Near-Term Mars Sample Return Using In-Situ Oxygen Generation

2007 ◽  
Author(s):  
Phillip Cunio ◽  
Takuto Ishimatsu ◽  
Jim Keller ◽  
Zahra Khan ◽  
Ryan Odegard ◽  
...  
Keyword(s):  
Sample Return ◽  
Oxygen Generation ◽  
Near Term

Mission Incredible: A Titan Sample Return Using In-Situ Propellants

2022 ◽  
Author(s):  
Geoffrey A. Landis ◽  
Steven R. Oleson ◽  
Elizabeth R. Turnbull ◽  
Ralph D. Lorenz ◽  
David A. Smith ◽  
...  
Keyword(s):  
Sample Return

scholarly journals Nanocrystals perovskites photocatalyzed singlet oxygen generation for light-driven organic reactions

2021 ◽  
Author(s):  
Marco Corti ◽  
Rossella Chiara ◽  
Lidia Romani ◽  
Barbara Mannucci ◽  
Lorenzo Malavasi ◽  
...  
Keyword(s):  
Diels Alder ◽  
Organic Reactions ◽  
Hydroxy Ketone ◽  
Oxidation Reactions ◽  
Perovskite Nanocrystals ◽  
Oxygen Generation ◽  
Unsaturated Ketones ◽  
Halide Perovskite ◽  
Lead Halide

AbstractLead halide perovskite nanocrystals were prepared and used as photocatalysts for the in situ 1O2 generation to perform hetero Diels–Alder, ene and oxidation reactions with suitable dienes and alkenes. The methodology has been reasonably standardized and made applicable to a variety of olefinic substrates. The scope of the method is finely illustrated by the results in all the tested reactions, which allowed to obtain desymmetrized hydroxy-ketone derivatives, unsaturated ketones and epoxides. Some limitations were also observed especially in the case of the alkene oxidations as well as poor chemoselectivity was somewhere observed. Graphic abstract 1O2 generated by lead halide perovskite nanocrystals as photocatalyst in organic reactions.

Search for molecular biosignatures on Mars: laboratory simulations of UV irradiation of molecule-mineral complexes

2021 ◽  
Author(s):  
Teresa Fornaro ◽  
Giovanni Poggiali ◽  
Maria Angela Corazzi ◽  
Cristina Garcia ◽  
Giulia Dimitri ◽  
...  
Keyword(s):  
Amino Acids ◽  
Organic Compounds ◽  
Uv Irradiation ◽  
Organic Molecules ◽  
Spectroscopic Characterization ◽  
Sample Return ◽  
Laboratory Simulations ◽  
Prebiotic Molecules

<div> </div> <p><strong>Abstract</strong></p> <p>We present laboratory activities of preparation, characterization, and UV irradiation processing of Mars soil analogues, which are key to support both in situ exploration and sample return missions devoted to detection of molecular biosignatures on Mars.</p> <p>In detail we prepared analog mineral samples relevant to the landing sites of past, present and future Mars exploration missions, such as Gale Crater, Jezero Crater, and Oxia Planum. We doped these samples with a large variety of organic molecules (both biotic and prebiotic molecules) like amino acids, nucleotides, monosaccharides, aldehydes, lipids. We investigated molecular photostability under UV irradiation by monitoring in situ possible modifications of infrared spectroscopic features. These investigations provide pivotal information for ground analysis carried out by rovers on Mars.</p> <p><strong>Introduction</strong></p> <p>Laboratory simulations of Mars are key to support the scientific activity and technology development of life detection instruments on board present and upcoming rover missions such as Mars2020 Perseverance [1] and ExoMars2022 Rosalind Franklin [2]. Studies about the stability of organic molecules in a Martian-like environment allow us to explore the conditions for the preservation of molecular biosignatures and develop models for their degradation in the Martian geological record. A systematic study of the effects of UV radiation on a variety of molecule-mineral complexes mimicking Martian soil can be key for the selection of the most interesting samples to analyse in situ or/and collect for sample return. Testing the sensitivity of different techniques for detection of the diagnostic features of molecular biosignatures embedded into mineral matrices as a function of the molecular concentration helps the choice, design and operation of flight instruments, as well as the interpretation of data collected on the ground during mission operative periods.</p> <p><strong>Methods</strong></p> <p>Experimental analyses were conducted in the Astrobiology Laboratory at INAF-Astrophysical Observatory of Arcetri (Firenze, Italy). Laboratory activities pertain to: (i) synthesis of Mars soil analogues doped with organic compounds that are considered potential molecular biosignatures; (ii) UV-irradiation processing of the Mars soil analogues under Martian-like conditions; and (iii) spectroscopic characterization of the Mars soil analogues.</p> <p><strong>Results</strong></p> <p>Such studies have shown to be very informative in identifying mineral deposits most suitable for preservation of organic compounds, while highlighting the complementarity of different techniques for biomarkers detection, which is critical for ensuring the success of space missions devoted to the search for signs of life on Mars.</p> <p>We will present a series of laboratory results on molecular degradation caused by UV on Mars and possible application to detection of organics by Martian rovers [3,4,5,6]. In detail, we investigated the photostability of several amino acids like glycine, alanine, methionine, valine, tryptophan, phenylalanine, glutamic acid, prebiotic molecules like urea, deoxyribose and glycolaldehyde, and biomarkers like nucleotides and phytane adsorbed on relevant Martian analogs. We monitored the degradation of these molecule-mineral complexes through in situ spectroscopic analysis, investigating the reflectance properties of the samples in the NIR/MIR spectral region. Such spectroscopic characterization of molecular alteration products provides support for two upcoming robotic missions to Mars that will employ NIR spectroscopy to look for molecular biosignatures, through the instruments SuperCam on board Mars 2020, ISEM, Ma_MISS and MicrOmega on board ExoMars 2022.</p> <p><strong>Acknowledgements</strong></p> <p>This research was supported by the Italian Space Agency (ASI) grant agreement ExoMars n. 2017-48-H.0.</p> <p><strong>References</strong></p> <p>[1] Farley K. A. et al. (2020) Space Sci. Rev. 216, 142.</p> <p>[2] Vago, J. L. et al. (2017) Astrobiology 6, 309–347.</p> <p>[3] Fornaro T. et al. (2013) Icarus 226, 1068–1085.</p> <p>[4] Fornaro T. et al. (2018) Icarus 313, 38-60.</p> <p>[5] Fornaro T. et al. (2020) Front. Astron. Space Sci. 7:539289.</p> <p>[6] Poggiali G. et al. (2020) Front. Astron. Space Sci. 7:18.</p>

In Situ Electrochemical Oxygen Generation with an Immunoisolation Device

1999 ◽  
Vol 875 (1) ◽  
pp. 105-125 ◽  
Author(s):  
HAIYAN WU ◽  
EFSTATHIOS S. AVGOUSTINIATOS ◽  
LARRY SWETTE ◽  
SUSAN BONNER‐WEIR ◽  
GORDON C. WEIR ◽  
...  
Keyword(s):  
Oxygen Generation ◽  
Electrochemical Oxygen
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