The link between H chondrites and silicate inclusions in group IIE iro
n meteorites has long been suspected, but direct evidence for a common
parentage has remained elusive. The discovery of an unmelted chondrit
ic inclusion in the Techado iron meteorite sheds light on the genetic
relation between these two groups, providing clues on the origin of ch
ondritic materials as inclusions in iron meteorites. It is proposed th
at the complex IIE iron meteorite breccias formed by collisions with s
everal different bodies, followed by deep burial of metal and silicate
fragments in the asteroidal megaregolith.