1
|
Hart R, Cardace D. Mineral Indicators of Geologically Recent Past Habitability on Mars. Life (Basel) 2023; 13:2349. [PMID: 38137950 PMCID: PMC10744562 DOI: 10.3390/life13122349] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/07/2023] [Revised: 11/25/2023] [Accepted: 12/05/2023] [Indexed: 12/24/2023] Open
Abstract
We provide new support for habitable microenvironments in the near-subsurface of Mars, hosted in Fe- and Mg-rich rock units, and present a list of minerals that can serve as indicators of specific water-rock reactions in recent geologic paleohabitats for follow-on study. We modeled, using a thermodynamic basis without selective phase suppression, the reactions of published Martian meteorites and Jezero Crater igneous rock compositions and reasonable planetary waters (saline, alkaline waters) using Geochemist's Workbench Ver. 12.0. Solid-phase inputs were meteorite compositions for ALH 77005, Nakhla, and Chassigny, and two rock units from the Mars 2020 Perseverance rover sites, Máaz and Séítah. Six plausible Martian groundwater types [NaClO4, Mg(ClO4)2, Ca(ClO4)2, Mg-Na2(ClO4)2, Ca-Na2(ClO4)2, Mg-Ca(ClO4)2] and a unique Mars soil-water analog solution (dilute saline solution) named "Rosy Red", related to the Phoenix Lander mission, were the aqueous-phase inputs. Geophysical conditions were tuned to near-subsurface Mars (100 °C or 373.15 K, associated with residual heat from a magmatic system, impact event, or a concentration of radionuclides, and 101.3 kPa, similar to <10 m depth). Mineral products were dominated by phyllosilicates such as serpentine-group minerals in most reaction paths, but differed in some important indicator minerals. Modeled products varied in physicochemical properties (pH, Eh, conductivity), major ion activities, and related gas fugacities, with different ecological implications. The microbial habitability of pore spaces in subsurface groundwater percolation systems was interrogated at equilibrium in a thermodynamic framework, based on Gibbs Free Energy Minimization. Models run with the Chassigny meteorite produced the overall highest H2 fugacity. Models reliant on the Rosy Red soil-water analog produced the highest sustained CH4 fugacity (maximum values observed for reactant ALH 77005). In general, Chassigny meteorite protoliths produced the best yield regarding Gibbs Free Energy, from an astrobiological perspective. Occurrences of serpentine and saponite across models are key: these minerals have been observed using CRISM spectral data, and their formation via serpentinization would be consistent with geologically recent-past H2 and CH4 production and sustained energy sources for microbial life. We list index minerals to be used as diagnostic for paleo water-rock models that could have supported geologically recent-past microbial activity, and suggest their application as criteria for future astrobiology study-site selections.
Collapse
Affiliation(s)
- Roger Hart
- Department of Physics and Engineering, Community College of Rhode Island, Lincoln, RI 02865, USA
- Department of Geosciences, University of Rhode Island, Kingston, RI 02881, USA;
| | - Dawn Cardace
- Department of Geosciences, University of Rhode Island, Kingston, RI 02881, USA;
| |
Collapse
|
2
|
Heubeck C, Reimann S, Homann M. Stromatolite-like Structures Within Microbially Laminated Sandstones of the Paleoarchean Moodies Group, Barberton Greenstone Belt, South Africa. ASTROBIOLOGY 2023; 23:926-935. [PMID: 37527187 DOI: 10.1089/ast.2023.0014] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 08/03/2023]
Abstract
We report abundant small calcareous mounds associated with fossilized kerogenous microbial mats in tidal-facies sandstones of the predominantly siliciclastic Moodies Group (ca. 3.22 Ga) of the Barberton Greenstone Belt (BGB), South Africa and Eswatini. Most of the bulbous, internally microlaminated mounds are several centimeters in diameter and formed at the sediment-water interface contemporaneously with sedimentation. They originally consisted of Fe-Mg-Mn carbonate, which is now largely silicified; subtle internal compositional laminations are composed of organic matter and sericite. Their presence for >6 km along strike, their restriction to the inferred photic zone, and the internal structure suggest that mineral precipitation was induced by photosynthetic microorganisms. Similar calcareous mounds in this unit also occur within and on top of fluid-escape conduits, suggesting that carbonate precipitation may either have occurred abiogenically or involved chemotrophic metabolism(s) utilizing the oxidation of organic matter, methane, or hydrogen, the latter possibly generated by serpentinization of underlying ultramafic rocks. Alternatively or additionally, carbonate may have precipitated abiotically where heated subsurface fluids, sourced by the intrusion of a major Moodies-age sill, reached the tidal flats. In summary, precipitation mechanisms may have been variable; the calcareous mounds may represent "hybrid carbonates" that may have originated from the small-scale overlap of bioinduced and abiotic processes in space and time. Significantly, the widespread occurrence of these stromatolite-like structures in a fully siliciclastic, high-energy tidal setting broadens search criteria in the search for life on Mars while their possible hybrid origin challenges our ability to unambiguously identify a biogenic component.
Collapse
Affiliation(s)
- C Heubeck
- Department of Geosciences, Friedrich-Schiller-University Jena, Germany
| | - S Reimann
- Department of Geosciences, Friedrich-Schiller-University Jena, Germany
| | - M Homann
- University College London, London, UK
| |
Collapse
|
3
|
Boulesteix D, Buch A, Samson J, Millan M, Jomaa J, Coscia D, Moulay V, McIntosh O, Freissinet C, Stern JC, Szopa C. Influence of pH and salts on DMF-DMA derivatization for future Space Applications. Anal Chim Acta 2023; 1266:341270. [PMID: 37244655 DOI: 10.1016/j.aca.2023.341270] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/30/2023] [Revised: 03/24/2023] [Accepted: 04/23/2023] [Indexed: 05/29/2023]
Abstract
For gas chromatography - mass spectrometry (GC-MS) analyses performed in situ, pH and salts (e.g., chlorides, sulfates) may enhance or inhibit the detection of targeted molecules of interest for astrobiology (e.g. amino acids, fatty acids, nucleobases). Obviously, salts influence the ionic strength of the solutions, the pH value, and the salting effect. But the presence of salts may also produce complexes or mask ions in the sample (masking effect on hydroxide ion, ammonia, etc.). For future space missions, wet chemistry will be conducted before GC-MS analyses to detect the full organic content of a sample. The defined organic targets for space GC-MS instrument requirements are generally strongly polar or refractory organic compounds, such as amino acids playing a role in the protein production and metabolism regulations for life on Earth, nucleobases essential for DNA and RNA formation and mutation, and fatty acids that composed most of the eukaryote and prokaryote membranes on Earth and resist to environmental stress long enough to still be observed on Mars or ocean worlds in geological well-preserved records. The wet-chemistry chemical treatment consists of reacting an organic reagent with the sample to extract and volatilize polar or refractory organic molecules (i.e. dimethylformamide dimethyl acetal (DMF-DMA) in this study). DMF-DMA derivatizes functional groups with labile H in organics, without modifying their chiral conformation. The influence of pH and salt concentration of extraterrestrial materials on the DMF-DMA derivatization remains understudied. In this research, we studied the influence of different salts and pHs on the derivatization of organic molecules of astrobiological interest with DMF-DMA, such as amino acids, carboxylic acids, and nucleobases. Results show that salts and pH influence the derivatization yield, and that their effect depend on the nature of the organics and the salts studied. Second, monovalent salts lead to a higher or similar organic recovery compared to divalent salts regardless of pH below 8. However, a pH above 8 inhibits the DMF-DMA derivatization influencing the carboxylic acid function to become an anionic group without labile H. Overall, considering the negative effect of the salts on the detection of organic molecules, future space missions may have to consider a desalting step prior to derivatization and GC-MS analyses.
Collapse
Affiliation(s)
- D Boulesteix
- Laboratoire Génie des Procédés et Matériaux, CentraleSupélec, University Paris-Saclay, 8-10 Rue Joliot-Curie, 91190, Gif-sur-Yvette, France.
| | - A Buch
- Laboratoire Génie des Procédés et Matériaux, CentraleSupélec, University Paris-Saclay, 8-10 Rue Joliot-Curie, 91190, Gif-sur-Yvette, France.
| | - J Samson
- Laboratoire Génie des Procédés et Matériaux, CentraleSupélec, University Paris-Saclay, 8-10 Rue Joliot-Curie, 91190, Gif-sur-Yvette, France
| | - M Millan
- LATMOS/IPSL, UVSQ University Paris-Saclay, Sorbonne University, CNRS, 11 Bd d'Alembert, 78280, Guyancourt, France
| | - J Jomaa
- Planetary Environments Laboratory (Code 699), NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA; School of Medicine, Wayne State University, 42 W. Warren Ave, Detroit, MI, 48202, USA
| | - D Coscia
- LATMOS/IPSL, UVSQ University Paris-Saclay, Sorbonne University, CNRS, 11 Bd d'Alembert, 78280, Guyancourt, France
| | - V Moulay
- LATMOS/IPSL, UVSQ University Paris-Saclay, Sorbonne University, CNRS, 11 Bd d'Alembert, 78280, Guyancourt, France
| | - O McIntosh
- LATMOS/IPSL, UVSQ University Paris-Saclay, Sorbonne University, CNRS, 11 Bd d'Alembert, 78280, Guyancourt, France
| | - C Freissinet
- LATMOS/IPSL, UVSQ University Paris-Saclay, Sorbonne University, CNRS, 11 Bd d'Alembert, 78280, Guyancourt, France
| | - J C Stern
- Space Science Exploration Division (Code 690), NASA, Goddard Space Flight Center, Greenbelt, MD, 20771, USA
| | - C Szopa
- LATMOS/IPSL, UVSQ University Paris-Saclay, Sorbonne University, CNRS, 11 Bd d'Alembert, 78280, Guyancourt, France
| |
Collapse
|
4
|
Tarasashvili MV, Elbakidze K, Doborjginidze ND, Gharibashvili ND. Carbonate precipitation and nitrogen fixation in AMG (Artificial Martian Ground) by cyanobacteria. LIFE SCIENCES IN SPACE RESEARCH 2023; 37:65-77. [PMID: 37087180 DOI: 10.1016/j.lssr.2023.03.002] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/23/2022] [Revised: 02/22/2023] [Accepted: 03/06/2023] [Indexed: 05/03/2023]
Abstract
This article describes experiments performed to study the survival, growth, specific adaptations and bioremediation potential of certain extreme cyanobacteria strains within a simulation of the atmospheric composition, temperature and pressure expected in a future Martian greenhouse. Initial species have been obtained from Mars-analogue sites in Georgia. The results clearly demonstrate that specific biochemical adaptations allow these autotrophs to metabolize within AMG (Artificial Martian Ground) and accumulate biogenic carbon and nitrogen. These findings may thus contribute to the development of future Martian agriculture, as well as other aspects of the life-support systems at habitable Mars stations. The study shows that carbonate precipitation and nitrogen fixation, performed by cyanobacterial communities thriving within the simulated Martian greenhouse conditions, are cross-linked biological processes. At the same time, the presence of the perchlorates (at low concentrations) in the Martian ground may serve as the initial source of oxygen and, indirectly, hydrogen via photo-Fenton reactions. Various carbonates, ammonium and nitrate salts were obtained as the result of these experiments. These affect the pH, salinity and solubility of the AMG and its components, and so the AMG's scanty biogenic properties improved, which is essential for the sustainable growth of the agricultural crops. Therefore, the use of microorganisms for the biological remediation and continuous in situ fertilization of Artificial Martian Ground is possible.
Collapse
Affiliation(s)
- M V Tarasashvili
- BTU - Business and Technology University, 82 Ilia Chavchavadze Avenue, 0179, Tbilisi, Georgia.
| | - Kh Elbakidze
- BTU - Business and Technology University, 82 Ilia Chavchavadze Avenue, 0179, Tbilisi, Georgia
| | - N D Doborjginidze
- GSRA - Georgian Space Research Agency, 4 Vasil Petriashvili Street, 0179, Tbilisi, Georgia
| | - N D Gharibashvili
- GSRA - Georgian Space Research Agency, 4 Vasil Petriashvili Street, 0179, Tbilisi, Georgia; SpaceFarms Ltd, 14 Kostava Street, 0108, Tbilisi, Georgia
| |
Collapse
|
5
|
Mao W, Fu X, Wu Z, Zhang J, Ling Z, Liu Y, Zhao YYS, Changela HG, Ni Y, Yan F, Zou Y. Solid-gas carbonate formation during dust events on Mars. Natl Sci Rev 2023; 10:nwac293. [PMID: 36960225 PMCID: PMC10029838 DOI: 10.1093/nsr/nwac293] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/27/2022] [Revised: 12/24/2022] [Accepted: 01/04/2023] [Indexed: 01/13/2023] Open
Abstract
Electrostatic discharge experiments under simulated martian atmospheric conditions indicate that atmospheric CO2 has been sequestered into carbonate by the Mars dust activities during the Amazonia era.
