Weekly Information about Bright Comets (2018 May 19: South)

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Updated on May 21, 2018
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Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Southern Hemisphere.
Azimuth indicates 0 for south, 90 for west, 180 for north, 270 for east.

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* C/2016 M1 ( PanSTARRS )

Now it is bright as 9.0 mag (May 16, Juan Jose Gonzalez). It stays bright as 9 mag for a while. In the Southern Hemisphere, it stays observable in good condition for a long time until the comet will fade out. In the Northern Hemisphere, it is observable only until June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  19 33.09  -16 41.4   1.678   2.408   125    9.9   3:48 (180, 72)  
May  26  19 25.19  -20 34.2   1.555   2.378   134    9.7   3:13 (180, 75)  

* 66P/du Toit

It brightened rapidly as expected. Now it is very bright as 10.5 mag (May 9, Chris Wyatt). It stays at 10-11 mag until June. In the Southern Hemisphere, it stays observable in excellent condition. In the Northern Hemisphere, it will be unobservable from April to June when the comet becomes brightest.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  23  7.25  -34 49.0   0.896   1.290    84   10.1   5:22 (278, 66)  
May  26  23 34.16  -32 41.2   0.899   1.293    84   10.2   5:26 (273, 66)  

* C/2016 R2 ( PanSTARRS )

Now it is 11.3 mag (May 15, Juan Jose Gonzalez). It stays bright as 11 mag for a long time until autumn. In the Southern Hemisphere, it is not observable for a long time after this. In the Northern Hemispehre, it stays observable for a long time until the comet fades out. But it stays very low until autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   5 51.70   46 37.1   3.329   2.604    37   11.1  18:30 (140,-11)  
May  26   6  7.62   47 43.6   3.363   2.608    35   11.1  18:27 (140,-13)  

* C/2017 T3 ( ATLAS )

Now it is 14.4 mag (Apr. 8, Alexander Baransky). It will brighten up to 9 mag in summer. However, it is hardly observable when it is bright. In the Northern Hemisphere, it is not observable until late December. In the Southern Hemisphere, it is observable from July to September, but it locates in extremely low.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   3 15.80   24 52.8   2.365   1.371     7   12.2   5:22 (250,-16)  
May  26   3 32.53   22 46.2   2.271   1.280     8   11.9   5:26 (250,-12)  

* C/2016 N6 ( PanSTARRS )

Now it is 11.6 mag (May 15, Juan Jose Gonzalez). It stays 12 mag for a long time until spring in 2019. In the Northern Hemisphere, it stays observable in good condition for a long time, although it becomes unobservable temporarily from mid June to August. In the Southern Hemisphere, it is not observable until September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   7 50.89   51  8.3   3.150   2.743    57   12.1  18:30 (158, -2)  
May  26   7 53.86   48 22.9   3.231   2.727    52   12.1  18:27 (154, -1)  

* C/2018 EF9 ( Lemmon )

It brightened very rapidly. Now it is very bright as 11.8 mag (May 16, Juan Jose Gonzalez). It may fade out very rapidly in June. In the Northern Hemisphere, it stays observable until it fades out. It is not observable in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   6 22.50   84 51.4   1.656   1.558    66   12.5  18:30 (175,-32)  
May  26   5 45.64   84 24.6   1.710   1.558    63   12.5  18:27 (174,-33)  

* 37P/Forbes

Now it is bright as 11.5 mag (May 16, Juan Jose Gonzalez). It will be observable at 12-13 mag in good condition from spring to summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  22 22.95  -14 15.6   1.345   1.617    85   13.1   5:22 (224, 63)  
May  26  22 37.37  -12 12.3   1.304   1.625    88   13.0   5:26 (214, 64)  

* C/2015 O1 ( PanSTARRS )

Now it is very bright as 12.0 mag (May 15, Juan Jose Gonzalez). It will be observable at 12-13 mag for a long time from 2017 to 2018. In the Southern Hemisphere, it will be hardly observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  13  0.44   56  1.6   3.554   3.812    97   13.1  21:11 (180, -1)  
May  26  12 42.71   55  1.7   3.652   3.826    92   13.2  20:26 (180,  0)  

* 48P/Johnson

Now it is 14.8 mag (Apr. 26, Catalina Sky Survey). It will brighten rapidly after this, and it will brighten up to 11 mag from summer to autumn. It is observable in excellent condition in the Southern Hemisphere. It locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  21 34.05  -15  7.4   1.739   2.113    96   13.4   5:22 (199, 69)  
May  26  21 44.83  -15  0.2   1.652   2.097   101   13.2   5:26 (184, 70)  

