I concur: I've seen several recent evening passes of SL-16 Rocket (25861, Okean-O r). In each case the sat was mag 1 before culmination and dimmed to the predicted magnitude soon afterwards. I suspect that the rotational period is now comparable to the duration of a pass, so no one observer can easily time the rotation. As I understand it, the rotational rate usually decays exponentially, i.e. the period increases exponentially with time. First-order decay. So the current period could be estimated using previous obs. Best, Mark ----------------------------------------------------------------- Unsubscribe from SeeSat-L by sending a message with 'unsubscribe' in the SUBJECT to SeeSat-L-request@lists.satellite.eu.org http://www2.satellite.eu.org/seesat/seesatindex.html
This archive was generated by hypermail 2b29 : Thu Jul 12 2001 - 14:06:07 PDT