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  • MPEC 2017-S192: 2017 SM16

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    M.P.E.C. 2017-S192                               Issued 2017 Sept. 27, 22:32 UT
    
         The Minor Planet Electronic Circulars contain information on unusual
             minor planets and routine data on comets.  They are published
        on behalf of Division F of the International Astronomical Union by the
              Minor Planet Center, Smithsonian Astrophysical Observatory,
                              Cambridge, MA 02138, U.S.A.
    
                 Prepared using the Tamkin Foundation Computer Network
    
                                  MPC@CFA.HARVARD.EDU
                URL https://www.minorplanetcenter.net/    ISSN 1523-6714
    
                                       2017 SM16
    
    Observations:
         K17S16M* C2017 09 24.35066 02 28 41.01 +18 39 07.3          20.9 VqES192G96
         K17S16M  C2017 09 24.35646 02 28 42.03 +18 39 09.4          21.0 VqES192G96
         K17S16M  C2017 09 24.36824 02 28 44.13 +18 39 12.2                qES192G96
         K17S16M  C2017 09 24.48766 02 29 05.34 +18 39 48.1                qES192I52
         K17S16M  C2017 09 24.49340 02 29 06.35 +18 39 50.7          21.0 VqES192I52
         K17S16M  C2017 09 24.49794 02 29 07.16 +18 39 51.7                qES192I52
         K17S16M KC2017 09 24.98273 02 30 38.70 +18 42 06.9          20.9 RvES192B18
         K17S16M KC2017 09 24.98491 02 30 39.07 +18 42 07.8          20.7 RvES192B18
         K17S16M KC2017 09 24.98600 02 30 39.28 +18 42 08.0          20.7 RvES192B18
         K17S16M KC2017 09 24.98708 02 30 39.45 +18 42 07.9          20.7 RvES192B18
         K17S16M KC2017 09 25.30417502 31 39.09 +18 43 36.9          21.0 VuES192H21
         K17S16M KC2017 09 25.31513402 31 41.08 +18 43 40.3          21.0 VuES192H21
         K17S16M KC2017 09 25.32697402 31 43.19 +18 43 43.6          21.1 VuES192H21
         K17S16M  C2017 09 25.38353 02 31 53.82 +18 44 01.7          20.5 VqES192I52
         K17S16M  C2017 09 25.38602 02 31 54.26 +18 44 02.4          21.5 VqES192I52
         K17S16M  C2017 09 25.38729 02 31 54.53 +18 44 02.0          20.6 VqES192I52
         K17S16M KC2017 09 26.32568202 34 49.33 +18 47 58.4          20.8 VuES192H21
         K17S16M KC2017 09 26.33361602 34 50.73 +18 48 00.2          20.8 VuES192H21
         K17S16M KC2017 09 26.34344402 34 52.49 +18 48 02.5          20.9 VuES192H21
         K17S16M  C2017 09 26.35649 02 34 55.43 +18 48 08.9          21.3 VqES192I52
         K17S16M  C2017 09 26.35859 02 34 55.79 +18 48 09.4          20.9 VqES192I52
         K17S16M  C2017 09 26.36069 02 34 56.16 +18 48 10.0          21.7 VqES192I52
         K17S16M  C2017 09 26.36276 02 34 56.53 +18 48 10.2          21.5 VqES192I52
         K17S16M  C2017 09 27.40719 02 38 09.84 +18 52 02.9          20.9 VqES192I52
         K17S16M  C2017 09 27.40928 02 38 10.17 +18 52 03.8          21.2 VqES192I52
         K17S16M  C2017 09 27.41228 02 38 10.66 +18 52 04.9          21.4 VqES192I52
    
