Weekly Information about Bright Comets (2004 Jan. 31: North)

Japanese version
Home page
Updated on February 2, 2004
Last week South Next week

Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Northern Hemisphere.

---------------------------------------------------------------------

* C/2002 T7 ( LINEAR )


It has been brightening in rapid pace since mid December, and already reached to 7.5 mag. It will be 0 mag in the southern sky in spring. In the Northern Hemisphere, it is getting lower in the evening sky after this, and will be unobservable in early March.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31   0 23.86   17 18.0   1.896   1.692    62    7.4     18.0 225.0  18:53 ( 80, 44)  
Feb.  7   0 18.39   15 55.8   1.948   1.587    54    7.2     14.7 222.4  18:59 ( 85, 36)  

* C/2001 Q4 ( NEAT )


It is expected to be 2 mag in spring. In the Southern Hemisphere, it keeps observable around the same altitude in the evening sky until that time. On the other hand, in the Northern Hemisphere, it is not observable until that time.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  23  7.46  -69 29.2   2.330   1.956    55    8.9      9.7  16.2  18:53 ( 21,-25)  
Feb.  7  23 11.92  -68 27.9   2.236   1.869    55    8.7      9.2  26.9  18:59 ( 23,-27)  

* 2P/Encke


In the Northern Hemisphere, it is not observable until when it becomes fainter than 18 mag. In the Southern Hemisphere, it appears in the very low sky at dawn in late February, but it will be fainter than 15 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  19 36.30  -26 56.6   1.684   0.825    19   12.1     50.4  81.8   5:33 (297, -9)  
Feb.  7  20  0.70  -25 59.4   1.796   0.946    21   13.2     44.8  78.9   5:28 (296, -8)  

* C/2003 T3 ( Tabur )


Not obesrvable. In the Northern Hemisphere, it will appear at dawn at 12.5 mag. However, because it had been fading since the discovery although it was coming closer to the Sun, the brightness in May is quite uncertain. Then it keeps low until autumn.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  22 14.32  -18 28.5   2.821   1.923    19   12.5     34.5  42.4  18:53 ( 69, -2)  
Feb.  7  22 25.86  -15 26.7   2.793   1.865    15   12.5     35.7  42.3  18:59 ( 75, -5)  

* 43P/Wolf-Harrington


It will be observable at 12-13 mag in the evening sky until April. But it will be getting lower gradually.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31   1  5.58   13 47.8   1.697   1.647    70   12.6     37.1  85.7  18:53 ( 67, 51)  
Feb.  7   1 23.71   14  8.7   1.733   1.629    67   12.5     38.5  85.2  18:59 ( 71, 48)  

* C/2003 H1 ( LINEAR )


It keeps observable at 12-13 mag in the south until April. In the Northern Hemisphere, it locates 30 deg high, not so high in the south.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  14 23.28  -19 30.4   2.020   2.255    90   12.8     27.4 237.3   5:33 (356, 35)  
Feb.  7  14  9.86  -21 16.8   1.856   2.247    99   12.6     34.8 243.3   5:05 (  0, 34)  

* C/2001 HT50 ( LINEAR-NEAT )


It will be too low in the evening sky at 14 mag in March. CCD observers reported it more than 1 mag fainter than this ephemeris.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31   0 38.16    8 50.8   3.831   3.478    61   13.3      2.1 301.4  18:53 ( 67, 42)  
Feb.  7   0 37.67    9  0.5   3.994   3.519    54   13.5      1.7 349.2  18:59 ( 74, 36)  

* 29P/Schwassmann-Wachmann 1


It will be too low to observe soon. After conjunction, it will appear at dawn again in May.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  22 53.14   -1 44.7   6.521   5.729    33   13.8     11.4  67.1  18:53 ( 77, 15)  
Feb.  7  22 58.13   -1 12.7   6.578   5.728    28   13.8     11.8  66.6  18:59 ( 82, 10)  

* C/2003 K4 ( LINEAR )


It will be 6.5 mag in the southern sky from autumn to winter in 2004. It is getting higher in the morning sky. In the Northern Hemisphere, it is observable in good condition until early September when it becomes to 7.5 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  19 48.32   15 48.9   4.431   3.691    36   13.9      8.7  73.3   5:33 (260, 14)  
Feb.  7  19 52.32   16  9.6   4.336   3.615    38   13.8      8.8  67.2   5:28 (262, 18)  

* 88P/Howell


It was observed as 16.1 mag on Dec. 31, 1.5 mag fainter than expected. Although it had been expected to reach to 10 mag in spring, it may be 12.5 or 14 mag at best. It is observable in good condition in the Southern Hemisphere. But in the Northern Hemisphere, it keeps locating lower than 15 deg until June.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  17 48.07  -23 42.0   2.143   1.575    43   14.1     47.2  93.7   5:33 (311, 12)  
Feb.  7  18 12.44  -23 56.0   2.077   1.540    44   13.8     48.4  91.4   5:28 (311, 12)  

* 40P/Vaisala 1


It will be observable in good condition at 14 mag to April.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  14 41.36   -4 13.1   1.485   1.798    91   14.0     31.8  92.6   5:33 (348, 50)  
Feb.  7  14 55.82   -4 18.4   1.432   1.803    94   14.0     30.0  90.2   5:28 (352, 50)  

* 81P/Wild 2


Appearing at dawn and observed as bright as expected. It is fading out gradually after this.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  17 36.06  -20 54.2   2.558   2.004    46   14.2     30.7  92.0   5:33 (311, 16)  
Feb.  7  17 51.06  -20 58.5   2.538   2.042    49   14.3     29.3  90.5   5:28 (312, 17)  

