Abstract—The problem of the origin of “white granite” in the Kester harpolith of the Arga–Ynnakh–Khaya Pluton is discussed. The morphology, occurrence, and nature of the intrusive contacts of the Kester harpolith prove its magmatic origin. The petrographic and petrochemical properties of “white granite” allow its identification as a postorogenic rare-metal high-phosphorus granite of the Li-F geochemical type. The magmatic genesis of the “white granite” texture is supported by statistical methods. The composition, typomorphic properties, ontogenetic features internal structure and relationship of accessory minerals indicate that the major accessories of the granite, that is, cassiterite, columbite, tantalite, “wolframoixiolite,” zircon, and ferberite, were formed at the late stage of the low-temperature rare-metal granitic melt. The Kester harpolith within the Arga–Ynnakh–Khaya granite pluton and the eponymous tin–rare-metal deposit genetically related to it are a part of the Far East Superprovince of rare-metal granites.

摘要-讨论了阿尔加－恩纳赫河－哈亚普鲁顿的凯斯特哈波利斯的“白色花岗岩”起源问题。Kester harpolith的侵入性接触的形态，发生和性质证明了其岩浆成因。“白色花岗岩”的岩石学和岩石化学性质使其可以鉴定为Li-F地球化学类型的后成因的稀有金属高磷花岗岩。统计方法支持“白色花岗岩”质地的岩浆成因。组成，错型性质，成因特征，内部构造和附属矿物之间的关系表明，花岗岩的主要附属物是锡石，哥伦比，钽铁矿，“钨辉闪石”，锆石和镁铁矿。低温稀有金属花岗石熔体。