Weekly Information about Bright Comets (2017 Dec. 30: North)

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 Updated on December 31, 2017
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Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Northern Hemisphere.
Azimuth indicates 0 for south, 90 for west, 180 for north, 270 for east.

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* C/2017 T1 ( Heinze )

Now it is very bright as 10.3 mag (Dec. 27, Katsumi Yoshimoto). It is approaching to Earth down to 0.2 a.u. now. In the Northern Hemisphre, it stays observable in good condition until January, but it will be extremely low after that. In the Southern Hemisphere, it is not observable from January to mid March, but it stays observable in good condition except for that period. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   8  2.96   34 37.9   0.277   1.245   157   10.9   1:33 (  0, 88)  
Jan.  6   4  4.99   68 14.0   0.226   1.133   126   10.2  20:25 (180, 56)

* 62P/Tsuchinshan 1

Now it is very bright as 10.4 mag (Dec. 15, Marco Goiato). It is observable in good condition in the Northern Hemisphere. It locates low in the Southern Hemisphere. It will be fading after January. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  13 10.54    3 52.6   1.206   1.468    83   10.9   5:37 (333, 56)  
Jan.  6  13 26.49    3  6.2   1.187   1.496    86   11.1   5:38 (339, 56)

* C/2016 R2 ( PanSTARRS )

Now it is bright as 10.7 mag (Dec. 27, Katsumi Yoshimoto). It will stay bright as 11 mag for a long time until spring. In the Southern Hemisphere, it stays observable in good condition until February. In the Northern Hemispehre, it stays observable for a long time after this until the comet fades out. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   4 26.43   13 32.6   2.063   2.943   147   11.3  21:50 (  0, 69)  
Jan.  6   4 18.51   15 37.3   2.089   2.910   139   11.2  21:14 (  0, 71)

* C/2017 O1 ( ASASSN )

It brightened up to 8.1 mag in autumn (Oct. 3, Juan Jose Gonzalez). Now it is fading. It has already faded down to 12.2 mag (Dec. 23, Carlos Labordena). It is observable all night in the Northern Hemisphere. In the Northern Hemisphere, it stays observable in excellent condition for a long time. In the Southern Hemisphere, it will never be observable again after this. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  23 56.70   85 44.3   1.213   1.829   112   12.0  18:28 (179, 39)  
Jan.  6   0 39.95   85 29.4   1.281   1.884   111   12.3  18:32 (179, 39)

* 185P/Petriew

Now it is 15.8 mag (Dec. 17, Ken-ichi Kadota). It will brighten very rapidly, and brighten up to 11 mag from January to February. In the Northern Hemisphere, it stays observable for a long time in the evening sky. In the Southern Hemisphere, it locates extremely low at the highlight. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  21 19.19   -9 51.4   1.534   1.025    41   12.8  18:28 ( 61, 21)  
Jan.  6  21 47.58   -8 46.5   1.491   0.987    40   12.3  18:32 ( 62, 21)

* 24P/Schaumasse

Now it is 12.0 mag (Dec. 18, Seiichi Yoshida). It is observable in good condition in the Northern Hemisphere. It locates very low for a long time in the Southern Hemisphere. It will be fading after this. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  14 35.75   -4 22.0   1.496   1.330    60   12.4   5:37 (312, 38)  
Jan.  6  14 54.85   -5 47.5   1.502   1.369    62   13.0   5:38 (315, 38)

* C/2015 V2 ( Johnson )

It brightened up to 7.1 mag from May to June (June 21, Juan Jose Gonzalez). Now it is fading. It has already faded down to 13.5 mag (Dec. 7, Chris Wyatt). In the Southern Hemisphere, it stays observable for a long time after this. It will never be observable again in the Northern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  20 57.95  -54 47.6   3.671   3.001    41   13.1  18:28 ( 31,-14)  
Jan.  6  21 17.05  -54  3.2   3.756   3.068    39   13.3  18:32 ( 33,-15)

* C/2016 N6 ( PanSTARRS )

Now it is 13.6 mag (Dec. 18, Toshihiko Ikemura, Hirohisa Sato). It is expected to brighten up to 12 mag from 2018 to 2019. In the Northern Hemisphere, it stays observable in good condition while the comet will be brightening gradually. In the Southern Hemisphere, it is not observable until 2018 October. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  15 41.31   52 47.9   3.314   3.372    84   13.5   5:37 (228, 49)  
Jan.  6  15 44.29   54 39.7   3.207   3.330    88   13.3   5:38 (224, 53)

