diogen,
I'm a little confused by your description of the problem.
Uranus is tipped over so that its rotational axis is almost in the plane of the ecliptic. It is not perpendicular to the ecliptic like the other planets. The plane of its equator is perpendicular to the plane of the Ecliptic.
The orbits of Uranus and its moon Miranda are defined for Celestia in its file Celestia/data/solarsys.ssc
If I'm interpreting your description correctly, your symptoms suggest that someone has edited that file. You should discuss the issue with whoever did those edits.
Official versions of solarsys.ssc are available at
http://celestia.cvs.sourceforge.net/cel ... c?view=log
For example, the orientation of Uranus is defined by the lines
Code: Select all
RotationPeriod 17.24 # System III (magnetic field)
Obliquity 97.81
EquatorAscendingNode 167.76
RotationOffset 331.18 # correct System III prime meridian
(these were taken from Celestia v1.4.1 final for Windows)
The Obliquity entry defines the tilt of the planet relative to the perpendicular to the Ecliptic. As you can see, Uranus should be tipped over so that its polar axis is slightly less than 8 degrees from the plane of the Ecliptic.
Here is what I see on my Windows system when viewing Uranus and Miranda with Celestia v1.4.1 final. It seems to be correct.