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  • 1
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2021
    In:  International Journal of Astrobiology Vol. 20, No. 6 ( 2021-12), p. 377-393
    In: International Journal of Astrobiology, Cambridge University Press (CUP), Vol. 20, No. 6 ( 2021-12), p. 377-393
    Abstract: In this work, we address the difficulty of reliably identifying traces of life on Mars. Several independent lines of evidence are required to build a compelling body of proof. In particular, we underline the importance of correctly interpreting the geological and mineralogical context of the sites to be explored for the presence of biosignatures. We use as examples to illustrate this, ALH84001 (where knowledge of the geological context was very limited) and other terrestrial deposits, for which this could be properly established. We also discuss promising locations and formations to be explored by ongoing and future rover missions, including Oxia Planum, which, dated at 4.0 Ga, is the most ancient Mars location targeted for investigation yet.
    Type of Medium: Online Resource
    ISSN: 1473-5504 , 1475-3006
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2021
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    SSG: 12
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  • 2
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2005
    In:  International Journal of Astrobiology Vol. 4, No. 3-4 ( 2005-10), p. 195-202
    In: International Journal of Astrobiology, Cambridge University Press (CUP), Vol. 4, No. 3-4 ( 2005-10), p. 195-202
    Abstract: The European Astrobiology Network Association (EANA) coordinates and promotes astrobiology in the 17 European countries that are member of the organization. Astrobiology includes the study of the origin, evolution and distribution of life in the Universe. It is a multi-disciplinary science that encompasses the disciplines of chemistry, biology, palaeontology, geology, atmospheric physics, planetary physics and stellar physics. The open questions to be addressed and the steps ahead in cosmochemistry, star and planet formation, the chemistry of life's origin, the study of bacterial life as a reference and the search for habitats and biosignatures beyond the Earth are presented.
    Type of Medium: Online Resource
    ISSN: 1473-5504 , 1475-3006
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2005
    detail.hit.zdb_id: 2079707-2
    SSG: 12
    SSG: 16,12
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  • 3
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2014
    In:  Journal of Paleontology Vol. 88, No. 2 ( 2014-03), p. 224-239
    In: Journal of Paleontology, Cambridge University Press (CUP), Vol. 88, No. 2 ( 2014-03), p. 224-239
    Abstract: Metazoans (multicellular animals) evolved during the Ediacaran Period as shown by the record of their imprints, carbonaceous compressions, trace fossils, and organic bodies and skeletal fossils. Initial evolutionary experiments produced unusual bodies that are poorly understood or conceived of as non-metazoan. It is accepted that sponges, ctenophorans, cnidarians, placozoans, and bilaterians were members of the Ediacaran fauna, many of which have uncertain affinities. The fossil Sabellidites cambriensis Yanishevsky, 1926, derived from the terminal Ediacaran strata, is the earliest known organically preserved animal that belonged to a newly evolving fauna, which replaced the Ediacara-type metazoans. Morphologically simple soft-bodied tubular fossils, such as S. cambriensis , and biomineralized, as contemporaneous Sinotubulites sp., are not easy to recognize phylogenetically because many unrelated organisms developed encasing tubes independently. Therefore, in addition to morphologic information, evidence derived from the microstructure of the organic wall and its biochemistry may be vital to resolving fossil origins and phylogenetic relationships. Here we present morphological, microstructural and biogeochemical studies on S. cambriensis using various microscopic and spectroscopic techniques, which provide new evidence that supports its siboglinid, annelidan affinity. The late Ediacaran age of Sabellidites fossil constrains the minimum age of siboglinids and the timing of the divergence of including them annelids by fossil record and this could be tested using molecular clock estimates. The fine microstructure of the organic tube in Sabellidites is multi-layered and has discrete layers composed of differently orientated and perfectly shaped fibers embedded in an amorphous matrix. The highly ordered and specific pattern of fiber alignment (i.e., the texture of organic matter) is similar to that of representatives of the family Siboglinidae. The biogeochemistry of the organic matter that comprised the tube, which was inferred from its properties, composition, and microstructure, is consistent with chitin and proteins as in siboglinids.
    Type of Medium: Online Resource
    ISSN: 0022-3360 , 1937-2337
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2014
    detail.hit.zdb_id: 219113-1
    detail.hit.zdb_id: 2047591-3
    SSG: 13
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  • 4
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2019
    In:  Geological Magazine Vol. 156, No. 9 ( 2019-09), p. 1631-1638
    In: Geological Magazine, Cambridge University Press (CUP), Vol. 156, No. 9 ( 2019-09), p. 1631-1638
    Abstract: Jurassic siliceous hot-spring (sinter) deposits from Argentine Patagonia were evaluated to determine the distribution and preservation quality of their entombed microbial fabrics. Detailed study showed that the Claudia palaeo-geothermal field hosts the best-preserved sinter apron in the Deseado Massif geological province, where we also found hot-spring silica–biotic interactions extending into hydrothermally influenced fluvial and lacustrine settings. Carbonaceous material was identified by petrography and Raman spectroscopy mapping; it is inter-laminated with silica across proximal vent to distal marsh facies. The ubiquitous presence of microbial biosignatures has application to studies of hydrothermal settings of early life on Earth and potentially Mars.
