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Bonaccorsi R, Glass B, Moreno-Paz M, García-Villadangos M, Warren-Rhodes K, Parro V, Manchado JM, Wilhelm MB, McKay CP. In Situ Real-Time Monitoring for Aseptic Drilling: Lessons Learned from the Atacama Rover Astrobiology Drilling Studies Contamination Control Strategy and Implementation and Application to the Icebreaker Mars Life Detection Mission. Astrobiology 2023; 23:1303-1336. [PMID: 38133823 DOI: 10.1089/ast.2022.0133] [Citation(s) in RCA: 2] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 12/23/2023]
Abstract
In 2019, the Atacama Rover Astrobiology Drilling Studies (ARADS) project field-tested an autonomous rover-mounted robotic drill prototype for a 6-Sol life detection mission to Mars (Icebreaker). ARADS drilled Mars-like materials in the Atacama Desert (Chile), one of the most life-diminished regions on Earth, where mitigating contamination transfer into life-detection instruments becomes critical. Our Contamination Control Strategy and Implementation (CCSI) for the Sample Handling and Transfer System (SHTS) hardware (drill, scoop and funnels) included out-of-simulation protocol testing (out-of-sim) for hardware decontamination and verification during the 6-Sol simulation (in-sim). The most effective five-step decontamination combined safer-to-use sterilants (3%_hydrogen-peroxide-activated 5%_sodium-hypochlorite), and in situ real-time verification by adenosine triphosphate (ATP) and Signs of Life Detector (SOLID) Fluorescence Immunoassay for characterization hardware bioburden and airborne contaminants. The 20- to 40-min protocol enabled a 4-log bioburden reduction down to <0.1 fmoles ATP detection limit (funnels and drill) to 0.2-0.7 fmoles (scoop) of total ATP. The (post-cleaning) hardware background was 0.3 to 1-2 attomoles ATP/cm2 (cleanliness benchmark background values) equivalent to ca. 1-10 colony forming unit (CFU)/cm2. Further, 60-100% of the in-sim hardware background was ≤3-4 bacterial cells/cm2, the threshold limit for Class <7 aseptic operations. Across the six Sols, the flux of airborne contaminants to the drill sites was ∼5 and ∼22 amoles ATP/(cm2·day), accounting for an unexpectedly high Fluorescence Intensity (FI) signal (FI: ∼6000) against aquatic cyanobacteria, but negligible anthropogenic contribution. The SOLID immunoassay also detected microorganisms from multiple habitats across the Atacama Desert (anoxic, alkaline/acidic microenvironments in halite fields, playas, and alluvial fans) in both airborne and post-cleaning hardware background. Finally, the hardware ATP background was 40-250 times lower than the ATP in cores. Similarly, the FI peaks (FImax) against the microbial taxa and molecular biomarkers detected in the post-cleaned hardware (FI: ∼1500-1600) were 5-10 times lower than biomarkers in drilled sediments, excluding significant interference with putative biomarker found in cores. Similar protocols enable the acquisition of contamination-free materials for ultra-sensitive instruments analysis and the integrity of scientific results. Their application can augment our scientific knowledge of the distribution of cryptic life on Mars-like grounds and support life-detection robotic and human-operated missions to Mars.
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Affiliation(s)
- Rosalba Bonaccorsi
- SETI Institute, Mountain View, California, USA
- NASA Ames Research Center, Moffett Field, California, USA
| | - Brian Glass
- NASA Ames Research Center, Moffett Field, California, USA
| | - Mercedes Moreno-Paz
- Department of Molecular Evolution, Centro de Astrobiología (INTA-CSIC), Madrid, Spain
| | | | - Kimberley Warren-Rhodes
- SETI Institute, Mountain View, California, USA
- NASA Ames Research Center, Moffett Field, California, USA
| | - Victor Parro
- Department of Molecular Evolution, Centro de Astrobiología (INTA-CSIC), Madrid, Spain
| | - Juan Manuel Manchado
- Department of Molecular Evolution, Centro de Astrobiología (INTA-CSIC), Madrid, Spain
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Wang H, Chen Y, Wang L, Liu Q, Yang S, Wang C. Advancing herbal medicine: enhancing product quality and safety through robust quality control practices. Front Pharmacol 2023; 14:1265178. [PMID: 37818188 PMCID: PMC10561302 DOI: 10.3389/fphar.2023.1265178] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/22/2023] [Accepted: 09/15/2023] [Indexed: 10/12/2023] Open
Abstract
This manuscript provides an in-depth review of the significance of quality control in herbal medication products, focusing on its role in maintaining efficiency and safety. With a historical foundation in traditional medicine systems, herbal remedies have gained widespread popularity as natural alternatives to conventional treatments. However, the increasing demand for these products necessitates stringent quality control measures to ensure consistency and safety. This comprehensive review explores the importance of quality control methods in monitoring various aspects of herbal product development, manufacturing, and distribution. Emphasizing the need for standardized processes, the manuscript delves into the detection and prevention of contaminants, the authentication of herbal ingredients, and the adherence to regulatory standards. Additionally, it highlights the integration of traditional knowledge and modern scientific approaches in achieving optimal quality control outcomes. By emphasizing the role of quality control in herbal medicine, this manuscript contributes to promoting consumer trust, safeguarding public health, and fostering the responsible use of herbal medication products.
