Weekly Information about Bright Comets (2015 Apr. 25: South)

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Updated on April 29, 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/2015 G2 ( MASTER )

New bright comet. Now it is 8.3 mag (Apr. 21, Marco Goiato). It is expected to brighten up to 6 mag in May. In the Southern Hemisphere, it keeps observable in good condition until late June. In the Northern Hemisphere, it keeps unobservable until September when the comet will be fainter than 13 mag. It must have been observable at 16 mag in good condition in 2014 autumn, but it was not discovered.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  22 52.56  -23 27.0   0.891   0.955    60    8.0   5:06 (271, 42)  
May   2  23 48.24  -29 14.5   0.665   0.886    59    7.1   5:10 (281, 40)  

* 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 7.2 mag still now (Apr. 22, Maik Meyer). In the Northern Hemisphere, it keeps observable all night until July when the comet will fade down to 13 mag. It is not observable in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   1 27.58   74 32.5   2.031   1.791    61    7.7   5:06 (199,-34)  
May   2   1 28.39   77 22.1   2.090   1.860    62    8.1   5:10 (195,-33)  

* 88P/Howell

Now it is very bright as 9.2 mag (Apr. 21, Marco Goiato). In the Southern Hemisphere, it keeps observable in good condition for a long time until the comet fades out. In the Northern Hemisphere, it keeps extremely low and hard to observe until June. It will be observable in good condition after June while the comet will be fading gradually.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  22 59.90   -9 56.4   1.742   1.374    52    8.7   5:06 (258, 33)  
May   2  23 21.02   -7 53.6   1.733   1.388    53    8.7   5:10 (254, 34)  

* 19P/Borrelly

It brightened up to 12.8 mag until March (Mar. 21, Michael Mattiazzo). It will brighten up to 10.5 mag in May and June, but it is not observable. In the Northern Hemisphere, it will be observable after autumn while the comet will be fading.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   2 46.21    6 13.1   2.377   1.406    11   11.1  18:49 ( 93, -7)  
May   2   3  6.16    9 14.1   2.368   1.385     9   10.9  18:42 ( 96, -8)  

* C/2013 US10 ( Catalina )

It brightened up to 13.6 mag until the end of 2014, brighter than originally expected (Dec. 19, Chris Wyatt). Now it is 12.7 mag (Apr. 19, Michael Mattiazzo). It is expected to brighten up to 4 mag from autumn to winter. It keeps observable in excellent condition until autumn in the Southern Hemisphere. In the Northern Hemisphere, it is hardly observable until December.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  23 29.33  -21 57.9   3.715   3.201    52   11.4   5:06 (275, 34)  
May   2  23 33.96  -22 17.9   3.533   3.118    57   11.2   5:10 (271, 39)  

* C/2014 Q1 ( PanSTARRS )

It will approach to the sun down to 0.3 a.u. in July, and it is expected to be bright. It brightened up to 15.6 mag in January (Jan. 13, Yasukazu Ikari). In the Southern Hemisphere, it keeps hard to observe for a while. But it will be observable after mid July, and keeps observable while the comet will be fading gradually. 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)  
Apr. 25   0 59.31    2 23.0   2.564   1.656    20   11.7   5:06 (266,  2)  
May   2   1 13.27    4 53.4   2.417   1.535    22   11.3   5:10 (261,  4)  

* C/2015 F3 ( SWAN )

Bright new comet. Now it is bright as 11.2 mag (Apr. 25, Marek Biely). However, it is getting diffuse rapidly. It seems to be a fragment of Comets C/1988 A1 (Liller) and C/1996 Q1 (Tabur). It must have been visible bright in the evening sky from December to February in the Northern Hemisphere, but it was not discovered. It will be fading after this. But it is observable in excellent condition in the Northern Hemisphere. In the Southern Hemisphere, it is not observable until June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   1 23.35   82 57.8   1.059   1.187    70   11.4   5:06 (189,-35)  
May   2   9 29.99   84 32.5   1.056   1.274    76   11.7  19:06 (180,-29)  

