"Pseudo-MPEC" for C0MJAL2

Created 2019 May 21 9:07:06 UT using Find_Orb

Click here for an explanation of pseudo-MPECs

 
 Astrometry: 
     C0MJAL2  C2019 05 14.22452 14 40 25.88 -19 38 17.7    ~5E7M 19.5 GVNEOCPG96
     C0MJAL2  C2019 05 14.23014 14 40 22.34 -19 37 08.7    ~5E7M 19.8 GVNEOCPG96
     C0MJAL2  C2019 05 14.23577 14 40 18.77 -19 35 59.0    ~5E7M 20.2 GVNEOCPG96
     C0MJAL2  C2019 05 14.24139 14 40 15.13 -19 34 49.2    ~5E7M 20.1 GVNEOCPG96
     C0MJAL2  C2019 05 14.30083014 39 35.14 -19 22 21.6    ~5E87 19.6 GVNEOCPH01
     C0MJAL2  C2019 05 14.30440714 39 32.81 -19 21 35.2    ~5E87 19.7 GVNEOCPH01
     C0MJAL2  C2019 05 14.31643314 39 24.98 -19 18 57.6    ~5E87 20.0 GVNEOCPH01
     C0MJAL2  C2019 05 14.32210414 39 21.30 -19 17 43.0    ~5E87 19.7 GVNEOCPH01
     C0MJAL2  C2019 05 14.38474 14 38 41.85 -19 03 37.7    ~5E9q 21.0 GVNEOCPI52
     C0MJAL2  C2019 05 14.38547 14 38 41.41 -19 03 27.4    ~5E9q 20.8 GVNEOCPI52
     C0MJAL2  C2019 05 14.38620 14 38 40.91 -19 03 17.0    ~5E9q 19.9 GVNEOCPI52
     C0MJAL2  C2019 05 14.38693 14 38 40.46 -19 03 07.1    ~5E9q 20.0 GVNEOCPI52
     C0MJAL2 |C2019 05 15Vv+I9'_Qb_K;@Oluwyo$?QRgB*i7J2GFrK_S0k;pp0jF#fCV[GO2807
     C0MJAL2 |C2019 05 15?(Tb2wS]c]5Kwh\h*R^nB*Kb'[CAstrometry)10H9d%o=2rHCw6807
     C0MJAL2 |C2019 05 15%?t1Wi.bnpCPnL;XO.vm3Ee*W]*%Z[:T6K1Y3M(^qXRwMd[`tH+9807
     C0MJAL2 |C2019 05 15Rv6B0K8J%Nv7bcdjG5S3O=9d#gfb?%V/!A[9k:AAQ)+pM,+O`rX#807
     C0MJAL2 |C2019 05 15fB[-/w4(redacted;VDkWep1AlRru7BID(R*1-f-Btp@bxv`DTJ$807
     C0MJAL2 KC2019 05 16kkJCF5`IYh!click=Cf$ctG7jASC=:gKtk*e]Tb!Tw;#0^YM'E,DH21
     C0MJAL2 KC2019 05 16sS\t5ak)(=#MGB0U+e0\[gG?FtFD?3]axSEZp#.qErL*^6As$h8JH21
     C0MJAL2 KC2019 05 16lpw6j0q'rheregKf:uiHforFiurM3/n,36D7SjbPR:w3f9k+.ft0H21
     C0MJAL2 KC2019 05 162=+_kH9J5PHexplanationL]8hgs@[JTHiG9t/ZH@FfK+1D-$HBTH21

Station data:
(807) Cerro Tololo Observatory, La Serena  (S30.169136 W70.805900)  Chile.
(G96) Mt. Lemmon Survey  (N32.442754 W110.788720)  US/Arizona.  Observers T.
   A. Pruyne, 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. 1.5-m reflector +
   10K CCD.
(H01) Magdalena Ridge Observatory, Socorro  (N33.984833 W107.189333)  US/New
   Mexico.  Observers W. H. Ryan, E. V. Ryan. Measurer W. H. Ryan. 2.4-m
   f/8.9 reflector + CCD.
(H21) Astronomical Research Observatory, Westfield  (N39.483057 W87.968270)
   US/Illinois. 0.76-m f/3.0 astrograph + CCD.
(I52) Steward Observatory, Mt. Lemmon Station  (N32.442547 W110.788920)
   US/Arizona.  Observers T. A. Pruyne, 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. 1.0-m reflector + CCD.

