Weekly Information about Bright Comets (2015 Sept. 5: South)

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Updated on September 6, 2015
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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/2013 US10 ( Catalina )

Now it is bright as 6.3 mag (Sept. 2, Marco Goiato). It is expected to brighten up to 4-5 mag from autumn to winter. It keeps observable in excellent condition until autumn in the Southern Hemisphere. In the Northern Hemisphere, it keeps unobservable until late November.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  15 16.26  -56 51.0   1.252   1.511    83    6.4  19:07 ( 39, 54)  
Sept.12  14 58.22  -50 50.8   1.347   1.418    72    6.2  19:12 ( 51, 48)  

* 322P/SOHO

It passed the perihelion on Sept. 4, and it was detected on the SOHO images. It is not observable from the ground because it locates too close to the Sun.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  10 44.36    8 52.5   1.075   0.084     2    7.4   4:50 (271,-17)  
Sept.12  11 35.34    2 13.3   1.377   0.383     4   15.2  19:12 ( 83,-13)  

* C/2014 Q2 ( Lovejoy )

It brightened up to 3.7 mag and became a naked eye comet in mid January (Jan. 13, Marek Biely). Now it is fading. But it is bright as 10.8 mag still now (Sept. 5, Neil Norman). In the Northern Hemisphere, it keeps observable for a long time until the comet fades out. It locates extremely low in the Southern Hemisphere, and it will be unobservable in late September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  15 47.68   42 30.7   3.329   3.186    73   10.9  19:07 (155,  7)  
Sept.12  15 55.14   39 55.0   3.441   3.259    71   11.0  19:12 (150,  7)  

* C/2014 Q1 ( PanSTARRS )

It approached to the sun down to 0.3 a.u. on July 6, and brighted up to 3.9 mag (July 6, Thomas Lehmann). Now it is 10.7 mag (Sept. 2, Marco Goiato). In the Northern Hemisphere, it keeps observable until the comet fades out. It will not be observable after this in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  12 48.75  -37  4.8   1.833   1.445    51   11.0  19:07 ( 63, 29)  
Sept.12  13 12.25  -40 13.7   1.978   1.569    51   11.5  19:12 ( 58, 28)  

* 22P/Kopff

Now it is 11.7 mag (Aug. 7, Marco Goiato). It will brighten up to 11 mag autumn. In this apparition, it is observable until the highlight while the comet is brightening.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  14 39.27  -12 21.2   1.903   1.639    59   11.2  19:07 (103, 39)  
Sept.12  14 56.72  -13 57.0   1.926   1.618    57   11.1  19:12 ( 99, 37)  

* C/2015 F4 ( Jacques )

It brightened rapidly up to 10.4 mag from July to August (July 18, Maik Meyer). Now it is fading, but it is bright as 10.8 mag still now (Sept. 5, Neil Norman). It is observable in good condition in the Northern Hemisphere, but it will be getting lower gradually in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  18 48.09   43  3.6   1.101   1.678   105   11.8  19:51 (180, 12)  
Sept.12  18 47.00   43 58.2   1.168   1.698   102   12.0  19:23 (180, 11)  

* 141P/Machholz 2

It brightened rapidly in mid August. Now it is very bright as 11.2 mag (Aug. 28, Juan Jose Gonzalez). Secondary component is also visible as 14.0 mag (Aug. 28, Michael Jager). In the Northern Hemisphere, it keeps observable in good condition in the morning sky. It keeps locating extremely low from summer to autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   8  4.62   21 51.7   1.104   0.783    43   11.8   4:50 (238,  6)  
Sept.12   8 32.13   18 22.6   1.185   0.819    42   12.1   4:41 (242,  7)  

* 67P/Churyumov-Gerasimenko

Now it is 11.8 mag (Aug. 26, Katsumi Yoshimoto). It keeps bright as 12 mag from August to October. In the Northern Hemisphere, it is getting higher gradually, and it keeps observable in good condition after this. In the Southern Hemisphere, it keeps low until November.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   7 59.25   23 26.6   1.774   1.275    44   12.2   4:50 (236,  6)  
Sept.12   8 24.61   22 37.6   1.780   1.296    45   12.1   4:41 (238,  5)  

* C/2015 P3 ( SWAN )

