Weekly Information about Bright Comets (2002 Apr. 20: North)

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Updated on April 24, 2002
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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/2002 F1 ( Utsunomiya )


It brightened rapidly after early April and reached to 4.5-5.0 mag in mid April. After now, it locates just on the horizon at dusk until early May in the Northern Hemisphere. In the Southern Hemisphere, it will be observable in May and June, but it only locates very low in the evening sky. It may vanish at the perihelion passage.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20   1 50.35   32 55.7   1.183   0.445    21    3.8    151.2  90.0   3:52 (226, -2)  
Apr. 27   3  8.45   29 59.8   1.233   0.451    20    4.0    135.8 109.1  20:13 (125,  2)  

* C/2002 C1 ( Ikeya-Zhang )


The return of comet in 1661 with 340 year period. It has been 0.5 mag brighter than this ephemeris since the perihelion passage.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20  22 25.39   59 27.1   0.428   0.882    61    4.5    125.8 291.1   3:52 (218, 39)  
Apr. 27  20 21.10   61 14.8   0.406   1.001    77    4.8    135.8 263.9   3:42 (210, 55)  

* 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 moving fast towards south and will be low in the evening sky in mid June.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20   9 16.04   59 52.8   0.558   1.154    90   10.1    177.7 174.5  20:06 (167, 65)  
Apr. 27   9 26.55   40 39.3   0.614   1.213    93   10.5    148.7 175.2  20:13 (113, 76)  

* 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. 20  19 25.65   45 17.8   1.404   1.672    86   10.5     69.9   1.9   3:52 (235, 68)  
Apr. 27  19 26.00   53  6.9   1.458   1.720    86   10.7     63.8 358.8   3:42 (214, 67)  

* C/2000 WM1 ( LINEAR )


It suddenly bursted out in late January and reached to 2.5 mag. Then it had been fading rapidly down to 9.5 mag. But the fading became slower in April. It must be 1 mag or more brighter than this ephemeris.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20  18 49.27   16 36.7   1.283   1.775   101   10.6     48.3 331.4   3:52 (317, 66)  
Apr. 27  18 36.94   21 20.0   1.318   1.880   107   11.0     46.7 325.3   3:42 (327, 74)  

* 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. 20   1 17.27   -2  3.1   2.541   1.598    15   12.0     42.9  75.2   3:52 (258,-20)  
Apr. 27   1 36.35   -0 48.6   2.570   1.639    17   12.0     41.6  75.7   3:42 (257,-20)  

* C/2002 G3 ( SOHO )


New comet. Appearing at dawn, but it must have vanished after the perihelion passage on Apr. 16.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20   1 13.30   17 11.1   0.932   0.195    10   12.2    145.4 289.4   3:52 (243, -8)  
Apr. 27   0 32.97   19 43.2   1.042   0.455    25   21.9     50.6 282.4   3:42 (249,  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. 20   0 39.65   68 46.9   3.965   3.545    58   12.9     19.8  30.9   3:52 (203, 28)  
Apr. 27   0 53.79   70 48.6   3.964   3.544    58   12.9     20.7  30.8   3:42 (201, 29)  

* 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. 20  21  1.82  -18 34.0   5.983   5.843    77   13.6      6.4  69.8   3:52 (310, 19)  
Apr. 27  21  4.55  -18 19.3   5.872   5.841    83   13.6      5.5  68.8   3:42 (313, 21)  

* 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. 20  19 42.76   -2 30.7   0.778   1.296    92   14.2     57.0 103.1   3:52 (317, 43)  
Apr. 27  20  9.00   -4  8.7   0.740   1.279    92   14.0     58.6 104.9   3:42 (316, 41)  

* 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. 20  20 26.09   18  9.2   2.992   2.955    78   14.6     11.8 303.2   3:52 (284, 50)  
Apr. 27  20 20.38   18 55.1   2.839   2.924    84   14.4     14.9 296.4   3:42 (288, 55)  

* 65P/Gunn


It will be observable at 15 mag until August when it becomes low in the evening sky. It is brighter than this ephemeris recently, 14.5 mag even by CCD.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20  11  1.79   20 14.6   2.553   3.266   127   15.0      5.0 246.2  21:08 (  0, 75)  
Apr. 27  11  0.01   19 56.8   2.609   3.245   121   15.0      4.0 219.8  20:38 (  0, 75)  

* 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. 20   9 55.78   69 53.5   5.007   5.097    89   15.1     11.6 174.2  20:06 (179, 55)  
Apr. 27   9 58.01   68 31.2   5.081   5.111    86   15.1     12.1 169.5  20:13 (174, 56)  

* C/2001 HT50 ( LINEAR-NEAT )


It will be 11 mag in 2003 February. Although it was reported as 13.5 mag visually, it is fainter than this ephemeris recently, fainter than 16 mag by CCD.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20  10  3.11   -5 37.5   4.474   5.098   123   15.1     14.8 299.7  20:09 (  0, 49)  
Apr. 27   9 57.46   -4 47.5   4.531   5.048   115   15.1     13.2 301.6  20:13 ( 14, 49)  