Collapse
Affiliation(s)
- Wenshuo Mao
- Shandong Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Institute of Space Sciences, Shandong University, China
| | | | | | - Jiang Zhang
- Shandong Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Institute of Space Sciences, Shandong University, China
| | - Zongcheng Ling
- Shandong Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Institute of Space Sciences, Shandong University, China
- CAS Center for Excellence in Comparative Planetology, China
| | - Yang Liu
- State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, China
| | - Yu-Yan Sara Zhao
- International Center for Planetary Science, College of Earth Science, Chengdu University of Technology, China
- CAS Center for Excellence in Comparative Planetology, China
| | - Hitesh G Changela
- J’Heyrovski Institute of Physical Chemistry, Czech Academy of Sciences, Czech Republic
- Department of Earth & Planetary Science, University of New Mexico, USA
| | - Yuheng Ni
- Shandong Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Institute of Space Sciences, Shandong University, China
| | - Fabao Yan
- School of Mechanical, Electrical & Information Engineering, Shandong University, China
| | - Yongliao Zou
- State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, China
| |
Collapse
|
6
|
Azua-Bustos A, Fairén AG, González-Silva C, Prieto-Ballesteros O, Carrizo D, Sánchez-García L, Parro V, Fernández-Martínez MÁ, Escudero C, Muñoz-Iglesias V, Fernández-Sampedro M, Molina A, Villadangos MG, Moreno-Paz M, Wierzchos J, Ascaso C, Fornaro T, Brucato JR, Poggiali G, Manrique JA, Veneranda M, López-Reyes G, Sanz-Arranz A, Rull F, Ollila AM, Wiens RC, Reyes-Newell A, Clegg SM, Millan M, Johnson SS, McIntosh O, Szopa C, Freissinet C, Sekine Y, Fukushi K, Morida K, Inoue K, Sakuma H, Rampe E. Dark microbiome and extremely low organics in Atacama fossil delta unveil Mars life detection limits. Nat Commun 2023; 14:808. [PMID: 36810853 PMCID: PMC9944251 DOI: 10.1038/s41467-023-36172-1] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/28/2022] [Accepted: 01/17/2023] [Indexed: 02/24/2023] Open
Abstract
Identifying unequivocal signs of life on Mars is one of the most important objectives for sending missions to the red planet. Here we report Red Stone, a 163-100 My alluvial fan-fan delta that formed under arid conditions in the Atacama Desert, rich in hematite and mudstones containing clays such as vermiculite and smectites, and therefore geologically analogous to Mars. We show that Red Stone samples display an important number of microorganisms with an unusual high rate of phylogenetic indeterminacy, what we refer to as "dark microbiome", and a mix of biosignatures from extant and ancient microorganisms that can be barely detected with state-of-the-art laboratory equipment. Our analyses by testbed instruments that are on or will be sent to Mars unveil that although the mineralogy of Red Stone matches that detected by ground-based instruments on the red planet, similarly low levels of organics will be hard, if not impossible to detect in Martian rocks depending on the instrument and technique used. Our results stress the importance in returning samples to Earth for conclusively addressing whether life ever existed on Mars.
Collapse
Affiliation(s)
- Armando Azua-Bustos
- Centro de Astrobiología (CAB) (CSIC-INTA), 28850, Madrid, Spain. .,Instituto de Ciencias Biomédicas, Facultad de Ciencias de la Salud, Universidad Autónoma de Chile, Santiago, Chile.
| | - Alberto G Fairén
- Centro de Astrobiología (CAB) (CSIC-INTA), 28850, Madrid, Spain.,Department of Astronomy, Cornell University, Ithaca, 14853, NY, USA
| | | | | | - Daniel Carrizo
- Centro de Astrobiología (CAB) (CSIC-INTA), 28850, Madrid, Spain
| | | | - Victor Parro
- Centro de Astrobiología (CAB) (CSIC-INTA), 28850, Madrid, Spain
| | | | | | | | | | - Antonio Molina
- Centro de Astrobiología (CAB) (CSIC-INTA), 28850, Madrid, Spain
| | | | | | - Jacek Wierzchos
- Museo Nacional de Ciencias Naturales (CSIC), 28006, Madrid, Spain
| | - Carmen Ascaso
- Museo Nacional de Ciencias Naturales (CSIC), 28006, Madrid, Spain
| | - Teresa Fornaro
- INAF-Astrophysical Observatory of Arcetri, Florence, Italy
| | | | | | - Jose Antonio Manrique
- Universidad de Valladolid, Valladolid, Spain.,Institut de Recherche en Astrophysique et Planétologie (IRAP), Toulouse, France
| | | | | | | | | | - Ann M Ollila
- Purdue University, Earth, Atmospheric, and Planetary Sciences, West Lafayette, USA
| | - Roger C Wiens
- Purdue University, Earth, Atmospheric, and Planetary Sciences, West Lafayette, USA
| | | | - Samuel M Clegg
- Purdue University, Earth, Atmospheric, and Planetary Sciences, West Lafayette, USA
| | - Maëva Millan
- Department of Biology, Georgetown University, Washington, DC, 20057, USA.,NASA Goddard Space Flight Center, Solar System Exploration Division, Greenbelt, MD, 20771, USA.,LATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, CNRS, 11 Bd d'Alembert, 78280, Guyancourt, France
| | - Sarah Stewart Johnson
- Department of Biology, Georgetown University, Washington, DC, 20057, USA.,Science, Technology, and International Affairs Program, Georgetown University, Washington, DC, 20057, USA
| | - Ophélie McIntosh
- INAF-Astrophysical Observatory of Arcetri, Florence, Italy.,Science, Technology, and International Affairs Program, Georgetown University, Washington, DC, 20057, USA
| | - Cyril Szopa
- Science, Technology, and International Affairs Program, Georgetown University, Washington, DC, 20057, USA
| | - Caroline Freissinet
- Science, Technology, and International Affairs Program, Georgetown University, Washington, DC, 20057, USA
| | - Yasuhito Sekine
- Earth-Life Science Institute (ELSI), Tokyo Institute of Technology, Tokyo, Japan.,Institute of Nature and Environmental Technology, Kanazawa University, Kanazawa, Japan
| | - Keisuke Fukushi
- Institute of Nature and Environmental Technology, Kanazawa University, Kanazawa, Japan
| | - Koki Morida
- Division of Natural System, Kanazawa University, Kanazawa, Japan
| | - Kosuke Inoue
- Division of Natural System, Kanazawa University, Kanazawa, Japan
| | - Hiroshi Sakuma
- National Institute for Materials Science, Tsukuba, Japan
| | - Elizabeth Rampe
- Astromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX, USA
| |
Collapse
|
7
|
Liu W, Wu Z, Chen W, Jin G, Zhang W, Lv X, Yu P, Zhao H. A potential application for life-related organics detection on Mars by diffuse reflectance infrared spectroscopy. Heliyon 2023; 9:e13560. [PMID: 36846659 PMCID: PMC9946848 DOI: 10.1016/j.heliyon.2023.e13560] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/03/2022] [Revised: 02/01/2023] [Accepted: 02/02/2023] [Indexed: 02/11/2023] Open
Abstract
Life information searching is a hot point for Mars exploration. Ancient Mars was very likely to reach a habitable environment, and there was a real possibility of arising life on Mars. However, the current Mars has a harsh environment. Under such conditions, life materials on Mars are supposed to have taken the form of relatively primitive microbial or organic residues, which might be preserved in some mineral matrices. Detection of these remnants is of great significance for understanding the origin and evolution of life on Mars. The best detection method is in-situ detection or sample return. Herein, diffuse reflectance infrared spectroscopy (DRIFTS) was used to detect characteristic spectra and the limit of detection (LOD) of potential representative organic compounds with associated minerals. In view of high oxidation due to the electrostatic discharge (ESD) during dust actives on Martian surface. The degradation of organic matter by ESD process was studied under simulated Mars conditions. Our results show that the spectral characteristics of organic matter are significantly different from that of associated minerals. The different organic samples have different mass loss and color change after ESD reaction. And the signal intensity of infrared diffuse reflection spectrum can also reflect the changes of organic molecules after ESD reaction. Our results indicated that the degradation products of organics rather than organic itself are most likely to be founded on current Martian surface.
Collapse
Affiliation(s)
- Wang Liu
- School of Space Science and Physics, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China,Research Center for Biological Adaptability in Space Environment, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China
| | - Zhongchen Wu
- School of Space Science and Physics, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China,Research Center for Biological Adaptability in Space Environment, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China,Corresponding author. School of Space Science and Physics, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China.
| | - Wenxi Chen
- School of Space Science and Physics, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China,Research Center for Biological Adaptability in Space Environment, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China
| | - Guobin Jin
- School of Space Science and Physics, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China,Research Center for Biological Adaptability in Space Environment, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China
| | - Wei Zhang
- Marine College, Shandong University, Weihai, Shandong, 264209, China,Research Center for Biological Adaptability in Space Environment, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China
| | - Xinfang Lv
- Marine College, Shandong University, Weihai, Shandong, 264209, China,Research Center for Biological Adaptability in Space Environment, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China
| | - Pei Yu
- SDU-ANU Joint Science College, Shandong University, Weihai, Shandong, 264209, China,Research Center for Biological Adaptability in Space Environment, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China
| | - Hong Zhao
- Marine College, Shandong University, Weihai, Shandong, 264209, China,Research Center for Biological Adaptability in Space Environment, Institute of Space Sciences, Shandong University, Weihai, Shandong, 264209, China
| |
Collapse
|
8
|
Understanding redox processes during iron precipitation in standing water: implications in formation of iron oxides minerals in the terrestrial planetary environment (especially Mars). PROCEEDINGS OF THE INDIAN NATIONAL SCIENCE ACADEMY 2022. [DOI: 10.1007/s43538-022-00092-3] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/15/2022]
|
9
|
Seaton KM, Cable ML, Stockton AM. Analytical Chemistry Throughout This Solar System. ANNUAL REVIEW OF ANALYTICAL CHEMISTRY (PALO ALTO, CALIF.) 2022; 15:197-219. [PMID: 35300527 DOI: 10.1146/annurev-anchem-061020-125416] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/14/2023]
Abstract
One of the greatest and most long-lived scientific pursuits of humankind has been to discover and study the planetary objects comprising our solar system. Information gained from solar system observations, via both remote sensing and in situ measurements, is inherently constrained by the analytical (often chemical) techniques we employ in these endeavors. The past 50 years of planetary science missions have resulted in immense discoveries within and beyond our solar system, enabled by state-of-the-art analytical chemical instrument suites on board these missions. In this review, we highlight and discuss some of the most impactful analytical chemical instruments flown on planetary science missions within the last 20 years, including analytical techniques ranging from remote spectroscopy to in situ chemical separations. We first highlight mission-based remote and in situ spectroscopic techniques, followed by in situ separation and mass spectrometry analyses. The results of these investigations are discussed, and their implications examined, from worlds as close as Venus and familiar as Mars to as far away and exotic as Titan. Instruments currently in development for planetary science missions in the near future are also discussed, as are the promises their capabilities bring. Analytical chemistry is critical to understanding what lies beyond Earth in our solar system, and this review seeks to highlight how questions, analytical tools, and answers have intersected over the past 20 years and their implications for the near future.
Collapse
Affiliation(s)
- Kenneth Marshall Seaton
- School of Chemistry and Biochemistry, Georgia Institute of Technology, Atlanta, Georgia, USA;
| | - Morgan Leigh Cable
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
| | | |
Collapse
|
10
|
Abstract
In this work, we study the kinetics of thermal decomposition of MgCO3 in the form of particles of known size. In the experiments, the material is heated to a known temperature in a vacuum oven, and it is characterized, both before and after heating, by infrared spectroscopy and gravimetry. The agreement between the results of the two techniques is excellent. These results are rationalized by means of a model based on Languir’s law, and the comparison with the experiments allows us to estimate the activation energy of the process. The reabsorption of atmospheric water by the oxide is shown spectroscopically, finding that is strongly influenced by the temperature of the process.
Collapse
|
11
|
Royle SH, Salter TL, Watson JS, Sephton MA. Mineral Matrix Effects on Pyrolysis Products of Kerogens Infer Difficulties in Determining Biological Provenance of Macromolecular Organic Matter at Mars. ASTROBIOLOGY 2022; 22:520-540. [PMID: 35171040 DOI: 10.1089/ast.2021.0074] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/14/2023]
Abstract
Ancient martian organic matter is likely to take the form of kerogen-like recalcitrant macromolecular organic matter (MOM), existing in close association with reactive mineral surfaces, especially iron oxides. Detecting and identifying a biological origin for martian MOM will therefore be of utmost importance for life-detection efforts at Mars. We show that Type I and Type IV kerogens provide effective analogues for putative martian MOM of biological and abiological (meteoric) provenances, respectively. We analyze the pyrolytic breakdown products when these kerogens are mixed with mineral matrices highly relevant for the search for life on Mars. We demonstrate that, using traditional thermal techniques as generally used by the Sample Analysis at Mars and Mars Organic Molecule Analyser instruments, even the breakdown products of highly recalcitrant MOM are transformed during analysis in the presence of reactive mineral surfaces, particularly iron. Analytical transformation reduces the diagnostic ability of this technique, as detected transformation products of both biological and abiological MOM may be identical (low molecular weight gas phases and benzene) and indistinguishable. The severity of transformational effects increased through calcite < kaolinite < hematite < nontronite < magnetite < goethite. Due to their representation of various habitable aqueous environments and the preservation potential of organic matter by iron, it is not advisable to completely avoid iron-rich strata. We conclude that hematite-rich localities, with evidence of extensive aqueous alteration of originally reducing phases, such as the Vera Rubin Ridge, may be relatively promising targets for identifying martian biologically sourced MOM.
Collapse
Affiliation(s)
- Samuel H Royle
- Department of Earth Science and Engineering, Imperial College London, London, UK
| | - Tara L Salter
- Department of Earth Science and Engineering, Imperial College London, London, UK
| | - Jonathan S Watson
- Department of Earth Science and Engineering, Imperial College London, London, UK
| | - Mark A Sephton
- Department of Earth Science and Engineering, Imperial College London, London, UK
| |
Collapse
|
12
|
Alvarez-Llamas C, Purohit P, Moros J, Laserna J. LIBS-Acoustic Mid-Level Fusion Scheme for Mineral Differentiation under Terrestrial and Martian Atmospheric Conditions. Anal Chem 2022; 94:1840-1849. [PMID: 35019262 PMCID: PMC8893358 DOI: 10.1021/acs.analchem.1c04792] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/28/2022]
Abstract
![]()
The shockwave produced alongside
the plasma during a laser-induced
breakdown spectroscopy event can be recorded as an acoustic pressure
wave to obtain information related to the physical traits of the inspected
sample. In the present work, a mid-level fusion approach is developed
using simultaneously recorded laser-induced breakdown spectroscopy
(LIBS) and acoustic data to enhance the discrimination capabilities
of different iron-based and calcium-based mineral phases, which exhibit
nearly identical spectral features. To do so, the mid-level data fusion
approach is applied concatenating the principal components analysis
(PCA)-LIBS score values with the acoustic wave peak-to-peak amplitude
and with the intraposition signal change, represented as the slope
of the acoustic signal amplitude with respect to the laser shot. The
discrimination hit rate of the mineral phases is obtained using linear
discriminant analysis. Owing to the increasing interest for in situ
applications of LIBS + acoustics information, samples are inspected
in a remote experimental configuration and under two different atmospheric
traits, Earth and Mars-like conditions, to validate the approach.
