PENN STATE (US) — A newly discovered star system is the closest discovered since 1916—and the third-closest star system to the sun.
Both stars in the system are brown dwarfs—too small in mass to ever become hot enough to ignite hydrogen fusion. As a result, they’re cool and dim, resembling a giant planet like Jupiter more than a bright star like the sun.
“The distance to this brown dwarf pair is 6.5 light years—so close that Earth’s television transmissions from 2006 are now arriving there,” says Kevin Luhman, associate professor of astronomy and astrophysics at Penn State.
“It will be an excellent hunting ground for planets because it is very close to Earth, which makes it a lot easier to see any planets orbiting either of the brown dwarfs.” Since it is the third-closest star system, in the distant future it might be one of the first destinations for manned expeditions outside our solar system, Luhman says.
Named “WISE J104915.57-531906” because it was discovered in a map of the entire sky obtained by the NASA-funded Wide-field Infrared Survey Explorer (WISE) satellite, the system is only slightly farther away than the second-closest star, Barnard’s star, at 6.0 light years from the sun and discovered in 1916.
The closest star system consists of Alpha Centauri, a neighbor of the sun that was found in 1839 at 4.4 light years, and the fainter Proxima Centauri, discovered in 1917 at 4.2 light years.
“One major goal when proposing WISE was to find the closest stars to the sun,” says Edward (Ned) Wright, principal investigator for the WISE satellite and a professor of physics and astronomy at UCLA.
“WISE 1049-5319 is by far the closest star found to date using the WISE data, and the close-up views of this binary system we can get with big telescopes like Gemini and the future James Webb Space Telescope will tell us a lot about the low mass stars known as brown dwarfs.”
Astronomers have long speculated about the possible presence of a distant, dim object orbiting the sun, which is sometimes called Nemesis. However, “We can rule out that the new brown dwarf system is such an object because it is moving across the sky much too fast to be in orbit around the sun,” Luhman says.
To discover the new star system, Luhman studied the images of the sky that the WISE satellite had obtained during a 13-month period ending in 2011. During its mission, WISE observed each point in the sky two to three times.
“In these time-lapse images, I was able to tell that this system was moving very quickly across the sky—which was a big clue that it was probably very close to our solar system.
After noticing its rapid motion in the WISE images, Luhman went hunting for detections of the suspected nearby star in older sky surveys. He found that it indeed was detected in images spanning from 1978 to 1999 from the Digitized Sky Survey, the Two Micron All-Sky Survey, and the Deep Near Infrared Survey of the Southern Sky.
“Based on how this star system was moving in the images from the WISE survey, I was able to extrapolate back in time to predict where it should have been located in the older surveys and, sure enough, it was there,” Luhman said.
By combining the detections of the star system from the various surveys, Luhman was able to measure its distance via parallax, which is the apparent shift of a star in the sky due to the Earth’s orbit around the sun. He then used the Gemini South telescope on Cerro Pachón in Chile to obtain a spectrum of it, which demonstrated that it had a very cool temperature, and hence was a brown dwarf.
“As an unexpected bonus, the sharp images from Gemini also revealed that the object actually was not just one but a pair of brown dwarfs orbiting each other,” Luhman says.
“It was a lot of detective work. There are billions of infrared points of light across the sky, and the mystery is which one—if any of them—could be a star that is very close to our solar system.”
Source: Penn State