恒星的例句大全

Astronomers can estimate the size and brightness of a star by its color.

天文学家从恒星的颜色可以估计它的大小和亮度.

" We now have a direct observation of a star at the moment of its death," says astronomer Robert Quimby of the California Institute of Technology in Pasadena.

“我们现在直接观测到一颗处于死亡时刻的恒星，”帕萨迪纳加州理工学院的天文学家罗伯特·奎姆比说。

This stellar population has a distribution that matches the extent of the 511 keV map.

这一恒星密度分布与511keV图的范围相符.

The image offers circumstantial evidence that a young star is being born inside the placental cloud.

该图片提供了一颗年轻恒星正从胚胎云中诞生的旁证。

Mean Positions of the 1800 Stars for the Begining of the Year During 3000 Years

1800颗恒星的三千年来的年首平位置

The chaotic pulsation in one zone stellar model

单带恒星模型的混沌脉动

Teacher: So as a star ages, it begins to using up the supply of hydrogen and it's swell begins turning red.

老师：随着恒星的年龄增加，其氢也逐渐用完，收缩变红。

A suitable method for finding the intrinsic brightness of a star was discovered by the American astronomer W. S. Adams.

美国天文学家W·S亚当斯发现了一种求恒星固有亮度的好办法。

The time for the earth to make one complete revolution around the sun, relative to the fixed stars.

以恒星为基准测定的地球在环绕太阳的轨道上公转一整周的时间。

When massive stars exhaust their nuclear fuel and can no longer resist the relentless, crushing force of gravity, they collapse violently.

当耗尽核燃料的时候，大型恒星再也抵挡不住核心引力造成的残酷的粉碎性重压，它们发生剧烈塌缩。

The Convective Effect in Stability of Stellar structure

恒星结构稳定性问题中的对流效应

The Influence of Turbulent Pressure on the Late Stages of Evolution of Low and Intermediate mass Star. ( II) The Effect of Turbulent Pressure on the Internal Structure and Evolution

湍流压对中小质量恒星后期演化的影响（I）湍流压对内部结构和演化的影响

Another expectation, which Hubble overturned, was that the circumstellar disks would be deeply embedded within their parent clouds and would therefore be impossible to see.

另外有一个被哈伯推翻的猜测，是因为环绕恒星的气盘深藏在其母云气之中，所以无从窥其究竟。

His statistics in the central plains of China can see stars about 2500.

他统计出在中国的中原地区能看到的恒星约有2500颗.

Instead, their large clouds of molecular gas and dust do, triggering furious episodes of star formation.

反而它们所在的巨大分子气体和尘埃云发生了碰撞, 形成了剧烈的恒星形成区域.

This paper summarizes the results of observation and study for star formation in different phases.

综述了恒星形成各个阶段的观测结果和研究现状以及成协的天体物理环境情况.

These waves compress existing gas and cause star formation.

这些波压缩现有的气体而引起恒星的形成.

Aether Drag, Stellar Aberration, and the Collapse of the Aether Theory.

以太的阻力，恒星光行差，以太理论的崩溃。

In 1952, Bondi solved the hydrodynamic version of the star in a static ambient medium, who showed a certain gravitational capture radius, got Bondi accretion rates.

Bondi（1952年）研究了恒星对静态气体的吸积问题，确定了引力捕获半径和得到了Bondi吸积率。

The early Proterozoic atmosphere and hydrosphere are similar to those of Archaeozoic in being still absent in oxygen. This is a very large circular collection of stars and gas that surrounds our Milky Way galaxy.

早元古代的大气圈、水圈与晚太古代相似，仍为缺氧性质。这是一个围绕银河系的恒星及大气圈群体。