Weekly Information about Bright Comets (2017 Aug. 26: South)

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Updated on August 29, 2017
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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/2017 O1 ( ASASSN )

New bright comet discovered by the All-Sky Automated Survey for Supernovae (ASASSN). Now it is bright as 8.7 mag (Aug. 25, Juan Jose Gonzalez). It is expected to brighten up to 7.5 mag in October. In the Northern Hemisphere, it stays observable in excellent condition for a long time. In the Southern Hemisphere, it is observable in good condition now. But it will be getting lower in September, and it will be unobservable for a long time after October.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   3 32.76    5 17.4   1.138   1.651   100    9.0   5:03 (185, 50)  
Sept. 2   3 43.37    9 35.5   1.045   1.613   103    8.7   4:54 (182, 45)  

* C/2015 V2 ( Johnson )

It brightened up to 7.1 mag from May to June (June 21, Juan Jose Gonzalez). Now it is fading. But it is bright as 10.3 mag still now (Aug. 23, Chris Wyatt). In the Southern Hemisphere, it is observable in good condition 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)  
Aug. 26  15  1.64  -42 39.5   1.745   1.913    83    9.7  19:00 ( 63, 62)  
Sept. 2  15 14.68  -45  0.4   1.860   1.961    80   10.0  19:05 ( 59, 59)  

* C/2015 ER61 ( PanSTARRS )

It brightened up to 6.2 mag in April (Apr. 7, Juan Jose Gonzalez). Now it is fading. But it is bright as 10.7 mag still now (Aug. 12, Seiichi Yoshida). It stays observable for a long time after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   3 54.03   23 29.3   1.678   1.980    91   10.6   5:03 (189, 31)  
Sept. 2   3 57.35   23 28.8   1.674   2.063    97   10.8   4:54 (185, 31)  

* 71P/Clark

Now it is bright as 10.9 mag (Aug. 10, Marco Goiato). 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)  
Aug. 26  17 47.29  -37 37.0   0.989   1.676   113   11.3  19:30 (  0, 87)  
Sept. 2  18  3.57  -37 20.9   1.056   1.698   110   11.5  19:18 (  0, 88)  

* 217P/LINEAR

Now it is bright as 12.2 mag (Aug. 21, Juan Jose Gonzalez). It stays 12 mag until September. In the Southern Hemisphere, it stays at the same altitude in the morning sky. In the Northern Hemisphere, it will be getting higher slowly.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   6  5.06   12  2.1   1.470   1.338    62   11.8   5:03 (228, 29)  
Sept. 2   6 24.72   11 57.6   1.477   1.374    63   11.9   4:54 (228, 29)  

* C/2016 R2 ( PanSTARRS )

Now it is 13.9 mag (Aug. 13, Thomas Lehmann). It will stay bright as 10 mag for a long time from autum to next spring. In the Southern Hemisphere, it stays observable in good condition until next February. In the Northern Hemispehre, it stays observable for a long time after this until the comet fades out.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   5 20.32   -3 32.8   3.823   3.703    75   12.6   5:03 (229, 48)  
Sept. 2   5 24.69   -3 14.3   3.685   3.655    80   12.5   4:54 (224, 50)  

* 29P/Schwassmann-Wachmann 1

Outburst occured on Aug. 27. Now it is very bright as 12.0 mag (Aug. 27, Luc Arnold).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  21 16.18  -14 20.7   4.844   5.823   164   13.2  22:56 (180, 69)  
Sept. 2  21 13.20  -14 28.9   4.881   5.822   156   13.2  22:26 (180, 69)  

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

Now it is 12.3 mag (Aug. 16, Juan Jose Gonzalez). It is observable at 13-14 mag in good condition until autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  21 15.13    2 45.6   1.751   2.720   159   13.4  22:53 (180, 52)  
Sept. 2  20 49.91   -0 15.2   1.797   2.721   150   13.5  22:01 (180, 55)  

* 213P/Van Ness

Now it is bright as 13.5 mag (Aug. 14, Chris Wyatt). It was expected to brighten up to 12 mag in summer. But actually, it is fainter than expected. 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)  
Aug. 26  18 50.67  -24 56.3   1.202   1.997   128   13.4  20:32 (180, 80)  
Sept. 2  18 54.38  -23 56.7   1.254   1.991   122   13.4  20:08 (180, 79)  

