A unified chronology of dust formation in the early solar system
The chronology of dust formation in the early solar system remains controversial.
Chondrules are the most abundant high-temperature objects formed during the evolution of …
Chondrules are the most abundant high-temperature objects formed during the evolution of …
Volatile element chemistry during accretion of the Earth
We review some issues relevant to volatile element chemistry during accretion of the Earth
with an emphasis on historical development of ideas during the past century and on issues …
with an emphasis on historical development of ideas during the past century and on issues …
Igneous meteorites suggest Aluminium-26 heterogeneity in the early Solar Nebula
The short-lived radionuclide aluminium-26 (26Al) isotope is a major heat source for early
planetary melting. The aluminium-26–magnesium-26 (26Al-26Mg) decay system also …
planetary melting. The aluminium-26–magnesium-26 (26Al-26Mg) decay system also …
[HTML][HTML] Linking asteroids and meteorites to the primordial planetesimal population
RC Greenwood, TH Burbine, IA Franchi - Geochimica et Cosmochimica …, 2020 - Elsevier
Meteorites provide a unique insight into early Solar System processes. However, to fully
interpret this record requires that these meteorites are related back to their source asteroids …
interpret this record requires that these meteorites are related back to their source asteroids …
A 4,565-My-old andesite from an extinct chondritic protoplanet
JA Barrat, M Chaussidon… - Proceedings of the …, 2021 - National Acad Sciences
The age of iron meteorites implies that accretion of protoplanets began during the first
millions of years of the solar system. Due to the heat generated by 26Al decay, many early …
millions of years of the solar system. Due to the heat generated by 26Al decay, many early …
Carbonaceous achondrites Northwest Africa 6704/6693: Milestones for early Solar System chronology and genealogy
Abstract Northwest Africa (NWA) 6704/6693 are medium-to coarse-grained achondrites with
unique petrologic and geochemical traits that are distinct from the currently established …
unique petrologic and geochemical traits that are distinct from the currently established …
[HTML][HTML] Early solar system chronology from short-lived chronometers
Age constraints on early solar system processes and events can be derived from meteorites
and their components using different radioisotope systems. Due to the short time interval …
and their components using different radioisotope systems. Due to the short time interval …
Al-Mg and U-Pb chronological records of Erg Chech 002 ungrouped achondrite meteorite
Achondrite meteorites are remnants of the earliest planetary differentiation processes in the
Solar System. They have been used to anchor short-lived radiochronometers to absolute …
Solar System. They have been used to anchor short-lived radiochronometers to absolute …
Radiogenic chromium isotope evidence for the earliest planetary volcanism and crust formation in the Solar system
Erg Chech (EC) 002 is a meteorite with andesitic composition, potentially recording the lava
crystallization and crust formation of its parent body. Nucleosynthetic Cr isotope composition …
crystallization and crust formation of its parent body. Nucleosynthetic Cr isotope composition …
Statistical chronometry of meteorites. I. A Test of 26Al homogeneity and the Pb-Pb age of the solar system'st= 0
We use rapidly cooled achondrites to test the assumption of 26 Al homogeneity in the solar
nebula, by checking if there is a single value of t SS, the absolute “Pb-Pb” age of the Solar …
nebula, by checking if there is a single value of t SS, the absolute “Pb-Pb” age of the Solar …