Particularities conditioning the response of both strategies under
each atmosphere are discussed to provide insight to better exploit
the complex phenomena resulting in the collected signals. Results
reported herein demonstrate for the first time that the characteristic
sample input in the laser-produced acoustic wave can be used for the
creation of a statistical descriptor to synergistically improve the
capabilities of LIBS of differentiation of rocks.
Collapse
Affiliation(s)
- César Alvarez-Llamas
- UMALASERLAB, Departamento de Química Analítica, Universidad de Málaga, C/Jiménez Fraud 4, Málaga 29010, Spain
| | - Pablo Purohit
- UMALASERLAB, Departamento de Química Analítica, Universidad de Málaga, C/Jiménez Fraud 4, Málaga 29010, Spain
| | - Javier Moros
- UMALASERLAB, Departamento de Química Analítica, Universidad de Málaga, C/Jiménez Fraud 4, Málaga 29010, Spain
| | - Javier Laserna
- UMALASERLAB, Departamento de Química Analítica, Universidad de Málaga, C/Jiménez Fraud 4, Málaga 29010, Spain
| |
Collapse
|
13
|
Zhao JJ, Zhang YF, Zhao TL, Li H, Yao QZ, Fu SQ, Zhou GT. Abiotic Formation of Calcium Oxalate under UV Irradiation and Implications for Biomarker Detection on Mars. ASTROBIOLOGY 2022; 22:35-48. [PMID: 35020413 DOI: 10.1089/ast.2020.2416] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/14/2023]
Abstract
A major objective in the exploration of Mars is to test the hypothesis that the planet has ever hosted life. Biogenic compounds, especially biominerals, are believed to serve as biomarkers in Raman-assisted remote sensing missions. However, the prerequisite for the development of these minerals as biomarkers is the uniqueness of their biogenesis. Herein, tetragonal bipyramidal weddellite, a type of calcium oxalate, is successfully achieved by UV-photolyzing pyruvic acid (PA). The as-prepared products are identified and characterized by micro-Raman spectroscopy and field emission scanning electron microscopy. Persistent mineralization of weddellite is observed with altering key experimental parameters, including pH, Ca2+ and PA concentrations. In particular, the initial concentration of PA can significantly influence the morphology of weddellite crystal. Oxalate acid is commonly of biological origin; thus calcium oxalate is considered to be a biomarker. However, our results reveal that calcium oxalate can be harvested by a UV photolysis pathway. Moreover, prebiotic sources of organics (e.g., PA, glycine, alanine, and aspartic acid) have been proven to be available through abiotic pathways. Therefore, our results may provide a new abiotic pathway of calcium oxalate formation. Considering that calcium oxalate minerals have been taken as biosignatures for the origin and early evolution of life on Earth and astrobiological investigations, its formation and accumulation by the photolysis of abiological organic compounds should be taken into account.
Collapse
Affiliation(s)
- Jia-Jian Zhao
- CAS Key Laboratory of Crust-Mantle Materials and Environments, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, P.R. China
| | - Yi-Fan Zhang
- CAS Key Laboratory of Crust-Mantle Materials and Environments, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, P.R. China
| | - Tian-Lei Zhao
- CAS Key Laboratory of Crust-Mantle Materials and Environments, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, P.R. China
| | - Han Li
- CAS Key Laboratory of Crust-Mantle Materials and Environments, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, P.R. China
| | - Qi-Zhi Yao
- School of Chemistry and Materials Science, University of Science and Technology of China, Hefei, P.R. China
| | - Sheng-Quan Fu
- Hefei National Laboratory for Physical Sciences at Microscale, University of Science and Technology of China, Hefei, P.R. China
| | - Gen-Tao Zhou
- CAS Key Laboratory of Crust-Mantle Materials and Environments, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, P.R. China
- CAS Center for Excellence in Comparative Planetology, University of Science and Technology of China, Hefei, P.R. China
| |
Collapse
|
14
|
Tarnas JD, Stack KM, Parente M, Koeppel AHD, Mustard JF, Moore KR, Horgan BHN, Seelos FP, Cloutis EA, Kelemen PB, Flannery D, Brown AJ, Frizzell KR, Pinet P. Characteristics, Origins, and Biosignature Preservation Potential of Carbonate-Bearing Rocks Within and Outside of Jezero Crater. JOURNAL OF GEOPHYSICAL RESEARCH. PLANETS 2021; 126:e2021JE006898. [PMID: 34824965 PMCID: PMC8597593 DOI: 10.1029/2021je006898] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/19/2021] [Revised: 09/24/2021] [Accepted: 09/24/2021] [Indexed: 05/20/2023]
Abstract
Carbonate minerals have been detected in Jezero crater, an ancient lake basin that is the landing site of the Mars 2020 Perseverance rover, and within the regional olivine-bearing (ROB) unit in the Nili Fossae region surrounding this crater. It has been suggested that some carbonates in the margin fractured unit, a rock unit within Jezero crater, formed in a fluviolacustrine environment, which would be conducive to preservation of biosignatures from paleolake-inhabiting lifeforms. Here, we show that carbonate-bearing rocks within and outside of Jezero crater have the same range of visible-to-near-infrared carbonate absorption strengths, carbonate absorption band positions, thermal inertias, and morphologies. Thicknesses of exposed carbonate-bearing rock cross-sections in Jezero crater are ∼75-90 m thicker than typical ROB unit cross-sections in the Nili Fossae region, but have similar thicknesses to ROB unit exposures in Libya Montes. These similarities in carbonate properties within and outside of Jezero crater is consistent with a shared origin for all of the carbonates in the Nili Fossae region. Carbonate absorption minima positions indicate that both Mg- and more Fe-rich carbonates are present in the Nili Fossae region, consistent with the expected products of olivine carbonation. These estimated carbonate chemistries are similar to those in martian meteorites and the Comanche carbonates investigated by the Spirit rover in Columbia Hills. Our results indicate that hydrothermal alteration is the most likely formation mechanism for non-deltaic carbonates within and outside of Jezero crater.
Collapse
Affiliation(s)
- J. D. Tarnas
- NASA Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadenaCAUSA
| | - K. M. Stack
- NASA Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadenaCAUSA
| | - M. Parente
- Department of Electrical and Computer EngineeringUniversity of Massachusetts at AmherstAmherstMAUSA
| | - A. H. D. Koeppel
- Department of Astronomy and Planetary ScienceNorthern Arizona UniversityFlagstaffAZUSA
| | - J. F. Mustard
- Department of Earth, Environmental and Planetary SciencesBrown UniversityProvidenceRIUSA
| | - K. R. Moore
- NASA Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadenaCAUSA
| | - B. H. N. Horgan
- Department of Earth, Atmospheric, and Planetary SciencesPurdue UniversityWest LafayetteINUSA
| | - F. P. Seelos
- Johns Hopkins University Applied Physics LabLaurelMDUSA
| | - E. A. Cloutis
- Department of GeographyUniversity of WinnipegWinnipegMBCanada
| | - P. B. Kelemen
- Lahmont‐Doherty Earth Observatory, Columbia UniversityPalisadesNYUSA
| | - D. Flannery
- School of Earth and Atmospheric SciencesQueensland University of TechnologyBrisbaneQLDAustralia
| | | | - K. R. Frizzell
- Department of Earth and Planetary SciencesRutgers UniversityPiscatawayNJUSA
| | - P. Pinet
- Institut de Recherche en Astrophysique et PlanétologieToulouseFrance
| |
Collapse
|
15
|
Yang L, Zhang C, Yu X, Yao Y, Li Z, Wu C, Yao W, Zou Z. Extraterrestrial artificial photosynthetic materials for in-situ resource utilization. Natl Sci Rev 2021; 8:nwab104. [PMID: 34691720 PMCID: PMC8363334 DOI: 10.1093/nsr/nwab104] [Citation(s) in RCA: 10] [Impact Index Per Article: 3.3] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/31/2020] [Revised: 05/28/2021] [Accepted: 06/10/2021] [Indexed: 02/06/2023] Open
Abstract
Aerospace milestones in human history, including returning to the moon and manned Martian missions, have been implemented in recent years. Space exploration has become one of the global common goals, and to ensure the survival and development of human beings in the extraterrestrial extreme environment has been becoming the basic ability and technology of manned space exploration. For the purpose of fulfilling the goal of extraterrestrial survival, researchers in Nanjing University and the China Academy of Space Technology proposed extraterrestrial artificial photosynthesis (EAP) technology. By simulating the natural photosynthesis of green plants on the Earth, EAP converts CO2/H2O into fuel and O2 in an in-situ, accelerated and controllable manner by using waste CO2 in the confined space of spacecraft, or abundant CO2 resources in extraterrestrial celestial environments, e.g. Mars. Thus, the material loading of manned spacecraft can be greatly reduced to support affordable and sustainable deep space exploration. In this paper, EAP technology is compared with existing methods of converting CO2/H2O into fuel and O2 in the aerospace field, especially the Sabatier method and Bosch reduction method. The research progress of possible EAP materials for in-situ utilization of extraterrestrial resources are also discussed in depth. Finally, this review lists the challenges that the EAP process may encounter, which need to be focused on for future implementation and application. We expect to deepen the understanding of artificial photosynthetic materials and technologies, and aim to strongly support the development of manned spaceflight.
Collapse
Affiliation(s)
- Liuqing Yang
- Eco-Materials and Renewable Energy Research Center (ERERC), Jiangsu Key Laboratory for Nano Technology, National Laboratory of Solid State Microstructures, School of Physics, Nanjing University, Nanjing 210093, China
| | - Ce Zhang
- Qian Xuesen Laboratory of Space Technology, China Academy of Space Technology, Beijing 100094, China
| | - Xiwen Yu
- Eco-Materials and Renewable Energy Research Center (ERERC), Jiangsu Key Laboratory for Nano Technology, National Laboratory of Solid State Microstructures, School of Physics, Nanjing University, Nanjing 210093, China
- Collaborative Innovation Center of Advanced Microstructures, College of Engineering and Applied Sciences, Nanjing University, Nanjing 210093, China
| | - Yingfang Yao
- Eco-Materials and Renewable Energy Research Center (ERERC), Jiangsu Key Laboratory for Nano Technology, National Laboratory of Solid State Microstructures, School of Physics, Nanjing University, Nanjing 210093, China
- Collaborative Innovation Center of Advanced Microstructures, College of Engineering and Applied Sciences, Nanjing University, Nanjing 210093, China
- KunshanInnovation Institute of Nanjing University, Suzhou 215347, China
- School of Science and Engineering, The Chinese University of Hong Kong, Shenzhen 518172, China
- Wuhan National Laboratory for Optoelectronics, Huazhong University of Science and Technology, Wuhan 430074, China
| | - Zhaosheng Li
- Eco-Materials and Renewable Energy Research Center (ERERC), Jiangsu Key Laboratory for Nano Technology, National Laboratory of Solid State Microstructures, School of Physics, Nanjing University, Nanjing 210093, China
- Collaborative Innovation Center of Advanced Microstructures, College of Engineering and Applied Sciences, Nanjing University, Nanjing 210093, China
| | - Congping Wu
- Eco-Materials and Renewable Energy Research Center (ERERC), Jiangsu Key Laboratory for Nano Technology, National Laboratory of Solid State Microstructures, School of Physics, Nanjing University, Nanjing 210093, China
- KunshanInnovation Institute of Nanjing University, Suzhou 215347, China
| | - Wei Yao
- Qian Xuesen Laboratory of Space Technology, China Academy of Space Technology, Beijing 100094, China
| | - Zhigang Zou
- Eco-Materials and Renewable Energy Research Center (ERERC), Jiangsu Key Laboratory for Nano Technology, National Laboratory of Solid State Microstructures, School of Physics, Nanjing University, Nanjing 210093, China
- Qian Xuesen Laboratory of Space Technology, China Academy of Space Technology, Beijing 100094, China
- Collaborative Innovation Center of Advanced Microstructures, College of Engineering and Applied Sciences, Nanjing University, Nanjing 210093, China
- School of Science and Engineering, The Chinese University of Hong Kong, Shenzhen 518172, China
- Macau Institute of Systems Engineering, Macau University of Science and Technology, Macau 999078, China
| |
Collapse
|
16
|
Scheller EL, Swindle C, Grotzinger J, Barnhart H, Bhattacharjee S, Ehlmann BL, Farley K, Fischer WW, Greenberger R, Ingalls M, Martin PE, Osorio-Rodriguez D, Smith BP. Formation of Magnesium Carbonates on Earth and Implications for Mars. JOURNAL OF GEOPHYSICAL RESEARCH. PLANETS 2021; 126:e2021JE006828. [PMID: 34422534 PMCID: PMC8378241 DOI: 10.1029/2021je006828] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/25/2021] [Accepted: 05/29/2021] [Indexed: 05/20/2023]
Abstract
Magnesium carbonates have been identified within the landing site of the Perseverance rover mission. This study reviews terrestrial analog environments and textural, mineral assemblage, isotopic, and elemental analyses that have been applied to establish formation conditions of magnesium carbonates. Magnesium carbonates form in five distinct settings: ultramafic rock-hosted veins, the matrix of carbonated peridotite, nodules in soil, alkaline lake, and playa deposits, and as diagenetic replacements within lime-and dolostones. Dominant textures include fine-grained or microcrystalline veins, nodules, and crusts. Microbial influences on formation are recorded in thrombolites, stromatolites, crinkly, and pustular laminites, spheroids, and filamentous microstructures. Mineral assemblages, fluid inclusions, and carbon, oxygen, magnesium, and clumped isotopes of carbon and oxygen have been used to determine the sources of carbon, magnesium, and fluid for magnesium carbonates as well as their temperatures of formation. Isotopic signatures in ultramafic rock-hosted magnesium carbonates reveal that they form by either low-temperature meteoric water infiltration and alteration, hydrothermal alteration, or metamorphic processes. Isotopic compositions of lacustrine magnesium carbonate record precipitation from lake water, evaporation processes, and ambient formation temperatures. Assessment of these features with similar analytical techniques applied to returned Martian samples can establish whether carbonates on ancient Mars were formed at high or low temperature conditions in the surface or subsurface through abiotic or biotic processes. The timing of carbonate formation processes could be constrained by 147Sm-143Nd isochron, U-Pb concordia, 207Pb-206Pb isochron radiometric dating as well as 3He, 21Ne, 22Ne, or 36Ar surface exposure dating of returned Martian magnesium carbonate samples.