New bright comet. Now it is 11.6 mag (Aug. 18, Chris Wyatt). In the Southern Hemisphere, it keeps observable in the evening sky until the comet becomes fainter than 18 mag in winter. In the Northern Hemisphere, it will never be observable again.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  14  6.01  -31 25.1   1.083   1.047    59   12.4  19:07 ( 76, 41)  
Sept.12  14 30.69  -38 55.6   1.191   1.143    61   13.0  19:12 ( 66, 42)  

* 10P/Tempel 2

Now it is faint as 16.0 mag (Aug. 27, Mitsunori Tsumura). It will brighten very rapidly after this. It will brighten up to 11 mag from autumn to winter. But it locates low at that time.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  15 19.28  -12  6.3   1.652   1.594    68   12.8  19:07 (111, 47)  
Sept.12  15 34.83  -13 58.9   1.670   1.563    66   12.5  19:12 (106, 45)  

* C/2013 X1 ( PanSTARRS )

Now it is 13.7 mag (Aug. 26, Hiroshi Abe). It will pass close to the earth from spring to summer in 2016, and it is expected to be observable at 6-7 mag in good condition. In the Northern Hemispehre, it keeps observable in excellent condition until winter. In the Southern Hemisphere, it keeps very low until winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   5 45.27   37 47.4   3.406   3.300    75   13.3   4:50 (204, 12)  
Sept.12   5 44.17   38 30.2   3.205   3.227    82   13.1   4:41 (200, 13)  

* 19P/Borrelly

It brightened up to 12.8 mag until March (Mar. 21, Michael Mattiazzo). It must have brightened up to 10.5 mag in May and June, but it was not observable. In the Northern Hemisphere, it is appearing in the morning sky. It keeps observable after this while the comet will be fading.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  10  6.84   29 47.3   2.608   1.749    25   13.1   4:50 (247,-21)  
Sept.12  10 26.98   28 58.7   2.629   1.796    27   13.3   4:41 (248,-21)  

* 88P/Howell

It is fading, but bright as 11.4 mag still now (Aug. 21, Uwe Pilz). It keeps observable in good condition until winter when the comet becomes fainter than 18 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   2 56.76   12 44.4   1.400   2.057   116   13.3   4:03 (180, 42)  
Sept.12   2 56.00   12 44.7   1.375   2.104   123   13.5   3:35 (180, 42)  

* C/2015 G2 ( MASTER )

It brightened up to 6.0 mag in mid May (May 14, Chris Wyatt). Now it is fading. It has faded down to 9.0 mag in late June (June 21, Marco Goiato). It is appearing in the morning sky. In the Northern Hemisphere, it keeps observable in good condition after this while the comet will be fading. It locates somewhat low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   8 40.18   17 58.7   2.703   1.953    34   13.6   4:50 (246,  2)  
Sept.12   8 41.49   18 47.0   2.699   2.047    40   13.8   4:41 (243,  5)  

* C/2012 F3 ( PanSTARRS )

Now it is 12.9 mag (July 11, Gabor Santa). In 2015, it keeps 13-14 mag and will be observable in good condition for a long time.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  19 11.02  -12 37.4   3.055   3.727   125   13.6  20:15 (180, 68)  
Sept.12  19 13.13  -13  2.8   3.159   3.751   118   13.7  19:49 (180, 68)  

* 29P/Schwassmann-Wachmann 1

Now it is so faint as 17.2 mag (Sept. 4, Jean-Francois Soulier).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  17 17.71  -29 40.4   5.773   6.011    98   13.6  19:07 (116, 79)  
Sept.12  17 19.47  -29 31.1   5.882   6.009    92   13.7  19:12 (103, 73)  

* C/2014 S2 ( PanSTARRS )

Now it is 13.8 mag and visible visually (Aug. 13, Sandor Szabo). It is expected to brighten up to 15 mag from autum to next spring, and to be observable in excellent condition in the Northern Hemisphere. It keeps unobservable in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   3  5.17   69  0.7   2.109   2.379    92   13.9   4:12 (180,-14)  
Sept.12   3 10.70   73 32.9   2.042   2.343    94   13.7   3:50 (180,-18)  

* C/2011 KP36 ( Spacewatch )

Now it is 14.1 mag and visible visually (July 10, Jakub Cerny). Distant object, but it keeps observable at 14-15 mag for a long time from 2015 to 2016.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  21 13.38   -3 46.4   4.314   5.245   154   14.4  22:16 (180, 59)  
Sept.12  21 11.75   -4 18.1   4.343   5.227   148   14.4  21:47 (180, 59)  

