Evaluation of petrologic evidence for high partial pressures of SiO(g) in the solar nebula
Alan E. Rubin LINK Meteorit Planet Sci. . doi:10.1111/maps.13180 “Although they cannot be ruled out, high partial pressures of SiO(g) in the solar nebula are not required to produce various petrologic features of chondrules. These…
Type-IAB Chondrules in LL3.0 Semarkona: No Need for High Partial Pressures of SiO(g) in the Solar Nebula
A. E. Rubin 48th Lunar and Planetary Science Conference (2017), Abstract #2700 PDF