Scientists identified a distant object with properties that lie between those of a galaxy and those of a so-called quasar.
The object was born relatively soon after the Big Bang.
Simulations had indicated that such objects would exist, but this is the first actual finding.
“The discovered object connects two rare populations of celestial objects, namely dusty starbursts and luminous quasars, and thereby provides a new avenue toward understanding the rapid growth of supermassive black holes in the early universe,” says Seiji Fujimoto, a postdoctoral fellow based at the Niels Bohr Institute at the University of Copenhagen.
The discovery can be attributed to the Hubble Space Telescope operated jointly by ESA and NASA.
With its location in space—undisturbed by weather changes, pollution etc.—the telescope can gaze further into the depths of the universe than would have been the case on the ground.
And in astronomy, looking further equals being able to observe phenomena which took place at earlier cosmic periods—since light and other types of radiation will have traveled longer to reach us.
The newly found object—named GNz7q by the team—was born 750 million years after the Big Bang which is generally accepted as the beginning of the universe as we know it.
Since the Big Bang occurred about 13.8 billion years ago, GNz7q origins in an epoch known as “Cosmic Dawn.”
The discovery is linked to a specific type of quasars. Quasars, also known as quasi-stellar objects, are extremely luminous objects.
Images from Hubble and other advanced telescopes have revealed that quasars occur in the centers of galaxies.
The host galaxy for GNz7q is an intensely star-forming galaxy, forming stars at a rate 1,600 times faster than our own galaxy, the Milky Way.
The stars, in turn, create and heat cosmic dust, making it glow in infrared to the extent that GNz7q’s host is more luminous in dust emission than any other known object at this period of the Cosmic Dawn.
In the most recent years it has transpired, that luminous quasars are powered by supermassive black holes, with masses ranging from millions to tens of billions of solar masses, surrounded by vast amounts of gas.
As the gas falls towards the black hole, it will heat up due to friction which provides the enormous luminous effect.
“Understanding how supermassive black holes form and grow in the early universe has become a major mystery.
Theorists have predicted that these black holes undergo an early phase of rapid growth: a dust-reddened compact object emerges from a heavily dust-obscured starburst galaxy, then transitions to an unobscured luminous compact object by expelling the surrounding gas and dust,” explains associate professor Gabriel Brammer, also of the Niels Bohr Institute.
“Although luminous quasars had already been found even at the earliest epochs of the universe, the transition phase of rapid growth of both the black hole and its star-bursting host had not been found at similar epochs,” Brammers says.
“Moreover, the observed properties are in excellent agreement with the theoretical simulations and suggest that GNz7q is the first example of the transitioning, rapid growth phase of black holes at the dusty star core, an ancestor of the later supermassive black hole.”
Curiously, GNz7q was found at the center of an intensely studied sky field known as the Hubble GOODS North field.
“This shows how big discoveries can often be hidden right in front of you,” Brammer says.
Finding GNz7q hiding in plain sight was only possible thanks to the uniquely detailed, multi-wavelength datasets available for GOODS North.
Without the richness of data, the object would have been easy to overlook, as it lacks the distinguishing features for quasars in the early universe.
“It’s unlikely that discovering GNz7q within the relatively small GOODS-N survey was just ‘dumb luck,’ but rather that the prevalence of such sources may in fact be significantly higher than previously thought,” Brammer adds.
The team now hopes to systematically search for similar objects using dedicated high-resolution surveys and to take advantage of the NASA/ESA/CSA James Webb Space Telescope.
“Fully characterizing these objects and probing their evolution and underlying physics in much greater detail will become possible with the James Webb Telescope.
Once in regular operation, Webb will have the power to decisively determine how common these rapidly growing black holes truly are,” Fujimoto concludes.
Both Fujimoto and Brammer are part of the Cosmic Dawn Center (DAWN), a collaboration between Niels Bohr Institute and DTU Space.
