Weekly Information about Bright Comets (2005 Feb. 26: South)

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Updated on February 27, 2005
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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 )


Fading slowly. It is visible all night in the Northern Hemisphere. In the Northern Hemisphere, it keeps observable in good condition for a long time while the comet is bright enough visible visually until 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)  
Feb. 26   3 39.89   81  5.4   0.744   1.304    96    5.5     34.6  29.3  20:09 (173,-28)  
Mar.  5   5  2.99   83 58.4   0.815   1.349    96    5.9     32.7  54.5  19:58 (177,-30)  

* C/2003 T4 ( LINEAR )


In the Northern Hemisphere, it will be unobservable in early April. In the Southern Hemisphere, it will appear in the morning low sky in mid March, then it keeps observable after that. It keeps bright as around 8 mag from March to May.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  20 21.01   13 48.4   1.622   1.081    40    9.3     45.1 134.8   4:15 (256, -4)  
Mar.  5  20 36.74    9 54.4   1.548   1.009    39    9.0     49.1 135.8   4:23 (256,  2)  

* C/2005 A1 ( LINEAR )


In the Southern Hemisphere, it keeps visible as bright as 9-10 mag until April, but it locates low after late March. In the Northern Hemisphere, it is not observable until June when it appears in the morning at 13 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  16 30.51  -75 23.8   0.804   1.184    81    9.8    131.0 143.1   4:15 (350, 48)  
Mar.  5  21 28.87  -80 30.5   0.815   1.111    75    9.5    125.4  72.4   4:23 (349, 34)  

* C/2003 K4 ( LINEAR )


It will be fading gradually in the evening sky. It becomes too low in the evening sky at 12-13 mag in April.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   3 31.25  -20 38.3   2.419   2.308    71   10.6     23.3 357.9  20:09 ( 97, 47)  
Mar.  5   3 31.46  -18  7.0   2.609   2.392    66   10.9     20.1   4.5  19:58 ( 98, 43)  

* 10P/Tempel 2


The condition of this return is bad. It is not observable around the perihelion passage. It will appear at dawn in 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)  
Feb. 26  22  3.13  -14 58.1   2.395   1.432    10   11.9     49.6  75.5   4:15 (294, -8)  
Mar.  5  22 26.10  -13 27.3   2.397   1.439    11   11.9     49.2  74.3   4:23 (291, -6)  

* 78P/Gehrels 2


Getting diffused in February. It will be visible visually until May when it becomes too low in the evening sky at 13-14 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   4 14.29   15 13.0   2.058   2.237    87   12.3     23.3  77.8  20:09 (141, 30)  
Mar.  5   4 25.54   15 46.5   2.160   2.261    82   12.4     24.1  78.9  19:58 (140, 29)  

* C/2004 Q1 ( Tucker )


In the Northern Hemisphere, it keeps the same altitude at 35 deg high in the evening sky until June when it fades down to 15 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   0 43.68   58 14.0   2.366   2.261    71   12.4     24.9  48.3  20:09 (144,-28)  
Mar.  5   1  1.33   60  9.5   2.433   2.297    70   12.5     26.0  50.3  19:58 (146,-29)  

* 62P/Tsuchinshan 1


Very diffused and widely spreading visually.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  12 52.02   18 15.6   0.798   1.710   145   12.5      9.7 332.3   2:29 (180, 37)  
Mar.  5  12 48.90   19 11.4   0.810   1.745   151   12.8     10.8 312.1   1:59 (180, 36)  

* 9P/Tempel 1


It was 15.5 mag in early February, much fainter than expected. The brightening is much slower than expected. The ephemeris says it will reach to 9 mag in spring and summer. It may become a naked-eye object due to the Deep Impact mission on July 4.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  13 27.89   10  6.8   1.101   1.950   137   13.0      6.9  48.7   3:05 (180, 45)  
Mar.  5  13 29.61   10 41.4   1.022   1.912   143   12.6      5.6  20.7   2:39 (180, 44)  

* 32P/Comas Sola


It keeps observable at 12-13 mag in the evening sky until May.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   3 33.51   25 57.4   1.759   1.862    79   12.6     29.2  68.3  20:09 (139, 16)  
Mar.  5   3 48.19   27 10.8   1.813   1.852    76   12.6     30.8  70.6  19:58 (139, 14)  

