Weekly Information about Bright Comets (2003 Jan. 25: South)

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Updated on January 25, 2003
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Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Southern Hemisphere.

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* C/2002 X5 ( Kudo-Fujikawa )


It only brightened to 6 mag, and became too close to the sun to observe. In the Southern Hemisphere, it will appear at dusk in mid February at 6 mag. In the Northern Hemisphere, in March at 7 mag. Then it will fade out slowly.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  20 18.32  -10 16.3   1.161   0.245     9    4.6    146.9 152.2   3:32 (302,-23)  
Feb.  1  20 58.43  -26 31.6   1.129   0.223     9    4.3    157.4 142.2  20:43 ( 46,-10)  

* C/2002 V1 ( NEAT )


It had been brightening extremely rapidly for about two months since discovery. But now it is brightening in normal pace. It is observable until early February in the Northern Hemisphere in the evening sky. It will approach to the sun down to 0.1 AU in February.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  23 26.37    8 41.8   0.912   0.835    52    5.8     51.9 258.0  20:51 ( 99, -2)  
Feb.  1  23  1.99    7 13.1   0.937   0.651    39    4.8     56.1 254.1  20:43 ( 92,-10)  

* C/2002 Y1 ( Juels-Holvorcem )


New comet. It is a widely diffused object. It will reach to 9 mag in March and April. In the Northern Hemisphere, it is observable until late April. In the Southern Hemisphere, it locates low in January, then it will not be observable for a while, and it becomes observable again after May.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  14 41.74   35 12.1   1.130   1.600    98   10.8     83.0  41.4   3:32 (215,  9)  
Feb.  1  15 19.81   43  5.1   1.008   1.499    97   10.3    101.9  44.3   3:42 (210,  3)  

* C/2001 RX14 ( LINEAR )


It will be observable in the good condition for a long time from winter to next spring. Strongly condensed and easy to see.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  12 12.01   44 41.2   1.308   2.059   127   10.6      4.4 196.4   3:32 (184, 10)  
Feb.  1  12  9.90   44  7.9   1.275   2.064   131   10.5      7.5 224.0   3:27 (180, 11)  

* 22P/Kopff


Not observable. It will appear at dawn in June at 15.5 mag, then it will be fading.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  20 41.87  -18 44.1   2.625   1.643     3   11.9     44.3  77.4  20:51 ( 53,-16)  
Feb.  1  21  2.88  -17 32.1   2.648   1.663     1   12.1     43.7  75.8  20:43 ( 54,-17)  

* 154P/2002 Q4 ( Brewington )


It brightened suddenly up to 12.5 mag visually and by photos in late December.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  23  7.92    2  5.7   2.158   1.615    44   12.2     42.4  58.6  20:51 ( 92, -1)  
Feb.  1  23 25.08    4 41.6   2.181   1.604    42   12.1     43.4  58.9  20:43 ( 94, -3)  

* C/2001 HT50 ( LINEAR-NEAT )


It will be observable in good condition at 11-12 mag in early 2003 and 2003 autumn.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   7 56.34   -3 10.4   2.329   3.255   156   12.3     44.3 282.8  23:36 (180, 58)  
Feb.  1   7 36.15   -1 56.3   2.314   3.220   152   12.2     44.4 284.7  22:49 (180, 57)  

* C/2002 Q5 ( LINEAR )


Before the perihelion passage, it brightened rapidly and reached to 13 mag. After appearing at dawn, it was bright at 12.5 mag and observed visually.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  15 45.01  -24 27.4   1.741   1.599    65   13.3     27.9 233.8   3:32 (275, 38)  
Feb.  1  15 31.58  -26 26.7   1.625   1.664    74   13.5     34.5 239.3   3:42 (271, 49)  

* 28P/Neujmin 1


It was much fainter than this ephemeris, 17.4 mag on July 31 by Akimasa Nakamura. No further observations were reported, so the current brightness is uncertain.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  22 24.90   -8 50.8   2.362   1.590    30   13.4     47.5  61.1  20:51 ( 77, -4)  
Feb.  1  22 44.32   -6  9.1   2.405   1.611    28   13.5     47.0  60.5  20:43 ( 79, -5)  

* 29P/Schwassmann-Wachmann 1


Not observable. It will be obervable again in April or May.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  21 27.81  -13 29.3   6.720   5.778    15   13.9     12.3  69.2  20:51 ( 64,-12)  
Feb.  1  21 33.34  -12 58.3   6.745   5.777     9   13.9     12.4  68.8  20:43 ( 62,-15)  

