The cut interior surface of this sample is a hued gray with a heterogeneous distribution of dark grains. Two sandy adges seen are the result of this meteorite’s residency in the Sahara Desert prior to its discovery. Modern cutting.
4¹⁄₂ x 3¹⁄₂in. (11.5 x 9.0 x 0.3cm.)
57g.

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
This lot has been imported from outside of the UK for sale and placed under the Temporary Admission regime. Import VAT is payable at 5% on the hammer price. VAT at 20% will be added to the buyer’s premium but will not be shown separately on our invoice.
Please note this lot is the property of a consumer. See H1 of the Conditions of Sale.

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As is the case with the Moon, specimens of the planet Mars are among the most exotic substances on Earth with less than 250 kg (550 lbs) known to exist. The delivery mechanism to Earth was an asteroid impact on Mars that ejected material of the Martian surface into an Earth-crossing orbit. The determination of Martian origin is the result of research conducted by hundreds of scientists throughout the world. In addition to many arcane chemical and isotopic markers, most Martian meteorites have an unusually young crystalline age. The link to Mars was speculative until an analysis was conducted on the glassy inclusions in other suspected Martian meteorites. Within the glass were tiny vugs, and within these vugs were tiny volumes of gas. The gas was analyzed and it matched perfectly with the signature of the Martian atmosphere as reported by NASA’s Viking Missions to Mars in 1976.

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