French et al. determined the orbits of the Uranian rings, the orientation of the pole of Uranus,
and the gravity harmonics of Uranus from Earth-based and Voyager ring occultations …

We present multiepoch imaging of the T5. 0+ T5. 5 binary 2MASS J15344984–2952274AB
obtained with the Keck laser guide star adaptive optics system. Combined with archival HST …

Context. There is a need in some research facilities for deriving ephemerides, controlling
observations, verifying various models of motion, and calculating the coordinates in space of …

RA Jacobson determined the orbits of the Uranian satellites, the masses of Uranus and its
satellites, and the orientation of the pole of Uranus from Earth-based astrometry, Earth …

This article presents revised orbital elements for the 10 small Uranian satellites discovered
by the Voyager 2 spacecraft. The elements have been determined from a fit to astrometric …

This paper presents 1155 accurate equatorial positions for the outer planets Uranus,
Neptune, and Pluto and 17 satellites of Jupiter–Neptune. Additional positions for Jupiter …

The η ring is one of the narrow rings of Uranus, consisting of a dense core that is 1–2 km
wide and a diffuse outer sheet spanning about 40 km. Its dense core lies just exterior to the …

An accurate technique has been developed for measuring planetocentric positions of
Jupiter's satellites from Wide Field/Planetary Camera images. Our method of finding the …

The ten small inner moons of Uranus, discovered in 1986, have so far only been studied
from space (Voyager 2, HST). The orbital elements derived from the observations indicate …

A knowledge base for natural satellites of planets is created. On the basis of observations,
new numerical models of motion are constructed for all 96 outer satellites of Jupiter, Saturn …