* 6P/d'Arrest

It will brighten up to 11 mag in April and May. But the condition is bad in this apparition. In the Southern Hemisphere, it is getting higher gradually in the morning sky. It will not be observable until late July in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   0 51.81   -2 32.4   2.348   1.491    24   11.4   5:06 (269,  6)  
May   2   1 12.21   -1 20.6   2.362   1.525    26   11.4   5:10 (266,  8)  

* C/2015 F5 ( SWAN-Xingming )

New bright comet. Now it is 10.4 mag (Apr. 24, Marek Biely). In the Northern Hemisphere, it is getting higher in the evening sky. But it will fade out rapidly after this. It is not observable in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   4 54.31   52 16.7   0.774   0.800    51   11.5  18:49 (147,-12)  
May   2   6 17.84   48 28.5   0.989   0.941    56   12.7  18:42 (152, -2)  

* C/2015 C2 ( SWAN )

It brightened up to 9.2 mag in March (Mar. 9, Juan Jose Gonzalez). Now it is fading, but it is bright as 11.7 mag still now (Apr. 23, Piotr Guzik). In the Northern Hemisphere, it will be getting higher gradually after this. It is not observable after this in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   1 32.39   42  3.6   1.976   1.216    30   13.0   5:06 (235,-25)  
May   2   1 37.40   46 56.0   2.026   1.316    33   13.6   5:10 (228,-23)  

* C/2012 F3 ( PanSTARRS )

Now it is 14.9 mag (Apr. 1, Taras Prystavski). 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)  
Apr. 25  19 17.65   -9 57.0   3.071   3.461   104   13.3   5:06 (181, 65)  
May   2  19 21.45   -9 34.3   2.988   3.465   110   13.3   4:44 (180, 65)  

* 29P/Schwassmann-Wachmann 1

Now it is so faint as 17.1 mag (Apr. 17, A. Maury, J.-F. Soulier, T. Noel, J.-G. Bosch).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  17 57.38  -31 35.2   5.424   6.049   124   13.5   3:48 (180, 87)  
May   2  17 56.15  -31 40.0   5.334   6.047   131   13.5   3:19 (180, 87)  

* 22P/Kopff

Now it is 15.2 mag and visible visually (Mar. 18, Sandor Szabo). It will brighten up to 11 mag in 2015 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)  
Apr. 25  12 34.19    4 41.6   1.396   2.326   150   13.7  22:21 (180, 50)  
May   2  12 29.10    5  8.4   1.398   2.284   142   13.6  21:49 (180, 50)  

* C/2014 W11 ( PanSTARRS )

It brightened very rapidly. Now it is so bright as 14.6 mag and visible visually (Apr. 12, Sandor Szabo). It keeps 14-15 mag for a while after this. In the Northern Hemisphere, it will be getting lower gradually after May, and will be unobservable in mid June. In the Southern Hemisphere, it will be getting lower gradually after June, and will be unobservable in early August.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   8 54.47    9  8.6   3.145   3.450    99   14.3  18:49 (178, 46)  
May   2   8 58.69    8 48.3   3.234   3.444    93   14.3  18:42 (172, 46)  

* C/2012 K1 ( PanSTARRS )

It brightened up to 6.9 mag in 2014 autumn (Oct. 17, Marco Goiato). Now it is fading. But it is bright as 12.6 mag still now (Feb. 9, Chris Wyatt). In the Southern Hemisphere, it had been unobservable temporarily for a while, but it will be observable in good condition again after this. It will be observable again in mid June also in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   0 47.16  -16 53.9   4.264   3.500    35   14.4   5:06 (280, 15)  
May   2   0 49.59  -16 44.0   4.273   3.576    41   14.5   5:10 (276, 21)  

* C/2013 A1 ( Siding Spring )

