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2MASS 19281982-2640123 is a Sun-like star located in the area of Sagittarius constellation where the Wow! Signal is most widely believed to have originated. [1] [2] The star was identified in a 2022 paper as the most similar to the Sun out of the three solar analogs found inside the sky region.
The Wow! signal represented as "6EQUJ5". The original printout with Ehman's handwritten exclamation is preserved by Ohio History Connection. [1]The Wow! signal was a strong narrowband radio signal detected on August 15, 1977, by Ohio State University's Big Ear radio telescope in the United States, then used to support the search for extraterrestrial intelligence.
[1] [2] He is known for having identified a Sun-like star in the sky region where the Wow! signal came from as one of the possible sources of the radio signal. [ 3 ] [ 4 ] Caballero is also known for founding and coordinating the Habitable Exoplanet Hunting Project, an international effort consisting of more than 30 observatories searching for ...
Gray is best known for his work as an independent SETI researcher. [7] The Atlantic called Gray "the 'Wow!' signal's most devoted seeker and chronicler, having traveled to the very ends of the earth in search of it." [8] The Wow! signal was detected by the Ohio State University Radio Observatory (also known as Big
[2] The Wow! signal represented as "6EQUJ5" on the original computer printout. In 1977, the Big Ear recorded an unusual and possible extraterrestrial radio signal, which became known as the Wow! signal. The observation would prove to be unique, since no similar signals were ever detected afterwards. [3]
The signal appears to have originated from the direction of Proxima Centauri. It has been given the name Breakthrough Listen Candidate 1 . As of December 2020, the researchers were still working to rule out terrestrial interference, which they considered the most likely cause. One researcher called it "on par" with the Wow! signal.
The great aurora that was witnessed across Europe, the Americas, and Oceania had not been seen/documented in Europe since 1709, and in the Americas since 1888. The storm was remarkable primarily because of how far and wide it was observed, and for the brightness of its green strip lights and red glow, which led many to believe the cause was a fire.
The region is unusually devoid of any nearby stars. The closest star systems in the approximate region of the signal include the binary star G 73-11A and B, which are 106.1 light-years from the Sun, although the unrelated star G 73-10 is only 108.7 light-years away, less than three light-years from G 73-11A and B.