Weekly Information about Bright Comets (2016 June 11: South)

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Updated on June 11, 2016
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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 X1 ( PanSTARRS )

Now it is bright as 6.4 mag (June 8, Marco Goiato). It keeps 6-7 mag until mid July. In the Southern Hemisphere, it keeps observable in excellent condition after this. In the Northern Hemisphere, it locates low in the south.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  21 53.56  -29 37.2   0.741   1.518   118    6.2   4:37 (180, 84)  
June 18  20 42.18  -40 42.2   0.653   1.571   139    6.0   3:00 (  0, 85)  

* C/2014 S2 ( PanSTARRS )

Now it is 11.6 mag (June 8, Chris Wyatt). It will be fading slowly after this. In the Northern Hemisphere, it will be getting lower gradually and will be unobservable in August. It is observable in the evening sky also in the Southern Hemisphere until August.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  11  5.72   31  2.3   3.047   2.968    75   11.2  18:25 (171, 24)  
June 18  11  9.49   28 29.2   3.189   3.021    71   11.4  18:25 (165, 25)  

* 9P/Tempel 1

Now it is 11.6 mag (June 9, Marco Goiato). It keeps 11-12 mag until September. In the Northern Hemisphere, it will be getting lower gradually after this. In the Southern Hemisphere, it keeps observable in good condition for a long time.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  12  5.06    8 14.2   1.145   1.626    97   11.6  18:45 (180, 47)  
June 18  12 14.71    5 54.5   1.175   1.606    94   11.5  18:27 (180, 49)  

* 81P/Wild 2

Now it is 10.9 mag (May 24, Thomas Lehmann). It keeps 11 mag until summer. In the Northern Hemisphere, it will be unobservable soon. It locates somewhat low in the Southern Hemisphere, but it keeps observable until August.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   8 39.90   19 10.5   2.153   1.640    47   11.7  18:25 (133, 21)  
June 18   8 59.24   18  3.2   2.173   1.624    45   11.6  18:25 (131, 20)  

* 252P/LINEAR

It passed only 0.036 a.u. from the earth on Mar. 21-22, and brightened up to 3.9 mag (Mar. 21, Thomas Lehmann). It kept brightening even after the perihelion passage. However, it is fading rapidly now. It has already faded down to 12.6 mag (June 5, Alan Hale). It keeps observable in excellent condition for a while after this both in the Northern Hemisphere and Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  16 39.17    4 52.7   0.558   1.526   150   11.8  23:18 (180, 50)  
June 18  16 36.42    3 22.0   0.632   1.588   148   12.7  22:48 (180, 52)  

* C/2015 WZ ( PanSTARRS )

Now it is bright as 12.5 mag (June 6, Michael Jager). It is observable in excellent conditione in the Northern Hemisphere. It locates very low in the Southern Hemisphere. It will fade out rapidly after July.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  20 24.30   52 37.9   1.162   1.597    94   12.4   3:09 (180,  2)  
June 18  19  8.40   53 20.9   1.116   1.649   101   12.7   1:26 (180,  2)  

* 43P/Wolf-Harrington

It will brighten up to 11 mag from summer to autumn. However, it was faint as 18.2 mag in February (Feb. 17, Alexander Baransky), fainter than this ephemeris by 2 mag. Now it is appearing in the morning sky, but it keeps low for some time.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   3  8.40   24 19.1   2.365   1.564    29   12.7   5:34 (235,  5)  
June 18   3 31.97   25  5.3   2.311   1.528    30   12.4   5:36 (234,  6)  

* C/2014 W2 ( PanSTARRS )

Now it is 12.6 mag (June 3, Giuseppe Pappa). It keeps 12-13 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 until July in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  16  0.32   65  5.0   2.642   2.840    90   12.5  22:37 (180,-10)  
June 18  15 42.68   61 59.3   2.661   2.866    91   12.5  21:53 (180, -7)  

* C/2013 US10 ( Catalina )

Now it is 13.4 mag (May 22, Ken-ichi Kadota). It brightened up to 6 mag from autumn to winter. Now it is fading. It is not observable after this in the Southern Hemisphere. It will be extremely low from May to June also in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   5 25.27   46 42.6   4.146   3.242    23   13.2  18:25 (130,-28)  
June 18   5 30.98   46 49.7   4.229   3.323    23   13.3   5:36 (230,-26)  