* 29P/Schwassmann-Wachmann 1

Appearing in the morning sky. Now it is 14.8 mag (May 10, Toshihiko Ikemura, Hirohisa Sato).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  23  9.97   -1  2.6   6.055   5.783    69   13.6   5:22 (227, 46)  
May  26  23 12.80   -0 35.4   5.950   5.782    75   13.6   5:26 (218, 49)  

* 21P/Giacobini-Zinner

Now it is 14.9 mag (May 9, Thomas Lehmann). It will brighten rapidly, and brighten up to 7 mag from August to September. In the Northern Hemisphere, it will be observable in excellent condition. In the Southern Hemisphere, it will be unobservable from July to August. But it will be observable in good condition before and after tha.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  20  8.82   26 38.2   1.320   1.803   100   14.0   4:23 (180, 28)  
May  26  20 19.70   30  7.8   1.230   1.738   101   13.6   4:06 (180, 25)  

* 169P/NEAT

The condition of this apparition is worst. It brightens up to 12.5 mag from April to May. But it is not observable at all.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   4 27.46   16 55.9   1.672   0.708    11   13.9  18:30 (106, -7)  
May  26   5  9.41   17 52.9   1.721   0.781    14   14.8  18:27 (109, -4)  

* 364P/2018 A2 ( PanSTARRS )

First return of a new periodic comet which brightened up to 13 mag in 2013. Now it is 16.3 mag (May 14, Toshihiko Ikemura, Hirohisa Sato). It will brighten very rapidly after this, up to 11 mag in summer. In the Southern Hemisphere, it stays observable in good condition all through this apparition. In the Northern Hemisphere, it is not observable at the high light from mid June to mid August.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   8 47.09   26 18.6   0.623   0.986    69   15.3  18:30 (158, 25)  
May  26   8 52.10   23 12.0   0.576   0.927    64   14.5  18:27 (152, 26)  

* C/2017 S3 ( PanSTARRS )

It is expected to approach to Sun down to 0.2 a.u. and brighten up to 3 mag in August. Now it is 16.4 mag (May 17, Toshihiko Ikemura, Hirohisa Sato). In the Northern Hemisphere, it stays observable in the morning sky until early August when the comet brightens up to 6 mag. It is not observable at all in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   0 34.73   56  5.8   2.494   2.005    50   15.0   5:22 (207,-11)  
May  26   0 52.90   56 48.8   2.362   1.890    50   14.6   5:26 (205,-11)  

* C/2017 M4 ( ATLAS )

Now it is 14.8 mag (May 14, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 13 mag in 2019 spring. In the Northern Hemisphere, it stays observable in good condition for a long time. In the Southern Hemisphere, it locates extremely low until summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  19  1.30   46 17.1   3.671   3.976   100   14.8   3:16 (180,  9)  
May  26  18 49.66   46 34.8   3.581   3.940   103   14.7   2:37 (180,  8)  

* C/2015 V2 ( Johnson )

It brightened up to 7.1 mag from May to June in 2017 (June 21, Juan Jose Gonzalez). Now it is fading. It has already faded down to 14.6 mag (May 14, Thomas Lehmann). 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)  
May  19   1 20.50  -43  0.9   4.551   4.321    70   15.0   5:22 (299, 41)  
May  26   1 28.27  -43  9.9   4.553   4.386    74   15.1   5:26 (298, 46)  

* C/2017 B3 ( LINEAR )

Now it is 15.5 mag (Apr. 25, J. Drummond). 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)  
May  19  12 22.47  -67 48.6   3.882   4.510   122   15.2  20:34 (  0, 57)  
May  26  12 13.72  -67 27.6   3.874   4.481   121   15.2  19:58 (  0, 57)  

* 65P/Gunn

Appearing in the morning sky. It is observable at 15 mag in 2018, in good condition in the Southern Hemisphere. It locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  22 59.53  -16  4.6   3.143   3.096    78   15.7   5:22 (240, 58)  
May  26  23  6.22  -15 43.9   3.062   3.107    83   15.7   5:26 (231, 62)  

* C/2018 C2 ( Lemmon )

It brightened rapidly. Now it is 15.8 mag (May 14, Toshihiko Ikemura, Hirohisa Sato). It stays 15.5 mag until June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  14 50.69   34 12.2   1.203   1.964   124   15.7  23:02 (180, 21)  
May  26  14 47.10   31 10.3   1.202   1.959   124   15.7  22:31 (180, 24)  

* C/2015 VL62 ( Lemmon-Yeung-PanSTARRS )

