Astrometry in the Uranian system of satellites

Details Astrometry in the Uranian system of satellites Astrometry in the Uranian system of satellites

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1043..159b&link_type=abstract

EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP Conference Proceedings, Volume 1043, pp. 159-162 (2008).

Computer Science

Databases

Artificial Earth Satellites, Astronomical Observations, Astronomical And Space-Research Instrumentation, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Quasars, Celestial Mechanics, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc.

Scientific paper

The predicted occultation between the satellites Miranda(UV) and Oberon(UIV) was observed on July 30, 2007 using SpeX/IRTF system and CODAM-Paris Observatory facility. Data analysis reveals that the predicted magnitude drop for this phenomenon was overestimated and we establish an upper limit of 0m.05 for the phenomenon, perhaps due to a non-lambertian limb scattering. The astrometry obtained from this run reveals good agreement with the LA06 numerical model.

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