It brightened up to 9 mag from autumn to winter in 2014. Now it is fading rapidly. It has already faded down to 14.2 mag (Apr. 11, Yasukazu Ikari). In the Northern Hemisphere, it will be observable in excellent condition after this while the comet will be fading. In the Southern Hemisphere, it is hardly observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  15 42.04   55 22.3   2.310   2.802   108   14.9   1:34 (180,  0)  
May   2  15 10.57   56 36.1   2.400   2.874   107   15.2   0:35 (180, -2)  

* C/2015 F4 ( Jacques )

Now it is 15.5 mag (Apr. 15, J. Oey, P. Camilleri, H. Williams). It is expected to brighten up to 12 mag from July to August. In the Southern Hemisphere, it keeps observable in good condition until summer. In the Northern Hemisphere, it will be getting higher gradually after May, and will be observable in good condition after summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  20 28.68  -39 17.7   1.855   2.175    94   15.2   5:06 (292, 75)  
May   2  20 37.05  -37 21.3   1.721   2.121    98   14.9   5:10 (287, 80)  

* 7P/Pons-Winnecke

It must have brightened up to 11 mag from January to February, but no observations have been reported. Now it is 16.3 mag (Mar. 29, A. Maury, J.-F. Soulier, J.-G. Bosch, T. Noel). In the Southern Hemisphere, it is observable in the morning sky after this while the comet will be fading. In the Northern Hemisphere, it will be getting higher after July, but the comet will be faitner than 17 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  23 59.71  -14 41.6   2.190   1.594    42   15.0   5:06 (272, 24)  
May   2   0 17.65  -13 44.7   2.202   1.643    44   15.1   5:10 (269, 26)  

* C/2015 D1 ( SOHO )

The spacecraft observed it brightened rapidly from 9 mag up to 2 mag when passing near by the sun. The nucleus has been already disintegrated, but the remnant was visible bright also on the earth (Mar. 7, Juan Jose Gonzalez). Now it is fainter than 10.3 mag (Mar. 17, Marek Biely). It locates high in the evening sky 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)  
Apr. 25   5  5.51   53 13.6   2.138   1.737    53   15.0  18:49 (149,-12)  
May   2   5 28.67   53 27.1   2.321   1.863    51   15.5  18:42 (149,-12)  

* C/2013 C2 ( Tenagra )

Very far object. However, outburst occured on Feb. 20, and it brightened up to 15 mag. It is bright as 15.8 mag still now (Mar. 28, Ken-ichi Kadota). It is reported so bright visually as 12.5 mag (Mar. 22, Marco Goiato). It locates high 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)  
Apr. 25  12  4.23  -21 57.5   8.265   9.143   149   15.2  21:52 (180, 77)  
May   2  12  2.96  -21 36.7   8.312   9.142   143   15.2  21:23 (180, 77)  

* 67P/Churyumov-Gerasimenko

Now it is 16.4 mag (Apr. 22, Jean-Francois Soulier). It will brighten up to 11 mag from August to October. In the Northern Hemisphere, it will be getting higher gradually after July, then it keeps observable in good condition. In the Southern Hemisphere, it keeps low until November.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   0 18.37   -2 48.9   2.563   1.784    31   15.5   5:06 (264, 13)  
May   2   0 35.80   -0 48.8   2.482   1.732    33   15.2   5:10 (260, 15)  

* C/2011 KP36 ( Spacewatch )

Now it is 15.3 mag (Mar. 28, Taras Prystavski). 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)  
Apr. 25  21 16.40   -2 30.9   5.849   5.655    73   15.4   5:06 (228, 47)  
May   2  21 19.88   -2  9.2   5.723   5.630    79   15.3   5:10 (218, 51)  

* 32P/Comas Sola

It brightened up to 13 mag in winter. Now it is fading, 15.2 mag (Apr. 12, Sandor Szabo). It keeps observable in good condition for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  11 12.27   17 58.6   1.856   2.587   126   15.3  21:00 (180, 37)  
May   2  11 13.33   17  6.1   1.960   2.623   120   15.5  20:33 (180, 38)  

