최초 시민과학 발견, 75억 광년 거리 희귀 ‘이상 전파 고리’ 공개

A recently identified cosmic structure, a rare “odd radio circle” (ORC) spotted through the collaboration of professional astronomers and citizen scientists, offers a unique glimpse into the universe’s energetic past. This newly discovered ORC, designated RAD J131346.9+500320, is the most distant one documented to date, located approximately 7.5 billion light-years from Earth. Its detection highlights the growing significance of public participation in 과학 탐사 and provides valuable data for understanding the 은하의 진화와 초거대 블랙홀을 이해하는 데 귀중한 데이터를 제공합니다.

A Celestial Rarity Revealed

Odd radio circles are enigmatic phenomena characterized by their faint, circular radio emissions and immense size, often spanning hundreds of thousands of light-years, dwarfing even our own Milky Way galaxy. These structures are believed to be composed of magnetized plasma and are typically found at the centers of galaxies. While initially discovered about six years ago, their elusive nature has made them difficult to study. The newly found ORC is particularly notable as it exhibits a double-ringed structure, a characteristic observed in only one other previously identified ORC. Researchers theorize that the apparent intersection of these rings is an artifact of our Earth-bound perspective, with the rings likely existing at different distances in space.

Citizen Science Drives Discovery

The discovery of RAD J131346.9+500320 marks a significant milestone as it is the first odd radio circle identified through the efforts of citizen scientists. These individuals, engaged through initiatives like the RAD@home Astronomy Collaboratory, are trained to analyze vast datasets from radio telescopes, such as the Low Frequency Array (LOFAR) Telescope. The LOFAR telescope, an extensive network of antennas across Europe, is highly sensitive to low-frequency radio waves. The unusual double-ring formation of this particular ORC stood out in the LOFAR data, prompting further investigation by the scientific community. This collaborative approach underscores the power of distributed scientific effort in uncovering cosmic anomalies that might otherwise go unnoticed.

Theories on Origin and Evolution

The precise origin of odd radio circles remains a subject of ongoing research. Current hypotheses suggest a connection to major energetic events within central galaxies. One leading theory posits that a powerful explosive event, possibly involving jets emanating from a supermassive black hole, could have re-energized dormant clouds of magnetized plasma. These re-energized plasma clouds would then emit the observed radio rings. Supermassive black holes are known to launch powerful jets of energetic particles, and these jets, along with galactic winds, are thought to interact with the surrounding interstellar medium, potentially shaping these colossal radio structures. The discovery of two additional ORCs, one associated with a distinctively curved jet, further supports the idea that these phenomena are integral components of galaxy evolution influenced by central black hole activity and their environments.

Future Prospects and Lingering Questions

The discovery of this distant ORC allows astronomers to effectively observe events from billions of years ago, offering critical insights into the role these structures play in galactic evolution over vast timescales. Understanding how these energetic outbursts influence surrounding gas and affect star formation is a key area of 미래 연구의 핵심 영역입니다. Despite recent advancements, several questions persist regarding odd radio circles, including why they are only observed at such large scales and whether they originate from smaller, undetectable precursors. The development of next-generation instruments, such as the Square Kilometre Array (SKA), is expected to provide unprecedented detail for studying these objects. The SKA, anticipated to be fully operational by 2028, will possess the sensitivity and survey speed necessary to investigate ORCs in greater detail, potentially unlocking further secrets about the co-evolution of black holes and galaxies across cosmic history.