Weekly Information about Bright Comets (2004 Nov. 6: South)

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Updated on November 6, 2004
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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/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)  
Nov.  6   5 12.59  -30 13.1   0.962   1.707   121    7.4      2.7 216.4   2:11 (180, 85)  
Nov. 13   5 10.63  -30 14.9   0.862   1.637   124    6.9      6.0 288.7   1:42 (180, 85)  

* C/2003 K4 ( LINEAR )


It is much fainter than expected, about 7-7.5 mag. The pictures show that the dust emission has stopped. 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 until 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)  
Nov.  6  12 16.39  -23 23.8   1.735   1.097    35    7.4     39.7 204.4   3:18 (289, 14)  
Nov. 13  12  6.98  -27 51.9   1.628   1.144    43    7.4     45.5 206.3   3:10 (290, 22)  

* 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)  
Nov.  6   0 34.24   33 48.3   1.185   2.080   145   10.4     39.8 300.4  21:28 (180, 21)  
Nov. 13   0 15.94   35 55.0   1.230   2.066   136   10.4     33.8 298.9  20:43 (180, 19)  

* 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)  
Nov.  6   3 18.81   14 33.9   1.024   2.010   171   11.2     10.5 224.7   0:18 (180, 40)  
Nov. 13   3 15.10   13 42.4   1.025   2.013   175   11.2     10.6 227.5  23:42 (180, 41)  

* C/2001 Q4 ( NEAT )


It keeps observable for a long time after this in the Northern Hemisphere. It is also visible at midnight or dawn, but low.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Nov.  6  17 22.28   69 42.9   2.601   2.783    90   11.3     30.3  94.6  20:09 (156,-32)  
Nov. 13  18  2.45   69 13.9   2.652   2.866    92   11.5     30.5  99.7  20:19 (156,-31)  

* 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)  
Nov.  6   9 24.09   15 35.8   1.245   1.528    85   13.1     44.1  96.4   3:18 (229, 23)  
Nov. 13   9 45.22   15  0.1   1.190   1.513    87   12.4     43.8  96.6   3:10 (230, 23)  

* C/2003 T4 ( LINEAR )


The brightening evolution has been slower than usual. But finally it comes to be visible visually. In the Northern Hemisphere, it keeps observable until 2005 spring when it reaches to 8 mag. Now it locates at the same altitude both in the evening and morning.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Nov.  6  15  1.63   59 55.5   2.559   2.511    75   12.8     35.0 118.2  20:09 (142,-46)  
Nov. 13  15 29.66   57 51.1   2.466   2.423    75   12.7     36.5 120.5  20:19 (140,-47)  

* 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)  
Nov.  6  23 58.13    9 49.3   4.943   5.726   138   13.2      4.1 236.0  20:54 (180, 45)  
Nov. 13  23 56.77    9 34.3   5.022   5.727   131   13.2      3.0 229.6  20:25 (180, 45)  

* C/2002 T7 ( LINEAR )


It was observed as 13.7 mag on Oct. 16, as bright as expected. It will be getting fainter gradually until 2005 June when it becomes 17 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Nov.  6  11 37.75  -14 34.0   3.843   3.223    45   13.5      5.0 156.1   3:18 (276, 17)  
Nov. 13  11 38.41  -15  5.5   3.831   3.308    51   13.6      4.4 171.1   3:10 (274, 21)  

* (944) Hidalgo


It will be fading slowly until 2005 August when it becomes low in the evening sky at 16.5 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Nov.  6   1 18.69   38 15.2   1.172   2.094   150   13.5     32.2 300.1  22:13 (180, 17)  
Nov. 13   1  2.50   39 56.4   1.185   2.070   144   13.6     28.7 296.9  21:29 (180, 15)  

* 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)  
Nov.  6   2 58.17   10  8.3   1.290   2.277   173   13.9     14.4 280.9  23:53 (180, 45)  
Nov. 13   2 51.27   10 29.6   1.260   2.242   170   13.7     15.2 283.0  23:18 (180, 44)  

* P/2004 T1 ( LINEAR-NEAT )


It was visible visually around 13.5 mag in October. It will be fading after this, but 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)  
Nov.  6   0 40.91   -5 59.7   0.815   1.710   142   14.1     16.2 354.9  21:36 (180, 61)  
Nov. 13   0 41.11   -4  2.9   0.852   1.710   136   14.2     17.4   7.8  21:09 (180, 59)  

* C/2003 T3 ( Tabur )


Diffused, but still bright as 14 mag. It keeps observable until 2005 May when it becomes fainter than 18 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Nov.  6  11 27.23   39 37.6   3.042   2.899    72   14.2     10.0 108.6   3:18 (230,-13)  
Nov. 13  11 32.51   39 22.4   3.025   2.966    77   14.3      8.0 103.5   3:10 (229,-10)  

* 88P/Howell


Diffused, but still bright as 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)  
Nov.  6   1 51.65    8 33.9   1.454   2.424   164   14.9     13.8 259.5  22:46 (180, 46)  
Nov. 13   1 45.83    8 19.3   1.530   2.469   156   15.3     11.1 261.5  22:13 (180, 47)  

