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Autor:
Sergey E. Borisovskiy, Andrey A. Burmistrov, Dmitriy V. Korost, Michail I. Petaev, Maria N. Logunova, Sergei I. Shornikov, A. V. Korochantsev, Cyril A. Lorenz, Marina A. Ivanova
Publikováno v:
Meteoritics & Planetary Science. 52:869-883
We investigated the khatyrkite–cupalite holotype sample, 1.2 × 0.5 mm across. It consists of khatyrkite (Cu,Zn)Al2, cupalite (Cu,Zn)Al, and interstitial material with approximate composition (Zn,Cu)Al3. All mineral phases of the holotype sample co