月球

The circumstances of an eclipse depend much on the apparent size of the Moon, and therefore on its phase in its anomalistic cycle and consequently in its full moon cycle.

一个食的状况与程度多少也也取决于月球外观的大小，因此对于满月时，其在近点月的阶段必然与满月周期有所关联。

If we make full use of the mid-infrared spectral features(i.e.,Christiansen Frequency features and reststrahlen bands),we could determine anorthite,olivine,quartz and alkali feldspar on the lunar surface successfully,which could not be accomplished by VIS-NIR spectra.

如果充分利用月球表面硅酸盐的红外光谱特征，即CF特征和Reststrahlen吸收带，将可以用于探测VIS-NIR光谱无法完成的探测目标：钙长石、橄榄石、石英和碱性长石等。

The anorthosite and similar rock types in the highlands and basalt lavas in the marea are the Moon's basic building blocks.

斜长岩和类似的岩石在高地典型，而玄武岩沉积在月球低地构成了月亮基本的建筑积木。

The crust became the white anorthosite, which floated atop the magma to form the lunar highlands. The basalt erupted later and subsequently solidified in the lowland marea.

这个壳后来变成白色的斜长岩，它漂在岩浆上面形成月球的高地，后来，玄武岩的岩浆喷发并且凝固在低地区域。

This conclusion, combined with the data obtained from the short-lived Hf-W and Sm-N d isotopic systematics, suggests that the Moon was initially accreted at 4.5 Ga, followed by development of the global lunar magma ocean. The primary lunar crust is composed by ferroan anorthosite which was produced by flotation of plagioclase during crystallization of the LMO. However, the mafic minerals, coevally crystallized with the plagioclase, sank to the base of the LMO due to their high density, and made up the main part of the lunar mantle, which served as the source during later mare basaltic magmatism.

根据这一年代资料，结合对月岩样品进行的短半衰期Hf-W与Sm-Nd同位素体系的研究结果，认为月球大致形成于45亿年，其后开始由岩浆海导致的内部核－幔－壳的分异，岩浆结晶的低密度斜长岩构成最初的月壳，而密度大的岩石构成月幔，而此月幔则成为后来月海玄武岩的主要岩浆源区。

It is at this apogee that it will come under the influcence of the moon's gravity.

正是在这个地点，它会根据月球的引力。

It is at this apogee that it will come under the influcence of themoon's gravity.

正是在这个地点，它会根据月球的引力。

With this, Chandrayaan-1 entered the Lunar Transfer Trajectory with an apogee of about 380,000 km.

与此，被输入月球调动弹道的Chandrayaan-1以远地点大约380，000公里。

However, there is a problem: the moon lacks any appreciable atmosphere.

然而目前面临的问题是：月球表面几乎没有大气存在。

The method does not require the supremum of the optimal approximation error being known.

引言月球探测车在松软土壤上行驶时的驱动动力学非常复杂。

The split between the two groups can hardly be papered over.

这两个团体间的分歧难以掩饰。

This approach not only encourages a greater number of responses, but minimizes the likelihood of stale groupthink.

这种做法不仅鼓励了更多的反应，而且减少跟风的可能性。