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Affiliation(s)
- Hongting Wang
- Anhui Provincial Engineering Laboratory for Screening and Re-evaluation of Active Compounds of Herbal Medicines in Southern Anhui, Anhui Provincial Engineering Research Center for Polysaccharide Drugs, Anhui Innovative Center for Drug Basic Research of Metabolic Diseases, School of Pharmacy, Wannan Medical College, Wuhu, China
| | | | | | | | | | - Cunqin Wang
- Anhui Provincial Engineering Laboratory for Screening and Re-evaluation of Active Compounds of Herbal Medicines in Southern Anhui, Anhui Provincial Engineering Research Center for Polysaccharide Drugs, Anhui Innovative Center for Drug Basic Research of Metabolic Diseases, School of Pharmacy, Wannan Medical College, Wuhu, China
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3
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Royle SH, Cropper L, Watson JS, Sinibaldi S, Entwisle M, Sephton MA. Solid-Phase Microextraction for Organic Contamination Control Throughout Assembly and Operational Phases of Space Missions. Astrobiology 2023; 23:127-143. [PMID: 36473197 DOI: 10.1089/ast.2021.0030] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/17/2023]
Abstract
Space missions concerned with life detection contain highly sensitive instruments for the detection of organics. Terrestrial contamination can interfere with signals of indigenous organics in samples and has the potential to cause false-positive biosignature detections, which may lead to incorrect suggestions of the presence of life elsewhere in the solar system. This study assessed the capability of solid-phase microextraction (SPME) as a method for monitoring organic contamination encountered by spacecraft hardware during assembly and operation. SPME-gas chromatography-mass spectrometry (SPME-GC-MS) analysis was performed on potential contaminant source materials, which are commonly used in spacecraft construction. The sensitivity of SPME-GC-MS to organics was assessed in the context of contaminants identified in molecular wipes taken from hardware surfaces on the ExoMars Rosalind Franklin rover. SPME was found to be effective at detecting a wide range of common organic contaminants that include aromatic hydrocarbons, aliphatic hydrocarbons, nitrogen-containing compounds, alcohols, and carbonyls. A notable example of correlation of contaminant with source material was the detection of benzenamine compounds in an epoxy adhesive analyzed by SPME-GC-MS and in the ExoMars rover surface wipe samples. The current form of SPME-GC-MS does not enable quantitative evaluation of contaminants, nor is it suitable for the detection of every group of organic molecules relevant to astrobiological contamination concerns, namely large and/or polar molecules such as amino acids. However, it nonetheless represents an effective new monitoring method for rapid, easy identification of organic contaminants commonly present on spacecraft hardware and could thus be utilized in future space missions as part of their contamination control and mitigation protocols.
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Affiliation(s)
- Samuel H Royle
- Department of Earth Science and Engineering, Imperial College London, London, United Kingdom
| | - Lorcan Cropper
- Department of Earth Science and Engineering, Imperial College London, London, United Kingdom
| | - Jonathan S Watson
- Department of Earth Science and Engineering, Imperial College London, London, United Kingdom
| | | | | | - Mark A Sephton
- Department of Earth Science and Engineering, Imperial College London, London, United Kingdom
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Pavlov AA, McLain HL, Glavin DP, Roussel A, Dwork In JP, Elsila JE, Yocum KM. Rapid Radiolytic Degradation of Amino Acids in the Martian Shallow Subsurface: Implications for the Search for Extinct Life. Astrobiology 2022; 22:1099-1115. [PMID: 35749703 DOI: 10.1089/ast.2021.0166] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/15/2023]
Abstract
Amino acids are fundamental to life as we know them as the monomers of proteins and enzymes. They are also readily synthesized under a variety of plausible prebiotic conditions and are common in carbon-rich meteorites. Thus, they represent a reasonable class of organics to target in the search for prebiotic chemistry or chemical evidence of life on Mars. However, regardless of their origin, amino acids and other organic molecules present in near-surface regolith and rocks on Mars can be degraded by exposure to cosmic rays that can penetrate to a depth of a few meters. We exposed several pure amino acids in dry and hydrated silicate mixtures and in mixtures of silicates with perchlorate salts to gamma radiation at various temperatures and radiation doses representative of the martian near-subsurface. We found that irradiation of amino acids mixed with dry silica powder increased the rate of amino acid radiolysis, with the radiolysis constants of amino acids in silicate mixtures at least a factor of 10 larger compared with the radiolysis constants of amino acids alone. The addition of perchlorate salts to the silicate samples or hydration of silicate samples further accelerated the rate of amino acid destruction during irradiation and increased the radiolysis constants by a factor of ∼1.5. Our results suggest that even low-molecular-weight amino acids could degrade in just ∼20 million years in the top 10 cm of the martian surface regolith and rock, and even faster if the material contains elevated abundances of hydrated silicate minerals or perchlorates. We did not detect evidence of amino acid racemization after gamma radiation exposure of the samples, which indicates that the chirality of some surviving amino acids may still be preserved. Our experimental results suggest serious challenges for the search of ancient amino acids and other potential organic biosignatures in the top 2 m of the martian surface.
