Examples of using 的白矮星 in Chinese and their translations into English
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结晶的白矮星不仅仅是恒星的好奇心；.
Crystallized white dwarfs aren't just a stellar curiosity;所有的白矮星都会在其演化过程中的某个时刻结晶.
All white dwarfs will crystallize at some point in their evolution.不寻常的是，联星系统的白矮星可能拥有磁场。
Unusually, the white dwarf may have a magnetic field.这个极限附近的白矮星正处于灾难性爆炸的边缘。
White dwarfs near this limit are on the verge of a catastrophic explosion.年，天文学家发现了两颗有着110亿年历史的白矮星，这意味着它们可能正在向黑矮星转变的路上。
垂死的太阳将变成一个稠密的白矮星，被炫目耀眼的行星状星云所包围。
The dying Sun will transform into a dense white dwarf surrounded by a dazzling planetary nebula.研究小组检查了大约7000颗斯隆数字巡天项目观测到的白矮星，发现其中一颗与其他的都不一样。
The team had inspected around 7000 white dwarfs observed by the Sloan Digital Sky Survey and found one to be unlike any other.恒星剩余的内核最终会变成炙热的白矮星，朝周围环境释放紫外线辐射。
The remaining core of the star eventually becomes a hot white dwarf pouring out ultraviolet radiation into its surroundings.天文学家发现了一颗独一无二的白矮星，其大气层99%为氧气。
But astronomers have just discovered a white dwarf whose outer atmosphere is greater than 99.99% pure oxygen.以前，科学家发现了100个质量很低的白矮星，这表明它们比我们的宇宙还要老。
Previously, scientists detected 100 white dwarfs with very low mass, which suggests that they are older than our universe.它会变成一个微小的，但是很热而且非常致密的白矮星，它会在数十亿年内缓慢冷却。
It will then become a tiny-but hot and very dense- white dwarf that will slowly cool over billions of years.科学家仍在探索被污染的白矮星，找寻它们可能拥有的系外行星。
Scientists are still exploring polluted white dwarfs and looking for the exoplanets they may host.Em一项新发表的研究表明，超新星遗迹3C397是一颗单一的白矮星，它可以从正常的伴星上积累物质。
A newly published study reveals that supernova remnant3C 397 is the remains a single white dwarf that accumulated matter from a normal companion star.科学家估计，在30,000年后，NGC40将逐渐暗淡，而只留下一颗如同地球大小的白矮星。
About 30,000 years from now, scientists theorize that NGC 40 will fade away,leaving only a white dwarf star approximately the size of Earth.所有的白矮星都会在它们的进化过程中的某个时刻结晶，尽管更多的巨大白矮星会更快的完成这一过程。
He said that all white dwarfs would crystallise at some point in their evolution, although more massive white dwarfs go through the process sooner.这个系统包含了一颗靠近轨道中子星和一颗白矮星，还有一颗更远的白矮星围绕着这两颗恒星运行。
This system contains a closely orbiting neutron star and a KenudaMasuda说，他和他的同事将继续与同伴一起寻找小的白矮星，以了解有关它们的特性的更多信息。
Kento Masuda said that he andhis colleagues would continue searching for small white dwarfs with companions in order to learn more about their properties.接下来它将逐渐黯淡下去，最后成为所谓的白矮星。
It will get smaller and smaller,eventually becoming what we then call a white dwarf.从2005年4月的观测结果来看，3C397已经比原来的白矮星大了18倍。
The observations, from April 2005, indicate 3C 397 has swept up amass some 18 times greater than the original white dwarf.所有白矮星都会在进化过程中的某个时刻结晶，质量更大的白矮星会更早地经历这个过程。
All 这-第一次这样的碳的比例被发现在周围的白矮星的尘土飞扬的废墟。
This is the first time such a proportion of carbon hasbeen detected in the dusty debris surrounding white dwarfs.在巨蟹座ι系统里没有找到这个贡献者，但是推测有一个未看见的白矮星。
No such donor has been detected in the ι Cancri system,but it is assumed that there is an unseen white dwarf.在盖亚之前，我们有100-200颗具有精确距离和光度的白矮星-现在我们有200,000只。
Before Gaia we had 100-200 white dwarfs with precise distances and luminosities- and now we have 200,000.而太阳预计在大约100亿年后也会变成结晶化的白矮星。
Our Sun is expected to become a crystallized white dwarf in about ten billion years.所有的白矮星都会在它们的进化过程中的某个时刻结晶，尽管更多的巨大白矮星会更快的完成这一过程。
All white dwarfs will crystalize at some point in their evolution, although more massive white dwarfs go through the process sooner.天文学家推测它可能是第一颗拥有多个环的白矮星。
Astronomers suspect this could be the first known white dwarf with multiple dust rings.经过数十亿年的相互环绕，这些所谓的白矮星合并并从死亡中复活。
After billions of years circling around each other these so-called white dwarves merged and rose from the dead.
