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Artykuły w czasopismach na temat „Extraterrestrial material analyses”

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Data publikacji: 8 czerwca 2024

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1

Dartois, Emmanuel, Ivan Alata, Cécile Engrand, et al. "Interstellar and interplanetary solids in the laboratory." Proceedings of the International Astronomical Union 11, A29B (2015): 416–19. http://dx.doi.org/10.1017/s1743921316005688.

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AbstractThe composition of interstellar matter is driven by environmental parameters and results from extreme interstellar medium physico-chemical conditions. Astrochemists must rely on remote observations to monitor and analyze the interstellar solids composition. They bring additional information from the study of analogues produced in the laboratory, placed in simulated space environments. Planetologists and cosmochemists access and spectroscopically examine collected extraterrestrial material in the laboratory. Diffuse interstellar medium and molecular clouds observations set constraints o

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2

Sighinolfi, Gian Paolo, Maurizio Barbieri, Daniele Brunelli, and Romano Serra. "Mineralogical and Chemical Investigations of the Amguid Crater (Algeria): Is there Evidence on an Impact Origin?" Geosciences 10, no. 3 (2020): 107. http://dx.doi.org/10.3390/geosciences10030107.

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Mineralogical and chemical investigations were carried out on intra-craterial bedrocks (Lower Devonian sandstone) and regolithic residual soil deposits present around the Amguid structure, to discuss the hypothesis of its formation through a relatively recent (about 0.1 Ma) impact event. Observations with an optical microscope on intra-craterial rocks do not unequivocally confirm the presence of impact correlated microscopic planar deformation features (PDFs) in quartz crystals. Field observations, and optical and instrumental analysis (Raman spectroscopy) on rocks and soils (including differe

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3

Isnard, R., A. Bardyn, N. Fray, et al. "H/C elemental ratio of the refractory organic matter in cometary particles of 67P/Churyumov-Gerasimenko." Astronomy & Astrophysics 630 (September 20, 2019): A27. http://dx.doi.org/10.1051/0004-6361/201834797.

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Context. Because comets are part of the most primitive bodies of our solar system, establishing their chemical composition and comparing them to other astrophysical bodies gives new constraints on the formation and evolution of organic matter throughout the solar system. For two years, the time-of-flight secondary ion mass spectrometer COmetary Secondary Ion Mass Analyzer (COSIMA) on board the Rosetta orbiter performed in situ analyses of the dust particles ejected from comet 67P/Churyumov-Gerasimenko (67P). Aims. The aim is to determine the H/C elemental ratio of the refractory organic compon

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4

Surkov, Yu A. "Analysis of extraterrestrial materials." TrAC Trends in Analytical Chemistry 6, no. 4 (1987): XXII. http://dx.doi.org/10.1016/0165-9936(87)87043-7.

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Albee, Arden L. "The Analysis of Extraterrestrial Materials." Eos, Transactions American Geophysical Union 69, no. 25 (1988): 670. http://dx.doi.org/10.1029/88eo00227.

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Lovering, John F. "The Analysis of Extraterrestrial Materials." Geochimica et Cosmochimica Acta 50, no. 12 (1986): 2865. http://dx.doi.org/10.1016/0016-7037(86)90234-6.

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7

Esposito, Madison, Kevin Souhrada, Erin Garland, et al. "Characterization of Potential Micrometeorites by Synchrotron Analysis." Geosciences 10, no. 7 (2020): 275. http://dx.doi.org/10.3390/geosciences10070275.

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Micrometeorites (MMs) are small particles that account for most of the extraterrestrial material deposited on Earth. Synchrotron X-ray fluorescence and diffraction allowed for chemical and mineral characterization to distinguish MM from atmospheric particulate. The relative components of iron, nickel, and other elements were considered in the identification of ferrous MM while high amounts of titanium were considered an indication that the particles were of atmospheric origin. Out of 100 samples collected by high school students and teachers, eight were taken to a synchrotron for analysis. Of

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8

Naraoka, Hashiguchi, Sato, and Hamase. "New Applications of High-Resolution Analytical Methods to Study Trace Organic Compounds in Extraterrestrial Materials." Life 9, no. 3 (2019): 62. http://dx.doi.org/10.3390/life9030062.

