The 182 Hf-182 W chronology of iron meteorites provides crucial information on the timescales of accretion and differentiation of some of the oldest planetesimals of the Solar …
The application of Hf–W chronometry to determine the timescales of core formation in the parent bodies of magmatic iron meteorites is severely hampered by 182W burnout during …
A Markowski, I Leya, G Quitté, K Ammon… - Earth and Planetary …, 2006 - Elsevier
Core formation in planetesimals can, in principle, be dated using the short-lived 182Hf– 182W chronometer. However, it has been predicted that burnout and production of W …
New, high-precision W isotope data on iron meteorites are presented that provide important constraints on the timing of silicate–metal segregation in planetesimals. Magmatic iron …
Tungsten isotope compositions of magmatic iron meteorites yield ages of differentiation that are within±2Ma of the formation of CAIs, with the exception of IVB irons that plot to …
To constrain the timescales and processes involved in the crystallization and cooling of protoplanetary cores, we examined the Pd-Ag isotope systematics of the IVA iron meteorites …
AN Halliday, T Kleine - Meteorites and the early solar system …, 2006 - ui.adsabs.harvard.edu
Isotopic studies of meteorites provide the fundamental data for determining how the terrestrial planets, including Earth, accreted. Over the past few years there have been major …
Iron meteorites provide some of the most direct insights into the processes and timescales of core formation in planetesimals. Of these, group IVB irons stand out by having one of the …
New high-precision W isotope measurements are presented for 33 iron meteorites from 8 magmatic groups (IC, IIAB, IID, IIIAB, IIIE, IIIF, I VA and IVB), 2 non-magmatic groups (IAB …