Weekly Information about Bright Comets (2002 Apr. 6: South)

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Updated on April 9, 2002
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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/2002 C1 ( Ikeya-Zhang )


The return of comet in 1661 with 340 year period. Strongly condensed with a stellar nucleus. Long tail over 3 degree is visible. It was reported as 3.0-3.5 mag by naked eye, brighter than this ephemeris.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6   0 43.39   43 31.3   0.538   0.660    37    3.8    100.0 323.4   4:52 (237,-33)  
Apr. 13  23 51.93   52 27.0   0.472   0.767    47    4.1    112.4 310.4   4:57 (221,-23)  

* C/2002 F1 ( Utsunomiya )


New comet. Though locating low now, it is strongly condensed and easy to see. It will be 6.5 mag in late April. In the Northern Hemisphere, it is observable only until mid April being very low in the morning sky. After the perihelion passage, it will be observable in the Southern Hemisphere, but it locates very low in the evening sky. It will locate high after August, but will be fainter than 15 mag at that time.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  23 23.37   23 26.4   1.255   0.610    28    7.8    127.2  59.3   4:52 (247, -8)  
Apr. 13   0 28.85   30  8.4   1.189   0.507    24    6.9    146.6  71.6   4:57 (245,-18)  

* C/2000 WM1 ( LINEAR )


It suddenly bursted out in late January and reached to 2.5 mag. Then it is fading rapidly, and now it is 9.0 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  19  7.54    6  6.3   1.246   1.559    87    9.7     49.2 342.3   4:52 (209, 45)  
Apr. 13  18 59.47   11 29.3   1.260   1.668    94   10.1     49.1 337.1   4:57 (193, 43)  

* C/2001 OG108 ( LONEOS )


After it brightened rapidly and reached to 10 mag in February, it did not brightened more and kept 10 mag all over though it became closer to the earth. It may fade out very soon after this. It is observable all through a night in the Northern Hemisphere.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  22 29.61   81 17.5   0.638   1.057    76   10.0    133.4  14.7   4:52 (190,-31)  
Apr. 13   8 35.23   80 19.9   0.568   1.101    84    9.9    169.7 164.8  19:16 (180,-24)  

* C/2002 E2 ( Snyder-Murakami )


New comet. It will move northwards after this. It keeps observable until it fades out in the Northerm Hemisphere. It keeps brighter than 12 mag until May. It will approach to C/2002 C1 ( Ikeya-Zhang ) around May 1.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  19 18.89   28 11.5   1.368   1.588    82   10.2     75.3   6.9   4:52 (202, 23)  
Apr. 13  19 23.08   36 53.3   1.373   1.628    84   10.3     74.0   4.6   4:57 (193, 17)  

* 6P/d'Arrest


The condition in this return is bad. It is not observable until June in the Southern Hemisphere, until August in the Northern Hemisphere.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6   0 37.26   -4 43.8   2.485   1.522    12   12.3     45.6  74.9   4:52 (281, -7)  
Apr. 13   0 57.57   -3 21.8   2.513   1.559    13   12.1     44.3  75.0   4:57 (278, -5)  

* C/2000 SV74 ( LINEAR )


It will be observable at 13 mag until September. It is fainter than 14 mag by CCD.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6   0 16.02   65  1.7   3.958   3.551    59   12.9     17.9  32.3   4:52 (210,-34)  
Apr. 13   0 27.19   66 51.0   3.963   3.548    58   12.9     18.9  31.4   4:57 (208,-32)  

* 29P/Schwassmann-Wachmann 1


Takuo Kojima reported that it was in outburst at 14.4 mag on Mar. 28.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  20 55.07  -19  7.9   6.196   5.847    65   13.7      8.1  71.2   4:52 (261, 46)  
Apr. 13  20 58.65  -18 50.2   6.091   5.845    71   13.7      7.3  70.5   4:57 (256, 52)  