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Organic compounds are present as complex mixtures in extraterrestrial materials including meteorites, which may have played important roles in the origin of life on the primitive Earth. However, the distribution and formation mechanisms of meteoritic organic compounds are not well understood, because conventional analytical methods have limited resolution and sensitivity to resolve their molecular complexity. In this study, advanced instrumental development and analyses are proposed in order to study the trace organic compounds of extraterrestrial materials: (1) a clean room environment to avo

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9

MacPherson, G. J., and M. H. Thiemens. "Cosmochemistry: Understanding the Solar System through analysis of extraterrestrial materials." Proceedings of the National Academy of Sciences 108, no. 48 (2011): 19130–34. http://dx.doi.org/10.1073/pnas.1111493108.

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Blake, D. F., T. W. Reilly, D. E. Brownlee, and T. E. Bunch. "Low voltage scanning electron microscopy of interplanetary dust particles." Proceedings, annual meeting, Electron Microscopy Society of America 45 (August 1987): 208–9. http://dx.doi.org/10.1017/s0424820100125944.

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Interplanetary Dust Particles (IDPs) are a relatively new class of extraterrestrial materials which are collected by high-flying aircraft in the stratosphere. The particles, ∼1.0-50 μm in size, enter the earth's atmosphere at ballistic velocities, but are sufficiently small to be decelerated without burning up. IDPs commonly have solar elemental abundances, and are thoughfto have undergone very little differentiation since the formation of the solar system. While these materials are called “particles,” they are in fact aggregates of a variety of mineral phases, glass, and carbonaceous material

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11

Bose, Maitrayee. "Light Element Analysis in Extraterrestrial Materials using Secondary Ion Mass Spectrometry." Microscopy and Microanalysis 27, S1 (2021): 2882–83. http://dx.doi.org/10.1017/s1431927621010047.

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12

Chifang, Chai. "Neutron Activation Analysis of Platinum Group Elements as Indicators of Extraterrestrial Materials." Isotopenpraxis Isotopes in Environmental and Health Studies 24, no. 7 (1988): 257–72. http://dx.doi.org/10.1080/10256018808623970.

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13

Terada, K., and Y. Sano. "In situ U–Pb dating and REE analyses of phosphates in extraterrestrial materials." Applied Surface Science 203-204 (January 2003): 810–13. http://dx.doi.org/10.1016/s0169-4332(02)00831-0.

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14

Kebukawa, Yoko, Mehmet Yesiltas, and Timothy D. Glotch. "Analytical Techniques for Identification and Characterization of Extraterrestrial Organic Matter." Elements 20, no. 1 (2024): 38–44. http://dx.doi.org/10.2138/gselements.20.1.38.

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Advances in analytical techniques are essential for understanding the nature, formation, and evolutionary history of extraterrestrial organic matter. In this chapter, we briefly review analytical techniques used to detect and characterize organic matter in extraterrestrial materials. Mass spectrometry is often coupled with gas chromatography or liquid chromatography for elemental and isotopic analysis, and for identifying specific organic compounds. Spectroscopy involves interaction of molecules with electromagnetic radiation at various wavelengths. Almost every wavelength—from X-rays to radio

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15

McDonnell, J. A. M. "Extraterrestrial material analysis: Achievements and future opportunities for laboratory analysis in NASA and ESA planetary programmes." Advances in Space Research 6, no. 7 (1986): 21–32. http://dx.doi.org/10.1016/0273-1177(86)90206-1.

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16

McGee, James J., and Klaus Keil. "Application of Electron Probe Microanalysis to the Study of Geological and Planetary Materials." Microscopy and Microanalysis 7, no. 2 (2001): 200–210. http://dx.doi.org/10.1007/s100050010081.

