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4.9" Eucrite Meteorite (101.6 g) Slice - NWA 14016
This is a 4.9" wide (101.6 gram) stony (achondrite) meteorite from northwestern Africa. It is a HED-eucrite largely composed of melt breccia, creating large, highly contrasted grains. This specimen has been sliced and polished on one side. It comes with an acrylic display stand.
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.
A true color image of 4 Vesta taken by NASA's Dawn probe in July of 2011.
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.
A true color image of 4 Vesta taken by NASA's Dawn probe in July of 2011.
TYPE
Eucrite, Melt Breccia
LOCATION
Northwestern Africa
SIZE
4.9 x 3.2 x 0.2", 101.6 grams
CATEGORY
SUB CATEGORY
ITEM
#247018
