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Wednesday, February 23, 2022

2009 PZ21 - Cometary orgin?

 Clones generation


Clones Target

mean sd   mean sd
q 3.85914782817777 2.37290442662423e-07   3.85914783140272 2.3537e-07
e 0.0801406801559403 6.09227507904535e-08   0.0801406839559804 6.2114e-08
i 17.137419366797 6.36351406517114e-06   17.137419930196 6.2706e-06
peri 320.523142499568 5.99473078348146e-05   320.523140865999 5.9474e-05
node 307.443365230246 2.42363482614464e-05   307.443369025924 2.384e-05
tp 2460899.33667196 0.000556445464595854   2460899.33668632 0.0005656

100 clones were generated to match the nominal orbital parameters (and uncertainty) of asteroid 2009 PZ21 (orbit condition code 0 - last observed in Feb 2022).

 

Backward simulation

Mercury 6 parameters:

)O+_06 Integration parameters  (WARNING: Do not delete this line!!)
) Lines beginning with `)' are ignored.
)---------------------------------------------------------------------
) Important integration parameters:
)---------------------------------------------------------------------
 algorithm (MVS, BS, BS2, RADAU, HYBRID etc) = BS
 start time (days)= 2459600.5
 stop time (days) = -1d8
 output interval (days) = 100
 timestep (days) = 0.05
 accuracy parameter=1.d-12 
...
 ejection distance (AU)= 100
 

Simulation results


 

  • 82 out of 100 clones arrived into the solar system from a distance greater than 100 AU, most of them about 54000 years ago (below they are flagged as being on a 'comet-like orbit')
  • the remaining 18 out of 100 asteroids are flagged as being on an 'asteroid-like' orbit

Plots

In the following plots, the simulation time has been divided into 50 slots and the relevant orbital inter-quartile distribution of the contributing clones is shown:









Best wishes,

Alessandro Odasso


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