* 29P/Schwassmann-Wachmann 1

Now it is 14.8 mag (June 10, Jean-Francois Soulier). It is observable in excellent condition in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  19 50.44  -25 26.7   5.068   5.930   145   13.3   2:33 (180, 80)  
June 18  19 47.82  -25 31.1   5.009   5.928   152   13.3   2:03 (180, 80)  

* P/2016 J3 ( STEREO )

New comet discovered from the STEREO spacecraft images in May. It brightened up to 8 mag due to the forward scattering. In the Southern Hemisphere, it is appearing in the evening sky, and it will be getting higher rapidly. It it not observable in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   7 28.94    7 28.8   1.136   0.660    35   13.5  18:25 (112, 17)  
June 18   8 19.25    3 11.7   1.113   0.769    42   14.1  18:25 (112, 24)  

* 116P/Wild 4

Now it is 13.2 mag (June 3, Giuseppe Pappa). It keeps 13 mag for a while. 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)  
June 11  15 21.46  -22 42.1   1.475   2.425   153   14.0  22:00 (180, 78)  
June 18  15 19.06  -22 34.2   1.536   2.445   146   14.1  21:31 (180, 78)  

* 53P/Van Biesbroeck

Now it is 14.4 mag (June 8, Chris Wyatt). It will be observable at 14 mag in good condition from spring to summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  21 12.51  -10 57.9   1.746   2.451   122   14.1   3:55 (180, 66)  
June 18  21 14.86  -10 55.6   1.690   2.460   129   14.0   3:29 (180, 66)  

* 118P/Shoemaker-Levy 4

It is not observable now. It will be observable at 16.5 mag in September in the Northern Hemisphere, or in November in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   5 51.12   18 31.1   2.977   1.981     9   14.2  18:25 (106, -9)  
June 18   6  8.93   18 41.1   2.985   1.980     6   14.2  18:25 (105,-11)  

* C/2011 KP36 ( Spacewatch )

Now it is 15.1 mag (Jan. 2, Ken-ichi Kadota). 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)  
June 11   0 27.74    2  9.1   5.083   4.885    73   14.4   5:34 (216, 47)  
June 18   0 32.33    2 19.4   4.984   4.886    78   14.4   5:36 (208, 49)  

* 77P/Longmore

Now it is bright as 13.7 mag (June 3, Giuseppe Pappa). In the Northern Hemisphere, it will be getting lower gradually after this, and it will be unobservable in late July. In the Southern Hemisphere, it keeps observable in good condition until autumn. But it will be fading slowly after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  12 32.67  -18 45.9   1.742   2.345   113   14.5  19:12 (180, 74)  
June 18  12 35.76  -19 37.6   1.821   2.350   108   14.6  18:48 (180, 75)  

* 146P/Shoemaker-LINEAR

Now it is 15.9 mag (May 4, Hidetaka Sato), brighter than originally predicted. It will brighten up to 14 mag in summer. In the Southern Hemisphere, it keeps observable until winter, but it locates somewhat low. In the Northern Hemisphere, it is not observable now. It will appear in the morning sky in July, then it will be observable in excellent condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   2 20.05   -1 34.9   1.878   1.447    49   14.7   5:34 (247, 31)  
June 18   2 40.15    1  1.0   1.852   1.437    50   14.6   5:36 (243, 31)  

* C/2015 TQ209 ( LINEAR )

It will brighten up to 13 mag in summer. But it keeps unobservable for a long time. It will appear in the morning sky in December, when the comet will be fainter than 15 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   5 46.31   18  5.2   2.788   1.789     8   14.8  18:25 (105,-10)  
June 18   6  6.26   17 52.8   2.736   1.732     7   14.6  18:25 (104,-11)  

* C/2015 T4 ( PanSTARRS )

Now it is bright as 14.9 mag (May 4, Hidetaka Sato). It keeps 15 mag until autumn. In the Southern Hemisphere, it keeps observable for a long time. It will be unobservable after this in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   5 44.80  -40  1.3   2.565   2.298    63   15.0  18:25 ( 55, 22)  
June 18   6  2.74  -41 58.3   2.524   2.296    65   14.9  18:25 ( 53, 21)  

* C/2015 V2 ( Johnson )