* C/2014 N3 ( NEOWISE )

Now it is 15.3 mag (Jan. 7, Taras Prystavski). It keeps 15 mag for a long time from 2014 to 2015. It is observable in excellent condition in 2014 in the Southern Hemisphere, or in 2015 in the Northern Hemisphere. It becomes unobservable temporarily from March to May.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   1 25.06    9 56.7   4.883   3.900    10   15.4   5:06 (263, -8)  
May   2   1 30.71   11 27.6   4.865   3.906    15   15.4   5:10 (258, -3)  

* C/2006 S3 ( LONEOS )

It brightened up to 11-12 mag in 2012. It has already faded down to 15.2 mag (Mar. 16, Taras Prystavski). It keeps observable at 15 mag in good condition until summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  11  8.14   -5 56.3   8.622   9.361   135   15.4  20:55 (180, 61)  
May   2  11  5.34   -5 34.2   8.748   9.399   127   15.4  20:25 (180, 61)  

* 205P/Giacobini

First return of a comet re-discovered after 112-year blank in 2008. It brightened up to 12 mag in 2008. It is expected to brighten up to 15 mag from spring to summer in this apparition. It keeps locating low in the morning sky for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  23 12.08    2 22.2   2.092   1.550    44   15.5   5:06 (249, 23)  
May   2  23 32.58    3 52.3   2.058   1.542    46   15.4   5:10 (246, 25)  

* 218P/LINEAR

Now it is 16.0 mag recently (Apr. 17, A. Maury, J.-F. Soulier, T. Noel, J.-G. Bosch). In this apparition, it turns to approach to the sun down to 1.17 a.u., and it was expected to brighten up to 13 mag from March to May. But actually, it brightened up to 15.5 mag at best.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  19 45.80  -15  7.9   0.469   1.172    98   15.5   5:06 (200, 69)  
May   2  20 12.31  -13 30.5   0.473   1.177    98   15.6   5:10 (196, 68)  

* C/2010 S1 ( LINEAR )

Now it is 14.7 mag (Apr. 1, Taras Prystavski). It is observable at 15-16 mag in good condition in 2015.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  18 54.73  -19  9.5   7.230   7.653   111   15.6   4:45 (180, 74)  
May   2  18 52.03  -19 30.9   7.147   7.682   118   15.6   4:15 (180, 74)  

* C/2015 F2 ( Polonia )

Now it is 14.7 mag (Apr. 8, C. W. Hergenrother). It approaches to the earth, and brightens up to 15-16 mag from April to May. But it will be fainter than 18 mag in late July. It is observable in excellent condition in the Southern Hemisphere. It will be observable in excellent condition after May also in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  20 53.96  -27  2.5   0.733   1.202    85   15.7   5:06 (256, 68)  
May   2  21 13.22  -19 54.2   0.720   1.201    86   15.7   5:10 (237, 66)  

* 57P/du Toit-Neujmin-Delporte

Now it is 16.6 mag (Apr. 1, Taras Prystavski). It is expected to brighten up to 15 mag in summer, and will be observable in excellent condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  21 36.77  -11 20.2   1.782   1.747    71   15.8   5:06 (242, 50)  
May   2  21 53.59   -9 50.6   1.723   1.739    73   15.7   5:10 (236, 52)  

* C/2014 R1 ( Borisov )

It brightened up to 10.6 mag from autumn to winter (Nov. 29, Seiichi Yoshida). Now it is 14.3 mag (Mar. 24, Taras Prystavski). It will be fading graudually after this. But it keeps observable for a long time until the comet fades out.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  17 38.25  -14 41.1   1.776   2.534   129   15.7   3:29 (180, 70)  
May   2  17 34.35  -14 45.8   1.780   2.607   136   15.9   2:58 (180, 70)  

