日本地球惑星科学連合2018年大会

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[EE] 口頭発表

セッション記号 H (地球人間圏科学) » H-CG 地球人間圏科学複合領域・一般

[H-CG23] 混濁流:発生源から堆積物・地形形成まで

2018年5月21日(月) 13:45 〜 15:15 102 (幕張メッセ国際会議場 1F)

コンビーナ:横川 美和(大阪工業大学情報科学部)、泉 典洋(北海道大学大学院工学研究院)、中嶋 健(産業技術総合研究所地圏資源環境研究部門、共同)、成瀬 元(京都大学大学院理学研究科)、座長:横川 美和泉 典洋(北海道大学)

14:00 〜 14:15

[HCG23-02] Can submarine fan successions be potential hydrocarbon source rocks?: A review

*中嶋 健1 (1.産業技術総合研究所地圏資源環境研究部門)

キーワード:海底扇状地、ハイパーピクナイト、根源岩、有機炭素、石油

Turbidites and submarine fan successions constitute major deep-water hydrocarbon reservoirs in the world oil fields. Yet, their potential for hydrocarbon source rocks has never been aware until recently. In this presentation, some cases of modern and ancient submarine fan systems which exhibit potential for hydrocarbon sources are reviewed. Hyperpycnal flows are thought to be particularly important agents to transport terrestrial organic matters to these submarine fan systems. These cases commonly include “rhythmite beds” often associated with inversely to normally graded structures and plant debris. These “rhythmite beds” are interpreted as hyperpycnites and commonly yield relatively high TOC with abundant signatures of land plants. Some ancient cases are actually associated with oil fields and yield high Hydrogen Index (oil-prone). Oil in these cases show abundant biomarkers characteristics in land plants (angiosperm). Hyperpycnites are therefore thought to have high hydrocarbon potential. Further sedimentological, stratigraphic and geochemical approach will be required to quantify how much submarine fan successions can contribute to hydrocarbon sources.