    Type of Medium: Online Resource
    ISSN: 0016-7568 , 1469-5081
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2019
    detail.hit.zdb_id: 956405-6
    detail.hit.zdb_id: 1479206-0
    SSG: 13
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  • 5
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 1997
    In:  International Astronomical Union Colloquium Vol. 161 ( 1997-01), p. 491-504
    In: International Astronomical Union Colloquium, Cambridge University Press (CUP), Vol. 161 ( 1997-01), p. 491-504
    Abstract: The oldest cell-like structures on Earth are preserved in silicified lagoonal, shallow sea or hydrothermal sediments, such as some Archean formations in Western Australia and South Africa. Previous studies concentrated on the search for organic fossils in Archean rocks. Observations of silicified bacteria (as silica minerals) are scarce for both the Precambrian and the Phanerozoic, but reports of mineral bacteria finds, in general, are increasing. The problems associated with the identification of authentic fossil bacteria and, if possible, closer identification of bacteria type can, in part, be overcome by experimental fossilisation studies. These have shown that not all bacteria fossilise in the same way and, indeed, some seem to be very resistent to fossilisation. This paper deals with a transmission electron microscope investigation of the silicification of four species of bacteria commonly found in the environment. The Gram positive Bacillus laterosporus and its spore produced a robust, durable crust upon silicification, whereas the Gram negative Pseudomonas fluorescens, Ps. vesicularis , and Ps. acidovorans presented delicately preserved walls. The greater amount of peptidoglycan, containing abundant metal cation binding sites, in the cell wall of the Gram positive bacterium, probably accounts for the difference in the mode of fossilisation. The Gram positive bacteria are, therefore, probably most likely to be preserved in the terrestrial and extraterrestrial rock record.
    Type of Medium: Online Resource
    ISSN: 0252-9211
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 1997
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  • 6
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2011
    In:  Geological Magazine Vol. 148, No. 3 ( 2011-05), p. 507-507
    In: Geological Magazine, Cambridge University Press (CUP), Vol. 148, No. 3 ( 2011-05), p. 507-507
    Type of Medium: Online Resource
    ISSN: 0016-7568 , 1469-5081
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2011
    detail.hit.zdb_id: 956405-6
    detail.hit.zdb_id: 1479206-0
    SSG: 13
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  • 7
    In: International Journal of Astrobiology, Cambridge University Press (CUP), Vol. 14, No. 1 ( 2015-01), p. 89-97
    Abstract: In order to confirm the results of previous experiments concerning the chemical behaviour of organic molecules in the space environment, organic molecules (amino acids and a dipeptide) in pure form and embedded in meteorite powder were exposed in the AMINO experiment in the EXPOSE-R facility onboard the International Space Station. After exposure to space conditions for 24 months (2843 h of irradiation), the samples were returned to the Earth and analysed in the laboratory for reactions caused by solar ultraviolet (UV) and other electromagnetic radiation. Laboratory UV exposure was carried out in parallel in the Cologne DLR Center (Deutsches Zentrum für Luft und Raumfahrt). The molecules were extracted from the sample holder and then (1) derivatized by silylation and analysed by gas chromatography coupled to a mass spectrometer (GC–MS) in order to quantify the rate of degradation of the compounds and (2) analysed by high-resolution mass spectrometry (HRMS) in order to understand the chemical reactions that occurred. The GC–MS results confirm that resistance to irradiation is a function of the chemical nature of the exposed molecules and of the wavelengths of the UV light. They also confirm the protective effect of a coating of meteorite powder. The most altered compounds were the dipeptides and aspartic acid while the most robust were compounds with a hydrocarbon chain. The MS analyses document the products of reactions, such as decarboxylation and decarbonylation of aspartic acid, taking place after UV exposure. Given the universality of chemistry in space, our results have a broader implication for the fate of organic molecules that seeded the planets as soon as they became habitable as well as for the effects of UV radiation on exposed molecules at the surface of Mars, for example.
    Type of Medium: Online Resource
    ISSN: 1473-5504 , 1475-3006
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2015
    detail.hit.zdb_id: 2079707-2
    SSG: 12
    SSG: 16,12
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  • 8
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2004
    In:  International Journal of Astrobiology Vol. 3, No. 2 ( 2004-04), p. 157-163
    In: International Journal of Astrobiology, Cambridge University Press (CUP), Vol. 3, No. 2 ( 2004-04), p. 157-163
    Abstract: One principal challenge in biology is defining a postulate by which the habitability of other planets can be assessed. Current assessments suffer from two potential weaknesses. With respect to other planets, either assumptions are made about the physical and chemical conditions of environments that err on the side of biological optimism without empirical constraint by spacecraft observations or novel physiologies of microorganisms are invented to fit extraterrestrial environmental conditions with no demonstrated microbiological counterparts on Earth. Attempts to assess the habitability of the early Earth suffer from similar problems. We discuss the following postulate: ‘the proposition that a planet is or was habitable requires that the physiological requirements of microorganisms on Earth known at the time of assessment match the empirically determined combined physical and chemical conditions in the extraterrestrial or early Earth environment being assessed’ as a means of evaluating ‘habitability’. We use as tests for our postulate the early Earth and the cloud deck of Venus (a habitat that has been a source of optimistic debate for forty years). We conclude that, although the early Earth was habitable, Venus is a dead world.
    Type of Medium: Online Resource
    ISSN: 1473-5504 , 1475-3006
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2004
    detail.hit.zdb_id: 2079707-2
    SSG: 12
    SSG: 16,12
    Location Call Number Limitation Availability
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