* C/2013 X1 ( PanSTARRS )

Now it is 14.8 mag and visible visually (Mar. 18, Sandor Szabo). 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. It is already unobservable in the Southern Hemisphere. In the Northern Hemispehre, it will be getting lower gradually and will be unobservable temporarily in mid May.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   4 48.84   33 24.0   5.329   4.629    41   15.8  18:49 (132,  0)  
May   2   4 51.10   33 21.6   5.341   4.562    35   15.7  18:42 (129, -3)  

* C/2013 V2 ( Borisov )

Now it is 14.8 mag (Mar. 21, Taras Prystavski). In the Northern Hemisphere, it keeps 15-16 mag and observable in excellent condition until early summer. It locates somewhat low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  12 52.08   31 45.0   3.181   3.923   131   15.9  22:39 (180, 23)  
May   2  12 48.13   30 41.2   3.256   3.951   127   16.0  22:08 (180, 24)  

* 116P/Wild 4

Now it is 17.6 mag (Apr. 17, A. Diepvens), fainter than predicted. It will brighten up to 13 mag in 2016. It will be getting lower after this, and will be unobservable in early June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   6 32.41   26 28.3   3.100   2.791    63   16.1  18:49 (145, 19)  
May   2   6 42.19   26 14.0   3.157   2.766    58   16.0  18:42 (143, 18)  

* C/2012 X1 ( LINEAR )

It brightened rapidly in outburst in mid October in 2013, then it keeps bright as 8-10 mag for a long time until 2014 summer. Now it is fading. It has already faded down to 15.8 mag (Feb. 9, Taras Prystavski). In the Southern Hemisphere, it keeps observable in good condition for a long time after this until the comet fades out. It is not observable in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   0 53.49  -31 51.7   5.701   5.087    48   16.6   5:06 (294, 22)  
May   2   1  0.09  -31 47.9   5.706   5.149    52   16.7   5:10 (292, 27)  

* C/2014 W9 ( PanSTARRS )

It brightened rapidly. Now it is 16.0 mag, much brighter than origianlly predicted (Mar. 28, Taras Prystavski). However, it will fade out rapidly after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  16 24.28  -32 26.5   0.892   1.802   143   16.6   2:15 (180, 87)  
May   2  16 21.73  -33 39.6   0.903   1.843   149   16.9   1:45 (180, 89)  

* 10P/Tempel 2

Now it is 16.7 mag (Apr. 19, J. Gonzalez). It keeps observable after this while the comet will be getting brighter graudually. 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)  
Apr. 25  14 37.39    6 10.1   1.409   2.377   159   16.8   0:29 (180, 49)  
May   2  14 30.48    6 54.2   1.369   2.334   157   16.7  23:49 (180, 48)  

* 51P/Harrington

It has not been observed yet in this apparition. But it must have already brightened up to 17 mag. It will be observable at 13 mag in good condition from summer to autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  21 59.37  -15 22.4   2.140   1.990    67   17.1   5:06 (252, 48)  
May   2  22 15.32  -14 14.3   2.048   1.958    70   16.8   5:10 (247, 51)  

* 110P/Hartley 3

It brightened up to 13.8 mag in winter (Feb. 15, Jakub Cerny). Now it is fading. It has already faded down to 16.8 mag (Apr. 11, N. Yanes). It will be getting lower after May. It will be unobservable in June in the Northern Hemisphere, or in July in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   7 19.67   17 34.7   2.670   2.594    74   16.8  18:49 (151, 32)  
May   2   7 29.57   17  2.9   2.765   2.607    70   17.0  18:42 (148, 32)  

* 299P/2014 D2 ( Catalina-PanSTARRS )

Now it is 17.7 mag (Feb. 17, K. Hills). It keeps observable at 17 mag from spring to summer. It locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  17 19.90  -28 49.9   2.384   3.155   132   16.9   3:11 (180, 84)  
May   2  17 18.50  -28 39.3   2.321   3.159   139   16.8   2:42 (180, 84)  

