{"id":11427,"date":"2024-07-10T12:07:18","date_gmt":"2024-07-10T16:07:18","guid":{"rendered":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/nasas-hubble-finds-strong-evidence-for-intermediate-mass-black-hole-in-omega-centauri\/"},"modified":"2024-07-10T12:07:18","modified_gmt":"2024-07-10T16:07:18","slug":"nasas-hubble-finds-strong-evidence-for-intermediate-mass-black-hole-in-omega-centauri","status":"publish","type":"post","link":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/nasas-hubble-finds-strong-evidence-for-intermediate-mass-black-hole-in-omega-centauri\/","title":{"rendered":"NASA\u2019s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri"},"content":{"rendered":"

NASA\u2019s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri<\/h2>\n

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4 Min Read<\/div>\n

\n\t\t\t\t\t\t\t\tNASA\u2019s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri\t\t\t\t\t\t\t<\/h1>\n<\/div>\n<\/div>\n
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This NASA Hubble Space Telescope image features the globular star cluster, Omega Centauri. <\/figcaption><\/div>\n<\/div>\n
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Most known black holes are either extremely massive, like the supermassive black holes that lie at the cores of large galaxies, or relatively lightweight, with a mass of under 100 times that of the Sun. Intermediate-mass black holes (IMBHs) are scarce, however, and are considered rare \u201cmissing links\u201d in black hole evolution.<\/p>\n

Now, an international team of astronomers has used more than 500 images from NASA\u2019s Hubble Space Telescope<\/a> \u2014 spanning two decades of observations \u2014 to search for evidence of an intermediate-mass black hole by following the motion of seven fast-moving stars in the innermost region of the globular star cluster Omega Centauri.<\/p>\n

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Omega Centauri is about 10 times as massive as other big globular clusters \u2013 almost as massive as a small galaxy \u2013 and consists of roughly 10 million stars that are gravitationally bound. <\/div>\n
ESA\/Hubble, NASA, Maximilian H\u00e4berle (MPIA)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n
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These stars provide new compelling evidence for the presence of the gravitational pull from an intermediate-mass black hole tugging on them. Only a few other IMBH candidates<\/a> have been found to date.<\/p>\n

Omega Centauri consists of roughly 10 million stars that are gravitationally bound. The cluster is about 10 times as massive as other big globular clusters \u2014 almost as massive as a small galaxy.<\/p>\n

Among the many questions scientists want to answer: Are there any IMBHs, and if so, how common are they? Does a supermassive black hole grow from an IMBH? How do IMBHs themselves form? Are dense star clusters their favored home?<\/p>\n

The astronomers have now created an enormous catalog for the motions of these stars<\/a>, measuring the velocities for 1.4 million stars gleaned from the Hubble images of the cluster. Most of these observations were intended to calibrate Hubble\u2019s instruments rather than for scientific use, but they turned out to be an ideal database for the team\u2019s research efforts.<\/p>\n

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This image shows the central region of the Omega Centauri globular cluster, where NASA\u2019s Hubble Space Telescope found strong evidence for an intermediate-mass black hole candidate.<\/div>\n
ESA\/Hubble, NASA, Maximilian H\u00e4berle (MPIA)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n
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\u201cWe discovered seven stars that should not be there,\u201d explained Maximilian H\u00e4berle of the Max Planck Institute for Astronomy in Germany, who led this investigation. \u201cThey are moving so fast that they would escape the cluster and never come back. The most likely explanation is that a very massive object is gravitationally pulling on these stars and keeping them close to the center. The only object that can be so massive is a black hole, with a mass at least 8,200 times that of our Sun.\u201d<\/p>\n

Several studies have suggested the presence of an IMBH in Omega Centauri. However, other studies proposed the mass could be contributed by a central cluster of stellar-mass black holes, and had suggested the lack of fast-moving stars above the necessary escape velocity made an IMBH less likely in comparison.<\/p>\n

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An international team of astronomers used more than 500 images from NASA\u2019s Hubble Space Telescope \u2013 spanning two decades of observations \u2013 to detect seven fast-moving stars in the innermost region of Omega Centauri, the largest and brightest globular cluster in the sky. These stars provide compelling new evidence for the presence of an intermediate-mass black hole (IMBH) tugging on them. Only a few other IMBH candidates have been found to date. This image shows the location of the IMBH in Omega Centauri. If confirmed, at its distance of 17,700 light-years the candidate black hole resides closer to Earth than the 4.3-million-solar-mass black hole in the center of the Milky Way, which is 26,000 light-years away. Besides the Galactic center, it would also be the only known case of a number of stars closely bound to a massive black hole. This image includes three panels. The first image at left shows the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space. The second image shows the details of the central region of this cluster, with a closer view of the individual stars. The third image shows the location of the IMBH candidate in the cluster.<\/div>\n
ESA\/Hubble, NASA, Maximilian H\u00e4berle (MPIA)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n
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\u201cThis discovery is the most direct evidence so far of an IMBH in Omega Centauri,\u201d added team lead Nadine Neumayer of the Max Planck Institute for Astronomy in Germany, who initiated the study, together with Anil Seth from the University of Utah, Salt Lake City. \u201cThis is exciting because there are only very few other black holes known with a similar mass. The black hole in Omega Centauri may be the best example of an IMBH in our cosmic neighborhood.\u201d<\/p>\n

If confirmed, at a distance of 17,700 light-years the candidate black hole resides closer to Earth than the 4.3-million-solar-mass black hole in the center of the Milky Way, located 26,000 light-years away.<\/p>\n

Omega Centauri is visible from Earth with the naked eye and is one of the favorite celestial objects for stargazers living in the southern hemisphere. Located just above the plane of the Milky Way, the cluster appears almost as large as the full Moon when seen from a dark rural area. It was first listed in Ptolemy\u2019s catalog nearly 2,000 years ago as a single star. Edmond Halley reported it as a nebula in 1677. In the 1830s the English astronomer John Herschel was the first to recognize it as a globular cluster.<\/p>\n

The discovery paper led by H\u00e4berle et al. is published online<\/a> today in the journal Nature<\/a>.<\/p>\n

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Scientists think a massive object is gravitationally pulling on the stars within Omega Centauri, keeping them close to its center. Credit: NASA\u2019s Goddard Space Flight Center, Lead Producer: Paul Morris<\/figcaption><\/figure>\n
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The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA\u2019s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, Colorado, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, Maryland, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.<\/p>\n

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Media Contacts<\/span>:<\/strong><\/p>\n

Claire Andreoli<\/strong>
NASA\u2019s\u00a0<\/strong>Goddard Space Flight Center<\/strong><\/a>,\u00a0Greenbelt, MD<\/strong>
claire.andreoli@nasa.gov<\/strong><\/a><\/p>\n

Ray Villard
Space Telescope Science Institute, Baltimore, MD<\/strong><\/p>\n

Bethany Downer
ESA\/Hubble.org<\/strong><\/p>\n

Science Contact<\/span>:
Maximilian H\u00e4berle
Max Planck Institute for Astronomy, Heidelberg, Germany<\/strong><\/p>\n

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