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Identification of the static backstop and its influence on the evolution of the accretionary prism in the Nankai Trough
To reveal the origin of a backstop and its influence on the evolution of the accretionary prism, we analyzed reflection seismic data acquired in the Nankai Trough off the Kii Peninsula. The deformation features of the forearc basin sequence show that the landward accretionary prism close to the coas...
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Published in: | Earth and planetary science letters 2015-12, Vol.431, p.15-25 |
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description | To reveal the origin of a backstop and its influence on the evolution of the accretionary prism, we analyzed reflection seismic data acquired in the Nankai Trough off the Kii Peninsula. The deformation features of the forearc basin sequence show that the landward accretionary prism close to the coast was not deformed after the development of the forearc basin about 2–4 Ma. The surface of the landward prism can be identified as strong amplitude reflector, indicating that the landward prism has higher seismic velocity. Therefore, the landward accretionary prism inferred to be of higher strength constitutes a static backstop. Based on seismic and geologic observations, we interpret that the backstop was generated due to the large age differences of accreted material resulting from an inferred hiatus in subduction between ∼13 and 6 Ma. The time-dependent processes such as the igneous activity in middle Miocene further contribute to the development of the backstop. A ridge structure beneath the forearc basin located trenchward of this backstop and running roughly parallel to it appears to reflect activity on an ancient splay fault. The strike of the ancient splay fault runs parallel to the backstop identified in this study and oblique to the current trench. This geometry suggests that location and mechanical behavior of this splay fault system is influenced by the backstop, and its distribution could be related to the coseismic rupture area.
•Backstop can be identified from deformation features of forearc basin sequence.•Static backstop is generated by age difference from hiatus in subduction process.•The igneous activity in middle Miocene contributes to originate lithified backstop.•Backstop controls fault system within accretionary prism including ancient splay fault.•Backstop distribution could relate to the coseismic rupture segment. |
doi_str_mv | 10.1016/j.epsl.2015.09.011 |
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•Backstop can be identified from deformation features of forearc basin sequence.•Static backstop is generated by age difference from hiatus in subduction process.•The igneous activity in middle Miocene contributes to originate lithified backstop.•Backstop controls fault system within accretionary prism including ancient splay fault.•Backstop distribution could relate to the coseismic rupture segment.</description><identifier>ISSN: 0012-821X</identifier><identifier>EISSN: 1385-013X</identifier><identifier>DOI: 10.1016/j.epsl.2015.09.011</identifier><language>eng</language><publisher>Elsevier B.V</publisher><subject>accretionary prism evolution ; backstop ; Basins ; Deformation ; Evolution ; fault system ; Faults ; forearc basin ; Nankai trough ; Peninsulas ; Prisms ; Reflection ; seismic profiles ; Strikes</subject><ispartof>Earth and planetary science letters, 2015-12, Vol.431, p.15-25</ispartof><rights>2015 The Authors</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a510t-ad07a26886b2f2d07ef80ae2c86dbf33d217a7cd069bac7fdcdd11f660323c793</citedby><cites>FETCH-LOGICAL-a510t-ad07a26886b2f2d07ef80ae2c86dbf33d217a7cd069bac7fdcdd11f660323c793</cites><orcidid>0000-0003-0951-4596</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Tsuji, Takeshi</creatorcontrib><creatorcontrib>Ashi, Juichiro</creatorcontrib><creatorcontrib>Strasser, Michael</creatorcontrib><creatorcontrib>Kimura, Gaku</creatorcontrib><title>Identification of the static backstop and its influence on the evolution of the accretionary prism in the Nankai Trough</title><title>Earth and planetary science letters</title><description>To reveal the origin of a backstop and its influence on the evolution of the accretionary prism, we analyzed reflection seismic data acquired in the Nankai Trough off the Kii Peninsula. The deformation features of the forearc basin sequence show that the landward accretionary prism close to the coast was not deformed after the development of the forearc basin about 2–4 Ma. The surface of the landward prism can be identified as strong amplitude reflector, indicating that the landward prism has higher seismic velocity. Therefore, the landward accretionary prism inferred to be of higher strength constitutes a static backstop. Based on seismic and geologic observations, we interpret that the backstop was generated due to the large age differences of accreted material resulting from an inferred hiatus in subduction between ∼13 and 6 Ma. The time-dependent processes such as the igneous activity in middle Miocene further contribute to the development of the backstop. A ridge structure beneath the forearc basin located trenchward of this backstop and running roughly parallel to it appears to reflect activity on an ancient splay fault. The strike of the ancient splay fault runs parallel to the backstop identified in this study and oblique to the current trench. This geometry suggests that location and mechanical behavior of this splay fault system is influenced by the backstop, and its distribution could be related to the coseismic rupture area.
