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  • 1
    Online-Ressource
    Online-Ressource
    Berlin, Heidelberg :Springer Berlin / Heidelberg,
    Schlagwort(e): Astrophysics. ; Electronic books.
    Materialart: Online-Ressource
    Seiten: 1 online resource (362 pages)
    Ausgabe: 2nd ed.
    ISBN: 9783540330882
    Serie: Advances in Astrobiology and Biogeophysics Series
    Sprache: Englisch
    Anmerkung: Intro -- CONTENTS -- 1 Comets and the Origin and Evolution of Life -- 1.1 Introduction -- 1.2 Comets and the Origin on Life: An Idea with a Long History -- 1.3 Chemical Evolution of Cometary Nuclei -- 1.4 The Collisional History of the Early Solar System -- 1.5 A Cometary Origin for the Terrestrial Volatiles? -- 1.6 Comets and Prebiotic Synthesis -- 1.7 Cometary Collisions and Biological Evolution -- References -- 2 The Origin of the Atmosphere and of the Oceans -- 2.1 Introduction -- 2.2 Hypothesis of the Volcanic Origin -- 2.2.1 The Missing Primary Atmosphere -- 2.2.2 The Origin of the Solar System -- 2.3 Existence of Accretion Disks -- 2.4 Numerical Models for a Protosolar Accretion Disk -- 2.5 The Chondrites as Clues on Planetary Formation -- 2.6 From Dust to Planets -- 2.7 Temperature History of the Earth's Material -- 2.8 Thermochemical Equilibrium in Solar Nebula -- 2.9 Discussion: Was the Earth Outgassed? -- 2.10 Formation of the Giant Planets -- 2.11 Orbital Diffusion of Comets -- 2.12 Chronology -- 2.13 Chronology Discussion -- 2.14 Observational Confirmations -- 2.14.1 Cratering Record -- 2.14.2 Geochemistry -- 2.14.3 Geochemical Model -- 2.14.4 Noble Gases -- 2.14.5 Deuterium -- 2.15 Nature of the Early Atmosphere -- 2.16 Prebiotic Organic Syntheses -- 2.17 Summary -- 2.17.1 Verified Predictions of the Model -- 2.17.2 Unverified Predictions of the Model -- 2.18 Conclusion -- References -- 3 Cometary Micrometeorites in Planetology, Exobiology, and Early Climatology -- 3.1 Introduction -- 3.2 Dark Micrometeorites in Blue Ices: Relationships with Hydrous-Carbonaceous Chondrites -- 3.3 Formation of the Earth's Atmosphere: Previous Scenarios -- 3.3.1 Volcanism, Nebular Gases, and Comets -- 3.3.2 A Wrong Neon in the Giant Asteroid? -- 3.4 The Micrometeoritic "Purity" of the Earth's Atmosphere. , 3.4.1 Concentrations of Volatiles in Antarctic Micrometeorites -- 3.4.2 The Micrometeoritic "Purity" of the Earth's Atmosphere -- 3.5 Formation of the Post-Lunar Earth's Atmosphere -- 3.5.1 An Accretion Formula Born with the Moon -- 3.5.2 Total Amounts of Micrometeoritic Volatiles in the Post-Lunar Atmosphere -- 3.6 Micrometeoritic Siderophile Elements in Planetology -- 3.6.1 Micrometeoritic Iridium in the Earth's Mantle -- 3.6.2 A Difficult Extrapolation to the Moon and Mars -- 3.7 Micrometeoritic Sulfur and Ferrihydrite in Exobiology -- 3.7.1 Micrometeoritic Sulfur and the "Worlds" of Iron Sulfides andThioesters -- 3.7.2 Ferrihydrite in Unmelted and Melted Micrometeorites -- 3.8 A Post-Lunar Micrometeoritic Greenhouse Effect? -- 3.9 Controversies About the Parent Bodies of Micrometeorites -- 3.10 From Prospects to Unsolved Problems -- References -- 4 Macromolecules: From Star-Forming Regions to Comets to the Origins of Life -- 4.1 Introduction -- 4.2 Interstellar Ices -- 4.3 Laboratory Simulations -- 4.4 Observations from Massive Star-Forming Regions -- 4.4.1 Current Research on Macromolecules in HMCs and Comets -- 4.4.2 Sgr B2(N-LMH) -- 4.4.3 Other Sources -- 4.4.4 Comets -- 4.5 Summary and Prognosis -- References -- 5 Impact Delivery of Prebiotic Organic Matter to Planetary