* C/2014 A4 ( SONEAR )

Now it is 15.4 mag (Aug. 26, D. Buczynski). It will brighten up to 14 mag from 2015 to 2016. It keeps observable in good condition for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   2 49.32   12 48.1   3.610   4.180   118   14.5   3:56 (180, 42)  
Sept.12   2 41.16   13 17.5   3.501   4.181   126   14.4   3:20 (180, 42)  

* C/2014 W2 ( PanSTARRS )

Now it is 14.7 mag (Aug. 26, Hiroshi Abe). It keeps 13 mag for a long time from 2015 autumn to 2016 summer. In the Northern Hemispehre, it keeps observable in good condition for a long time. It keeps unobservable in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   6 28.24   54 11.3   3.493   3.297    70   14.6   4:50 (203, -6)  
Sept.12   6 38.80   56 22.8   3.363   3.256    75   14.5   4:41 (201, -7)  

* 318P/2014 M6 ( McNaught-Hartley )

First return of a periodic comet discovered in 1994. Now it is 15.4 mag (Aug. 27, Mitsunori Tsumura). It will brighten up to 15 mag from summer to autumn, and will be 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)  
Sept. 5  22 48.07  -35 40.7   1.553   2.485   151   14.9  23:50 (  0, 89)  
Sept.12  22 43.31  -35 10.4   1.562   2.475   148   14.9  23:18 (  0, 90)  

* C/2014 N3 ( NEOWISE )

Now it is 14.9 mag (Aug. 26, D. Buczynski). It keeps 15 mag for a long time from 2014 to 2015. It is observable in excellent 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)  
Sept. 5   2 15.82   39 19.4   3.656   4.171   114   15.0   3:22 (180, 16)  
Sept.12   2 11.00   40 46.4   3.598   4.193   120   15.0   2:50 (180, 14)  

* 116P/Wild 4

It is not observable now. It will be observable after mid October in the Northern Hemisphere, or after December in the Southern Hemisphere. It is expected to brighten up to 13 mag from winter to spring. It will be observable in excellent condition in the Southern Hemisphere. But it locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  10 27.04   11 48.2   3.358   2.363     8   15.5   4:50 (266,-15)  
Sept.12  10 40.40   10 26.1   3.325   2.346    11   15.4   4:41 (267,-14)  

* C/2014 W11 ( PanSTARRS )

It brightened very rapidly, and brightened up to 13.8 mag (May 11, Sandor Szabo). It is not observable now. It will appear in the morning sky in November, but it will be fainter than 17 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  11 21.84   -5 20.4   4.446   3.478    14   15.4  19:07 ( 80, -5)  
Sept.12  11 31.19   -6 26.8   4.469   3.488    11   15.5  19:12 ( 75, -9)  

* 61P/Shajn-Schaldach

Now it is 16.3 mag (Aug. 24, S. Shurpakov). It will be observable at 15 mag in good condition in autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   2 26.97    9 27.8   1.386   2.124   124   15.5   3:33 (180, 45)  
Sept.12   2 30.79    9  9.8   1.326   2.120   130   15.4   3:09 (180, 46)  

* C/2012 K1 ( PanSTARRS )

It brightened up to 6.9 mag in 2014 autumn (Oct. 17, Marco Goiato). Now it is fading. It has already faded down to 16.2 mag (Aug. 22, K. Hills). In the Southern Hemisphere, it keeps observable in good condition until the comet fades out. In the Northern Hemisphere, it keeps observable until winter, but it locates somewhat low.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  23 45.89  -27 40.7   3.930   4.868   155   15.6   0:53 (180, 83)  
Sept.12  23 36.34  -28 15.6   4.001   4.936   155   15.7   0:16 (180, 83)  

* 57P/du Toit-Neujmin-Delporte

Now it is 14.6 mag and visible visually (July 12, Jakub Cerny). It keeps observable in good condition for a while. But it will be fading after this, and will be fainter than 18 mag in November.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   0 28.91    4 31.8   1.020   1.974   153   15.7   1:35 (180, 50)  
Sept.12   0 24.92    3 49.6   1.024   2.004   161   15.8   1:04 (180, 51)  

