Weekly Information about Bright Comets (2000 Apr. 8: North)

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 Updated on May 2, 2000
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Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Northern Hemisphere.

Please see also the Comet Rendezvous Calendar, Latest Pictures of Comets.

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* C/1999 S4 ( LINEAR )

 Image: 2000 Feb. 12
It will be 3 mag in 2000 July, but it is a few mag fainter actually. Not observable now. In the Northern Hemisphere, it will appear at dawn in late May as 10 mag, then keeps observable until early August. In the Southern Hemisphere, it locates very low between late May and mid June, however, it locates high after late July. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   1 40.17   26 23.6   2.929   2.023    20   12.4      6.0  59.7  19:53 (123,  0)  
Apr. 15   1 42.98   26 47.5   2.864   1.928    17   12.1      6.8  55.9  20:01 (128, -5)

* C/1997 BA6 ( Spacewatch )

 Image: 1998 Dec. 5
Only southern people can observe it. Recently it was observed as 12 mag. It will appear again in 2000 August as 13 mag. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  22 43.07  -51 52.7   3.924   3.647    66   13.0      9.5  48.0   4:10 (319,-22)  
Apr. 15  22 48.00  -51 11.4   3.876   3.669    70   13.0      8.1  48.2   3:59 (319,-20)

* 9P/Tempel 1
Only observable in the Southern Hemisphere. In the Northern Hemisphere, it appears at dawn in 2000 June, when it will be already fainter than 15 mag. It was fainter than 12.0 mag on Feb. 11 by KenIchi Kadota, Ageo. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  22 16.89  -17 58.6   2.257   1.773    49   13.5     34.7  75.3   4:10 (293,  1)  
Apr. 15  22 32.93  -16 56.7   2.242   1.808    52   13.7     33.2  74.8   3:59 (292,  2)

* C/1999 T1 ( McNaught-Hartley )
It is expected to be bright as 7 mag in late 2000. Northern people cannot observe it until December. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   2 14.34  -32 22.5   4.226   3.554    42   13.6     16.4  77.8  19:53 ( 68,-27)  
Apr. 15   2 23.44  -32  0.0   4.139   3.480    43   13.5     17.3  80.3  20:01 ( 71,-31)

* C/1995 O1 ( Hale-Bopp )
Only southern people can observe it. Northern people can never see it again. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   4 44.21  -71  9.2  10.850  10.827    86   13.5      4.7  38.2  19:53 ( 19,-25)  
Apr. 15   4 48.68  -70 44.5  10.883  10.875    86   13.5      4.7  45.0  20:01 ( 21,-27)

* 29P/Schwassmann-Wachmann 1

 Image: 1999 June 12
The altitude will be 23 deg at best in the Northern Hemisphere. Now it is not in outburst. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  17 18.91  -32  2.9   5.555   6.075   116   13.6      1.1 208.6   4:10 (359, 23)  
Apr. 15  17 18.30  -32  9.3   5.457   6.073   123   13.6      1.9 243.1   3:45 (  0, 23)

* C/1999 K5 ( LINEAR )

 Image: 1999 July 31
It will reach to 13.5 mag in June, but will not be observable in the Northern Hemisphere. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  21 52.12  -55 18.9   3.486   3.360    74   14.0     24.5 130.1   4:10 (326,-18)  
Apr. 15  22  8.13  -57 12.6   3.386   3.344    79   13.9     25.6 131.2   3:59 (328,-19)

* 64P/Swift-Gehrels
Not observable at all in this return. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   1 19.17   13 31.6   2.339   1.350     6   14.3     53.1  67.4  19:53 (116,-12)  
Apr. 15   1 43.04   15 50.7   2.334   1.342     6   14.2     53.5  68.7  20:01 (120,-12)

* C/1999 K8 ( LINEAR )

 Image: 1999 Dec. 30
Because it is far away, it keeps 14 mag until late 2000. It will not be observable until May. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   0  7.15   13 24.7   5.155   4.203    16   14.3     17.2  85.8   4:10 (252, -2)  
Apr. 15   0 15.30   13 33.3   5.133   4.201    19   14.3     16.9  85.9   3:59 (253, -1)