Collapse
Affiliation(s)
- Eva L Scheller
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Carl Swindle
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - John Grotzinger
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Holly Barnhart
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Surjyendu Bhattacharjee
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Bethany L Ehlmann
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - Ken Farley
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Woodward W Fischer
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Rebecca Greenberger
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Miquela Ingalls
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
- Department of Geosciences, Pennsylvania State University, State College, PA, USA
| | - Peter E Martin
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
- Geological Sciences Department, University of Colorado Boulder, Boulder, CO, USA
| | - Daniela Osorio-Rodriguez
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Ben P Smith
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| |
Collapse
|
17
|
Seaton KM, Cable ML, Stockton AM. Analytical Chemistry in Astrobiology. Anal Chem 2021; 93:5981-5997. [PMID: 33835785 DOI: 10.1021/acs.analchem.0c04271] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/28/2022]
Abstract
This Feature introduces and discusses the findings of key analytical techniques used to study planetary bodies in our solar system in the search for life beyond Earth, future missions planned for high-priority astrobiology targets in our solar system, and the challenges we face in performing these investigations.
Collapse
Affiliation(s)
- Kenneth Marshall Seaton
- School of Chemistry & Biochemistry, Georgia Institute of Technology, North Avenue NW, Atlanta, Georgia 30332, United States
| | - Morgan Leigh Cable
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, United States
| | - Amanda Michelle Stockton
- School of Chemistry & Biochemistry, Georgia Institute of Technology, North Avenue NW, Atlanta, Georgia 30332, United States
| |
Collapse
|
18
|
Rojas Vivas JA, Navarro-González R, de la Rosa J, Molina P, Sedov S, McKay CP. Radiolytic Degradation of Soil Carbon from the Mojave Desert by 60Co Gamma Rays: Implications for the Survival of Martian Organic Compounds Due to Cosmic Radiation. ASTROBIOLOGY 2021; 21:381-393. [PMID: 33351679 DOI: 10.1089/ast.2020.2257] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/12/2023]
Abstract
The martian surface has been continuously exposed to galactic cosmic radiation. Since organic compounds are degraded by ionizing radiation, knowledge of their decay constants is fundamental to predicting their stability on the martian surface. In this study, we report the radiolysis constant for the destruction of soil organic compounds at a starting concentration of ∼2011 μg C/gsoil from the Mojave Desert. The soils were exposed to gamma irradiation with absorbed doses of up to 19 MGy at room temperature, representing ∼250 million years of exposure to galactic cosmic rays. The destruction of total soil organic carbon and the formation of gases were investigated by a sequential on-line analytical array coupled to gas chromatography-mass spectrometry. Soil inorganic and organic carbon were degraded exponentially with a radiolysis constant 0.3 MGy-1(30%) producing mostly carbon dioxide (93.2%), carbon monoxide (6.2%), and methane (0.6%). Using the dose rate measured by the Radiation Assessment Detector on board the Curiosity rover, we make predictions on the survival of organic compounds in the cold martian subsurface. It is estimated that soil organic compounds with initial concentrations as those found today at the Mojave Desert would have been destroyed to levels <1 ppb at 0.1 m in depth in ∼2000 Myr. Pristine organic compounds are expected to be present at a depth of ∼1.5 m. These results are relevant for the search of organic compounds in past, present, and future missions to Mars. In particular, we predict that the upcoming ExoMars will encounter pristine organic compounds at this depth.
Collapse
Affiliation(s)
- José Alfredo Rojas Vivas
- Posgrado en Ciencias de la Tierra, Universidad Nacional Autónoma de México, Circuito de la investigación S/N, Ciudad Universitaria, Ciudad de México, Mexico
- Laboratorio de Química de Plasmas y Estudios Planetarios, Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Circuito Exterior S/N, Ciudad Universitaria, Ciudad de México, Mexico
| | - Rafael Navarro-González
- Laboratorio de Química de Plasmas y Estudios Planetarios, Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Circuito Exterior S/N, Ciudad Universitaria, Ciudad de México, Mexico
| | - José de la Rosa
- Laboratorio de Química de Plasmas y Estudios Planetarios, Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Circuito Exterior S/N, Ciudad Universitaria, Ciudad de México, Mexico
| | - Paola Molina
- Laboratorio de Química de Plasmas y Estudios Planetarios, Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Circuito Exterior S/N, Ciudad Universitaria, Ciudad de México, Mexico
| | - Sergey Sedov
- Departamento de Ciencias Ambientales y del Suelo, Instituto de Geología, Universidad Nacional Autónoma de México, Circuito de la investigación S/N, Ciudad Universitaria, Ciudad de México, Mexico
| | | |
Collapse
|
19
|
Hydrogeochemical Study on Closed-Basin Lakes in Cold and Semi-Arid Climates of the Valley of the Gobi Lakes, Mongolia: Implications for Hydrology and Water Chemistry of Paleolakes on Mars. MINERALS 2020. [DOI: 10.3390/min10090792] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 12/23/2022]
Abstract
Previous studies suggested that, generally, the climate of early Mars would have been semi-arid when the surface temperatures were above freezing. On early Mars, closed-basin lakes would have been created; however, the hydrogeochemical cycles of the lake systems are poorly constrained. Here we report results of our field surveys to terrestrial analogs of closed-basin lake systems that developed in cold and semi-arid climates: The Valley of the Gobi Lakes of Mongolia. Our results show that groundwater plays a central role not only in hydrology, but also in geochemical cycles in the lake systems. We find that groundwater predominantly flows into the lakes through local seepage and regional flows in semi-arid climates. Through the interactions with calcite-containing soils, local groundwater seepage provides Ca2+ and HCO3− to the lakes. In the wetland located in between the lakes, high-salinity shallow pools would provide Cl− and Na+ to the groundwater through infiltration. If similar processes occurred on early Mars, local seepage of groundwater would have provided magnesium and alkalinity to the early Jezero lakes, possibly leading to authigenic precipitation of lacustrine carbonates. On early Mars, infiltration of surface brine may have transported salts and oxidants on the surface to lakes via regional groundwater flows. We suggest that inflows of multiple types of groundwater in semi-arid climates could have caused redox disequilibria in closed-basin lakes on early Mars.
Collapse
|
20
|
Vimercati L, Bueno de Mesquita CP, Schmidt SK. Limited Response of Indigenous Microbes to Water and Nutrient Pulses in High-Elevation Atacama Soils: Implications for the Cold-Dry Limits of Life on Earth. Microorganisms 2020; 8:E1061. [PMID: 32708721 PMCID: PMC7409055 DOI: 10.3390/microorganisms8071061] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/02/2020] [Revised: 07/07/2020] [Accepted: 07/09/2020] [Indexed: 01/05/2023] Open
Abstract
Soils on the world's highest volcanoes in the Atacama region represent some of the harshest ecosystems yet discovered on Earth. Life in these environments must cope with high UV flux, extreme diurnal freeze-thaw cycles, low atmospheric pressure and extremely low nutrient and water availability. Only a limited spectrum of bacterial and fungal lineages seems to have overcome the harshness of this environment and may have evolved the ability to function in situ. However, these communities may lay dormant for most of the time and spring to life only when enough water and nutrients become available during occasional snowfalls and aeolian depositions. We applied water and nutrients to high-elevation soils (5100 meters above sea level) from Volcán Llullaillaco, both in lab microcosms and in the field, to investigate how microbial communities respond when resource limitations are alleviated. The dominant taxon in these soils, the extremophilic yeast Naganishia sp., increased in relative sequence abundance and colony-forming unit counts after water + nutrient additions in microcosms, and marginally in the field after only 6 days. Among bacteria, only a Noviherbaspirillum sp. (Oxalobacteraceae) significantly increased in relative abundance both in the lab and field in response to water addition but not in response to water and nutrients together, indicating that it might be an oligotroph uniquely suited to this extreme environment. The community structure of both bacteria and eukaryotes changed significantly with water and water + nutrient additions in the microcosms and taxonomic richness declined with amendments to water and nutrients. These results indicate that only a fraction of the detected community is able to become active when water and nutrients limitations are alleviated in lab microcosms, and that water alone can dramatically change community structure. Our study sheds light on which extremophilic organisms are likely to respond when favorable conditions occur in extreme earthly environments and perhaps in extraterrestrial environments as well.
Collapse
Affiliation(s)
- Lara Vimercati
- Department of Ecology and Evolutionary Biology, University of Colorado, Boulder, CO 80309-0334, USA; (L.V.); (C.P.B.d.M.)
| | - Clifton P. Bueno de Mesquita
- Department of Ecology and Evolutionary Biology, University of Colorado, Boulder, CO 80309-0334, USA; (L.V.); (C.P.B.d.M.)
- Institute of Arctic and Alpine Research, University of Colorado, Boulder, CO 80309-0450, USA
| | - Steven K. Schmidt
- Department of Ecology and Evolutionary Biology, University of Colorado, Boulder, CO 80309-0334, USA; (L.V.); (C.P.B.d.M.)
| |
Collapse
|
21
|
Abstract
To assess Mars’ potential for both harboring life and providing useable resources for future human exploration, it is of paramount importance to comprehend the water situation on the planet. Therefore, studies have been conducted to determine any evidence of past or present water existence on Mars. While the presence of abundant water on Mars very early in its history is widely accepted, on its modern form, only a fraction of this water can be found, as either ice or locked into the structure of Mars’ plentiful water-rich materials. Water on the planet is evaluated through various evidence such as rocks and minerals, Martian achondrites, low volume transient briny outflows (e.g., dune flows, reactivated gullies, slope streaks, etc.), diurnal shallow soil moisture (e.g., measurements by Curiosity and Phoenix Lander), geomorphic representation (possibly from lakes and river valleys), and groundwater, along with further evidence obtained by probe and rover discoveries. One of the most significant lines of evidence is for an ancient streambed in Gale Crater, implying ancient amounts of “vigorous” water on Mars. Long ago, hospitable conditions for microbial life existed on the surface of Mars, as it was likely periodically wet. However, its current dry surface makes it almost impossible as an appropriate environment for living organisms; therefore, scientists have recognized the planet’s subsurface environments as the best potential locations for exploring life on Mars. As a result, modern research has aimed towards discovering underground water, leading to the discovery of a large amount of underground ice in 2016 by NASA, and a subglacial lake in 2018 by Italian scientists. Nevertheless, the presence of life in Mars’ history is still an open question. In this unifying context, the current review summarizes results from a wide variety of studies and reports related to the history of water on Mars, as well as any related discussions on the possibility of living organism existence on the planet.
Collapse
|
22
|
The role of primordial atmosphere composition in organic matter delivery to early Earth. RENDICONTI LINCEI. SCIENZE FISICHE E NATURALI 2020. [DOI: 10.1007/s12210-020-00878-x] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 10/25/2022]
|
23
|
Shao Y, Ying Y, Ping J. Recent advances in solid-contact ion-selective electrodes: functional materials, transduction mechanisms, and development trends. Chem Soc Rev 2020; 49:4405-4465. [DOI: 10.1039/c9cs00587k] [Citation(s) in RCA: 143] [Impact Index Per Article: 35.8] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/13/2022]
Abstract
This article presents a comprehensive overview of recent progress in the design and applications of solid-contact ion-selective electrodes (SC-ISEs).
Collapse
Affiliation(s)
- Yuzhou Shao
- Laboratory of Agricultural Information Intelligent Sensing
- School of Biosystems Engineering and Food Science
- Zhejiang University
- Hangzhou
- China
| | - Yibin Ying
- Laboratory of Agricultural Information Intelligent Sensing
- School of Biosystems Engineering and Food Science
- Zhejiang University
- Hangzhou
- China
| | - Jianfeng Ping
- Laboratory of Agricultural Information Intelligent Sensing
- School of Biosystems Engineering and Food Science
- Zhejiang University
- Hangzhou
- China
| |
Collapse
|
24
|
Preston LJ, Barcenilla R, Dartnell LR, Kucukkilic-Stephens E, Olsson-Francis K. Infrared Spectroscopic Detection of Biosignatures at Lake Tírez, Spain: Implications for Mars. ASTROBIOLOGY 2020; 20:15-25. [PMID: 31592682 PMCID: PMC6987737 DOI: 10.1089/ast.2019.2106] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/21/2019] [Accepted: 08/13/2019] [Indexed: 06/10/2023]
Abstract
The detection of potential biosignatures with mineral matrices is part of a multifaceted approach in the search for life on other planetary bodies. The 2020 ExoMars Rosalind Franklin rover includes within its payload three IR spectrometers in the form of ISEM (Infrared Spectrometer for ExoMars), MicrOmega, and Ma-MISS (Mars Multispectral Imager for Subsurface Studies). The use of this technique in the detection and characterization of biosignatures is of great value. Organic materials are often co-deposited in terrestrial evaporites and as such have been proposed as relevant analogs in the search for life on Mars. This study focuses on Ca-sulfates collected from the hypersaline Tírez Lake in Spain. Mid infrared and visible near infrared analysis of soils, salt crusts, and crystals with green and red layering indicative of microbial colonization of the samples was acquired from across the lake and identified the main mineral to be gypsum with inputs of carbonate and silica. Organic functional groups that could be attributed to amides and carboxylic acids were identified as well as chlorophyll; however, due to the strong mineralogical absorptions observed, these were hard to unambiguously discern. Taxonomical assignment demonstrated that the archaeal community within the samples was dominated by the halophilic extremophile Halobacteriaceae while the bacterial community was dominated by the class Nocardiaceae. The results of this research highlight that sulfates on Mars are a mixed blessing, acting as an effective host for organic matter preservation but also a material that masks the presence of organic functional groups when analyzed with spectroscopic tools similar to those due to fly on the 2020 ExoMars rover. A suite of complementary analytical techniques therefore should be used to support the spectral identification of any candidate extraterrestrial biosignatures.