* 65P/Gunn


It is observable at 12.5 mag for long time from April to August in 2003.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  16 43.65  -20  4.9   3.009   2.533    52   14.0     25.9 102.0   3:32 (278, 24)  
Feb.  1  16 56.18  -20 40.8   2.927   2.522    56   14.0     25.4 101.2   3:42 (276, 29)  

* 30P/Reinmuth 1


It reached to 14 mag by CCD, a bit brighter than expected. It was also observed visually at around 13.5 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  11 29.57   10 40.2   1.067   1.898   135   14.0      9.4  47.9   3:14 (180, 44)  
Feb.  1  11 32.03   11 29.6   1.033   1.908   141   14.0      8.5  23.8   2:49 (180, 44)  

* C/2001 K5 ( LINEAR )


It is observable in good condition at 14-15 mag until autumn.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  18 11.46   25 11.5   5.742   5.245    55   14.1     15.7  53.7   3:32 (252,-19)  
Feb.  1  18 17.93   26 19.3   5.705   5.253    58   14.1     15.9  50.6   3:42 (247,-13)  

* 116P/Wild 4


Although it was expected to be 11 mag, the brightening pace is very slow in this return. It is still 14.5 mag. It will be 13 mag at best in spring.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  14 40.39  -15 13.9   2.073   2.170    82   14.2     24.4 110.9   3:32 (254, 47)  
Feb.  1  14 51.12  -16 12.3   1.996   2.171    86   14.2     22.9 110.6   3:42 (249, 52)  

* C/2002 X1 ( LINEAR )


It will keep 14-15 mag until the end of 2003.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   8 44.16   28  2.0   2.098   3.073   170   14.5     48.5 280.3   0:31 (180, 27)  
Feb.  1   8 18.23   28 51.6   2.067   3.031   165   14.4     49.8 276.6  23:30 (180, 26)  

* 155P/2002 R2 ( Shoemaker 3 )


It keeps observable in good condition until April when it becomes fainter than 18 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   9 52.46   21  8.2   0.912   1.868   159   14.9      7.3 350.7   1:38 (180, 34)  
Feb.  1   9 51.34   21 57.6   0.915   1.887   166   15.1      7.5 335.2   1:09 (180, 33)  

* C/2002 O7 ( LINEAR )


It will reach to 7 mag in autumn. In the Northern Hemisphere, it will observable only until July, when it reaches to 10 mag. After that, only southern people can observe it until December, when it fades to 9 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  15 48.14   28 27.6   3.562   3.570    82   15.3      7.0  45.6   3:32 (230,  5)  
Feb.  1  15 50.43   29  6.6   3.400   3.492    87   15.1      7.2  29.6   3:42 (224, 10)  

* 67P/Churyumov-Gerasimenko


It brightened about 1 mag after perihelion passage and reached to 12 mag. Now already getting fainter, but still bright as 14 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  12  2.13   11 19.4   1.419   2.167   127   15.1      7.1 314.6   3:32 (185, 44)  
Feb.  1  11 58.87   11 57.6   1.405   2.220   135   15.2     10.4 304.5   3:16 (180, 43)  

* C/2001 Q4 ( NEAT )


It will reach to 1 mag in 2004 spring. In the Northern Hemisphere, it locates low in the evening sky until February, then it will not be observable until 2004 spring.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   1 48.89  -38 20.8   6.154   5.905    70   15.2      5.2   2.7  20:51 ( 70, 50)  
Feb.  1   1 49.36  -37 43.8   6.164   5.841    66   15.1      5.5  14.0  20:43 ( 70, 46)  

* C/2000 SV74 ( LINEAR )


It became a bit fainter after the perihelion passage.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  15 10.23   41  0.5   4.097   4.293    94   15.2      3.5 355.3   3:32 (216,  1)  
Feb.  1  15  9.53   41 27.3   4.063   4.327    98   15.3      4.6 334.2   3:42 (210,  5)  

* C/2001 N2 ( LINEAR )


It keeps 15 mag until spring, but it will be low for the northern observers.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  15 27.56  -29 41.1   3.367   3.134    67   15.4     12.5 211.3   3:32 (280, 44)  
Feb.  1  15 23.37  -30 56.7   3.270   3.172    75   15.3     14.2 219.8   3:42 (277, 53)  

* 81P/Wild 2


It had brightened very rapidly since September and reached to 15 mag in late November. On the contrary, it has been at 15.5 mag for two months after that. It is only observable until spring. It is not observable around the perihelion passage.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   3 50.30   16 33.5   2.122   2.683   114   15.4      1.6 356.9  20:51 (157, 35)  
Feb.  1   3 50.96   16 47.2   2.173   2.642   107   15.4      3.6  51.0  20:43 (152, 33)  

* C/2002 U2 ( LINEAR )


