More then three years of motion determination and control operations in INT
ERBALL Project gave several lessons:
simple trigonometric approximation of attitude motion allows to determine a
nd control s/c attitude even in situation when the actual inertia moments t
ensor is not known a priori;
in the cases when the angular momentum vector evolution in inertial space c
ould be predicted, than with the case of mentioned approximation the full s
et of attitude parameters can be determined based only on Sun sensors measu
rements;
solar radiation pressure can be used for spin stabilize s/c allowing to kee
p spin axis directed towards Sun with some oscillations;
spin stabilization around the inertia axis of the maximum inertia moment do
es not guarantee the stable motion in the case when the source of energy pu
mping (like a flexible boom) does exist. (C) 2000 Elsevier Science Ltd. All
rights reserved.