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2.21" Polished Diogenite Meteorite (8.63 g) Slice - NWA 7947
This is a 2.21" wide, 8.63 gram slice of the diogenite meteorite known as NWA 7947. The polishing on one side allows for the angular grains of orthopyroxene to be seen.
Comes with a floating frame display case.
About NWA 7947
NWA 7947 is an HED achondrite (diogenite), specifically classified as a diogenite breccia. It was collected in 2013 in Northwest Africa and later purchased in Temara, Morocco by Adam Aaronson. It's a clast-rich breccia composed predominantly of angular grains of orthopyroxene with accessory olivine, chromite, and minor troilite.
Meteoritical Bulletin: Entry for NWA 7947
NWA 7947 is an HED achondrite (diogenite), specifically classified as a diogenite breccia. It was collected in 2013 in Northwest Africa and later purchased in Temara, Morocco by Adam Aaronson. It's a clast-rich breccia composed predominantly of angular grains of orthopyroxene with accessory olivine, chromite, and minor troilite.
Meteoritical Bulletin: Entry for NWA 7947
Diogenite Meteorites
Diogenite meteorites are a class of achondritic (stony) meteorites believed to originate from the inner crust of the asteroid (or minor planet) 4 Vesta.
4 Vesta, or simply Vesta, is the second largest object in the asteroid belt, with a mean diameter of about 525 kilometers (326 miles) and an elliptical shape. Vesta is likely the remnant of a destroyed planet, since it still retains a differentiated interior just like the layers of Earth and other rocky planets. It is one of just seven bodies in the solar system that humans have physical samples of. It is also the brightest asteroid visible from Earth, and can be seen with the naked eye!
Diogenites themselves are from a distinct part of Vesta: they come from the inner crust and are plutonic. They formed from intrusive igneous processes: in other words, diogenites were lava that cooled long enough to create crystals larger than what are found in howardites and eucrites, two other kinds of Vesta meteorites more commonly found on Vesta's surface. Thus, diogenites could indicate that Vesta was once part of a larger rocky planet with differentiated layers!
Diogenites are named for the ancient Greek philosopher Diogenes of Apollonia, who was the first person known to suggest that meteorites came from outer space.
A true color image of 4 Vesta taken by NASA's Dawn probe in July of 2011.
Diogenite meteorites are a class of achondritic (stony) meteorites believed to originate from the inner crust of the asteroid (or minor planet) 4 Vesta.
4 Vesta, or simply Vesta, is the second largest object in the asteroid belt, with a mean diameter of about 525 kilometers (326 miles) and an elliptical shape. Vesta is likely the remnant of a destroyed planet, since it still retains a differentiated interior just like the layers of Earth and other rocky planets. It is one of just seven bodies in the solar system that humans have physical samples of. It is also the brightest asteroid visible from Earth, and can be seen with the naked eye!
Diogenites themselves are from a distinct part of Vesta: they come from the inner crust and are plutonic. They formed from intrusive igneous processes: in other words, diogenites were lava that cooled long enough to create crystals larger than what are found in howardites and eucrites, two other kinds of Vesta meteorites more commonly found on Vesta's surface. Thus, diogenites could indicate that Vesta was once part of a larger rocky planet with differentiated layers!
Diogenites are named for the ancient Greek philosopher Diogenes of Apollonia, who was the first person known to suggest that meteorites came from outer space.
A true color image of 4 Vesta taken by NASA's Dawn probe in July of 2011.
TYPE
HED Achondrite (Diogenite)
AGE
LOCATION
Northwest Africa
SIZE
2.21 x 1.50 x .08", Weight: 8.63 grams
CATEGORY
SUB CATEGORY
ITEM
#301053