* C/2016 N4 ( MASTER )

Now it is 14.8 mag (Aug. 21, Gabor Santa). In the Northern Hemisphere, it will brighten up to 14 mag from summer to winter, and it will be observable in excellent condition. It is not observable at all after this in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  23 53.96   64 57.1   2.832   3.206   102   13.8   1:39 (180,-10)  
Sept. 2  23 32.31   67 11.8   2.800   3.202   104   13.8   0:50 (180,-12)  

* C/2015 O1 ( PanSTARRS )

Now it is 14.1 mag (Aug. 14, Chris Wyatt). It will be observable at 14 mag for a long time from 2017 to 2018.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  16 18.11   22  8.8   3.989   4.045    85   14.6  19:00 (163, 31)  
Sept. 2  16 13.96   21 39.9   4.071   4.022    80   14.6  19:05 (154, 29)  

* 65P/Gunn

Now it is 14.1 mag (June 30, Chris Wyatt). It stays 14 mag from spring to summer. It locates somewhat low in the Northern Hemisphere. The perihelion distance increased from 2.4 a.u. to 2.9 a.u. in this apparition. So it will not be bright as before.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  16  3.09  -24 28.8   2.727   2.922    90   14.6  19:00 (117, 71)  
Sept. 2  16  9.88  -24 53.7   2.816   2.919    85   14.6  19:05 (108, 66)  

* 96P/Machholz 1

Now it is 17.5 mag (Aug. 6, Jean-Francois Soulier). It will pass the perihelion on Oct. 27. In the Southern Hemisphere, it stays observable while the comet will be brightening, until early October when the comet will brighten up to 9 mag. In the Northern Hemisphere, it is not observable at all in this apparition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  14 23.76  -72 49.7   1.104   1.522    91   15.1  19:00 ( 18, 46)  
Sept. 2  14  4.81  -68 15.0   1.092   1.407    83   14.7  19:05 ( 26, 44)  

* P/2017 M2 ( LINEAR-NEAT )

Now it is 18.8 mag (Aug. 2, Mike Olason). Return of a new periodic comet which brightened up to 13 mag in 2004. It will be observable in excellent condition in autumn. It is expected to brighten up to 14 mag, if the comet is as bright as when it was discovered. But actually, it is not brightening as expected.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   2 23.50   -0 34.7   1.053   1.772   118   14.9   4:07 (180, 56)  
Sept. 2   2 31.22    0 12.1   0.992   1.757   122   14.7   3:47 (180, 55)  

* C/2016 M1 ( PanSTARRS )

Now it is 14.7 mag (Aug. 22, Kunihiro Shima). It is expected to brighten up to 9 mag in summer in 2018. In the Northern Hemisphere, it stays observable until 2018 summer while the comet will be brightening. In the Southern Hemisphere, it is hardly observable in 2017, but it will be observable in good condition in 2018.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  17  5.61   40 19.8   4.175   4.329    91   15.0  19:00 (177, 15)  
Sept. 2  17  3.84   38  9.9   4.171   4.272    88   15.0  19:05 (170, 16)  

* C/2016 N6 ( PanSTARRS )

Now it is 15.0 mag (Aug. 18, Gabor Santa). It is expected to brighten up to 11-12 mag from 2018 to 2019. In the Northern Hemisphere, it stays observable in good condition while the comet will be brightening gradually. In the Southern Hemisphere, it is not observable until 2018 October.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  14 58.06   54 39.7   4.459   4.218    69   15.1  19:00 (160, -5)  
Sept. 2  14 55.29   53 32.3   4.447   4.168    67   15.0  19:05 (155, -6)  

* 240P/NEAT

Although it was faint as 17.7 mag in July (July 8, ATLAS-MLO, Mauna Loa), now it is very bright as 13.8 mag (Aug. 22, Kunihiro Shima). It is observable in excellent condition in the Southern Hemisphere. It stays low for a while in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   0 44.02  -33  6.5   2.031   2.878   139   15.3   2:28 (180, 88)  
Sept. 2   0 40.86  -34  6.5   1.979   2.847   142   15.1   1:57 (180, 89)  

* C/2015 V1 ( PanSTARRS )

