Astronomers say an object observed speeding through our solar system last month has an unexpected cigar-like shape and originated from another star, making it the first confirmed interstellar asteroid.
The asteroid was first detected Oct. 19 by the University of Hawaii’s Pan-STARRS 1 telescope on Haleakala, Hawaii, as it scanned the sky to search for near-Earth objects for NASA. Calculations suggested it might be an interstellar interloper, and scientists announced Monday they have confirmed it came from outside our solar system.
Designated 1I/2017 U1 and nicknamed ‘Oumuamua — a Hawaiian word for messenger or scout — the object appears reddish in color and has an elongated shape.
“This thing is an oddball,” said Karen Meech from the University of Hawaii’s Institute for Astronomy, leader of an international team studying ‘Oumuamua. “What we found was a rapidly rotating object, at least the size of a football field, that changed in brightness quite dramatically. This change in brightness hints that ‘Oumuamua could be more than 10 times longer than it is wide — something which has never been seen in our own solar system.”
Measurements from an array of telescopes indicate the object is up to a quarter-mile (400 meters) long and spins once every 7.3 hours.
“This object is simply a piece of another solar system that was expelled, and it has been traveling through interstellar space for hundreds of millions of years, or billions of years. We don’t know,” said Paul Chodas, manager of NASA’s Center for Near-Earth Object Studies at the Jet Propulsion Laboratory in Pasadena, California.
“We think this object — 2017 U1 — is very long … and very narrow, perhaps maybe 40 meters (130 feet) or so in the other dimension,” Chodas said. “That’s a very unusual shape. We don’t see that in our solar system. None of the asteroids in our solar system look like that, so it’s very puzzling how it could have obtained this shape.”
Data and findings on the interstellar asteroid were published in the Nov. 20 issue of the journal Nature.
Astronomers initially classified the discovery as a comet last month, but further observations showed it to be inert, with no signs of gas or dust around it, prompting scientists to consider it an asteroid.
‘Oumuamua’s dark reddish color is similar to the hue of many objects in the Kuiper Belt, a zone of dwarf planets and asteroid-like worlds orbiting the sun beyond Neptune. Its appearance suggests ‘Oumuamua is dense, made up of rock or metallic elements and lacks significant water or ice, scientists said.
“We also see that it’s very reddish in color, which indicates that it’s been possibly in space a long time and irradiated by not only the light from our sun, but other suns as well,” said Lindley Johnson, NASA’s planetary defense officer.
The European Southern Observatory’s Very Large Telescope in Chile aimed its aperture at the object to determine its, color, brightness and orbit, revealing it came from the approximate direction of the bright star Vega in the constellation Lyra. But Vega has moved in its path around the Milky Way galaxy since ‘Oumuamua passed near its current position some 300,000 years ago, so the asteroid’s origin is still unknown.
After following a steep trajectory toward the inner solar system, ‘Oumuamua is now on the outbound leg of its hyperbolic orbit traveling more than 85,000 mph (38 kilometers per second) relative to the sun. As of Monday, the object was about 124 million miles (200 million kilometers) from Earth, positioned between the orbits of Mars and Jupiter but tilted on a trajectory inclined around 20 degrees from the plane of the planets that orbit the sun.
It will pass Jupiter’s orbit in May 2018 and surpass Saturn’s distance from the sun in January 2019. ‘Oumuamua’s trajectory will next take it toward the constellation Pegasus.
‘Oumuamua made its closest approach to Earth on Oct. 14 — before its discovery — at a distance of about 15 million miles (24 million kilometers), or around 60 times the distance between the Earth and the moon.
“It’s fading very fast,” Johnson said. “It’s a relatively small object, so it’s very dim, but we are continuing to try to use NASA assets like the Hubble Space Telescope and Spitzer to take observations to determine more about its size and composition.”
“We are continuing to observe this unique object,” said Olivier Hainaut, an astronomer at the European Southern Observatory. “And we hope to more accurately pin down where it came from and where it is going next on its tour of the galaxy. And now that we have found the first interstellar rock, we are getting ready for the next ones!”
Astronomers expect an interstellar object like ‘Oumuamua passes through the inner solar system about once per year, but they are difficult to find because of their faintness and quick movement, according to an ESO press release.
But ‘Oumuamua’s discovery did pose a nomenclature dilemma. The International Astronomical Union, the organization responsible for formally naming celestial objects, had to create a new classification for interstellar objects earlier this month, resulting in in the “I” in the official name 1I/2017 U1.
‘Oumuamua is moving too fast for any conventional rocket to catch up, and plans for future interstellar travel using light sails and miniature spacecraft have not been realized.
“For decades we’ve theorized that such interstellar objects are out there, and now — for the first time — we have direct evidence they exist,” said Thomas Zurbuchen, associate administrator for NASA’s science mission directorate. “This history-making discovery is opening a new window to study formation of solar systems beyond our own.”
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