Now it is 14.8 mag (May 19, Artyom Novichonok). It is expected to brighten up to 7 mag in 2017 summer. In the Northern Hemisphere, it becomes low temporarily in summer, but it keeps observable in good condition until the highlight while the comet will be brightening. In the Southern Hemisphere, it is not observable until early 2017.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   7 51.76   56 14.7   5.241   4.558    43   15.2  18:25 (151,-14)  
June 18   8  2.18   55 47.5   5.214   4.494    40   15.1  18:25 (149,-15)  

* C/2014 W11 ( PanSTARRS )

It brightened very rapidly in 2015 spring, and reached up to 13.8 mag (2015 May 11, Sandor Szabo). It is bright as 14.4 mag still now (May 12, Yasukazu Ikari). 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)  
June 11  13 40.38  -26 12.1   3.570   4.303   130   15.8  20:20 (180, 81)  
June 18  13 40.72  -25 48.1   3.675   4.332   124   15.9  19:53 (180, 81)  

* C/2015 ER61 ( PanSTARRS )

Now it is 16.3 mag (May 20, Artyom Novichonok). It is expected to brighten up to 7 mag in 2017 spring. But it locates somewhat low at the high light.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  11  7.79   -0  5.1   4.390   4.467    87   16.2  18:25 (164, 54)  
June 18  11  9.61   -0  6.1   4.430   4.397    81   16.2  18:25 (153, 52)  

* 65P/Gunn

Now it is 16.5 mag (May 31, Michael Jager). It will be getting lower after this, and will be unobservable in August. It will brighten up to 14 mag in 2017. The perihelion distance increases from 2.4 a.u. to 2.9 a.u. in this apparition, and the comet will not brighten as before.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  11 27.22   12 16.8   3.576   3.672    87   16.3  18:25 (174, 43)  
June 18  11 30.67   11 35.0   3.661   3.656    81   16.4  18:25 (166, 42)  

* C/2015 O1 ( PanSTARRS )

Now it is 17.2 mag (May 8, Space Surveillance Telescope, Atom Site). It will be observable at 13 mag for a long time from 2017 to 2018. In 2016, it keeps observable at 16-17 mag in good condition until autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  20  1.84  -11 51.7   5.578   6.384   139   16.6   2:44 (180, 67)  
June 18  19 56.30  -11 34.7   5.463   6.340   147   16.5   2:11 (180, 67)  

* 22P/Kopff

It brightened up to 10 mag in 2015 autumn. Now it is appearing in the morning sky, but it must be already fainter than 16 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   2 23.75   10 19.0   3.247   2.604    43   16.6   5:34 (238, 22)  
June 18   2 33.50   11  0.6   3.223   2.646    47   16.7   5:36 (234, 25)  

* C/2016 B1 ( NEOWISE )

Now it is bright as 15.9 mag (Apr. 9, Hidetaka Sato). It keeps 16 mag for a long time from 2016 to 2017. In 2016, it is observable in excellent condition in the Southern Hemisphere, but it locates extremely low in the Northern Hemispehre.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  12  7.40  -30 52.6   3.115   3.617   111   16.6  18:47 (180, 86)  
June 18  12 12.01  -29 19.0   3.165   3.587   106   16.6  18:25 (178, 84)  

* C/2014 Q2 ( Lovejoy )

It brightened up to 3.7 mag and became a naked eye comet in mid January in 2015 (Jan. 13, Marek Biely). Now it is fading. It has already faded down to 16.0 mag (May 7, Yuji Ohshima). In the Northern Hemisphere, it keeps observable for a long time until the comet fades out. It locates somewhat low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  17 53.32   26 42.9   5.183   5.881   129   16.6   0:36 (180, 28)  
June 18  17 47.79   26 22.1   5.236   5.943   130   16.7   0:03 (180, 29)  

* C/2015 B2 ( PanSTARRS )

Now it is 17.0 mag (Feb. 7, iTelescope Observatory, Siding Spring). It keeps 16.5 mag for a long time in 2016, and it will be observable in excellent condition in the Southern Hemisphere. It is hardly observable in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   3 43.25  -36 50.6   3.707   3.386    63   16.6   5:34 (295, 33)  
June 18   3 44.29  -37  2.7   3.659   3.393    66   16.6   5:36 (293, 38)  

* C/2014 OE4 ( PanSTARRS )

