Cham wrote:Vincent has replicated the rotation problem on his machine.
Did you tried the SSC (with reference frame) that I gave to you, with Jack's data for the Spitzer space telescope ?
I was able to replicate the problem by letting the year reach 6000 (not 4000 as in the original report.) That's the year at which the VSOP87 series expressing the motion of the Sun around the solar system barycenter is no longer used. Instead, the Sun remains fixed with respect to the SSB. With the Sun not moving, the reference frame described in spitzer.ssc is no longer valid. One of the axes of that frame is the velocity of Spitzer with respect to M51, a fixed object as far as Celestia is concerned. Spitzer isn't moving either--the SSB is considered fixed, the Sun is considered fixed with respect to the SSB after the year 6000, and the motion of Spitzer relative to the Sun is described by an xyz file valid over a limited time range some time around the present. Thus, the velocity vector of Spitzer is zero, and can't be used to define a reference frame. In short: Don't Do That. I could figure out something better to do with the Sun's motion outside the range for which VSOP87 is valid, but I don't know of any longer range predictions for this motion. If you just want to point Spitzer at M51, you don't need a velocity vector anyway; use a constant vector instead and the frame will be valid at any time.
--Chris