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Tempe, Arizona 85287–1604, USA 2 Center for Meteorite Studies, Arizona State University, Tempe, Arizona...less than 10 nmole g1 of meteorite and a maximum of 6.8 nmole g1 of meteorite for suberic acid in SM12...and of some stones of the C2-ungrouped Tagish Lake meteorite, where they are abundant and varied. Powder...combination of molecular species original to the meteorite as well as secondary products formed during parent-body...heating. INTRODUCTION The Sutter’s Mill (SM) meteorite a carbonaceous chondrites that fell in 2012, was |
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The oxygen isotopic composition of water from Tagish Lake: Its relationship to low-temperature phases and...ofpapers on the Tagish Lake meteorite) Abstract-The fall and recovery of the Tagish Lake meteorite in British...stepped pyrolysis from a bulk sample of this meteorite have allowed us to make comparisons with similar...terrestrial signature in Tagish Lake is indicative of the pristine nature of the meteorite. The relationship...parent-body aqueous alteration occurred. In Tagish Lake the difference in ~ 170 isotopic composition |
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groups (designated here as A through D). Spectral group A includes type 1 and 2 chondrites and exhibits...peaks. Spectral group B includes the least metamorphosed type 3 chondrites and Tagish Lake, and exhibits...spectral group C, the carbonyl stretching is assigned to cyclic unsaturated lactones; in spectral group D carbonyl...between spectral grouping and chondrite class or group. Ó 2011 Elsevier Ltd. All rights reserved. 1. INTRODUCTION...over a wide range of chondrites of different class, group, and petrologic type has not been performed. Here |
| Baú, João Paulo T., Villafañe-Barajas, Sául A., da Costa, Antônio Carlos S., Negrón-Mendoza, Alicia, Colín-Garcia, María, Zaia, Dimas A.M. (2020) Adenine Adsorbed onto Montmorillonite Exposed to Ionizing Radiation: Essays on Prebiotic Chemistry. Astrobiology, 20 (1) 26-38 doi:10.1089/ast.2018.1909 | Journal (article/letter/editorial) |
transform infrared spectroscopy showed that NH2 group and electrostatic interactions, between negatively...montmorillonite (2:1 clay), a phyllosilicate from the smectite group, is a good organicmolecule-adsorbent material...performed sequential leaching of the meteorite samples from Tagish Lake. They obtained the following order...anions SO42- >> Cl-. It should be noted that Tagish lake meteorite samples are probably one of the oldest materials...negatively charged, and (2) interaction of the –NH2 group of adenine with montmorillonite. The shift of the |
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continuity of magnesiosilica material with a mostly smectite-dehydroxylate composition. The results may have...olivine and pyroxene crystals to serpentine and smectite, respectively, will not be efficient under nebula...that layer silicates were found in the Tagish Lake meteorite, which has D-type IR spectral features (Brown...(Jessberger et al. 1988) and could include Na-bearing smectite (Rietmeijer et al. 1989). Another reason that...nm × 12 nm) formed in amorphous magnesiosilica smectite-dehydroxylate material after hydration above 357 |
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and the band center of the 3-lm feature. The first group, which we call ‘‘sharp’’, exhibits a sharp 3-lm...asteroids in this group are located in the 2.5 < a < 3.3 AU region. The second group, which we call ‘‘Ceres-like’’...absorption feature from 2.8 to 3.7 lm. The third group, which we call ‘‘Europa-like’’, includes 52 Europa...Euphrosyne, and 451 Patientia. Objects in this group exhibit a 3-lm feature with a band center of 3.15...concentrated in the 2.5 < a < 3.3 AU region. The fourth group, which we call ‘‘rounded’’, is concentrated in the |
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University, Sapporo, 001-0021, Japan, 3Antarctic Meteorite Research Center, National Institute of Polar Research...to one of the most primitive meteorites. This meteorite contains highly abundance of presolar grains [1]...anticipated [6]. [6] observed that Fe,Ni metal in this meteorite was invariably and extensively altered to form...small in the low ∆17O end (H-group) and becomes larger in high ∆17O end (LL-group). It is plausible that the...increasing metamorphism, reaching ~12,000‰ in one meteorite. This enrichment is almost 4 times that in the |
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. . . . . . . . . . . . . . . . . . . Calcite Group, 3̄2/m . . . . . . . . . . . . . . . . . . . . ... . . . . . . . . . . . . . . . . . . Aragonite Group, 2/m2/m2/m. . . . . . . . . . . . . . . . . . ..... . . . . . . . . . . . . . . . . . . Dolomite Group. . . . . . . . . . . . . . . . . . . . . . . . ... . . . . . . . . . . . . . . Azurite-Malachite Group. . . . . . . . . . . . . . . . . . . . . . . . ...different directions (. Fig. 1.3). . Fig. 1.1 Group of quartz crystals, Arkansas, USA, approximately |
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FIB sections retrieved from the matrix of each meteorite using a Talos F200X. All observations were conducted...temperatures below the domain represented by the group term “heated CMs” [e.g. 8-11]. Whereas all silicates... [14] Schrader & Davidson (submitted) GCA. METEORITE MATERIAL MODEL FOR STRUCTURAL PROPERTIES Parul...needed to achieve this objective. At present, the meteorite material found on earth are the only objects from...properties for the entire family of asteroids, meteorite unit models are developed to determine the effective |
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atoms and one or more carbon atoms of an organyl group. In addition to the traditional metals and semimetals...reported in Fig. 1.5 like: identify the symmetry group from the geometry, fix a reference axial system...Organic-Mineral Interactions in Meteorites The Murchison meteorite classified as a carbon rich carbonaceous chondrite...C=O were found. Furthermore, in the Murchinson meteorite OH and aliphatic molecules coexist, re-confirming...organic matter and phyllosilicates. In the Bells meteorite the organic matter showed a spatial bead-like |
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Strashimir Borisov Strashimirov, University of Mining and Geology “St. Ivan Rilski” (BG), Nada Vasković................................245 EG52 Platinum-group minerals in the new millennium....................Geological Sciences, University of Manitoba, Winnipeg, Canada (frank_hawthorne@umanitoba.ca) Recent advances...consideration remains the environmental impacts of mining uranium and the final disposition of nuclear wastes...dominant, negligible amount of interstratified illite-smectite was detected. Plagioclase, Ca-dominant, was detected |
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recognized by the Meteoritical Society as Barringer Meteorite Crater. When one reads Barringer and Tilghman’s...papers are the outcome of a conference—Large Meteorite Impacts and Planetary Evolution—held every five...the immense Sudbury impact structure in Ontario, Canada, where this series of conferences commenced in... We welcome you to the fifth volume of Large Meteorite Impacts and Planetary Evolution. Gordon R. Osinski...in Osinski, G.R., and Kring, D.A., eds., Large Meteorite Impacts and Planetary Evolution V: Geological |