Astronomy and Astrophysics – Astronomy
Scientific paper
May 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975gecoa..39..569b&link_type=abstract
Geochimica et Cosmochimica Acta, vol. 39, May 1975, p. 569-584.
Astronomy and Astrophysics
Astronomy
65
Condensates, Fractionation, Rare Earth Elements, Solar System, Yttrium, Abundance, Astronomical Models, Planetary Evolution, Planetary Nebulae, Stellar Evolution, Thermodynamic Equilibrium
Scientific paper
The condensation of Y and the rare earth elements (REE) from the solar nebula may be controlled by thermodynamic equilibrium between gas and condensed solids. Highly fractionated REE patterns may result if condensates are removed from the gas before condensation is complete. It is found that the fractionation is not a smooth function of REE ionic radius but varies in an extremely irregular pattern. Both Yb and Eu are predicted to be extremely depleted in the early condensate without the requirement of condensation in the divalent state. The model is discussed with respect to a highly fractionated pattern observed by Tanaka and Masuda (1973), in a pink Ca-Al-rich inclusion from the Allende meteorite and can account for the abundances of each REE determined. According to the model this inclusion represents a condensate from a previously fractionated gas rather than from a gas of solar composition. Before the condensation of this inclusion, an earlier condensate was formed and was removed from equilibrium with the gas.
No associations
LandOfFree
Fractionation in the solar nebula - Condensation of yttrium and the rare earth elements does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Fractionation in the solar nebula - Condensation of yttrium and the rare earth elements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fractionation in the solar nebula - Condensation of yttrium and the rare earth elements will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1048512