Collapse
Affiliation(s)
- Louisa J. Preston
- Department of Earth and Planetary Sciences, Birkbeck College, University of London, London, UK
| | - Rebeca Barcenilla
- Department of Earth and Planetary Sciences, Birkbeck College, University of London, London, UK
- Department of Life Sciences, University of Westminster, London, UK
| | | | | | | |
Collapse
|
25
|
Arevalo R, Ni Z, Danell RM. Mass spectrometry and planetary exploration: A brief review and future projection. JOURNAL OF MASS SPECTROMETRY : JMS 2020; 55:e4454. [PMID: 31663201 PMCID: PMC7050511 DOI: 10.1002/jms.4454] [Citation(s) in RCA: 24] [Impact Index Per Article: 6.0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/08/2019] [Revised: 09/25/2019] [Accepted: 10/04/2019] [Indexed: 05/11/2023]
Abstract
Since the inception of mass spectrometry more than a century ago, the field has matured as analytical capabilities have progressed, instrument configurations multiplied, and applications proliferated. Modern systems are able to characterize volatile and nonvolatile sample materials, quantitatively measure abundances of molecular and elemental species with low limits of detection, and determine isotopic compositions with high degrees of precision and accuracy. Consequently, mass spectrometers have a rich history and promising future in planetary exploration. Here, we provide a short review on the development of mass analyzers and supporting subsystems (eg, ionization sources and detector assemblies) that have significant heritage in spaceflight applications, and we introduce a selection of emerging technologies that may enable new and/or augmented mission concepts in the coming decades.
Collapse
Affiliation(s)
- Ricardo Arevalo
- Department of GeologyUniversity of MarylandCollege ParkMaryland
| | - Ziqin Ni
- Department of GeologyUniversity of MarylandCollege ParkMaryland
| | | |
Collapse
|
26
|
Elpa DP, Prabhu GRD, Wu SP, Tay KS, Urban PL. Automation of mass spectrometric detection of analytes and related workflows: A review. Talanta 2019; 208:120304. [PMID: 31816721 DOI: 10.1016/j.talanta.2019.120304] [Citation(s) in RCA: 22] [Impact Index Per Article: 4.4] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/24/2019] [Revised: 08/26/2019] [Accepted: 08/28/2019] [Indexed: 12/13/2022]
Abstract
The developments in mass spectrometry (MS) in the past few decades reveal the power and versatility of this technology. MS methods are utilized in routine analyses as well as research activities involving a broad range of analytes (elements and molecules) and countless matrices. However, manual MS analysis is gradually becoming a thing of the past. In this article, the available MS automation strategies are critically evaluated. Automation of analytical workflows culminating with MS detection encompasses involvement of automated operations in any of the steps related to sample handling/treatment before MS detection, sample introduction, MS data acquisition, and MS data processing. Automated MS workflows help to overcome the intrinsic limitations of MS methodology regarding reproducibility, throughput, and the expertise required to operate MS instruments. Such workflows often comprise automated off-line and on-line steps such as sampling, extraction, derivatization, and separation. The most common instrumental tools include autosamplers, multi-axis robots, flow injection systems, and lab-on-a-chip. Prototyping customized automated MS systems is a way to introduce non-standard automated features to MS workflows. The review highlights the enabling role of automated MS procedures in various sectors of academic research and industry. Examples include applications of automated MS workflows in bioscience, environmental studies, and exploration of the outer space.
Collapse
Affiliation(s)
- Decibel P Elpa
- Department of Applied Chemistry, National Chiao Tung University, 1001 University Rd., Hsinchu, 300, Taiwan; Department of Chemistry, National Tsing Hua University, 101, Section 2, Kuang-Fu Rd., Hsinchu, 30013, Taiwan
| | - Gurpur Rakesh D Prabhu
- Department of Applied Chemistry, National Chiao Tung University, 1001 University Rd., Hsinchu, 300, Taiwan; Department of Chemistry, National Tsing Hua University, 101, Section 2, Kuang-Fu Rd., Hsinchu, 30013, Taiwan
| | - Shu-Pao Wu
- Department of Applied Chemistry, National Chiao Tung University, 1001 University Rd., Hsinchu, 300, Taiwan.
| | - Kheng Soo Tay
- Department of Chemistry, Faculty of Science, University of Malaya, 50603 Kuala Lumpur, Malaysia
| | - Pawel L Urban
- Department of Chemistry, National Tsing Hua University, 101, Section 2, Kuang-Fu Rd., Hsinchu, 30013, Taiwan; Frontier Research Center on Fundamental and Applied Sciences of Matters, National Tsing Hua University, 101, Section 2, Kuang-Fu Rd., Hsinchu, 30013, Taiwan.
| |
Collapse
|
27
|
Hare BJ, Maiti D, Meier AJ, Bhethanabotla VR, Kuhn JN. CO2 Conversion Performance of Perovskite Oxides Designed with Abundant Metals. Ind Eng Chem Res 2019. [DOI: 10.1021/acs.iecr.9b01153] [Citation(s) in RCA: 11] [Impact Index Per Article: 2.2] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/28/2022]
Affiliation(s)
- Bryan J. Hare
- Department of Chemical & Biomolecular Engineering, University of South Florida, Tampa, Florida 33620, United States
| | - Debtanu Maiti
- Department of Chemical & Biomolecular Engineering, University of South Florida, Tampa, Florida 33620, United States
| | - Anne J. Meier
- Department of Chemical & Biomolecular Engineering, University of South Florida, Tampa, Florida 33620, United States
- Analytical Laboratories Branch, NASA Kennedy Space Center, Mail Stop NE-L3, Merritt Island, Florida 32899, United States
| | - Venkat R. Bhethanabotla
- Department of Chemical & Biomolecular Engineering, University of South Florida, Tampa, Florida 33620, United States
| | - John N. Kuhn
- Department of Chemical & Biomolecular Engineering, University of South Florida, Tampa, Florida 33620, United States
| |
Collapse
|
28
|
Montgomery W, Jaramillo EA, Royle SH, Kounaves SP, Schulze-Makuch D, Sephton MA. Effects of Oxygen-Containing Salts on the Detection of Organic Biomarkers on Mars and in Terrestrial Analog Soils. ASTROBIOLOGY 2019; 19:711-721. [PMID: 31062993 DOI: 10.1089/ast.2018.1888] [Citation(s) in RCA: 16] [Impact Index Per Article: 3.2] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/09/2023]
Abstract
The detection of chlorinated hydrocarbons by Curiosity on Mars has been attributed to the presence of unidentified indigenous organic matter. Similarly, oxychlorines on Earth have been proposed to be responsible for the apparent lack of organics in the Atacama Desert. The presence of perchlorate (ClO4-) poses a unique challenge to the measurement of organic matter due to the oxidizing power of oxychlorines during commonly used pyrolysis-gas chromatography-mass spectrometry (py-GC-MS) methods. Here, we show that perchlorates and other oxyanion salts inhibit the detection of organic compounds but that removing these problematic species prior to pyrolysis by using an optimal sample extraction duration and suitable ratios of water to sample mass enables analysis. We have characterized leached and unleached samples containing perchlorates from the Atacama Desert and have found that after leaching, the py-GC-MS chromatograms of the dried mineral residues show identifiable biomarkers associated with indigenous cyanobacteria. Samples which were pyrolyzed without leaching showed no detectable organic matter other than background siloxane and very weak or no trace of detectable polychlorinated benzenes. Dried sample residues remaining after leaching, the mineral matrix and water-insoluble organic matter, showed a strong organic response in all cases when analyzed by py-GC-MS. These residues are most likely the product of the pyrolysis of water-insoluble organics originally present in the samples. In addition, our results imply that previous soil analyses which contained high levels of oxyanions and concluded that organics were either not present or were present at extremely low levels should be reexamined.
Collapse
Affiliation(s)
- Wren Montgomery
- 1 Department of Earth Science and Engineering, Imperial College London, London, UK
| | | | - Samuel H Royle
- 1 Department of Earth Science and Engineering, Imperial College London, London, UK
| | - Samuel P Kounaves
- 1 Department of Earth Science and Engineering, Imperial College London, London, UK
- 2 Department of Chemistry, Tufts University, Medford, Massachusetts, USA
| | - Dirk Schulze-Makuch
- 3 Astrobiology Group, Center of Astronomy and Astrophysics, Technical University of Berlin, Berlin, Germany
| | - Mark A Sephton
- 1 Department of Earth Science and Engineering, Imperial College London, London, UK
| |
Collapse
|
29
|
Williams AJ, Eigenbrode J, Floyd M, Wilhelm MB, O'Reilly S, Johnson SS, Craft KL, Knudson CA, Andrejkovičová S, Lewis JM, Buch A, Glavin DP, Freissinet C, Williams RH, Szopa C, Millan M, Summons RE, McAdam A, Benison K, Navarro-González R, Malespin C, Mahaffy PR. Recovery of Fatty Acids from Mineralogic Mars Analogs by TMAH Thermochemolysis for the Sample Analysis at Mars Wet Chemistry Experiment on the Curiosity Rover. ASTROBIOLOGY 2019; 19:522-546. [PMID: 30869535 PMCID: PMC6459279 DOI: 10.1089/ast.2018.1819] [Citation(s) in RCA: 14] [Impact Index Per Article: 2.8] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/08/2018] [Accepted: 01/14/2019] [Indexed: 05/21/2023]
Abstract
The Mars Curiosity rover carries a diverse instrument payload to characterize habitable environments in the sedimentary layers of Aeolis Mons. One of these instruments is Sample Analysis at Mars (SAM), which contains a mass spectrometer that is capable of detecting organic compounds via pyrolysis gas chromatography mass spectrometry (py-GC-MS). To identify polar organic molecules, the SAM instrument carries the thermochemolysis reagent tetramethylammonium hydroxide (TMAH) in methanol (hereafter referred to as TMAH). TMAH can liberate fatty acids bound in macromolecules or chemically bound monomers associated with mineral phases and make these organics detectable via gas chromatography mass spectrometry (GC-MS) by methylation. Fatty acids, a type of carboxylic acid that contains a carboxyl functional group, are of particular interest given their presence in both biotic and abiotic materials. This work represents the first analyses of a suite of Mars-analog samples using the TMAH experiment under select SAM-like conditions. Samples analyzed include iron oxyhydroxides and iron oxyhydroxysulfates, a mixture of iron oxides/oxyhydroxides and clays, iron sulfide, siliceous sinter, carbonates, and shale. The TMAH experiments produced detectable signals under SAM-like pyrolysis conditions when organics were present either at high concentrations or in geologically modern systems. Although only a few analog samples exhibited a high abundance and variety of fatty acid methyl esters (FAMEs), FAMEs were detected in the majority of analog samples tested. When utilized, the TMAH thermochemolysis experiment on SAM could be an opportunity to detect organic molecules bound in macromolecules on Mars. The detection of a FAME profile is of great astrobiological interest, as it could provide information regarding the source of martian organic material detected by SAM.
Collapse
Affiliation(s)
- Amy J. Williams
- Department of Physics, Astronomy, and Geosciences, Towson University, Towson, Maryland, USA
- Center for Research and Exploration in Space Sciences and Technology/University of Maryland Baltimore County, Baltimore, Maryland, USA
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| | - Jennifer Eigenbrode
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| | - Melissa Floyd
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| | | | - Shane O'Reilly
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA
- School of Earth Sciences, University College Dublin, Dublin, Ireland
| | | | - Kathleen L. Craft
- Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA
| | - Christine A. Knudson
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
- Center for Research and Exploration in Space Sciences and Technology/University of Maryland College Park, College Park, Maryland, USA
| | - Slavka Andrejkovičová
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
- Center for Research and Exploration in Space Sciences and Technology/University of Maryland College Park, College Park, Maryland, USA
| | - James M.T. Lewis
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
- Universities Space Research Association, Columbia, Maryland, USA
| | - Arnaud Buch
- Laboratoire de Génie des Procédés et Matériaux, CentraleSupelec, Gif sur Yvette, France
| | - Daniel P. Glavin
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| | - Caroline Freissinet
- CNRS–UVSQ Laboratoire Atmosphères Milieux Observations Spatiales LATMOS, Guyancourt, France
| | - Ross H. Williams
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
- Center for Research and Exploration in Space Sciences and Technology/University of Maryland College Park, College Park, Maryland, USA
| | - Cyril Szopa
- CNRS–UVSQ Laboratoire Atmosphères Milieux Observations Spatiales LATMOS, Guyancourt, France
| | - Maëva Millan
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
- Department of Biology, Georgetown University, Washington, DC, USA
| | - Roger E. Summons
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA
| | - Amy McAdam
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| | - Kathleen Benison
- Department of Geology and Geography, West Virginia University, Morgantown, West Virginia, USA
| | - Rafael Navarro-González
- Instituto de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico, Circuito Exterior, Ciudad Universitaria, Ciudad de Mexico, Mexico
| | - Charles Malespin
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| | - Paul R. Mahaffy
- Space Science Exploration Division (Code 690), NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| |
Collapse
|
30
|
Kinetics of White Soft Minerals (WSMs) Decomposition under Conditions of Interest for Astrobiology: A Theoretical and Experimental Study. GEOSCIENCES 2019. [DOI: 10.3390/geosciences9020101] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
In this paper, the thermal decomposition kinetics of a class of minerals that we call White Soft Minerals (WSMs) is studied by means of theoretical and experimental methods, in connection to the transport of extraterrestrial organic matter to Earth and the possible use of the decomposition reaction in the characterization of these minerals in space. WSMs include, under a single denomination, carbonates and sulphates of Mg, Fe, and Ca. To improve the present knowledge of the properties of such materials, we use the following techniques: kinetic models for chemical decomposition, atmospheric entry models, spectroscopy, and gravimetric analyses. Model results show that the atmospheric entry of WSM grains is strongly affected by their thermal decomposition. The decomposition reaction, being strongly endothermic, tends to significantly lower the grain temperature during the atmospheric entry, especially at high altitudes and for grazing entries. A previously proposed infrared spectroscopic technique to evaluate the degree of advancement of the reaction is found to be in good agreement with gravimetric measurements for calcium carbonate. The numerical model developed for the atmospheric entry scenarios is used to interpret experimental results. These main findings show that an additional contribution to the reaction enthalpy is needed to reproduce the experimental results, suggesting that the present theoretical model needs improvements such as the account of gas diffusion in the materials.
