日本地球惑星科学連合2019年大会

講演情報

[E] 口頭発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS02] 地球掘削科学

2019年5月27日(月) 09:00 〜 10:30 A07 (東京ベイ幕張ホール)

コンビーナ:山田 泰広(海洋研究開発機構 海洋掘削科学研究開発センター)、針金 由美子(産業技術総合研究所)、黒柳 あずみ(東北大学学術資源研究公開センター東北大学総合学術博物館)、山口 耕生(東邦大学, NASA Astrobiology Institute.)、座長:黒柳 あずみ(東北大学)、Kan Hsiung(海洋研究開発機構)

10:15 〜 10:30

[MIS02-06] Recent progress and perspective on paleomagnetism by means of deep-sea drilling

*山崎 俊嗣1山本 裕二2金松 敏也3熊谷 祐穂4中村 教博4 (1.東京大学大気海洋研究所、2.高知大学海洋コア総合研究センター、3.海洋研究開発機構、4.東北大学)

キーワード:古地磁気学、古地磁気強度、国際深海科学掘削計画

We review recent progress of paleomagnetism using deep-sea drilling cores since the beginning of IODP in 2003, in particular for estimations of paleomagnetic-field intensity (paleointensity) from sediments, and discuss problems to be resolved and perspectives.

For the establishment of the high-resolution relative paleointensity stack for the last 1.5 m.y., sediment cores of Exp. 303/306 from the North Atlantic were utilized. While only few records were available before about 3 m.y. previously, some Eocene to Miocene relative paleointensity records were obtained from the cores in the east equatorial Pacific taken during Exp. 320/321. Applicability of relative paleointensity to inter-core correlations and age estimations has extended to older ages accordingly. On the other hand, contamination of sediment lithological variations induced by paleoclimate changes, in particular fluctuations of the proportion of biogenic and terrigenous magnetites, to paleointensity estimations has become widely recognized. It is urgently necessary to resolve this problem and recover reliable long-term paleointensity records for tackling fundamental issues in geomagnetism such as possible dependence of field intensity to the length of polarity intervals and a possible relation between Earth’s orbital parameters and the geomagnetic field. Better understanding of the role of biogenic magnetite in remanent magnetization acquisition processes is important to solve the contamination problem. Information on the variations of time-averaged field in 105 to 106 year time-scales is also important for geomagnetism. Departure from the geocentric axial dipole (GAD) field of these time-scales may reflect boundary conditions of the geodynamo at the core-mantle boundary. The departure from GAD emerges as inclination anomalies in sediment cores. IODP cores may be useful for such studies although little studied before.

Acquisition of long deep-sea sediment cores is still required for obtaining continuous paleomagnetic records of Miocene and older ages, and IODP will continue to be the only means for this. Paleointensity estimations from sediments of older ages are hindered by dissolution of magnetite by reductive diagenesis; as sediments are buried deeper, reductive diagenesis becomes more serious. Successful expeditions resulted from the strategic selections of drilling sites; for example, the sediments of target ages are not covered with thick younger sediments (Exp. 320/321), and sediments in relatively oxic environments exist even buried under thick sediments (drift sediments of Exp. 363). Recently, the importance of silicate-hosted magnetic minerals as a carrier of remanent magnetization of sediments becomes recognized; they could escape from dissolution even in anoxic conditions. We need to revisit anoxic sediment cores to investigate the possibility for recovering paleomagnetic records from such sediments. Previously paleomagnetists just discarded them without detailed studies.