Weekly Information about Bright Comets (2004 Oct. 23: North)

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Updated on October 25, 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/2003 K4 ( LINEAR )


Appearing at dawn in November. In the Southern Hemisphere, it keeps observable in good condition for a while after this. In the Northern Hemisphere, it is visible in the morning low sky from mid November to early December, but becomes unobservable soon, then keeps unobservable until January.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  12 30.32  -15 46.0   1.912   1.036    20    5.9     32.3 202.3   4:48 (286, -4)  
Oct. 30  12 23.94  -19 24.1   1.831   1.060    27    5.9     35.4 203.1   4:53 (295,  1)  

* C/2004 Q2 ( Machholz )


It will be getting brighter on and on after this, then it will reach to 4 mag locating high in the evening sky in December and January. In the Northern Hemisphere, it keeps observable in good condition for a long time while the comet is bright enough visible visually until 2005 October when it becomes faint as 14 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   5 10.55  -29  7.2   1.173   1.851   117    8.5      8.3 142.3   3:04 (  0, 26)  
Oct. 30   5 12.47  -29 47.7   1.066   1.778   119    8.1      5.3 157.8   2:39 (  0, 25)  

* C/2004 Q1 ( Tucker )


It brightened rapidly and reached to 10 mag. It keeps high in the evening sky and bright as around 11 mag until December. It will be fading after January, however, it keeps high in the evening sky for a long time in the Northern Hemisphere.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   1 14.71   28 11.3   1.149   2.115   161   10.8     47.3 306.1  23:03 (  0, 83)  
Oct. 30   0 54.24   31 13.5   1.158   2.096   154   10.7     44.6 303.0  22:16 (  0, 86)  

* C/2001 Q4 ( NEAT )


It locates visible all night in the northern sky. It keeps observable after this in the Northern Hemisphere.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  16  1.80   69 42.8   2.522   2.617    84   11.0     29.1  84.1  18:40 (155, 39)  
Oct. 30  16 41.62   69 52.4   2.558   2.701    87   11.2     29.8  89.2  18:33 (155, 41)  

* 78P/Gehrels 2


Well condensed and easy to see visually. It is observable in good condition as bright as 11-12 mag until January.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   3 24.50   16 15.5   1.055   2.008   156   11.2      7.8 209.6   1:19 (  0, 71)  
Oct. 30   3 22.08   15 26.0   1.034   2.008   164   11.2      9.5 219.4   0:49 (  0, 70)  

* C/2003 T3 ( Tabur )


It has been fading slowly and it will keep 13 mag still in December. However, no observations have been reported in October.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  11 13.68   40 39.1   3.054   2.758    63   12.8     13.8 113.6   4:48 (243, 40)  
Oct. 30  11 20.96   40  4.3   3.051   2.828    67   12.9     12.0 111.5   4:53 (246, 44)  

* C/2003 T4 ( LINEAR )


The brightening evolution is slower than usual. In the Northern Hemisphere, it keeps observable until 2005 spring when it reaches to 8 mag. It keeps observable both in the evening and morning until December, however, it keeps locating low at 20-25 deg high.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  14  2.70   63 21.8   2.767   2.684    74   13.2     31.7 113.1  18:40 (151, 26)  
Oct. 30  14 32.58   61 45.9   2.660   2.598    75   13.0     33.3 115.8  18:33 (148, 26)  

* 29P/Schwassmann-Wachmann 1


It burst out on Oct. 6 and reached to 11 mag. Then it was as bright as 12 mag still in mid October. But it came to be diffused in late October.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   0  2.27   10 24.5   4.820   5.726   153   13.1      5.9 242.9  21:53 (  0, 65)  
Oct. 30  23 59.98   10  6.2   4.875   5.726   146   13.1      5.1 240.0  21:23 (  0, 65)  

* C/2002 T7 ( LINEAR )


Appearing at dawn, however, it will be mid November when the altitude exceeds 20 deg high. It was observed as 13.7 mag on Oct. 16, as bright as expected.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  11 34.66  -13 28.0   3.832   3.050    33   13.3      6.5 138.1   4:48 (293,  8)  
Oct. 30  11 36.48  -14  1.4   3.844   3.137    39   13.4      5.7 145.6   4:53 (298, 13)  

* (944) Hidalgo


It is observable at 13.5 mag in good condition in October and November.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   1 51.31   33 47.3   1.193   2.146   157   13.5     34.9 308.7  23:40 (  0, 89)  
Oct. 30   1 35.32   36 11.3   1.175   2.119   155   13.5     34.4 304.2  22:57 (180, 89)  

