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哈勃望远镜新发现:37 个矮星系中氧气离奇“失踪”

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NASA 近日公布了一张由哈勃太空望远镜拍摄的 NGC 4449 矮星系图像,这张发布于 2026 年 11 月 2 日的照片背后,是一项名为 GLOW(Galaxies Losing Oxygen via Winds)的系统性研究。研究团队利用哈勃望远镜对 37 个邻近矮星系进行了观测,结果发现这些星系中由恒星核合成的氧元素大量"失踪"——矮星系仅能保留其恒星所制造氧气的很小一部分,其余部分去向成谜。

氧气失踪案:矮星系的物质流失之谜

矮星系是宇宙中数量最多的星系类型,通常只包含数千至数亿颗恒星,与拥有数千亿颗恒星的银河系相比,其引力井明显更浅。这一结构特征正是 GLOW 研究关注的焦点:恒星内部的核聚变持续产生氧等重元素,并经由超新星爆发和恒星风将这些元素抛射到星际空间。但在引力束缚较弱的矮星系中,这些富含氧的气体很容易被星系风"吹出"星系边界,逃逸至星系际介质中。

观测数据显示,被研究的 37 个矮星系实际保有的氧气含量,远低于基于恒星形成历史推算的理论预期。这意味着大量金属元素已经通过外流机制永久离开了宿主星系,或者在星系外围以温热气体形态存在而难以被常规手段探测。无论哪种情形,这一发现都直接影响学界对矮星系化学演化模型的判断。

【关键数据】

- 观测样本: 37 个邻近矮星系

- 星系恒星规模: 数千至数亿颗恒星

- 代表性目标: NGC 4449 不规则矮星系

- 核心结论: 矮星系仅能保留恒星所产氧气的很小一部分

- 图像发布时间: 2026 年 11 月 2 日

哈勃望远镜拍摄的NGC 4449矮星系

宇宙化学演化的拼图缺口

氧是宇宙中丰度第三的元素,也是示踪星系气体循环的关键指标。矮星系作为宇宙化学演化的"活化石",其金属流失效率直接关系到对早期宇宙星系形成过程的理解。GLOW 研究的结果提示,现有模拟可能低估了矮星系中物质外流的强度,或者在反馈机制的物理细节上存在偏差。

后续观测:韦伯望远镜或将接棒

从长期看,确认这些"失踪"氧气的具体去向,需要更深入的紫外和红外观测能力。詹姆斯·韦伯太空望远镜的高灵敏度光谱设备有望探测矮星系外围的温热气体晕,从而验证氧气是以星系风形式彻底逃逸,还是以弥散形态潜伏在星系周边。这一谜题的解答,将为星系反馈与重元素循环理论补上关键一环,也为理解银河系自身的化学演化历史提供参照。


出处:Hubble Reveals Cosmic Mystery

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Researchers found that dwarf galaxies can hold onto only a small fraction of the oxygen made by their stars. NASA, ESA, Hubble Heritage–ESA/Hubble Collaboration, Alessandra Aloisi (STScI, ESA) This photo released on Nov. 2, 2026, showcases NGC ?4449, a dwarf irregular. Researchers using NASA’s Hubble Space Telescope studied 37 nearby dwarf galaxies — small galaxies containing a few thousand to hundreds of millions of stars — including NGC 4449 and found that much of the oxygen they expected to see is missing. Read more about this mystery. Image credit: NASA, ESA, Hubble Heritage–ESA/Hubble Collaboration, Alessandra Aloisi (STScI, ESA) Was this page helpful? ×
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