This Specimen has been sold.
1.0" Eucrite Meteorite (5.2 g) End-Cut - NWA 11704
This is a 1.0" wide (5.2 gram) end-cut of the NWA 11704 eucrite meteorite. This is a gabbroic polymict breccia with both eucrite and diogenite clasts. A little over a kilogram was recovered and sold in Mauritania. The cut face is expertly polished on one side, displaying the various colorful clasts in the meteorite's interior. A beautiful addition to anyone's collection!
Eucrite Meteorites - Fragments Of 4 Vesta
Eucrites are achondritic stony meteorites thought to have originated from the surface of the giant asteroid (or minor planet) 4 Vesta. Vesta is the second largest body in the asteroid belt, measuring 326 miles wide. Like Earth, it has the differentiated layers of crust, mantle, and core common to rocky planets: this may mean that 4 Vesta is the remnant of a larger destroyed planet.
Eucrites consist of basaltic rock from Vesta's crust ejected during a collision with another asteroid. Eucrites are mostly composed of calcium-poor pyroxene, pigeonite, and calcium-rich plagioclase (anorthite). Vesta is currently one of just seven identified solar system bodies of which we have physical samples.
Eucrites are achondritic stony meteorites thought to have originated from the surface of the giant asteroid (or minor planet) 4 Vesta. Vesta is the second largest body in the asteroid belt, measuring 326 miles wide. Like Earth, it has the differentiated layers of crust, mantle, and core common to rocky planets: this may mean that 4 Vesta is the remnant of a larger destroyed planet.
Eucrites consist of basaltic rock from Vesta's crust ejected during a collision with another asteroid. Eucrites are mostly composed of calcium-poor pyroxene, pigeonite, and calcium-rich plagioclase (anorthite). Vesta is currently one of just seven identified solar system bodies of which we have physical samples.
TYPE
Eucrite (Polymict Breccia)
LOCATION
Mauritania
SIZE
1.0 x .67 x .35", 5.2 grams
CATEGORY
SUB CATEGORY
ITEM
#266171