    Observer details:
    B18 Terskol.  Observers A. Sergeev, M. Andreev, A. Bondar, V. Godunova.
        Measurer M. Andreev.
    G96 Mt. Lemmon Survey.  Observer A. R. Gibbs.  Measurers E. J. Christensen,
        D. C. Fuls, A. R. Gibbs, A. D. Grauer, J. A. Johnson, R. A. Kowalski,
        S. M. Larson, G. J. Leonard, R. G. Matheny, R. L. Seaman, F. C. Shelly.
        1.5-m reflector + 10K CCD.
    H21 Astronomical Research Observatory, Westfield.  Observer R. Holmes.
        Measurers S. Foglia, L. Buzzi, T. Linder, R. Holmes.  0.76-m f/3.0
        astrograph + CCD.
    I52 Steward Observatory, Mt. Lemmon Station.  Observers G. J. Leonard,
        D. C. Fuls.  Measurers E. J. Christensen, D. C. Fuls, A. R. Gibbs,
        A. D. Grauer, J. A. Johnson, R. A. Kowalski, S. M. Larson, G. J. Leonard,
        R. G. Matheny, R. L. Seaman, F. C. Shelly.  1.0-m reflector + CCD.
    
    Orbital elements:
    2017 SM16                                                Earth MOID = 0.2597 AU
    Epoch 2017 Sept. 4.0 TT = JDT 2458000.5                 MPC
    M 353.59136              (2000.0)            P               Q
    n   0.17018167     Peri.  177.89044     +0.89954215     -0.43601997
    a   3.2249837      Node   208.00796     +0.39995162     +0.84659772
    e   0.6106518      Incl.    3.25399     +0.17567762     +0.30521940
    P   5.79           H   21.7           G   0.15           U   8
    Residuals in seconds of arc
    170924 G96  0.2+  0.4-    170924 B18  0.5-  0.3-    170926 H21  0.2+  0.2-
    170924 G96  0.1+  0.1-    170925 H21  0.7-  0.3-    170926 I52  0.4+  0.2+
    170924 G96  0.2+  1.0-    170925 H21  0.1-  0.0     170926 I52  0.2+  0.1+
    170924 I52  0.2+  0.2+    170925 H21  0.0   0.1+    170926 I52  0.2+  0.2+
    170924 I52  0.0   1.3+    170925 I52  0.1-  0.2-    170926 I52  0.3+  0.1-
    170924 I52  0.0   1.0+    170925 I52  0.1-  0.2-    170927 I52  0.3+  0.4-
    170924 B18  0.1-  0.0     170925 I52  0.5+  0.9-    170927 I52  0.2-  0.1+
    170924 B18  0.4-  0.2+    170926 H21  0.1-  0.0     170927 I52  0.7-  0.6+
    170924 B18  0.2-  0.1+    170926 H21  0.1-  0.2-
    
    Ephemeris:
    2017 SM16                a,e,i = 3.22, 0.61, 3                   q = 1.2556
    Date    TT    R. A. (2000) Decl.     Delta      r     Elong.  Phase     V
    2017 08 28    01 06 29.2 +13 50 43   0.4525  1.3627   133.7    32.4    22.0
    ...
    2017 09 12    01 50 08.1 +17 01 33   0.3721  1.3046   137.3    31.5    21.5
    ...
    2017 09 20    02 15 02.4 +18 12 47   0.3412  1.2821   139.2    30.8    21.2
    ...
    2017 09 26    02 33 48.5 +18 46 48   0.3234  1.2696   140.7    30.0    21.1
    2017 09 27    02 36 54.3 +18 50 43   0.3209  1.2679   141.0    29.9    21.0
    2017 09 28    02 39 59.3 +18 54 07   0.3185  1.2663   141.3    29.7    21.0
    ...
    2017 10 04    02 58 01.1 +19 03 48   0.3066  1.2590   143.1    28.5    20.9
    ...
    2017 10 12    03 20 03.2 +18 49 37   0.2972  1.2556   146.1    26.3    20.8
    ...
    2017 10 27    03 51 27.5 +17 21 42   0.2987  1.2690   153.9    20.1    20.6
    
    A. U. Tomatic                (C) Copyright 2017 MPC           M.P.E.C. 2017-S192
    

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