Surfaces -- 5.1 Introduction -- 5.2 Sources of Organic Material -- 5.3 Hydrocode Simulations -- 5.4 Earth:Significant Delivery -- 5.5 Mars: Balancing Factors -- 5.6 Europa: Impactor Loss -- 5.7 Amino Acids on the Moon: Impact Delivery? -- 5.8 Summary and Conclusions -- References -- 6 Comets and Prebiotic Organic Molecules on Early Earth -- 6.1 The Uninhabitable Habitable Zone -- 6.1.1 The Habitable Zone and Liquid Water -- 6.1.2 Are the Earth's Oceans Extraterrestrial? -- 6.1.3 D/H Ratios and Noble Gas Evidence -- 6.2 The Time Window for the Origin of Life. , 6.2.1 Frustration of the Origin of Life -- 6.2.2 Microfossils and Stromatolites -- 6.2.3 Molecular Biomarkers -- 6.2.4 Carbon Isotope Fractionation -- 6.3 Endogenous Production of Prebiotic Organic Molecules -- 6.3.1 Nature of the Early Atmosphere -- 6.3.2 Energy Sources and Atmospheric Organic Production -- 6.3.3 Organic Production at Hydrothermal Vents -- 6.4 The Lunar Cratering Record -- 6.4.1 A Terminal Lunar Cataclysm? -- 6.4.2 Implications for the Mass Flux on Early Earth -- 6.5 Impact Delivery of Intact Exogenous Organics -- 6.5.1 Interplanetary Dust Particles and Micrometeorites -- 6.5.2 Interstellar Dust -- 6.5.3 Meteorites -- 6.5.4 Catastrophic Airbursts -- 6.5.5 Big Impacts -- 6.6 Atmospheric Shock Synthesis of Organic Molecules -- 6.6.1 Shocks from Meteors -- 6.6.2 Shocks from Airburst -- 6.6.3 Shocks from Giant Impact Plumes -- 6.7 Postimpact Recombination -- 6.8 Amino Acids at the K/T Boundary -- 6.9 An Inventory of Organic Production on Early Earth -- 6.10 Organic Sinks and Concentrations -- 6.11 Prebiotic Organics on the Early Earth -- References -- 7 Impacts and the Early Evolution of Life -- 7.1 Prologue -- 7.2 Introduction -- 7.3 The Lunar Record -- 7.3.1 Energies of Basin-Forming Impacts -- 7.3.2 Crustal Contamination by Chondrites -- 7.3.3 Chronology of the Late Bombardment -- 7.4 The Late Bombardment on the Earth -- 7.4.1 Impactor Mass Distribution -- 7.4.2 Scaling the Lunar Impact Record to the Earth -- 7.5 Environmental Effects of Large Impacts on the Earth -- 7.5.1 An Ocean Vaporizing Impact -- 7.5.2 Imbrium on the Earth -- 7.5.3 Evolutionary Filters -- 7.6 The Late Bombardment on Mars -- 7.6.1 Environmental Effects of Large Impacts on Mars -- 7.6.2 Local Panspermia -- 7.7 Conclusions -- 7.8 Epilogue -- References -- 8 Extraterrestrial Impact Episodes and Archaean to Early Proterozoic (3.8-2.4 Ga) Habitats of Life. , 8.1 Introduction -- 8.2 PRE-3.8-Ga Events -- 8.3 Post-3.8-Ga Extraterrestrial Impacts -- 8.4 Archaean to Early Proterozoic Impacts, Pilbara, and Kaapvaal Cratons -- 8.4.1 About 3.5-Ga Impact Cluster -- 8.4.2 About 3.26-3.225-Ga Asteroid Bombardment -- 8.4.3 About 2.6-2.4-Ga Impact Clusters and Associated Tsunami -- 8.5 Possible and Demonstrated Connections Between Extraterrestrial Impacts and Habitats of Life -- References -- 9 The Contemporary Hazard of Comet Impacts -- 9.1 Introduction -- 9.2 Impactor Population -- 9.3 Nature of the Hazard -- 9.3.1 Penetration Through the Atmosphere -- 9.3.2 Globally Catastrophic Impacts -- 9.3.3 Threshold for a Globally Catastrophic Climate Perturbation -- 9.4 Hazard Analysis -- 9.5 Risk Reduction and Mitigation -- 9.5.1 Impact Prediction -- 9.5.2 Deflection or Destruction -- 9.5.3 The Challenge of Comets -- 9.6 Summary and Conclusions -- References -- 10 The Conditions for Liquid Water in Cometary Nuclei -- 10.1 Introduction -- 10.2 Reconsidering Internal Heat Sources -- 10.2.1 Radioactive Heating -- 10.2.2 Amorphous-Crystalline Transition -- 10.3 Cooling Mechanisms -- 