* 29P/Schwassmann-Wachmann 1

Now it is 14.7 mag (Dec. 15, Toshihiko Ikemura, Hirohisa Sato). 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  21 33.98  -11 57.8   6.472   5.801    43   13.8  18:28 ( 56, 22)  
Jan.  6  21 38.77  -11 31.1   6.545   5.800    37   13.8  18:32 ( 62, 17)

* C/2016 M1 ( PanSTARRS )

Now it is 13.7 mag (Nov. 14, Gabor Santa). It is expected to brighten up to 10 mag in summer in 2018. In the Northern Hemisphere, it stays observable until 2018 summer while the comet will be brightening. However, it will be extremely low from December to January. In the Southern Hemisphere, it is hardly observable in 2017, but it will be observable in good condition in 2018. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  18 15.50    8 24.9   4.110   3.317    31   14.0   5:37 (262,  4)  
Jan.  6  18 22.44    7 23.8   4.057   3.264    31   13.9   5:38 (266,  8)

* C/2017 K6 ( Jacques )

Now it is 14.0 mag (Dec. 13, Chris Wyatt). It stays 14 mag for a while. In the Southern Hemisphere, it stays observable in good condition until spring in 2018. It is getting higher gradually also in the Northern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   1 45.33  -45 42.1   1.836   2.003    84   14.1  19:10 (  0, 10)  
Jan.  6   1 52.51  -40 43.1   1.858   2.003    83   14.1  18:49 (  0, 15)

* C/2015 O1 ( PanSTARRS )

Now it is 14.2 mag (Nov. 14, Artyom Novichonok). It will be observable at 14 mag for a long time from 2017 to 2018. In the Southern Hemisphere, it will be hardly observable after this. It will be extremely low from November to December in the Northern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  16 31.73   22 48.7   4.234   3.757    55   14.4   5:37 (263, 32)  
Jan.  6  16 33.77   23 57.8   4.152   3.750    59   14.4   5:38 (266, 39)

* 174P/(60558) 2000 EC98 ( Echeclus )

Brian Skiff found a bright outburst on Dec. 7. It brightened up to 13.2 mag (Dec. 11, Seiichi Yoshida). It stays bright as 13.3 mag still now (Dec. 20, Toshihiko Ikemura, Hirohisa Sato). This is the 4th outburst following those in January 2006, May 2011 and August 2016. It stays observable in good condition for a while. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   2 35.62   11 15.6   6.785   7.350   121   15.1  20:00 (  0, 66)  
Jan.  6   2 35.29   11 16.4   6.904   7.368   114   15.4  19:32 (  0, 66)

* 240P/NEAT

It brightened very rapidly up to 13.8 mag in August (Aug. 22, kunihiro Shima). After that, it is fading gradually. Now it is 15.0 mag (Dec. 19, Martin Masek). It is observable in excellent condition in the Southern Hemisphere. It stays low for a while in the Northern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   0 16.44  -19 24.8   2.378   2.381    78   15.3  18:28 ( 13, 35)  
Jan.  6   0 23.85  -17 20.1   2.434   2.358    73   15.4  18:32 ( 21, 35)

* 145P/Shoemaker-Levy 5

Now it is 15.6 mag (Dec. 19, Toshihiko Ikemura, Hirohisa Sato). It brightened rapidly. It is observable in good condition in the Northern Hemisphere. It locates low in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   5  3.64   40 10.6   1.259   2.187   154   15.4  22:27 (180, 85)  
Jan.  6   5  0.18   39 54.4   1.320   2.217   148   15.5  21:56 (180, 85)

* C/2015 V1 ( PanSTARRS )

Now it is 15.6 mag (Dec. 13, Toshihiko Ikemura, Hirohisa Sato). It stays observable at 15-16 mag for a long time from 2017 to 2018. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   0 11.70    0  8.6   4.248   4.268    84   15.4  18:28 ( 22, 53)  
Jan.  6   0 10.78   -0 41.3   4.385   4.270    76   15.5  18:32 ( 34, 49)

* 71P/Clark

It brightened up to 10 mag from spring to summer. Now it is fading. It has already faded down to 14.7 mag (Dec. 13, Thomas Lehmann). It is observable in excellent condition in the Southern Hemisphere. It locates low in the Northern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  22 28.75  -17 22.2   2.690   2.267    54   15.8  18:28 ( 41, 26)  
Jan.  6  22 41.59  -15 50.3   2.795   2.305    50   16.0  18:32 ( 47, 25)

