COMPLETE DHOFAR 1658 METEORITE
COMPLETE DHOFAR 1658 METEORITE
COMPLETE DHOFAR 1658 METEORITE
2 More
This lot is offered without reserve. These lots h… Read more
COMPLETE DHOFAR 1658 METEORITE

LL6Dhofar, Zufar, Oman (18°21’ N, 54° 24’ E)

Details
COMPLETE DHOFAR 1658 METEORITE
LL6
Dhofar, Zufar, Oman (18°21’ N, 54° 24’ E)
Dark fusion crust and regmaglypts are in evidence. Terrestrial tinting is also seen along with desert soil in the breaches fusion crust. This palm-sized specimen has a deceptively smooth, textured surface with a gently-curved slope. All surfaces are blanketed in a natural desert varnish — the result of being sandblasted for hundreds of years, if not longer, while residing at the surface of an ancient seabed that geologists refer to as “desert pavement.” Accompanying this lot is an in-situ image of the meteorite and its surrounding desert pavement environs.



113 x 79 x 53mm (4½ x 3 x 2in.)
465g
Special notice
This lot is offered without reserve. These lots have been imported from outside the EU for sale using a Temporary Import regime. Import VAT is payable (at 5%) on the Hammer price. VAT is also payable (at 20%) on the buyer’s Premium on a VAT inclusive basis. When a buyer of such a lot has registered an EU address but wishes to export the lot or complete the import into another EU country, he must advise Christie's immediately after the auction.

Lot Essay

To enable scientists to refer to the unique attributes of a given meteorite, there must be a nomenclature system, and so a committee of scientists name meteorites after the location to which they’ve been “delivered,” (e.g., a city, village, mountain, river, county, etc.). In a desert, where there are few distinguishing geological features, meteorites are named after a grid encompassing a restricted area and are assigned a sequential number. Dhofar 1658 is the 1658th meteorite to be catalogued following its recovery in the Dhofar grid of Oman bordering Yemen. Dhofar 1658 experienced extreme thermal metamorphism on its parent asteroid: its once-spherical chondrules were extensively recrystallized and the mineral grains within the rock (which initially had diverse compositions) became chemically uniform. It was derived from the LL parent asteroid responsible for other LL (low-iron, low metallic iron) chemical group of meteorites. The meteorite is a breccia; it is made up of small metamorphosed rock fragments fused together by minor impact-melting along grain boundaries.

More from Meteorites

View All
View All