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Affiliation(s)
- Alexander A Pavlov
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| | - Hannah L McLain
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
- Department of Physics, Catholic University of America, Washington, District of Columbia, USA
- Center for Research and Exploration in Space Science and Technology, NASA/GSFC, Greenbelt, Maryland, USA
| | - Daniel P Glavin
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| | - Anaïs Roussel
- Department of Biology, Georgetown University, Washington, District of Columbia, USA
| | - Jason P Dwork In
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| | - Jamie E Elsila
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
| | - Katarina M Yocum
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
- Department of Chemistry, University of Wisconsin-Madison, Madison, Wisconsin, USA
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5
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Lymer EA, Konstantinidis M, Lalla EA, Daly MG, Tait KT. UV Time-Resolved Laser-Induced Fluorescence Spectroscopy of Amino Acids Found in Meteorites: Implications for Space Science and Exploration. Astrobiology 2021; 21:1350-1362. [PMID: 34314603 DOI: 10.1089/ast.2021.0006] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/13/2023]
Abstract
Laser-induced fluorescence spectroscopy is a useful laboratory and in situ technique for planetary exploration, with applications in biosignature detection and the search for life on Mars. However, little work has been completed on the utility of fluorescence spectroscopy techniques on asteroid relevant material. In preparation for asteroid sample return missions such as NASA's OSIRIS-REx and JAXA's Hayabusa2, we conducted UV time resolved laser-induced fluorescence spectroscopy (TR-LIF) analysis of 10 amino acids, all of which have been found in the carbonaceous meteorites Murchison and Allende. We present the calculation of decay rates of each amino acid (1.55-3.56 ns) and compare with those of relevant homogeneous minerals (15-70 ns). Moreover, we demonstrate a linear relationship between calculated lifetimes and elemental abundance of nitrogen and carbon (p < 0.025). The quantitative and qualitative fluorescence analyses presented in this work will lead to more reliable identification of organic material within meteorites and asteroids in a time-efficient, minimally destructive way.
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Affiliation(s)
- Elizabeth A Lymer
- Centre for Research in Earth and Space Science, York University, Toronto, Canada
| | - Menelaos Konstantinidis
- Centre for Research in Earth and Space Science, York University, Toronto, Canada
- Dalla Lana School of Public Health, University of Toronto, Toronto, Canada
| | - Emmanuel A Lalla
- Centre for Research in Earth and Space Science, York University, Toronto, Canada
| | - Michael G Daly
- Centre for Research in Earth and Space Science, York University, Toronto, Canada
| | - Kimberly T Tait
- Department of Natural History, Centre for Applied Planetary Mineralogy, Royal Ontario Museum, Toronto, Canada
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6
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Regberg AB, Castro CL, Connolly HC, Davis RE, Dworkin JP, Lauretta DS, Messenger SR, Mclain HL, McCubbin FM, Moore JL, Righter K, Stahl-Rommel S, Castro-Wallace SL. Prokaryotic and Fungal Characterization of the Facilities Used to Assemble, Test, and Launch the OSIRIS-REx Spacecraft. Front Microbiol 2020; 11:530661. [PMID: 33250861 PMCID: PMC7676328 DOI: 10.3389/fmicb.2020.530661] [Citation(s) in RCA: 4] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/29/2020] [Accepted: 09/30/2020] [Indexed: 01/04/2023] Open
Abstract
To characterize the ATLO (Assembly, Test, and Launch Operations) environment of the OSIRIS-REx spacecraft, we analyzed 17 aluminum witness foils and two blanks for bacterial, archaeal, fungal, and arthropod DNA. Under NASA’s Planetary Protection guidelines, OSIRIS-REx is a Category II outbound, Category V unrestricted sample return mission. As a result, it has no bioburden restrictions. However, the mission does have strict organic contamination requirements to achieve its primary objective of returning pristine carbonaceous asteroid regolith to Earth. Its target, near-Earth asteroid (101955) Bennu, is likely to contain organic compounds that are biologically available. Therefore, it is useful to understand what organisms were present during ATLO as part of the larger contamination knowledge effort—even though it is unlikely that any of the organisms will survive the multi-year deep space journey. Even though these samples of opportunity were not collected or preserved for DNA analysis, we successfully amplified bacterial and archaeal DNA (16S rRNA gene) from 