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浙赣中生代火山岩岩相与铀矿床类型研究 总被引:2,自引:0,他引:2
浙赣火山岩分布广泛并且产有重要的火山岩型铀矿床(赣杭构造带发育有五十一个火山岩型铀矿床)。通过对浙赣中生代火山岩相的划分及其特征的描述,划分出与其相对应的火山岩型铀矿床类型,即潜火山相对应于次火山岩型铀矿床、火山通道相对应于火山角砾岩筒型铀矿床、火山侵出相及火山喷发相之喷溢亚相对应于火山熔岩型铀矿床、火山喷发相之爆发亚相对应于火山碎屑岩型铀矿床、喷发沉积相对应于沉积火山碎屑岩型铀矿床。说明火山岩相与铀矿类型之间存在某种联系,研究火山岩相与其相对应的铀矿床对寻找火山岩型铀矿床有一定的指导意义。 相似文献
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IO Cnc was classified to be a new G-type(G0)W UMa-type eclipsing binary system.Our first multicolor photometric solutions show that IO Cnc is a new W-subtype shallow contact binary with a fill-out factor of f=16.1%and a low mass ratio of q=3.12(or 1/q=0.32).During orbital period investigations,a cyclic variation and a downward parabolic variation with a rate of(-1.28±0.43)×10-7 d yr-1 was discovered in the observed–calculated(O-C)curve.The cyclic variation was analyzed by the light travel time effect(LTTE)via a potential red dwarf companion star,an orbital semi-major axis shorter than 4.88±0.82 AU was obtained.Finally,we collect physical parameters of a sample of 50 G-type shallow contact binaries(f≤20%),it is suggested that most of the G-type shallow contact binaries are undergoing a longterm and periodic orbital period changes,especially more systems show long-term decreases.The long-term orbital period decrease indicates that IO Cnc is in a mass transferring from the more massive component to the less massive one.With the long-term decrease of the orbital period,this shallow contact binary will evolve into a deeper contact one. 相似文献
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