* 58P/Jackson-Neujmin


Not yet recovered in this return. At the previous appearance, it brightened after the perihelion passage and reached to 10 mag. If it behaves so again, it may brighten after the perihelion passage on Jan. 9 and reach to 13 mag in March. However, it keeps locating very low in the evening sky.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  23 31.39   -9  8.4   2.020   1.411    39   15.1     52.0  72.9  18:53 ( 64, 18)  
Feb.  7  23 54.69   -7 18.8   2.056   1.428    38   14.6     51.7  72.1  18:59 ( 68, 18)  

* 123P/West-Hartley


It is observable in good condition at 15 mag until April.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  13 24.32   10 22.2   1.576   2.169   113   15.0      9.9 100.7   4:46 (  0, 65)  
Feb.  7  13 28.18   10 12.1   1.519   2.180   119   15.0      6.7  99.2   4:23 (  0, 65)  

* 65P/Gunn


Not observable. It becomes observable again at 15.5 mag after June.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  22 12.17  -19 31.6   3.810   2.899    19   15.3     24.8  68.4  18:53 ( 68, -3)  
Feb.  7  22 23.51  -18 27.3   3.857   2.919    15   15.3     24.7  68.1  18:59 ( 72, -7)  

* P/2002 T6 ( NEAT-LINEAR )


It reached to 15.5 mag in January, much brighter than expected.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31   6 34.12    9  7.6   2.849   3.704   145   16.1      5.2 294.7  21:53 (  0, 64)  
Feb.  7   6 32.28    9 23.7   2.925   3.723   138   16.3      3.9 308.8  21:24 (  0, 64)  

* C/2003 L2 ( LINEAR )


It will be observable around 16 mag until March in the northern sky.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  23 14.28   70 30.3   2.666   2.867    91   16.2     34.4 100.7  18:53 (156, 41)  
Feb.  7  23 59.74   69 28.2   2.703   2.871    89   16.3     34.4 107.4  18:59 (155, 43)  

* C/2003 T4 ( LINEAR )


It is expected to be 5 mag in 2005 spring. Until that time, it keeps observable in the Northern Hemisphere, which the comet will be getting brighter gradually.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31   5 26.98   77 39.6   5.041   5.531   115   16.4     10.2 246.5  20:45 (180, 47)  
Feb.  7   5  8.68   77  5.9   5.031   5.464   111   16.4      9.5 235.4  20:00 (180, 48)  

* C/2003 T2 ( LINEAR )


It will get fainter on and on after this and be too low in the evening sky at 18 mag in March. It seems to be fading much faster than expected recently.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31   2 11.20   -1 54.9   1.972   2.043    79   16.5     22.1 138.1  18:53 ( 32, 48)  
Feb.  7   2 18.26   -3 38.5   2.126   2.086    74   16.8     20.4 130.8  18:59 ( 39, 44)  

* 118P/Sheomaker-Levy 4


It will be fading slowly and become fainter than 18 mag in April.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  12 11.27    1 30.4   1.765   2.499   128   16.6      4.5 357.3   3:34 (  0, 56)  
Feb.  7  12 10.52    2  6.5   1.725   2.527   135   16.6      6.5 332.6   3:05 (  0, 57)  

* P/2002 T5 ( LINEAR )


It is observable around 17 mag until spring.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31   8  6.08   19 19.6   3.151   4.123   169   16.6     10.9 313.0  23:25 (  0, 74)  
Feb.  7   8  2.28   20 10.7   3.190   4.135   161   16.7     10.2 314.4  22:54 (  0, 75)  

* C/2003 G1 ( LINEAR )


Appearing at dawn. It keeps 17 mag until early summer, and observable in good condition brighter than 18 mag until October.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  18 35.36   18 53.6   6.233   5.643    49   16.8     13.8  53.4   5:33 (267, 30)  
Feb.  7  18 40.72   19 53.2   6.211   5.669    52   16.8     13.8  50.1   5:28 (268, 34)  

* C/2003 V1 ( LINEAR )


It will be observable until March when it will be fainter than 18 mag. It was a bit brighter than this ephemeris recently.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  10 16.36   48 49.4   3.308   4.149   144   17.0     10.4 287.8   1:39 (180, 76)  
Feb.  7  10  9.22   49  6.6   3.366   4.212   144   17.1     10.3 279.8   1:05 (180, 76)  

* C/2002 J5 ( LINEAR )


It keeps 17 mag until July.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31  17  3.30   37 53.7   5.947   5.807    77   17.0      9.9   6.3   5:33 (252, 56)  
Feb.  7  17  3.65   39  5.2   5.889   5.815    80   17.0     10.6   0.4   5:28 (251, 60)  

* 2003 WN188


Unusual minor planet with a period of 55 years. It becomes to be at peak in mid February, and fainter than 18 mag in late March.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31   9 45.02   24 54.6   1.352   2.319   165   17.3     20.5 353.8   1:08 (  0, 80)  
Feb.  7   9 43.60   27 17.8   1.325   2.296   167   17.2     20.6 351.2   0:39 (  0, 82)  

* C/2003 W1 ( LINEAR )


It will be fainter than 18 mag in early February.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Jan. 31   1 58.90   35 41.7   1.691   1.958    90   17.6     46.0 135.3  18:53 ( 98, 71)  
Feb.  7   2 16.27   32  9.0   1.827   2.006    85   17.8     40.8 133.3  18:59 ( 90, 67)  

---------------------------------------------------------------------

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