* 141P/Machholz 2


Not yet observed in this return. The condition of this appearance is bad. It will appear at the evening low sky in March at 12.5 mag in the Northern Hemisphere, or in April at 14 mag in the Southern Hemisphere. Then it will become faint rapidly while locating very low in the evening.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  23 48.60    2 59.8   1.586   0.757    21   13.0     83.2  72.8  20:09 ( 86,-11)  
Mar.  5   0 26.57    5 49.3   1.542   0.754    24   12.6     85.8  73.9  19:58 ( 92, -8)  

* (3200) Phaethon


It passes the perihelion in early March and becomes bright as 12 mag. However it is not observable because too close to the sun.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  22 58.65  -12 37.5   0.782   0.232     6   19.1    121.0 257.0  20:09 ( 65,-12)  
Mar.  5  22 30.30   -8 19.4   1.080   0.174     8   12.7    103.7  30.4   4:23 (288,-10)  

* 49P/Arend-Rigaux


It brightened rapidly in January and reached to 13 mag. Now it is visible visually. It will keep bright at 13 mag in the evening sky until April.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   3 21.41    8 59.3   1.275   1.369    73   12.9     51.9  57.4  20:09 (125, 27)  
Mar.  5   3 42.57   12 10.3   1.305   1.372    71   13.0     52.6  59.6  19:58 (128, 25)  

* 29P/Schwassmann-Wachmann 1


It has been rather faint, diffused, and hard to see since mid January. It is already very low in the evening sky. It is not observable from March to May. It will appear at dawn again in June.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   0 34.10   11 53.0   6.508   5.734    35   13.8     11.3  68.6  20:09 (100, -7)  
Mar.  5   0 39.19   12 22.5   6.569   5.735    30   13.8     11.7  68.2  19:58 ( 99,-10)  

* C/2004 L1 ( LINEAR )


It will be at opposition and reach to 13.5 mag in March and April. Recent observations are a bit fainter than this ephemeris.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  14 29.52  -36 51.3   1.540   2.083   108   14.1     50.4 255.4   4:07 (  0, 88)  
Mar.  5  13 56.08  -38  3.5   1.384   2.069   120   13.9     65.6 263.1   3:07 (  0, 87)  

* C/2001 Q4 ( NEAT )


Completely diffused, but still bright at 12 mag visually. It keeps observable for a long time after this in the Northern Hemisphere. It is also visible in the morning low sky.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  23 39.87   54 38.7   4.355   4.034    64   13.9     15.5  99.5  20:09 (136,-35)  
Mar.  5  23 51.93   54 23.4   4.490   4.108    61   14.1     14.8  96.6  19:58 (136,-36)  

* C/2002 T7 ( LINEAR )


It will be getting fainter gradually until June when it becomes 17 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  10 11.53  -12 55.8   3.566   4.496   157   14.8     20.9 295.4  23:44 (180, 68)  
Mar.  5  10  2.79  -11 51.2   3.643   4.571   156   14.9     20.0 298.0  23:08 (180, 67)  

* C/2003 WT42 ( LINEAR )


It keeps 14.5 mag until June when it becomes too low in the evening.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   5 21.65   47 42.5   5.702   6.020   104   14.9      2.4 131.6  20:09 (168,  6)  
Mar.  5   5 23.28   47 31.5   5.776   5.995    97   14.9      3.3 118.1  19:58 (165,  5)  

* 161P/2004 V2 ( Hartley-IRAS )


It was 18.5 mag still in mid January. The brightening is slower than expected. The ephemeris says it will brighten rapidly after this, and reach to 8 mag from July to August. However, it is not observable for a while. In the Northern Hemisphere, it will appear at dawn at 11.5 mag in late May, then it keeps observable for a long time after that. In the Southern Hemisphere, it only appears in the morning very low sky from late April to mid June, but not observable when the comet is bright.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   0 15.15  -20 54.5   2.810   1.976    26   15.2     27.1  16.7  20:09 ( 70,  8)  
Mar.  5   0 19.20  -17 52.9   2.795   1.913    22   14.9     27.3  18.3  19:58 ( 71,  4)  

