We present the discovery and initial physical and dynamical characterization of the object 2003 UB313. The object is sufficiently bright that for all reasonable values of the albedo it is certain to be larger than Pluto. Prediscovery observations back to 1989 are used to obtain an orbit with extremely small errors. The object is currently at aphelion in what appears to be a typical orbit for a scattered Kuiper Belt object, except that it is inclined by about 44° from the ecliptic. The presence of such a large object at this extreme inclination suggests that high-inclination Kuiper Belt objects formed preferentially closer to the Sun. Observations from Gemini Observatory show that the infrared spectrum is, like that of Pluto and 2005 FY9, do...
The goal of the project was to identify a statistically significant sample of large (200 km-sized) K...
As a result of our continuing photometric survey, we report here optical colors for 36 Kuiper Belt o...
We present the first results of the Hubble Wide Field Camera 3 Test of Surfaces in the Outer Solar S...
We present the discovery and initial physical and dynamical characterization of the object 2003 UB31...
We have used the Hubble Space Telescope to directly measure the angular size of the large Kuiper Bel...
We present measurements at optical wavelengths of the spectral reflectance, rotational light curve, ...
We have searched the four brightest objects in the Kuiper Belt for the presence of satellites using ...
The original publication is available at http://iopscience.iop.org/1538-3881/International audienceW...
After flying past Pluto in 2015, the New Horizons spacecraft shifted course to encounter (486958) 20...
The newly commissioned laser guide star adaptive optics system at Keck Observatory has been used to ...
The Kuiper belt is a collection of small bodies (Kuiper belt objects, KBOs) that lie beyond the orbi...
We present the results of a pencil-beam survey of the Kuiper Belt using the Keck 10-m telescope. A s...
The Kuiper belt, the population of small icy planetesimals orbiting the Sun beyond Neptune, offers a...
The small bodies in the Solar System are thought to have been highly affected by collisions and eros...
The Kuiper belt is a remnant of the primordial Solar System. Measurements of its size distribution c...
The goal of the project was to identify a statistically significant sample of large (200 km-sized) K...
As a result of our continuing photometric survey, we report here optical colors for 36 Kuiper Belt o...
We present the first results of the Hubble Wide Field Camera 3 Test of Surfaces in the Outer Solar S...
We present the discovery and initial physical and dynamical characterization of the object 2003 UB31...
We have used the Hubble Space Telescope to directly measure the angular size of the large Kuiper Bel...
We present measurements at optical wavelengths of the spectral reflectance, rotational light curve, ...
We have searched the four brightest objects in the Kuiper Belt for the presence of satellites using ...
The original publication is available at http://iopscience.iop.org/1538-3881/International audienceW...
After flying past Pluto in 2015, the New Horizons spacecraft shifted course to encounter (486958) 20...
The newly commissioned laser guide star adaptive optics system at Keck Observatory has been used to ...
The Kuiper belt is a collection of small bodies (Kuiper belt objects, KBOs) that lie beyond the orbi...
We present the results of a pencil-beam survey of the Kuiper Belt using the Keck 10-m telescope. A s...
The Kuiper belt, the population of small icy planetesimals orbiting the Sun beyond Neptune, offers a...
The small bodies in the Solar System are thought to have been highly affected by collisions and eros...
The Kuiper belt is a remnant of the primordial Solar System. Measurements of its size distribution c...
The goal of the project was to identify a statistically significant sample of large (200 km-sized) K...
As a result of our continuing photometric survey, we report here optical colors for 36 Kuiper Belt o...
We present the first results of the Hubble Wide Field Camera 3 Test of Surfaces in the Outer Solar S...