Collapse
|
31
|
Arevalo R, Selliez L, Briois C, Carrasco N, Thirkell L, Cherville B, Colin F, Gaubicher B, Farcy B, Li X, Makarov A. An Orbitrap-based laser desorption/ablation mass spectrometer designed for spaceflight. RAPID COMMUNICATIONS IN MASS SPECTROMETRY : RCM 2018; 32:1875-1886. [PMID: 30048021 DOI: 10.1002/rcm.8244] [Citation(s) in RCA: 17] [Impact Index Per Article: 2.8] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/11/2018] [Revised: 07/05/2018] [Accepted: 07/18/2018] [Indexed: 06/08/2023]
Abstract
RATIONALE The investigation of cryogenic planetary environments as potential harbors for extant life and/or contemporary sites of organic synthesis represents an emerging focal point in planetary exploration. Next generation instruments need to be capable of unambiguously determining elemental and/or molecular stoichiometry via highly accurate mass measurements and the separation of isobaric interferences. METHODS An Orbitrap™ analyzer adapted for spaceflight (referred to as the CosmOrbitrap), coupled with a commercial pulsed UV laser source (266 nm), was used to successfully characterize a variety of planetary analog samples via ultrahigh resolution laser desorption/ablation mass spectrometry. The materials analyzed in this study include: jarosite (a hydrous sulfate detected on Mars); magnesium sulfate (a potential component of the subsurface ocean on Europa); uracil (a nucleobase of RNA); and a variety of amino acids. RESULTS The instrument configuration tested here enables: measurement of major elements and organic molecules with ultrahigh mass resolution (m/Δm ≥ 120,000, FWHM); quantification of isotopic abundances with <1.0% (2σ) precision; and identification of highly accurate masses within 3.2 ppm of absolute values. The analysis of a residue of a dilute solution of amino acids demonstrates the capacity to detect twelve amino acids in positive ion mode at concentrations as low as ≤1 pmol/mm2 while maintaining mass resolution and accuracy requirements. CONCLUSIONS The CosmOrbitrap mass analyzer is highly sensitive and delivers mass resolution/accuracy unmatched by any instrument sent into orbit or launched into deep space. This prototype instrument, which maps to a spaceflight implementation, represents a mission-enabling technology capable of advancing planetary exploration for decades to come.
Collapse
Affiliation(s)
- Ricardo Arevalo
- Department of Geology, University of Maryland, College Park, MD, 20742, USA
| | - Laura Selliez
- Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), UMR 7328 du CNRS, 45071, Orléans, France
- Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), 78280, Guyancourt, France
| | - Christelle Briois
- Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), UMR 7328 du CNRS, 45071, Orléans, France
| | - Nathalie Carrasco
- Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), 78280, Guyancourt, France
| | - Laurent Thirkell
- Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), UMR 7328 du CNRS, 45071, Orléans, France
| | - Barnabé Cherville
- Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), UMR 7328 du CNRS, 45071, Orléans, France
| | - Fabrice Colin
- Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), UMR 7328 du CNRS, 45071, Orléans, France
| | - Bertrand Gaubicher
- Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), UMR 7328 du CNRS, 45071, Orléans, France
| | - Benjamin Farcy
- Department of Geology, University of Maryland, College Park, MD, 20742, USA
| | - Xiang Li
- Center for Space Science & Technology, University of Maryland, Baltimore County, Baltimore, MD, 21250, USA
| | | |
Collapse
|
32
|
Fornaro T, Steele A, Brucato JR. Catalytic/Protective Properties of Martian Minerals and Implications for Possible Origin of Life on Mars. Life (Basel) 2018; 8:life8040056. [PMID: 30400661 PMCID: PMC6315534 DOI: 10.3390/life8040056] [Citation(s) in RCA: 17] [Impact Index Per Article: 2.8] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/05/2018] [Revised: 10/28/2018] [Accepted: 10/30/2018] [Indexed: 11/16/2022] Open
Abstract
Minerals might have played critical roles for the origin and evolution of possible life forms on Mars. The study of the interactions between the "building blocks of life" and minerals relevant to Mars mineralogy under conditions mimicking the harsh Martian environment may provide key insight into possible prebiotic processes. Therefore, this contribution aims at reviewing the most important investigations carried out so far about the catalytic/protective properties of Martian minerals toward molecular biosignatures under Martian-like conditions. Overall, it turns out that the fate of molecular biosignatures on Mars depends on a delicate balance between multiple preservation and degradation mechanisms, often regulated by minerals, which may take place simultaneously. Such a complexity requires more efforts in simulating realistically the Martian environment in order to better inspect plausible prebiotic pathways and shed light on the nature of the organic compounds detected both in meteorites and on the surface of Mars through in situ analysis.
Collapse
Affiliation(s)
- Teresa Fornaro
- Geophysical Laboratory of the Carnegie Institution for Science, 5251 Broad Branch Rd. NW, Washington, DC 20015, USA.
| | - Andrew Steele
- Geophysical Laboratory of the Carnegie Institution for Science, 5251 Broad Branch Rd. NW, Washington, DC 20015, USA.
| | - John Robert Brucato
- INAF-Astrophysical Observatory of Arcetri, L.go E. Fermi 5, 50125 Firenze, Italy.
| |
Collapse
|
33
|
Cheptsov VS, Vorobyova EA, Osipov GA, Manucharova NA, Polyanskaya LM, Gorlenko MV, Pavlov AK, Rosanova MS, Lomasov VN. Microbial activity in Martian analog soils after ionizing radiation: implications for the preservation of subsurface life on Mars. AIMS Microbiol 2018; 4:541-562. [PMID: 31294232 PMCID: PMC6604939 DOI: 10.3934/microbiol.2018.3.541] [Citation(s) in RCA: 9] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/30/2018] [Accepted: 07/04/2018] [Indexed: 11/18/2022] Open
Abstract
At present, the surface of Mars is affected by a set of factors that can prevent the survival of Earth-like life. However, the modern concept of the evolution of the planet assumes the existence more favorable for life climate in the past. If in the past on Mars had formed a biosphere, similar to the one that originated in the early Earth, it is supposed that it is preserved till now in anabiotic state in the bowels of the planet, like microbial communities inhabiting the ancient permafrost of Arctic and Antarctic. In the conditions of modern Martian regolith, this relic life seems to be deprived of the possibility of damage reparation (or these processes occur on a geological time scale), and ionizing radiation should be considered the main factor inhibiting such anabiotic life. In the present study, we studied soil samples, selected in two different extreme habitats of the Earth: ancient permafrost from the Dry Valleys of Antarctica and Xerosol soil from the mountain desert in Morocco, gamma-irradiated with 40 kGy dose at low pressure (1 Torr) and low temperature (-50 °C). Microbial communities inhabiting these samples showed in situ high resistance to the applied effects, retained high number of viable cells, metabolic activity, and high biodiversity. Based on the results, it is assumed that the putative biosphere could be preserved in the dormant state for at least 500 thousand years and 8 million years in the surface layer of Mars regolith and at 5 m depth, respectively, at the current level of ionizing radiation intensity.
Collapse
Affiliation(s)
- Vladimir S Cheptsov
- Soil Science Faculty, Lomonosov Moscow State University, Moscow, Russia.,Space Research Institute, Russian Academy of Sciences, Moscow, Russia
| | - Elena A Vorobyova
- Soil Science Faculty, Lomonosov Moscow State University, Moscow, Russia.,Space Research Institute, Russian Academy of Sciences, Moscow, Russia
| | - George A Osipov
- International Analytical Center, Interlab, N.D.Zelinsky Institute of Organic Chemistry, Moscow, Russia
| | | | | | | | - Anatoli K Pavlov
- Ioffe Physical-Technical Institute, Russian Academy of Sciences, St. Petersburg, Russia
| | - Marina S Rosanova
- Soil Science Faculty, Lomonosov Moscow State University, Moscow, Russia
| | - Vladimir N Lomasov
- Peter the Great St. Petersburg State Polytechnic University, St. Petersburg, Russia
| |
Collapse
|
34
|
McMahon S, Bosak T, Grotzinger JP, Milliken RE, Summons RE, Daye M, Newman SA, Fraeman A, Williford KH, Briggs DEG. A Field Guide to Finding Fossils on Mars. JOURNAL OF GEOPHYSICAL RESEARCH. PLANETS 2018; 123:1012-1040. [PMID: 30034979 PMCID: PMC6049883 DOI: 10.1029/2017je005478] [Citation(s) in RCA: 38] [Impact Index Per Article: 6.3] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/07/2017] [Revised: 03/28/2018] [Accepted: 04/23/2018] [Indexed: 05/05/2023]
Abstract
The Martian surface is cold, dry, exposed to biologically harmful radiation and apparently barren today. Nevertheless, there is clear geological evidence for warmer, wetter intervals in the past that could have supported life at or near the surface. This evidence has motivated National Aeronautics and Space Administration and European Space Agency to prioritize the search for any remains or traces of organisms from early Mars in forthcoming missions. Informed by (1) stratigraphic, mineralogical and geochemical data collected by previous and current missions, (2) Earth's fossil record, and (3) experimental studies of organic decay and preservation, we here consider whether, how, and where fossils and isotopic biosignatures could have been preserved in the depositional environments and mineralizing media thought to have been present in habitable settings on early Mars. We conclude that Noachian-Hesperian Fe-bearing clay-rich fluvio-lacustrine siliciclastic deposits, especially where enriched in silica, currently represent the most promising and best understood astropaleontological targets. Siliceous sinters would also be an excellent target, but their presence on Mars awaits confirmation. More work is needed to improve our understanding of fossil preservation in the context of other environments specific to Mars, particularly within evaporative salts and pore/fracture-filling subsurface minerals.
Collapse
Affiliation(s)
- S. McMahon
- Department of Geology and GeophysicsYale UniversityNew HavenCTUSA
- UK Centre for Astrobiology, School of Physics and AstronomyUniversity of EdinburghEdinburghUK
| | - T. Bosak
- Department of Earth, Atmospheric and Planetary SciencesMassachusetts Institute of TechnologyCambridgeMAUSA
| | - J. P. Grotzinger
- Division of Geological and Planetary SciencesCalifornia Institute of TechnologyPasadenaCAUSA
| | - R. E. Milliken
- Department of Earth, Environmental and Planetary SciencesBrown UniversityProvidenceRIUSA
| | - R. E. Summons
- Department of Earth, Atmospheric and Planetary SciencesMassachusetts Institute of TechnologyCambridgeMAUSA
| | - M. Daye
- Department of Earth, Atmospheric and Planetary SciencesMassachusetts Institute of TechnologyCambridgeMAUSA
| | - S. A. Newman
- Department of Earth, Atmospheric and Planetary SciencesMassachusetts Institute of TechnologyCambridgeMAUSA
| | - A. Fraeman
- Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadenaCAUSA
| | - K. H. Williford
- Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadenaCAUSA
| | - D. E. G. Briggs
- Department of Geology and GeophysicsYale UniversityNew HavenCTUSA
| |
Collapse
|
35
|
Moros J, ElFaham MM, Laserna JJ. Dual-Spectroscopy Platform for the Surveillance of Mars Mineralogy Using a Decisions Fusion Architecture on Simultaneous LIBS-Raman Data. Anal Chem 2018; 90:2079-2087. [DOI: 10.1021/acs.analchem.7b04124] [Citation(s) in RCA: 37] [Impact Index Per Article: 6.2] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
Affiliation(s)
- Javier Moros
- Universidad de Málaga, Departamento de
Química Analítica, UMALASERLAB, 29010 Málaga, Spain
| | | | - J. Javier Laserna
- Universidad de Málaga, Departamento de
Química Analítica, UMALASERLAB, 29010 Málaga, Spain
| |
Collapse
|
36
|
Uckert K, Chanover NJ, Getty S, Voelz DG, Brinckerhoff WB, McMillan N, Xiao X, Boston PJ, Li X, McAdam A, Glenar DA, Chavez A. The Characterization of Biosignatures in Caves Using an Instrument Suite. ASTROBIOLOGY 2017; 17:1203-1218. [PMID: 29227156 DOI: 10.1089/ast.2016.1568] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/07/2023]
Abstract
The search for life and habitable environments on other Solar System bodies is a major motivator for planetary exploration. Due to the difficulty and significance of detecting extant or extinct extraterrestrial life in situ, several independent measurements from multiple instrument techniques will bolster the community's confidence in making any such claim. We demonstrate the detection of subsurface biosignatures using a suite of instrument techniques including IR reflectance spectroscopy, laser-induced breakdown spectroscopy, and scanning electron microscopy/energy dispersive X-ray spectroscopy. We focus our measurements on subterranean calcium carbonate field samples, whose biosignatures are analogous to those that might be expected on some high-interest astrobiology targets. In this work, we discuss the feasibility and advantages of using each of the aforementioned instrument techniques for the in situ search for biosignatures and present results on the autonomous characterization of biosignatures using multivariate statistical analysis techniques. Key Words: Biosignature suites-Caves-Mars-Life detection. Astrobiology 17, 1203-1218.
