HED Diogenite - NWA 14917 - Asteroid 4 Vesta Fragment - 19.55 g

Diogenite refers to a subgroup of HED meteorites, believed to originate from the asteroid 4 Vesta, one of the largest bodies in the asteroid belt. These meteorite fragments provide unique insights into the early solar system's differentiation processes.

A 19.55 gram piece of Diogenite is significant for collectors and researchers alike, as these stony meteorites consist predominantly of orthopyroxene and are relatively rare compared to other meteorite types. Their composition reflects deep crustal or mantle material from Vesta, making them valuable for planetary science.

Owning or studying such meteorites connects us to extraterrestrial geology, offering a window into the formation history of our solar system and the processes shaping rocky bodies beyond Earth.