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恒星

与 恒星 相关的网络例句 [注:此内容来源于网络,仅供参考]

However, the ultimate mass of the star is determined both by the mass of the cloud out of which the star forms and by a number of feedback processes that occur during the evolution of the protostar.

然而,最终形成的恒星的质量是由恒星形成于其中的气体云的质量和星坯演化过程中的一系列反馈过程共同决定的。

We must continue our studies in this area to understand how the initially tiny protostar grows, layer by layer, to eventually form a massive star.

我们必须在此领域继续开展研究,以理解宇宙中最初的很小的原恒星是如何逐步发展,最终演化成大质量恒星

The protostar develops into a full-fledged star powered by thermonuclear fusion of hydrogen and other light elements in its core.

恒星在热核聚变的作用下最终成为一颗完全发育的恒星

Depending on the details, the gas orbiting star/protostar may be unstable and start to compress under its own gravity.

基于详细资料,围绕恒星、原恒星的气体会变得不稳定,然后开始在自己的重力下开始压缩。

As the cloud collapses, the material heats up and forms an embryonic star, or "protostar," at its center.

随后在星云中心形成一颗胚胎恒星,或&原恒星&。

According to their simulation, gravity acted on minute density variations in matter, gases, and the mysterious "dark matter" of the universe after the Big Bang in order to form this early stage of a star -- a protostar with a mass of just one percent of our sun.

根据他们的模拟,大爆炸之后,引力对宇宙中的物质、气体和神秘的&暗物质&起作用使其分布密度产生变化,从而形成原恒星状态——形成的原恒星质量只有太阳的1%。

A stellar flash like this has never been seen before -- supernovas and novas expel matter out into space.

恒星发生超新星或新星爆发过程中,恒星外层物质被抛射到太空之中。

We believe,however,that about two million years ago,another star wandering through space,happened to come near our sun just as the sun and the moon raise tides on the earth,so this star must have raised the surface of the sun.

我们相信,不管怎样,大约200万年前,有另一颗恒星在空间中漂移时,正好离太阳很近,就像太阳和月亮潮汐,所以这颗恒星肯定加速了日表的形成。

It would maneuver to a position along the line of sight between the telescope and a nearby star.

它能够移动至望远镜与恒星的视线中间,阻挡恒星的辐射,使其行星能被观测得到。

In order to know the effect of the turbulence, we performed calculations for the evolution of the Star with 8M (subscript ☉), and stadied the effect of turbulent stress on the evolution and structure of the star by comparing the ratio of the turbulent stress gradient to gravitation.

通过计算8M恒星从主序星到早期AGB星演化过程中湍流应力梯度与引力的比值来研究湍流作用对恒星演化与结构的影响。

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