日本地球惑星科学連合2024年大会

講演情報

[J] ポスター発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS23] 地質学のいま

2024年5月31日(金) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

コンビーナ:辻森 樹(東北大学)、山口 飛鳥(東京大学大気海洋研究所)、尾上 哲治(九州大学 大学院理学研究院 地球惑星科学部門)、小宮 剛(東京大学大学院総合文化研究科広域科学専攻)

17:15 〜 18:45

[MIS23-P03] パンダヒル産ソバイト様カーボナタイトに含まれる初生流体包有物

*梅宮 穂花1辻森 樹1、ボニファス ネルソン2 (1.国立大学法人東北大学、2.ダルエスサラーム大学)

キーワード:カーボナタイト、流体包有物、初生包有物、パンダヒル

Carbonatites, defined by either >30 vol% of igneous carbonate minerals or >50 wt% of carbonate in igneous rocks, host the largest deposits of rare earth elements (REEs) and niobium (Nb), making them critical sources of 'essential elements.'

In the East African rift system of western Tanzania, the Panda Hill Carbonatite Complex of Cretaceous age is notable for its pyrochlore-bearing sovite-type carbonatite (e.g., Boniface, 2017). This study investigates the primary magmatic fluids by examining fluid inclusions within calcite and apatite from the sovite carbonatite at Panda Hill Complex. The analyzed sovite samples contain mainly calcite with a subordinate amount of apatite, and minor accessory minerals such as magnetite, phlogopite, and pyrochlore.

Our observations reveal that both calcite and apatite host abundant fluid inclusions. In calcite, these are predominantly pseudosecondary and secondary (1 to 10 μm in size), and exhibit varied morphologies including spherical, polygonal, and irregular shapes. In contrast, primary fluid inclusions with spherical shapes (1 to 15 μm in size), dominate in apatite. Fluid inclusions in both minerals vary from liquid-only, two-phase (liquid with gas), to multiphase (liquid with gas and daughter mineral phases), regard less of their generation.

This poster presentation will detail our preliminary results on the characteristics of primary fluid inclusions, supplemented by Raman spectroscopic analysis.