* 62P/Tsuchinshan 1


Michael Jager reported that it was bright as 13 mag on Oct. 24. The comet is now brightening very rapidly, as expected. It will be visible visually at 11 mag from November to January.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   8 41.58   16 40.7   1.368   1.567    81   15.0     43.8  95.3   4:48 (301, 60)  
Oct. 30   9  2.84   16  9.7   1.304   1.546    83   14.0     44.0  96.0   4:53 (306, 62)  

* P/2004 T1 ( LINEAR-NEAT )


It is also visible visually around 13.5 mag. Now it is brightest, and it will start fading after November. It keeps observable until it becomes fainter than 18 mag in 2005 spring.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   0 45.41   -9 23.4   0.766   1.715   153   14.0     14.9 328.6  22:36 (  0, 46)  
Oct. 30   0 42.41   -7 47.5   0.786   1.711   147   14.0     15.4 341.6  22:05 (  0, 47)  

* 32P/Comas Sola


It has been already visible visually around 14 mag. It will be 12-13 mag in winter, locating high in the evening sky. It keeps observable until that time in good condition while the comet is getting brighter.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   3 10.01    9 37.3   1.389   2.350   160   14.4     10.5 279.8   1:04 (  0, 65)  
Oct. 30   3  4.54    9 51.2   1.333   2.314   167   14.1     12.8 279.9   0:31 (  0, 65)  

* 88P/Howell


Diffused, but some reported that it is still 14 mag. It keeps observable in good condition until December when it becomes fainter than 18 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   2  6.27    9 18.3   1.340   2.333   175   14.3     17.3 257.7   0:01 (  0, 64)  
Oct. 30   1 58.56    8 54.0   1.390   2.379   173   14.6     15.9 258.4  23:21 (  0, 64)  

* C/2004 R2 ( ASAS )


Appearing at dawn, however, it has not been detected yet. Because it rapidly faded out just after the perihelion passage, now it may be much fainter than this ephemeris. Or, it may have already disappeared. Anyway, it will fade out rapidly after this.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  15 56.13    5 11.1   0.896   0.580    35   14.4    170.0  87.3  18:40 ( 84, 18)  
Oct. 30  17 11.51    5 25.2   0.925   0.769    47   15.7    149.1  90.9  18:33 ( 75, 29)  

* C/2004 S1 ( Van Ness )


It approached to the earth in mid October and reached to 15 mag. It will go far away from the earth after this. Because it will be closer to the sun, the ephemeris says it keeps 16 mag for a while after this. However, it may disappear due to its small perihelion distance. In November, it will be getting lower and lower rapidly.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  20 23.23   18 54.5   0.410   1.147   101   15.2    191.8 256.3  18:40 ( 24, 72)  
Oct. 30  19 18.05   14 17.3   0.563   1.047    79   15.5     99.1 251.4  18:33 ( 58, 57)  

* 103P/Hartley 2


Appearing at dawn. It was observed as 16.5 mag on Oct. 6, 1.5 mag fainter than this ephemeris. After this, it keeps observable while it will be fading gradually until it becomes fainter than 18 mag in 2005 April.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  10 53.28   -3 56.3   2.781   2.188    44   15.2     24.0 116.7   4:48 (292, 22)  
Oct. 30  11  2.95   -5 10.4   2.775   2.248    48   15.4     22.4 117.5   4:53 (297, 25)  

* 121P/Shoemaker-Holt 2


It tends to become brightest after the perihelion passage. It was 17 mag on Sept. 18. In this return, it will reach to 14 mag in 2005 February at the opposition.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   9 34.10   20 19.8   2.825   2.667    70   15.4     20.6  92.5   4:48 (282, 52)  
Oct. 30   9 44.06   20 14.9   2.743   2.672    75   15.3     19.5  91.2   4:53 (287, 57)  

* 48P/Johnson


In the Northern Hemisphere, it keeps to be locating only around 30 deg high. It will be fading after this, and will be fainter than 18 mag in February.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  20 26.06  -27 24.8   2.046   2.311    92   15.7     18.9  81.7  18:40 (  5, 27)  
Oct. 30  20 36.26  -27  2.3   2.129   2.313    87   15.9     20.5  79.7  18:33 (  8, 28)  

* 65P/Gunn


It will be as faint as 17.5 mag in 2005 March when it becomes low in the evening western sky.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   1  9.48   -4 18.4   2.734   3.690   161   15.8     10.4 260.6  23:00 (  0, 51)  
Oct. 30   1  4.89   -4 27.6   2.790   3.709   154   15.9      9.3 264.5  22:27 (  0, 51)  

