The system of Uranus has been observed in May 1999 by
means of the {\sc adonis}/SHARPII+ Adaptive Optics system implemented on
the 3.6~m telescope of La Silla-ESO (Chile). The use of the Shack-Hartmann
wavefront sensor on the planet itself and the excellent seeing conditions
have permitted to reach an angular resolution of ~0.14'' in the H broad
band (1.6\mum). The sharpness of the images has been subsequently restored
using a new myopic deconvolution method (MAP) including a specific edge
preserving object prior.\\ The images have revealed the presence of a latitudinal
structure of the atmospheric clouds on the planetary disk (J and H bands),
the presence of the Epsilon ring and its longitudinal anomaly.The most
internal rings (Delta, Gamma, Eta) are also visible after deconvolution.
Three of the known satellites has been detected: Ariel, Miranda and Puck
(discovered by Voyager in 1989). We detect a significant shift of Puck's
position with respect to the expected position, derived from the NASA/JPL
Ephemeris Generator. We also present photometry of the 3 satellites and
of the ring Epsilon using the J, H, K filters.


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Satellites detected:
Miranda, Puck, Bianca (South).
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Satellites detected
Miranda, Puck, Bianca, Rosalind and Portia (?) |
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Satellites detected:
Miranda, Puck and Portia |
© fmarchis@astron.berkeley.edu - Last modified: Fri Aug 27 21:43:01 CST 1999
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