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interstellar water

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Spatial distribution and isotopic compositions of the different <span class="search-highlight">water</span> reser...
Published: 01 June 2022
enough (≤170 K) for water ice grains to form. ( B ) Distribution of D/H ratios for water in ordinary (OC) and carbonaceous (CV, CO, CM, CR, CI) chondrites, comets, and interstellar water ice. ( C ) Distribution of mass-independent oxygen isotopic anomalies (∆ 17 O) recorded by secondary minerals
Image
Scheme of <span class="search-highlight">interstellar</span> normal (H 2 O) and heavy <span class="search-highlight">water</span> (HDO) formation on th...
Published: 01 June 2022
Figure 2. Scheme of interstellar normal (H 2 O) and heavy water (HDO) formation on the surface of dust grains. ( left ) The HDO abundance surpasses that of the available D/H ratio because of the reaction between H 3+ and HD, the reservoir of deuterium, whose reverse reaction is inhibited
Journal Article
Journal: Elements
Published: 01 June 2022
Elements (2022) 18 (3): 149–153.
... , Robert F ( 1995 ) Interstellar water in meteorites? Geochimica et Cosmochimica Acta 59 : 4695 - 4706 , doi: 10.1016/0016-7037(95)00313-4 DeMeo FE , Carry B ( 2014 ) Solar System evolution from compositional mapping of the asteroid belt . Nature 505 : 629 - 634 , doi...
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Journal Article
Published: 01 October 2020
Geochemical Perspectives (2020) 9 (2): 274–283.
...-molecule exchange and/or interactions between solar/interstellar photons and the gas. Figure A3 Assembling the ingredients. • Left : In the inner-most regions of the disk, water ice could not exist. Chondrules are ≤1 mm diameter spherical assemblages of refractory silicates formed during...
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Journal Article
Published: 01 October 2020
American Mineralogist (2020) 105 (10): 1508–1535.
... < 20 K 2,3 Oxygen (O 2 ) [Interstellar oxygen] Most molecular oxygen reacts with H 2 to form H 2 O 4,5 Oxides Water (H 2 O) Interstellar cubic ice Diagnostic sharp IR emission features at 44 and 60 µm 6–8 Interstellar amorphous H 2 O Diagnostic O-H stretch at 3.05 µm 7–10...
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Journal Article
Journal: Elements
Published: 01 June 2022
Elements (2022) 18 (3): 175–180.
... enough (≤170 K) for water ice grains to form. ( B ) Distribution of D/H ratios for water in ordinary (OC) and carbonaceous (CV, CO, CM, CR, CI) chondrites, comets, and interstellar water ice. ( C ) Distribution of mass-independent oxygen isotopic anomalies (∆ 17 O) recorded by secondary minerals...
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Journal Article
Published: 01 January 2008
Reviews in Mineralogy and Geochemistry (2008) 68 (1): 55–72.
...% in crystalline enstatite and forsterite (Mg-rich end members) and 5–10% is contained in water ice, usually in its crystalline form ( Kemper et al. 2001 , 2002 ). The dust production by M supergiants, the other major contributors to the interstellar dust reservoir, is not easily described as a class, as it shows...
Journal Article
Published: 01 December 2007
European Journal of Mineralogy (2007) 19 (6): 771–782.
... interstellar matter: the ISO revolution , eds. L. d’Hendecourt , C. Joblin and A. Jones , EDP Sciences (les Ulis) , EDP Sciences-Springer-Verlag , 183 – 198 . Waters , L.B.F.M. ( 2004 ): Dust in evolved stars . in Astrophysics of Dust, ASP Conference Series , 309 , eds. A.N...
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Journal Article
Journal: Elements
Published: 01 June 2022
Elements (2022) 18 (3): 155–160.
...Figure 2. Scheme of interstellar normal (H 2 O) and heavy water (HDO) formation on the surface of dust grains. ( left ) The HDO abundance surpasses that of the available D/H ratio because of the reaction between H 3+ and HD, the reservoir of deuterium, whose reverse reaction is inhibited...
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Journal Article
Published: 01 January 2008
Reviews in Mineralogy and Geochemistry (2008) 68 (1): 247–272.
