Nd, Sr and Noble Gas Isotopic Compositions of Alkali Basaltic Rocks and Mantle Xenoliths in the Baegryongdo

백령도에 분포하는 알칼리 현무암과 맨틀 포획암의 Nd-Sr과 영족기체 동위원소 조성

  • 김규한 (이화여자대학교 과학교육과) ;
  • ;
  • 장형숙 (이화여자대학교 과학교육과) ;
  • ;
  • 정정인 (이화여자대학교 과학교육과)
  • Published : 2002.12.01

Abstract

The rare earth elements (REE) and Nd, Sr and noble gas isotopic compositions eHer'He, 4$^{\circ}$Arp6Ar) for the Quaternary alkali basaltic rocks and mantle xenoliths in the basaltic rocks from the Baegryongdo were investigated to decipher the origin of alkali basaltic magma and xenolith beneath the Sino-Korean craton. Analytical results are summarized as follows; (1) The alkali volcanic rocks with voluminous xenoliths which are represented by the Mg-olivine and clinopyroxene dominant spinel-lherzolite in the Baegryongdo consist mainly of the basalt-mugearite and basaltic andesite. (2) The REE pattern of alkali basaltic rocks characterized by high HREE is similar to that of oceanic island basalt (OlB). Relatively concordant REE patterns of the basaltic rocks suggest that the alkali basaltic magma be formed by the identical source materials. (3) The Nd-Sr isotopic data of the alkali basaltic rocks suggest that the alkali basaltic magma be originated from the depleted mantle source with a little contamination of the continental crustal materials. (4) The $^3$He/ $^4$He ratios in olivines of xenoliths ranging from 5.0${\pm}$1.lRa to 6.7${\pm}$1.3Ra are lower than that of MORB (ca. 8.0Ra). It suggest that the xenolith be derived from the subcontinental lithospheric mantle. However, the high $^3$Her'He value of 16.8${\pm}$3.IRa at 1800$^{\circ}$C fraction (sample no OL-7) might be resulted from the post-eruptive cosmogenic $^3$He. The 4OAr/ 36 Ar ratios in olivines of mantle xenoliths are comparable to that of atmospheric argon, and are much lower than that of the MORB type mantle. These facts can lead to conclusion that the olivine of the xenolith in the Baegryongdo is affected by the post-eruptive atmospheric contamination during the slow degassing process.

백령도에서 산출되는 알칼리 현무암과 현무암내의 맨틀포획암에 대하여 REE와 Nd-Sr, 영족기체의 동위원소비를 분석하여 초염기성 포획암과 알칼리 현무암질 마그마의 기원을 해석하였다. 연구결과를 요약하면 다음과 같다. (1) 스피넬-러조라이트 맨틀 포획암을 다량 함유한 알칼리 현무암은 주로 현무암-뮤저라이트(mugearite)와 현무암질 안산암으로 구성되어 있다. (2)높은 HREE특징을 가지는 알칼리 현무암의 REE패턴은 OIB패턴과 유사하다. 그리고 상이한 시료들 간에 비교적 균일한 REE패턴은 알칼리 현무암질 마그마가 동일 기원물질에서 유래하였음을 시준하고 있다. (3)현무암의 Nd-Sr동위원소비는 알칼리 현무암질 마그마가 지각물질의 혼입영향이 없는 결핍맨틀 기원임을 가르키고 있다. (4)포획암중 감람석의 헬릅동위원소비($^3$He/$^4$He)는 5.0${\pm}$1.1Ra-6.7${\pm}$1.3Ra로 MORB 값(ca. 8.0Ra) 보다 낮으며 대륙지각 하부 리소스피어 맨틀의 특성을 나타내고 있다. 그러나 시료 OL-7 감람석의 높은 ($^3$He$^4$He(16.8${\pm}$3.1Ra) 값은 분출후 우주선 기원$^3$He의 혼입으로 추정된다. 감람석의 아르곤 동위원소비$^{40}$Ar$^{36}$Ar=300~500)는 MORB값(10,000~30,000)보다 훨씬 낮은 대기 아르곤의 동위원소비(295.5)에 가깝다. 이는 백령도 포획암의 감람석이 마그마 분출후 느린 탈가스 과정에 대기의 혼염이 있었음을 암시하고 있다.

Keywords

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