Collapse
Affiliation(s)
- Kyle Uckert
- 1 Department of Astronomy, New Mexico State University , Las Cruces, New Mexico
| | - Nancy J Chanover
- 1 Department of Astronomy, New Mexico State University , Las Cruces, New Mexico
| | | | - David G Voelz
- 3 Department of Electrical and Computer Engineering, New Mexico State University , Las Cruces, New Mexico
| | | | - Nancy McMillan
- 4 Department of Geological Sciences, New Mexico State University , Las Cruces, New Mexico
| | - Xifeng Xiao
- 3 Department of Electrical and Computer Engineering, New Mexico State University , Las Cruces, New Mexico
| | - Penelope J Boston
- 5 NASA Astrobiology Institute , NASA Ames Research Center, Moffett Field, California
| | - Xiang Li
- 6 University of Maryland , Baltimore County, Baltimore, Maryland
| | - Amy McAdam
- 2 NASA/Goddard Space Flight Center , Greenbelt, Maryland
| | - David A Glenar
- 6 University of Maryland , Baltimore County, Baltimore, Maryland
| | - Arriana Chavez
- 4 Department of Geological Sciences, New Mexico State University , Las Cruces, New Mexico
| |
Collapse
|
37
|
Cataldi G, Brandeker A, Thébault P, Singer K, Ahmed E, de Vries BL, Neubeck A, Olofsson G. Searching for Biosignatures in Exoplanetary Impact Ejecta. ASTROBIOLOGY 2017; 17:721-746. [PMID: 28692303 DOI: 10.1089/ast.2015.1437] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/07/2023]
Abstract
With the number of confirmed rocky exoplanets increasing steadily, their characterization and the search for exoplanetary biospheres are becoming increasingly urgent issues in astrobiology. To date, most efforts have concentrated on the study of exoplanetary atmospheres. Instead, we aim to investigate the possibility of characterizing an exoplanet (in terms of habitability, geology, presence of life, etc.) by studying material ejected from the surface during an impact event. For a number of impact scenarios, we estimate the escaping mass and assess its subsequent collisional evolution in a circumstellar orbit, assuming a Sun-like host star. We calculate the fractional luminosity of the dust as a function of time after the impact event and study its detectability with current and future instrumentation. We consider the possibility to constrain the dust composition, giving information on the geology or the presence of a biosphere. As examples, we investigate whether calcite, silica, or ejected microorganisms could be detected. For a 20 km diameter impactor, we find that the dust mass escaping the exoplanet is roughly comparable to the zodiacal dust, depending on the exoplanet's size. The collisional evolution is best modeled by considering two independent dust populations, a spalled population consisting of nonmelted ejecta evolving on timescales of millions of years, and dust recondensed from melt or vapor evolving on much shorter timescales. While the presence of dust can potentially be inferred with current telescopes, studying its composition requires advanced instrumentation not yet available. The direct detection of biological matter turns out to be extremely challenging. Despite considerable difficulties (small dust masses, noise such as exozodiacal dust, etc.), studying dusty material ejected from an exoplanetary surface might become an interesting complement to atmospheric studies in the future. Key Words: Biosignatures-Exoplanets-Impacts-Interplanetary dust-Remote sensing. Astrobiology 17, 721-746.
Collapse
Affiliation(s)
- Gianni Cataldi
- 1 AlbaNova University Centre, Stockholm University , Department of Astronomy, Stockholm, Sweden
- 2 Stockholm University Astrobiology Centre , Stockholm, Sweden
| | - Alexis Brandeker
- 1 AlbaNova University Centre, Stockholm University , Department of Astronomy, Stockholm, Sweden
- 2 Stockholm University Astrobiology Centre , Stockholm, Sweden
| | - Philippe Thébault
- 3 LESIA-Observatoire de Paris, UPMC Univ. Paris 06, Univ. Paris-Diderot , Paris, France
| | - Kelsi Singer
- 4 Southwest Research Institute , Boulder, Colorado, USA
| | - Engy Ahmed
- 2 Stockholm University Astrobiology Centre , Stockholm, Sweden
- 5 Royal Institute of Technology (KTH) , Science for Life Laboratory, Solna, Sweden
- 6 Stockholm University , Department of Geological Sciences, Stockholm, Sweden
| | - Bernard L de Vries
- 1 AlbaNova University Centre, Stockholm University , Department of Astronomy, Stockholm, Sweden
- 2 Stockholm University Astrobiology Centre , Stockholm, Sweden
- 7 Scientific Support Office, Directorate of Science, European Space Research and Technology Centre (ESA/ESTEC) , Noordwijk, The Netherlands
| | - Anna Neubeck
- 2 Stockholm University Astrobiology Centre , Stockholm, Sweden
- 6 Stockholm University , Department of Geological Sciences, Stockholm, Sweden
| | - Göran Olofsson
- 1 AlbaNova University Centre, Stockholm University , Department of Astronomy, Stockholm, Sweden
- 2 Stockholm University Astrobiology Centre , Stockholm, Sweden
| |
Collapse
|
38
|
Goesmann F, Brinckerhoff WB, Raulin F, Goetz W, Danell RM, Getty SA, Siljeström S, Mißbach H, Steininger H, Arevalo RD, Buch A, Freissinet C, Grubisic A, Meierhenrich UJ, Pinnick VT, Stalport F, Szopa C, Vago JL, Lindner R, Schulte MD, Brucato JR, Glavin DP, Grand N, Li X, van Amerom FHW. The Mars Organic Molecule Analyzer (MOMA) Instrument: Characterization of Organic Material in Martian Sediments. ASTROBIOLOGY 2017; 17:655-685. [PMID: 31067288 PMCID: PMC5685156 DOI: 10.1089/ast.2016.1551] [Citation(s) in RCA: 85] [Impact Index Per Article: 12.1] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/19/2016] [Accepted: 04/10/2017] [Indexed: 05/09/2023]
Abstract
The Mars Organic Molecule Analyzer (MOMA) instrument onboard the ESA/Roscosmos ExoMars rover (to launch in July, 2020) will analyze volatile and refractory organic compounds in martian surface and subsurface sediments. In this study, we describe the design, current status of development, and analytical capabilities of the instrument. Data acquired on preliminary MOMA flight-like hardware and experimental setups are also presented, illustrating their contribution to the overall science return of the mission. Key Words: Mars-Mass spectrometry-Life detection-Planetary instrumentation. Astrobiology 17, 655-685.
Collapse
Affiliation(s)
- Fred Goesmann
- Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany
| | | | - François Raulin
- LISA, U. Paris-Est, Créteil, U. Paris Diderot, Paris, CNRS, France
| | - Walter Goetz
- Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany
| | | | | | - Sandra Siljeström
- RISE Research Institutes of Sweden, Bioscience and Materials/Chemistry and Materials, Stockholm, Sweden
| | - Helge Mißbach
- Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany
| | | | | | - Arnaud Buch
- LPGM, CentraleParis, Chatenay-Malabry, France
| | | | - Andrej Grubisic
- NASA GSFC, Greenbelt, Maryland, USA
- University of Maryland, College Park, Maryland, USA
| | | | | | - Fabien Stalport
- LISA, U. Paris-Est, Créteil, U. Paris Diderot, Paris, CNRS, France
| | - Cyril Szopa
- LATMOS/IPSL, Guyancourt, France
- Institut Universitaire de France, Paris, France
| | | | | | | | | | | | - Noel Grand
- LISA, U. Paris-Est, Créteil, U. Paris Diderot, Paris, CNRS, France
| | - Xiang Li
- NASA GSFC, Greenbelt, Maryland, USA
- University of Maryland, Baltimore County, Baltimore, Maryland, USA
| | | |
Collapse
|
39
|
Potter-McIntyre SL, Williams J, Phillips-Lander C, O'Connell L. Taphonomy of Microbial Biosignatures in Spring Deposits: A Comparison of Modern, Quaternary, and Jurassic Examples. ASTROBIOLOGY 2017; 17:216-230. [PMID: 28323483 DOI: 10.1089/ast.2016.1495] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2023]
Abstract
On Earth, microorganisms commonly enhance mineral precipitation and mediate mineralogical and chemical compositions of resulting deposits, particularly at spring systems. However, preservation of any type of microbial fossil or chemical or textural biosignature depends on the degree of alteration during diagenesis and factors such as exposure to diagenetic fluids. Little is known about the transformation of biosignatures during diagenesis over geologic time. Ten Mile Graben, Utah, USA, hosts a cold spring system that is an exceptional site for evaluation of diagenetic alteration of biosignatures because of the presence of modern springs with actively precipitating microbial mats and a series of progressively older tufa terraces (<400 ka) preserved in the area from the same spring system. A previously undescribed Jurassic laminated carbonate unit within the upper part of the Brushy Basin Member of the Morrison Formation is also exposed in Ten Mile Graben. This research characterizes the geology of these modern and Quaternary saline, Fe-undersaturated, circumneutral Ten Mile Graben cold springs and provides the first description in the literature of the Jurassic Brushy Basin Member of the Morrison Formation carbonate deposit. Taphonomy of microbial fossils is characterized by scanning electron microscopy (SEM). The data highlight two distinct methods of biosignature formation: (1) precipitation of minerals from an undersaturated solution owing to metabolic activity of the cells and (2) mineral precipitation on charged cell surfaces that produce distinctive microbial trace fossils. Although diagenesis can destroy or severely degrade biosignatures, particularly microbial fossils, some fossils and trace fossils are preserved because entombment by Ostwald ripening limits diagenetic alteration. Recognizing spring-fed, biogenic tufas is crucial for astrobiological research and the search for life on Mars. Key Words: Biosignatures-Taphonomy-Diagenesis-Carbonates-Hot springs. Astrobiology 17, 216-230.
Collapse
Affiliation(s)
| | - Jason Williams
- 1 Geology Department, Southern Illinois University , Carbondale, Illinois
| | - Charity Phillips-Lander
- 2 Conoco Phillips School of Geology and Geophysics, University of Oklahoma , Norman, Oklahoma
| | - Laura O'Connell
- 1 Geology Department, Southern Illinois University , Carbondale, Illinois
| |
Collapse
|
40
|
Lasne J, Noblet A, Szopa C, Navarro-González R, Cabane M, Poch O, Stalport F, François P, Atreya SK, Coll P. Oxidants at the Surface of Mars: A Review in Light of Recent Exploration Results. ASTROBIOLOGY 2016; 16:977-996. [PMID: 27925795 DOI: 10.1089/ast.2016.1502] [Citation(s) in RCA: 15] [Impact Index Per Article: 1.9] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/06/2023]
Abstract
In 1976, the Viking landers carried out the most comprehensive search for organics and microbial life in the martian regolith. Their results indicate that Mars' surface is lifeless and, surprisingly, depleted in organics at part-per-billion levels. Several biology experiments on the Viking landers gave controversial results that have since been explained by the presence of oxidizing agents on the surface of Mars. These oxidants may degrade abiotic or biological organics, resulting in their nondetection in the regolith. As several exploration missions currently focus on the detection of organics on Mars (or will do so in the near future), knowledge of the oxidative state of the surface is fundamental. It will allow for determination of the capability of organics to survive on a geological timescale, the most favorable places to seek them, and the best methods to process the samples collected at the surface. With this aim, we review the main oxidants assumed to be present on Mars, their possible formation pathways, and those laboratory studies in which their reactivity with organics under Mars-like conditions has been evaluated. Among the oxidants assumed to be present on Mars, only four have been detected so far: perchlorate ions (ClO4-) in salts, hydrogen peroxide (H2O2) in the atmosphere, and clays and metal oxides composing surface minerals. Clays have been suggested as catalysts for the oxidation of organics but are treated as oxidants in the following to keep the structure of this article straightforward. This work provides an insight into the oxidizing potential of the surface of Mars and an estimate of the stability of organic matter in an oxidizing environment. Key Words: Mars surface-Astrobiology-Oxidant-Chemical reactions. Astrobiology 16, 977-996.
Collapse
Affiliation(s)
- J Lasne
- 1 LISA, Universités Paris-Est Créteil and Paris Diderot, Institut Pierre Simon Laplace , CNRS UMR 7583, Créteil, France
| | - A Noblet
- 1 LISA, Universités Paris-Est Créteil and Paris Diderot, Institut Pierre Simon Laplace , CNRS UMR 7583, Créteil, France
| | - C Szopa
- 2 LATMOS, UPMC Université Paris 06, Université Versailles St Quentin , CNRS, Guyancourt, France
| | - R Navarro-González
- 3 Laboratorio de Química de Plasmas y Estudios Planetarios, Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México , Ciudad de México, México
| | - M Cabane
- 2 LATMOS, UPMC Université Paris 06, Université Versailles St Quentin , CNRS, Guyancourt, France
| | - O Poch
- 1 LISA, Universités Paris-Est Créteil and Paris Diderot, Institut Pierre Simon Laplace , CNRS UMR 7583, Créteil, France
- 4 NCCR PlanetS, Physikalisches Institut, Universität Bern , Bern, Switzerland
| | - F Stalport
- 1 LISA, Universités Paris-Est Créteil and Paris Diderot, Institut Pierre Simon Laplace , CNRS UMR 7583, Créteil, France
| | - P François
- 1 LISA, Universités Paris-Est Créteil and Paris Diderot, Institut Pierre Simon Laplace , CNRS UMR 7583, Créteil, France
- 5 IC2MP, Equipe Eau Géochimie Santé, Université de Poitiers , CNRS UMR 7285, Poitiers, France
| | - S K Atreya
- 6 Department of Climate and Space Sciences, University of Michigan , Ann Arbor, Michigan, USA
| | - P Coll
- 1 LISA, Universités Paris-Est Créteil and Paris Diderot, Institut Pierre Simon Laplace , CNRS UMR 7583, Créteil, France
| |
Collapse
|
41
|
Karna RR, Hettiarachchi GM, Newville M, Sun C, Ma Q. Synchrotron-based X-Ray Spectroscopy Studies for Redox-based Remediation of Lead, Zinc, and Cadmium in Mine Waste Materials. JOURNAL OF ENVIRONMENTAL QUALITY 2016; 45:1883-1893. [PMID: 27898777 DOI: 10.2134/jeq2015.12.0616] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/19/2023]
Abstract
Several studies have examined the effect of submergence on the mobility of metals present in mine waste materials. This study examines the effect of organic carbon (OC) and sulfur (S) additions and submergence time on redox-induced biogeochemical transformations of lead (Pb), zinc (Zn), and cadmium (Cd) present in mine waste materials collected from the Tri-State mining district located in southeastern Kansas, southwestern Missouri, and northeastern Oklahoma. A completely randomized design, with a two-way treatment structure, was used for conducting a series of column experiments. Two replicates were used for each treatment combination. Effluent samples were collected at several time points, and soil samples were collected at the end of each column experiment. Because these samples are highly heterogeneous, we used a variety of synchrotron-based techniques to identify Pb, Zn, and Cd speciation at both micro- and bulk-scale. Spectroscopic analysis results from the study revealed that the addition of OC, with and without S, promoted metal-sulfide formation, whereas metal carbonates dominated in the nonamended flooded materials and in mine waste materials only amended with S. Therefore, the synergistic effect of OC and S may be more promising for managing mine waste materials disposed of in flooded subsidence mine pits instead of individual S or OC treatments. The mechanistic understanding gained in this study is also relevant for remediation of waste materials using natural or constructed wetland systems.
