Diogenite meteorites are thought to represent mantle rocks that formed as cumulates in magma chambers on 4 Vesta or a similar differentiated asteroid. Microstructural analysis of olivine grains from a diogenite meteorite show that the preferred orientation of their crystal lattice was formed through plastic deformation, indicating dynamic, planet-like processes in its parent body.
- B. J. Tkalcec
- G. J. Golabek
- F. E. Brenker