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  • 1
    Publication Date: 2011-10-25
    Description: Icy bodies may have delivered the oceans to the early Earth, yet little is known about water in the ice-dominated regions of extrasolar planet-forming disks. The Heterodyne Instrument for the Far-Infrared on board the Herschel Space Observatory has detected emission lines from both spin isomers of cold water vapor from the disk around the young star TW Hydrae. This water vapor likely originates from ice-coated solids near the disk surface, hinting at a water ice reservoir equivalent to several thousand Earth oceans in mass. The water's ortho-to-para ratio falls well below that of solar system comets, suggesting that comets contain heterogeneous ice mixtures collected across the entire solar nebula during the early stages of planetary birth.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hogerheijde, Michiel R -- Bergin, Edwin A -- Brinch, Christian -- Cleeves, L Ilsedore -- Fogel, Jeffrey K J -- Blake, Geoffrey A -- Dominik, Carsten -- Lis, Dariusz C -- Melnick, Gary -- Neufeld, David -- Panic, Olja -- Pearson, John C -- Kristensen, Lars -- Yildiz, Umut A -- van Dishoeck, Ewine F -- New York, N.Y. -- Science. 2011 Oct 21;334(6054):338-40. doi: 10.1126/science.1208931.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Leiden Observatory, Leiden University, Post Office Box 9513, 2300 RA Leiden, Netherlands. michiel@strw.leidenuniv.nl〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22021851" target="_blank"〉PubMed〈/a〉
    Keywords: Evolution, Planetary ; Extraterrestrial Environment ; *Ice ; *Planets ; *Stars, Celestial ; *Steam
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2014-09-27
    Description: Identifying the source of Earth's water is central to understanding the origins of life-fostering environments and to assessing the prevalence of such environments in space. Water throughout the solar system exhibits deuterium-to-hydrogen enrichments, a fossil relic of low-temperature, ion-derived chemistry within either (i) the parent molecular cloud or (ii) the solar nebula protoplanetary disk. Using a comprehensive treatment of disk ionization, we find that ion-driven deuterium pathways are inefficient, which curtails the disk's deuterated water formation and its viability as the sole source for the solar system's water. This finding implies that, if the solar system's formation was typical, abundant interstellar ices are available to all nascent planetary systems.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Cleeves, L Ilsedore -- Bergin, Edwin A -- Alexander, Conel M O'D -- Du, Fujun -- Graninger, Dawn -- Oberg, Karin I -- Harries, Tim J -- New York, N.Y. -- Science. 2014 Sep 26;345(6204):1590-3. doi: 10.1126/science.1258055.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Astronomy, University of Michigan, 311 West Hall, 1085 South University Avenue, Ann Arbor, MI 48109, USA. cleeves@umich.edu. ; Department of Astronomy, University of Michigan, 311 West Hall, 1085 South University Avenue, Ann Arbor, MI 48109, USA. ; Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA. ; Harvard-Smithsonian Center for Astrophysics, Harvard University, Cambridge, MA 02138, USA. ; Department of Physics and Astronomy, University of Exeter, Stocker Road, Exeter EX4 4QL, UK.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25258075" target="_blank"〉PubMed〈/a〉
    Keywords: Deuterium/chemistry ; Earth (Planet) ; *Ice ; Origin of Life ; *Solar System
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 3
    Publication Date: 2011-10-07
    Description: For decades, the source of Earth's volatiles, especially water with a deuterium-to-hydrogen ratio (D/H) of (1.558 +/- 0.001) x 10(-4), has been a subject of debate. The similarity of Earth's bulk composition to that of meteorites known as enstatite chondrites suggests a dry proto-Earth with subsequent delivery of volatiles by local accretion or impacts of asteroids or comets. Previous measurements in six comets from the Oort cloud yielded a mean D/H ratio of (2.96 +/- 0.25) x 10(-4). The D/H value in carbonaceous chondrites, (1.4 +/- 0.1) x 10(-4), together with dynamical simulations, led to models in which asteroids were the main source of Earth's water, with 〈/=10 per cent being delivered by comets. Here we report that the D/H ratio in the Jupiter-family comet 103P/Hartley 2, which originated in the Kuiper belt, is (1.61 +/- 0.24) x 10(-4). This result substantially expands the reservoir of Earth ocean-like water to include some comets, and is consistent with the emerging picture of a complex dynamical evolution of the early Solar System.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hartogh, Paul -- Lis, Dariusz C -- Bockelee-Morvan, Dominique -- de Val-Borro, Miguel -- Biver, Nicolas -- Kuppers, Michael -- Emprechtinger, Martin -- Bergin, Edwin A -- Crovisier, Jacques -- Rengel, Miriam -- Moreno, Raphael -- Szutowicz, Slawomira -- Blake, Geoffrey A -- England -- Nature. 2011 Oct 5;478(7368):218-20. doi: 10.1038/nature10519.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Max-Planck-Institut fur Sonnensystemforschung, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany. hartogh@mps.mpg.de〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21976024" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 4
