High-precision magnesium isotope measurements of whole chondrules from the
Allende carbonaceous chondrite meteorite show that some aluminum-rich Allen
de chondrules formed at or near the time of formation of calcium-aluminum-r
ich intrusions and that some others formed later and incorporated precursor
s previously enriched in magnesium-26. Chondrule magnesium-25/ magnesium-24
correlates with [magnesium]/[aluminum] and size, the aluminum-rich, smalle
r chondrules being the most enriched in the heavy isotopes of magnesium. Th
ese relations imply that high gas pressures prevailed during chondrule form
ation in the solar nebula.