Appearing in the morning sky. It is fading now. But it stays 16 mag until summer. But actually, it is 18.1 mag (Mar. 23, Toshihiko Ikemura, Hirohisa Sato), fainter than this ephemeris.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  18  1.63  -27 34.3   2.914   3.803   147   15.9   2:18 (180, 83)  
May  26  17 45.46  -27 57.7   2.896   3.850   157   15.9   1:34 (180, 83)  

* C/2015 V1 ( PanSTARRS )

Fading now. It stays observable in good condition for a long time after this in the Southern Hemisphere. It is not observable until June in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   0 55.30   -8 15.3   5.038   4.450    49   16.0   5:22 (257, 31)  
May  26   0 57.23   -8 58.1   4.953   4.467    56   16.0   5:26 (252, 38)  

* (3552) Don Quixote

Now it is 15.5 mag (Mar. 16, iTelescope Observatory, Siding Spring). In the Southern Hemisphere, it stays observable until August, but it will be unobservable after that. In the Northern Hemisphere, it stays unobservable until June, but it will be observable in good condition after that. Its cometary activity was observed on Mar. 26 (M. Mommert, D. Polishook, N. Moskovitz).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   0 35.82  -10 43.5   1.516   1.249    54   16.0   5:22 (256, 37)  
May  26   0 51.90   -6 31.4   1.513   1.263    55   16.0   5:26 (249, 37)  

* C/2016 A1 ( PanSTARRS )

Now it is 16.4 mag (May 10, 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)  
May  19   7  9.74   45 17.3   6.088   5.487    49   16.2  18:30 (149, -1)  
May  26   7 12.26   45 28.2   6.178   5.500    44   16.3  18:27 (146, -3)  

* 74P/Smirnova-Chernykh

Now it is 15.9 mag (May 4, Kunihiro Shima). It will be fading slowly until summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  11 21.32   12 10.7   3.107   3.559   108   16.4  19:34 (180, 43)  
May  26  11 23.17   11 42.2   3.204   3.561   102   16.5  19:08 (180, 43)  

* C/2017 K4 ( ATLAS )

It was observed at 16 mag from summer to autumn in 2017. It will be observable at 16.5 mag in good condition also in 2018. It locates somewhat low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   0  7.58   13 10.0   3.471   2.952    51   16.4   5:22 (230, 26)  
May  26   0 16.23   14 39.2   3.433   2.982    55   16.4   5:26 (224, 28)  

* 64P/Swift-Gehrels

It has not been observed yet in this apparition. It will brighten rapidly, and it is expected to brighten up to 10 mag in autumn. It will be observable in excellent condition in the Northern Hemisphere. It stays low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  22 19.38   -9  3.3   2.201   2.330    84   16.7   5:22 (217, 59)  
May  26  22 29.31   -7 40.8   2.069   2.276    88   16.4   5:26 (206, 60)  

* 105P/Singer Brewster

Unexpectedly, it brightened rapidly. Now it is 16.6 mag (May 15, Toshihiko Ikemura, Hirohisa Sato). It stays at 16.5 mag until July.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  12 20.08    1 35.5   1.382   2.141   126   16.5  20:32 (180, 53)  
May  26  12 22.98    1 46.2   1.430   2.126   120   16.5  20:08 (180, 53)  

* C/2017 S6 ( Catalina )

It brightened up to 15-16 mag in winter. Appearing in the morning sky. It stays observable at 16.5 mag for a while. It will be observable in good condition after this in the Southern Hemisphere. But it stays low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  22 40.96  -11 22.2   1.784   1.896    80   16.5   5:22 (228, 58)  
May  26  22 31.47  -14 29.8   1.662   1.951    90   16.5   5:26 (213, 66)  

* C/2017 E3 ( PanSTARRS )

Now it is 16.9 mag (May 15, Toshihiko Ikemura, Hirohisa Sato). It will be fainter than 18 mag in summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  14 38.84   -8 27.1   5.449   6.414   161   16.8  22:50 (180, 63)  
May  26  14 36.00   -7 36.7   5.510   6.433   153   16.8  22:20 (180, 63)  

* C/2014 B1 ( Schwartz )

Now it is 16.6 mag (May 10, 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)  
May  19  10 19.15    9 12.8   9.507   9.658    95   16.8  18:32 (180, 46)  
May  26  10 20.35    9 16.7   9.627   9.664    89   16.8  18:27 (172, 46)  

* C/2014 OE4 ( PanSTARRS )

