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This is a stunning fragment of the very rare Veevers classified meteorite weighing 1.74 grams. This meteorite is one of only 15 associated with a crater larger than 10 meters across. The crater is about 1 million years old and is one of only 2 craters older than 50,000 years that have meteorites associated with them. This amazingly well preserved specimen measures 13x8x4 mm.

The Veevers crater is located in the Gibson Desert of Western Australia. It has a diameter of 60-80 meters across and a depth of about 6-7 meters. The crater's rim is raised 1.5m above the surrounding plain, and contains exposed rocks thrown from the center of the crater. The sides are gravelly rock with a few larger rocks mixed within. The bottom of the crater is covered with sand.  Veevers is isolated in a vast, flat landscape with no other features in sight. Discovered in the mid-1970's and named by Yeates, A.N., Crowe, R.W.A. & Towner, R.R., in 1976, as The Veevers Crater in honor of Australian geologist Prof. John Veevers, for his work at mapping Western Australia.

In 1984, Dr. Carolyn and Eugene Shoemaker investigated meteorite craters and ancient impact structures throughout Australia. Their search recovered thirty-six small meteoritic fragments from the Veevers crater. Their finds totaled 298.1 grams, and included the largest found to date, 36.3g., now cleaned and coated it weighs 37.0 grams. The Veevers fragments have been described as single crystals of kamacite. Kamacite is a metallic iron with up to 7.5% nickel. Since the Shoemaker trip, more meteorite fragments have been found, bringing the total known weight to around 1 kg. The Veevers crater is naturally rich in iron-rich laterite, which makes recovery of small meteorite fragments hard. It is one of only two impact craters where group IIAB meteorites have been discovered. The other being the Sikhote-Alin craters in Eastern Siberia, Russia.

Would be an exceptional and rare addition to any new or existing collection.  This historically important specimen will come with a ELKK Meteorite Collection and Canagem Collection specimen cards.

This is a Selenite sphere from Morocco. The sphere comes from a selenite mass of Satin Spar, and is partially clear (the rest is translucent), with a lovely Chatoyancy.

Selenite, also known as Gypsum, is one of the more common minerals in sedimentary environments. It is a major rock forming mineral that produces massive beds, usually from precipitation out of highly saline waters. Since it forms easily from saline water, gypsum can have many inclusions of other minerals and even trapped bubbles of air and water.

Gypsum has several variety names that are widely used in the mineral trade. "Selenite" is the colorless and transparent variety that shows a pearl like luster and has been described as having a moon like glow. The word selenite comes from the Greek for Moon and means moon rock. Another variety is a compact fibrous aggregate called "satin spar" . This variety has a very satin like look that gives a play of light up and down the fibrous crystals. A fine grained massive material is called "alabaster" and is an ornamental stone used in fine carvings for centuries, even eons.

Selenite is believed to be a calming stone that instills deep peace and is excellent for meditation.  Selenite has an ethereal quality and is said to inhabit the place between light and matter.  Although an ancient stone, it is still one of the most powerful crystals.

It is thought that Selenite can be used to form a protective grid around a house, creating a safe and quiet space that does not allow outside influences in.  A large piece of Selenite placed in the house ensures a peaceful atmosphere.

Would be a beautiful addition to any new or existing collection.

Name: Selenite Satin Spar Sphere
Dimensions: 72 mm - 2.8 inches
Weight: 465 grams - 1 lb
Origin: Midelt Morocco

This is a nice end cut of the Northwest Africa 978 meteorite. This is another of the great and rare meteorites from the Sahara. It is classified as a Stone, Chondrite Rumurutiite, (R3.8). This meteorite was found in 2001 in many fragments and small individuals, very fresh but sandblasted, for a low TKW of 722 grams. The Shock stage is registered at 3 and the Weathering grade at 2.

It is one of the rarest meteorite types with only 9 Rumuruti 3.8 type meteorites known,  most being found in Antarctica. This unique group of chondrites has basically no FeNi-metal in comparison to other chondrite groups. The R chondrites also have the highest 17O value of any other solar system material. This piece weighs 5.02 grams an measures 31x18x8mm. Note the flat edge of this piece is crusted, it is not a cut surface.

This hard to acquire piece displays very well with its diamond lap finish.  This high quality specimen would make an amazing addition to any new or existing collection. Comes with a ELKK Meteorites and a Canagem Collection specimen cards.

Product Type:  Opal Cats Eye
Approx Weight (per piece):  6.33ct
Size:   13.5x10.5mm
Shape:  Oval Cabochon
Color:  Dark Honey
Clarity:  Fine crystal
Origin:  Africa
Treatment:  None

The Gold Hill Wash Prospect, part of the Clifton-Gold Hill Mining District, is known for its rich mineral resources, including jarosite. This mineral is part of the larger group of minerals found in the area, which also includes limonite.

The Gold Hill Mine, operated by the Western Utah Copper Company in the early 20th century, was significant for its arsenic deposits, although it closed after World War I. The mine's portals and shafts have since been sealed by the state of Utah.

This specimen from the Gold Hill Mine is a matrix covered with minute jarosite crystals.  This specimen is an interesting addition to any mineral collection.

Name: Jarosite
Specimen Size:  Miniature-Sized
Dimensions:  53x49x33 mm / 2.1x1.9x1.3 inches
Weight:  64.91 Grams / 2.3 ounces
Origin: Mined in Gold Hill Mine, Gold Hill, Gold Hill Mining District (Clifton Mining District), Tooele County, Utah, USA