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  • MPEC 2013-T90 : 2013 TM127

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    M.P.E.C. 2013-T90                                Issued 2013 Oct. 12, 01:17 UT
    
         The Minor Planet Electronic Circulars contain information on unusual
             minor planets and routine data on comets.  They are published
       on behalf of Commission 20 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
    
                                      2013 TM127
    
    Observations:
         K13TC7M* C2013 10 11.21510 23 17 24.17 +13 06 37.4          18.9 VqET090703
         K13TC7M  C2013 10 11.22003 23 17 14.36 +13 06 32.3          19.6 VqET090703
         K13TC7M  C2013 10 11.22509 23 17 04.50 +13 06 25.4          18.9 VqET090703
         K13TC7M  C2013 10 11.23013 23 16 54.27 +13 06 19.7                qET090703
         K13TC7M  C2013 10 11.25536 23 16 04.09 +13 05 47.2          19.3 VqET090703
         K13TC7M  C2013 10 11.25579 23 16 03.25 +13 05 46.7          18.7 VqET090703
         K13TC7M  C2013 10 11.25624 23 16 02.28 +13 05 45.6          18.8 VqET090703
         K13TC7M  C2013 10 11.25668 23 16 01.41 +13 05 43.6          18.9 VqET090703
         K13TC7M KC2013 10 11.29309623 14 41.09 +13 03 42.6          19.1  rET090H21
         K13TC7M KC2013 10 11.29663823 14 34.01 +13 03 36.2          19.2  rET090H21
         K13TC7M KC2013 10 11.30016823 14 26.98 +13 03 30.8          18.9  rET090H21
         K13TC7M  C2013 10 11.35786 23 12 33.77 +13 03 00.5          20.0 VqET090703
         K13TC7M  C2013 10 11.35830 23 12 32.72 +13 02 59.1          19.4 VqET090703
         K13TC7M  C2013 10 11.35873 23 12 31.90 +13 02 58.3          19.5 VqET090703
         K13TC7M  C2013 10 11.35917 23 12 31.00 +13 02 58.1          19.3 VqET090703
         K13TC7M |C2013 10 11.37837 23 11 49.65 +13 02 09.3                cET090H06
         K13TC7M |C2013 10 11.37948 23 11 47.39 +13 02 07.7          19.2 VcET090H06
         K13TC7M  C2013 10 11.56406 23 05 35.33 +12 57 34.2          19.6 RoET090300
         K13TC7M  C2013 10 11.56736 23 05 27.38 +12 57 27.1          19.9 RoET090300
         K13TC7M  C2013 10 11.57066 23 05 19.33 +12 57 20.7          19.7 RoET090300
         K13TC7M  C2013 10 11.57562 23 05 07.28 +12 57 10.9          19.7 RoET090300
         K13TC7M 5C2013 10 11.60709 23 03 42.99 +13 04 34.3          19.1 RtET090E10
         K13TC7M 5C2013 10 11.60838 23 03 39.78 +13 04 30.9          19.1 RtET090E10
         K13TC7M KC2013 10 11.87084122 52 59.20 +12 44 22.5          19.1 VuET090I93
         K13TC7M KC2013 10 11.88678222 52 12.14 +12 43 37.9          19.2 VuET090I93
         K13TC7M KC2013 10 11.90103522 51 29.55 +12 42 55.8          19.1 VuET090I93
    
    Observer details:
    300 Bisei Spaceguard Center--BATTeRS.  Observers A. Asami, K. Nishiyama.
        1.0-m f/3.0 reflector + CCD.
    703 Catalina Sky Survey.  Observer R. E. Hill.  Measurers A. Boattini,
        E. J. Christensen, A. R. Gibbs, A. D. Grauer, R. E. Hill, J. A. Johnson,
        R. A. Kowalski, S. M. Larson, F. C. Shelly.  0.68-m Schmidt + CCD.
    E10 Siding Spring-Faulkes Telescope South.  Observer R. Miles.  2.0-m f/10.0
        Ritchey-Chretien + CCD.
    H06 iTelescope Observatory, Mayhill.  Observer H. Sato.  0.43-m f/6.8
        astrograph + CCD + f/4.5 focal reducer.
    H21 Astronomical Research Observatory, Westfield.  Observer R. Holmes.
        Measurers S. Foglia, L. Buzzi, H. Devore, A. Kostin, T. Linder,
        T. Lister. T.  0.61-m f/4.0 astrograph + CCD.
    I93 St Pardon de Conques.  Observer F. Losse.  0.40-m f/3.7 reflector + CCD.
    
    Orbital elements:
    2013 TM127                                               Earth MOID = 0.0035 AU
    Epoch 2013 Nov. 4.0 TT = JDT 2456600.5                  MPC
    M 336.12805              (2000.0)            P               Q
    n   0.68653684     Peri.  258.45190     -0.22335503     -0.97455459
    a   1.2726046      Node   204.47902     +0.91111029     -0.20185835
    e   0.4186275      Incl.    2.60946     +0.34639656     -0.09745029
    P   1.44           H   26.6           G   0.15           U   7
    Residuals in seconds of arc
    131011 703  0.6+  0.0     131011 H21  0.5+  0.3-    131011 300  0.5+  0.7-
    131011 703  0.9-  0.7+    131011 H21  0.9+  0.4+    131011 300  0.0   0.5-
    131011 703  1.0+  0.2-    131011 703  1.0+  0.4+    131011 300  0.4+  0.2-
    131011 703  2.6-  0.3+    131011 703  0.9-  0.2-    131011 E10  0.7+  0.1+
    131011 703  0.5+  0.7+    131011 703  0.2+  0.2-    131011 E10  0.1+  0.4-
    131011 703  0.9+  0.7+    131011 703  0.4+  0.4+    131011 I93  0.6-  0.2+
    131011 703  0.1-  0.3+    131011 H06  2.0-  1.3-    131011 I93  0.1+  0.5+
    131011 703  0.2+  1.1-    131011 H06  1.2-  0.7-    131011 I93  0.1+  0.1+
    131011 H21  0.6+  0.0     131011 300  0.3-  0.2-
    
    Ephemeris:
    2013 TM127               a,e,i = 1.27, 0.42, 3                   q = 0.7399
    Date    TT    R. A. (2000) Decl.     Delta      r     Elong.  Phase     V
    2013 09 12    00 40 20.1 +11 56 19   0.2299  1.2178   154.3    21.0    24.9
    ...
    2013 09 27    00 35 34.4 +12 56 36   0.1160  1.1158   167.4    11.3    22.9
    ...
    2013 10 05    00 21 05.8 +13 16 34   0.06070 1.0599   169.8     9.6    21.3
    ...
    2013 10 11    23 23 28.4 +13 12 35   0.02148 1.0178   154.2    25.2    19.5
    2013 10 12    22 46 42.5 +12 42 41   0.01549 1.0107   144.6    34.9    19.0
    2013 10 13    21 29 53.3 +10 39 20   0.01031 1.0037   125.0    54.5    18.7
    ...
    2013 10 19    13 43 36.8 -12 04 34   0.03402 0.9621     3.1   176.8
    ...
    2013 10 27    13 11 13.5 -12 43 21   0.08804 0.9084    13.2   165.6    34.6
    ...
    2013 11 11    13 07 48.7 -13 04 45   0.2008  0.8191    28.4   144.9    30.2
    
    A. U. Tomatic                (C) Copyright 2013 MPC           M.P.E.C. 2013-T90
    

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