* (944) Hidalgo


It will be fading slowly until 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)  
Feb. 26   1 56.99   56 21.3   1.954   1.983    77   15.0     28.0  65.5  20:09 (147,-18)  
Mar.  5   2 19.72   57 39.0   2.006   1.996    75   15.1     29.5  68.5  19:58 (149,-19)  

* C/2004 B1 ( LINEAR )


It will reach to 9 mag in 2006 spring. In the Southern Hemisphere, it keeps observable until that. In the Northern Hemisphere, it will be too low in the evening in March. Then it keeps unobservable until 2006 March, except it appears very low in the morning at 12 mag from late August to early September. After 2006 March, northern people can observe it for a long time while it is getting fainter.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   4  9.70  -17 12.7   4.432   4.389    81   15.2      4.9 314.0  20:09 (110, 53)  
Mar.  5   4  8.38  -16 48.5   4.468   4.324    75   15.1      4.0 331.2  19:58 (106, 49)  

* 21P/Giacobini-Zinner


It will reach to 10 mag in June and July. It keeps locating rather low in the morning until that. It must have been already bright, but no observations have been reported since 2004 June.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  19 27.01    2 14.3   2.425   1.917    48   15.6     38.7  74.2   4:15 (258, 13)  
Mar.  5  19 44.72    3 32.4   2.322   1.854    50   15.2     40.4  73.0   4:23 (254, 16)  

* 121P/Shoemaker-Holt 2


It is brightest now, about 5 months after the perihelion passage. It is fainter than expected in this return, and reaches to 15.5 mag at best.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  10 18.99   32 31.1   1.923   2.856   155   15.4     10.5 302.5  23:52 (180, 22)  
Mar.  5  10 14.28   33  4.2   1.964   2.871   150   15.5      8.9 295.5  23:20 (180, 22)  

* C/2004 RG113 ( LINEAR )


It was reported as 14.5 mag visually.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   7 52.47   51 57.9   1.194   1.944   125   15.8     21.9 160.0  21:27 (180,  3)  
Mar.  5   7 58.92   49 28.1   1.225   1.942   122   15.8     24.3 155.5  21:06 (180,  6)  

* 117P/Helin-Roman-Alu 1


It will brighten gradually, then it will be 15 mag in spring and summer.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  15 57.71  -17 57.9   3.099   3.356    96   16.1      9.3 107.5   4:15 (231, 66)  
Mar.  5  16  1.66  -18 16.4   2.986   3.343   102   16.0      7.6 109.1   4:23 (215, 70)  

* C/2003 T3 ( Tabur )


It will be observable in good condition until 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)  
Feb. 26  10 28.37   42 41.2   3.142   4.002   146   16.2     15.1 257.2   0:06 (180, 12)  
Mar.  5  10 19.41   42 12.5   3.236   4.070   142   16.4     14.4 250.6  23:25 (180, 13)  

* 69P/Taylor


In its last return in 1997, it burst out after the perihelion passage and became extremely bright, reached to 11 mag. However, it is faint in this return. It will be fading gradually after this, and will be fainter than 18 mag in April.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   8 47.32   37 35.5   1.201   2.074   142   16.4      6.5 343.9  22:21 (180, 17)  
Mar.  5   8 47.03   38  9.6   1.267   2.094   135   16.6      3.6  13.5  21:53 (180, 17)  

* C/2004 K1 ( Catalina )


Appearing at dawn. It will be observable in good condition at 15.5 mag from April to June.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  18 16.46   -0 47.8   3.906   3.604    65   16.5      8.3 341.4   4:15 (248, 29)  
Mar.  5  18 14.77    0 10.4   3.761   3.583    72   16.4      9.9 332.2   4:23 (240, 35)  

* C/2004 U1 ( LINEAR )


It kept bright as 13.5 mag until early January since the outburst in late November. However, it is fading rapidly after that.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   2 46.10   50  7.7   2.785   2.786    79   16.4      9.8 230.6  20:09 (147, -9)  
Mar.  5   2 41.66   49 29.8   2.933   2.809    73   16.8      6.7 226.2  19:58 (144,-11)  

* 37P/Forbes


It keeps visible as bright as 12-13 mag for a long time from May to September. The condition is good in the Southern Hemisphere, but it locates very low in the Northern Hemisphere.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  15 13.00  -29  9.4   1.707   2.163   103   16.9     20.5 122.0   4:15 (233, 81)  
Mar.  5  15 22.10  -30 25.1   1.594   2.123   108   16.6     19.6 123.5   4:23 (201, 85)  