Orbital elements:  C0MJAL2
   Perihelion 2019 Aug 1.043278 +/- 0.0138 TT =  1:02:19 (JD 2458696.543278)
Epoch 2019 May 16.0 TT = JDT 2458619.5   Earth MOID: 0.0051   AutoNEOCP
M 289.56961932 +/- 0.020            (J2000 ecliptic)
n   0.91416646 +/- 0.000105         Peri.   98.53382 +/- 0.0024
a   1.05144330 +/- 8.03e-5          Node   233.68737 +/- 0.00016
e   0.2381965 +/- 0.000173          Incl.    4.57355 +/- 0.0036
P   1.08/393.79d           H 27.8   G  0.15   U  6.6  
q 0.80099311 +/- 0.000121    Q 1.30189349 +/- 0.000281
From 21 observations 2019 May 14-16 (46.9 hr); mean residual 0".25
Residuals in arcseconds: 
190514 G96  .63-  .28-    190514 H01  .30+  .21+    190515 807  .08+  .13+    
190514 G96  .24-  .21-    190514 I52  .05-  .63-    190515 807  .12+  .10+    
190514 G96  .04+  .15+    190514 I52  .35+  .34-    190515 807  .06+  .13+    
190514 G96  .56-  .44+    190514 I52  .12-  .04+    190516 H21  .21+  .04-    
190514 H01  .11+  .08+    190514 I52  .12+  .09-    190516 H21  .06+  .13-    
190514 H01  .12+  .05-    190515 807  .17+  .19+    190516 H21  .07-  .06+    
190514 H01  .16+  .25+    190515 807  .33+  .14+    190516 H21  .49-  .07-    