* C/2001 HT50 ( LINEAR-NEAT )


It will fade out gradually, and keeps observable brighter than 17 mag until the end of 2004.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  22 42.87    8 10.7   4.558   5.292   133   15.8     14.2 240.1  20:33 (  0, 63)  
Oct. 30  22 37.52    7 23.2   4.705   5.343   125   16.0     12.3 238.1  20:01 (  0, 62)  

* 56P/Slaughter-Burnham


It keeps observable at 16 mag in good condition until the end of 2004.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  23 24.39    0 32.6   1.758   2.615   141   16.0      3.8 284.6  21:15 (  0, 56)  
Oct. 30  23 23.23    0 42.0   1.805   2.603   134   16.0      2.1 324.9  20:46 (  0, 56)  

* C/2004 B1 ( LINEAR )


It will reach to 9 mag in 2006 spring. It has been brightening well as expected. In this season, it keeps observable until 2005 March when it becomes 15.5 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   5 53.40   -9 55.8   5.011   5.522   116   16.4     11.6 216.0   3:47 (  0, 45)  
Oct. 30   5 49.76  -11  2.1   4.870   5.461   121   16.3     12.7 221.8   3:16 (  0, 44)  

* 69P/Taylor


It is already bright, as 17 mag on Oct. 21. It will be observable in good conditon at 15.5 mag in winter. In its last return in 1997, it burst out after the perihelion passage and became extremely bright, reached to 11 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   7 59.02   11 55.5   1.691   1.969    90   16.5     25.2  85.8   4:48 (324, 63)  
Oct. 30   8 10.71   12 10.7   1.611   1.960    94   16.3     24.0  83.8   4:53 (334, 65)  

* C/2003 WT42 ( LINEAR )


It keeps observable in good condition at 16 mag until 2005 spring. It will reach to 15 mag in 2006.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   6  4.89   44  8.6   6.016   6.527   116   16.5      5.0 358.8   3:59 (180, 81)  
Oct. 30   6  4.48   44 43.2   5.900   6.497   123   16.4      5.1 346.9   3:31 (180, 80)  

* 160P/2004 NL21 ( LINEAR )


It will fade out after this, and become fainter than 18 mag at the end of 2004.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  22 13.01   -0 30.0   1.352   2.084   124   16.8      9.9  29.6  20:04 (  0, 55)  
Oct. 30  22 16.05    0 30.9   1.420   2.087   118   17.0     11.9  42.6  19:40 (  0, 56)  

* 119P/Parker-Hartley


It is observable at 17 mag in good condition until January.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   1  3.61   12  7.7   2.261   3.241   168   16.9     10.1 239.5  22:54 (  0, 67)  
Oct. 30   0 59.68   11 32.2   2.275   3.229   160   16.9      9.2 237.1  22:22 (  0, 67)  

* 129P/Shoemaker-Levy 3


It is observable at 16.5 mag in good condition from November to February.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   6 10.83   28  4.1   2.433   3.023   117   17.2      3.5  82.2   4:04 (  0, 83)  
Oct. 30   6 12.06   28  7.3   2.340   3.011   124   17.1      1.2  69.6   3:38 (  0, 83)  

* (3200) Phaethon


It keeps observable at 15.5 mag from mid November to mid February.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   5 47.49   37 44.1   1.279   1.987   121   17.5      9.7 303.1   3:41 (180, 87)  
Oct. 30   5 40.78   38 21.6   1.153   1.939   129   17.2     15.7 290.0   3:07 (180, 87)  

* 53P/Van Biesbroeck


It will be fainter than 18 mag in November.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   0 33.03   -3  3.0   2.804   3.734   155   17.4      7.8 247.0  22:23 (  0, 52)  
Oct. 30   0 29.97   -3 21.5   2.888   3.768   148   17.5      6.3 249.2  21:53 (  0, 52)  

* C/2003 L2 ( LINEAR )


It keeps observable at 18 mag in good condition until January.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23   7 17.50   18 45.7   3.621   3.941   101   17.7     11.3 206.0   4:48 (341, 73)  
Oct. 30   7 14.57   17 34.3   3.551   3.986   108   17.7     12.4 214.4   4:41 (  0, 73)  

* C/2003 G1 ( LINEAR )


It will be fainter than 18 mag in November.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Oct. 23  18 33.94   38 45.5   6.867   6.811    82   17.8      7.0 121.0  18:40 (108, 63)  
Oct. 30  18 37.75   38 21.7   6.948   6.845    79   17.9      7.5 115.2  18:33 (108, 60)  

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