A petrological study of 270 ordinary chondrites (115 H, 116 L and 39 L
(LL) + (LL) revealed chromite chondzules and inclusions occuring mainl
s among H (73%) chondrites; they are less common in L (21%) and L(LL)
(6%) chondrites. There are no obvious correlations between the occurre
nce of Chr-objects and petrological types or shock stages of the meteo
rite hosts. These inclusions consist mostly of chromite + plagioclase
(or plagioclase-like glass) and accessory ilmenite, high-Ca pyroxene,
merrillite and (or) chlorapatite. Based on mineralogy and chemistry th
e inclusions can be divided into two types: (1) Those consisting of lo
w-Al chromite (Al2O3 < 8.5%), uniform in composition and feldspar of v
ariable Na-K-composition. (2) Consisting of hign-Al chromite (Al2O3 >
9%), often variable in composition and feldspar of variable Na-Ca comp
osition. Chr-objects are a subst of Al-rich objects that contain more
than 10 wt% bulk Al2O3 but they have higher contents of Cr2O3 and FeO
and lower contents of SiO2 and MgO than the other Al-rich objects. Mod
els for the formation of Chr-objects include the following: (1) meltin
g and incomplete evaporation of presolar lumps, this resulted in enric
hment of the residue in Cr and Al; (2) formation of Chr-rich objects f
rom oxidized precursor materials that originally consisted of Cr-P-Si-
rich metal; (3) alteration of Sp-inclusions during parent-body metamor
phism.