A 220 x 430 mum Mg-Al-chromite fragment in the Raguli H3.8 ordinary ch
ondrite exhibits distinct optical and compositional zoning. The dark c
entral region of the Mg-Al-chromite is enriched in MgO, Al2O3 and ZnO
and depleted in TiO2, Cr2O3, FeO and MnO relative to the lighter outer
region. A subhedral olivine grain attached to radiating euhedral ilme
nites is present in the central region of the fragment. One of the ilm
enite crystals contains a tiny grain (0.5 x 5.8 mum) of baddeleyite (Z
rO2). Two end-member pyrophanite grains (MnTiO3) occur in the outer po
rtion of the fragment. This is the first occurrence of pyrophanite and
baddeleyite in an ordinary chondrite. Although it is possible that th
e Mg-Al-chromite fragment was derived from an achondritic projectile o
f unusual composition, we offer two alternative models for its formati
on. These include (a) a multi-stage process involving nebular melting
of a chromian-spinel chondrule that had accreted some olivine-bearing,
Mn-rich material followed by metamorphism on the parent body, and (b)
formation of the fragment on a metamorphosed parent body from an impa
ct melt of a chromite-rich assemblage containing Mn-rich ilmenite. We
favor the latter alternative.