puck2017 May 24, 2013
--- In find_orb@yahoogroups.com, Bill Gray <pluto@...> wrote:
>
> Hi Glen,
>
> > As I understand it, the authors of that paper used NOVAS to calculate
> > the orbit. Couldn't they just as well have used Find_Orb?
>
> Yes. Very shortly after the impact, I got an inquiry about this
> from someone hoping the object might be found on recent survey images.
> That resulted in my posting this pseudo-MPEC, with a (G96)-centric
> ephemeris to see if any of the southwestern US folks might have
> gotten the object on the way in :
>
> http://www.projectpluto.com/temp/chelyab.htm
>
> You'll notice that this was computed on the day of the impact, and
> was intended just to get a rough idea (enough to say, "Sorry, no,
> there aren't going to be any precovery images.") I'm sure Esko
> Lyytinen and/or Rob Matson and/or somebody else got more and better
> data after that. But even the very approximate data were enough to
> make it clear: this object came from too low an elongation to be
> spotted on its way in.
>
> I will not be surprised if it's a long time before another case
> occurs of an impactor observed before impact. It _has_ happened
> once (2008 TC3), and I keep an eye on NEOCP for objects that might
> do this. (The key sign is that the ephemerides show virtually no
> motion, then suddenly show _lots_ of motion. That was what clued
> me in for 2008 TC3.) But I'm not really optimistic.
>
> -- Bill
>