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Journal ArticleDOI

Origin and chronology of chondritic components: A review

TLDR
In this article, the x-wind model vs. the shock-wave model of the origin of chondritic components and irradiation vs. stellar origin of short-lived radionuclides are compared.
About
This article is published in Geochimica et Cosmochimica Acta.The article was published on 2009-09-01. It has received 200 citations till now. The article focuses on the topics: Chondrule & Chondrite.

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Journal ArticleDOI

The Absolute Chronology and Thermal Processing of Solids in the Solar Protoplanetary Disk

TL;DR: U-corrected Pb-Pb dating from primitive meteorites indicates that chondrule formation started contemporaneously with CAIs and lasted ~3 million years, suggesting that the formation ofCAIs and chondrules reflects a process intrinsically linked to the secular evolution of accretionary disks.
Book ChapterDOI

Chondrites and Their Components

TL;DR: In this article, the properties of carbonaceous, ordinary and enstatite chondrites focusing on the most pristine samples are reviewed to establish the chemical, isotopic, and mineralogical properties and origins of their components and to elucidate the asteroidal processes that modified them.
Journal ArticleDOI

U-Pb chronology of the Solar System's oldest solids with variable 238 U/ 235 U

TL;DR: In this article, the authors presented the first combined high-precision U and Pb isotopic data for a CAI, and U isotope data for chondrules and whole rock fractions of the Allende meteorite.
Journal ArticleDOI

Evidence for magnesium isotope heterogeneity in the solar protoplanetary disk

TL;DR: In this article, the authors report high-precision Mg-isotope measurements of inner solar system solids, asteroids, and planets demonstrating the existence of widespread heterogeneity in the mass independent 26Mg composition (μ26Mg*) of bulk solar system reservoirs with solar or near-solar Al/Mg ratios.
Journal ArticleDOI

Molybdenum isotope anomalies in meteorites: Constraints on solar nebula evolution and origin of the Earth

TL;DR: The early evolution of the solar nebula involved substantial transport of mass, resulting in mixing and homogenization of isotopically diverse materials that were contributed to the solar system from multiple stellar nucleosynthetic sources as mentioned in this paper.
References
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Book

Treatise on geochemistry

TL;DR: This extensively updated new edition of the widely acclaimed Treatise on Geochemistry has increased its coverage beyond the wide range of geochemical subject areas in the first edition, with five new volumes which include: the history of the atmosphere, geochemistry of mineral deposits, archaeology and anthropology, organic geochemistry and analytical geochemistry as discussed by the authors.
Journal ArticleDOI

Meteorites and the Early Solar System

TL;DR: 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.
Journal ArticleDOI

Rapid planetesimal formation in turbulent circumstellar disks

TL;DR: It is reported that boulders can undergo efficient gravitational collapse in locally overdense regions in the midplane of the disk, and it is found that gravitationally bound clusters form with masses comparable to dwarf planets and containing a distribution of boulder sizes.
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