Now it is 16.5 mag (May 11, D. Buczynski). It keeps 16.5 mag from 2016 to 2017. It is observable in good condition in the Northern Hemisphere. In the Southern Hemisphere, it locates low in 2016, and it is not observable in 2017.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  17  0.19   34  4.9   5.763   6.369   122   16.7  23:38 (180, 21)  
June 18  16 55.73   34 38.6   5.781   6.360   120   16.7  23:06 (180, 20)  

* 237P/LINEAR

It brightened rapidly up to 15.6 mag (May 13, iTelescope Observatory, Siding Spring). It keeps observable at 16 mag until autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  12 58.05  -14 43.4   1.535   2.207   118   16.7  19:38 (180, 70)  
June 18  13  2.71  -14  2.3   1.581   2.185   112   16.7  19:15 (180, 69)  

* C/2014 R3 ( PanSTARRS )

Now it is 16.9 mag (May 7, K. Sarneczky). It brightened rapidly, and became brighter than originally expected. It keeps 17 mag until 2017. 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)  
June 11  13 38.64   72 26.8   7.434   7.285    77   16.9  20:17 (180,-17)  
June 18  13 27.80   71 25.3   7.472   7.283    75   16.9  19:39 (180,-16)  

* C/2014 A4 ( SONEAR )

It brightened up to 15 mag from late 2014 to early 2016. Now it is fading slowly. In the Northern Hemisphere, it will be observable at 17 mag in autumn in good condition. It locates extremely low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   0 21.19   34 48.0   5.130   4.781    64   16.9   5:34 (199, 17)  
June 18   0 18.79   36  1.3   5.056   4.809    70   16.9   5:36 (192, 18)  

* C/2015 LC2 ( PanSTARRS )

Now it is 16.4 mag (May 10, Catalina Sky Survey). It keeps brightening even after the perihelion passage. It keeps observable at 17 mag in good condition until autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  14 41.25    6 30.6   5.827   6.546   131   16.9  21:20 (180, 49)  
June 18  14 38.54    7  3.1   5.933   6.567   124   17.0  20:50 (180, 48)  

* P/2008 J3 ( McNaught )

First return of a new periodic comet which brightened up to 16.5 mag in 2008. The condition of this apparition is very good. It is expected to brighten up to 15.5 mag in autumn and will be observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  23 58.42  -21 43.5   2.379   2.581    89   17.1   5:34 (232, 70)  
June 18   0  5.65  -21  0.6   2.278   2.560    94   17.0   5:36 (217, 73)  

* 219P/LINEAR

Now it is 19.3 mag (May 4, Hidetaka Sato). It will brighten up to 16.5 mag in summer and will be observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  18  7.39  -12 45.3   1.866   2.857   164   17.1   0:50 (180, 68)  
June 18  18  2.10  -12 16.4   1.832   2.835   168   17.0   0:18 (180, 67)  

* 100P/Hartley 1

It brightened rapidly up to 15.1 mag in May (May 12, Yuji Ohshima). It will fade out rapidly after this. 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)  
June 11  14 44.68  -39 32.6   1.175   2.082   143   17.1  21:24 (  0, 85)  
June 18  14 40.44  -40 11.5   1.232   2.097   137   17.3  20:52 (  0, 85)  

* 188P/LINEAR-Mueller

It is expected to brighten up to 16 mag and observable in good condition in autumn. However, it is so faint as 19.7 mag now (Apr. 16, A. Maury, J.-B. de Vanssay, J.-G. Bosch, J.-F. Soulier).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  23  5.30  -13 23.1   2.748   3.059    98   17.3   5:34 (189, 68)  
June 18  23  9.81  -12 55.3   2.634   3.036   103   17.1   5:24 (180, 68)  

* C/2012 F3 ( PanSTARRS )

It brightened up to 13-14 mag from 2014 to 2015. Now it is fading. It has already faded down to 18.1 mag (Apr. 23, Slooh.com Canary Islands Observatory). It will be observable at 17 mag in 2016.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  23 22.07   -2 48.1   5.057   5.160    90   17.2   5:34 (194, 57)  
June 18  23 24.11   -2 42.4   4.993   5.203    96   17.2   5:36 (181, 58)  

* C/2010 S1 ( LINEAR )

