Gadamis 004 Lunar Meteorite

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.

Gadamis 004 Lunar Meteorite

Gadamis 004 is classified as a Lunar Ferroan Anorthosite, cataclastic and has a texture similar to the Apollo 16 cataclastic Ferroan Anorthosites. Saw cut surfaces of Gadamis 004 reveal centimeter sized clasts of anorthsite bounded by darker fine grained cataclastic zones. Gadamis 004 is a breccia consisting of a 98-99% anorthitic plagioclase host with very small oilivine and proxene blebs. Larger pyroxene grains are sparse. Together the olivine and pyroxene make up only 1-2% of the meteorite.