* C/2013 V4 ( Catalina )

Now it is 15.8 mag (Aug. 5, Ken-ichi Kadota). It keeps 15-16 mag for a long time until 2016. It keeps observable in excellent condition in the Northern Hemisphere. It keeps unobservable in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   5 26.20   56 10.1   5.279   5.191    79   15.8   4:50 (194, -4)  
Sept.12   5 30.33   57 35.9   5.185   5.189    84   15.7   4:41 (192, -4)  

* 117P/Helin-Roman-Alu 1

It brightened up to 13 mag in 2014. Now it is 16.3 mag (Aug. 27, A. Maury, J.-G. Bosch, J.-F. Soulier, T. Noel). It will be fading slowly after this. It is observable at 16 mag in excellent condition from summer to winter in 2015.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   1 38.56    1 47.7   3.052   3.859   137   16.0   2:45 (180, 53)  
Sept.12   1 35.91    1 30.2   3.005   3.875   145   16.0   2:15 (180, 53)  

* 230P/LINEAR

Now it is 17.1mag (Aug. 27, A. Maury, J.-G. Bosch, J.-F. Soulier, T. Noel). It is expected to brighten rapidly, and to be observable at 14.5 mag in good condition in autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   3 34.79   -5 27.1   1.033   1.673   110   16.3   4:40 (180, 60)  
Sept.12   3 49.35   -5 59.4   0.966   1.642   112   16.1   4:27 (180, 61)  

* 44P/Reinmuth 2

It brightened up to 16.4 mag in 2014 (Nov. 14, J. F. Hernandez). Now it is 17.2 mag (Aug. 27, D. Buczynski). It will be observable at 16 mag again from summer to autumn in 2015. However, it is fainter than this ephemeris recently.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   4 11.64   27 20.6   2.133   2.451    95   16.1   4:50 (187, 27)  
Sept.12   4 17.29   27 42.5   2.072   2.476   101   16.1   4:41 (184, 27)  

* C/2010 S1 ( LINEAR )

Now it is 15.1 mag (July 13, Yuji Ohshima). It is observable at 15-16 mag in good condition until autumn. It locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  17 37.33  -25 47.7   7.950   8.235   102   16.2  19:07 (147, 79)  
Sept.12  17 35.92  -26  2.1   8.103   8.267    95   16.3  19:12 (121, 74)  

* C/2014 W5 ( Lemmon-PanSTARRS )

No observations have been reported after November in 2014. Current brightness is uncertain. It must keep 16 mag for a long time from 2015 autumn to 2016 summer. It keeps 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)  
Sept. 5   3  5.51  -15 48.1   2.476   3.078   117   16.9   4:12 (180, 71)  
Sept.12   2 55.67  -19 11.7   2.347   3.039   125   16.7   3:34 (180, 74)  

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

Now it is 17.5 mag (July 25, Katsumi Yoshimoto). It has brightened in outburst up to 14 mag twice, in 2006 January and 2011 May. It is around the perihelion now. It keeps observable at 17 mag for a long time after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  23 18.45   -3 54.7   4.851   5.853   172   16.9   0:25 (180, 59)  
Sept.12  23 15.93   -4 14.1   4.850   5.857   179   16.8  23:51 (180, 59)  

* C/2011 J2 ( LINEAR )

Now it is 15.9 mag (Aug. 20, Catalina Sky Survey). It is fading, but it is observable at 17 mag in good condition until late autumn. The fragments B and C are already fainter than 20 mag (June 12, Takaaki Oribe).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  23 10.22    4 58.1   5.366   6.353   167   16.9   0:17 (180, 50)  
Sept.12  23  5.15    3 56.9   5.403   6.399   170   16.9  23:40 (180, 51)  

* 162P/Siding Spring

Now it is 16.3 mag (Aug. 22, E. Bryssinck). In the Northern Hemisphere, it is getting higher gradually in the morning sky. It is not observable in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   7 27.65   37  1.5   1.695   1.395    55   17.1   4:50 (221,  1)  
Sept.12   7 53.05   37 57.9   1.697   1.433    57   17.1   4:41 (222,  0)  

* 151P/Helin

Now it is 18.3 mag (Aug. 18, Jean-Francois Soulier). It will be observable at 17 mag in good condition from summer to autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  23 41.83   -5 41.5   1.494   2.489   167   17.2   0:48 (180, 61)  
Sept.12  23 39.02   -6 19.2   1.479   2.483   174   17.1   0:18 (180, 61)  

