天文学家证实了单个黑洞的存在。
Astronomers confirm the existence of a lone black hole

原始链接: https://phys.org/news/2025-04-astronomers-lone-black-hole.html

天文学家首次证实了独立黑洞的存在。由空间望远镜科学研究所领导的一个团队研究了一个最初在2022年被认定为可能是独立黑洞的天体,这一说法后来受到了质疑。利用哈勃太空望远镜和盖亚空间探测器(2021-2022年的数据)的新数据,他们证实该天体的质量大约是太阳的七倍,排除了它是中子星的可能性。最初,研究小组注意到这个可能的独立黑洞是在它经过一颗遥远恒星前方时。这一事件放大了光线并改变了恒星的位置。另一个团队先前认为它是一颗中子星,现在已修改了他们的研究结果,支持它是黑洞的认定。这一证实标志着一个重大突破,因为此前所有被发现的黑洞都拥有伴星。研究小组希望利用计划于2027年发射的即将到来的南希·格雷斯·罗曼太空望远镜发现更多独立黑洞。

天文学家证实了单个黑洞的存在,这一发现之所以困难,是因为它不像之前发现的黑洞那样拥有伴星,那些黑洞是通过其与伴星光线的相互作用被发现的。这增加了这样一种可能性:宇宙中可能存在更多这样的孤独黑洞,但尚未被探测到。 一位评论者表达了对这些在太空中漂流的隐形实体的不安,它们能够吞噬行星和恒星。然而,其他人澄清说,黑洞的引力只有在物体穿过其事件视界时才会构成威胁,在远处,它的行为与任何其他具有可比质量的天体相似。真正的危险在于一个小而未被探测到的黑洞可能进入我们的太阳系并扰乱行星轨道,造成严重的引力扰动。

原文

A team of astronomers at the Space Telescope Science Institute, working with one colleague from the University of St Andrews' Center for Exoplanet Science and another from the European Southern Observatory, has confirmed the existence of a lone black hole. In their paper published in The Astrophysical Journal, the group describes how they studied newer data regarding an object they had spotted several years ago to confirm its identity.

In 2022, members of essentially the same team reported the discovery of what they described as a "dark object" moving through the constellation Sagittarius. They suggested it might be a lone black hole. Shortly thereafter, a second research team challenged that result, suggesting it was more likely a neutron star. After continuing to study the object, the original research team has found more evidence backing up their original claim that it is likely a lone black hole.

Prior to this new finding, all the that have been identified have also had a —they are discovered due to their impact on light emitted by their companion star. Without such a companion star, it would be very difficult to see a black hole. The one identified by the team was only noticed because it passed in front of a distant non-companion star, magnifying its light and shifting its position in the sky for a short while.

The research team made their initial observations using data from Hubble over the years 2011 to 2017. This time around, they looked at data from Hubble for the years 2021 and 2022, as well as from the Gaia space probe. They found that the object under review was approximately seven times as massive as the sun, showing that it could not be a neutron star, leaving only a black hole as the sole option.

Additionally, the second research team revised their neutron star assessment in 2023, agreeing that the object was indeed a black hole. They found that the object was around six solar masses, but the higher uncertainty in their measurement still keeps it consistent with the more recent results.

Now, the latest study by the original research team marks the first time the existence of a lone black hole has ever been confirmed. They hope to find more examples with the Nancy Grace Roman Space Telescope, which is scheduled to launch in 2027.

More information: Kailash C. Sahu et al, OGLE-2011-BLG-0462: An Isolated Stellar-mass Black Hole Confirmed Using New HST Astrometry and Updated Photometry, The Astrophysical Journal (2025). DOI: 10.3847/1538-4357/adbe6e

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Citation: Astronomers confirm the existence of a lone black hole (2025, April 18) retrieved 21 April 2025 from https://phys.org/news/2025-04-astronomers-lone-black-hole.html

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