Weekly Information about Bright Comets (2004 Apr. 24: North)

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Updated on April 24, 2004
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Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Northern Hemisphere.

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* C/2001 Q4 ( NEAT )


Good condition and visible with naked-eye in the Southern Hemisphere. In the Northern Hemisphere, it is not observable until early May. It reaches to 2 mag in early and mid May.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24   4 28.05  -60 28.4   0.516   1.035    78    3.3    134.5  57.2  20:11 ( 35,-28)  
May   1   6 14.04  -44 28.7   0.369   0.997    77    2.4    262.4  35.5  20:19 ( 44,-10)  

* C/2002 T7 ( LINEAR )


Good condition and visible with naked-eye in the Southern Hemisphere. In the Northern Hemisphere, it locates extremely low sky at dawn until early May. It reaches to 1.5-2 mag in mid May.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  23 54.81    3 24.8   1.078   0.615    34    4.0     23.7 148.3   3:45 (267,  2)  
May   1   0  6.09    0 38.4   0.815   0.639    39    3.5     48.9 125.7   3:35 (270,  2)  

* C/2004 F4 ( Bradfield )


It reached to -2 mag at the perihelion passage. It has been observed at dawn since Apr. 22, and the comet is bright as 3-4 mag. In the Northern Hemisphere, the comet will be higher and higher after this. Although it becomes fainter rapidly, it will be a good target for visual observation in May. Not observable in the Southern Hemisphere. It passes very close by C/2003 T3 ( Tabur ) on Apr. 25.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24   1  6.30   23 48.3   0.913   0.316    18    4.8    119.8 342.3   3:45 (241,  0)  
May   1   0 59.01   33 27.3   1.092   0.519    28    7.3     60.7 359.9   3:35 (236, 10)  

* C/2003 T3 ( Tabur )


Appearing at dawn. Now it is 9.5 mag, as bright as expected. In the Northern Hemisphere, it keeps low after this until autumn. Not observable in the Southern Hemisphere. It passes very close by a new comet C/2004 F4 ( Bradfield ) on Apr. 25.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24   0 57.64   25 40.1   2.379   1.482    20    9.5     50.6  43.5   3:45 (240,  3)  
May   1   1 16.50   29 56.4   2.353   1.481    23    9.6     51.6  44.8   3:35 (237,  5)  

* 88P/Howell


It keeps 10-11 mag until mid May. Good condition in the Southern Hemisphere, but it locates lower than 10 deg in the Northern Hemisphere. It becomes higher after June, but the comet will be fading at that time.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  22 45.89  -11 22.4   1.663   1.373    55   10.8     49.4  69.8   3:45 (289,  7)  
May   1  23  7.52   -9 21.7   1.650   1.382    56   10.9     48.0  69.0   3:35 (287,  8)  

* 103P/Hartley 2


The condition is worst in this return. It is not observable around the perihelion passage. It will appear at dawn in autumn, when it will already fade to 15 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24   1 20.95   12  4.5   2.058   1.090    11   11.3     63.4  75.0   3:45 (248,-10)  
May   1   1 50.68   13 53.7   2.038   1.064    10   11.1     64.5  76.6   3:35 (244,-11)  

* C/2003 K4 ( LINEAR )


Well condensed and easy to see. It is about 0.5 mag brighter than this ephemeris visually. It will be 6.5 mag in the southern sky from autumn to winter in 2004. 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)  
Apr. 24  20 11.55   28 33.7   2.686   2.750    82   11.5     18.6 340.1   3:45 (273, 60)  
May   1  20  7.16   30 42.7   2.508   2.669    87   11.3     21.8 332.4   3:35 (272, 65)  

* C/2003 H1 ( LINEAR )


It was diffused around 11.5 mag visually in February and March. But it began to fade in mid April. It will be lower and fainter gradually in the evening sky after this.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24   8 45.12  -15 11.2   1.918   2.347   102   12.8     30.0 300.9  20:11 ( 29, 35)  
May   1   8 34.48  -13 33.2   2.085   2.372    93   13.0     22.6 303.9  20:19 ( 42, 31)  

* 43P/Wolf-Harrington


It will be lower and lower while fading after this.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24   5  8.63   16 10.3   2.189   1.622    43   13.0     43.2  93.4  20:11 ( 97, 19)  
May   1   5 29.50   15 48.0   2.239   1.640    42   13.1     43.0  94.8  20:19 ( 99, 16)  

* 29P/Schwassmann-Wachmann 1


Appearing at dawn. But no observations have been reported yet.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  23 55.02    5 35.1   6.537   5.725    33   13.8     11.5  62.0   3:45 (265,  3)  
May   1  23 59.68    6 12.5   6.474   5.725    38   13.7     11.1  61.4   3:35 (267,  6)  

* C/2001 HT50 ( LINEAR-NEAT )


Not observable. It will appear at dawn soon.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24   0 52.95   13  9.3   4.950   4.006    18   14.6      4.9  38.4   3:45 (251, -4)  
May   1   0 54.30   13 36.1   4.952   4.053    24   14.6      4.6  33.8   3:35 (253, -1)  

* 58P/Jackson-Neujmin


At the previous appearance, it brightened after the perihelion passage and reached to 10 mag. If it has behaved so again, it could have reach to 13 mag in February and March. However, it must be much fainter actually than expected. It seems to go while nobody succeeded to observe it in this return.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24   3 42.65   10 25.2   2.710   1.831    23   14.6     39.5  77.1  20:11 (104, -2)  
May   1   4  0.69   11 22.8   2.782   1.880    21   14.9     38.2  78.4  20:19 (107, -5)  

