一颗白矮星 - 翻译成英语

• a white dwarf

在 中文 中使用 一颗白矮星 的示例及其翻译为 英语

它是一颗巨大的恒星，如螃蟹的祖先，还是一颗白矮星，就像1006,1572和1604的恒星一样？四十年前，天文学历史学家FRichardStephen…?
Was it a massive star, like the Crab's progenitor, or a tiny white dwarf, like the stars of 1006, 1572, and 1604?

结果，它变成了一颗白矮星，阿尔梅达解释道。
As a result, it became a white dwarf, Almeida explained.

十亿后，太阳将成为一颗白矮星。
After 7.9 billion years from now, the Sun will become a White dwarf.

亿年后，太阳将变成一颗白矮星。
Six billion years from now the sun will become a white dwarf.

最终，太阳将变成一颗白矮星。
Ultimately, our Sun will turn into a white dwarf.

太阳寿命的最后将变成一颗白矮星。
At the end of its life, the Sun will become a white dwarf.

伴星B是一颗白矮星，有效温度为36,885K，已经冷却了约400万年。
The companion, component B, is a white dwarf of class DA with an effective temperature of 36,885 K that has been cooling down for around four million years.

当太阳变成一颗白矮星时，它在抛出外层的气体后加热会比较缓慢，”奥德尔说。
When the sun becomes a white dwarf, it will heat more slowly after it ejects its outer gaseous layers,” O'Dell said.

LP145-141是一颗白矮星，距离太阳系15光年，是距离太阳系第四近的白矮星。
LP 145-141 is a white dwarf located 15 light-years distant- the fourth-closest to the Solar System.

当一颗白矮星从另一颗恒星吸收物质时，这系统就会被称为“激变星(cataclysmicvariablestar)”。
When a white dwarf pulls material from another star, the system is described as a cataclysmic variable star.

当一对恒星诞生时，其中一颗恒星会先死亡，通常它会形成一颗白矮星。
When pairs of stars are born, the most massive dies first, often creating a white dwarf.

MiraA是一颗红巨星，MiraB是一颗白矮星。
Mira A is a red giant star, and Mira B(VZ Ceti) is a white dwarf.

此时它会经历红巨星阶段，然后再温和下来，成为一颗白矮星。
At this point it will pass through a red giant stage, then settle down to become a white dwarf.

随着时间的流逝，巨大的恒星失去了它们的气体，变成了一颗白矮星。
Over time, the giant star lost all its gas and became a white dwarf.

其伴星天狼星B，已经度过了主序星的过程，成为了一颗白矮星。
Its companion, Sirius B, is a star that has already evolved off the main sequence and become a white dwarf.

它还有一个伴星天狼星B，是一颗白矮星。
It also has a companion star called Sirius B, which is a white dwarf.

如果这颗恒星的质量和我们的太阳差不多，它的最终状态将是一颗白矮星。
If the star is about the mass of our sun, its end state will be a white dwarf.

核心本身会进一步收缩，成为一颗白矮星。
The core itself will shrink even more and it will become a white dwarf.

为了证明假设，多伊尔和杨的团队观察了一颗白矮星大气中的化学元素。
In order to prove their hypothesis, Doyle and Young's team observed the elements in the atmosphere of a white dwarf.

Ia型超新星需要完全破坏一颗白矮星，这是由太阳等恒星产生的紧凑残余物。
Type Ia supernovas entail the total destruction of a white dwarf, a compact remnant produced by stars like the Sun.