* 7P/Pons-Winnecke


It was as faint as 16.5 mag in mid March. It may reach only to 13.5 mag in May.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  18 52.17    0  3.2   0.873   1.347    91   14.8     53.5  99.9   4:52 (206, 52)  
Apr. 13  19 17.12   -1  7.2   0.823   1.319    92   14.5     55.3 101.4   4:57 (204, 54)  

* 19P/Borrelly


Fading now. It is observable in good condition until to fade out.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  11 41.30   50 28.6   1.827   2.492   120   14.7     14.5 217.3  22:42 (180,  5)  
Apr. 13  11 35.80   49  1.5   1.920   2.542   117   14.9     14.7 205.9  22:09 (180,  6)  

* C/2001 N2 ( LINEAR )


Getting higher in the morning sky. It will be 13 mag in June and July.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  20 32.90   16 43.9   3.289   3.019    65   14.9      7.1 322.3   4:52 (224, 25)  
Apr. 13  20 30.17   17 25.1   3.143   2.986    71   14.7      9.2 311.6   4:57 (216, 29)  

* 15P/Finlay


It bursted out in early February and reached to 13.5 mag. Then it did not become so fainter. It must be brighter than this ephemeris. But the condition is worst. It always locates very low in the evening sky.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6   2 46.38   17  1.3   2.097   1.306    28   14.8     56.0  70.7  19:12 (109, -2)  
Apr. 13   3 11.89   19  0.6   2.167   1.364    27   15.2     53.4  72.7  19:03 (112, -2)  

* C/1999 U4 ( Catalina-Skiff )


It is observable until autumn at 15 mag. It was reported as 14 mag visually, but as 16 mag by CCD, so there is a large difference.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6   9 55.62   72 27.9   4.866   5.069    95   15.0     10.5 185.7  20:57 (180,-17)  
Apr. 13   9 54.90   71 12.7   4.935   5.083    92   15.0     11.1 179.6  20:29 (180,-16)  

* 65P/Gunn


It will be observable at 15 mag until August when it becomes low in the evening sky. It is already brighter than 15.0 mag even by CCD, and observed visually these days.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  11  8.19   20 26.7   2.464   3.309   141   15.0      8.1 272.3  22:09 (180, 35)  
Apr. 13  11  4.54   20 24.8   2.504   3.288   134   15.0      6.5 262.4  21:38 (180, 35)  

* C/2001 HT50 ( LINEAR-NEAT )


It will be 11 mag in 2003 February. Although it was reported as 13.5 mag visually, it was reported as 15.5 mag by CCD, a bit fainter than this ephemeris.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  10 16.63   -7 24.2   4.396   5.200   139   15.2     17.6 296.2  21:17 (180, 62)  
Apr. 13  10  9.52   -6 30.1   4.428   5.149   131   15.1     16.3 297.9  20:43 (180, 61)  

* C/2001 K5 ( LINEAR )


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)  
Apr.  6  17  8.85    4  4.7   4.847   5.372   116   15.2     11.9 351.6   4:13 (180, 51)  
Apr. 13  17  7.72    5 28.0   4.752   5.359   122   15.2     12.4 345.5   3:44 (180, 50)  

* 116P/Wild 4


It will be 10.5 mag in 2003 spring. It was a bit fainter than this ephemeris, around 16 mag recently.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6   5 59.63   26 55.1   3.004   2.892    73   15.4     14.8  93.5  19:12 (149, 21)  
Apr. 13   6  7.75   26 48.2   3.070   2.866    68   15.4     16.3  93.8  19:03 (147, 20)  

* P/2001 MD7 ( LINEAR )


Fading rapidly after February. It will be fainter than 16 mag in May when it becomes low.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6   4 47.16   16 20.5   2.316   1.954    56   15.4     36.2  75.0  19:12 (128, 20)  
Apr. 13   5  3.95   17 20.3   2.431   2.010    53   15.7     34.8  76.9  19:03 (129, 19)  