* 40P/Vaisala 1


The brightness evolution is gradual in this return. So it will reach to 15 mag at best.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  16  3.98    1 16.9   1.097   2.020   147   15.1      7.1 301.2   1:56 (  0, 56)  
May   1  16  0.61    1 37.3   1.103   2.052   152   15.1      8.5 284.4   1:25 (  0, 57)  

* 123P/West-Hartley


It became brighter than expected after the perihelion passage, and it was observed visually around 13.5 mag in February and March. After this, it will be fading.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  12 48.73    7 52.0   1.444   2.377   151   15.1     12.0 235.5  22:36 (  0, 63)  
May   1  12 44.65    7  0.9   1.504   2.400   145   15.3     10.8 223.6  22:05 (  0, 62)  

* 118P/Sheomaker-Levy 4


Althouhg it must be fainter than 17 mag, it unexpectedly brightened from February to March and reached to 14.5 mag. It has already begun to fade, and faded to 16 mag in mid April.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  11 29.32   10  2.4   2.056   2.853   134   15.7      2.4 299.6  21:18 (  0, 65)  
May   1  11 28.86   10  6.4   2.154   2.883   127   15.9      0.1 105.5  20:50 (  0, 65)  

* 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)  
Apr. 24   5  3.16   69 58.3   5.074   4.708    63   15.8      7.2 115.1  20:11 (155, 36)  
May   1   5 12.53   69 38.8   5.061   4.637    59   15.7      7.8 108.9  20:19 (155, 34)  

* P/2004 F3 ( NEAT )


New periodic comet. It is observable at 15-16 mag for a long time until 2005 autumn.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  13 24.80   12  8.2   2.236   3.165   152   15.8     10.4 269.2  23:12 (  0, 67)  
May   1  13 20.06   12  2.5   2.255   3.150   147   15.7      9.6 261.0  22:40 (  0, 67)  

* 81P/Wild 2


In the Northern Hemisphere, it keeps fading at about 35 deg high until August when it becomes fainter than 18 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  19 37.87  -18 42.3   2.094   2.489   100   15.8      7.5  78.4   3:45 (331, 31)  
May   1  19 40.81  -18 33.3   2.045   2.531   107   15.9      4.7  77.3   3:35 (335, 32)  

* 48P/Johnson


It was 18.5 mag in early April, about 1 mag fainter than this ephemeris. It will reach to 15 mag in summer.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  19 48.96  -14 33.0   2.243   2.576    97   16.9     14.9  86.3   3:45 (326, 34)  
May   1  19 55.76  -14 27.6   2.138   2.557   102   16.8     13.3  87.7   3:35 (329, 35)  

* C/2003 G1 ( LINEAR )


It will be fading slowly until November when it becomes fainter than 18 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  19 14.67   34  1.1   5.830   5.974    93   16.9     11.7   1.7   3:45 (268, 73)  
May   1  19 14.55   35 21.9   5.803   6.004    96   16.9     11.4 356.1   3:35 (264, 77)  

* C/2004 G1 ( LINEAR )


New comet. Now it is at peak at 17 mag. It will be low in May, and will fade out while locating low.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24   1 37.46   83 58.6   1.305   1.366    71   16.9     71.3 116.2   3:45 (186, 32)  
May   1   3 52.83   78  7.5   1.405   1.319    63   16.9     59.8 151.9  20:19 (166, 31)  

* 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)  
Apr. 24  16  4.74   53 59.5   5.538   5.936   108   17.0     16.7 297.9   1:57 (180, 71)  
May   1  15 52.61   54 47.6   5.558   5.949   108   17.0     16.5 291.3   1:17 (180, 70)  

* C/2003 E1 ( NEAT )


It will be observable at 17.5 mag in good condition until August.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  18 32.43   11  7.9   2.815   3.298   109   17.0      5.4  46.6   3:45 (338, 65)  
May   1  18 33.83   11 31.8   2.755   3.308   114   17.0      3.6  32.4   3:35 (347, 66)  

* C/2004 DZ61 ( Catalina-LINEAR )


It was at peak in mid April. It will be lower while fading after this.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  11 57.94   44 51.0   1.409   2.051   115   17.4     25.4 347.8  21:46 (180, 80)  
May   1  11 55.22   47 25.0   1.484   2.037   108   17.4     19.5 352.1  21:16 (180, 77)  

* C/2000 SV74 ( LINEAR )


It was observed around 17.5 mag recently. It will be fainter than 18 mag in late May.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  13 31.21    7 28.2   6.116   7.057   157   17.5      9.2 264.5  23:19 (  0, 62)  
May   1  13 27.00    7 20.6   6.196   7.103   152   17.6      8.8 261.5  22:47 (  0, 62)  

* C/2003 F1 ( LINEAR )


It will be observable around 17.5 mag until June.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  18 15.25   -8 34.3   4.038   4.612   119   17.7      7.2 224.4   3:45 (352, 46)  
May   1  18 12.49   -9 11.7   3.969   4.638   126   17.7      8.7 230.0   3:35 (  0, 46)  

* C/2003 V1 ( LINEAR )


Fading slowly. It will be observable in good condition until May when it will be fainter than 18 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24   9 29.20   43 30.1   4.697   4.894    95   17.8      7.7 165.0  20:11 (134, 77)  
May   1   9 30.85   42 37.4   4.854   4.956    89   17.9      8.2 157.4  20:19 (121, 72)  

* 117P/Helin-Roman-Alu 1


It was brighter than this ephemeris recently, around 17.5 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 24  11 37.81   12 30.1   3.250   4.025   135   18.2      5.4 267.8  21:26 (  0, 67)  
May   1  11 35.57   12 25.8   3.310   4.009   127   18.2      4.1 255.3  20:56 (  0, 67)  

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