* 63P/Wild 1

 Image: 2000 Feb. 11
It is 1 mag fainter than this ephemeris by CCD. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  13 52.64  -31 10.9   1.259   2.202   153   14.8     15.9 237.5   0:48 (  0, 24)  
Apr. 15  13 45.13  -32  2.3   1.273   2.233   157   15.0     15.1 245.9   0:13 (  0, 23)

* C/1999 T2 ( LINEAR )

 Image: 2000 Jan. 8
It will be 13 mag at good position in 2000 September. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  22 41.69   34 25.9   4.435   3.769    43   15.0     13.4  14.0   4:10 (244, 25)  
Apr. 15  22 43.31   36  0.4   4.347   3.730    46   14.9     14.2   9.7   3:59 (244, 29)

* C/1999 H3 ( LINEAR )

 Image: 2000 Feb. 17
It will fade out gradually after this, but it can be observed as 17.5 mag in 2001 spring. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  11 49.10   41 40.7   3.402   4.094   127   15.1     24.5 255.0  22:39 (180, 83)  
Apr. 15  11 35.14   40 48.8   3.500   4.126   122   15.2     22.8 248.8  21:58 (180, 84)

* C/1999 J2 ( Skiff )

 Image: 2000 Jan. 28
It will be observable as 15 mag with a good condition. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  16 25.55   38  4.8   6.621   7.110   115   15.1      7.3 285.3   3:20 (180, 87)  
Apr. 15  16 21.11   38 16.0   6.582   7.110   118   15.1      8.0 279.2   2:48 (180, 87)

* 74P/Smirnova-Chernykh

 Image: 2000 Jan. 15
Actually, it will be brighter than this ephemeris. It is 14 mag visually. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   7  3.81   27 16.3   3.613   3.677    85   16.1      9.3  98.4  19:53 ( 81, 64)  
Apr. 15   7  9.01   27  5.9   3.709   3.671    80   16.1     10.7  98.5  20:01 ( 86, 58)

* 95P/(2060) Chiron

 Image: 1999 June 12
No observations reported since 1999 June. The altitude will be 38 deg at best after this in the Northern Hemisphere. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  17  6.11  -17 49.9   9.424   9.980   121   16.4      1.3 305.8   4:00 (  0, 37)  
Apr. 15  17  5.45  -17 44.5   9.340   9.992   128   16.3      1.8 294.9   3:32 (  0, 37)

* C/1998 M5 ( LINEAR )

 Image: 2000 Jan. 28
Gradually fading. The altitude in the Northerm Hemisphere will not high after this. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   9 12.40  -20 15.3   4.567   5.162   121   16.4      7.2 302.1  20:04 (  0, 35)  
Apr. 15   9  9.78  -19 49.0   4.708   5.223   115   16.5      5.8 309.3  20:01 (  8, 35)

* P/2000 C1 ( Hergenrother )

 Image: 2000 Feb. 11
It keeps 16.5-17 mag until April. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  11 53.16   11  5.9   1.155   2.101   153   16.5      5.7 295.9  22:44 (  0, 66)  
Apr. 15  11 51.26   11 16.8   1.192   2.105   146   16.6      2.9 282.6  22:15 (  0, 66)

* C/1999 L3 ( LINEAR )

 Image: 2000 Feb. 17
It faded out extremely rapidly in February and reached to 15 mag by CCD at the end of February. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   5 23.21   30 23.8   2.540   2.282    63   16.5      5.4 272.2  19:53 (100, 44)  
Apr. 15   5 21.05   30 26.1   2.720   2.323    56   16.8      2.8 279.2  20:01 (104, 37)

* C/1998 T1 ( LINEAR )

 Image: 2000 Feb. 11
Gradually fading. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  11 40.28   -4 54.7   2.909   3.856   158   16.6     27.0 298.9  22:30 (  0, 50)  
Apr. 15  11 29.90   -3 27.3   3.032   3.924   148   16.7     23.9 299.8  21:53 (  0, 52)

* C/1999 E1 ( Li )