* C/2011 KP36 ( Spacewatch )

Now it is 15.0 mag (Nov. 22, Sandor Szabo). It stays 17 mag in 2018. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   3 13.15   -1  5.8   5.766   6.382   125   15.9  20:37 (  0, 54)  
Jan.  6   3 12.59   -0 55.4   5.886   6.413   118   15.9  20:09 (  0, 54)

* C/2016 N4 ( MASTER )

Now it is 15.3 mag (Dec. 17, Toshihiko Ikemura, Hirohisa Sato). It will be fading after this. In the Northern Hemisphere, it stays observable in the northern sky for a long time. It is not observable at all after this in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  20  5.30   62 12.0   3.252   3.352    87   15.9  18:28 (146, 38)  
Jan.  6  20 11.98   62 39.5   3.291   3.372    86   15.9  18:32 (147, 35)

* C/2014 B1 ( Schwartz )

Now it is 16.5 mag (Dec. 18, Toshihiko Ikemura, Hirohisa Sato). It stays 16-17 mag for a long time from 2016 to 2019. It stays near by the equator. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  10 34.32    4 10.1   9.054   9.576   119   15.9   4:01 (  0, 59)  
Jan.  6  10 34.05    4 19.3   8.959   9.579   126   15.9   3:33 (  0, 59)

* C/2017 S6 ( Catalina )

Now it is 15.6 mag (Nov. 22, Sandor Szabo). It stays observable at 16 mag for a long time until summer in 2018. It is observable in good condition in the Northern Hemisphere in 2017, and in the Southern Hemisphere in 2018. Mikhail Maslov reported that it looks bright as 13 mag with a large coma by his photo on Dec. 19. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  22 58.01   25 21.1   1.620   1.742    79   16.0  18:28 ( 79, 61)  
Jan.  6  22 53.38   21  5.5   1.755   1.700    70   16.0  18:32 ( 79, 52)

* C/2016 A1 ( PanSTARRS )

Now it is 15.6 mag (Dec. 13, Toshihiko Ikemura, Hirohisa Sato). It stays 16 mag for a long time from 2017 to 2018. It is observable in excellent condition in the Northern Hemisphere. It locates very low in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   8 48.67   33 10.6   4.466   5.335   149   16.0   2:16 (  0, 88)  
Jan.  6   8 40.91   34 38.5   4.424   5.338   156   16.0   1:41 (  0, 90)

* 217P/LINEAR

It brightened up to 12.2 mag in August (Aug. 21, Juan Jose Gonzalez). It is fading now. It has already faded down to 15.5 mag (Dec. 13, Toshihiko Ikemura, Hirohisa Sato). 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   7 56.54   14 33.9   1.329   2.274   159   16.0   1:24 (  0, 69)  
Jan.  6   7 48.20   15 39.1   1.360   2.331   168   16.3   0:48 (  0, 71)

* C/2017 T3 ( ATLAS )

Now it is 16.5 mag (Dec. 15, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 9 mag in 2018 summer. However, it is hardly observable when it is bright. In the Northern Hemisphere, it is observable only until March when it brightens up to 14 mag. In the Southern Hemisphere, it is observable from July to September in 2018, but it locates in extremely low. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  22 38.01   57 37.1   2.911   3.156    95   16.3  18:28 (144, 57)  
Jan.  6  22 50.32   55 19.6   2.891   3.073    91   16.2  18:32 (139, 55)

* 74P/Smirnova-Chernykh

Now it is 16.5 mag (Dec. 17, Toshihiko Ikemura, Hirohisa Sato). It will be observable at 16 mag in good condition from winter to spring. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  11 55.50    8 28.2   3.192   3.538   102   16.4   5:22 (  0, 63)  
Jan.  6  11 58.12    8 27.7   3.093   3.537   109   16.3   4:57 (  0, 63)

* C/2017 B3 ( LINEAR )

It stays 15 mag from 2018 to 2019, and it will be observable for a long time in the Southern Hemisphere. In the Northern Hemisphere, it will never be observable again. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  13 52.63  -46 36.3   5.592   5.177    60   16.6   5:37 (343,  5)  
Jan.  6  13 57.14  -48  1.3   5.476   5.141    65   16.5   5:38 (347,  5)

* 355P/2017 M2 ( LINEAR-NEAT )