* 22P/Kopff


The condition in this return is bad. We can observe it only until August before perihelion passage when it becomes to 13 mag in the evening sky.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  11 52.35    7 48.9   1.770   2.725   158   15.7     13.9 294.4  22:53 (180, 47)  
Apr. 13  11 46.65    8 25.7   1.768   2.684   150   15.5     12.3 292.5  22:20 (180, 47)  

* 28P/Neujmin 1


It will reach to 13 mag at the end of this year. In the northern hemisphere, it keeps low in the south after this.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  16  3.30  -37 42.2   2.530   3.241   127   15.8      6.2 195.9   3:07 (  0, 87)  
Apr. 13  16  1.64  -38 23.0   2.405   3.185   134   15.7      6.8 214.8   2:38 (  0, 87)  

* 2001 TX16


Asteroid with a cometary orbit of 6.8 year period. Fading now.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  10 18.60   27 19.2   0.850   1.669   128   15.7     22.5 140.0  21:20 (180, 28)  
Apr. 13  10 26.51   25 17.5   0.923   1.707   124   16.0     23.6 137.6  21:01 (180, 30)  

* 77P/Longmore


Now it is at the peak.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  10 35.52   27 50.0   1.743   2.519   131   15.9     14.0 217.8  21:36 (180, 27)  
Apr. 13  10 31.75   26 28.2   1.786   2.501   125   15.9     13.6 205.1  21:05 (180, 29)  

* 74P/Smirnova-Chernykh


It keeps brighter than 17 mag until August.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  15 59.37  -16 43.7   3.075   3.845   134   16.1      3.7 277.3   3:04 (180, 72)  
Apr. 13  15 57.16  -16 39.6   3.012   3.853   142   16.1      5.4 277.5   2:34 (180, 72)  

* C/1999 T2 ( LINEAR )


Fading. It will be about 18 mag in June when it becomes low in the evening.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  12 23.97  -13 19.0   4.517   5.502   168   16.7     15.9 274.9  23:24 (180, 68)  
Apr. 13  12 16.53  -13  8.6   4.585   5.551   162   16.8     15.2 275.9  22:49 (180, 68)  

* C/2001 B2 ( NEAT )


Fading very slowly. It was brighter than the ephemeris recently, reported around 16 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6   9 19.78   15 53.0   6.219   6.794   121   16.7      9.0 301.9  20:21 (180, 39)  
Apr. 13   9 16.37   16 24.4   6.361   6.825   113   16.8      7.7 303.4  19:50 (180, 39)  

* P/2001 TU80 ( LINEAR-NEAT )


It bursted out and reached to 15 mag in early January. It is getting fainter rather rapidly these days.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6   8 42.11   24 33.4   1.602   2.164   110   16.9     15.6 105.2  19:44 (180, 30)  
Apr. 13   8 50.23   24  1.8   1.697   2.189   105   17.2     17.4 106.4  19:25 (180, 31)  

* 95P/(2060) Chiron


It keeps 17 mag locating at the same altitude until October in the Northerm Hemisphere.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  18 37.69  -16 47.0  11.169  11.332    96   17.1      1.2  53.0   4:52 (214, 69)  
Apr. 13  18 38.00  -16 42.2  11.068  11.346   103   17.1      0.7  26.1   4:57 (193, 71)  

* P/2002 CW134 ( LINEAR )


New periodic comet. Now it is at the peak, and it will fade out soon.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6  12 25.36  -18 51.7   0.883   1.867   165   17.4     15.8 239.3  23:26 (180, 74)  
Apr. 13  12 19.06  -19 41.8   0.903   1.879   160   17.5     13.3 241.7  22:52 (180, 75)  

* 31P/Schwassmann-Wachmann 2


Already passed the peak and fading now.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  6   8 54.20   20 23.0   2.888   3.423   114   17.5      3.0 104.8  19:56 (180, 35)  
Apr. 13   8 56.10   20 15.6   2.983   3.426   107   17.6      4.9 105.9  19:30 (180, 35)  

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