* 129P/Shoemaker-Levy 3


It keeps 17 mag until May when it becomes low in the evening.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   5 28.74   25 22.8   2.423   2.852   105   16.7      8.0 101.3  20:09 (163, 28)  
Mar.  5   5 33.33   25 12.4   2.508   2.846    99   16.8     10.0  98.1  19:58 (160, 27)  

* C/2005 B1 ( Christensen )


Recovery of a peculiar asteroid 2004 FS101 discovered in 2004 spring. It keeps observable at 15-16 mag for a long time from 2005 spring to 2006 winter. Because it moves in the northern sky, it keeps observable 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)  
Feb. 26  14 36.82   29  0.9   4.060   4.640   120   17.2     17.8 356.0   4:14 (180, 26)  
Mar.  5  14 35.70   31  7.7   3.963   4.596   124   17.1     18.6 351.1   3:45 (180, 24)  

* 164P/2004 Y1 ( Christensen )


It will be fainter than 18 mag in April.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  10 32.36   33 10.4   1.813   2.745   155   17.2     13.0 290.8   0:10 (180, 22)  
Mar.  5  10 25.81   33 35.5   1.876   2.786   151   17.3     11.4 283.0  23:31 (180, 21)  

* 162P/2004 TU12 ( Siding Spring )


Almost stellar. 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)  
Feb. 26   3 25.92   51 13.7   1.485   1.728    86   17.2     35.7  81.3  20:09 (153, -6)  
Mar.  5   3 52.24   51 41.2   1.581   1.778    84   17.4     35.0  85.2  19:58 (154, -5)  

* C/2004 D1 ( NEAT )


Because it moves in the northern sky, it keeps observable for a long time in the Northern Hemisphere. It will reach to 16 mag at best in early 2006.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   4 52.63   48 12.0   5.402   5.646    99   17.2      1.8  93.7  20:09 (163,  4)  
Mar.  5   4 54.36   48 11.5   5.478   5.621    93   17.2      3.1  90.6  19:58 (161,  3)  

* P/2004 VR8 ( LONEOS )


It keeps 17.5 mag until May when it becomes low in the evening sky. It will be observable again at 16.5 mag in 2006.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   3 38.79   22  4.3   2.781   2.788    80   17.4     15.0  60.4  20:09 (137, 19)  
Mar.  5   3 45.81   22 56.2   2.848   2.762    74   17.4     16.5  63.2  19:58 (136, 17)  

* P/2004 V5 ( LINEAR-Hill )


Split comets. It is observable in good condition at 17.5 mag until March.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   9 15.78   41 12.9   3.580   4.411   142   17.5      5.9 263.0  22:49 (180, 14)  
Mar.  5   9 12.42   41  4.2   3.631   4.411   137   17.5      5.2 250.6  22:18 (180, 14)  

* C/2004 X3 ( LINEAR )


It will be observable at 17.5 mag until May.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  10 56.67   -0 51.0   3.520   4.496   169   17.8     18.7 255.5   0:34 (180, 56)  
Mar.  5  10 48.13   -1 22.9   3.501   4.485   171   17.7     18.9 256.5  23:53 (180, 56)  

* C/2003 O1 ( LINEAR )


It keeps 18 mag until summer.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  16 39.57   38  1.7   7.061   7.212    94   17.8      8.0 332.7   4:15 (204, 12)  
Mar.  5  16 37.03   38 52.3   7.007   7.226    98   17.8      8.7 326.6   4:23 (197, 14)  

* C/2002 J5 ( LINEAR )


It keeps 18 mag until spring.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26  13 42.40   51 19.1   6.239   6.829   122   17.8     12.7 304.3   3:20 (180,  4)  
Mar.  5  13 34.12   52  6.1   6.245   6.855   124   17.8     13.0 298.7   2:44 (180,  3)  

* 163P/2004 V4 ( NEAT )


Although the condition is good, it will be fainter than 18 mag in late February.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Feb. 26   4 41.10   21 51.2   1.586   1.932    94   17.9     26.0  66.3  20:09 (151, 27)  
Mar.  5   4 53.57   23  0.9   1.662   1.940    90   18.0     27.2  69.6  19:58 (150, 26)  

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