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Abstract The impact of electron probe microanalysis on the study of geological and planetary materials has been tremendous. Electron microprobes evolved into routine analytical instruments in geological research laboratories as instrument capabilities improved and applications to geologic/planetary materials expanded. The contributions of electron probe microanalysis to the characterization of minerals, both terrestrial and extraterrestrial, and to other significant geological research, such as light element analysis, trace element analysis, and element mapping, is described.

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17

Guttenberg, Nicholas, Huan Chen, Tomohiro Mochizuki, and H. Cleaves. "Classification of the Biogenicity of Complex Organic Mixtures for the Detection of Extraterrestrial Life." Life 11, no. 3 (2021): 234. http://dx.doi.org/10.3390/life11030234.

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Searching for life in the Universe depends on unambiguously distinguishing biological features from background signals, which could take the form of chemical, morphological, or spectral signatures. The discovery and direct measurement of organic compounds unambiguously indicative of extraterrestrial (ET) life is a major goal of Solar System exploration. Biology processes matter and energy differently from abiological systems, and materials produced by biological systems may become enriched in planetary environments where biology is operative. However, ET biology might be composed of different

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18

Ebihara, Mitsuru, and Yoshiji Oura. "Applicability of prompt gamma-ray analysis to the initial analysis of the extraterrestrial materials for chemical composition." Earth, Planets and Space 53, no. 11 (2001): 1039–45. http://dx.doi.org/10.1186/bf03351702.

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19

Burleigh, Richard, and Nigel Meeks. "Glassy Microspherules from Bomb Combustion of Charcoal." Radiocarbon 28, no. 1 (1986): 165–66. http://dx.doi.org/10.1017/s0033822200060069.

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Glassy microspherules, typically 200μm or less in diameter, are well documented from a variety of terrestrial and extraterrestrial sources (Baker, 1959, p 192–198; Glass, 1969; Rost, 1969; McKay, Greenwood & Morrison, 1970; Mueller & Hinsch, 1970; Cross, 1971; O'Keefe, 1980). To these we would add the formation of microspherules of similar habit when wood charcoal is burned in a combustion bomb (Barker, Burleigh & Meeks, 1969; Burleigh, 1973, 1974; Switsur, 1973; Switsur et al, 1974) as a first step in the chemical synthesis of samples for 14C age measurement. The glassy material o

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20

Uesugi, Masayuki, Kaori Hirahara, Kentaro Uesugi, et al. "Development of a sample holder for synchrotron radiation-based computed tomography and diffraction analysis of extraterrestrial materials." Review of Scientific Instruments 91, no. 3 (2020): 035107. http://dx.doi.org/10.1063/1.5122672.

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Noguchi, Takaaki, Minako Takase, Rikako Matsumoto, et al. "An Another Protocol to Make Sulfur Embedded Ultrathin Sections of Extraterrestrial Small Samples." Life 10, no. 8 (2020): 135. http://dx.doi.org/10.3390/life10080135.

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Another protocol to make sulfur embedded ultrathin sections was developed for STXM–XANES, AFM–IR and TEM analyses of organic materials in small extraterrestrial samples. Polymerized liquid sulfur—instead of low-viscosity liquid sulfur—is the embedding media in this protocol. Due to high viscosity of the polymerized sulfur, the embedded samples stay near the surface of polymerized liquid sulfur, which facilitates trimming of glassy sulfur and ultramicrotomy of tiny embedded samples. In addition, well-continued ribbons of ultramicrotomed sections can be obtained, which are suitable for the above

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22

Ruf, Alexander, Pauline Poinot, Claude Geffroy, Louis Le Sergeant d’Hendecourt, and Gregoire Danger. "Data-Driven UPLC-Orbitrap MS Analysis in Astrochemistry." Life 9, no. 2 (2019): 35. http://dx.doi.org/10.3390/life9020035.

