USA 129 search elements

From: Ted Molczan (molczan@rogers.com)
Date: Sat Jan 04 2003 - 14:40:20 EST

  • Next message: Leo Barhorst: "Obs Jan 4"

    The 2.3 min late arrival on 2003 Jan 04 at 12:51 UTC reported by Tony Beresford was unexpected, but plausible.
    
    I found no other candidate objects in the vicinity of the observation.
    
    If the object were to manoeuvre to an orbit more like those of the two eastern plane objects, then it would have to manoeuvre at
    perigee to lower its apogee, and manoeuvre at apogee to raise its perigee. If its apogee was lowered first, then, that would have
    caused the object to arrive earlier, until its perigee was raised.
    
    There are too many possible combinations of apogee-lowering and perigee-raising times to evaluate, so I have instead created several
    search orbits, that fit Tony's single point.
    
    The first assumes that only the apogee had been lowered:
    
    1 70016U          03004.53525230  .00029109  00000-0  30000-3 0    06
    2 70016  97.9000  69.8000 0411000 182.6069 137.3000 15.02500000    09
    
    The others assume that both manoeuvres had been performed, and differ only in the mean motion and apogee height:
    
    1 70017U          03004.53525231  .00005389  00000-0  30000-3 0    02
    2 70017  97.9000  69.8000 0313000 182.6069 138.0000 14.81000000    00
    
    1 70018U          03004.53525232  .00005389  00000-0  30000-3 0    04
    2 70018  97.9000  69.8000 0324000 182.6069 137.9000 14.78500000    02
    
    Of course, it would be wise to look for the object in the original orbit, just in case there was a problem with Tony's observation
    (I doubt it, but most of us have been fooled from time to time):
    
    1 24680U 96072A   03003.53256872  .00029166  00000-0  33101-3 0    06
    2 24680  97.8541  69.0038 0493681 185.8948 173.6324 14.83264394    06
    
    Plotting all of the above should help to bracket the search. The object is unlikely to be much earlier than the 70016 orbit, and not
    much later than the 70018 orbit. On high elevation passes, the tracks will be far apart.
    
    Ted Molczan
    
    
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