* C/2001 K5 ( LINEAR )


It will be 15 mag in spring and summer. It was a bit brighter than this ephemeris recently.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20  17  5.95    6 52.3   4.667   5.345   128   15.1     12.8 340.0   3:15 (  0, 62)  
Apr. 27  17  3.59    8 16.6   4.594   5.333   133   15.1     13.2 334.9   2:45 (  0, 63)  

* 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. 20  11 32.14   47 24.3   2.019   2.591   113   15.1     15.0 195.6  21:38 (180, 78)  
Apr. 27  11 30.21   45 40.4   2.124   2.640   109   15.4     15.3 186.4  21:09 (180, 79)  

* 116P/Wild 4


It will be 10.5 mag in 2003 spring. It was 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. 20   6 16.59   26 39.8   3.132   2.840    64   15.3     17.6  94.2  20:06 ( 96, 42)  
Apr. 27   6 26.05   26 29.6   3.191   2.814    59   15.3     18.8  94.9  20:13 ( 99, 37)  

* 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. 20  11 41.69    8 54.5   1.777   2.642   142   15.4     10.1 290.1  21:47 (  0, 64)  
Apr. 27  11 37.71    9 14.2   1.796   2.601   134   15.3      7.5 286.5  21:16 (  0, 64)  

* 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. 20  15 58.64  -39  0.3   2.290   3.130   140   15.5      7.9 230.5   2:08 (  0, 16)  
Apr. 27  15 54.31  -39 32.9   2.185   3.074   146   15.4      9.3 242.7   1:36 (  0, 15)  

* P/2001 MD7 ( LINEAR )


Fading rapidly after February. The observation season will end soon.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20   5 20.35   18 10.2   2.546   2.067    51   15.9     33.6  78.8  20:06 ( 94, 27)  
Apr. 27   5 36.35   18 50.9   2.661   2.124    48   16.1     32.5  80.7  20:13 ( 97, 23)  

* 77P/Longmore


It is brighter than this ephemeris recently, 15.5 mag.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20  10 29.53   24 58.7   1.837   2.485   119   15.9     13.5 192.1  20:36 (  0, 80)  
Apr. 27  10 28.82   23 23.4   1.894   2.468   113   15.9     13.9 179.8  20:13 (  7, 78)  

* 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. 20  15 54.16  -16 33.9   2.961   3.861   149   16.1      6.9 277.4   2:03 (  0, 38)  
Apr. 27  15 50.50  -16 27.1   2.922   3.869   157   16.1      8.2 277.3   1:32 (  0, 39)  

* 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. 20  10 34.98   23 15.2   1.002   1.746   120   16.2     24.5 135.4  20:42 (  0, 78)  
Apr. 27  10 43.91   21 13.8   1.088   1.787   117   16.4     25.1 133.4  20:23 (  0, 76)  

* 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. 20  12  9.56  -12 57.2   4.672   5.600   155   16.8     14.1 276.8  22:15 (  0, 42)  
Apr. 27  12  3.18  -12 45.5   4.774   5.649   147   16.9     12.8 277.4  21:41 (  0, 42)  

* 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. 20   9 13.56   16 52.1   6.511   6.856   105   16.8      6.3 305.6  20:06 ( 32, 69)  
Apr. 27   9 11.33   17 16.2   6.665   6.887    98   16.9      5.1 309.0  20:13 ( 52, 64)  

* 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. 20  18 38.01  -16 37.6  10.970  11.359   110   17.1      0.7 335.7   3:52 (344, 37)  
Apr. 27  18 37.73  -16 33.5  10.877  11.373   117   17.1      1.0 302.8   3:42 (349, 38)  

* 57P/du Toit-Neujmin-Delporte


Not yet observed in this return. It is getting brighter in the morning sky. It will reach to 15.5 mag in July and August. It bursted out and became 6 mag brighter than this ephemeris in the previous return in 1996.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20  18 59.26  -19 10.9   1.434   1.960   105   17.7     23.9  78.9   3:52 (339, 33)  
Apr. 27  19 10.52  -18 37.0   1.344   1.932   109   17.4     22.8  77.2   3:42 (340, 34)  

* 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. 20   8 58.90   20  4.1   3.081   3.429   101   17.6      6.8 106.4  20:06 ( 46, 70)  
Apr. 27   9  2.52   19 48.9   3.182   3.432    95   17.7      8.4 106.8  20:13 ( 59, 65)  

* P/2001 TU80 ( LINEAR-NEAT )


It bursted out and reached to 15 mag in early January. It is getting fainter rapidly these days.
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr. 20   8 59.09   23 24.8   1.796   2.216   100   17.7     18.9 107.4  20:06 ( 52, 73)  
Apr. 27   9  8.53   22 42.7   1.898   2.243    96   18.0     20.2 108.2  20:13 ( 62, 68)  

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