    Publication Date: 2013-02-01
    Description: From the masses of the planets orbiting the Sun, and the abundance of elements relative to hydrogen, it is estimated that when the Solar System formed, the circumstellar disk must have had a minimum mass of around 0.01 solar masses within about 100 astronomical units of the star. (One astronomical unit is the Earth-Sun distance.) The main constituent of the disk, gaseous molecular hydrogen, does not efficiently emit radiation from the disk mass reservoir, and so the most common measure of the disk mass is dust thermal emission and lines of gaseous carbon monoxide. Carbon monoxide emission generally indicates properties of the disk surface, and the conversion from dust emission to gas mass requires knowledge of the grain properties and the gas-to-dust mass ratio, which probably differ from their interstellar values. As a result, mass estimates vary by orders of magnitude, as exemplified by the relatively old (3-10 million years) star TW Hydrae, for which the range is 0.0005-0.06 solar masses. Here we report the detection of the fundamental rotational transition of hydrogen deuteride from the direction of TW Hydrae. Hydrogen deuteride is a good tracer of disk gas because it follows the distribution of molecular hydrogen and its emission is sensitive to the total mass. The detection of hydrogen deuteride, combined with existing observations and detailed models, implies a disk mass of more than 0.05 solar masses, which is enough to form a planetary system like our own.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Bergin, Edwin A -- Cleeves, L Ilsedore -- Gorti, Uma -- Zhang, Ke -- Blake, Geoffrey A -- Green, Joel D -- Andrews, Sean M -- Evans, Neal J 2nd -- Henning, Thomas -- Oberg, Karin -- Pontoppidan, Klaus -- Qi, Chunhua -- Salyk, Colette -- van Dishoeck, Ewine F -- England -- Nature. 2013 Jan 31;493(7434):644-6. doi: 10.1038/nature11805.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, Michigan 48109, USA. ebergin@umich.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23364742" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 5
    Publication Date: 2015-04-10
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Blake, Geoffrey A -- Bergin, Edwin A -- England -- Nature. 2015 Apr 9;520(7546):161-2. doi: 10.1038/520161a.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA. ; Department of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25855449" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 6
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 442 (2006), S. 425-427 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Nitrogen is the fifth most abundant element in the Universe. In the interstellar medium, it has been thought to be mostly molecular (N2). However, N2 has no observable rotational or vibrational transitions, so its abundance in the interstellar medium remains poorly known. ...
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  • 7
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 78 (1997), S. 29-35 
    ISSN: 1573-0794
    Keywords: Comets ; interstellar molecules
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract The abundance ratio of the isomers HCN and HNC has been investigated in comet Hale-Bopp (C/1995 O1) through observations of the J = 4−3 rotational transitions of both species for heliocentric distances 0.93 〈 r 〈 3 AU, both pre- and post-perihelion. After correcting for the optical depth of the stronger HCN line, we find that the column density ratio of HNC/HCN in our telescope beam increases significantly as the comet approaches the Sun. We compare this behavior to that predicted from an ion-molecule chemical model and conclude that the HNC is produced insignificant measure by chemical processes in the coma; i.e., for comet Hale-Bopp, HNC is not a parent molecule sublimating from the nucleus.
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 77 (1997), S. 253-258 
    ISSN: 1573-0794
    Keywords: Comets ; HCO+ ; chemistry ; plasmas
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Maps of comet C/1995 O1 (Hale-Bopp) in the millimeter-wave emission of the ion HCO+ revealed a local minimum near the nucleus position, with a maximum about 100,000 km in the antisolar direction. These observed features of the HCO+ emission require a low abundance of HCO+ due to enhanced destruction in the inner coma of the comet, within a region of low electron temperature (Te). To set constraints on the formation of HCO+ in the coma, as well as the location and magnitude of the transition to higher Te, the data are compared with the results of ion-molecule chemistry models.
    Type of Medium: Electronic Resource
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  • 9
  • 10
    Publication Date: 2013-12-01
    Print ISSN: 0004-6361
    Electronic ISSN: 1432-0746
    Topics: Physics
    Published by EDP Sciences
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