* 81P/Wild 2

No observations have been reported after November in 2014. It will brighten up to 11 mag from spring to summer in 2016. In the Northern Hemisphere, it keeps observable in good condition while the comet will be brightening. It locates somewhat low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   5 31.07   20 13.9   3.145   3.110    78   17.4   4:50 (209, 29)  
Sept.12   5 37.93   20 13.6   3.011   3.071    83   17.2   4:41 (206, 30)  

* C/2015 K1 ( MASTER )

Now it is 16.0 mag (Aug. 20, Catalina Sky Survey). It keeps observable in good condition until the comet fades out. In 2014, it must have been observable at 14 mag in good condition in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   0 37.08    2 17.6   3.255   4.175   152   17.3   1:44 (180, 53)  
Sept.12   0 32.40    2 23.2   3.265   4.227   160   17.3   1:11 (180, 53)  

* P/2003 WC7 ( LINEAR-Catalina )

It has not been recovered yet. But it must be already bright as 17.5 mag. It will approach to the earth from autumn to winter, and it is expected to brighten up to 15 mag and observable in excellent condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   3 59.72   -7 15.0   1.415   1.927   104   17.6   4:50 (188, 62)  
Sept.12   4 10.85   -7 11.2   1.329   1.891   107   17.4   4:41 (184, 62)  

* 319P/2015 G1 ( Catalina-McNaught )

First return of a periodic comet discovered in 2008. It approached to the earth and brightened up to 16 mag from spring to summer (June 2, WISE). Now it is fading. It has already faded down to 17.9 mag (Aug. 13, W. Hasubick).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   3 50.49   -8 28.4   0.791   1.448   106   17.4   4:50 (183, 63)  
Sept.12   3 54.78   -9 19.4   0.799   1.496   111   17.6   4:33 (180, 64)  

* 51P/Harrington

It brightened up to 15.9 mag in June as predicted (June 23, Ken-ichi Kadota). It was expected to be observable at 13 mag in good condition from summer to autumn. However, Jean-Gabriel Bosch detected the comet became disintegrating in July. Now it is so faint as 19.3 mag (Aug. 26, W. Hasubick). The fragment D and B are also observed as 19.4 mag (July 28, iTelescope Observatory, Siding Spring) and 20.9 mag (Aug. 21, Pan-STARRS 1, Haleakala) respectively.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   2 18.18    3  3.8   0.899   1.715   127   17.6   3:24 (180, 52)  
Sept.12   2 22.59    3 12.3   0.871   1.725   133   17.6   3:01 (180, 52)  

* 327P/2015 P2 ( Van Ness )

Now it is 18.8 mag (Aug. 10, A. Sodor, K. Sarneczky). It was predicted to be observable at 17.5 mag in good condition from autumn to winter, but it is a bit fainter actually.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  18 18.18   17 56.2   1.271   1.847   107   17.7  19:22 (180, 37)  
Sept.12  18 24.02   14 38.7   1.274   1.812   104   17.6  19:12 (176, 40)  

* 299P/2014 D2 ( Catalina-PanSTARRS )

Now it is 16.5 mag (Aug. 8, J. Oey, P. Camilleri, H. Williams). It will be fading after this, and will be fainter than 18 mag in October.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  16 54.96  -22 22.3   3.078   3.290    93   17.6  19:07 (126, 71)  
Sept.12  17  0.79  -22 16.9   3.186   3.301    87   17.7  19:12 (115, 66)  

* C/2013 G3 ( PanSTARRS )

Now it is 17.8 mag (Aug. 19, A. Diepvens). It was observed at 17 mag in 2014 summer. In the Northern Hemisphere, it is observable at 17.5 mag in excellent condition also in 2015. It is not observable in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  21 55.13   52 26.5   4.034   4.610   119   17.7  22:57 (180,  3)  
Sept.12  21 52.02   51 21.6   4.041   4.643   121   17.7  22:27 (180,  4)  

* C/2014 AA52 ( Catalina )

