[Iaude] MPEC S175: 2019 SO7 [a=2.78,e=0.62,i=8.3,H=23.1]

mpec at marsden.cfa.harvard.edu mpec at marsden.cfa.harvard.edu
Mon Sep 30 09:35:38 EDT 2019


M.P.E.C. 2019-S175                           Issued 2019 September 30, 13:34 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 at CFA.HARVARD.EDU
            URL https://www.minorplanetcenter.net/    ISSN 1523-6714

                                    2019 SO7                                    


Observations:
     K19S07O* C2019 09 28.35465 02 50 18.78 +25 51 51.3          21.3 GVES175G96
     K19S07O  C2019 09 28.35979 02 50 21.04 +25 51 50.2          21.4 GVES175G96
     K19S07O  C2019 09 28.36492 02 50 23.28 +25 51 48.5          21.3 GVES175G96
     K19S07O  C2019 09 28.37006 02 50 25.53 +25 51 47.1          21.1 GVES175G96
     K19S07O  C2019 09 28.38629202 50 32.46 +25 51 41.5          21.4 GVES175H01
     K19S07O  C2019 09 28.38991902 50 34.05 +25 51 40.3          21.2 GVES175H01
     K19S07O  C2019 09 28.40077702 50 38.80 +25 51 37.3          21.6 GVES175H01
     K19S07O  C2019 09 28.40789002 50 41.93 +25 51 35.0          20.7 GVES175H01
     K19S07O  C2019 09 28.49226 02 51 19.14 +25 51 08.1          21.3 GVES175G96
     K19S07O  C2019 09 28.49336 02 51 19.63 +25 51 08.0          21.3 GVES175G96
     K19S07O  C2019 09 28.49446 02 51 20.13 +25 51 07.3          21.5 GVES175G96
     K19S07O  C2019 09 28.49556 02 51 20.61 +25 51 06.9          21.1 GVES175G96
     K19S07O pC2019 09 29.10314702 56 01.12 +25 47 23.3          21.2 GVES175L01
     K19S07O KC2019 09 29.10409102 56 01.56 +25 47 22.7          21.0 GVES175L01
     K19S07O KC2019 09 29.10905902 56 03.78 +25 47 19.7          20.8 GVES175L01
     K19S07O  C2019 09 29.26182902 57 17.70 +25 46 20.9          21.5 GVES175H01
     K19S07O  C2019 09 29.28550702 57 28.52 +25 46 12.5          21.5 GVES175H01
     K19S07O  C2019 09 29.29399702 57 32.38 +25 46 09.5          21.0 GVES175H01
     K19S07O  C2019 09 29.29833402 57 34.35 +25 46 07.8          21.1 GVES175H01
     K19S07O  C2019 09 30.31742 03 05 39.49 +25 37 36.7          20.9 GVES175V06
     K19S07O  C2019 09 30.31900 03 05 40.25 +25 37 35.6          21.2 GVES175V06
     K19S07O  C2019 09 30.32058 03 05 40.97 +25 37 34.9          21.2 GVES175V06
     K19S07O  C2019 09 30.32217 03 05 41.73 +25 37 33.7          21.0 GVES175V06
     K19S07O KC2019 09 30.35341503 05 55.36 +25 37 13.4          21.6 VuES175H21
     K19S07O KC2019 09 30.36213803 05 59.41 +25 37 08.5          21.6 VuES175H21
     K19S07O KC2019 09 30.36999203 06 03.11 +25 37 02.8          21.3 VuES175H21

Observer details:
G96 Mt. Lemmon Survey.  Observer G. J. Leonard.  Measurers B. M. Africano, E. 
   J. Christensen, G. A. Farneth, D. C. Fuls, A. R. Gibbs, A. D. Grauer, H. 
   Groeller, R. A. Kowalski, S. M. Larson, G. J. Leonard, T. A. Pruyne, D. 
   Rankin, R. L. Seaman, F. C. Shelly.  1.5-m reflector + 10K CCD.
H01 Magdalena Ridge Observatory, Socorro.  Observers W. H. Ryan, E. V. Ryan.  
    Measurer W. H. Ryan.  2.4-m f/8.9 Ritchey-Chretien + 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.
L01 Visnjan Observatory, Tican.  Observers K. Korlevic, F. Valentine.  Measurer 
   K. Korlevic.  1.0-m f/2.9 reflector + CCD.
V06 Catalina Sky Survey-Kuiper.  Observer H. Groeller.  Measurers B. M. 
   Africano, E. J. Christensen, G. A. Farneth, D. C. Fuls, A. R. Gibbs, A. D. 
   Grauer, H. Groeller, R. A. Kowalski, S. M. Larson, G. J. Leonard, T. A. 
   Pruyne, D. Rankin, R. L. Seaman, F. C. Shelly.  1.55-m reflector + CCD.

Orbital elements:
2019 SO7                                                 Earth MOID = 0.0828 AU
Epoch 2019 Apr. 27.0 TT = JDT 2458600.5                 Veres
M 319.17750              (2000.0)            P               Q
n   0.21234767     Peri.  209.72032     +0.60800617     -0.79192735
a   2.7825163      Node   202.98051     +0.75393225     +0.59817486
e   0.6216442      Incl.    8.30422     +0.24882657     +0.12262919
P   4.64           H   23.1           G   0.15           U   8
Residuals in seconds of arc
190928 G96  0.1-  0.1+    190928 G96  0.1+  0.3+    190929 H01  0.1+  0.1-
190928 G96  0.0   0.3+    190928 G96  0.3+  0.0     190930 V06  0.2-  0.1+
190928 G96  0.0   0.0     190928 G96  0.2+  0.0     190930 V06  0.1+  0.1-
190928 G96  0.0   0.0     190929 L01  0.3-  0.2+    190930 V06  0.2-  0.0
190928 H01  0.1-  0.0     190929 L01  0.1-  0.0     190930 V06  0.0   0.4-
190928 H01  0.1-  0.2-    190929 L01  0.4-  0.9-    190930 H21  0.4+  0.4+
190928 H01  0.1-  0.1+    190929 H01  0.0   0.1-    190930 H21  0.1-  0.6+
190928 H01  0.1+  0.0     190929 H01  0.2+  0.1-    190930 H21  0.1+  0.4-
190928 G96  0.0   0.0     190929 H01  0.2+  0.0

Ephemeris:
2019 SO7                 a,e,i = 2.78, 0.62, 8                   q = 1.0528
Date    TT    R. A. (2000) Decl.     Delta      r    Elong.  Phase     V
2019 08 31    00 40 13.9 +21 04 23   0.4200  1.3479   137.1    30.7    23.2
...
2019 09 15    01 31 26.0 +24 39 28   0.2934  1.2428   139.2    31.9    22.3
...
2019 09 23    02 13 35.1 +25 50 24   0.2396  1.1930   138.2    34.1    21.8
...
2019 09 29    02 55 13.4 +25 48 18   0.2070  1.1593   135.7    37.1    21.5
2019 09 30    03 03 04.7 +25 40 41   0.2024  1.1540   135.1    37.8    21.5
2019 10 01    03 11 11.4 +25 30 32   0.1979  1.1488   134.5    38.5    21.4
...
2019 10 07    04 04 33.8 +23 27 30   0.1767  1.1202   129.4    43.6    21.3
...
2019 10 15    05 21 24.8 +17 46 12   0.1642  1.0891   120.1    52.4    21.3
...
2019 10 30    07 17 35.5 +03 44 56   0.1854  1.0558   104.8    65.5    21.9

A. U. Tomatic                (C) Copyright 2019 MPC           M.P.E.C. 2019-S175




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