Now it is 15.3 mag (Aug. 22, Kunihiro Shima). It stays observable at 16 mag for a long time from 2017 to 2018.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   2 28.74   28 21.5   3.947   4.370   108   15.4   4:12 (180, 27)  
Sept. 2   2 22.42   27 30.2   3.814   4.358   116   15.3   3:39 (180, 27)  

* C/2011 KP36 ( Spacewatch )

Now it is 15.4 mag (Aug. 19, Gabor Santa). It stays observable at 16 mag unil the end of 2017.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   3 36.61    3 38.4   5.613   5.868    99   15.4   5:03 (187, 51)  
Sept. 2   3 38.08    3 17.9   5.538   5.895   105   15.4   4:54 (180, 52)  

* C/2017 K6 ( Jacques )

Now it is 17.0 mag (May 29, iTelescope Observatory, Siding Spring). It will brighten up to 14.5 mag in winter. In the Southern Hemisphere, it stays observable in excellent condition until spring in 2018. In the Northern Hemisphere, it stays unobservable until 2018.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   3  1.46  -78  5.0   2.084   2.530   104   15.6   4:43 (  0, 47)  
Sept. 2   3 17.12  -78 59.6   2.068   2.482   101   15.5   4:31 (  0, 46)  

* 47P/Ashbrook-Jackson

Now it is 16.5 mag (July 26, Toshiyuki Takahashi). It was observed at 17 mag in 2016. In 2017, it will be observable at 15.5 mag in good condition from summer to autumn. It is fainter than this ephemeris recently.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   1 44.12   15 44.5   2.176   2.853   122   15.7   3:28 (180, 39)  
Sept. 2   1 43.45   16 21.5   2.110   2.859   129   15.6   3:00 (180, 39)  

* 352P/2017 L1 ( Skiff )

First return of a new periodic comet discovered in 2000. Now it is 17.3 mag (July 17, Mike Olason). It will brighten rapidly, and it is expected to be observable at 15.5 mag in good condition from July to September. But actually, it is fainter than this ephemeris.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   1 16.34   -8 53.9   1.770   2.596   136   15.7   3:00 (180, 64)  
Sept. 2   1 13.83   -8 33.1   1.731   2.609   142   15.8   2:30 (180, 63)  

* C/2017 K4 ( ATLAS )

Now it is 15.7 mag (July 18, Ken-ichi Kadota). It stays 16 mag for a long time until summer in 2018. In the Southern Hemisphere, it stays observable in excellent condition until autumn. It locates low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  16 55.38  -30 30.2   2.572   2.969   103   15.8  19:00 (131, 83)  
Sept. 2  17  1.22  -29 51.3   2.629   2.939    97   15.8  19:05 (113, 78)  

* 24P/Schaumasse

Now it is 19.0 mag (July 26, Jean-Gabriel Bosch). It will brighten very rapidly, and brighten up to 10 mag from October to December. It is observable in good condition in the Northern Hemisphere. It locates very low for a long time in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   6 49.48   21 41.1   2.022   1.597    51   16.7   5:03 (230, 15)  
Sept. 2   7 13.56   21 43.8   1.936   1.544    52   15.9   4:54 (231, 14)  

* 145P/Shoemaker-Levy 5

Now it is 16.0 mag (Aug. 19, Gabor Santa). It will brighten rapidly, up to 15 mag in autumn, and will be observable in good condition in the Northern Hemisphere. It locates low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   4 16.28   23  0.4   1.678   1.905    86   16.2   5:03 (195, 30)  
Sept. 2   4 29.64   24 19.9   1.615   1.904    89   16.1   4:54 (193, 29)  

* C/2014 OE4 ( PanSTARRS )

Now it is 16.0 mag (Aug. 22, Kunihiro Shima). It stays 16 mag from 2016 to 2017. 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)  
Aug. 26  17 47.46   64 47.4   6.418   6.490    89   16.5  19:27 (180,-10)  
Sept. 2  17 46.68   64 18.5   6.435   6.504    89   16.6  19:05 (179, -9)  

* C/2017 D2 ( Barros )

Now it is 15.6 mag (Aug. 22, Kunihiro Shima). It will brighten up to 16 mag in summer. It will be observable in excellent condition in the Southern Hemisphere. It will be getting higher gradually in the morning sky also in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  21 20.24  -25  3.3   1.555   2.528   159   16.6  23:00 (180, 80)  
Sept. 2  21 14.72  -23 11.3   1.599   2.543   153   16.7  22:27 (180, 78)  

