals in Jökulhlaup deposits of Southern Iceland, with implications for detecting past or present habitable environments on Mars.

Authors:  Nicholas H Warner; Jack D Farmer
Journal:  Astrobiology       Date:  2010-06       Impact factor: 4.335

6.  Water alteration of rocks and soils on Mars at the Spirit rover site in Gusev crater.

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Journal:  Nature       Date:  2005-07-07       Impact factor: 49.962

7.  Pigmenting agents in Martian soils: inferences from spectral, Mossbauer, and magnetic properties of nanophase and other iron oxides in Hawaiian palagonitic soil PN-9.

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Journal:  Geochim Cosmochim Acta       Date:  1993-10       Impact factor: 5.010

8.  Chloride-bearing materials in the southern highlands of Mars.

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Journal:  Science       Date:  2008-03-21       Impact factor: 47.728

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Journal:  Science       Date:  2008-05-23       Impact factor: 47.728

10.  A geochemical model for the formation of hydrothermal carbonates on Mars.

Authors:  L L Griffith; E L Shock
Journal:  Nature       Date:  1995-10-05       Impact factor: 49.962

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  1 in total

Review 1.  Microbial Morphology and Motility as Biosignatures for Outer Planet Missions.

Authors:  Jay Nadeau; Chris Lindensmith; Jody W Deming; Vicente I Fernandez; Roman Stocker
Journal:  Astrobiology       Date:  2016-08-23       Impact factor: 4.335

  1 in total

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