16 of the 17 witness foils containing as few as 7 ± 3 cells per sample. Fungal DNA (ITS1) was detected in 12 of the 17 witness foils. Despite observing arthropods in some of the ATLO facilities, arthropod DNA (COI gene) was not detected. We observed 1,009 bacterial and archaeal sOTUs (sub-operational taxonomic units, 100% unique) and 167 fungal sOTUs across all of our samples (25–84 sOTUs per sample). The most abundant bacterial sOTU belonged to the genus Bacillus. This sOTU was present in blanks and may represent contamination during sample handling or storage. The sample collected from inside the fairing just prior to launch contained several unique bacterial and fungal sOTUs that describe previously uncharacterized potential for contamination during the final phase of ATLO. Additionally, fungal richness (number of sOTUs) negatively correlates with the number of carbon-bearing particles detected on samples. The total number of fungal sequences positively correlates with total amino acid concentration. These results demonstrate that it is possible to use samples of opportunity to characterize the microbiology of low-biomass environments while also revealing the limitations imposed by sample collection and preservation methods not specifically designed with biology in mind.
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Affiliation(s)
- Aaron B Regberg
- Astromaterials Research and Exploration Science Division, National Aeronautics and Space Administration (NASA) Johnson Space Center, Houston TX, United States
| | | | - Harold C Connolly
- Department of Geology, Rowan University, Glassboro, NJ, United States.,Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, United States
| | - Richard E Davis
- Jacobs@NASA/Johnson Space Center, Houston, TX, United States
| | - Jason P Dworkin
- Astrochemistry Laboratory, Goddard Space Flight Center, Greenbelt, MD, United States
| | - Dante S Lauretta
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, United States
| | - Scott R Messenger
- Astromaterials Research and Exploration Science Division, National Aeronautics and Space Administration (NASA) Johnson Space Center, Houston TX, United States
| | - Hannah L Mclain
- Astrochemistry Laboratory, Goddard Space Flight Center, Greenbelt, MD, United States
| | - Francis M McCubbin
- Astromaterials Research and Exploration Science Division, National Aeronautics and Space Administration (NASA) Johnson Space Center, Houston TX, United States
| | - Jamie L Moore
- Lockheed Martin Space Systems, Littleton, CO, United States
| | - Kevin Righter
- Astromaterials Research and Exploration Science Division, National Aeronautics and Space Administration (NASA) Johnson Space Center, Houston TX, United States
| | | | - Sarah L Castro-Wallace
- Biomedical Research and Environmental Sciences Division, Johnson Space Center, Houston, TX, United States
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7
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Chan QHS, Stroud R, Martins Z, Yabuta H. Concerns of Organic Contamination for Sample Return Space Missions. Space Sci Rev 2020; 216:56. [PMID: 32624626 PMCID: PMC7319412 DOI: 10.1007/s11214-020-00678-7] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 06/27/2019] [Accepted: 04/23/2020] [Indexed: 06/11/2023]
Abstract
Analysis of organic matter has been one of the major motivations behind solar system exploration missions. It addresses questions related to the organic inventory of our solar system and its implication for the origin of life on Earth. Sample return missions aim at returning scientifically valuable samples from target celestial bodies to Earth. By analysing the samples with the use of state-of-the-art analytical techniques in laboratories here on Earth, researchers can address extremely complicated aspects of extra-terrestrial organic matter. This level of detailed sample characterisation provides the range and depth in organic analysis that are restricted in spacecraft-based exploration missions, due to the limitations of the on-board in-situ instrumentation capabilities. So far, there are four completed and in-process sample return missions with an explicit mandate to collect organic matter: Stardust and OSIRIS-REx missions of NASA, and Hayabusa and Hayabusa2 missions of JAXA. Regardless of the target body, all sample return missions dedicate to minimise terrestrial organic contamination of the returned samples, by applying various degrees or strategies of organic contamination mitigation methods. Despite the dedicated efforts in the design and execution of contamination control, it is impossible to completely eliminate sources of organic contamination. This paper aims at providing an overview of the successes and lessons learned with regards to the identification of indigenous organic matter of the returned samples vs terrestrial contamination.
