Astronomers have discovered the most distant quasar known, which is so far from us that its light has taken more than 13 billion years to reach us. We see this quasar as it was a mere 690 million years after the Big Bang, and its light carries valuable information about the early history of the universe, in particular the reionization phase.

At the center of the quasar is a massive black hole with a mass of almost 1 billion solar masses. In addition, the quasar's host galaxy has been found to contain a large amount of gas and dust, challenging models of galactic evolution. The results have now been published in Nature and in the Astrophysical Journal Letters.

Astronomers have discovered the most distant known black hole: a so-called quasar whose light has taken 13 billion years to reach us. In consequence, the light shows that quasar as it was 13 billion years ago, a mere 690 million years after the Big Bang.

The discovery was part of a concerted, multi-year search for ever more distant quasars led by Fabian Walter and Bram Venemans of the Max Planck Institute for Astronomy. It was made by Eduardo Banados, of the Carnegie Institution for Science, using the institution's 6.5-meter Magellan telescopes in Chile.

Quasars are powered by supermassive black holes in the centers of galaxies - in this case, a black hole with almost a billion times the mass of the Sun. Matter such as gas falling onto the black hole will form an ultra-hot accretion disk before falling in, making the whole setup one of the most luminous objects in the universe: a quasar. The newly discovered quasar shines as brightly as 40 trillion Suns.

Distant quasars are valuable sources of information about the early universe. For one, they can be used to "X-ray" the universe over large distances. Quasar light can be decoded to yield information about the hydrogen atoms the light has encountered along its billion-light-year-journey. The light of the newly discovered most distant quasar yet carries crucial information regarding one of the earliest phases of the universe, the so-called reionization phase.

About 380,000 years after the Big Bang, the universe had cooled down sufficiently to form hydrogen atoms. Some hundreds of millions of years later, the energetic ultraviolet radiation of the first stars and the accretion disks of the first black holes reionized nearly all of the hydrogen in the universe, separating the electrons from the hydrogen nuclei (protons).

The timing and specifics of this cosmic reionization are still an open question. Eduardo Banados, lead author of the article describing the discovery, says: "Reionization was the universe's last major transition, and it is one of the current frontiers in astrophysics."

The newly discovered quasar adds a crucial data point: Its light shows that a significant fraction of hydrogen was still neutral 690 million years after the Big Bang. This favours models which predict that reionization happened comparatively late in the history of the universe.

Quasars as young as this one also yield valuable information about galaxy evolution. For instance, at almost a billion solar masses, the quasar's central black hole is comparatively massive. Explaining how such a massive black hole could have formed in such a comparatively short amount of available time is a challenge for models of supermassive black hole formation, and effectively rules out some of those models. Banados says: "Gathering all this mass in fewer than 690 million years is an enormous challenge for theories of supermassive black hole growth."

In an effort led by MPIA's Bram Venemans, the astronomers targeted the quasar with the millimeter telescope NOEMA, operated by IRAM, in the French Alps and the VLA radio telescope array in Socorro, New Mexico. With those observations, the astronomers were able to identify and examine the quasar's host galaxy.

Although the galaxy can be no more than 690 million years old, it has already formed an enormous amount of dust, and heavy chemical elements. This means it must already have formed a large amount of stars. Again, this is a challenge for models, this time for models of galaxy evolution.

Bram Venemans says: "Models of galaxy evolution will need to be able to explain how a galaxy could form the stars needed to produce the observed amounts of dust and heavier chemical elements in such a comparatively short time."

Reionization, black hole evolution, galaxy evolution - even with these first observations, the newly discovered quasar has given astronomers key information about cosmic history. Follow-up observations, as well as a search for similar quasars, are on track to put our picture of early cosmic history onto a solid footing.

* "An 800 Million Solar Mass Black Hole in a Significantly Neutral Universe at Redshift 7.5," Eduardo Banados et al., 2017 Dec. 7, Nature

* "Copious Amounts of Dust and Gas in a z = 7.5 Quasar Host Galaxy," Bram Venemans et al., 2017, Astrophysical Journal Letters

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ALMA discovers infant stars surprisingly near galaxy's supermassive black hole
Charlottesville VA (SPX) Dec 04, 2017
At the center of our galaxy, in the immediate vicinity of its supermassive black hole, is a region wracked by powerful tidal forces and bathed in intense ultraviolet light and X-ray radiation. These harsh conditions, astronomers surmise, do not favor star formation, especially low-mass stars like our sun. Surprisingly, new observations from the Atacama Large Millimeter/submillimeter Array (ALMA) ... read more

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Max Planck Institute For Astronomy
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