It brightened up to 15.3 mag in winter (Jan. 17, Taras Prystavski). Now it is fading. It has already faded down to 16.6 mag (Aug. 18, Catalina Sky Survey). It keeps observable in good condition for a while. But it will be fainter than 18 mag in September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  21 40.78  -10 37.1   2.007   2.981   161   17.7  22:42 (180, 65)  
Sept.12  21 24.98   -9 48.3   2.116   3.038   151   17.8  21:59 (180, 65)  

* 118P/Shoemaker-Levy 4

It will brighten up to 14 mag in 2016 summer. But it is not observable at the highlight. It keeps observable until March while the comet will be brightening gradually up to 15-16 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   0 55.61   -0 56.7   1.952   2.864   148   17.9   2:02 (180, 56)  
Sept.12   0 52.67   -1 44.1   1.882   2.833   156   17.7   1:32 (180, 57)  

* 221P/LINEAR

It brightened up to 15.6 mag from spring to summer (July 8, Taras Prystavski). Now it is fading. It has already faded down to 16.8 mag (Aug. 21, B. Haeusler). It will be fainter than 18 mag in September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  17 35.91   -8 47.0   1.336   1.828   101   17.7  19:07 (165, 63)  
Sept.12  17 49.04   -9 12.7   1.410   1.846    98   17.9  19:12 (155, 62)  

* 50P/Arend

Now it is 17.1 mag (Aug. 23, E. Bryssinck). It was expected to brighten rapidly, and to be observable at 16 mag in good condition from summer to winter. But actually, it is much fainter than predicted.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  23 11.96  -13  5.9   1.348   2.352   172   17.9   0:19 (180, 68)  
Sept.12  23  4.21  -12 37.4   1.319   2.319   171   17.8  23:39 (180, 67)  

* 74P/Smirnova-Chernykh

Now it is 18.9 mag (Aug. 25, S. Shurpakov). Now it is near the aphelion. It is observable at 17 mag in good condition from autumn to winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   3 53.47   16 31.9   4.041   4.366   102   17.8   4:50 (183, 38)  
Sept.12   3 54.79   16 35.0   3.931   4.358   108   17.8   4:33 (180, 38)  

* P/2015 Q2 ( Pimentel )

New comet. It is brightest now. It will be fading rapidly after October. It is observable in excellent condition in the SOuthern Hemisphere. But it will be unobservable soon in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   2 18.54  -46 41.6   1.084   1.821   121   17.8   3:26 (  0, 79)  
Sept.12   1 30.96  -56 51.8   1.080   1.820   121   17.8   2:12 (  0, 69)  

* 220P/McNaught

Now it is 17.8 mag (Aug. 14, Space Surveillance Telescope, Atom Site). It will be fading after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   3 25.63    8 53.0   1.118   1.746   110   17.9   4:31 (180, 46)  
Sept.12   3 31.46    8 18.4   1.091   1.776   115   17.9   4:10 (180, 47)  

* C/2010 U3 ( Boattini )

It will pass the perihelion in 2019. However, it has not been brightening since the discovery in 2010. Now it is 18.3 mag (Aug. 23, S. Shurpakov). It keeps observable in excellent condition from autumn to next spring in the Northern Hemisphere. It is not observable in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   3 53.91   44 35.4  11.036  11.176    95   18.0   4:50 (182, 10)  
Sept.12   3 53.65   45  1.0  10.906  11.151   101   17.9   4:32 (180, 10)  

* 205P/Giacobini

Now it is 19.2 mag (Aug. 26, W. Hasubick). First return of a comet re-discovered after 112-year blank in 2008. It brightened up to 12 mag in 2008. In this apparition, it was expected to brighten up to 15 mag from spring to summer, but it is much fainter than predicted.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5   4 32.86   10 30.1   1.567   1.917    93   18.2   4:50 (196, 43)  
Sept.12   4 40.54    9 31.1   1.535   1.957    98   18.3   4:41 (193, 45)  

* 320P/2015 HC10 ( McNaught )

It was expected to brighten rapidly up to 15 mag in August. But actually, it is so faint as 19.7 mag, much fainter than predicted (Aug. 15, Slooh.com Canary Islands Observatory).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Sept. 5  17 35.04   -6 10.2   0.184   1.059   101   18.4  19:07 (168, 60)  
Sept.12  18 55.09   -2 51.7   0.193   1.100   114   18.6  19:36 (180, 58)  

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Copyright(C) Seiichi Yoshida (comet@aerith.net). All rights reserved.