... Eberhardt P , Reber M , Krankowsky D , Hodges RR ( 1995 ) The D/H and 18 O/ 16 O- ratios in water from comet P/Halley . Astron Astrophys 302 : 301 – 316 Ehrenfreund P , Charnley SB ( 2000 ) Organic molecules in the interstellar medium, comets, and meteorites...
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Journal Article
Published: 01 January 2008
Reviews in Mineralogy and Geochemistry (2008) 68 (1): 187–218.
... fractionation in the early Solar System because it appeals to a process that apparently occurs in the interstellar medium, but it lacks experimental verification. Three astrophysical settings for CO self-shielding are proposed as sites for generating Δ 17 O variability in the early Solar System. One...
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Sketch of the four major steps involved in the formation of a planetary sys...
Published: 01 June 2022
Figure 1. Sketch of the four major steps involved in the formation of a planetary system similar to the Solar System and of water (C ourtesy of M. D e S imone ), as described in the text. STEP 1: In cold (≤10 K) and dense clumps, water is formed on the surface of the interstellar grains. STEP 2
Journal Article
Journal: Elements
Published: 01 April 2018
Elements (2018) 14 (2): 101–106.
... in the protoplanetary disk and allow us to unveil the formation history of the organics and volatiles. Copyright © 2018 by the Mineralogical Society of America 2018 Mineralogical Society of America organic molecules water carbon monoxide carbon dioxide sublimation processes volatiles Credit: ESA...
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Journal Article
Journal: Elements
Published: 01 April 2018
Elements (2018) 14 (2): 87–93.
... system. Cometary silicates appear to have formed in numerous hot solar system regions. Preserved interstellar grains are rare, unless they have eluded identification by having solar isotopic compositions. Copyright © 2018 by the Mineralogical Society of America 2018 Mineralogical Society of America...
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Journal Article
Journal: Elements
Published: 01 December 2016
Elements (2016) 12 (6): 401–406.
... the time of Earth's formation to the end of the late heavy bombardment at ~3.8 Ga. Abiogenic synthesis of organic compounds must have occurred in the atmosphere, in aqueous solutions, and at the mineral–water interface in multiple geological settings ( F ig . 1 ). It was once believed that organic...
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Journal Article
Published: 01 October 2020
Geochemical Perspectives (2020) 9 (2): 135–136.
... the deepest regions of the Earth, and what can they tell us about the processes occurring there? My approach has been to establish geochemical links between the noble gases, physical tracers par excellence , with major volatile elements of environmental importance, such as water, carbon and nitrogen...
Journal Article
Journal: Elements
Published: 01 April 2018
Elements (2018) 14 (2): 83–86.
... reactions with liquid water, or was that water always present in a frozen state? Beyond that, what is the structure of water ice in comet nuclei, does it preserve crystal structures revealing formation at the very low temperatures of interstellar space? How complex was organic evolution in cometary nuclei...
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Series: GSA Special Papers
Published: 01 January 1982
DOI: 10.1130/SPE190-p211
... The impact of a large body in the oceans would inject large quantities of water through the tropopause cold trap into the stratosphere and lower mesosophere. We consider the consequences of enhanced water vapor concentrations on the middle atmosphere (50–100 km) chemistry and heat budget...
Journal Article
Journal: Elements
Published: 01 August 2017
Elements (2017) 13 (4): 225–229.
...Edward S. Grew Boron is rare in the cosmos because its nucleus is “fragile.” So, how does one get from the interstellar medium, where boron was first produced, to Earth's upper continental crust where boron is concentrated in deposits containing remarkably diverse suites of boron minerals...
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Journal Article
Journal: Elements
Published: 01 February 2011
Elements (2011) 7 (1): 23–28.
.... The grains are samples of interstellar dust produced by dying stars. Their stable isotope ratios of Xe, Ne, 15 N/ 14 N, 13 C/ 12 C, 29 Si/ 28 Si, 30 Si/ 28 Si, 18 O/ 16 O, and 17 O/ 16 O differ by tens of percent (thousands per mil) from Solar System values. The anomalous stable isotope abundances can...
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