* 10P/Tempel 2


The condition of this return is bad. It is not observable around the perihelion passage. It will appear at dawn in 2005 July at 14.5 mag, then it will be fading after that.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Nov.  6  16  2.45  -14 49.7   2.668   1.757    18   15.3     38.6 106.4  20:09 ( 68, -5)  
Nov. 13  16 20.74  -16  3.3   2.648   1.719    16   14.9     39.8 104.8  20:19 ( 64, -8)  

* 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)  
Nov.  6   9 53.49   20 13.8   2.660   2.678    80   15.2     18.4  89.4   3:18 (231, 15)  
Nov. 13  10  2.31   20 17.5   2.577   2.685    85   15.1     17.1  86.9   3:10 (229, 17)  

* 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)  
Nov.  6  11 11.92   -6 21.4   2.762   2.308    53   15.6     20.8 118.5   3:18 (265, 18)  
Nov. 13  11 20.14   -7 29.2   2.743   2.368    57   15.8     19.1 119.5   3:10 (265, 20)  

* 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)  
Nov.  6   1  0.84   -4 30.9   2.858   3.729   146   15.9      8.0 269.6  21:56 (180, 59)  
Nov. 13   0 57.48   -4 28.2   2.939   3.748   139   16.0      6.4 277.3  21:25 (180, 59)  

* 69P/Taylor


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)  
Nov.  6   8 21.34   12 30.7   1.533   1.953    99   16.1     22.5  80.8   3:18 (217, 34)  
Nov. 13   8 31.56   13  0.2   1.457   1.947   103   16.0     21.0  76.5   3:10 (214, 35)  

* 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)  
Nov.  6  23 23.28    0 56.6   1.861   2.591   127   16.1      2.9  29.6  20:19 (180, 54)  
Nov. 13  23 24.56    1 17.0   1.923   2.581   121   16.1      5.2  50.6  20:19 (169, 53)  

* C/2001 HT50 ( LINEAR-NEAT )


It will be too low in the evening sky at 17.5 mag in early February.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Nov.  6  22 33.06    6 40.2   4.863   5.394   117   16.1     10.3 235.8  20:09 (165, 47)  
Nov. 13  22 29.49    6  2.1   5.029   5.445   109   16.2      8.4 232.9  20:19 (151, 45)  

* 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)  
Nov.  6   5 45.33  -12  8.3   4.740   5.400   127   16.2     13.8 227.1   2:44 (180, 67)  
Nov. 13   5 40.11  -13 13.3   4.621   5.338   132   16.1     14.8 232.0   2:11 (180, 68)  

* C/2004 S1 ( Van Ness )


It approached to the earth in mid October and reached to 15 mag. However, it has been reported fainter than expected after that. 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)  
Nov.  6  18 43.90   11 17.9   0.733   0.951    64   16.1     58.3 249.4  20:09 (112, 11)  
Nov. 13  18 22.65    9 15.7   0.903   0.862    53   16.1     40.3 248.1  20:19 (102,  1)  

* 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)  
Nov.  6   6  3.38   45 17.4   5.791   6.467   129   16.4      5.3 335.7   3:02 (180, 10)  
Nov. 13   6  1.59   45 50.6   5.693   6.437   135   16.3      5.6 325.6   2:33 (180,  9)  

* (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)  
Nov.  6   5 29.61   38 57.1   1.033   1.886   137   16.8     23.4 281.6   2:29 (180, 16)  
Nov. 13   5 12.86   39 23.2   0.922   1.831   146   16.4     33.0 274.6   1:45 (180, 16)  

* 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)  
Nov.  6  18 14.49    4 51.5   1.022   0.941    55   16.8    119.5  92.9  20:09 (103, 10)  
Nov. 13  19  3.83    4  6.3   1.163   1.100    60   17.7     92.6  93.8  20:19 (105, 13)  

* 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)  
Nov.  6   6 12.05   28 10.1   2.253   2.999   131   17.0      1.3 286.3   3:11 (180, 27)  
Nov. 13   6 10.74   28 12.3   2.175   2.987   138   16.9      3.7 273.7   2:42 (180, 27)  

* 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)  
Nov.  6   0 56.31   10 58.2   2.303   3.218   152   16.9      7.9 233.8  21:52 (180, 44)  
Nov. 13   0 53.67   10 27.3   2.343   3.207   145   16.9      6.2 228.7  21:21 (180, 45)  

* 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)  
Nov.  6  22 20.50    1 33.1   1.493   2.092   113   17.1     14.2  50.6  20:09 (159, 51)  
Nov. 13  22 26.22    2 36.9   1.569   2.098   108   17.2     16.4  55.6  20:19 (148, 47)  

* C/2004 U1 ( LINEAR )


It will be 17 mag at best in December and January.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Nov.  6   8 51.00   26 10.6   2.397   2.685    95   17.7     24.8 340.6   3:18 (216, 19)  
Nov. 13   8 45.50   29  7.6   2.250   2.677   104   17.5     30.0 335.0   3:10 (209, 19)  

* 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)  
Nov.  6   7 10.63   16 22.0   3.487   4.031   116   17.6     13.8 221.2   3:18 (195, 37)  
Nov. 13   7  5.73   15  9.1   3.432   4.076   124   17.6     15.3 226.8   3:10 (188, 39)  

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