Astronomers Discover "10th Planet"
It is bigger than Pluto, the 9th planet.
The object, designated 2003 UB313, is currently 97 astronomical units (Earth-Sun distances) away more than twice Pluto's average distance from the Sun. This makes it the farthest object ever seen in the solar system. It is a scattered-disk object, meaning that at some point in its history, an encounter with some massive object moved it into its highly inclined (44°) orbit. It's currently glowing at magnitude 18.9 in the constellation Cetus. Its high inclination is the only reason it wasn't discovered years ago; no one was looking for planets so far from the plane of the solar system.
Discoverers Michael E. Brown (Caltech), Chad Trujillo (Gemini Observatory), and David Rabinowitz (Yale University) first imaged the object on October 21, 2003, but didn't see it move in the sky until they reimaged the same area 15 months later, on January 8, 2005. Working backward from there, the astronomers have found old images of 2003 UB313 in much earlier surveys, allowing them to determine its orbit accurately. The object turns out to be currently near aphelion (its farthest from the Sun) in a very elliptical orbit. It ranges as close as 38 a.u. to the Sun in a 557-year orbit.
"It's a big sucker!" says Brown.
Preliminary near-infrared spectra, obtained by team member Chad Trujillo at the 8-meter Gemini North telescope, show methane ice on the object's surface much like the spectrum of Pluto, which is also dominated by methane ice in the near infrared. Trujillo says in a Gemini press release, "It is clear that [2003 UB313] is very similar to Pluto in both size and composition, at least upon first glance." Pluto is about 30 percent reflective. Methane ice is unusual and suggests a primitive surface that has never been warmed much since the formation of the solar system. "To date," notes Trujillo, "no one has seen methane on any other Kuiper Belt object, only on Pluto and Neptune's moon Triton."
Early October: R.A. 1h 37.7m, dec. 5° 34'.
Late October: R.A. 1h 37.2m, dec. 5° 36'.
Early November: R.A. 1h 36.7m, dec. 5° 39'.
Late November: R.A. 1h 36.1m, dec. 5° 40'.
Early December: R.A. 1h 35.7m, dec. 5° 40'.
Late December: R.A. 1h 35.4m, dec. 5° 39'.
Early January: R.A. 1h 35.2m, dec. 5° 37'.
Late January: R.A. 1h 35.2m, dec. 5° 34'.
And a Second Big KBO
If that weren't enough, a second big Kuiper Belt discovery also made news the same day: 2003 EL61. A team of astronomers at the Sierra Nevada Observatory in Spain reported their discovery (details here) to the Minor Planet Center in Cambridge, Massachusetts. It had been spotted by Brown and his team more than a year ago, but, as Brown notes on his website for this object, "There is no question that the Spanish group is rightly credited with discovery. We could have announced the object earlier, but we took a chance that no one else would find it while we were awaiting our observations from the Spitzer Space Telescope. We were wrong!"
Located about 52 a.u. away and now situated in eastern Coma Berenices, 2003 EL61 is about 70 percent of Pluto's diameter.
Moreover, by a great stroke of luck, 2003 EL61 has a tiny satellite revolving around it, at an apparent distance of about 1.5 arcseconds. According to Brown's group, the satellite completes an orbit every 49 days in a nearly circular orbit some 49,500 km (30,760 miles) from the main body. The satellite's orbit has allowed the team to determine the parent object's mass: about a quarter that of Pluto.
Based on a quick look at the Spitzer observations of 2003 EL61, Brown believes that the infrared spectrum is dominated by water ice. "It looks much like [Pluto's moon] Charon," he notes.