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Affiliation(s)
- Queenie Hoi Shan Chan
- Planetary and Space Sciences, School of Physical Sciences, The Open University, Walton Hall, Milton Keynes, MK7 6AA UK
- Present Address: Department of Earth Sciences, Royal Holloway University of London, Egham Surrey, TW20 0EX UK
| | - Rhonda Stroud
- Code 6360, Naval Research Laboratory, Washington, DC 20375 USA
| | - Zita Martins
- Centro de Química Estrutural, Departamento de Engenharia Química, Instituto Superior Técnico (IST), Universidade de Lisboa, Avenida Rovisco Pais 1, 1049-001 Lisbon, Portugal
| | - Hikaru Yabuta
- Department of Earth and Planetary Systems Science, Hiroshima University, 1-3-1 Kagamiyama, Hiroshima, 739-8526 Japan
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Uesugi M, Hirahara K, Uesugi K, Takeuchi A, Karouji Y, Shirai N, Ito M, Tomioka N, Ohigashi T, Yamaguchi A, Imae N, Yada T, Abe M. Development of a sample holder for synchrotron radiation-based computed tomography and diffraction analysis of extraterrestrial materials. Rev Sci Instrum 2020; 91:035107. [PMID: 32259948 DOI: 10.1063/1.5122672] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/02/2019] [Accepted: 02/11/2020] [Indexed: 06/11/2023]
Abstract
A sample holder for a suite of synchrotron radiation measurements on extraterrestrial materials, which are fragile and irregularly shaped, was developed using carbon nanotubes and polyimide. The holder enables investigation of such samples with multiple analytical instruments, which means that we can reduce the number of sample transfers between holders. The holder developed in our study also enables investigation of such samples without exposure to the terrestrial atmosphere, which contains abundant contaminants, such as water vapor and organic substances. The stability of the samples in the holder during the measurements and disturbance of the analysis result by the holder were evaluated, which showed that sample drift motion and image disturbance due to x-ray attenuation and scattering of the holder materials are insignificant.
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Affiliation(s)
- Masayuki Uesugi
- Japan Synchrotron Radiation Research Institute (JASRI/SPring-8), 1-1-1 Kouto, Sayo, Hyogo 679-5198, Japan
| | - Kaori Hirahara
- Department Mechanical Engineering and Center for Atomic and Molecular Technology, Osaka University, 2-1 Yamadaoka, Suita, Osaka 565-0871, Japan
| | - Kentaro Uesugi
- Japan Synchrotron Radiation Research Institute (JASRI/SPring-8), 1-1-1 Kouto, Sayo, Hyogo 679-5198, Japan
| | - Akihisa Takeuchi
- Japan Synchrotron Radiation Research Institute (JASRI/SPring-8), 1-1-1 Kouto, Sayo, Hyogo 679-5198, Japan
| | - Yuzuru Karouji
- JAXA Space Exploration Center, Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Sagamihara, Kanagawa 252-5210, Japan
| | - Naoki Shirai
- Department of Chemistry, Graduate School of Science, Tokyo Metropolitan University, Hachioji, Tokyo 192-0397, Japan
| | - Motoo Ito
- Kochi Institute for Core Sample Research, Japan Agency for Marine-Earth Science Technology (JAMSTEC), 200 Monobe Otsu, Nankoku, Kochi 783-8502, Japan
| | - Naotaka Tomioka
- Kochi Institute for Core Sample Research, Japan Agency for Marine-Earth Science Technology (JAMSTEC), 200 Monobe Otsu, Nankoku, Kochi 783-8502, Japan
| | - Takuji Ohigashi
- UVSOR Facility, Institute for Molecular Science, 38 Nishigo-Naka, Myodaiji, Okazaki 444-8585, Japan
| | - Akira Yamaguchi
- Antarctic Meteorite Research Center, National Institute of Polar Research, Tokyo 173-8515, Japan
| | - Naoya Imae
- Antarctic Meteorite Research Center, National Institute of Polar Research, Tokyo 173-8515, Japan
| | - Toru Yada
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1, Yoshinodai, Sagamihara, Kanagawa 252-5210, Japan
| | - Masanao Abe
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1, Yoshinodai, Sagamihara, Kanagawa 252-5210, Japan
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Golish DR, Drouet d'Aubigny C, Rizk B, DellaGiustina DN, Smith PH, Becker K, Shultz N, Stone T, Barker MK, Mazarico E, Tatsumi E, Gaskell RW, Harrison L, Merrill C, Fellows C, Williams B, O'Dougherty S, Whiteley M, Hancock J, Clark BE, Hergenrother CW, Lauretta DS. Ground and In-Flight Calibration of the OSIRIS-REx Camera Suite. Space Sci Rev 2020; 216:12. [PMID: 32025061 DOI: 10.1007/s11214-017-0460-7] [Citation(s) in RCA: 20] [Impact Index Per Article: 5.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/18/2019] [Accepted: 11/27/2019] [Indexed: 05/29/2023]
Abstract
The OSIRIS-REx Camera Suite (OCAMS) onboard the OSIRIS-REx spacecraft is used to study the shape and surface of the mission's target, asteroid (101955) Bennu, in support of the selection of a sampling site. We present calibration methods and results for the three OCAMS cameras-MapCam, PolyCam, and SamCam-using data from pre-flight and in-flight calibration campaigns. Pre-flight calibrations established a baseline for a variety of camera properties, including bias and dark behavior, flat fields, stray light, and radiometric calibration. In-flight activities updated these calibrations where possible, allowing us to confidently measure Bennu's surface. Accurate calibration is critical not only for establishing a global understanding of Bennu, but also for enabling analyses of potential sampling locations and for providing scientific context for the returned sample.
