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 …
The short-lived 182Hf–182W isotope system can provide powerful constraints on the timescales of planetary core formation, but its application to iron meteorites is hampered by …
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 …
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 …
An obstacle for establishing the chronology of iron meteorite formation using 182 Hf–182 W systematics (t 1/2= 8.9 Myr) is to find proper neutron fluence monitors to correct for cosmic …
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 …
We determined the Fe isotope fractionation between the metal and silicate phases of two aubrite meteorites, Norton County and Mount Egerton. We find that the metallic phase is …
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 …
MF Horan, MI Smoliar, RJ Walker - Geochimica et Cosmochimica Acta, 1998 - Elsevier
W isotopic compositions (measured by N-TIMS) in five iron meteorite groups are used in conjunction with 187Re-187Os isotopic data to constrain the timing of metal segregation and …