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Meteorites have been found to be rich and highly diverse in organic compounds. Next to previous direct infusion high resolution mass spectrometry experiments (DI-HR-MS), we present here data-driven strategies to evaluate UPLC-Orbitrap MS analyses. This allows a comprehensive mining of structural isomers extending the level of information on the molecular diversity in astrochemical materials. As a proof-of-concept study, Murchison and Allende meteorites were analyzed. Both, global organic fingerprint and specific isomer analyses are discussed. Up to 31 different isomers per molecular compositio

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23

De Gregorio, Bradley T., and Cécile Engrand. "Diversity of Complex Organic Matter in Carbonaceous Chondrites, IDPs, and UCAMMs." Elements 20, no. 1 (2024): 24–30. http://dx.doi.org/10.2138/gselements.20.1.24.

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Complex organic matter is present in many extraterrestrial materials such as chondrite meteorites, micrometeorites, and interplanetary dust. The observed complexity of this organic matter is due to the combination of diversity of primitive organic materials that accreted onto asteroids and the subsequent effect of hydrothermal and/or metamorphic alteration that took place after accretion. These processes resulted in a variety of carbonaceous grain morphologies, elemental abundances, and organic functional group compositions. Some carbonaceous dust grains and micrometeorites have cometary origi

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24

Fkiri, Rihab, Ramzi Timoumi, Guillaume Rioland, et al. "Gas Chromatography Fingerprint of Martian Amino Acids before Analysis of Return Samples." Chemosensors 11, no. 2 (2023): 76. http://dx.doi.org/10.3390/chemosensors11020076.

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Within the perspective of the current and future space missions, the detection and separation of building blocks such as amino acids are important subjects which are becoming fundamental in the search for the origin of life and traces of life in the solar system. In this work, we have developed and optimized a strategy adapted to space experimentation to detect the presence of amino acid-like compounds using gas chromatography coupled to mass spectrometry (GC-MS). Selected derivatization methods meet the instrument design constraints imposed on in situ extraterrestrial experiments. Coupled to

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25

Neubeck, Anna, Marek Tulej, Magnus Ivarsson, et al. "Mineralogical determination in situ of a highly heterogeneous material using a miniaturized laser ablation mass spectrometer with high spatial resolution." International Journal of Astrobiology 15, no. 2 (2015): 133–46. http://dx.doi.org/10.1017/s1473550415000269.

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AbstractTechniques enabling in situ elemental and mineralogical analysis on extraterrestrial planets are strongly required for upcoming missions and are being continuously developed. There is ample need for quantitative and high-sensitivity analysis of elemental as well as isotopic composition of heterogeneous materials. Here we present in situ spatial and depth elemental profiles of a heterogeneous rock sample on a depth-scale of nanometres using a miniaturized laser ablation mass spectrometer (LMS) designed for planetary space missions. We show that the LMS spectra alone could provide highly

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Flynn, G. J., L. P. Keller, S. Wirick, and C. Jacobsen. "Organic matter in interplanetary dust particles." Proceedings of the International Astronomical Union 4, S251 (2008): 267–76. http://dx.doi.org/10.1017/s174392130802173x.

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AbstractAnhydrous interplanetary dust particles (IDPs), which are the most mineralogically primitive extraterrestrial materials available for laboratory analysis, contain several percent organic matter. The high O:C and N:C ratios suggest the organic matter in the anhydrous IDPs is significantly less altered by thermal processing than the organic matter in meteorites. X-ray Absorption Near-Edge Structure (XANES) spectroscopy and infrared spectroscopy demonstrate the presence of C=C, most likely as C-rings, C=O, and aliphatic C-H2and C-H3in all the IDPs examined. A D-rich spot, containing mater

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Dubey Sonali, Kumar Rohit, Rai Abhishek K., and Rai Awadhesh K. "Laser Induced breakdown spectroscopy (LIBS): Application to geological materials." Optics and Spectroscopy 130, no. 13 (2022): 2053. http://dx.doi.org/10.21883/eos.2022.13.53989.1003-21.