The brightening pace is slow and it has been around 15.5 mag since late October.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  17  0.02   26 16.1   1.250   1.265    67   15.5     22.3 170.5   3:32 (242, -6)  
Feb.  1  17  1.27   23 47.0   1.239   1.301    70   15.5     20.7 176.9   3:42 (239,  2)  

* C/2002 T7 ( LINEAR )


It is expected to be 1 mag in the southern sky in 2004 spring.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   4 42.79   27 57.3   5.292   5.951   128   15.9      9.9 261.5  20:51 (174, 27)  
Feb.  1   4 37.97   27 47.0   5.329   5.885   120   15.8      8.6 260.3  20:43 (167, 26)  

* C/1999 U4 ( Catalina-Skiff )


It keeps 16 mag until June.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  13 33.05   36 12.0   5.578   6.015   111   16.0      2.8 349.7   3:32 (202, 15)  
Feb.  1  13 32.40   36 32.2   5.535   6.045   116   16.0      3.4 329.7   3:42 (194, 17)  

* 53P/Van Biesbroeck


Appearing at dawn. It will be 14 mag from spring to summer.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  15 19.70  -12 26.0   3.275   3.146    73   16.3     17.4  98.6   3:32 (258, 37)  
Feb.  1  15 27.76  -12 42.2   3.150   3.114    78   16.1     16.6  97.1   3:42 (253, 43)  

* C/2002 R3 ( LONEOS )


It will be observable at 16-17 mag until the end of 2003.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   1  8.87   14  6.5   4.167   4.056    76   16.5      6.5 258.1  20:51 (120, 15)  
Feb.  1   1  6.26   13 59.7   4.284   4.039    69   16.6      4.6 262.2  20:43 (116, 11)  

* P/2002 T5 ( LINEAR )


It is observable at 16.5 mag in this winter and in next winter.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   4  3.90   -8 25.2   3.594   4.031   109   16.8      9.6   2.6  20:51 (147, 60)  
Feb.  1   4  4.51   -7 16.9   3.671   4.022   103   16.9     10.1  12.2  20:43 (140, 56)  

* C/2002 A3 ( LINEAR )


It keeps 17 mag until April.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   9 29.38   15 32.8   4.601   5.557   164   17.1      9.5 324.2   1:15 (180, 40)  
Feb.  1   9 26.58   16 27.1   4.598   5.576   172   17.1      9.8 322.8   0:45 (180, 39)  

* D/1978 C2 ( Tritton )


The ephemeris says it is 17 mag at dusk in February. But it will not appear as predicted. It must have reached to 18 mag at meridian transit in the evening in 2002 autumn, but not recovered. It implies the comet is really fainter than this ephemeris.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   1  6.89   14 16.2   1.373   1.490    76   17.2     38.7  74.1  20:51 (120, 15)  
Feb.  1   1 25.41   15 31.4   1.397   1.470    73   17.1     40.9  74.5  20:43 (120, 14)  

* 79P/du Toit-Hartley


It will be 17 mag in winter and spring in the morning sky. After the last appearance in 1987, it has been missed twice in 1992 and 1997. It may be much fainter than this ephemeris. Because it keeps low in the morning sky, it will not be recovered by automated survey.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25  15 10.13  -20 30.3   1.101   1.256    73   17.2     60.6 107.7   3:32 (266, 43)  
Feb.  1  15 39.20  -22 28.9   1.077   1.242    73   17.1     60.0 105.2   3:42 (267, 46)  

* 90P/Gehrels 1


It did not begin to fade even after the perihelion passage, it kept 16 mag for a while. Now it has already begun to fade out gradually.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   4 52.30   34 31.6   2.606   3.327   130   17.2      2.5 182.5  20:51 (176, 20)  
Feb.  1   4 52.83   34 14.6   2.703   3.348   123   17.4      3.1 140.2  20:43 (172, 20)  

* C/2001 B2 ( NEAT )


It is getting fainter gradually. It keeps brighter than 18 mag until March.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   9  3.00   26 55.0   7.230   8.198   168   17.6     11.3 295.2   0:49 (180, 28)  
Feb.  1   8 57.63   27 27.5   7.262   8.233   169   17.6     11.2 293.7   0:16 (180, 28)  

* 2002 CE10


Asteroid with a cometary orbit. It will be 15.7 mag at opposition in early September in 2003.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 25   2 36.18   58 20.7   2.091   2.562   107   17.6     38.6 220.3  20:51 (161, -9)  
Feb.  1   2 18.02   54 58.5   2.176   2.521    98   17.7     33.3 213.2  20:43 (154, -9)  

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Copyright(C) Seiichi Yoshida (comet@aerith.net). All rights reserved.