How were Supermassive Black Holes Already Forming and Releasing Powerful Jets Shortly After the Big Bang? - Universe Today | Canada News Media
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How were Supermassive Black Holes Already Forming and Releasing Powerful Jets Shortly After the Big Bang? – Universe Today

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In the past few decades, astronomers have been able to look farther into the Universe (and also back in time), almost to the very beginnings of the Universe. In so doing, they’ve learned a great deal about some of the earliest galaxies in the Universe and their subsequent evolution. However, there are still some things that are still off-limits, like when galaxies with supermassive black holes (SMBHs) and massive jets first appeared.

According to recent studies from the International School for Advanced Studies (SISSA) and a team of astronomers from Japan and Taiwan provide new insight on how supermassive black holes began forming just 800 million years after the Big Bang, and relativistic jets less than 2 billion years after. These results are part of a growing case that shows how massive objects in our Universe formed sooner than we thought.

Astronomers have known about SMBHs for over half a century. In time, they came to realize that most massive galaxies (including the Milky Way) have them at their cores. The role they play in the evolution of galaxies has also been the subject of study, with modern astronomers concluding that they are directly related to the rate of star formation in galaxies.

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Similarly, astronomers have found that SMBHs have tight accretion disks around them where gas and dust are accelerated to close to the speed of light. This causes the center of some galaxies to become so bright – what are known as active galactic nuclei (AGNs) – that they outshine the stars in their disks. In some cases, these accretion disks also lead to jets of hot material that can be seen from billions of light-years away.

According to conventional models, galaxies didn’t have enough time to develop central black holes when the Universe was less than a billion years old (ca. 13 billion years ago). However, recent observations have shown that black holes were already forming at the center of galaxies at the time. Addressing this, a team of scientists from SISSA proposed a new model that offers a possible explanation.

For their study, which was led by Lumen Boco – a Ph.D. student from the Institute for Fundamental Physics of the Universe (IFPU) – the team started with the well-known fact that SMBHs grow in the central regions of early galaxies. These objects, the progenitors of elliptical galaxies today, had a very high concentration of gas and an extremely intense rate of new star formation.

The first generations of stars in these galaxies was short-lived and quickly evolved into black holes that were relatively small, but significant in number. The dense gas that surrounded them led to significant dynamic friction and caused them to migrate quickly to the center of the galaxy. This is where they merged to create the seeds of supermassive black holes – which slowly grew over time.

Artist’s impression of the path of the star S2 as it passes very close to the supermassive black hole at the center of the Milky Way. Credit: ESO/M. Kornmesser

As the research team explained in recent SISS press release:

“According to classical theories, a supermassive black hole grows at the centre of a galaxy capturing the surrounding matter, principally gas, “growing it” on itself and finally devouring it at a rhythm which is proportional to its mass. For this reason, during the initial phases of its development, when the mass of the black hole is small, the growth is very slow. To the extent that, according to the calculations, to reach the mass observed, billions of times that of the Sun, a very long time would be required, even greater than the age of the young Universe.”

However, the original mathematical model they developed showed that the formation process for central black holes could be very rapid in its initial phases. This not only offers an explanation for the existence of SMBH seeds in the early Universe but also reconciles the timing of their growth with the known age of the Universe.

In short, their study showed that the process of migration and mergers of early black holes can lead to the creation of an SMBH seed of 10,000 to 100,000 solar masses in just 50-100 million years. As the team explained:

“[T]he growth of the central black hole according to the aforementioned direct accretion of gas, envisaged by the standard theory, will become very fast, because the quantity of gas it will succeed in attracting and absorbing will become immense, and predominant on the process we propose. Nevertheless, precisely the fact of starting from such a big seed as envisaged by our mechanism speeds up the global growth of the supermassive black hole and allows its formation, also in the Young Universe. In short, in light of this theory, we can state that 800 million years after the Big Bang the supermassive black holes could already populate the Cosmos.”

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In addition to proposing a working model for observed SMBH seeds, the team also suggested a method for testing it. On the one hand, there are the gravitational waves that these mergers would cause, which could be identifiable using gravitational wave detectors like Advanced LIGO/Virgo and characterized by the future Einstein Telescope.