10.3.1 Thermal Diffusivity -- 10.4 Simple Physics -- 10.4.1 Energy Considerations -- 10.4.2 Timescales -- 10.5 Numerical Models -- 10.6 What Further Studies May Show -- References -- 11 Spacecraft Missions to Comets -- 11.1 Overview -- 11.2 The Relevance for Issues of the Origin of Life -- 11.3 Space Missions to Comets -- 11.4 Results and Expectations -- 11.4.1 The Measurements at Halley -- 11.4.2 Current Missions -- 11.4.3 Future Missions -- 11.5 Conclusions -- References -- 12 Interstellar and Cometary Dust in Relation to the Origin of Life -- 12.1 First In Situ Chemical Analysis of Interstellar Dust -- 12.1.1 Quinone Derivatives as Main Organic Component -- 12.1.2 Hydrated "Dirty" PAHs as Products of Radiative Chemistry in Nebulae. , 12.1.3 Possible Thermochemical Implications for the Accretion Process to Comets -- 12.2 New In Situ Analysis of Cometary Dust at p/Wild-2 -- 12.2.1 Corroboration of the Cometary Dust Prevalence of Nitrogen Chemistry -- 12.2.2 Precursors of Amino Acids, Sugars, and Some Other Building Blocks in Cosmic Dust -- 12.3 Combined Scenario of Origin of Life with Both Dust Types -- 12.3.1 Hydrolysis Mechanisms of Cometary Dust in Water -- 12.3.2 Some Necessary Conditions for Systemic Chemical Self-Organization -- 12.3.3 The Question of Redox Catalysis Needed -- 12.3.4 Possibilities and Limitations of Heterocatalysis by Mineral Surfaces -- 12.3.5 Interstellar Dust and the "PQQ-Enigma" for Catalysis -- 12.4 Conclusions and Further Goals -- References -- Index.
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  • 2
    Online-Ressource
    Online-Ressource
    New York, NY :Springer,
    Schlagwort(e): Life-Origin. ; Electronic books.
    Materialart: Online-Ressource
    Seiten: 1 online resource (302 pages)
    Ausgabe: 1st ed.
    ISBN: 9781475726886
    Sprache: Englisch
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  • 3
    Digitale Medien
    Digitale Medien
    [s.l.] : Nature Publishing Group
    Nature 325 (1987), S. 343-345 
    ISSN: 1476-4687
    Quelle: Nature Archives 1869 - 2009
    Thema: Biologie , Chemie und Pharmazie , Medizin , Allgemeine Naturwissenschaft , Physik
    Notizen: [Auszug] Lake Hoare (77°38f S, 162°53' E) is at the eastern end of Taylor Valley in southern Victoria Land, Antarctica. It is 58 m above sea level, 4.1 km long, 1.0 km wide, with a surface area of 1.8 km2, a maximum depth of 34 m, and a mean depth of 14.2 m. The perennial ice cover of Lake Hoare ...
    Materialart: Digitale Medien
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  • 4
    ISSN: 1476-4687
    Quelle: Nature Archives 1869 - 2009
    Thema: Biologie , Chemie und Pharmazie , Medizin , Allgemeine Naturwissenschaft , Physik
    Notizen: [Auszug] Microbialites are organosedimentary structures that can be constructed by a variety of metabolically distinct taxa. Consequently, microbialite structures abound in the fossil record, although the exact nature of the biogeochemical processes that produced them is often unknown. One such ...
    Materialart: Digitale Medien
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  • 5
    ISSN: 1476-4687
    Quelle: Nature Archives 1869 - 2009
    Thema: Biologie , Chemie und Pharmazie , Medizin , Allgemeine Naturwissenschaft , Physik
    Notizen: [Auszug] The average air temperature at the Earth's surface has increased by 0.06 °C per decade during the 20th century, and by 0.19 °C per decade from 1979 to 1998. Climate models generally predict amplified warming in polar regions, as observed in Antarctica's peninsula ...
