Reviews
2.15" Rare Gujba Meteorite (17.50 g) Slice - 1984 Witnessed Fall!
This is an absolutely breathtaking, 17.50 gram slice of the witnessed meteorite, Gujba. It measures 2.15" wide and has been sliced and lightly polished on one side to display its multicolored interior chondrules. The metallic nodules display an exceptional luster when tilted back and fourth. It comes in a display case.
About the Gujba Meteorite
The Gujba meteorite made quite an entrance as it fell in Yobe, Nigeria on April 3rd, 1984 around 6:30 local time.
"A conical meteorite fell in a corn field near the village of Bogga Dingare after a bright fireball was witnessed moving west to east and an explosion was heard. The local people hammered the meteorite into many pieces, and most of the material was dispersed. The original mass is unknown, although secondhand reports indicate that it had a volume of ~20 000 cm3, and thus a mass of approximately 100 kg. Material that almost certainly came from this fall has been sold in the last few years elsewhere in Nigeria, with claims that the specimens were new finds."
It is classified as a Bencubbin-like Carbonaceous Chondrite. When sliced, it shows metal nodules measuring 1.5 to 8 mm in diameter, silicate nodules measuring 1 to 15 mm in diameter, and fan-like aggregates of pyroxene.
Meteoritical Bulletin: Entry for the Gujba Meteorite
The Gujba meteorite made quite an entrance as it fell in Yobe, Nigeria on April 3rd, 1984 around 6:30 local time.
"A conical meteorite fell in a corn field near the village of Bogga Dingare after a bright fireball was witnessed moving west to east and an explosion was heard. The local people hammered the meteorite into many pieces, and most of the material was dispersed. The original mass is unknown, although secondhand reports indicate that it had a volume of ~20 000 cm3, and thus a mass of approximately 100 kg. Material that almost certainly came from this fall has been sold in the last few years elsewhere in Nigeria, with claims that the specimens were new finds."
It is classified as a Bencubbin-like Carbonaceous Chondrite. When sliced, it shows metal nodules measuring 1.5 to 8 mm in diameter, silicate nodules measuring 1 to 15 mm in diameter, and fan-like aggregates of pyroxene.
Meteoritical Bulletin: Entry for the Gujba Meteorite
About Carbonaceous Chondrites
Carbonaceous chondrites consist of about 5 percent of known chondrites. They contain the highest concentrations of water, organic, and volatile compounds of all chondrites, and, true to their name, contain carbonate minerals! These chondrites are the least oxidized, indicating they came from the outer asteroid belt or beyond. Because of their unique compositions, they are some of the most frequently studied meteorites in the world, and have been considered as an origin for life due to their abundance of organic compounds, including amino acids.
Due to their complexity and variety, carbonaceous chondrites have several sub-classes grouped by chondrule width, each named after the type specimens of each class. CI carbonaceous chondrites, the class of finest grains, are named for the Ivuna meteorite that fell in Tanzania in 1938. CI chondrites almost entirely lack chondrules, and are composed mostly of fine-grained material that underwent aqueous alteration on their parent asteroids. Their chemical composition most closely resembles the sun’s photosphere of any chondrite. Other notable classes include:
CO and CM (Ornans/Mighei), with the smallest chondrules;
CR (Renazzo), CB (Bencubbin) and CH (high metal), which contain unique chondrules that formed from impacts after normal chondrules formed;
CV (Vigarano) and CK (Karoonda), two groups with distinctively large chondrules that formed only once at the beginning of the solar system; and
CL (Loongana), which contain large chondrule and calcium-aluminum-rich inclusions, or CAIs, but low amounts of volatile compounds and matrix.
Carbonaceous chondrites consist of about 5 percent of known chondrites. They contain the highest concentrations of water, organic, and volatile compounds of all chondrites, and, true to their name, contain carbonate minerals! These chondrites are the least oxidized, indicating they came from the outer asteroid belt or beyond. Because of their unique compositions, they are some of the most frequently studied meteorites in the world, and have been considered as an origin for life due to their abundance of organic compounds, including amino acids.
Due to their complexity and variety, carbonaceous chondrites have several sub-classes grouped by chondrule width, each named after the type specimens of each class. CI carbonaceous chondrites, the class of finest grains, are named for the Ivuna meteorite that fell in Tanzania in 1938. CI chondrites almost entirely lack chondrules, and are composed mostly of fine-grained material that underwent aqueous alteration on their parent asteroids. Their chemical composition most closely resembles the sun’s photosphere of any chondrite. Other notable classes include:
About Chondrites
Chondrites are stony (non-metallic) meteorites that have not been modified by either melting or differentiation of the parent body. They are formed when various types of dust and small grains in the early Solar System accreted to form primitive asteroids. Some such bodies are captured in the planet’s gravity well and pulled to the surface. They are by far the most common type of meteorite, representing about 86 percent of all meteorites that have fallen to Earth.
Prominent among the components present in chondrites are the enigmatic chondrules, millimeter-sized spherical objects that originated as freely floating, molten or partially molten droplets in space; most chondrules are rich in the silicate minerals olivine and pyroxene. Chondrites also contain particles of various metals such as nickel, iron, and aluminum. These formed at the very beginning of the solar system and aggregated over time: they are the oldest rocks known on Earth!
Chondrites are divided into about fifteen distinct groups on the basis of their mineralogy, bulk chemical composition, and oxygen isotope compositions. The various chondrite groups likely originated on separate asteroids or groups of related asteroids. Each chondrite group has a distinctive mixture of chondrules, refractory inclusions, matrix (dust), characteristic chondrule sizes, and other components. Other ways of classifying chondrites include weathering and shock. The L chondrite group is the most common of these.
Chondrites are stony (non-metallic) meteorites that have not been modified by either melting or differentiation of the parent body. They are formed when various types of dust and small grains in the early Solar System accreted to form primitive asteroids. Some such bodies are captured in the planet’s gravity well and pulled to the surface. They are by far the most common type of meteorite, representing about 86 percent of all meteorites that have fallen to Earth.
Prominent among the components present in chondrites are the enigmatic chondrules, millimeter-sized spherical objects that originated as freely floating, molten or partially molten droplets in space; most chondrules are rich in the silicate minerals olivine and pyroxene. Chondrites also contain particles of various metals such as nickel, iron, and aluminum. These formed at the very beginning of the solar system and aggregated over time: they are the oldest rocks known on Earth!
Chondrites are divided into about fifteen distinct groups on the basis of their mineralogy, bulk chemical composition, and oxygen isotope compositions. The various chondrite groups likely originated on separate asteroids or groups of related asteroids. Each chondrite group has a distinctive mixture of chondrules, refractory inclusions, matrix (dust), characteristic chondrule sizes, and other components. Other ways of classifying chondrites include weathering and shock. The L chondrite group is the most common of these.
$2,950
TYPE
CBa (Bencubbin-like Carbonaceous Chondrite)
LOCATION
Bogga Dingare Village, Yobe, Nigeria
SIZE
Size: 2.15 x 1.28 x .12", Weight: 17.50 grams
CATEGORY
ITEM
#301182
