超新星遗迹西梅斯147
(原标题: Supernova Remnant Simeis 147)
2024-02-27
浏览次数: 15
我们很容易迷失在超新星遗迹西美斯147错综复杂、环状和扭曲的细丝中。这个丝状星云也被编号为Sharpless 2-240,它有一个流行的绰号——意大利面星云。在牛星座(金牛座)和御夫星座(御夫座)的交界处,令人印象深刻的气体结构覆盖了天空近3度,相当于6个满月。这大约是150光年,而恒星碎片云的估计距离是3000光年。这张合成图像包括通过窄带滤光片分离出的氢(红色)和氧(蓝色)发光气体的发射数据。据估计,这颗超新星的遗迹大约有4万年的历史,这意味着,当长毛象在地球上自由漫游时,这颗巨大的恒星爆炸发出的光第一次到达地球。除了不断膨胀的残骸,这场宇宙灾难还留下了一颗脉冲星,一颗旋转的中子星,是原恒星核心的残骸。
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It's easy to get lost following the intricate, looping, and twisting filaments of supernova remnant Simeis 147. Also cataloged as Sharpless 2-240, the filamentary nebula goes by the popular nickname the Spaghetti Nebula. Seen toward the boundary of the constellations of the Bull (Taurus) and the Charioteer (Auriga), the impressive gas structure covers nearly 3 degrees on the sky, equivalent to 6 full moons. That's about 150 light-years at the stellar debris cloud's estimated distance of 3,000 light-years. This composite image includes data taken through narrow-band filters isolating emission from hydrogen (red) and oxygen (blue) glowing gas. The supernova remnant has an estimated age of about 40,000 years, meaning light from this massive stellar explosion first reached the Earth when woolly mammoths roamed free. Besides the expanding remnant, this cosmic catastrophe left behind a pulsar, a spinning neutron star that is the remnant of the original star's core.
© Stéphane Vetter (Nuits sacrées)