NROL-24 observations by Richard Miles; payload elset

From: Ted Molczan (ssl2molcz@rogers.com)
Date: Tue Dec 11 2007 - 22:44:22 UTC

  • Next message: Peter Wakelin: "SATOBS 2007 December 11 (cont)"

    Richard Miles, who observes minor planets, imaged the payload of NROL-24 over a
    wide arc. He has kindly reduced his observations into the MPC reporting format:
    
    http://satobs.org/seesat_ref/misc/MPCReportA.txt
    
    For ease of use by our analysts, I have converted them to the U.K. format:
    
    http://satobs.org/seesat_ref/misc/Richard_Miles.txt
    
    http://www.satobs.org/position/UKformat.html
    
    Richards site coordinates are 50.9310 N, 2.4053 W, 72 m. For my internal use, I
    have assigned a site number of 9011, which appears in above U.K. format file.
    
    Combining Richard's and Peter Wakelin's observations yields the following
    elements for the payload, with excellent residuals:
    
    1 32378U 07060A   07344.98097734  .00000000  00000-0  00000-0 0    04
    2 32378  60.0096 318.1644 5542864 286.8880  21.5711  4.77472119    06
    Arc 2007 Dec 11.01 - 11.13, WRMS residuals = 0.009 deg	
    
    The orbit is 261 X 16775 km, inclined at 60 deg, with a period of 301.6 min.
    
    The objects from this launch have yet to appear in the public catalogue;
    however, the international designator can only be 07060A. I have speculatively
    assigned the next available catalogue number, 32378.
    
    As is often the case soon after a launch, we have yet to reach consensus as to
    which object is the payload and which is the rocket body. I agree with Daniel
    Deak that the payload is the object that appeared to be within the Centaur's
    propellant dump cloud, and the Centaur was the one that appeared well clear of
    it. In fact, neither object was within the cloud, but the payload happened to be
    in line with it and the observer.
    
    Richard reported his single Centaur and 47 payload points in agreement with this
    interpretation. Peter Wakelin's identifications are the reverse.
    
    Scott Campbell and Mike McCants have produced accurate elements for what I
    believe to be the Centaur (Mike labelled it as the payload), which differ from
    those of the payload mainly in the inclination and RAAN:
    
    1 99999U 000000   07344.98098874 0.00000172  00000-0  50000-4 0    08
    2 99999  60.7019 318.7838 5501400 285.6245  22.3875  4.77454958    05
    
    1 32378U 07060A   07344.98106975  .00000000  00000-0  00000+0 0    01
    2 32378  60.7184 318.7781 5536000 286.5100  21.8181  4.77400000    00
    
    It makes sense to me that the payload would have a nice round numbered
    inclination, i.e. 60.0 deg, and that the Centaur would end up in 60.7 deg, as a
    result of its CCAM (collision and contamination avoidance manoeuvre) and
    subsequent venting.
    
    If the payload behaves like that of NROL-1, then it will manoeuvre to a Molniya
    orbit within about one week of launch.
    
    The initial orbital plane is about 16 deg east of the 90028 / 04846A Molniya
    object that I and others expected NROL-24 to target for replacement. I am
    surprised to see such a wide planar separation, so perhaps the 90028 replacement
    theory needs to be reconsidered. Note that due to their different rates of
    precession, NROL-24 would overtake the plane of 90028 in about 41 days, but that
    seems a long time to wait in the intermediate orbit. Perhaps the plane will be
    shifted west as part of the manoeuvres to Molniya; I have not analysed this
    possibility.
    
    Ted Molczan
    
    -------------------------------------------------------------------------
    Subscribe/Unsubscribe info, Frequently Asked Questions, SeeSat-L archive:  
    http://www.satobs.org/seesat/seesatindex.html
    



    This archive was generated by hypermail 2b29 : Tue Dec 11 2007 - 22:45:06 UTC