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Laser-induced breakdown spectroscopy (LIBS) is emerging as an analytical tool for investigating geological materials. The unique abilities of this technique proven its potential in the area of geology. Detection of light elements, portability for in-field analysis, spot detection, and no sample preparation are some features that make this technique appropriate for the study of geological materials. The application of the LIBS technique has been tremendously developed in recent years. In this report, results obtained from previous and most recent studies regarding the investigation of geologica

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Haenecour, Pierre, and Maitrayee Bose. "Understanding our solar system history through in situ nanoscale analysis of extraterrestrial materials: A special issue for Dr. Christine Floss." Meteoritics & Planetary Science 55, no. 6 (2020): 1153–59. http://dx.doi.org/10.1111/maps.13489.

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NAKAMURA, Eizo, Akio MAKISHIMA, Takuya MORIGUTI, et al. "Establishment of Comprehensive Analytical System for Terrestrial and Extraterrestrial Materials behind the Initial Analysis of Particles Returned by Hayabusa Spacecraft." Hyomen Kagaku 33, no. 12 (2012): 681–86. http://dx.doi.org/10.1380/jsssj.33.681.

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Mezzina, Lidia, Angelo Nicosia, Fabiana Vento, Guido De Guidi, and Placido Giuseppe Mineo. "Photosensitized Thermoplastic Nano-Photocatalysts Active in the Visible Light Range for Potential Applications Inside Extraterrestrial Facilities." Nanomaterials 12, no. 6 (2022): 996. http://dx.doi.org/10.3390/nano12060996.

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Among different depollution methods, photocatalysis activated by solar light is promising for terrestrial outdoor applications. However, its use in underground structures and/or microgravity environments (e.g., extraterrestrial structures) is forbidden. In these cases, there are issues related to the energy emitted from the indoor lighting system because it is not high enough to promote the photocatalytic mechanism. Moreover, microgravity does not allow the recovery of the photocatalytic slurry from the depolluted solution. In this work, the synthesis of a filmable nanocomposite based on semic

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31

Dubey, Sonali, Rohit Kumar, Abhishek K. Rai, and Awadhesh K. Rai. "Laser Induced Breakdown Spectroscopy (LIBS): Application to Geological Materials-=SUP=-*-=/SUP=-." Оптика и спектроскопия 129, no. 10 (2021): 1336. http://dx.doi.org/10.21883/os.2021.10.51502.1003-21.

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Laser-induced breakdown spectroscopy (LIBS) is emerging as an analytical tool for investigating geological materials. The unique abilities of this technique proven its potential in the area of geology. Detection of light elements, portability for in-field analysis, spot detection, and no sample preparation are some features that make this technique appropriate for the study of geological materials. The application of the LIBS technique has been tremendously developed in recent years. In this report, results obtained from previous and most recent studies regarding the investigation of geologica

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32

Gu, Lixin, Nian Wang, Xu Tang, and H. G. Changela. "Application of FIB-SEM Techniques for the Advanced Characterization of Earth and Planetary Materials." Scanning 2020 (July 25, 2020): 1–15. http://dx.doi.org/10.1155/2020/8406917.

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Advanced microanalytical techniques such as high-resolution transmission electron microscopy (HRTEM), atom probe tomography (APT), and synchrotron-based scanning transmission X-ray microscopy (STXM) enable one to characterize the structure and chemical and isotopic compositions of natural materials down towards the atomic scale. Dual focused ion beam-scanning electron microscopy (FIB-SEM) is a powerful tool for site-specific sample preparation and subsequent analysis by TEM, APT, and STXM to the highest energy and spatial resolutions. FIB-SEM also works as a stand-alone technique for three-dim

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Neal, Clive R. "Issues involved in a Martian sample return: Integrity preservation and the Curation and Analysis Planning Team for Extraterrestrial Materials (CAPTEM) position." Journal of Geophysical Research: Planets 105, E9 (2000): 22487–506. http://dx.doi.org/10.1029/1999je001185.

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Pérez-Fernández, Cristina, Elena González-Toril, Eva Mateo-Martí, and Marta Ruiz-Bermejo. "Multivariate Analysis Applied to Microwave-Driven Cyanide Polymerization: A Statistical View of a Complex System." Polymers 15, no. 2 (2023): 410. http://dx.doi.org/10.3390/polym15020410.

