This one looked and behaved more like a typical comet. It is currently past Neptune on its way out of the solar system," Bergner said.Ī second interstellar object, the comet 2I/Borisov, was discovered visiting our solar system in 2019. It had a reddish color consistent with the colors of many small bodies in the solar system. "We don't know its place of origin but it was probably traveling through interstellar space for less than 100 million years. 'Oumuamua, whose name refers in the native Hawaiian language to a messenger arriving from a great distance, was first detected by the University of Hawaii's Pan-STARRS1 telescope. "The simplest explanation, and exactly what we would expect for an interstellar comet, fits all of the data with no fine-tuning," said study co-author Darryl Seligman, a postdoctoral fellow in planetary science at Cornell University. This model can explain the strange behavior of 'Oumuamua without needing to resort to any exotic physics or chemistry," said University of California, Berkeley astrochemist Jenny Bergner, lead author of the research published this week in the journal Nature. "The key finding is that 'Oumuamua may have started as a water-rich icy planetesimal broadly similar to solar system comets. The release of this hydrogen in a process called outgassing would not cause a visible tail. 'Oumuamua then was warmed up as it passed through our inner solar system, causing the comet's ice structure to rearrange and releasing the trapped hydrogen gas - giving 'Oumuamua a little bit of a kick as it headed away from the sun. This converted some of the comet's ice - frozen water - into hydrogen gas that was trapped within the rest of its ice. Researchers said it appears that 'Oumuamua was born like many other comets as what is called a planetesimal - a small object formed in the early stages of planet formation - and was essentially a large, icy space rock.Īfter it was somehow ejected from its solar system of origin, they said, the comet's chemistry changed as it was bombarded by high-energy radiation while venturing through interstellar space. Smaller than originally estimated, it is now pegged at approximately 375 feet (115 meters) by 365 feet (111 meters), with a thickness of about 60 feet (19 meters). It was previously described as being cigar-shaped but now is thought to resemble a rocky pancake. 'Oumuamua (pronounced oh-MOO-uh-MOO-uh) lacks the tail of gas and dust characteristic of many comets. A new study has offered a more sober explanation - that 'Oumuamua's speed-up was due to the release of hydrogen gas as the comet warmed up in the sunlight. Hypotheses were floated in light of its unexpected behavior, including fleeting speculation that it might actually have been an alien spacecraft. “Yes, if it made a sudden, unexplainable turn that would certainly have warranted further exploration,” Knight added.WASHINGTON, March 23 (Reuters) - The quirky comet 'Oumuamua, the first interstellar object found visiting our solar system, has been the subject of fascination since being spotted in 2017, including its curious acceleration as it hurtled away from the sun. “Our key finding is that ‘Oumuamua’s properties are consistent with a natural origin, and an alien explanation is unwarranted,” said University of Maryland astronomer Matthew Knight, co-leader of the research published in the Nature Astronomy. It is estimated to be a half-mile (800 meters) long, tumbling through space. 2, 2018, after which it became too faint to detect even using the most powerful telescopes. Scientists tracked the reddish-colored ‘Oumuamua from Oct. But after poring over the data, an international team of researchers wrote that “we find no compelling evidence to favor an alien explanation.” Its odd shape and motion had prompted some scientists to wonder whether ‘Oumuamua - the first object from another star system found passing through our solar system - was some sort of alien technology perhaps exploring the cosmos. This artist's impression shows the first-known interstellar object to visit the solar system, 'Oumuamua, which was discovered on October 19, 2017, by the Pan-STARRS 1 telescope in Hawaii, U.S., with subsequent observations from ESO's Very Large Telescope in Chile and other observatories around the world.
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