these were my olds elements made at the time the orbits were
not "split".

I have changed the file with the new elements from JPL, and now that
enough observations have been made the orbits are different.

elements from JPL and S.Yoshida for fragments R and S that have not
been observed enough yet to have their own orbit.

magnitudes parameters are from S.Yoshida for fragments B to L and the
other fragments are from current observation assuming the same slope
parameter.

sincerely

Nicolas Lefaudeux

--- In guide-user@yahoogroups.com, "Ireneusz Wlodarczyk"
<astrobit@...> wrote:

>
> Hi Bill,
> Between 3K and 3S there are only differences in magnitudo.
> --Irek
> 553 Chorzow
>
>
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