Mifflin is a rare basaltic eucrite linked to the crust of asteroid Vesta, formed through ancient volcanic activity that produced its tight intergrowth of plagioclase and pyroxene. Unlike chondrites, eucrites come from differentiated bodies with real geological history, and Mifflin’s fine‑grained, coherent texture reflects repeated heating, cooling, and impact processing on a young protoplanet. Its 1844 fall in Wisconsin makes it one of the earliest documented meteorite events in the United States, valued for its clear connection to planetary crust formation and the evolution of small rocky worlds. Energetically, eucrites are chosen for their sharpening, clarifying influence — they cut through noise, stabilise focus, and support decisive movement by anchoring attention to what is structurally sound and genuinely progressing. Each specimen is housed in a clear acrylic display box (3.5 cm × 5.5 cm) with an identification label.
Includes:
1X MIFFLIN EUCRITE CHONDRITE METEORITE | APPROX 1.5CM
Mifflin - Eucrite Chondrite Meteorite - Wisconsin 1844
20% OFF EASTER SALE
MIFFLIN EUCRITE METEORITE CHONDRITE METEORITE
Mifflin is a crustal eucrite from the HED family, composed mainly of plagioclase and low‑calcium pyroxene that formed through volcanic activity on a differentiated asteroid. Its chemistry and texture preserve evidence of early basaltic crust, impact brecciation, and repeated thermal events that shaped the surfaces of young planetary bodies. Eucrites are often selected in energetic work for their clean, directive quality — they help consolidate intention, refine priorities, and reinforce the kind of grounded momentum that comes from acting with clarity rather than overwhelm.