Return of a new periodic comet which brightened up to 13 mag in 2004. It brightened rapidly up to 14.3 mag (Nov. 15, Catalina Sky Survey). Now it is fading. It has already faded down to 16.5 mag (Dec. 17, Toshihiko Ikemura, Hirohisa Sato). 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   2 27.53   19 52.8   1.137   1.861   122   16.6  19:52 (  0, 75)  
Jan.  6   2 34.57   21  4.8   1.220   1.887   117   16.8  19:32 (  0, 76)

* C/2016 T3 ( PanSTARRS )

Now it is 16.8 mag (Dec. 20, Toshihiko Ikemura, Hirohisa Sato). It will be observable at 16.5 mag in good condition in winter. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   9 59.43  -10 55.7   2.287   2.902   119   16.6   3:26 (  0, 44)  
Jan.  6   9 58.50  -12 11.7   2.250   2.932   125   16.6   2:58 (  0, 43)

* C/2015 ER61 ( PanSTARRS )

It brightened up to 6.2 mag in April (Apr. 7, Juan Jose Gonzalez). Now it is fading rapidly. It has already faded down to 15.5 mag (Dec. 20, Thomas Lehmann). It stays observable for a long time after this. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   2 42.49   15 33.6   2.773   3.431   124   16.7  20:07 (  0, 71)  
Jan.  6   2 42.88   15 29.0   2.940   3.507   117   17.0  19:40 (  0, 71)

* C/2010 U3 ( Boattini )

Now it is 16.5 mag (Dec. 18, Toshihiko Ikemura, Hirohisa Sato). It will pass the perihelion in 2019. However, it has not been brightening since the discovery in 2010. It is observable in good conditioin in the Northern Hemisphere. It is not observable for a long time in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   6 22.92   76 40.8   8.187   8.807   126   16.8  23:47 (180, 48)  
Jan.  6   6 14.06   76 48.5   8.190   8.796   125   16.8  23:11 (180, 48)

* 30P/Reinmuth 1

Now it is 17.1 mag (Dec. 21, Katsumi Yoshimoto). It stays observable at 17 mag in good condition for a while. It will be fainter than 18 mag in May. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  14 12.17   -5 58.1   2.416   2.199    65   16.9   5:37 (319, 40)  
Jan.  6  14 23.33   -6 34.6   2.369   2.230    69   16.9   5:38 (324, 42)

* 47P/Ashbrook-Jackson

Now it is 16.9 mag (Dec. 13, Toshihiko Ikemura, Hirohisa Sato). It will be fading after this, and it will be fainter than 18 mag in March. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   1  2.81   17 46.6   2.668   3.042   102   16.9  18:28 (  0, 73)  
Jan.  6   1  7.35   18  7.3   2.777   3.056    97   17.0  18:32 ( 22, 72)

* 90P/Gehrels 1

Now it is 16.9 mag (Dec. 13, Toshihiko Ikemura, Hirohisa Sato). In the Northern Hemisphere, it will be observable at 17 mag in excellent condition from autumn to winter. It locates low in the Southern Hemisphere. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   5  9.53   35 50.7   2.340   3.270   157   16.9  22:33 (180, 89)  
Jan.  6   5  5.63   35 37.9   2.397   3.290   150   16.9  22:02 (180, 89)

* 103P/Hartley 2

Now it is 18.2 mag (Dec. 19, Toshihiko Ikemura, Hirohisa Sato). It will be fading slowly after this. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  12  1.31  -13 10.1   2.734   2.947    92   17.4   5:28 (  0, 42)  
Jan.  6  12  2.47  -13 36.7   2.681   2.998    99   17.4   5:01 (  0, 41)

* C/2015 XY1 ( Lemmon )

Now it is 16.9 mag (Dec. 22, Toshihiko Ikemura, Hirohisa Sato). It stays observable at 18 mag for a long time until 2019. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30   6 14.55   18 12.7   6.986   7.962   172   17.7  23:38 (  0, 73)  
Jan.  6   6  8.58   18  0.2   7.002   7.959   165   17.7  23:04 (  0, 73)

* C/2017 D3 ( ATLAS )

Now it is 17.8 mag (Nov. 23, H. Nohara). It was observed at 17 mag in former 2017. It will be observable at 18 mag in good condition from winter to spring. 

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Dec. 30  12 54.71    3 26.8   5.281   5.321    87   17.9   5:37 (339, 57)  
Jan.  6  12 54.23    4 25.6   5.172   5.341    94   17.8   5:38 (353, 59)

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