    Materialart: Digitale Medien
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  • 6
    Digitale Medien
    Digitale Medien
    [s.l.] : Nature Publishing Group
    Nature 383 (1996), S. 780-780 
    ISSN: 1476-4687
    Quelle: Nature Archives 1869 - 2009
    Thema: Biologie , Chemie und Pharmazie , Medizin , Allgemeine Naturwissenschaft , Physik
    Notizen: [Auszug] The Case for Mars: The Plan to Settle the Red Planet and Why We Must. By Robert Zubrin with Richard Wagner. Free Press: 1996. Pp. 318. $25, £16.99. "THE Case for Mars" is the title of a series of conferences held at the University of Colorado every three years since 1980. The goal of the ...
    Materialart: Digitale Medien
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  • 7
    Digitale Medien
    Digitale Medien
    [s.l.] : Nature Publishing Group
    Nature 375 (1995), S. 26-27 
    ISSN: 1476-4687
    Quelle: Nature Archives 1869 - 2009
    Thema: Biologie , Chemie und Pharmazie , Medizin , Allgemeine Naturwissenschaft , Physik
    Notizen: [Auszug] TERRAFORMING - a wonderfully self-defining word that means altering another planet to make it Earth-like - is not what it used to be. Once the sole province of science fiction, terraforming - at least as applied to Mars - is now seriously discussed by space scientists. In ...
    Materialart: Digitale Medien
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  • 8
    Digitale Medien
    Digitale Medien
    [s.l.] : Macmillian Magazines Ltd.
    Nature 412 (2001), S. 61-64 
    ISSN: 1476-4687
    Quelle: Nature Archives 1869 - 2009
    Thema: Biologie , Chemie und Pharmazie , Medizin , Allgemeine Naturwissenschaft , Physik
    Notizen: [Auszug] Nitrogen is an essential element for life and is often the limiting nutrient for terrestrial ecosystems. As most nitrogen is locked in the kinetically stable form, N2, in the Earth's atmosphere, processes that can fix N2 into biologically available forms—such as ...
    Materialart: Digitale Medien
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  • 9
    ISSN: 1432-2056
    Quelle: Springer Online Journal Archives 1860-2000
    Thema: Biologie
    Notizen: Summary A satellite mediated station for monitoring nanoclimate (climate in the millimeter range) data, suitable for use in polar regions is described. The station, located in the Ross desert of Antarctica, has been in operation for more than 3 years, measuring rock temperatures, air temperature, light, snow, wind, and moisture. The data indicate that biological activity in the cryptoendolithic microbial ecosystem is limited to the period from mid November to mid February. The total number of hours of biological activity, based on assumptions of the minimum light, temperature and moisture requirements of the community, is less than 1000 h/year. The time above 0°C, representing more nearly optimal conditions, is between 50 and 550 h/year, depending on the orientation of the surface.
    Materialart: Digitale Medien
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  • 10
    Digitale Medien
    Digitale Medien
    Springer
    Journal of paleolimnology 13 (1995), S. 267-283 
    ISSN: 1573-0417
    Schlagwort(e): Mars ; martian paleolakes ; lacustrine sediments ; ice-covered lakes
    Quelle: Springer Online Journal Archives 1860-2000
    Thema: Biologie , Geologie und Paläontologie
    Notizen: Abstract Observational evidence such as outflow channels and valley networks suggest that in the past there was flowing water on Mars. The images of fluvial features on Mars logically suggest that there must exist downstream locations in which the water pooled and the sediment load deposited (i.e. lakes). Sediments and morphological features associated with the martian paleolakes are believed to occur in Valles Marineris, and several large basins including Amazonis, Chryse and Elysium planitia. As Mars became progressively colder over geological time, any lakes on its surface would have become seasonally, and eventually perennially ice-covered. We know from polar lakes on Earth that ice-covered lakes can persist even when the mean annual temperature falls below freezing. Thus, the most recent lacustrine sediments on Mars were probably deposited in ice-covered lakes. While life outside of the Earth's atmosphere has yet to be observed, there is a general consensus among exobiologists that the search for extraterrestrial life should be based upon liquid water. The inference that there was liquid water on Mars during an earlier epoch is the primary motivation for considering the possibility of life during this time. It would be of enormous interest from both an exobiological and paleolimnological perspective to discover lakes or the evidence of former lakes on another planet such as Mars. Limnology would then become an interplanetary science.
    Materialart: Digitale Medien
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