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Affiliation(s)
- D R Golish
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | | | - B Rizk
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | - D N DellaGiustina
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | - P H Smith
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | - K Becker
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | - N Shultz
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | - T Stone
- United States Geological Survey Astrogeology Science Center, Flagstaff, AZ USA
| | - M K Barker
- 3Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD USA
| | - E Mazarico
- 3Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD USA
| | - E Tatsumi
- 4Department of Earth and Planetary Science, The University of Tokyo, Tokyo, Japan
| | - R W Gaskell
- 5Planetary Science Institute, Tucson, AZ USA
| | - L Harrison
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | - C Merrill
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | - C Fellows
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | - B Williams
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | - S O'Dougherty
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | - M Whiteley
- 6Space Dynamics Laboratory, Utah State University, Logan, UT USA
| | - J Hancock
- 6Space Dynamics Laboratory, Utah State University, Logan, UT USA
| | - B E Clark
- 7Department of Physics and Astronomy, Ithaca College, Ithaca, NY USA
| | - C W Hergenrother
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
| | - D S Lauretta
- 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ USA
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10
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Glavin DP, Burton AS, Elsila JE, Aponte JC, Dworkin JP. The Search for Chiral Asymmetry as a Potential Biosignature in our Solar System. Chem Rev 2019; 120:4660-4689. [DOI: 10.1021/acs.chemrev.9b00474] [Citation(s) in RCA: 88] [Impact Index Per Article: 17.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/07/2023]
Affiliation(s)
- Daniel P. Glavin
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, United States
| | - Aaron S. Burton
- NASA Johnson Space Center, Houston, Texas 77058, United States
| | - Jamie E. Elsila
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, United States
| | - José C. Aponte
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, United States
- Catholic University of America, Washington, D.C. 20064, United States
| | - Jason P. Dworkin
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, United States
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Royle SH, Watson JS, Zhang Y, Chatzitheoklitos G, Sephton MA. Solid Phase Micro Extraction: Potential for Organic Contamination Control for Planetary Protection of Life-Detection Missions to the Icy Moons of the Outer Solar System. Astrobiology 2019; 19:1153-1166. [PMID: 31216175 DOI: 10.1089/ast.2018.1968] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/09/2023]
Abstract
Conclusively detecting, or ruling out the possibility of, life on the icy moons of the outer Solar System will require spacecraft missions to undergo rigorous planetary protection and contamination control procedures to achieve extremely low levels of organic terrestrial contamination. Contamination control is necessary to avoid forward contamination of the body of interest and to avoid the detection of false-positive signals, which could either mask indigenous organic chemistry of interest or cause an astrobiological false alarm. Here we test a new method for rapidly and inexpensively assessing the organic cleanliness of spaceflight hardware surfaces using solid phase micro extraction (SPME) fibers to directly swab surfaces. The results suggest that the method is both time and cost efficient. The SPME-gas chromatography-mass spectrometry (SPME-GC-MS) method is sensitive to common midweight, nonpolar contaminant compounds, for example, aliphatic and aromatic hydrocarbons, which are common contaminants in laboratory settings. While we demonstrate the potential of SPME for surface sampling, the GC-MS instrumentation restricts the SPME-GC-MS technique's sensitivity to larger polar and nonvolatile compounds. Although not used in this study, to increase the potential range of detectable compounds, SPME can also be used in conjunction with high-performance liquid chromatography/liquid chromatography-mass spectrometry systems suitable for polar analytes (Kataoka et al., 2000). Thus, our SPME method presents an opportunity to monitor organic contamination in a relatively rapid and routine way that produces information-rich data sets.
