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Isotopic evidence for a young lunar magma ocean

机译:年轻农历海洋的同位素证据

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Mare basalt sources and ferroan anorthosite suite cumulates define a linear array on a (146)sm/Nd-144 versus Nd-142/Nd-144 isochron plot demonstrating these materials were derived from a common reservoir at 4336(+31)/-32 Ma. The minimum proportion of the Moon that was in isotopic equilibrium at this time is estimated to be 1-3% of its entire volume based on the geographic extent from which the analyzed samples were collected and the calculated depths from which the samples were derived. Scenarios in which large portions of the Moon were molten to depths of many hundreds of kilometers are required to produce the observed Sm-Nd isotopic equilibrium between the mantle and crustal rocks at 4.34 Ga. This is a consequence of the fact that limited heating of a solid Moon above the blocking temperature of the Sm-Nd isotopic system is insufficient to diffusively homogenize radiogenic Nd throughout the mantle and crust. There are three scenarios that might account for global-scale isotopic equilibrium on the Moon relatively late in Solar System history including: (1) Sm-Nd re-equilibration of a solid Moon resulting from widespread melting in response to mantle overturn or a very large impact, (2) early accretion of the Moon followed by delayed cooling due to the presence of an additional heat source that kept a large portion of the Moon molten until 4.34 Ga, or (3) late accretion of the Moon followed by rapid cooling of the magma ocean late in Solar System history. Neither density-driven overturn of the mantle, nor a large impact, are likely to homogenize the mantle and crust to the extent required by the Sm-Nd isochron. Likewise, secondary heating mechanisms, such as tidal heating or radioactive decay, are not efficient enough to keep the Moon molten to the depth of the mare basalt source regions for many tens to hundreds of millions of years. Instead, the age of equilibrium between such a compositionally diverse set of rocks, produced on a global scale, likely records the t
机译:海玄武岩源和斜长含铁套件限定进行累积上的线性阵列(146)的SM / ND-144对的Nd-142 / ND-144等时线情节证明这些材料从一公用的蓄液衍生的4336(31)/ - 32嘛。那是在同位素平衡此时的月亮的最小比例估计为基于从收集分析样品的地理范围,并从该样品获得的计算出的深度其整个体积的1-3%。其中月亮的大部分被熔融到数百公里的深度场景需出示地幔和地壳岩石在4.34嘎之间的观测的Sm-Nd同位素平衡,这是以下事实的一个结果,即一个有限的加热固体月亮上述的Sm-Nd同位素系统的阻塞温度在整个地幔和地壳不足以漫搅匀放射的Nd。有三种情况可能在太阳系历史占月球全球规模的同位素平衡相对较晚,包括:从大范围融化响应产生的固体月亮(1)的Sm-Nd再平衡地幔翻倒或非常大的影响,(2)月亮的早期增生随后延迟到额外的热源的存在下保持熔化,直到4.34 Ga或月亮的大部分冷却由于(3)月亮的后期积之后迅速冷却的岩浆海洋在太阳系的历史晚了。既不密度驱动地幔的翻转,也有很大的影响,有可能以均质化地幔和地壳到由SM-Nd等时所要求的程度。同样地,二次加热机构,例如潮汐加热或放射性衰变,效率不高,足以让熔融到海玄武岩源极区为几十深度数亿年月亮。相反,这样的组成多样的岩石,在全球范围内生产之间的平衡的年龄,可能记录的T

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