NASA’s Hubble Telescope Spots Runaway Supermassive Black Hole Leaving Behind Trail of Newborn Stars

A supermassive black hole, weighing as much as 20 million Suns, has left behind a 2,00,000-light-year-long condensed trail of newborn stars, twice the diameter of the Milky Way galaxy, in its wake, according to the National Aeronautics and Space Administration (NASA), US.

Captured accidentally by NASA‘s Hubble Space Telescope, the black hole was seen racing through the intergalactic space so fast that, within our solar system, it could travel from Earth to the Moon in 14 minutes.

“We think we’re seeing a wake behind the black hole where the gas cools and is able to form stars. So, we’re looking at star formation trailing the black hole,” said Pieter van Dokkum of Yale University in New Haven, Connecticut, US.

“What we’re seeing is the aftermath. Like the wake behind a ship, we’re seeing the wake behind the black hole,” said van Dokkum.

The researchers have published their paper in The Astrophysical Journal Letters.

They said that the black hole lies at one end of the column, at the other end of which lies its parent galaxy. They think that the gas is being ‘shocked’ and heated from the motion of the black hole hitting the gas, or it could be radiation from an accretion disk around the black hole.

“This is pure serendipity that we stumbled across it,” van Dokkum added. He was looking for globular star clusters in a nearby dwarf galaxy.

“I was just scanning through the Hubble image and then I noticed that we have a little streak. I immediately thought, ‘oh, a cosmic ray hitting the camera detector and causing a linear imaging artifact.’ When we eliminated cosmic rays we realized it was still there. It didn’t look like anything we’ve seen before,” said van Dokkum.

Van Dokkum and his team followed up the sight with spectroscopy with the W M Keck Observatories in Hawaii. The star trail being “quite astonishing, very, very bright and very unusual” made them conclude that they were looking at the aftermath of a black hole flying through a halo of gas surrounding the host galaxy.

Astronomers suspect this phenomenon to likely be the result of multiple collisions of supermassive black holes, the first two having perhaps merged 50 million years ago. Brought together closer at their centres, they whirled around each other as a binary black hole, they said.

Then came another galaxy with its own supermassive black hole, mixing up the three to form a chaotic and an unstable configuration. One of the black holes robbed momentum from the other two black holes and got thrown out of the host galaxy, they said.

Following this, the remaining binary system of black holes shot off in the opposite direction, they said.

There is a feature seen on the opposite side of the host galaxy that might be the runaway binary black hole. Circumstantial evidence for this is that there is no sign of an active black hole remaining at the galaxy’s core, they said.

The next step, they said, would be to do follow-up observations with NASA’s James Webb Space Telescope and the Chandra X-ray Observatory to confirm the black hole explanation.


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Supermassive Black Holes Formed in Rare Regions of Gas Behind the Earliest Quasars: Study

Scientists have managed to determine one of the biggest mysteries in recent astrophysics – the formation of quasars in the early universe. These cosmic entities were first spotted in 2003, and soon after, over 200 quasars were identified by supermassive black holes. These 200 quasars had formed within the first billion years after the formation of the universe. Scientists had never managed to conclusively determine how these quasars formed so early in the universe. Now, a team of researchers has found out that these primordial quasars naturally formed in chaotic conditions of rare gas reservoirs of the early universe.

“The first supermassive black holes were simply a natural consequence of structure formation in cold dark matter cosmologies – children of the cosmic web,” said Dr Daniel Whalen from the University of Portsmouth.

Dr Whalen led the team of researchers behind the study that determined the origin of the quasars. The study was published on July 6 in the Nature.

The researchers used a supercomputer model to run simulations about where these quasars could form. Scientists found that the quasars managed to form when supermassive black holes, with a mass at least 1,00,000 times that of our Sun, in areas of space where cold powerful streams of gasses were found in strong concentrations. These gaseous streams were only found in about a dozen or so regions across a region of space 1 billion light-years across.

“Consequently, the only primordial clouds that could form a quasar just after cosmic dawn — when the first stars in the universe formed — also conveniently created their own massive seeds. This simple, beautiful result not only explains the origin of the first quasars but also their demographics – their numbers at early times,” Dr Whalen said.

Quasars are some of the most powerful and energetic objects in the universe. Found in the centre of distant galaxies, quasars are powered by supermassive black holes whose mass ranges from millions to tens of billions of solar masses. These black holes accrete nearby matter that heats up due to friction and pressure as they fall towards the black hole. The heat and electromagnetic energy created in this way are then released by the quasars in the form of electromagnetic energy.


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