* C/2013 G9 ( Tenagra )

Now it is 16.3 mag (Apr. 19, Catalina Sky Survey). It keeps 17 mag for a long time from 2014 to 2016.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  11 13.78  -19 42.8   4.602   5.389   137   16.8  21:01 (180, 75)  
May   2  11  6.39  -18 55.1   4.691   5.397   130   16.9  20:26 (180, 74)  

* P/2014 X1 ( Elenin )

Brightened rapidly, and it kept brightening even after the perihelion passage. It brightened up to 15.8 mag and visible visually in March (Mar. 18, Sandor Szabo). But it will be fading after this. Now it is 16.8 mag (Apr. 17, T. Linder, R. Holmes). It is observable in excellent condition 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)  
Apr. 25   8 14.86   47 47.1   2.039   2.138    81   16.9  18:49 (172,  7)  
May   2   8 32.80   46 13.1   2.134   2.176    78   17.0  18:42 (172,  8)  

* 70P/Kojima

It Brightened up to 15.2 mag and visible visually in March (Mar. 18, Sandor Szabo). Now it is fading. It has already faded down to 17.0 mag (Apr. 18, E. Bryssinck). It keeps observable in good condition for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  11 46.78   11 35.0   1.644   2.479   137   17.0  21:34 (180, 44)  
May   2  11 46.61   11 19.1   1.732   2.508   130   17.1  21:07 (180, 44)  

* 221P/LINEAR

Now it is 18.3 mag (Apr. 19, Mt. Lemmon Survey). It will brighten rapidly, and will be observable at 16.5 mag in good condition from May to July.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  16 30.85  -21  9.7   0.978   1.891   144   17.2   2:21 (180, 76)  
May   2  16 32.45  -19 54.1   0.921   1.870   151   17.0   1:56 (180, 75)  

* 269P/2012 R2 ( Jedicke )

Now it is 16.7 mag (Apr. 14, Palomar Transient Factory). It keeps observable at 16-17 mag in good condition for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   8  6.51   13 59.7   4.118   4.180    86   17.1  18:49 (163, 39)  
May   2   8 11.09   13 51.6   4.228   4.188    80   17.2  18:42 (158, 38)  

* P/2015 F1 ( PanSTARRS )

Now it is 17.2 mag (Mar. 24, iTelescope Observatory, Siding Spring). It keeps 17 mag until July. 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)  
Apr. 25  16 46.05  -23 42.0   1.689   2.552   141   17.2   2:37 (180, 79)  
May   2  16 43.74  -23 48.7   1.642   2.555   148   17.2   2:07 (180, 79)  

* 318P/2014 M6 ( McNaught-Hartley )

First return of a periodic comet discovered in 1994. Now it is 17.5 mag (Mar. 23, iTelescope Observatory, Siding Spring). 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)  
Apr. 25  21 38.20  -32 35.5   2.943   2.919    78   17.3   5:06 (276, 60)  
May   2  21 49.00  -32 23.8   2.829   2.887    83   17.2   5:10 (273, 65)  

* 53P/Van Biesbroeck

Now it is 17.4 mag (Apr. 15, Catalina Sky Survey). It will brighten up to 14 mag and will be observable in good condition in 2016.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  12 39.26    2 41.1   2.771   3.696   152   17.3  22:26 (180, 52)  
May   2  12 35.77    3  4.1   2.787   3.661   145   17.3  21:55 (180, 52)  

* 61P/Shajn-Schaldach

It has not been observed yet in this apparition. But it must have already brightened up to 17 mag. 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)  
Apr. 25  23 10.48   -4  3.4   2.998   2.430    47   17.4   5:06 (254, 28)  
May   2  23 22.79   -2 55.0   2.913   2.406    50   17.3   5:10 (250, 31)  

* C/2012 K8 ( Lemmon )

