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M27:不是彗星

(原标题: M27: Not a Comet)

2024-10-05

浏览次数: 17

在18世纪的法国上空寻找彗星时,天文学家查尔斯·梅西耶勤奋地记录了他在望远镜探险中遇到的东西,这些东西肯定不是彗星。这是他现在著名的非彗星名单上的第27名。事实上,21世纪的天文学家将其识别为行星状星云,但它也不是行星,尽管在小型望远镜中它可能看起来像行星一样圆形。梅西耶27 (M27)是一个很好的例子,它是由一颗类似太阳的恒星在其核心耗尽核燃料而形成的气体发射星云。当恒星的外层被驱逐到太空时,星云就形成了,在垂死恒星强烈但不可见的紫外线的激发下,原子产生了可见的光芒。这片美丽对称的星际气体云被称为哑铃星云,直径超过2.5光年,距离Vulpecula星座约1200光年。这张令人印象深刻的彩色图像突出了研究充分的中心区域的细节,以及星云外晕中较暗的、很少被成像的特征。

查看原文解释

While hunting for comets in the skies above 18th century France, astronomer Charles Messier diligently kept a list of the things encountered during his telescopic expeditions that were definitely not comets. This is number 27 on his now famous not-a-comet list. In fact, 21st century astronomers would identify it as a planetary nebula, but it's not a planet either, even though it may appear round and planet-like in a small telescope. Messier 27 (M27) is an excellent example of a gaseous emission nebula created as a sun-like star runs out of nuclear fuel in its core. The nebula forms as the star's outer layers are expelled into space, with a visible glow generated by atoms excited by the dying star's intense but invisible ultraviolet light. Known by the popular name of the Dumbbell Nebula, the beautifully symmetric interstellar gas cloud is over 2.5 light-years across and about 1,200 light-years away in the constellation Vulpecula. This impressive color image highlights details within the well-studied central region and fainter, seldom imaged features in the nebula's outer halo.

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