In addition, the subsequent development phases of SMBHs is something that could be investigated by missions like the ESA’s Laser Interferometer Space Antenna (LISA), which is expected to launch by around 2034. In a similar vein, another team of astronomers recently used the Atacama Large Millimeter/submillimeter Array (ALMA) to address another mystery about galaxies, which is why some have jets and others don’t.

These fast-moving streams of ionized matter, which travel at relativistic speeds (a fraction of the speed of light), have been observed emanating from the center of some galaxies. These jets have been linked to a galaxy’s rate of star formation because of the way they expel matter that would otherwise collapse to form new stars. In other words, these jets play a role in the evolution of galaxies, much like SMBHs.

For this reason, astronomers have sought to learn more about how black hole jets and gaseous clouds have interacted over time. Unfortunately, it has been difficult to observe these kinds of interactions during the early Universe. Using the Atacama Large Millimeter/submillimeter Array (ALMA), a team of astronomers managed to obtain the first resolved image of disturbed gaseous clouds coming from a very distant quasar.

Reconstructed images of MG J0414+0534, showing emissions from dust and ionized gas around a quasar (red) and carbon monoxide gas (green), which have a bipolar structure along the jets. Credit: ALMA (ESO/NAOJ/NRAO), K. T. Inoue et al.

The study that describes their findings, led by Prof. Kaiki Taro Inoue of Kindai University, recently appeared in the Astrophysical Journal Letters. As Inoue and his colleagues explained, the ALMA data revealed young bipolar jets emanating from MG J0414+0534, a quasar located roughly 11 billion light-years from Earth. These findings show that galaxies with SMBHs and jets existed when the Big Bang was less than 3 billion years old.

In addition to ALMA, the team relied on a technique known as gravitational lensing, where the gravity of an intervening galaxy magnifies light coming from a distant object. Thanks to this “cosmic telescope” and ALMA’s high resolution, the team was able to observe the disturbed gaseous clouds around MG J0414+0534 and determine that they were caused by young jets emanating from an SMBH at the center of the galaxy.

As Kouichiro Nakanishi, a project associate professor at the National Astronomical Observatory of Japan/SOKENDAI, explained in an ALMA press release:

“Combining this cosmic telescope and ALMA’s high-resolution observations, we obtained exceptionally sharp vision, that is 9,000 times better than human eyesight. With this extremely high resolution, we were able to obtain the distribution and motion of gaseous clouds around jets ejected from a supermassive black hole.”

These observations also showed that the gas was impacted where it followed the direction of the jets, causing particles to move violently and become accelerated to speeds of up to 600 km/s (370 mps). What’s more, these impacted gaseous clouds and the jets themselves were much smaller than the size of a typical galaxy at this age.

Artist’s impression of MG J0414+0534, showing the powerful jets that disturb the surrounding gas in the host galaxy. Credit: Kindai University

From this, the team concluded that they were witnessing a very early phase of jet evolution in the MG J0414+0534 galaxy. If true, these observations allowed the team to witness a key evolutionary process in galaxies during the early Universe. As Inoue summarized:

“MG J0414+0534 is an excellent example because of the youth of the jets. We found telltale evidence of significant interaction between jets and gaseous clouds even in the very early evolutionary phase of jets. I think that our discovery will pave the way for a better understanding of the evolutionary process of galaxies in the early Universe.”

Together, these studies demonstrate that two of the most powerful astronomical phenomena in the Universe emerged earlier than expected. This discovery also provides astronomers with the opportunity to explore how these phenomena evolved over time, and the role they played in the evolution of the Universe.

Further Reading: SISSA, ALMA, Astrophysical Journal, Astrophysical Journal Letters

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Here’s how Helene and other storms dumped a whopping 40 trillion gallons of rain on the South

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More than 40 trillion gallons of rain drenched the Southeast United States in the last week from Hurricane Helene and a run-of-the-mill rainstorm that sloshed in ahead of it — an unheard of amount of water that has stunned experts.

That’s enough to fill the Dallas Cowboys’ stadium 51,000 times, or Lake Tahoe just once. If it was concentrated just on the state of North Carolina that much water would be 3.5 feet deep (more than 1 meter). It’s enough to fill more than 60 million Olympic-size swimming pools.