•Backstop can be identified from deformation features of forearc basin sequence.•Static backstop is generated by age difference from hiatus in subduction process.•The igneous activity in middle Miocene contributes to originate lithified backstop.•Backstop controls fault system within accretionary prism including ancient splay fault.•Backstop distribution could relate to the coseismic rupture segment.</description><subject>accretionary prism evolution</subject><subject>backstop</subject><subject>Basins</subject><subject>Deformation</subject><subject>Evolution</subject><subject>fault system</subject><subject>Faults</subject><subject>forearc basin</subject><subject>Nankai trough</subject><subject>Peninsulas</subject><subject>Prisms</subject><subject>Reflection</subject><subject>seismic profiles</subject><subject>Strikes</subject><issn>0012-821X</issn><issn>1385-013X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNp9kLFO5DAQhi0EEsseL0DlkiZhxtE6iUSD0N2BhI6Gk-gsrz0GL9l4sR1OvD0OS3EVbqyx_2808zF2hlAjoLzY1LRLQy0AVzX0NSAesAU23aoCbB4P2QIARdUJfDxmJyltAECuZL9g_24tjdk7b3T2YeTB8fxMPOVSGr7W5iXlsON6tNznxP3oholGQ7xk5yC9hWH6n9TGRJofdHznu-jTtkCfP3_0-KI9f4hhenr-wY6cHhKdft1L9vfXz4frm-ru_vft9dVdpVcIudIWWi1k18m1cKIU5DrQJEwn7do1jRXY6tZYkH2ZtXXWWIvopIRGNKbtmyU73_fdxfA6Ucpq65OhYdAjhSkpbKVAAU05Syb2URNDSpGcKuNvyxoKQc2W1UbNltVsWUGviuUCXe4hKku8eYoqGT8Lsj6SycoG_x3-AefwiJU</recordid><startdate>20151201</startdate><enddate>20151201</enddate><creator>Tsuji, Takeshi</creator><creator>Ashi, Juichiro</creator><creator>Strasser, Michael</creator><creator>Kimura, Gaku</creator><general>Elsevier B.V</general><scope>6I.</scope><scope>AAFTH</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0003-0951-4596</orcidid></search><sort><creationdate>20151201</creationdate><title>Identification of the static backstop and its influence on the evolution of the accretionary prism in the Nankai Trough</title><author>Tsuji, Takeshi ; Ashi, Juichiro ; Strasser, Michael ; Kimura, Gaku</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a510t-ad07a26886b2f2d07ef80ae2c86dbf33d217a7cd069bac7fdcdd11f660323c793</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>accretionary prism evolution</topic><topic>backstop</topic><topic>Basins</topic><topic>Deformation</topic><topic>Evolution</topic><topic>fault system</topic><topic>Faults</topic><topic>forearc basin</topic><topic>Nankai trough</topic><topic>Peninsulas</topic><topic>Prisms</topic><topic>Reflection</topic><topic>seismic profiles</topic><topic>Strikes</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Tsuji, Takeshi</creatorcontrib><creatorcontrib>Ashi, Juichiro</creatorcontrib><creatorcontrib>Strasser, Michael</creatorcontrib><creatorcontrib>Kimura, Gaku</creatorcontrib><collection>ScienceDirect Open Access Titles</collection><collection>Elsevier:ScienceDirect:Open Access</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Earth and planetary science letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Tsuji, Takeshi</au><au>Ashi, Juichiro</au><au>Strasser, Michael</au><au>Kimura, Gaku</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Identification of the static backstop and its influence on the evolution of the accretionary prism in the Nankai Trough</atitle><jtitle>Earth and planetary science letters</jtitle><date>2015-12-01</date><risdate>2015</risdate><volume>431</volume><spage>15</spage><epage>25</epage><pages>15-25</pages><issn>0012-821X</issn><eissn>1385-013X</eissn><abstract>To reveal the origin of a backstop and its influence on the evolution of the accretionary prism, we analyzed reflection seismic data acquired in the Nankai Trough off the Kii Peninsula. The deformation features of the forearc basin sequence show that the landward accretionary prism close to the coast was not deformed after the development of the forearc basin about 2–4 Ma. The surface of the landward prism can be identified as strong amplitude reflector, indicating that the landward prism has higher seismic velocity. Therefore, the landward accretionary prism inferred to be of higher strength constitutes a static backstop. Based on seismic and geologic observations, we interpret that the backstop was generated due to the large age differences of accreted material resulting from an inferred hiatus in subduction between ∼13 and 6 Ma. The time-dependent processes such as the igneous activity in middle Miocene further contribute to the development of the backstop. A ridge structure beneath the forearc basin located trenchward of this backstop and running roughly parallel to it appears to reflect activity on an ancient splay fault. The strike of the ancient splay fault runs parallel to the backstop identified in this study and oblique to the current trench. This geometry suggests that location and mechanical behavior of this splay fault system is influenced by the backstop, and its distribution could be related to the coseismic rupture area.
•Backstop can be identified from deformation features of forearc basin sequence.•Static backstop is generated by age difference from hiatus in subduction process.•The igneous activity in middle Miocene contributes to originate lithified backstop.•Backstop controls fault system within accretionary prism including ancient splay fault.•Backstop distribution could relate to the coseismic rupture segment.</abstract><pub>Elsevier B.V</pub><doi>10.1016/j.epsl.2015.09.011</doi><tpages>11</tpages><orcidid>https://orcid.org/0000-0003-0951-4596</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | accretionary prism evolution backstop Basins Deformation Evolution fault system Faults forearc basin Nankai trough Peninsulas Prisms Reflection seismic profiles Strikes |
title | Identification of the static backstop and its influence on the evolution of the accretionary prism in the Nankai Trough |
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