十万个为什么·科学启蒙30篇(3)
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What Is the Milky Way?
银河系是什么
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The Milky Way is our home galaxy—a vast, rotating disk of over 100 billion stars.银河系是我们的家园星系——一个拥有超过一千亿颗恒星的巨大旋转盘。
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It looks like a hazy band of light across the night sky because we see it edge-on from inside.它在夜空中呈现为一条朦胧光带,因为我们正从内部侧向观测它。
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Our Solar System sits about 27,000 light-years from the galaxy’s dense, star-packed center.我们的太阳系位于距银河系致密、恒星密集的中心约2.7万光年处。
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Most stars, including the Sun, orbit the galactic center once every 225–250 million years.包括太阳在内的大多数恒星,每2.25亿至2.5亿年绕银河中心公转一周。
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A supermassive black hole named Sagittarius A* lives at the very heart of the Milky Way.银河系核心坐落着一个名为人马座A*的超大质量黑洞。
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Dark matter makes up about 90% of the galaxy’s total mass, though we cannot see it directly.暗物质约占银河系总质量的90%,但我们无法直接观测到它。
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Spiral arms—like the Orion Arm where Earth resides—contain young stars and glowing gas clouds.旋臂——例如地球所在的猎户臂——包含年轻恒星和发光气体云。
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The Milky Way is slowly merging with the smaller Andromeda Galaxy, a process that will take billions of years.银河系正缓慢地与较小的仙女座星系合并,这一过程将持续数十亿年。
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Radio telescopes help map its structure by detecting invisible hydrogen gas emissions.射电望远镜通过探测不可见的氢气辐射来绘制其结构。
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From outside, astronomers believe it would look like a bright white spiral with soft blue arms.天文学家认为,从外部看,银河系将呈现为一个明亮的白色漩涡,伴以柔和的蓝色旋臂。