Details
This unusually angular abstract meteorite exhibits the signature rounded ridges and finely stippled surface of premium Campo del Cielo meteorites. A large scoop defines the front surface, the whole is draped in a gun metal patina.
414 x 434 x 4in. (11 x 12 x10cm.)
2.3kg.
Special notice
Specified lots are being stored at Crozier Park Royal (details below) or will be removed from Christie’s, 8 King Street, London, SW1Y 6QT by 5.00pm on the day of the sale. Christie’s will inform you if the lot has been sent offsite. If the lot has been transferred to Crozier Park Royal, it will be available for collection from 12.00pm on the second business day following the sale. Please call Christie’s Client Service 24 hours in advance to book a collection time at Crozier Park Royal. All collections from Crozier Park Royal will be by pre-booked appointment only. Tel: +44 (0)20 7839 9060 Email: cscollectionsuk@christies.com. If the lot remains at Christie’s, 8 King Street, it will be available for collection on any working day (not weekends) from 9.00am to 5.00pm
Please note this lot is the property of a consumer. See H1 of the Conditions of Sale.
Brought to you by
James HyslopHead of Department, Science & Natural History
A Christie's specialist may contact you to discuss this lot or to notify you if the condition changes prior to the sale.

Lot Essay

About 4000 years after having collided with Earth, Campo del Cielo (“Field of the Sky”) meteorites were first written about in 1576 by Spanish explorers when their unearthly origins had yet to be understood. It was a “Campo” that was the first large meteorite displayed at the British Museum of Natural History, and several large Campo del Cielo masses can be found today in the finest museums throughout the world.

The frictional stresses during atmospheric passage caused it to explode and break up into thousands of pieces. The larger iron masses ploughed into the ground at such a high velocity that an array of at least 26 impact craters formed , the largest being 91x115 meters. The meteorite is from chemical group IAB and has been modelled as having formed on a chondritic asteroid as a result of a cataclysmic collision at cosmic velocity with another asteroid in deep space.

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