Collapse
|
42
|
Georgiou CD, Zisimopoulos D, Panagiotidis K, Grintzalis K, Papapostolou I, Quinn RC, McKay CP, Sun HJ. Martian Superoxide and Peroxide O2 Release (OR) Assay: A New Technology for Terrestrial and Planetary Applications. ASTROBIOLOGY 2016; 16:126-142. [PMID: 26881470 DOI: 10.1089/ast.2015.1345] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/05/2023]
Abstract
This study presents an assay for the detection and quantification of soil metal superoxides and peroxides in regolith and soil. The O2 release (OR) assay is based on the enzymatic conversion of the hydrolysis products of metal oxides to O2 and their quantification by an O2 electrode based on the stoichiometry of the involved reactions. The intermediate product O₂˙⁻ from the hydrolysis of metal superoxides is converted by cytochrome c to O2 and by superoxide dismutase (SOD) to ½ mol O2 and ½ mol H2O2, which is then converted by catalase (CAT) to ½ mol O2. The product H2O2 from the hydrolysis of metal peroxides and hydroperoxides is converted to ½ mol O2 by CAT. The assay method was validated in a sealed sample chamber by using a liquid-phase Clark-type O2 electrode with known concentrations of O₂˙⁻ and H2O2, and commercial metal superoxide and peroxide mixed with Mars analog Mojave and Atacama Desert soils. Carbonates and perchlorates, both present on Mars, do not interfere with the assay. The assay lower limit of detection, when using luminescence quenching/optical sensing O2-electrodes, is 1 nmol O2 cm(-3) or better. The activity of the assay enzymes SOD and cytochrome c was unaffected up to 6 Gy exposure by γ radiation, while CAT retained 100% and 40% of its activity at 3 and 6 Gy, respectively, which demonstrates the suitability of these enzymes for planetary missions, for example, on Mars or Europa.
Collapse
Affiliation(s)
| | | | | | | | | | - Richard C Quinn
- 2 SETI Institute, Carl Sagan Center , Mountain View, California, USA
| | | | - Henry J Sun
- 4 Desert Research Institute , Las Vegas, Nevada, USA
| |
Collapse
|
43
|
Summons RE, Sessions AL, Allwood AC, Barton HA, Beaty DW, Blakkolb B, Canham J, Clark BC, Dworkin JP, Lin Y, Mathies R, Milkovich SM, Steele A. Planning considerations related to the organic contamination of Martian samples and implications for the Mars 2020 Rover. ASTROBIOLOGY 2014; 14:969-1027. [PMID: 25495496 DOI: 10.1089/ast.2014.1244] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/04/2023]
Affiliation(s)
- R E Summons
- 1 Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology , Cambridge, Massachusetts
| | | | | | | | | | | | | | | | | | | | | | | | | |
Collapse
|
44
|
Chatzitheodoridis E, Haigh S, Lyon I. A conspicuous clay ovoid in Nakhla: evidence for subsurface hydrothermal alteration on Mars with implications for astrobiology. ASTROBIOLOGY 2014; 14:651-693. [PMID: 25046549 PMCID: PMC4126275 DOI: 10.1089/ast.2013.1069] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/13/2013] [Accepted: 05/19/2014] [Indexed: 06/03/2023]
Abstract
Abstract A conspicuous biomorphic ovoid structure has been discovered in the Nakhla martian meteorite, made of nanocrystalline iron-rich saponitic clay and amorphous material. The ovoid is indigenous to Nakhla and occurs within a late-formed amorphous mesostasis region of rhyolitic composition that is interstitial to two clinopyroxene grains with Al-rich rims, and contains acicular apatite crystals, olivine, sulfides, Ti-rich magnetite, and a new mineral of the rhoenite group. To infer the origin of the ovoid, a large set of analytical tools was employed, including scanning electron microscopy and backscattered electron imaging, wavelength-dispersive X-ray analysis, X-ray mapping, Raman spectroscopy, time-of-flight secondary ion mass spectrometry analysis, high-resolution transmission electron microscope imaging, and atomic force microscope topographic mapping. The concentric wall of the ovoid surrounds an originally hollow volume and exhibits internal layering of contrasting nanotextures but uniform chemical composition, and likely inherited its overall shape from a preexisting vesicle in the mesostasis glass. A final fibrous layer of Fe-rich phases blankets the interior surfaces of the ovoid wall structure. There is evidence that the parent rock of Nakhla has undergone a shock event from a nearby bolide impact that melted the rims of pyroxene and the interstitial matter and initiated an igneous hydrothermal system of rapidly cooling fluids, which were progressively mixed with fluids from the melted permafrost. Sharp temperature gradients were responsible for the crystallization of Al-rich clinopyroxene rims, rhoenite, acicular apatites, and the quenching of the mesostasis glass and the vesicle. During the formation of the ovoid structure, episodic fluid infiltration events resulted in the precipitation of saponite rinds around the vesicle walls, altered pyrrhotite to marcasite, and then isolated the ovoid wall structure from the rest of the system by depositing a layer of iron oxides/hydroxides. Carbonates, halite, and sulfates were deposited last within interstitial spaces and along fractures. Among three plausible competing hypotheses here, this particular abiotic scenario is considered to be the most reasonable explanation for the formation of the ovoid structure in Nakhla, and although compelling evidence for a biotic origin is lacking, it is evident that the martian subsurface contains niche environments where life could develop.
Collapse
Affiliation(s)
- Elias Chatzitheodoridis
- Department of Geological Sciences, School of Mining and Metallurgical Engineering, National Technical University of Athens, Athens, Greece
| | - Sarah Haigh
- School of Materials, The University of Manchester, Manchester, UK
| | - Ian Lyon
- School of Earth, Atmospheric and Environmental Sciences, The University of Manchester, Manchester, UK
| |
Collapse
|
45
|
Shelor CP, Dasgupta PK, Aubrey A, Davila AF, Lee MC, McKay CP, Liu Y, Noell AC. What can in situ ion chromatography offer for Mars exploration? ASTROBIOLOGY 2014; 14:577-588. [PMID: 24963874 DOI: 10.1089/ast.2013.1131] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/03/2023]
Abstract
The successes of the Mars exploration program have led to our unprecedented knowledge of the geological, mineralogical, and elemental composition of the martian surface. To date, however, only one mission, the Phoenix lander, has specifically set out to determine the soluble chemistry of the martian surface. The surprising results, including the detection of perchlorate, demonstrated both the importance of performing soluble ion measurements and the need for improved instrumentation to unambiguously identify all the species present. Ion chromatography (IC) is the state-of-the-art technique for soluble ion analysis on Earth and would therefore be the ideal instrument to send to Mars. A flight IC system must necessarily be small, lightweight, low-power, and have low eluent consumption. We demonstrate here a breadboard system that addresses these issues by using capillary IC at low flow rates with an optimized eluent generator and suppressor. A mix of 12 ions known or plausible for the martian soil, including 4 (oxy)chlorine species, has been separated at flow rates ranging from 1 to 10 μL/min, requiring as little as 200 psi at 1.0 μL/min. This allowed the use of pneumatic displacement pumping from a pressurized aluminum eluent reservoir and the elimination of the high-pressure pump entirely (the single heaviest and most energy-intensive component). All ions could be separated and detected effectively from 0.5 to 100 μM, even when millimolar concentrations of perchlorate were present in the same mixtures.
Collapse
Affiliation(s)
- C Phillip Shelor
- 1 Department of Chemistry and Biochemistry, The University of Texas at Arlington , Arlington, Texas
| | | | | | | | | | | | | | | |
Collapse
|
46
|
Groemer G, Foresta L, Turetschek T, Bothe C, Boyd A, Dinkelaker A, Dissertori M, Fasching D, Fischer M, Föger D, Frischauf N, Fritsch L, Fuchs H, Gautsch C, Gerard S, Goetzloff L, Gołebiowska I, Gorur P, Groemer G, Groll P, Haider C, Haider O, Hauth E, Hauth S, Hettrich S, Jais W, Jones N, Taj-Eddine K, Karl A, Kauerhoff T, Khan MS, Kjeldsen A, Klauck J, Losiak A, Luger M, Luger T, Luger U, McArthur J, Moser L, Neuner J, Orgel C, Ori GG, Paternesi R, Peschier J, Pfeil I, Prock S, Radinger J, Ragonig C, Ramirez B, Ramo W, Rampey M, Sams A, Sams E, Sams S, Sandu O, Sans A, Sansone P, Scheer D, Schildhammer D, Scornet Q, Sejkora N, Soucek A, Stadler A, Stummer F, Stumptner W, Taraba M, Tlustos R, Toferer E, Winter E, Zanella-Kux K. A case for using ground-based thermal inertia measurements to detect Martian caves. ASTROBIOLOGY 2014; 14:431-437. [PMID: 24823802 DOI: 10.1089/ast.2013.1063] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/03/2023]
Abstract
Martian caves are regarded as one of the most interesting locations in which to search for life on the planet. Data obtained during the MARS2013 expedition at Hamar Laghdad Ridge in the Tafilalt region of Morocco indicate that even small cavities can display thermal behavior that is characteristic for caves. For example, temperature in a cavity equaled 14°C±0.1°C before sunrise, which was higher than the temperature of the ambient air (10°C±0.1°C) and proximate rocks (9°C±0.1°C) at the same time. Within 30 min after sunrise, when the temperature of surrounding rocks corresponded to 15°C, this thermal relationship reversed. Measurements were conducted under simulated spaceflight conditions, including near-real-time interpretation of data that were acquired in a complex flight planning environment. We conclude that using ground-based thermal contrast measurements, in 7-14 μm band before and after sunset, is an effective method for Mars astronauts to identify caves, possibly superior to usage of space-based or ground-penetrating data.
Collapse
Affiliation(s)
- Gernot Groemer
- 1 Austrian Space Forum, Innsbruck Office , Innsbruck, Austria
| | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | |
Collapse
|
47
|
Attenello FJ, Lee B, Yu C, Liu CY, Apuzzo ML. Supplementing the Neurosurgical Virtuoso: Evolution of Automation from Mythology to Operating Room Adjunct. World Neurosurg 2014; 81:719-29. [DOI: 10.1016/j.wneu.2014.03.011] [Citation(s) in RCA: 9] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/17/2013] [Revised: 02/25/2014] [Accepted: 03/05/2014] [Indexed: 12/01/2022]
|
48
|
Forget F, Leconte J. Possible climates on terrestrial exoplanets. PHILOSOPHICAL TRANSACTIONS. SERIES A, MATHEMATICAL, PHYSICAL, AND ENGINEERING SCIENCES 2014; 372:20130084. [PMID: 24664919 DOI: 10.1098/rsta.2013.0084] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/03/2023]
Abstract
What kind of environment may exist on terrestrial planets around other stars? In spite of the lack of direct observations, it may not be premature to speculate on exoplanetary climates, for instance, to optimize future telescopic observations or to assess the probability of habitable worlds. To begin with, climate primarily depends on (i) the atmospheric composition and the volatile inventory; (ii) the incident stellar flux; and (iii) the tidal evolution of the planetary spin, which can notably lock a planet with a permanent night side. The atmospheric composition and mass depends on complex processes, which are difficult to model: origins of volatiles, atmospheric escape, geochemistry, photochemistry, etc. We discuss physical constraints, which can help us to speculate on the possible type of atmosphere, depending on the planet size, its final distance for its star and the star type. Assuming that the atmosphere is known, the possible climates can be explored using global climate models analogous to the ones developed to simulate the Earth as well as the other telluric atmospheres in the solar system. Our experience with Mars, Titan and Venus suggests that realistic climate simulators can be developed by combining components, such as a 'dynamical core', a radiative transfer solver, a parametrization of subgrid-scale turbulence and convection, a thermal ground model and a volatile phase change code. On this basis, we can aspire to build reliable climate predictors for exoplanets. However, whatever the accuracy of the models, predicting the actual climate regime on a specific planet will remain challenging because climate systems are affected by strong positive feedbacks. They can drive planets with very similar forcing and volatile inventory to completely different states. For instance, the coupling among temperature, volatile phase changes and radiative properties results in instabilities, such as runaway glaciations and runaway greenhouse effect.
Collapse
Affiliation(s)
- F Forget
- Laboratoire de Météorologie Dynamique, IPSL, Paris, France
| | | |
Collapse
|
49
|
Archer PD, Ming DW, Sutter B. The effects of instrument parameters and sample properties on thermal decomposition: interpreting thermal analysis data from Mars. ACTA ACUST UNITED AC 2013. [DOI: 10.1186/2191-2521-2-2] [Citation(s) in RCA: 22] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
|
50
|
Abbey W, Salas E, Bhartia R, Beegle LW. The Mojave vadose zone: a subsurface biosphere analogue for Mars. ASTROBIOLOGY 2013; 13:637-646. [PMID: 23848498 DOI: 10.1089/ast.2012.0948] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/02/2023]
Abstract
If life ever evolved on the surface of Mars, it is unlikely that it would still survive there today, but as Mars evolved from a wet planet to an arid one, the subsurface environment may have presented a refuge from increasingly hostile surface conditions. Since the last glacial maximum, the Mojave Desert has experienced a similar shift from a wet to a dry environment, giving us the opportunity to study here on Earth how subsurface ecosystems in an arid environment adapt to increasingly barren surface conditions. In this paper, we advocate studying the vadose zone ecosystem of the Mojave Desert as an analogue for possible subsurface biospheres on Mars. We also describe several examples of Mars-like terrain found in the Mojave region and discuss ecological insights that might be gained by a thorough examination of the vadose zone in these specific terrains. Examples described include distributary fans (deltas, alluvial fans, etc.), paleosols overlain by basaltic lava flows, and evaporite deposits.
Collapse
Affiliation(s)
- William Abbey
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | | | | | | |
Collapse
|