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For the first time, chemometrics was applied to the recently reported microwave-driven cyanide polymerization. Fast, easy, robust, low-cost, and green-solvent processes are characteristic of these types of reactions. These economic and environmental benefits, originally inspired by the constraints imposed by plausible prebiotic synthetic conditions, have taken advantage of the development of a new generation of HCN-derived multifunctional materials. HCN-derived polymers present tunable properties by temperature and reaction time. However, the apparently random behavior observed in the evolutio

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35

Tsou, P. "Hypervelocity Capture of Meteoroids in Aerogel." International Astronomical Union Colloquium 150 (1996): 237–42. http://dx.doi.org/10.1017/s0252921100501614.

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Micrometeoroids of cometary or asteroidal origin constitute a unique repository of information concerning the formation and subsequent processing history of materials in the solar nebula. One of the current goals of planetary science is to return samples from a known primitive extraterrestrial body for detailed laboratory analysis (NASA Solar System Exploration Committee, SSEC 1983). Planetary flyby orbital motions dictate that dust particles will approach the spacecraft at relative speeds up to tens of km/s. It has always been thought that these hypervelocity particles could not be captured w

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36

Panitz, Corinna, Gerda Horneck, Elke Rabbow, et al. "The SPORES experiment of the EXPOSE-R mission: Bacillus subtilis spores in artificial meteorites." International Journal of Astrobiology 14, no. 1 (2014): 105–14. http://dx.doi.org/10.1017/s1473550414000251.

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AbstractThe experiment SPORES ‘Spores in artificial meteorites’ was part of European Space Agency's EXPOSE-R mission, which exposed chemical and biological samples for nearly 2 years (March 10, 2009 to February 21, 2011) to outer space, when attached to the outside of the Russian Zvezda module of the International Space Station. The overall objective of the SPORES experiment was to address the question whether the meteorite material offers enough protection against the harsh environment of space for spores to survive a long-term journey in space by experimentally mimicking the hypothetical sce

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Zolensky, Michael, and Ruth Barrett. "The genetic relationship between hydrous and anhydrous interplanetary dust particles." Proceedings, annual meeting, Electron Microscopy Society of America 50, no. 2 (1992): 1720–21. http://dx.doi.org/10.1017/s0424820100133230.

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It is a fundamental goal of interplanetary dust particle (IDP) research to determine the sources and histories of these primitive extraterrestrial materials. Chondritic IDPs have been divided into anhydrous and hydrous varieties, with sub-classification being made on the grounds of the dominant anhydrous (olivine or pyroxene) or hydrous (smectite or serpentine) present. The presumption is that hydrated IDPs experienced aqueous alteration on parent bodies (hydrous asteroids or possibly comets); we wish to discover whether the anhydrous IDPs were the initial raw materials for these reactions. We

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38

Hornbogen, Erhard. "Entropy, Transformations and Sustainability of Industrial Life Cycles." International Journal of Materials Research 92, no. 7 (2001): 626–31. http://dx.doi.org/10.1515/ijmr-2001-0123.

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Abstract Life cycles of materials are analysed in a systematic manner as a six-stage process. It starts with primary or secondary raw materials and ends with recycling or deposition of waste. The purpose of the industrial process is the transformation of matter into materials from which useful goods are produced. The complete cycle can be described as a sequence of man-made transformations with defined changes in entropy and energy. Entropy is the measure for any type of disorder. Changes in entropy are due to separation (mining, purification: negative entropy), ordering (consolidation, constr

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New, James S., Bahar Kazemi, Vassilia Spathis, Mark C. Price, Richard A. Mathies, and Anna L. Butterworth. "Quantitative evaluation of the feasibility of sampling the ice plumes at Enceladus for biomarkers of extraterrestrial life." Proceedings of the National Academy of Sciences 118, no. 37 (2021): e2106197118. http://dx.doi.org/10.1073/pnas.2106197118.