“That’s an astronomical amount of precipitation,” said Ed Clark, head of the National Oceanic and Atmospheric Administration’s National Water Center in Tuscaloosa, Alabama. “I have not seen something in my 25 years of working at the weather service that is this geographically large of an extent and the sheer volume of water that fell from the sky.”

The flood damage from the rain is apocalyptic, meteorologists said. More than 100 people are dead, according to officials.

Private meteorologist Ryan Maue, a former NOAA chief scientist, calculated the amount of rain, using precipitation measurements made in 2.5-mile-by-2.5 mile grids as measured by satellites and ground observations. He came up with 40 trillion gallons through Sunday for the eastern United States, with 20 trillion gallons of that hitting just Georgia, Tennessee, the Carolinas and Florida from Hurricane Helene.

Clark did the calculations independently and said the 40 trillion gallon figure (151 trillion liters) is about right and, if anything, conservative. Maue said maybe 1 to 2 trillion more gallons of rain had fallen, much if it in Virginia, since his calculations.

Clark, who spends much of his work on issues of shrinking western water supplies, said to put the amount of rain in perspective, it’s more than twice the combined amount of water stored by two key Colorado River basin reservoirs: Lake Powell and Lake Mead.

Several meteorologists said this was a combination of two, maybe three storm systems. Before Helene struck, rain had fallen heavily for days because a low pressure system had “cut off” from the jet stream — which moves weather systems along west to east — and stalled over the Southeast. That funneled plenty of warm water from the Gulf of Mexico. And a storm that fell just short of named status parked along North Carolina’s Atlantic coast, dumping as much as 20 inches of rain, said North Carolina state climatologist Kathie Dello.

Then add Helene, one of the largest storms in the last couple decades and one that held plenty of rain because it was young and moved fast before it hit the Appalachians, said University of Albany hurricane expert Kristen Corbosiero.

“It was not just a perfect storm, but it was a combination of multiple storms that that led to the enormous amount of rain,” Maue said. “That collected at high elevation, we’re talking 3,000 to 6000 feet. And when you drop trillions of gallons on a mountain, that has to go down.”

The fact that these storms hit the mountains made everything worse, and not just because of runoff. The interaction between the mountains and the storm systems wrings more moisture out of the air, Clark, Maue and Corbosiero said.

North Carolina weather officials said their top measurement total was 31.33 inches in the tiny town of Busick. Mount Mitchell also got more than 2 feet of rainfall.

Before 2017’s Hurricane Harvey, “I said to our colleagues, you know, I never thought in my career that we would measure rainfall in feet,” Clark said. “And after Harvey, Florence, the more isolated events in eastern Kentucky, portions of South Dakota. We’re seeing events year in and year out where we are measuring rainfall in feet.”

Storms are getting wetter as the climate change s, said Corbosiero and Dello. A basic law of physics says the air holds nearly 4% more moisture for every degree Fahrenheit warmer (7% for every degree Celsius) and the world has warmed more than 2 degrees (1.2 degrees Celsius) since pre-industrial times.

Corbosiero said meteorologists are vigorously debating how much of Helene is due to worsening climate change and how much is random.

For Dello, the “fingerprints of climate change” were clear.

“We’ve seen tropical storm impacts in western North Carolina. But these storms are wetter and these storms are warmer. And there would have been a time when a tropical storm would have been heading toward North Carolina and would have caused some rain and some damage, but not apocalyptic destruction. ”

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Follow AP’s climate coverage at https://apnews.com/hub/climate

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Follow Seth Borenstein on Twitter at @borenbears

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Associated Press climate and environmental coverage receives support from several private foundations. See more about AP’s climate initiative here. The AP is solely responsible for all content.

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‘Big Sam’: Paleontologists unearth giant skull of Pachyrhinosaurus in Alberta

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It’s a dinosaur that roamed Alberta’s badlands more than 70 million years ago, sporting a big, bumpy, bony head the size of a baby elephant.

On Wednesday, paleontologists near Grande Prairie pulled its 272-kilogram skull from the ground.

They call it “Big Sam.”

The adult Pachyrhinosaurus is the second plant-eating dinosaur to be unearthed from a dense bonebed belonging to a herd that died together on the edge of a valley that now sits 450 kilometres northwest of Edmonton.

It didn’t die alone.

