This image shows the orbit of the newly discovered solar system object SQ372 (blue), in comparison to the orbits of Neptune, Pluto, and Sedna (white, green, red). The location of the Sun is marked by the yellow dot at the center. The inset panel shows an expanded view, including the orbits of Uranus, Saturn, and Jupiter inside the orbit of Neptune. Even on this expanded scale, the size of Earth's orbit would be barely distinguishable from the central dot.Credit: N. Kaib
Astronomers find an unusual new denizen of the solar system. Provided by the Sloan Digital Sky Survey
A "minor planet" with the prosaic name 2006 SQ372 is just over 2 billion miles from Earth, a bit closer than the planet Neptune. But this lump of ice and rock is beginning the return leg of a 22,500-year journey that will take it to a distance of 150 billion miles, nearly 1,600 times the distance from the Earth to the Sun, according to a team of researchers from the Sloan Digital Sky Survey (SDSS-II).
The discovery of this remarkable object was reported August 18 in Chicago, at an international symposium titled "The Sloan Digital Sky Survey: Asteroids to Cosmology." A paper describing the discovery technique and the properties of 2006 SQ372 is being prepared for submission to the Astrophysical Journal.
The orbital paths of the major planets are nearly circular, but the orbit of 2006 SQ372 is an ellipse that is 4 times longer than it is wide, says University of Washington astronomer Andrew Becker, who led the discovery team. The only known object with a comparable orbit is Sedna — a distant, Pluto-like dwarf planet discovered in 2003 — but 2006 SQ372's orbit takes it more than 1.5 times further from the Sun, and its orbital period is nearly twice as long.
The new object is much smaller than Sedna, Becker says, probably 30-60 miles across instead of nearly 1,000. "It's basically a comet, but it never gets close enough to the Sun to develop a long, bright tail of evaporated gas and dust."
Becker's team found 2006 SQ372 by applying a specialized computer searching algorithm to data taken for a completely different purpose: finding supernovae explosions billions of light-years away to measure the expansion of the universe. The SDSS-II supernovae survey scanned the same long stripe of sky, an area 1,000 times larger than the Full Moon, every clear night in the fall of 2005, 2006, and 2007.
"If you can find things that explode, you can also find things that move, but you need different tools to look for them," says team member Lynne Jones, also of the University of Washington. The only objects close enough to change position noticeably from one night to the next are in our own solar system, Jones explains.
SQ372 was first discovered in a series of images taken between September 27 and October 21, 2006. Team member Andrew Puckett, of the University of Alaska Anchorage, then searched the supernovae survey's fall 2005 observations to find earlier detections, thus securing the discovery. Subsequent SDSS detections of SQ372 have been found in data from the 2006 and 2007 observing seasons.
University of Washington graduate student Nathan Kaib, another member of the discovery team, has been running computer simulations to try to understand out how 2006 SQ372 might have acquired its unusual orbit. "It could have formed, like Pluto, in the belt of icy debris beyond Neptune, then been kicked to large distance by a gravitational encounter with Neptune or Uranus," says Kaib. "However, we think it is more probable that SQ372 comes from the inner edge of the Oort Cloud."
In 1950, Kaib explains, the Dutch astronomer Jan Oort hypothesized that most comets come from a distant reservoir of icy, asteroid-like bodies, which were ejected from the inner solar system by gravitational kicks from the giant planets as the planets themselves were forming 4.5 billion years ago. Most objects in the Oort Cloud orbit the Sun at distances of several trillion miles, but the gravity of passing stars can alter their orbits, flinging some into interstellar space and deflecting others to the inner solar system where they "light up" as comets.
Even at its most distant turning point, 2006 SQ372 will be 10 times closer to the Sun than the supposed main body of the Oort Cloud, says Kaib. "The existence of an 'inner' Oort Cloud has been theoretically predicted for many years, but SQ372 and perhaps Sedna are the first objects we have found that seem to originate there. It's exciting that we are beginning to verify these predictions."