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Affiliation(s)
- Samuel H Royle
- Impacts and Astromaterials Research Centre, Earth Science and Engineering, South Kensington Campus, Imperial College London, London, UK
| | - Jonathan S Watson
- Impacts and Astromaterials Research Centre, Earth Science and Engineering, South Kensington Campus, Imperial College London, London, UK
| | - Yuting Zhang
- Impacts and Astromaterials Research Centre, Earth Science and Engineering, South Kensington Campus, Imperial College London, London, UK
| | - Georgios Chatzitheoklitos
- Impacts and Astromaterials Research Centre, Earth Science and Engineering, South Kensington Campus, Imperial College London, London, UK
| | - Mark A Sephton
- Impacts and Astromaterials Research Centre, Earth Science and Engineering, South Kensington Campus, Imperial College London, London, UK
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Simkus DN, Aponte JC, Elsila JE, Parker ET, Glavin DP, Dworkin JP. Methodologies for Analyzing Soluble Organic Compounds in Extraterrestrial Samples: Amino Acids, Amines, Monocarboxylic Acids, Aldehydes, and Ketones. Life (Basel) 2019; 9:E47. [PMID: 31174308 PMCID: PMC6617175 DOI: 10.3390/life9020047] [Citation(s) in RCA: 17] [Impact Index Per Article: 3.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/04/2019] [Revised: 05/18/2019] [Accepted: 05/27/2019] [Indexed: 11/19/2022] Open
Abstract
Soluble organic compositions of extraterrestrial samples offer valuable insights into the prebiotic organic chemistry of the solar system. This review provides a summary of the techniques commonly used for analyzing amino acids, amines, monocarboxylic acids, aldehydes, and ketones in extraterrestrial samples. Here, we discuss possible effects of various experimental factors (e.g., extraction protocols, derivatization methods, and chromatographic techniques) in order to highlight potential influences on the results obtained from different methodologies. This detailed summary and assessment of current techniques is intended to serve as a basic guide for selecting methodologies for soluble organic analyses and to emphasize some key considerations for future method development.
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Affiliation(s)
- Danielle N Simkus
- NASA Postdoctoral Program at NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
| | - José C Aponte
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
- Department of Chemistry, Catholic University of America, Washington, D.C. 20064, USA.
| | - Jamie E Elsila
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
| | - Eric T Parker
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
| | - Daniel P Glavin
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
| | - Jason P Dworkin
- Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
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Mogul R, Barding GA, Lalla S, Lee S, Madrid S, Baki R, Ahmed M, Brasali H, Cepeda I, Gornick T, Gunadi S, Hearn N, Jain C, Kim EJ, Nguyen T, Nguyen VB, Oei A, Perkins N, Rodriguez J, Rodriguez V, Savla G, Schmitz M, Tedjakesuma N, Walker J. Metabolism and Biodegradation of Spacecraft Cleaning Reagents by Strains of Spacecraft-Associated Acinetobacter. Astrobiology 2018; 18:1517-1527. [PMID: 29672134 PMCID: PMC6276816 DOI: 10.1089/ast.2017.1814] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/30/2017] [Accepted: 03/23/2018] [Indexed: 05/17/2023]
Abstract
Spacecraft assembly facilities are oligotrophic and low-humidity environments, which are routinely cleaned using alcohol wipes for benchtops and spacecraft materials, and alkaline detergents for floors. Despite these cleaning protocols, spacecraft assembly facilities possess a persistent, diverse, dynamic, and low abundant core microbiome, where the Acinetobacter are among the dominant members of the community. In this report, we show that several spacecraft-associated Acinetobacter metabolize or biodegrade the spacecraft cleaning reagents of ethanol (ethyl alcohol), 2-propanol (isopropyl alcohol), and Kleenol 30 (floor detergent) under ultraminimal conditions. Using cultivation and stable isotope labeling studies, we show that ethanol is a sole carbon source when cultivating in 0.2 × M9 minimal medium containing 26 μM Fe(NH4)2(SO4)2. Although cultures expectedly did not grow solely on 2-propanol, cultivations on mixtures of ethanol and 2-propanol exhibited enhanced plate counts at mole ratios of ≤0.50. In support, enzymology experiments on cellular extracts were consistent with oxidation of ethanol and 2-propanol by a membrane-bound alcohol dehydrogenase. In the presence of Kleenol 30, untargeted metabolite profiling on ultraminimal cultures of Acinetobacter radioresistens 50v1 indicated (1) biodegradation of Kleenol 30 into products including ethylene glycols, (2) the potential metabolism of decanoate (formed during incubation of Kleenol 30 in 0.2 × M9), and (3) decreases in the abundances of several hydroxy- and ketoacids in the extracellular metabolome. In ultraminimal medium (when using ethanol as a sole carbon source), A. radioresistens 50v1 also exhibits a remarkable survival against hydrogen peroxide (∼1.5-log loss, ∼108 colony forming units (cfu)/mL, 10 mM H2O2), indicating a considerable tolerance toward oxidative stress under nutrient-restricted conditions. Together, these results suggest that the spacecraft cleaning reagents may (1) serve as nutrient sources under oligotrophic conditions and (2) sustain extremotolerances against the oxidative stresses associated with low-humidity environments. In perspective, this study provides a plausible biochemical rationale to the observed microbial ecology dynamics of spacecraft-associated environments.
