“Something” Sends Strange Radio Circular Signals to Earth from Space – Teach Me About Science

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“Something” Sends Strange Radio Circular Signals to Earth from Space – Teach Me About Science

As the universe is a vast place full of mysteries we still don’t know, we only have an idea of ​​a small part of its vastness, so many more years of research and better technology are needed to answer the most challenging questions. For years we have been receiving radio signals from different points in the universe, and today astronomers seem to have an idea of ​​what is going on, and let’s take a look at their incredible discovery.

“Exciting Discovery in Space: Astronomers Reveal Secret of ‘Strange Radio Circles'”.

revealed the riddle “Radio Circles”, Intense star formation is important in distant galaxies

Since their discovery in 2019, “radio circles” (ORCs) have fascinated the scientific community. These giant rings of radio waves, which appear larger than galaxies in size, remain an unsolved mystery. At the American Astronomical Society meeting in New Orleans, a team of researchers presented a groundbreaking discovery that sheds light on the origins of these fascinating phenomena.

ORC: A Cosmic Puzzle

ORCs have been the subject of intense debate among astronomers since their initial discovery in 2019. Australian Square Kilometer Array Pathfinder (ASKAP), Consisting of 36 satellite dishes with a diameter of 12 meters, this led to the identification of these unusual rings. Despite intensive research, fewer than a dozen ORCs have been discovered and their nature remains largely a mystery. Some hypotheses have suggested that they may come from the remnants of supernova explosions in our own galaxy. However, a study published in October 2023 by researchers including Sumit Sarbadikari of Ohio State University compared six ORCs to samples of supernova remnants and found only one suitable candidate.

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The starburst theory

Most astronomers agree on that ORC remote objects And on a larger scale, they often have a galaxy at their center. Many galaxies have supermassive black holes at their centers, capable of swallowing matter and ejecting matter in opposite directions. These jets, caused by the impact of the gas surrounding the galaxy, appear as two giant lobes of radio waves.

Credits to Radio Signals, National Geographic

Galaxies can eject material when their central black hole engulfs an entire star, or when two galaxies merge and their black holes come together. However, these explanations have failed to convince astronomers because the radio emissions from ORCs lack distinct features and do not emit light at other wavelengths.

A massive stellar explosion a billion years ago: the origin of the ORCs

A possible explanation for ORCs emerged when Alison Coyle of the University of California, San Diego and her team studied the ORC4 material in more detail. Using the Keck Telescope in Hawaii, they observed the glow of oxygen atoms (OII), a phenomenon that occurs when ultraviolet light from bright young stars ionizes oxygen in surrounding gas clouds.

The team found that ORC4’s OII signal covered almost the entire galaxy and was ten times brighter than normal. This gas also had an unusually high velocity, indicating intense activity.

Based on a computational model, the researchers propose that about a billion years ago, the galaxy at the center of ORC4 experienced a brief but violent phase of star formation. This “starburst” led to the formation of large, bright stars that quickly extinguished and exploded as supernovae. This series of explosions created a powerful “galactic wind” that blew gas out of the galaxy. When it collided with the faint gas surrounding the galaxy, a shock wave was created. Radio telescopes have now detected this massive, slowly expanding shock wave that originated a billion years ago.

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Synchrotron light and radio waves

Within this shock wave, high-speed electrons perform spiral motions along the magnetic field lines, which the researchers believe creates synchrotron light. This phenomenon explains radio waves ORC4. The model also predicts that the interstellar wind will retreat toward the galaxy at the end of its path, creating a second shock wave. This wave ionizes additional oxygen atoms and explains the unusual production of OII light.

Implications of the invention

Confirmation of this model alone does not solve the problem ORC MYSTERY, but will also provide new knowledge about starbursts and their consequences. ORCs can act as “relics of past outflows,” allowing astronomers to observe gas at greater distances from galaxies. This has important implications for understanding spillovers.

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