Now it is 16.8 mag (May 15, Toshihiko Ikemura, Hirohisa Sato). It will be fading gradually after this, and it will be fainter than 18 mag in winter. In the Northern Hemisphere, it stays observable in good condition for a long time. In the Southern Hemisphere, it will never be observable again.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  23  9.66   69 51.0   7.573   7.189    64   16.9   5:22 (191,-17)  
May  26  23 17.38   70 37.2   7.587   7.212    64   16.9   5:26 (188,-17)  

* C/2018 A3 ( ATLAS )

Now it is 16.7 mag (May 10, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 15 mag in January, 2019. It stays observable in excellent condition in the Northern Hemispehre. It is observable only until June in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  10 40.21   34 25.8   3.823   3.960    90   16.9  18:52 (180, 21)  
May  26  10 35.26   34 41.1   3.915   3.925    83   16.9  18:27 (178, 20)  

* 38P/Stephan-Oterma

Now it is 16.7 mag (May 13, Hidetaka Sato). It will brighten rapidly after this, and it is expected to brighten up to 9 mag from autumn to winter. In the Northern Hemisphere, it stays observable in good condition for a long time until it fades out. In the Southern Hemispehre, it is observable in good condition until autumn, but it will be low in winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   1 11.11   -8 24.9   3.212   2.621    46   17.5   5:22 (260, 28)  
May  26   1 23.19   -7 18.2   3.096   2.562    49   17.2   5:26 (255, 32)  

* C/2017 M5 ( TOTAS )

Now it is 18.0 mag (May 15, Toshihiko Ikemura, Hirohisa Sato). It stays observable at 17 mag in good condition from spring to autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  20 59.79    0 16.2   5.735   5.990    99   17.2   5:14 (180, 55)  
May  26  21  1.08    0 40.8   5.634   5.990   105   17.2   4:48 (180, 54)  

* 62P/Tsuchinshan 1

It brightened up to 9.2 mag from November to December (Nov. 16, Juan Jose Gonzalez). Now it is fading rapidly. It has already faded down to 18.5 mag (May 15, Toshihiko Ikemura, Hirohisa Sato).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  13 33.76    3 56.1   1.453   2.325   140   17.3  21:45 (180, 51)  
May  26  13 31.89    3 11.3   1.552   2.374   134   17.7  21:16 (180, 52)  

* C/2017 D3 ( ATLAS )

Now it is 17.8 mag (May 15, Toshihiko Ikemura, Hirohisa Sato). It will be fading after this, and it will be fainter than 18 mag in July.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  11 25.78   26 39.5   5.475   5.780   102   17.4  19:38 (180, 28)  
May  26  11 23.38   26 58.8   5.619   5.807    95   17.5  19:08 (180, 28)  

* C/2014 R3 ( PanSTARRS )

Now it is 17.3 mag (May 15, Toshihiko Ikemura, Hirohisa Sato). It will be fading gradually after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  10 36.69   35 36.1   8.296   8.343    89   17.6  18:49 (180, 20)  
May  26  10 35.64   34 55.0   8.425   8.365    83   17.7  18:27 (179, 20)  

* 143P/Kowal-Mrkos

Now it is 16.6 mag (May 15, Toshihiko Ikemura, Hirohisa Sato). It is observable at 17 mag in good condition in spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  12 43.11   -9  3.0   1.710   2.534   135   17.7  20:55 (180, 64)  
May  26  12 44.27   -8 48.4   1.772   2.536   129   17.8  20:29 (180, 64)  

* 30P/Reinmuth 1

Now it is 17.7 mag (May 4, Kunihiro Shima). It stays observable at 17-18 mag in good condition for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  14 43.03   -3 26.5   1.922   2.886   158   17.9  22:54 (180, 59)  
May  26  14 38.49   -3 26.6   1.991   2.922   151   18.0  22:22 (180, 59)  

* 186P/Garradd

Now it is 17.8 mag (Apr. 6, J. Drummond). It stays 18 mag from 2018 to 2020. It is observable in good condition in the Southern Hemisphere. It locates extremely low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19  12 17.98  -36  4.1   3.753   4.500   132   17.9  20:30 (  0, 89)  
May  26  12 16.44  -35 32.5   3.809   4.496   127   17.9  20:01 (  0, 89)  

* 2018 EN4

Now it is bright as 18.0 mag (May 14, Hidetaka Sato). Hidetaka Sato pointed out its cometary activity. In the Northern Hemisphere, it stays observable at 18 mag until June. It is not observable in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  19   7 18.98   37 17.6   1.902   1.475    50   18.0  18:30 (146,  7)  
May  26   7 31.33   40 12.4   1.956   1.460    46   17.9  18:27 (146,  3)  

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