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Affiliation(s)
- Rakesh Mogul
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Gregory A. Barding
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Sidharth Lalla
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Sooji Lee
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Steve Madrid
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Ryan Baki
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Mahjabeen Ahmed
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Hania Brasali
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Ivonne Cepeda
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Trevor Gornick
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Shawn Gunadi
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Nicole Hearn
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Chirag Jain
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Eun Jin Kim
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Thi Nguyen
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Vinh Bao Nguyen
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Alex Oei
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Nicole Perkins
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Joseph Rodriguez
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Veronica Rodriguez
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Gautam Savla
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Megan Schmitz
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Nicholas Tedjakesuma
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
| | - Jillian Walker
- Chemistry and Biochemistry Department, California State Polytechnic University, Pomona (Cal Poly Pomona), Pomona, California
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Sugahara H, Meinert C, Nahon L, Jones NC, Hoffmann SV, Hamase K, Takano Y, Meierhenrich UJ. d-Amino acids in molecular evolution in space - Absolute asymmetric photolysis and synthesis of amino acids by circularly polarized light. Biochim Biophys Acta Proteins Proteom 2018; 1866:743-758. [PMID: 29357311 DOI: 10.1016/j.bbapap.2018.01.004] [Citation(s) in RCA: 22] [Impact Index Per Article: 3.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/06/2017] [Revised: 12/22/2017] [Accepted: 01/05/2018] [Indexed: 02/02/2023]
Abstract
Living organisms on the Earth almost exclusively use l-amino acids for the molecular architecture of proteins. The biological occurrence of d-amino acids is rare, although their functions in various organisms are being gradually understood. A possible explanation for the origin of biomolecular homochirality is the delivery of enantioenriched molecules via extraterrestrial bodies, such as asteroids and comets on early Earth. For the asymmetric formation of amino acids and their precursor molecules in interstellar environments, the interaction with circularly polarized photons is considered to have played a potential role in causing chiral asymmetry. In this review, we summarize recent progress in the investigation of chirality transfer from chiral photons to amino acids involving the two major processes of asymmetric photolysis and asymmetric synthesis. We will discuss analytical data on cometary and meteoritic amino acids and their potential impact delivery to the early Earth. The ongoing and future ambitious space missions, Hayabusa2, OSIRIS-REx, ExoMars 2020, and MMX, are scheduled to provide new insights into the chirality of extraterrestrial organic molecules and their potential relation to the terrestrial homochirality. This article is part of a Special Issue entitled: d-Amino acids: biology in the mirror, edited by Dr. Loredano Pollegioni, Dr. Jean-Pierre Mothet and Dr. Molla Gianluca.
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Affiliation(s)
- Haruna Sugahara
- Institut de Chimie de Nice, Université Côte d'Azur, CNRS, UMR 7272, 06108 Nice, France
| | - Cornelia Meinert
- Institut de Chimie de Nice, Université Côte d'Azur, CNRS, UMR 7272, 06108 Nice, France
| | - Laurent Nahon
- L'Orme des Merisiers, Synchrotron SOLEIL, BP 48 Saint Aubin, 91192 Gif-sur-Yvette, France
| | - Nykola C Jones
- ISA, Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark
| | - Søren V Hoffmann
- ISA, Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark
| | - Kenji Hamase
- Graduate School of Pharmaceutical Sciences, Kyushu University, Fukuoka, Japan
| | - Yoshinori Takano
- Department of Biogeochemistry, Japan Agency for Marine-Earth Science and Technology (JAMSTEC), 2-15 Natsushima, Yokosuka, Kanagawa 237-0061, Japan
| | - Uwe J Meierhenrich
- Institut de Chimie de Nice, Université Côte d'Azur, CNRS, UMR 7272, 06108 Nice, France.
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