http://chineseinput.net/에서 pinyin(병음)방식으로 중국어를 변환할 수 있습니다.
변환된 중국어를 복사하여 사용하시면 됩니다.
권성택,남정영,Kwon, Sung-Tack,Lan, Ching-Ying 대한자원환경지질학회 1991 자원환경지질 Vol.24 No.3
We applied Sm-Nd isotopic system to so-called amphibolites occurring within the Ogcheon group to provide constraints on the age of the metasedimentary rocks and to characterize tectonic environment of basaltic magmatism. An internal mineral isochron age of $677{\pm}91Ma({\sigma})$ was obtained from a coarse-grained, intrusive, amphibolite near Mungyeong. Considering previous studies on the age of the Ogcheon group, we interpret that the isochron represents either early metamorphic or emplacement age. The depositional age of the metasedimentary rocks intruded by the amphibolite would be prior to late Proterozoic. The present study and Cambro-Ordovician fossil evidences of previous workers suggest that both Precambrian and Phanerozoic rocks are present in the Ogcheon group. Positive ${\varepsilon}$ Nd values(+2.4 to +3.5) of four whole rocks indicate mantle origin for the amphibolite. These isotopic data, along with published immobile trace element data of Cluzel et al.(1989), strongly suggest that parental rocks of the amphibolite formed in an intraplate environment rather than in island arc or midocean ridge. The age and tectonic environment of amphibolites in the Ogcheon belt suggest that the basaltic magmatism may be related to the late Proterozoic break-up of a presumed supercontinent, but not to the Triassic(?) collision between North and South China continents.
권성택(Sung-Tack Kwon) 한국암석학회 2014 암석학회지 Vol.23 No.3
이 논문은 지구의 나이를 알기 위한 초기의 다양한 시도를 간략히 소개하고, 운석의 납동위원소 연대측정으로 처음으로 지구의 나이가 4,550±70Ma임을 밝힌 Patterson (1956)의 연구를 재조명한다. 태양계 초기의 진화과정은 성운가스가 식으면서 응축되어 만들어지는 고체입자 -> 이들 입자들이 서로 들러붙어 커지는 첨합과정을 통하여 행성 크기의 물체가 생성되는 것으로 생각되고 있다. 또한 이때 생긴 원시지구가 화성 크기의 물체와 충돌하면서 그 잔해가 달을 만들었다고 생각되고 있다. 이 일련의 과정에서 지구가 생성된 시기를 꼭 집어 말하기 힘들긴 하나, 현재 지구는 이 충돌의 직접적인 결과로 생각할 수 있기 때문에 이 충돌 시기를 지구의 나이로 정할 것을 제안한다. 기존 연구를 고려하면 충돌시기는 태양계에서 가장 먼저 만들어진 운석물질의 나이(즉, 태양계의 나이) 4567.30±0.16 Ma와 지구와 달 암석에서 가장 오래된 나이 4,456±40 Ma 사이로 개략적으로 제한될 수 있다. 이 충돌시기는 태양계 초기 행성 크기의 물체가 만들어지는 시간간격을 밝히고, 충돌 이후 생성된 지구와 달의 마그마 바다의 열 역사를 규명하는데 매우 중요하기 때문에, 앞으로 보다 정확한 충돌시기를 측정하려는 노력이 요구된다. This paper presents a brief historical review of various attempts to estimate the age of the Earth, and reappraises the study of Patterson (1956) which revealed for the first time that the age of the Earth is 4550±70 Ma by measuring Pb isotope ratios of several meteorites and a marine sediment. The standard model for the planetary formation of early solar system is: formation of solid particles condensed from the cooling of hot nebular gas -> formation of planet-sized bodies by accretion of those solid particles. The Moon is supposed to have formed from the accretion of the relicts produced by the collision of proto-Earth with Mars-sized body. It is not easy to pinpoint the age of the Earth, considering the series of events related to the formation of the Earth. So, I propose that the collision age as that of the Earth, since the present status of the Earth is thought to be the direct product of the collision. According to the previous studies, the collision age can be broadly constrained between the age (4567.30±0.16Ma) of the earliest condensates (CAI, calcium-aluminum rich inclusion) of the nebula gas, i.e., the age of the solar system, and the oldest age (4,456±40 Ma) among rocks and minerals of the Earth and the Moon. We need more precise estimation of the collision age, since it is important in estimating time scale for the formation of planet-size body and in revealing thermal evolution of magma oceans of the Earth and the Moon presumably developed right after the collision.