T263 Planetary Mantles—Using Samples to Explore Earth, the Moon, and Mars (Posters): Memorial Session in Memory of Lawrence A. Taylor
Wednesday, 7 November 2018
9:00 AM - 6:30 PM
Halls J-K
K2CA(CO3)2 AND NA2MG(CO3)2 IN DIAMOND FROM YAKUTIAN KIMBERLITE: THE FIRST OBSERVATION
Paper number: T263-3
Program: Technical Sessions
Time: 9:00 AM – 6:30 PM
Authors
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A.M. Logvinova Presenting AuthorV.S. Sobolev Institute of Geology and Mineralogy SB RAS, Novosibirsk
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R. WirthGFZ, German Research Centre for Geosciences, Potsdam
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S.S. Ugap'evaInstitute of Diamond and Precious Metal Geology SB RAS, Yakutsk
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A.А. TomilenkoV.S. Sobolev Institute of Geology and Mineralogy SB RAS, Novosibirsk
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N.V. SobolevV.S. Sobolev Institute of Geology and Mineralogy SB RAS, Novosibirsk
Abstract
In this study polyphase inclusion, composed of CaMg(CO3)2 (dolomite), K2Ca(CO3)2 (buetschliite), Na2Mg(CO3)2 (eitelite) and MgCO3 (magnesite), was identified in Yakutian diamond, using TEM and Raman spectroscopy. Buetschliite and eitelite as inclusions in diamond are reported for the first time. The characteristic Raman bands lie for buetschliite at 1092cm -1, weak lines at 693, 222, 165 cm-1. For eitelite – at 1105 cm-1 and weak lines at 261, 207 cm-1. The polyphase inclusion is located in the centre of a monocrystalline diamond from Sytykanskaya pipe (Yakutia). It is enolgated 35 microns in size shaped and alkalis presence inclusion. Dolomite predominates in polyphase inclusion. Careful CL imaging reveals the total absence of cracks around the dolomite inclusion. Buetschliite and eitelite are located closer to the peripheral zone of inclusion. The origin of the studied diamond may be due to high-Mg carbonatitic HDFs, which have been described in fibrous cubic and coated Yakutian diamonds (Klein-BenDavid et al., 2009), but having the complex alkali-rich carbonate compositions. Variations of carbonate - inclusion compositions among diamonds indicate the variability in the source media at the formation of diamond.
Financial support for this study was provided by RFBR (16-05-00841; 17-05-00668), RSF (14-17-00602P)
Geological Society of America Abstracts with Programs. Vol. 50, No. 6
doi: 10.1130/abs/2018AM-322000
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