排序方式： 共有3条查询结果，搜索用时 437 毫秒
1
1.
A. A. MARAKUSHEV A. V. BOBROV V. G. BUTVINA SANG Longkang LIU Rong Department of Petrology Geological Faculty Moscow State University Vorob''''evy Gory Moscow Russia Faculty of the Earth Sciences China University of Geosciences Wuhan 《Continental Dynamics》2001,(2)
1. IntroductionThe Maksyutov high-pressure complex is a part of Precambrian folded belt (mainly Proterozoic but reactivated in Phanerozoic) with eclogites, garnet pyroxenites, peridotites, and blueschists. As a global structure crossing the Asian continent (Fig. 1), this belt comprises two branches-the outer eclogite blueschist " peri-oceanic" (1-5 and 11-12 in Fig. 1) and the inner clinopyroxenite eclogite "peri-continental" (6-10 in Fig. 1) ones. Comparative petrological study of these co… 相似文献
2.
A new method has been suggested for evaluating the overall basicityof minerals and rocks by using ionization reactions involvingone proton: (sum of cations) + H2O = mineral + H+, (sum of cations) + H2O = (sum of normative minerals of a rock)+ H+. The basicity indicators are expressed as standard free energychanges of these reactions (). At standard water pressure (logPH2O = 0) and chemical activity of the metal ions ( log Mn+= 0), the relationship between and alkalinity of solutions(pH) becomes: = –2.303 RTlog H+ = 2.303 RT pH. The overall basicities of rock-forming oxides, minerals andmajor rocks were calculated from the thermodynamic data on ionsin water solutions and solid compounds. 相似文献
3.
A.A.MARAKUSHEV 《地学前缘》2002,9(3):13-22
宇宙中恒星的演化始于巨星的形成 ,后者的质量是太阳系的数百倍 ,寿命估计为数百万年。重元素合成于巨星的内部。它们控制了巨星爆炸过程中 (超新星 )形成的气态云和盘状物的冷凝加速度。冷凝和旋转的加速导致后代恒星质量越来越小 ,寿命越来越长 ,直到形成像太阳这样的小星体 ,其质量为 1.989× 10 30 kg ,寿命已有几十亿年。这些小恒星的形成是冷凝过程中产生的水成冰氢星子不断聚集的结果。上一代巨星的原始星盘中的物质只有一小部分参与了冰氢星子的形成。这些星体形成于致密、高速旋转的原始恒星星盘中 ,周围环绕着巨行星和褐矮星。由于星体达到恒星状态 ,它们开始影响原恒星盘 ,结果导致星体相互分散 ,同时 ,最近的巨星发生表面去气作用。后者可以从巨星到恒星的质量衰减得到证实。UpsilonAndromedae、5 5Cancri和HD16 84 4 3等天体的巨行星记载了这样的事实。太阳系中的表面去气作用主要反映在近太阳巨星的流体外壳完全消失。由于流体外壳消失 ,铁硅酸盐熔融核暴露地表 ,形成小的类地行星。木星也经历过表面去气作用 ,依据是木星具有很高的平均密度 (1.3g cm3) ,几乎是土星密度 (0 .7g cm3)的两倍。因此 ,类地行星的形成经历了两个阶段 :原行星 (其父巨星具有重的熔融核 )和正常行星 (在其父行星 相似文献
1