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Colossal Black Hole From the Early Universe Outgrows Its Host Galaxy





A new discovery runs counter to most observations about black holes, which are massive areas of space with extraordinarily strong gravity that can pull in anything -- even light. In most cases, black holes and their host galaxies expand at the same rate. But astronomers have spotted a super-sized black hole in the early universe that grew much faster than its host galaxy.

This particular black hole formed in the early universe, roughly two billion years after the Big Bang. An international research group made the discovery during a project to map the growth of supermassive black holes across cosmic time. The team included astronomers from Yale University, ETH Zurich, the Max-Planck Institute in Germany, Harvard University, the University of Hawaii, INAF-Osservatorio Astronomico di Roma, and Oxford University.

"Our survey was designed to observe the average objects, not the exotic ones," said C. Megan Urry, Yale's Israel Munson Professor of Astrophysics and co-author of a study about the phenomenon in the journal Science. "This project specifically targeted moderate black holes that inhabit typical galaxies today. It was quite a shock to see such a ginormous black hole in such a deep field."

Deep-field surveys are intended to look at faint galaxies; they point at small areas of the sky for a longer period of time, meaning the total volume of space being sampled is relatively small.

This particular black hole, located in the galaxy CID-947, is among the most massive black holes ever found. It measures nearly 7 billion solar masses (a solar mass is equivalent to the mass of our Sun).

However, it was the mass of the surrounding galaxy that most surprised the research team. "The measurements correspond to the mass of a typical galaxy," said lead author Benny Trakhtenbrot, a researcher at ETH Zurich's Institute for Astronomy. "We therefore have a gigantic black hole within a normal-size galaxy."

Most galaxies, including our own Milky Way, have a black hole at their center, holding millions to billions of solar masses. Not only does the new study challenge previous notions about the way host galaxies grow in relation to black holes, it also challenges earlier suggestions that the radiation emitted by expanding black holes curtails the creation of stars.

Stars were still forming in CID-947, the researchers said, and the galaxy could continue to grow. They said CID-947 could be a precursor of the most extreme, massive systems observed in today's local universe, such as the galaxy NGC 1277 in the Perseus constellation, 220 million light years from the Milky Way. But if so, they said, the growth of the black hole still greatly anticipated the growth of the surrounding galaxy, contrary to what astronomers thought previously.

Urry and her colleagues credited the W.M. Keck Observatory in Hawaii and the Chandra COSMOS legacy survey in aiding the team's work. "The sensitivity and versatility of Keck's new infrared spectrometer, MOSFIRE, was critical to this discovery," Urry said.

The black hole at the center of the super giant elliptical galaxy M87 shoen at the top of the page in cluster Virgo fifty million light-years away, is the most massive black hole for which a precise mass has been measured -6.6 billion solar masses. Orbiting the galaxy is an abnormally large population of about 12,000 globular clusters, compared to 150-200 globular clusters orbiting the Milky Way.

The team theorized that the M87 black hole grew to its massive size by merging with several other black holes. M87 is the largest, most massive galaxy in the nearby universe, and is thought to have been formed by the merging of 100 or so smaller galaxies. The M87 black hole’s large size and relative proximity, astronomers think that it could be the first black hole that they could actually “see.”

The Daily Galaxy via Yale University

Image credit: NASA/Canada-France-Hawaii Telescope, J.-C. Cuillandre (CFHT).


light is not pulled into a black hole because of gravity, light is massless.

A photon has no "rest" mass because it is never at rest. But, it does have energy. Remember E=mc^2? This converts to E/c^2=m. The energy of a photo varies with it's frequency. The higher the frequency, the higher the energy. The current view estimates the high limit being 7 × 10^−17 eV. So, light does have a type of "mass" other than rest mass. Gravitational lenses bend light. The event horizon of a black hole is where the degree of bend causes it to orbit, like a satellite orbits the Earth. Any light that crosses this event horizon distance is pulled in.

12.000 globular clusters around M87 is the key to the dark matter mass of the galaxy, if we count at least one large black hole in the Globular cluster's center.

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