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The doughnut-shaped rings surrounding many supermassive black holes tell researchers how fast extraterrestrial objects are feeding and could change how black holes are viewed from Earth. Credits: ESA/NASA, AVO project and Paolo Padovani The researchers used X-ray telescopes and new data analysis techniques to describe extraterrestrial objects. Black holes with different light signatures that were once thought to be the same object viewed from different angles are actually in different stages of their life cycle, according to a study led by Dartmouth scientists. New research on black holes known as “active galactic nuclei,” or AGNs, says that it definitively demonstrates the need to revise the widely used “AGN unified model” that characterizes supermassive black holes because they all share the same properties. This study provides an answer to a troubling space mystery and should allow researchers to create more precise models of the evolution of the universe and...

Origin of ‘ghost particles’ DISCOVERED: Tiny bodies that pass through our body and planet undetected emitted from galactic cores fed by supermassive black holes in outer space ‘Ghost particles,’ or neutrinos, are particles that originate from outer space These particles have no mass and hardly interact with matter Scientists believe they came from the core of a galaxy that was fed by a supermassive black hole Blazars are known for emitting bright beams of light and wind and are thought to also produce cosmic rays By Stacy Liberatore For Dailymail.com Published: 2:04pm EDT, July 25, 2022 | Updated: 2:18 p.m. EDT, 25 July 2022 Extraterrestrial ‘ghost particles’ likely originate from the cores of galaxies fed by supermassive black holes, according to a new study that could unravel the mystery of subatomic particles that formed before the universe. Ghost particles, or neutrinos, have baff...

A team of European astronomers led by Professor Kalliopi Dasyra of the National and Kapodistrian University of Athens, Greece, under the participation of Dr. Thomas Bisbas, University of Cologne modeled several emission lines in the Atacama Large Millimeter Array (ALMA) and the Very Large Telescope (VLT). ) observations to measure gas pressure in jet-affected clouds and surrounding clouds. With this unprecedented measurement, published recently in Natural Astronomy , they found that the bursts significantly changed the internal and external pressures of the molecular cloud in its path. Depending on which of the two pressures changes the most, both cloud compression and star formation triggers and cloud dissipation and star formation delays are possible in the same galaxy. “Our results suggest that supermassive black holes, even though they are located at the center of galaxies, can influence star formation across galaxies” said Professor Dasyra, adding that “study...

Credit: Public Domain CC0 A team of European astronomers led by Professor Kalliopi Dasyra of the National and Kapodistrian University of Athens, Greece, under the participation of Dr. Thomas Bisbas, University of Cologne modeled several emission lines in the Atacama Large Millimeter Array (ALMA) and the Very Large Telescope (VLT). ) observations to measure gas pressure in jet-affected clouds and surrounding clouds. With this unprecedented measurement, published recently in Natural Astronomy they found that the bursts significantly changed the internal and external pressures of the molecular cloud in its path. Depending on which of the two pressures changes the most, both cloud compression and star formation triggers and cloud dissipation and star formation delays are possible in the same galaxy. “Our results show that supermassive black holes, even though they are located at the center of galaxies, can influence star formation a...

A newly discovered star is so close to the center of our galaxy’s supermassive black hole that it completes an orbit in just four years. It is the shortest orbit for any of the stars around Sagittarius A*. This is an oval-shaped journey around a black hole that takes the star to an orbital speed of more than 2.5 percent of the speed of light. This discovery adds exciting new information about the strange dynamics of the center of the Milky Way. Although the center of our galaxy is quite quiet compared to other galaxies, the environment around Sgr A* is an extreme place. Black holes are monsters, which have a mass about 4 million times the mass of the Sun. Before astronomers confirmed its existence with live images, scientists deduced its existence and calculated its mass based on the star locked in orbit around Sgr A*. The star, called S2, is just one of a group of stars known as S-stars, which follow a long, sharp elliptical orbit around Sgr A*, with a black hole at one end of...