“We have hundreds of juvenile bones in the bonebed, so we know that there are many babies and some adults among all of the big adults,” Emily Bamforth, a paleontologist with the nearby Philip J. Currie Dinosaur Museum, said in an interview on the way to the dig site.

She described the horned Pachyrhinosaurus as “the smaller, older cousin of the triceratops.”

“This species of dinosaur is endemic to the Grand Prairie area, so it’s found here and nowhere else in the world. They are … kind of about the size of an Indian elephant and a rhino,” she added.

The head alone, she said, is about the size of a baby elephant.

The discovery was a long time coming.

The bonebed was first discovered by a high school teacher out for a walk about 50 years ago. It took the teacher a decade to get anyone from southern Alberta to come to take a look.

“At the time, sort of in the ’70s and ’80s, paleontology in northern Alberta was virtually unknown,” said Bamforth.

When paleontogists eventually got to the site, Bamforth said, they learned “it’s actually one of the densest dinosaur bonebeds in North America.”

“It contains about 100 to 300 bones per square metre,” she said.

Paleontologists have been at the site sporadically ever since, combing through bones belonging to turtles, dinosaurs and lizards. Sixteen years ago, they discovered a large skull of an approximately 30-year-old Pachyrhinosaurus, which is now at the museum.

About a year ago, they found the second adult: Big Sam.

Bamforth said both dinosaurs are believed to have been the elders in the herd.

“Their distinguishing feature is that, instead of having a horn on their nose like a triceratops, they had this big, bony bump called a boss. And they have big, bony bumps over their eyes as well,” she said.

“It makes them look a little strange. It’s the one dinosaur that if you find it, it’s the only possible thing it can be.”

The genders of the two adults are unknown.

Bamforth said the extraction was difficult because Big Sam was intertwined in a cluster of about 300 other bones.

The skull was found upside down, “as if the animal was lying on its back,” but was well preserved, she said.

She said the excavation process involved putting plaster on the skull and wooden planks around if for stability. From there, it was lifted out — very carefully — with a crane, and was to be shipped on a trolley to the museum for study.

“I have extracted skulls in the past. This is probably the biggest one I’ve ever done though,” said Bamforth.

“It’s pretty exciting.”

This report by The Canadian Press was first published Sept. 25, 2024.

The Canadian Press. All rights reserved.

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The ancient jar smashed by a 4-year-old is back on display at an Israeli museum after repair

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TEL AVIV, Israel (AP) — A rare Bronze-Era jar accidentally smashed by a 4-year-old visiting a museum was back on display Wednesday after restoration experts were able to carefully piece the artifact back together.

Last month, a family from northern Israel was visiting the museum when their youngest son tipped over the jar, which smashed into pieces.

Alex Geller, the boy’s father, said his son — the youngest of three — is exceptionally curious, and that the moment he heard the crash, “please let that not be my child” was the first thought that raced through his head.

The jar has been on display at the Hecht Museum in Haifa for 35 years. It was one of the only containers of its size and from that period still complete when it was discovered.

The Bronze Age jar is one of many artifacts exhibited out in the open, part of the Hecht Museum’s vision of letting visitors explore history without glass barriers, said Inbal Rivlin, the director of the museum, which is associated with Haifa University in northern Israel.

It was likely used to hold wine or oil, and dates back to between 2200 and 1500 B.C.

Rivlin and the museum decided to turn the moment, which captured international attention, into a teaching moment, inviting the Geller family back for a special visit and hands-on activity to illustrate the restoration process.

Rivlin added that the incident provided a welcome distraction from the ongoing war in Gaza. “Well, he’s just a kid. So I think that somehow it touches the heart of the people in Israel and around the world,“ said Rivlin.

Roee Shafir, a restoration expert at the museum, said the repairs would be fairly simple, as the pieces were from a single, complete jar. Archaeologists often face the more daunting task of sifting through piles of shards from multiple objects and trying to piece them together.

Experts used 3D technology, hi-resolution videos, and special glue to painstakingly reconstruct the large jar.

Less than two weeks after it broke, the jar went back on display at the museum. The gluing process left small hairline cracks, and a few pieces are missing, but the jar’s impressive size remains.

The only noticeable difference in the exhibit was a new sign reading “please don’t touch.”

The Canadian Press. All rights reserved.

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