 Image: 2000 Jan. 28
It keeps 16 mag at good position until 2000 May. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  10  5.56   38 15.4   4.495   5.041   117   16.8      1.7 299.0  20:57 (180, 87)  
Apr. 15  10  5.02   38 18.3   4.616   5.072   111   16.9      0.3 272.7  20:29 (180, 87)

* C/1999 K2 ( Ferris )

 Image: 1999 May 31
Fading gradually. It keeps 17-18 mag at good position until October. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  20 35.57   22 39.4   6.232   5.914    67   17.2     12.0  12.7   4:10 (272, 45)  
Apr. 15  20 36.66   24  1.9   6.173   5.937    71   17.2     12.0   7.8   3:59 (273, 49)

* 4P/Faye

 Image: 2000 Feb. 9
It was fading gradually after November and still keeps 16.5 mag. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   9 27.75    6 52.4   2.648   3.305   123   17.3      3.5  13.3  20:19 (  0, 62)  
Apr. 15   9 28.61    7 13.5   2.773   3.344   116   17.5      3.8  46.9  20:01 (  4, 62)

* C/1999 F2 ( Dalcanton )

 Image: 1999 June 30
It keeps the good condition until autumn. It will fade out gradually. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  17 32.42   24  9.8   6.163   6.549   108   17.4      8.6 357.7   4:10 (341, 79)  
Apr. 15  17 31.98   25  8.8   6.137   6.584   112   17.4      8.4 350.7   3:58 (  0, 80)

* C/1999 N4 ( LINEAR )
It keeps 17 mag at good position until August. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8  18  6.15    1 13.3   5.166   5.514   105   17.5     11.2 298.0   4:10 (338, 54)  
Apr. 15  18  1.12    1 50.2   5.049   5.511   112   17.4     12.8 294.3   3:59 (347, 56)

* (10199) Chariklo

 Image: 1999 Jan. 22
A Centaur asteroid. The perihelion passage is in 2004. It will keep the current brightness over 10 years after this. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   9 37.73    0 48.1  12.707  13.333   126   17.5      1.7 299.7  20:29 (  0, 56)  
Apr. 15   9 37.16    0 53.6  12.798  13.330   120   17.6      1.2 306.6  20:01 (  0, 56)

* 1999 LD31
Retrograde asteroid. It will be fainter and lower rapidly after this. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   8 45.72   30 18.3   2.347   2.806   106   17.6     25.0 257.0  19:53 ( 38, 84)  
Apr. 15   8 34.23   29 36.6   2.526   2.844    97   17.8     19.5 251.7  20:01 ( 72, 76)

* D/1984 H1 ( Kowal-Mrkos )
Only 8 observations reported during one month in 1984. The orbit and brightness are extremely uncertain. The ephemeris says it is highest and brightest until April. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   8 51.94   10 49.4   2.460   3.006   113   17.7      3.9  79.3  19:53 (  6, 66)  
Apr. 15   8 54.30   10 52.3   2.528   2.987   107   17.8      6.1  89.1  20:01 ( 24, 64)

* 114P/Wiseman-Skiff

 Image: 2000 Feb. 12
Rapidly fading now. It may be brighter than this ephemeris. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   6 31.68   10  5.9   1.679   1.796    79   17.8     35.0  98.6  19:53 ( 63, 48)  
Apr. 15   6 47.99    9 28.1   1.769   1.830    77   18.2     34.7  99.1  20:01 ( 66, 44)

* 59P/Kearns-Kwee

 Image: 1999 Dec. 29
Although it had been 16 mag for a while, it is fading out rapidly now. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   8  8.65   18 38.3   2.414   2.796   101   17.8     11.7 112.7  19:53 ( 39, 70)  
Apr. 15   8 14.35   18  5.8   2.530   2.823    96   18.0     13.2 111.1  20:01 ( 52, 65)

* P/2000 B3 ( LINEAR )
Brightened gradually and reached to 17 mag. 
Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1    Mot.(') p.a.  Best Time(A, h)  
Apr.  8   8  6.93   25 33.8   1.310   1.781    99   18.1     31.5 119.7  19:53 ( 54, 75)  
Apr. 15   8 21.13   23 44.4   1.386   1.803    96   18.3     32.0 119.1  20:01 ( 60, 70)

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