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  • MPEC 2018-T33 : 2018 SK3

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    M.P.E.C. 2018-T33                                Issued 2018 Oct. 3, 01:27 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
    
                                       2018 SK3
    
    Observations:
         K18S03K* C2018 09 30.30310 23 54 34.84 +23 31 01.6          19.4 GVET033703
         K18S03K  C2018 09 30.30843 23 54 33.71 +23 31 10.0          20.0 GVET033703
         K18S03K  C2018 09 30.31371 23 54 32.50 +23 31 16.4          19.2 GVET033703
         K18S03K KC2018 09 30.99568723 52 05.11 +23 46 35.3          19.7 GVET033L01
         K18S03K KC2018 09 30.99800623 52 04.60 +23 46 38.4          19.8 GVET033L01
         K18S03K KC2018 10 01.00774623 52 02.41 +23 46 51.1          19.8 GVET033L01
         K18S03K KC2018 10 01.21652123 51 17.06 +23 51 33.9          20.2 VuET033H21
         K18S03K KC2018 10 01.21910923 51 16.47 +23 51 37.4          20.1 VuET033H21
         K18S03K KC2018 10 01.22195123 51 15.82 +23 51 41.1          19.9 VuET033H21
         K18S03K KC2018 10 02.16513223 47 46.85 +24 12 43.5          20.0 VuET033H21
         K18S03K KC2018 10 02.16966823 47 45.81 +24 12 49.6          20.0 VuET033H21
         K18S03K KC2018 10 02.17861123 47 43.76 +24 13 01.6          20.0 VuET033H21
         K18S03K KC2018 10 02.75639 23 45 33.51 +24 25 46.7                VET033118
         K18S03K KC2018 10 02.76075 23 45 32.44 +24 25 51.4                VET033118
         K18S03K KC2018 10 02.76462 23 45 31.60 +24 25 57.1                VET033118
         K18S03K KC2018 10 02.76849 23 45 30.68 +24 26 01.6                VET033118
         K18S03K KC2018 10 02.79955 23 45 23.64 +24 26 43.0          19.0 RrET033106
         K18S03K KC2018 10 02.80460 23 45 22.50 +24 26 50.2          19.9 RrET033106
         K18S03K KC2018 10 02.80965 23 45 21.25 +24 26 56.9          19.5 RrET033106
         K18S03K KC2018 10 02.83172 23 45 16.12 +24 27 26.8          19.1 RoET033K88
         K18S03K KC2018 10 02.83730 23 45 14.86 +24 27 34.7          18.7 RoET033K88
         K18S03K KC2018 10 02.84289 23 45 13.54 +24 27 41.6          19.2 RoET033K88
         K18S03K KC2018 10 03.01561323 44 33.48 +24 31 30.2          19.5 RqET033K63
         K18S03K KC2018 10 03.01869223 44 32.73 +24 31 34.2          19.7 RqET033K63
         K18S03K KC2018 10 03.02177123 44 32.01 +24 31 38.2          19.4 RqET033K63
    
    Observer details:
    106 Crni Vrh.  Observer S. Maticic.  0.6-m f/3.3 Deltagraph + CCD.
    118 Modra.  Observer S. Gajdos.  0.6-m f/5.5 reflector + CCD.
    703 Catalina Sky Survey.  Observer R. A. Kowalski.  Measurers B. M. Africano,
        E. J. Christensen, G. A. Farneth, D. C. Fuls, A. R. Gibbs, A. D. Grauer,
        H. Groeller, J. A. Johnson, R. A. Kowalski, S. M. Larson, G. J. Leonard,
        R. L. Seaman, F. C. Shelly.  0.68-m Schmidt + 10K CCD.
    H21 Astronomical Research Observatory, Westfield.  Observer R. Holmes.
        Measurers S. Foglia, L. Buzzi, T. Linder, R. Holmes.  0.61-m f/4.5
        astrograph + CCD, 0.76-m f/3.0 astrograph + CCD.
    K63 G. Pascoli Observatory, Castelvecchio Pascoli.  Observer R. Bacci.  0.41-m
        f/3.2 Newtonian reflector + CCD.
    K88 GINOP-KHK, Piszkesteto.  Observer A. Bodi.  Measurer K. Sarneczky.  0.60-m
        Schmidt + CCD.
    L01 Visnjan Observatory, Tican.  Observer K. Korlevic.  1.0-m f/2.9 reflector
        + CCD.
    
    Orbital elements:
    2018 SK3                                            PHA, Earth MOID = 0.0376 AU
    Epoch 2019 Apr. 27.0 TT = JDT 2458600.5                 MPC
    M  22.23766              (2000.0)            P               Q
    n   0.21583607     Peri.  123.62610     -0.48294272     -0.87375470
    a   2.7524538      Node   354.26123     +0.48125913     -0.20988594
    e   0.7199803      Incl.   35.18037     +0.73154356     -0.43874892
    P   4.57           H   18.7           G   0.15           U   9
    Residuals in seconds of arc
    180930 703  0.0   0.6-    181002 H21  0.2+  0.2-    181002 106  0.4-  0.5-
    180930 703  0.5+  0.6+    181002 H21  0.2+  0.2-    181002 K88  0.2+  0.2+
    180930 703  0.3-  0.2-    181002 H21  0.2+  0.1-    181002 K88  0.6+  0.6+
    180930 L01  0.1+  0.2+    181002 118  0.1+  1.0+    181002 K88  0.3+  0.1+
    180930 L01  0.2+  0.2+    181002 118  0.9-  0.2-    181003 K63  0.1+  0.1+
    181001 L01  0.3-  0.1-    181002 118  0.2-  0.3+    181003 K63  0.3-  0.1+
    181001 H21  0.0   0.1+    181002 118  0.6-  0.4-    181003 K63  0.4-  0.0
    181001 H21  0.2-  0.1+    181002 106  0.4+  0.8-
    181001 H21  0.4-  0.0     181002 106  0.8+  0.4-
    
    Ephemeris:
    2018 SK3                 a,e,i = 2.75, 0.72, 35                  q = 0.7707
    Date    TT    R. A. (2000) Decl.     Delta      r     Elong.  Phase     V
    2018 09 03    00 56 39.2 +13 49 57   1.0726  1.9637   141.2    18.8    21.3
    ...
    2018 09 18    00 31 00.4 +18 52 21   0.8533  1.8169   155.7    13.2    20.4
    ...
    2018 09 26    00 09 01.9 +21 52 58   0.7622  1.7363   159.2    11.9    20.0
    ...
    2018 10 02    23 48 23.8 +24 09 06   0.7078  1.6750   156.8    13.6    19.9
    2018 10 03    23 44 37.6 +24 31 13   0.7000  1.6647   156.0    14.2    19.8
    2018 10 04    23 40 46.0 +24 53 04   0.6925  1.6543   155.0    14.8    19.8
    ...
    2018 10 10    23 15 59.4 +26 56 02   0.6551  1.5919   147.8    19.5    19.8
    ...
    2018 10 18    22 40 13.7 +29 08 35   0.6244  1.5076   135.7    27.5    19.8
    ...
    2018 11 02    21 35 46.4 +31 24 12   0.6128  1.3472   112.0    43.1    20.0
    
    A. U. Tomatic                (C) Copyright 2018 MPC           M.P.E.C. 2018-T33
    

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