The Journal of the Petrological Society of Korea (암석학회지)

The Petrological Society of Korea (한국암석학회)
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The Characteristic of Mangerite and Gabbro in the Odaesan Area and its Meaning to the Triassic Tectonics of Korean Peninsula

오대산 지역에 나타나는 맨거라이트와 반려암의 특징과 트라이아스기 한반도 지체구조 해석에 대한 의미

  • Kim, Tae-Sung (Department of Earth and Environmental Sciences and The Earth and Environmental Science System Research Center Chonbuk National University) ;
  • Oh, Chang-Whan (Department of Earth and Environmental Sciences and The Earth and Environmental Science System Research Center Chonbuk National University) ;
  • Kim, Jeong-Min (Division of Earth and Environmental Sciences, Korea Basic Science Institute)
  • 김태성 (전북대학교 지구환경과학과, 전북대 지구환경시스템 연구소) ;
  • 오창환 (전북대학교 지구환경과학과, 전북대 지구환경시스템 연구소) ;
  • 김정민 (한국기초과학지원연구원)
  • Received : 2010.12.30
  • Accepted : 2011.04.20
  • Published : 2011.06.30
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Abstract

The igneous complex consisting of mangerite and gabbro in the Odaesan area, the eastem part of the Gyeonggi Massif, South Korea, intruded early Paleo-proterozoic migmatitic gneiss. The mangerite is composed of orthopyroxene, clinopyroxene, amphibole, biotite, plagioclase, pethitic K-feldspar, quartz. The gabbro has similar mineral assemblage but gabbro has minor amounts of amphibole and no perthitic K-feldspar. The gabbro occurs as enclave and irregular shaped body within the mangerite, and the boundary between the mangerite and gabbro is irregular. Leucocratic lenses with perthitic K-feldspar are included in the gabbro enclaves. These textures represent mixing of two different magmas in liquid state. SHRIMP U-Pb zircon age dating gave $234{\pm}1.2$ Ma and $231{\pm}1.3$ Ma for mangerite and gabbro, respectively. These ages are similar with the intrusion ages of post collision granitoids in the Hongseong (226~233 Ma) and Yangpyeong (227~231 Ma) areas in the Gyeonggi Massif. The mangerite and gabbro are high Ba-Sr granites, shoshonitic and formed in post collision tectonic setting. These rocks also show the characters of subduction-related igneous rock such as enrichment in LREE, LILE and negative Nb-Ta-P-Ti anomalies. These data represent that the mangerite and gabbro formed in the post collision tectonic setting by the partial melting of an enriched lithospheric mantle during subduction which occurred before collision. The heat for the partial melting was supplied by asthenospheric upwelling through the gab between continental and oceanic slabs formed by slab break-off after continental collision. The distribution of post-collisional igneous rocks (ca. 230 Ma) in the Gyeonggi Massif including Odaesan mangerite and gabbro strongly suggests that the tectonic boundary between the North and South China blocks in Korean peninsula passes the Hongseong area and futher exteneds into the area between the Yangpyeong-Odaesan line and Ogcheon metamorphic belt.

경기육괴 동부에 위치하는 오대산 지역에서는 맨거라이트와 반려암으로 구성된 화성암체가 원생대 초기에 형성된 혼성편마암을 관입하고 있다. 맨거라이트는 사방휘석, 단사휘석, 각섬석, 흑운모, 사장석, 퍼어사이틱 K-장석, 석영으로 이루어져 있으며 반려암의 광물군은 맨거라이트와 유사하나 반려암내에서는 각섬석이 사방휘석 주변에 적은 양으로 나타나며 퍼어사이틱 K-장석이 나타나지 않는다. 맨거라이트내에 반려암이 포획암 형태나 불규칙한 형태로 나타나며 두 암석의 경계가 불분명하다. 반려암질 포획암내에는 맨거라이트에서 볼 수 있는 퍼어사이틱 K-장석을 포함한 우백질부가 렌즈상으로 포함되어 있다. 이러한 것들은 두 개의 화성암이 액체상태에서 서로 혼합되었음을 지시한다. SHRIMP 저어콘 연대 측정결과 맨거라이트와 반려암으후부터 각각 $234{\pm}1.2$ Ma와 $231{\pm}1.3$ Ma의 트라이아스기 중기에 해당하는 연령을 얻었다. 이 연령은 홍성(226~233 Ma)과 양평 (227~231 Ma)지역의 트라이아스기 대륙충돌 후 화성암들의 연령과 유사하다. 맨거라이트와 반려암은 고함량 Ba-Sr 화성암(high Ba-Sr granite)이고 쇼쇼나이틱(shoshonitic) 하며, 대륙충돌 후 판 내부 환경에서 만들어졌다. 한편, 이 암석들은 대부분 경희토류와 친석원소가 부화되어 있으며 Nb-Ta-P-Ti 부(-) 이상을 보이는 섭입대 화성암의 특정도 보여준다. 위의 지화학적 특징들은 오대산 맨거라이트와 반려암은 대륙충돌 이전에 있었던 섭입시기에 지각물질에 의해 부화된 맨틀이 대륙충돌 후 분리된 대륙판과 해양판 사이 공간으로 유입된 연약권의 열에 의해 부분용융이 되면서 만들어졌음을 지시한다 오대산 지역의 맨거라이트와 반려암을 포함한 경기육괴와 임진강대 북부에 나타나는 약 230Ma의 대륙충돌 후 화성암의 분포는 이 시기에 일어난 한반도내 북중국판과 남중국판 충돌의 경계가 홍성 지역을 지나 양평-오대산지역과 옥천변성대 사이 지역으로 연결될 것임을 강하게 시사한다.

Keywords

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