Now it is 17.4 mag (Apr. 14, A. Klotz, F. Kugel, J. Nicolas, C. Rinner). It keeps observable at 17-18 mag for a long time from 2013 to 2016. It keeps locating high in the Northern Hemisphere. It keeps locating very low in the Southern Hemipshere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  16 34.98   63 49.4   6.459   6.678    98   17.3   2:25 (180, -9)  
May   2  16 22.07   64 38.8   6.481   6.690    97   17.3   1:45 (180,-10)  

* 40P/Vaisala 1

It brightened up to 15.5 mag from autumn to winter (Nov. 25, Taras Prystavski). Now it is fading. It has already faded down to 17.5 mag (Apr. 15, A. Diepvens). It keeps observable in good condition for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  17 59.12   -8 36.2   1.689   2.393   123   17.3   3:50 (180, 64)  
May   2  17 58.38   -8 21.9   1.663   2.434   129   17.4   3:21 (180, 63)  

* C/2013 G3 ( PanSTARRS )

Now it is 17.9 mag (Mar. 21, W. Hasubick). 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)  
Apr. 25  21 38.46   44 44.7   4.423   4.099    64   17.4   5:06 (204,  4)  
May   2  21 46.17   45 51.8   4.412   4.120    66   17.4   5:10 (200,  5)  

* C/2015 H1 ( Bressi )

Now it is 17.5 mag (Apr. 21, T. H. Bressi, R. A. Mastaler). It keeps 17 mag until summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  21 30.88    6 42.0   2.084   1.952    68   17.5   5:06 (224, 37)  
May   2  21 21.81    9 43.3   1.942   1.963    76   17.4   5:10 (211, 40)  

* 319P/2015 G1 ( Catalina-McNaught )

First return of a periodic comet discovered in 2008. Now it is 19 mag (Apr. 5, WISE). It will approach to the earth from spring to summer, and brighten rapidly. It will brighten up to 16 mag, and will be observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  20  9.26   -8  9.8   1.038   1.465    91   18.0   5:06 (208, 60)  
May   2  20 34.89   -7 43.3   0.964   1.418    91   17.7   5:10 (204, 61)  

* C/2013 U2 ( Holvorcem )

Now it is 17.0 mag (Apr. 1, Catalina Sky Survey). It was observed around 17-18 mag in early 2014. It will be observable around 17-18 mag again from 2014 autumn to 2015 spring, in excellent condition 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)  
Apr. 25   9 51.21   49  6.9   5.093   5.297    96   17.8  19:39 (180,  6)  
May   2   9 52.16   47 53.9   5.193   5.311    91   17.8  19:13 (180,  7)  

* 65P/Gunn

Now it is 17.9 mag (Apr. 8, A. Diepvens). Now it is around the aphelion. In the Northern Hemisphere, it is observable at 18 mag in good condition from winter to spring. It locates somewhat low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25   8 33.53   28  4.9   4.390   4.494    89   17.8  18:49 (173, 27)  
May   2   8 36.31   27 43.8   4.486   4.483    83   17.9  18:42 (169, 26)  

* C/2014 W6 ( Catalina )

Now it is 17.8 mag (Mar. 29, K. Hills). It keeps observable at 17 mag from winter to spring. It is 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)  
Apr. 25  10  8.06  -32  5.4   2.455   3.109   122   17.9  19:55 (180, 87)  
May   2  10  4.84  -32 15.7   2.529   3.117   116   18.0  19:25 (180, 87)  

* P/2012 B1 ( PanSTARRS )

It had been observed at 15 mag for a long time from 2013 to 2014. Now it is fading. It will be observable at 18 mag in good condition from spring to summer. It locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Apr. 25  19 35.01  -29  2.5   4.760   5.088   103   18.0   5:06 (216, 83)  
May   2  19 36.09  -29 12.3   4.677   5.109   109   17.9   4:59 (180, 84)  

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