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Enceladus, an icy moon of Saturn, is a compelling destination for a probe seeking biosignatures of extraterrestrial life because its subsurface ocean exhibits significant organic chemistry that is directly accessible by sampling cryovolcanic plumes. State-of-the-art organic chemical analysis instruments can perform valuable science measurements at Enceladus provided they receive sufficient plume material in a fly-by or orbiter plume transit. To explore the feasibility of plume sampling, we performed light gas gun experiments impacting micrometer-sized ice particles containing a fluorescent dye

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40

Ryan, Conor, Tobias Haist, Gennadii Laskin, Susanne Schröder, and Stephan Reichelt. "Technology Selection for Inline Topography Measurement with Rover-Borne Laser Spectrometers." Sensors 24, no. 9 (2024): 2872. http://dx.doi.org/10.3390/s24092872.

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This work studies enhancing the capabilities of compact laser spectroscopes integrated into space-exploration rovers by adding 3D topography measurement techniques. Laser spectroscopy enables the in situ analysis of sample composition, aiding in the understanding of the geological history of extraterrestrial bodies. To complement spectroscopic data, the inclusion of 3D imaging is proposed to provide unprecedented contextual information. The morphological information aids material characterization and hence the constraining of rock and mineral histories. Assigning height information to lateral

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Edwards, H. G. M., R. Moeller, S. E. Jorge Villar, G. Horneck, and E. Stackebrandt. "Raman spectroscopic study of the photoprotection of extremophilic microbes against ultraviolet radiation." International Journal of Astrobiology 5, no. 4 (2006): 313–18. http://dx.doi.org/10.1017/s147355040600348x.

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Extremophiles use a range of pigments for protection against low-wavelength radiation in exposed terrestrial habitats and photoaccessory materials are synthesized for the effective harnessing of photosynthetically active radiation. Raman spectroscopy has been demonstrated to be a useful probe for information on the survival strategies employed by extremophilic bacteria through the identification of key biomolecular signatures of the suite of protective chemicals synthesized by the organisms in stressed environments. Raman spectroscopic analyses of Bacillus spp. spores, Bacillus atrophaeus (DSM

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Cockell, Charles S., John Holt, Jim Campbell, et al. "Subsurface scientific exploration of extraterrestrial environments (MINAR 5): analogue science, technology and education in the Boulby Mine, UK." International Journal of Astrobiology 18, no. 2 (2018): 157–82. http://dx.doi.org/10.1017/s1473550418000186.

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AbstractThe deep subsurface of other planetary bodies is of special interest for robotic and human exploration. The subsurface provides access to planetary interior processes, thus yielding insights into planetary formation and evolution. On Mars, the subsurface might harbour the most habitable conditions. In the context of human exploration, the subsurface can provide refugia for habitation from extreme surface conditions. We describe the fifth Mine Analogue Research (MINAR 5) programme at 1 km depth in the Boulby Mine, UK in collaboration with Spaceward Bound NASA and the Kalam Centre, India

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Mróz, Tomasz, Katarzyna Szufa, Marina V. Frontasyeva, et al. "Determination of element composition and extraterrestrial material occurrence in moss and lichen samples from King George Island (Antarctica) using reactor neutron activation analysis and SEM microscopy." Environmental Science and Pollution Research 25, no. 1 (2017): 436–46. http://dx.doi.org/10.1007/s11356-017-0431-2.

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Takeshima, Yuko, Hironobu Hyodo, Tatsuki Tsujimori, Chitaro Gouzu, and Tetsumaru Itaya. "In Situ Argon Isotope Analyses of Chondrule-Forming Materials in the Allende Meteorite: A Preliminary Study for 40Ar/39Ar Dating Based on Cosmogenic 39Ar." Minerals 13, no. 1 (2022): 31. http://dx.doi.org/10.3390/min13010031.

