Meteorites and the Early Solar System
TLDR
Chondrite classification, primordial matter composition and early solar system chemical processes, discussing cosmic gas condensation and refractory element fractionation are discussed in this paper, with a focus on early solar systems chemical processes.Abstract:
Chondrite classification, primordial matter composition and early solar system chemical processes, discussing cosmic gas condensation and refractory element fractionationread more
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The composition of the Earth
William F. McDonough,Shen-Su Sun +1 more
TL;DR: In this paper, the authors compared the relative abundances of the refractory elements in carbonaceous, ordinary, and enstatite chondritic meteorites and found that the most consistent composition of the Earth's core is derived from the seismic profile and its interpretation, compared with primitive meteorites, and chemical and petrological models of peridotite-basalt melting relationships.
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Abundances of the elements: Meteoritic and solar
Edward Anders,Nicolas Grevesse +1 more
TL;DR: In this article, new abundance tables have been compiled for C1 chondrites and the solar photosphere and corona, based on a critical review of the literature to mid-1988.
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Solar System Abundances and Condensation Temperatures of the Elements
TL;DR: In this article, solar photospheric and meteoritic CI chondrite abundance determinations for all elements are summarized and the best currently available photosphere abundances are selected, including the meteoritic and solar abundances of a few elements (e.g., noble gases, beryllium, boron, phosphorous, sulfur).
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Terrestrial in situ cosmogenic nuclides: theory and application
John C. Gosse,Fred M. Phillips +1 more
TL;DR: In this paper, the authors present the theory necessary for interpreting cosmogenic nuclide data, reviews estimates of parameters, describes strategies and practical considerations in field applications, and assesses sources of error in interpreting Cosmogenic Nuclide measurements.
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Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation
Koichi Iwamoto,F. Brachwitz,Ken'ichi Nomoto,N. Kishimoto,Hideyuki Umeda,W. Raphael Hix,Friedrich-Karl Thielemann,Friedrich-Karl Thielemann +7 more
TL;DR: In this paper, the authors calculate explosive nucleosynthesis in relatively slow deflagrations with a variety of deflagration speeds and ignition densities to put new constraints on the above key quantities.
References
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Book
Origin of the solar system
TL;DR: The current status of the classical model of solar-system formation is surveyed in this paper, reviewing the results of recent observational and theoretical investigations, including the formation of the sun, planetesimal accumulation, planetary accumulation, major planetary collisions, the development of planetary atmospheres, and comets.
Journal ArticleDOI
Origin of organic matter in early solar system—II. Nitrogen compounds
TL;DR: Organic matter origin in early solar system from carbonaceous meteorites composition, stressing nitrogen compounds was discussed in this paper, where the authors proposed a method to find the origin of organic matter from carbon-composition of meteorites.