NOSS search elements revised

From: Ted Molczan (molczan@rogers.com)
Date: Tue Dec 02 2003 - 09:12:56 EST

  • Next message: Robert Holdsworth: "Article on decay of SNOE"

    Here are my revisions:
    
    Centaur         10.1  3.0  0.0  3.7 v
    1 71004U          03336.53841546  .00000000  00000-0  00000-0 0    06
    2 71004  63.4733 300.8682 0149592 188.4793 171.3703 13.43448178    02
    
    NOSS leader      0.0  0.0  0.0  4.9 v
    1 71001U          03336.53861882  .00000000  00000-0  00000-0 0    08
    2 71001  63.4247 301.5580 0135067 185.2161 174.7465 13.42002823    04
    
    NOSS trailer     0.0  0.0  0.0  4.9 v
    1 71002U          03336.53863180  .00000000  00000-0  00000-0 0    02
    2 71002  63.4241 301.5547 0135680 184.7387 175.2364 13.41930476    04
    
    The late (compared with the 2001 launch) final Centaur burn, should have little
    effect on the final elements of the NOSS leader and NOSS trailer, so I am
    reasonably confident in those.
    
    The late burn may have a more significant effect on the Centaur's final orbit. I
    would not be surprised if its inclination is somewhat different, and it could
    end up in a slightly lower orbit, or even a higher orbit - perhaps sufficient to
    cause it to trail the payloads.
    
    My strategy would be to start observing about 2 min ahead of the predicted time
    of the Centaur elset, but to be prepared for the possibility that the first
    objects I see are the payloads. The payloads can be expected to follow one
    another at several second intervals. There may be two or three payloads. I
    expect three, but time will tell.
    
    The Centaur usually is more than one magnitude brighter than the NOSS, but their
    range in magnitude is such that one of the payloads could outshine it on a given
    pass.
    
    Finally, I plan to plot both the Centaur and the payloads on my finder charts,
    because their planes will be sufficiently different to put them on different
    tracks.
    
    Happy hunting!
    Ted Molczan
    
    
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