dwarf star

It orbits a dim red dwarf star at such a close distance that temperatures on its surface could be as high as 104 ° C-too hot for most forms of life on Earth.

科学家怀疑这是因为它的大气层更厚。这颗行星围绕一颗暗红色的小行星近距离运行，因此其表面温度高达104摄氏度，这个温度对于地球上的大部分生物来说都太高。

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Another hypothesis is that the unusual radio source originates from a binary system containing a hot white dwarf, neutron star, or black hole, and that the waterfall is just a jet from this energetic system.

另一个假说认则为这种不寻常的射电源源于二进制系统，包含热白矮星、中子星或黑洞，瀑布只是能量系统在释放而已。

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Is it an accretion, black hole, corona or dwarf star?

是冲积层，黑洞，日冕还是矮星？

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Or, it seems, when you're cruising past a white dwarf star.

或者可以说在你缓慢驶过一颗白矮星时。

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How such a dense planet formed is unclear, the researchers say, but it's probably the crystalline vestige of a white dwarf star whose atmosphere was stripped away by the parent pulsar.

研究人员称，至于密度这么高的行星是如何形成的，这一点尚不清楚，但它很可能是一颗被主脉冲星剥夺了大气的白矮星留下的晶体残骸。

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It may be the remains of a carbon-rich white dwarf star.

它很可能是白矮星留下的残余物，白矮星核心堆积有大量的碳。

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The white dwarf star at the center of this planetary nebula may be accompanied by a second-generation world, formed from the debris of the dying star's original planets.

这颗濒临死亡的恒星将原有行星撕成碎块，第二代行星形成于这些碎块。

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In some ways, this Earth would resemble one of the tidally locked exoplanets commonly found in a red dwarf star's habitable zone, but a better comparison might be a very early Venus.

从某种角度来说，此时的地球会与那些潮汐锁定的地外行星类似——这样的行星常见于红矮星宜居带里，但更好的比较对象也许是非常早期的金星。

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The White Dwarf Star Sytems& The Composite System Compased of the Electron-Positive Energy System and the Helium-Ion-Negative Energy System

白矮星系统&正能谱电子系统与负能谱氦离子系统的复合系统

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Badenes's team examined archival observations and found a white dwarf and neutron star orbiting one another extremely closely.

Badenes的团队试验档案观测并发现白色小的中子星体非常近的围绕另一个运转。

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The planet, reported in the Astrophysical Journal Letters, is one of three detected orbiting a small red dwarf star called Wolf 1061 in the constellation Ophiuchus.

据《天体物理学》杂志报道，这颗行星系围绕红矮星沃尔夫1061旋转的三颗行星之一，这三颗行星都处于蛇夫座当中。

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Gliese 581g is one of two new worlds the team discovered orbiting the red dwarf star Gliese 581, bumping that nearby star's family of planets to six.

Gliese581g是环绕红矮星Gliese581两颗行星中的其中一颗，它的发现使该行星系内行星数量增加至6颗。

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The fundamental properties of white dwarf star in the evolution process of early stage has been analysed in detail.

详细地剖析了初期演化过程中的白矮星的基本特性。

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The rising red dwarf star shows expected stellar magnetic activity which includes dramatic and violent prominences.

上升中的红矮星有著可预期的磁场活动,包含了激烈的日珥现象.

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Solar system conspiracy theorists have long harbored suspicions that a hidden extra planet or dwarf star lies beyond the orbit of Pluto.

太阳系阴谋论者一直以来长期庇护这样一个观点，那就是在冥王星轨道深处还隐藏着一颗行星或是矮星。

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According as the original theory has regarded the white dwarf star system is a electron system alone, the helium-ion system is only looked as a external condition that the electron system is restricted.

但是PNES理论的基本原理和思路与原有的理论完全不同，按照原有理论，白矮星系统只是一种电子系统，氦离子系统只被视为约束电子系统的外部约束条件。

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Point a high-powered telescope at the constellation Cetus, the sea monster, and it is just possible to make out a dim red dwarf star shining in the tail.

使用高倍率望远镜观察鲸鱼座（Ceuts，名为海怪），也只能勉强看到星座尾部有一颗昏暗的红矮星在发光。

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Since a 7-solar-mass is too large to be a white dwarf or neutron star, it must be a black hole.

因为有着7个太阳质量的星体不可能是白矮星或中于星，所以它一定是黑洞。

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Who they are: Ray Palmer is a physicist who, will studying the molecular density of a white dwarf star, gains the ability to reduce his molecular density.

他们是谁？雷·帕尔默是一名科学家，后通过研究一块白矮星碎片获得了压缩自身分子结构的能力。

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The Upper-limit of the Equilibrium Mass of the White Dwarf Star

白矮星的平衡质量上限

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After it swallows the Earth, it will instead go through some phases of expansion and collapse, and will eventually settle down, leaving behind a small white dwarf star with the bullet still lodged in the center.

在它吞没地球后，它会经历一系列的膨胀和坍缩，最终一切都安宁下来，只留下一颗小小的白矮星，而那颗子弹还留在中央。

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Theory predicts that a white dwarf star will explode when infalling matter from a companion star increases the mass of the white dwarf beyond a critical mass limit, known as the Chandrasekhar limit.

理论预言，当来自伴星的物质让白矮星的质量增加到了临界质量极限即钱德拉塞卡极限时，白矮星就会爆发。

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But it's in the habitable zone because Proxima Centauri is a red dwarf star about 100 times fainter than the sun.

但因为比邻星是一颗红矮星，它比太阳暗100倍左右，因此行星位于宜居区。

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After this point, it would collapse into something like a sputtering white dwarf or neutron star, and then-if its mass kept increasing-eventually become a black hole.

自那以后，它会不断坍缩，直到变成一颗白矮星或者中子星——如果质量还是不停增加，它最终会变成一个黑洞。

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What is left after an explosion is a dwarf star of extraordinary density.

爆炸后所留下的是一个密度巨大的矮星。

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As a slowly contracting dwarf the star may remain luminous for billions of years.

收缩较慢的白矮星仍会发光几十亿年.

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The cluster of planets orbit a dim dwarf star, just barely the size of Jupiter, called Trappist-1.

这群行星围绕的暗矮星和木星差不多大，被称为特拉普1号。

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The sun's upper layers will expand and lose material, and eventually the core will cool enough to become a white dwarf star, and finally a black dwarf.

太阳的上层也将扩大，失去物质重量，最后中心冷却到一定程度就成了白矮星，最终成黑矮星。

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A Practical Negative-Energy Spectrum System& The White Dwarf Star

一个实际存在的负能谱系统&白矮星

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Most scientists agree a Type1a supernova occurs when a white dwarf star a collapsed remnant of an elderly star exceeds its weight limit, becomes unstable and explodes.

大多数科学家认为，当白矮星（年老恒星坍缩而成的残骸）超过质量极限，变得不稳定并爆发的时候，会产生Ia型超新星。

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