Results 141 to 150 of about 446 (179)
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Meteoritics & Planetary Science, 2002
Abstract— We measured the sizes and textural types of 719 intact chondrules and 1322 chondrule fragments in thin sections of Semarkona (LL3.0), Bishunpur (LL3.1), Krymka (LL3.1), Piancaldoli (LL3.4) and Lewis Cliff 88175 (LL3.8). The mean apparent diameter of chondrules in these LL3 chondrites is 0.80 φ units or 570 μm, much smaller than the previous ...
Victoria E. Nelson, Alan E. Rubin
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Abstract— We measured the sizes and textural types of 719 intact chondrules and 1322 chondrule fragments in thin sections of Semarkona (LL3.0), Bishunpur (LL3.1), Krymka (LL3.1), Piancaldoli (LL3.4) and Lewis Cliff 88175 (LL3.8). The mean apparent diameter of chondrules in these LL3 chondrites is 0.80 φ units or 570 μm, much smaller than the previous ...
Victoria E. Nelson, Alan E. Rubin
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Impact jetting as the origin of chondrules
Nature, 2015Chondrules are the millimetre-scale, previously molten, spherules found in most meteorites. Before chondrules formed, large differentiating planetesimals had already accreted. Volatile-rich olivine reveals that chondrules formed in extremely solid-rich environments, more like impact plumes than the solar nebula.
Brandon C, Johnson +3 more
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Chondrules: Suggestion Concerning the Origin
Science, 1966The millimeter-sized, sometimes glassy spheroids called chondrules that occur abundantly in stony meteorites may have been produced by lightning in the primitive Laplacian-type nebula while earthy materials were condensing and collecting to form the asteroids and the terrestrial planets.
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Abstract Chondrules are millimeter-scale rocky particles that occur as the dominant component in most chondrite meteorites. Chondrules formed within the first few million years of formation of the first solids in the solar system, 4,562–4,567 million years ago.
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Early Evolution of the Solar Accretion Disk Inferred From Cr-Ti-O Isotopes in Individual Chondrules
Earth and Planetary Science Letters, 2020Yves Marrocchi +2 more
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