Supermassive black holes can be millions to billions of times the mass of our sun. To grow this big, you’d think these gravitational behemoths would need a lot of time to grow. But you’d be wrong.
When looking back into the dawn of our universe, astronomers can see these monsters pumping out huge quantities of radiation as they consume stellar material. Known as quasars, these objects are the centers of primordial galaxies with supermassive black holes at their hearts.
Now, using the twin W. M. Keck Observatory telescopes on Hawaii, researchers have found three quasars all with billion solar mass supermassive black holes in their cores. This is a puzzle; all three quasars have apparently been active for short periods and exist in an epoch when the universe was less than a billion years old.
Currently, astrophysical models of black hole accretion (basically models of how fast black holes consume matter — likes gas, dust, stars and anything else that might stray too close) woefully overestimate how long it takes for black holes to grow to supermassive proportions. What’s more, by studying the region surrounding these quasars, researchers at the Max Planck Institute for Astronomy (MPIA) in Germany have found that these quasars have been active for less than 100,000 years.
To put it mildly, this makes no sense.
“We don’t understand how these young quasars could have grown the supermassive black holes that power them in such a short time,” said lead author Christina Eilers, a post-doctorate student at MPIA.
Using Keck, the team could take some surprisingly precise measurements of the quasar light, thereby revealing the conditions of the environment surrounding these bright baby galaxies.
Models predict that after forming, quasars began funneling huge quantities of matter into the central black holes. In the early universe, there was a lot of matter in these baby galaxies, so the matter was rapidly consumed. This created superheated accretion disks that throbbed with powerful radiation. The radiation blew away a comparatively empty region surrounding the quasar called a “proximity zone.” The larger the proximity zone, the longer the quasar had been active and therefore the size of this zone can be used to gauge the age (and therefore mass) of the black hole.
But the proximity zones measured around these quasars revealed activity spanning less than 100,000 years. This is a heartbeat in cosmic time and nowhere near enough time for a black hole pack on the supermassive pounds.
“No current theoretical models can explain the existence of these objects,” said Joseph Hennawi, who led the MPIA team. “The discovery of these young objects challenges the existing theories of black hole formation and will require new models to better understand how black holes and galaxies formed.”
The researchers now hope to track down more of these ancient quasars and measure their proximity zones in case these three objects are a fluke. But this latest twist in the nature of supermassive black holes has only added to the mystery of how they grow to be so big and how they relate to their host galaxies.
These questions will undoubtedly reach fever-pitch later this year when the Event Horizon Telescope (EHT) releases the first radio images of the 4 million solar mass black hole lurking at the center of our galaxy. Although it’s a relative light-weight among supermassives, direct observations of Sagittarius A* may uncover some surprises as well as confirm astrophysical models.
But as for how supermassive black holes can possibly exist at the dawn of our universe, we’re obviously missing something — a fact that is as exciting as it is confounding.
One thought on “We’re Really Confused Why Supermassive Black Holes Exist at the Dawn of the Cosmos”
Shortly after the dawn of this present universe (Notice how I avoid the use of Big Bang.), all pervasive energy began to ‘cool and condense’ into matter. This occurred along corridors or as rivulets in reaction to pulses and waves passing through the medium. Long, hot, twisting, gyrating, growing/shrinking filaments developed throughout. As this metamorphosis progressed, segments of all sizes were loosened and flung near and far. As these units, now called (here) Omega Bodies, traveled through space, each collected an amount of dark matter and ‘real’ matter commensurate with their gravitational mass, speed of transit, density of matter through which they traveled, and duration of trip. This burgeoning halo tended to slow the object. Drawing upon this cache of matter, when slowed sufficiently the Omega Body set about the business of constructing a galaxy of stars. This ‘homestead’ galaxy was/is always elliptical in shape and character.
Thus, black holes, formally Omega Bodies, may be of any size. Dependent upon how a particular early universe filament disintegrated. An Omega Body may or may not stimulate the formation of a galaxy. Those that have not or do not are called dark galaxies. It is the destiny of all galaxies, families of galaxies, clusters or cratons* of galaxies, and super clusters to return to the natal area of all their founding Omega Bodies.
(Have I lost you?)