It was observed as bright as 13-14 mag for a long time from 2011 to 2014. Now it is fading. It is observable in excellent condition in the Southern Hemisphere. It locates extremely low in the Northern Hemisphere. No observations have been reported since August, 2015.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  17 36.51  -36 56.5   8.573   9.559   165   17.4   0:20 (  0, 88)  
June 18  17 31.64  -37  7.6   8.605   9.593   165   17.4  23:43 (  0, 88)  

* C/2015 H2 ( PanSTARRS )

Now it is 18.0 mag (Apr. 12, A. Maury, J.-B. de Vanssay, J.-G. Bosch, J.-F. Soulier). It keeps observable at 17.5 mag in good condition from spring to autumn in the Southern Hemisphere. It is not observable in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  18  3.40  -64 27.8   4.220   5.020   137   17.6   0:47 (  0, 61)  
June 18  17 58.09  -64 30.5   4.203   5.013   138   17.6   0:14 (  0, 60)  

* 47P/Ashbrook-Jackson

Now it is 18.5 mag (Apr. 14, Hidetaka Sato). It will brighten up to 16 mag and will be observable in good condition in 2017. In 2016, it is observable in excellent condition in the Southern Hemisphere, but it keeps low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  19 26.91  -39 32.2   2.534   3.438   148   17.7   2:10 (  0, 86)  
June 18  19 22.47  -39 53.8   2.477   3.419   153   17.6   1:38 (  0, 85)  

* C/2016 K1 ( LINEAR )

Now it is 17.5 mag (June 3, iTelescope SRO Observatory, Auberry). It keeps 17-18 mag until autumn. It keeps observable in excellent condition in the Northern Hemisphere. It will be getting lower gradually in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  23 20.18    2  6.2   2.110   2.320    88   17.8   5:34 (192, 52)  
June 18  23 15.17    5 26.2   1.985   2.308    95   17.6   5:30 (180, 50)  

* 180P/NEAT

Now it is 16.8 mag (May 10, Catalina Sky Survey). It will be fading after this, and will be fainter than 18 mag soon.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  14 27.59   -0  5.1   1.949   2.742   132   17.7  21:07 (180, 55)  
June 18  14 26.52   -1  4.8   2.030   2.760   126   17.9  20:38 (180, 56)  

* P/2006 F1 ( Kowalski )

Although it was bright as 17 mag at the discovery in 2006, it faded out before the perihelion passage in 2008, and it became lost. Now it is fainter than 19 mag (May 30, Jean-Francois Soulier).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  15 34.01    6 18.1   3.632   4.469   141   17.8  22:13 (180, 49)  
June 18  15 30.96    5 59.5   3.678   4.462   135   17.8  21:42 (180, 49)  

* C/2013 C2 ( Tenagra )

Very far object. Outburst occured on Feb. 20, 2015, and it brightened up to 15 mag. Now it is 16.7 mag (Apr. 4, Hidetaka Sato). 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)  
June 11  13 10.69  -22 52.2   8.592   9.193   123   17.8  19:50 (180, 78)  
June 18  13 10.67  -22 36.0   8.688   9.196   117   17.8  19:23 (180, 78)  

* P/2008 T1 ( Boattini )

It has not been observed in this apparition yet. It will brighten up to 17.5 mag in summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11  20 45.10  -17 53.3   2.408   3.172   131   17.9   3:27 (180, 73)  
June 18  20 44.26  -17 52.1   2.331   3.163   138   17.8   2:59 (180, 73)  

* C/2014 Y1 ( PanSTARRS )

Now it is 16.8 mag (Apr. 12, Hidetaka Sato). It was expected to brighten up to 14 mag from winter to summer. But it is much fainter actually. It will be 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)  
June 11  16 11.64  -40  9.7   1.810   2.777   157   18.1  22:51 (  0, 85)  
June 18  16  8.32  -40  4.8   1.877   2.823   153   18.3  22:20 (  0, 85)  

* 333P/LINEAR

First return of an object discovered as an asteroid 2007 VA85 in 2007. It brightened very rapidly since mid February, and brightened up to 11.3 mag in spring (Mar. 5, Juan Jose Gonzalez). In the Northern Hemisphere, it located extremely low in May, but it is appearing in the morning sky again. However, it may fade out very rapidly and may be fainter than 18 mag. It keeps unobservable until September in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
June 11   2 44.94   48 51.2   2.075   1.445    39   18.6   5:34 (215, -9)  
June 18   2 37.74   50 44.1   2.030   1.503    45   18.7   5:36 (209, -6)  

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