我国某地工业白云母成因类型、控制矿化因素及其矿物学的研究

工业白云母的成因类型、控制矿化因素及其矿物学特征的研究,有助于白云母矿床的工业评价。作者根据三年的室內外工作所获实际资料对本区上述问题作一探讨。不当之处,敬希指正。在野外工作期间,得到张克安、刘人俊工程师和队上领导及其他同志的帮助;本文完     

Radiometry of near-earth asteroids

We report 10 micrometers infrared photometry for 22 Aten, Apollo, and Amor asteroids. Thermal models are used to derive the corresponding radiometric albedos and diameters. Several of these asteroids appear to have surfaces of relatively high thermal inertia due to the exposure of bare rock or a coarse regolith. The Apollo asteroid 3103, 1982 BB, is recognized as class E. The Jupiter-crossing Amor asteroid 3552, 1983 SA, is confirmed as class D, but low albedos remain rare for near-Earth asteroids.     

Cycle anatomy and variability in the storm-dominated type cincinnatian (Upper Ordovician): coming to grips with cycle delineation and genesis

Although parasequence and sequence are scale-independent terms, they are frequently applied only to specific scales of cycles. For example, meter-scale cycles are commonly assumed to be parasequences or PACs. In the Upper Ordovician Kope and Fairview Formations of northern Kentucky, we examined a succession of 50 meter-scale cycles that have been variously interpreted as deepening-upward, shallowing-upward, or showing no relationship with water depth. Our analysis shows that these cycles, characterized by shifts in storm-bed proximality, are highly variable in their thickness and internal construction. Most cycles are best considered high-frequency sequences, because deepening-upward intervals are common, and many cycles contain evidence of abrupt basinward shifts in facies as expected at sequence boundaries. A minority fit the parasequence model of shallowing-upward cycles bounded by flooding surfaces. Larger, 20 m scale cycles are defined by systematic thickening and thinning trends of meter-scale cycles. However, meter-scale cycles do not display any systematic trends in cycle anatomy as a function of position within the 20 m cycles or position within the Kope and Fairview Formations. The high cycle variability and the lack of systematic stratigraphic organization with respect to longer-term cyclicity reflect either the irregularity of relative sea-level changes, the poor recording of sea-level changes in this deep-water setting, or the generation of these cycles by climate-induced cyclicity in storm intensity. These three mechanisms would generate similar patterns at the outcrop scale, so it is not possible at the present to distinguish between them.     

陕西金堆城钼矿床中铁钼华的矿物学特征及其意义

铁钼华产于陕西金堆城斑岩钼矿床的氧化带内,该矿物以往被认为是钼华。笔者对该矿物进行了物理光学性质、化学成分、X射线衍射、穆斯堡尔谱、红外光谱以及失重和差热分析的研究,定名为铁钼华,其分子式为Fe_2(MoO_4)_3·6.8H_2O。同时,将其与国外天然和人工合成的铁钼华作了对比,确定其是在酸性氧化环境中形成的次生矿物。它是原生钼矿床的直接找矿标志。     

地壳究竟在哪里

矿物学资料与比较行星学提出了一个有争议的新假说一绝大部分地壳可能被埋在地幔深处.地球科学家早就猜想,在太阳系的星球中,我们星球的地质特征是独特的.在跨入行星探索时代的今天,比较行星学已经有力地证明了这个猜想.行星间相似性和差异性为我们提供了尚待发展的、关于行星(包括地球)起源与演化的普遍性理论的原始资料.我们已经知道,现存的一套关于地球的理论、规律和修正并来提供其他行星具体结构的约束条件.与其进一步修正这些“规律”,不如现在开始新的计划——即使这意味着放弃那些为绝大多数地球科学家“信”以为真的信条和假设.     

东秦岭地区钼矿床的铼-锇同位素年龄及其意义

金属矿床的成矿年龄多年来一直是矿床地质工作者关注的问题之一。中国地质科学院岩矿测试技术研究所建立的铼－锇同位素定年实验室，为研究钼矿床的形成时代提供了新的手段。因辉钼矿是最主要的含铼矿物之一，且基本上不含普通锇，其中所含＾１８７Ｏｓ是由＾１８７Ｒｅ衰变而来，故放射成因＾１８７Ｏｓ的积累是矿物年龄及铼含量的函数。本文采用同位素稀释－等离子体质谱法，测定了东秦岭钼矿带中几个不同类型的大型钼矿床的Ｒｅ－