Becker notes that 2006 SQ372 was bright enough to find with the SDSS only because it is near its closest approach to the Sun, and that the SDSS-II supernovae survey observed less than one percent of the sky. "There are bound to be many more objects like this waiting to be discovered by the next generation of surveys, which will search to fainter levels and cover more area," says Becker. "In a decade, we should know a lot more about this population than we do now."
"One of our goals," says Kaib, "is to understand the origin of comets, which are among the most spectacular celestial events. But the deeper goal is to look back into the early history of our solar system and piece together what was happening when the planets formed."
The discovery of this remarkable object was reported August 18 in Chicago, at an international symposium titled "The Sloan Digital Sky Survey: Asteroids to Cosmology." A paper describing the discovery technique and the properties of 2006 SQ372 is being prepared for submission to the Astrophysical Journal.
The orbital paths of the major planets are nearly circular, but the orbit of 2006 SQ372 is an ellipse that is 4 times longer than it is wide, says University of Washington astronomer Andrew Becker, who led the discovery team. The only known object with a comparable orbit is Sedna — a distant, Pluto-like dwarf planet discovered in 2003 — but 2006 SQ372's orbit takes it more than 1.5 times further from the Sun, and its orbital period is nearly twice as long.
The new object is much smaller than Sedna, Becker says, probably 30-60 miles across instead of nearly 1,000. "It's basically a comet, but it never gets close enough to the Sun to develop a long, bright tail of evaporated gas and dust."
Becker's team found 2006 SQ372 by applying a specialized computer searching algorithm to data taken for a completely different purpose: finding supernovae explosions billions of light-years away to measure the expansion of the universe. The SDSS-II supernovae survey scanned the same long stripe of sky, an area 1,000 times larger than the Full Moon, every clear night in the fall of 2005, 2006, and 2007.
"If you can find things that explode, you can also find things that move, but you need different tools to look for them," says team member Lynne Jones, also of the University of Washington. The only objects close enough to change position noticeably from one night to the next are in our own solar system, Jones explains.
SQ372 was first discovered in a series of images taken between September 27 and October 21, 2006. Team member Andrew Puckett, of the University of Alaska Anchorage, then searched the supernovae survey's fall 2005 observations to find earlier detections, thus securing the discovery. Subsequent SDSS detections of SQ372 have been found in data from the 2006 and 2007 observing seasons.
University of Washington graduate student Nathan Kaib, another member of the discovery team, has been running computer simulations to try to understand out how 2006 SQ372 might have acquired its unusual orbit. "It could have formed, like Pluto, in the belt of icy debris beyond Neptune, then been kicked to large distance by a gravitational encounter with Neptune or Uranus," says Kaib. "However, we think it is more probable that SQ372 comes from the inner edge of the Oort Cloud."
In 1950, Kaib explains, the Dutch astronomer Jan Oort hypothesized that most comets come from a distant reservoir of icy, asteroid-like bodies, which were ejected from the inner solar system by gravitational kicks from the giant planets as the planets themselves were forming 4.5 billion years ago. Most objects in the Oort Cloud orbit the Sun at distances of several trillion miles, but the gravity of passing stars can alter their orbits, flinging some into interstellar space and deflecting others to the inner solar system where they "light up" as comets.
Even at its most distant turning point, 2006 SQ372 will be 10 times closer to the Sun than the supposed main body of the Oort Cloud, says Kaib. "The existence of an 'inner' Oort Cloud has been theoretically predicted for many years, but SQ372 and perhaps Sedna are the first objects we have found that seem to originate there. It's exciting that we are beginning to verify these predictions."
Becker notes that 2006 SQ372 was bright enough to find with the SDSS only because it is near its closest approach to the Sun, and that the SDSS-II supernovae survey observed less than one percent of the sky. "There are bound to be many more objects like this waiting to be discovered by the next generation of surveys, which will search to fainter levels and cover more area," says Becker. "In a decade, we should know a lot more about this population than we do now."
"One of our goals," says Kaib, "is to understand the origin of comets, which are among the most spectacular celestial events. But the deeper goal is to look back into the early history of our solar system and piece together what was happening when the planets formed."
