日本地球惑星科学連合2018年大会

講演情報

[EE] 口頭発表

セッション記号 S (固体地球科学) » S-VC 火山学

[S-VC39] Pre-eruptive magmatic processes: petrologic analyses, experimental simulations and dynamics modeling

2018年5月24日(木) 13:45 〜 15:15 A08 (東京ベイ幕張ホール)

コンビーナ:中村 美千彦(東北大学大学院理学研究科地学専攻地球惑星物質科学講座)、東宮 昭彦(産業技術総合研究所地質調査総合センター)、Shanaka L de Silva (共同)、Costa Fidel(Earth Observatory of Singapore, Nanynag Technological University)、座長:中村 美千彦de Silva Shanaka

14:45 〜 15:00

[SVC39-03] 阿蘇4カルデラ形成噴火の準備過程

★招待講演

*長谷中 利昭1椎原 航介2安田 敦3外西 奈津美3森 康4 (1.熊本大学 くまもと水循環・減災研究教育センター 減災型社会システム部門、2.熊本大学大学院自然科学研究科、3.東京大学地震研究所、4.北九州市立自然史・歴史博物館)

キーワード:噴火準備過程、カルデラ形成噴火、阿蘇火山、大峰火砕丘、阿蘇ABCDテフラ

We measured compositions of plagioclase and pyroxenes and their melt inclusions from the precursory eruption products of 89 ka Aso-4 caldera-forming eruption. Aso-4 was the largest (VEI=7) of the four caldera-forming eruptions of Aso volcano, Kyushu island. Precursory eruptions include Omine pyroclastic cone and associated Takayubaru lava flows which erupted ca. 1,000 years before Aso-4, and Aso-ABCD tephra which erupted 9,000 years before Aso-4. Tephra units of Aso-A, B, C and D have no soils between the four, thus are considered as a series of continuous eruption.

Despite similar compositional trends observed in bulk rock chemistry, melt inclusions from Aso-ABCD tephra, those from Omine cone, and those from Aso-4 main eruptions show compositional trends distinct from all the others. Silica content of melt inclusions varies from 70-72 wt.% for Aso-ABCD, 67-70 wt.% for Omine, and 73-74 wt.% for the earliest subunit of Aso-4, followed by 71-74 wt.% for the next and voluminous subunit. Melt inclusions from Aso-ABCD tephra show similar composition to 123 ka Aso-3 tephra. Plagioclase also shows distinct compositions between Aso-ABCD, Omine, and Aso-4. Orthopyroxene and clinopyroxene often show a disequilibrium relationship in terms of Fe-Mg exchange.

When all the data are considered, a remnant of Aso-3 magma reservoir was possibly still active 9000 years before Aso-4 eruption. Magma reservoir for Omine was similar to Aso-4, however different compositional trend indicate a subsidiary reservoir to Aso-4 main one. Eruption of Aso-4 started from the top of most silica-rich part of a main reservoir, followed by mixing products of layers from a compositionally zoned large reservoir.