Ephemerides (geocentric):
Date (UTC) HH   RA              Dec         delta   r     elong  mag " sig PA
---- -- -- --  -------------   -----------  ------ ------ -----  --- ---- ---
2019 05 21 09  06 16 11.384   +60 28 19.80  .01321 1.0032  47.8 24?? 32.8  67
2019 05 21 10  06 12 43.667   +60 17 25.73  .01336 1.0030  47.4 24?? 32.6  66
2019 05 21 11  06 09 22.806   +60 06 26.68  .01351 1.0029  46.9 24?? 32.3  65
2019 05 21 12  06 06 08.548   +59 55 23.89  .01366 1.0027  46.5 24?? 32.1  65
2019 05 21 13  06 03 00.647   +59 44 18.46  .01381 1.0025  46.0 24?? 31.9  64
2019 05 21 14  05 59 58.862   +59 33 11.39  .01396 1.0023  45.6 24?? 31.6  63
2019 05 21 15  05 57 02.959   +59 22 03.60  .01412 1.0022  45.2 24?? 31.4  63
2019 05 21 16  05 54 12.713   +59 10 55.93  .01427 1.0020  44.8 24?? 31.2  62
2019 05 21 17  05 51 27.904   +58 59 49.12  .01443 1.0018  44.4 24?? 31.0  62
2019 05 21 18  05 48 48.321   +58 48 43.86  .01458 1.0017  44.0 24?? 30.8  61
2019 05 21 19  05 46 13.760   +58 37 40.77  .01474 1.0015  43.6 25?? 30.6  60
2019 05 21 20  05 43 44.026   +58 26 40.39  .01490 1.0013  43.3 25?? 30.4  60
2019 05 21 21  05 41 18.928   +58 15 43.22  .01505 1.0011  42.9 25?? 30.2  59
2019 05 21 22  05 38 58.286   +58 04 49.72  .01521 1.0010  42.5 25?? 30.0  59
2019 05 21 23  05 36 41.926   +57 54 00.26  .01537 1.0008  42.2 25?? 29.8  58
2019 05 22 00  05 34 29.681   +57 43 15.22  .01553 1.0006  41.8 25?? 29.6  58
2019 05 22 01  05 32 21.391   +57 32 34.90  .01569 1.0005  41.5 25?? 29.4  57
2019 05 22 02  05 30 16.901   +57 21 59.57  .01585 1.0003  41.2 25?? 29.2  57
2019 05 22 03  05 28 16.066   +57 11 29.49  .01601 1.0001  40.9 25?? 29.0  57
2019 05 22 04  05 26 18.744   +57 01 04.86  .01617 0.9999  40.5 25?? 28.8  56
2019 05 22 05  05 24 24.801   +56 50 45.87  .01634 0.9998  40.2 25?? 28.7  56
2019 05 22 06  05 22 34.108   +56 40 32.68  .01650 0.9996  39.9 25?? 28.5  55
2019 05 22 07  05 20 46.542   +56 30 25.42  .01666 0.9994  39.6 25?? 28.3  55
2019 05 22 08  05 19 01.984   +56 20 24.20  .01683 0.9993  39.3 25?? 28.1  55
2019 05 22 09  05 17 20.322   +56 10 29.13  .01699 0.9991  39.1 25?? 28.0  54
2019 05 22 10  05 15 41.447   +56 00 40.28  .01715 0.9989  38.8 25?? 27.8  54
2019 05 22 11  05 14 05.258   +55 50 57.71  .01732 0.9987  38.5 26?? 27.6  54
2019 05 22 12  05 12 31.654   +55 41 21.46  .01748 0.9986  38.2 26?? 27.5  53
2019 05 22 13  05 11 00.541   +55 31 51.57  .01765 0.9984  38.0 26?? 27.3  53
2019 05 22 14  05 09 31.829   +55 22 28.07  .01782 0.9982  37.7 26?? 27.2  53
2019 05 22 15  05 08 05.432   +55 13 10.96  .01798 0.9981  37.5 26?? 27.0  52
2019 05 22 16  05 06 41.266   +55 04 00.23  .01815 0.9979  37.2 26?? 26.9  52
2019 05 22 17  05 05 19.252   +54 54 55.89  .01832 0.9977  37.0 26?? 26.7  52
2019 05 22 18  05 03 59.315   +54 45 57.92  .01848 0.9975  36.7 26?? 26.6  51
2019 05 22 19  05 02 41.382   +54 37 06.30  .01865 0.9974  36.5 26?? 26.4  51
2019 05 22 20  05 01 25.384   +54 28 20.98  .01882 0.9972  36.3 26?? 26.3  51
2019 05 22 21  05 00 11.253   +54 19 41.95  .01899 0.9970  36.0 26?? 26.1  51
2019 05 22 22  04 58 58.926   +54 11 09.16  .01916 0.9969  35.8 26?? 26.0  50
2019 05 22 23  04 57 48.342   +54 02 42.55  .01932 0.9967  35.6 26?? 25.9  50
2019 05 23 00  04 56 39.443   +53 54 22.09  .01949 0.9965  35.4 26?? 25.7  50
2019 05 23 01  04 55 32.172   +53 46 07.72  .01966 0.9963  35.2 26?? 25.6  50
2019 05 23 02  04 54 26.475   +53 37 59.39  .01983 0.9962  35.0 26?? 25.5  49
2019 05 23 03  04 53 22.301   +53 29 57.03  .02000 0.9960  34.7 26?? 25.3  49
2019 05 23 04  04 52 19.600   +53 22 00.58  .02017 0.9958  34.5 26?? 25.2  49
2019 05 23 05  04 51 18.325   +53 14 09.98  .02034 0.9957  34.4 26?? 25.1  49
2019 05 23 06  04 50 18.430   +53 06 25.17  .02051 0.9955  34.2 27?? 25.0  49
2019 05 23 07  04 49 19.872   +52 58 46.08  .02069 0.9953  34.0 27?? 24.9  48
2019 05 23 08  04 48 22.607   +52 51 12.63  .02086 0.9951  33.8 27?? 24.7  48