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The argon isotopic compositions of chondrule-forming minerals of the Allende (CV3) meteorite were examined to evaluate the possibility of in situ 40Ar/39Ar dating of planetary surface rocks based on cosmogenic 39Ar without neutron irradiation in a reactor. The investigated Allende meteorite sample (ME-247H: 50 mm × 45 mm × 5 mm; 28.85 g) contains at least three textural types of chondrules: barred olivine chondrule (BOC), porphyritic olivine chondrule (POC), and unclassified chondrule (UC). Most chondrules contain olivine, low-Ca pyroxene, clinopyroxene, and plagioclase as primary phases, with

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Freissinet, C., A. Buch, C. Szopa, and R. Sternberg. "Enantiomeric separation of volatile organics by gas chromatography for the in situ analysis of extraterrestrial materials: Kinetics and thermodynamics investigation of various chiral stationary phases." Journal of Chromatography A 1306 (September 2013): 59–71. http://dx.doi.org/10.1016/j.chroma.2013.07.058.

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Evatt, G. W., A. R. D. Smedley, K. H. Joy, et al. "The spatial flux of Earth’s meteorite falls found via Antarctic data." Geology 48, no. 7 (2020): 683–87. http://dx.doi.org/10.1130/g46733.1.

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Abstract Contemporary calculations for the flux of extraterrestrial material falling to the Earth’s surface (each event referred to as a “fall”) rely upon either short-duration fireball monitoring networks or spatially limited ground-based meteorite searches. To date, making accurate fall flux estimates from the much-documented meteorite stranding zones of Antarctica has been prohibited due to complicating glacial ice dynamics and difficulties in pairing together distinct meteorite samples originating from the same fall. Through glaciological analysis and use of meteorite collection data, we d

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Micca Longo, Gaia, Marcella D’Elia, Sergio Fonti, Savino Longo, Francesca Mancarella, and Vincenzo Orofino. "Kinetics of White Soft Minerals (WSMs) Decomposition under Conditions of Interest for Astrobiology: A Theoretical and Experimental Study." Geosciences 9, no. 2 (2019): 101. http://dx.doi.org/10.3390/geosciences9020101.

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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 ent

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Schröder, Susanne, Kristin Rammelkamp, Franziska Hanke, et al. "Effects of pulsed laser and plasma interaction on Fe, Ni, Ti, and their oxides for LIBS Raman analysis in extraterrestrial environments." Journal of Raman Spectroscopy 51, no. 9 (2019): 1667–81. http://dx.doi.org/10.1002/jrs.5650.

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Percot, Aline, Farah Mahieddine, Hajime Yano, et al. "Surface-Enhanced Raman Spectroscopy (SERS) for Identifying Traces of Adenine in Organic-Bearing Extraterrestrial Dust Analogs Captured in the Tanpopo Aerogel after Hypervelocity Impacts." Gels 10, no. 4 (2024): 249. http://dx.doi.org/10.3390/gels10040249.

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Raman spectroscopy is a non-destructive analytical technique for characterizing organic and inorganic materials with spatial resolution in the micrometer range. This makes it a method of choice for space-mission sample characterization, whether on return or in situ. To enhance its sensitivity, we use signal amplification via interaction with plasmonic silver-based colloids, which corresponds to surface-enhanced Raman scattering (SERS). In this study, we focus on the analysis of biomolecules of prebiotic interest on extraterrestrial dust trapped in silica aerogel, jointly with the Japanese Tanp

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Schröder, Susanne, Fabian Seel, Enrico Dietz, et al. "A Laser-Induced Breakdown Spectroscopy (LIBS) Instrument for In-Situ Exploration with the DLR Lightweight Rover Unit (LRU)." Applied Sciences 14, no. 6 (2024): 2467. http://dx.doi.org/10.3390/app14062467.

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In the framework of the Helmholtz ARCHES project, a multitude of robots, including rovers and drones, were prepared for the autonomous exploration of a test site at the foothills of Mt. Etna, Sicily—a terrain resembling extraterrestrial locations such as the Moon. To expand the suite of tools and sensors available for the exploration and investigation of the test site, we developed a laser-induced breakdown spectroscopy (LIBS) instrument for the geochemical analysis of local geological samples. In alignment with the mission scenario, this instrument is housed in a modular payload box that can

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