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The applet was implemented using 2-body methods, and hence should not be used for determining accurate long-term trajectories (over several years or decades)
The applet was implemented using 2-body methods, and hence should not be used for determining accurate long-term trajectories (over several years or decades)
Originally posted by wWizard
But the question is this: Is the data really off by 3000 years? I highly doubt it.
Originally posted by wWizard
Oh wow. Is what you posted somewhat accurate?
Near perihelion, using an August 2011 epoch, Kazuo Kino#a shows C/2010 X1 to have a heliocentric orbital period of 600,000 years, though more perturbations will occur.