* (457175) 2008 GO98

Hilda-type minor planet, but the cometary activity was detected on July 3. Now it is bright as 16.5 mag (July 3, G. J. Leonard).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  20 59.41    0 38.8   2.448   3.403   157   16.8  22:40 (180, 54)  
Sept. 2  20 56.12   -0  9.3   2.497   3.420   151   16.8  22:09 (180, 55)  

* 189P/NEAT

Now it is 19.3 mag (Aug. 23, Michael Jager). It brightens up to 16.5-17 mag in August, and it will be observable in good condition. But actually, it is much fainter than this ephemeris.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  17 37.85    7 40.6   0.468   1.237   107   16.9  19:20 (180, 47)  
Sept. 2  18  1.33   10 22.8   0.506   1.255   107   17.0  19:16 (180, 44)  

* (944) Hidalgo

Now it is 17.9 mag (June 2, MASTER-OAFA Observatory). It will brighten up to 14 mag from autumn to winter in 2018, and it will be observable in excellent condition in the Northern Hemisphere. In 2017, it is observable at 17 mag in excellent condition in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   0  8.67  -45 33.9   3.323   4.128   137   17.1   1:53 (  0, 80)  
Sept. 2   0  1.64  -45 59.7   3.275   4.086   138   17.1   1:18 (  0, 79)  

* C/2017 M4 ( ATLAS )

Now it is 17.4 mag (July 20, Yuji Ohshima). It is expected to brighten up to 13-14 mag from 2018 to 2019. In the Northern Hemisphere, it stays observable in good condition for a long time. In the Southern Hemisphere, it is not observable until summer in 2018.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  19  7.28   67  5.5   5.435   5.616    95   17.2  20:46 (180,-12)  
Sept. 2  18 55.46   65 40.7   5.383   5.569    95   17.1  20:07 (180,-11)  

* C/2010 U3 ( Boattini )

It will pass the perihelion in 2019. However, it has not been brightening since the discovery in 2010. It will be getting higher gradually in the morning sky in the Northern Hemisphere. It is not observable for a long time in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   6 24.02   65 56.1   9.374   9.043    67   17.1   5:03 (198,-17)  
Sept. 2   6 30.60   66 30.8   9.285   9.029    72   17.1   4:54 (197,-17)  

* 62P/Tsuchinshan 1

Now it is 18.5 mag (Aug. 13, Francois Kugel). It brightens rapidly, and brightens up to 11 mag from autumn to winter. It is observable in good condition in the Northern Hemisphere. It locates low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   6 25.98   19 51.2   1.976   1.653    56   17.5   5:03 (226, 20)  
Sept. 2   6 48.08   19 58.3   1.898   1.614    58   17.1   4:54 (227, 19)  

* 130P/McNaught-Hughes

Now it is 17.9 mag (May 27, T. Ikemura, H. Sato). It will be brightening slowly until autumn when it becomes 16.5-17 mag. It will be getting lower gradually in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  14 57.58  -17 11.3   2.251   2.203    74   17.3  19:00 (110, 54)  
Sept. 2  15  8.00  -18  8.3   2.298   2.173    70   17.2  19:05 (104, 50)  

* 81P/Wild 2

It brightened up to 11 mag from spring to summer in 2016. Now it is 17.4 mag (July 14, Ken-ichi Kadota). It stays observable for a long time after this, but it will be fainter than 18 mag in October.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  19 33.54  -20 41.9   2.708   3.534   139   17.2  21:14 (180, 76)  
Sept. 2  19 31.40  -20 52.0   2.815   3.567   131   17.4  20:45 (180, 76)  

* 90P/Gehrels 1

Now it is 18.0 mag (Aug. 22, Kunihiro Shima). In the Northern Hemisphere, it will be observable at 17 mag in excellent condition from autumn to winter. It locates low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   5  0.81   29 23.9   3.098   3.014    75   17.5   5:03 (204, 21)  
Sept. 2   5  9.22   29 57.7   3.018   3.022    80   17.4   4:54 (201, 22)  

* 188P/LINEAR-Mueller

It was observed at 17 mag in 2016. It stays 17 mag also in 2017. It is observable in good 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)  
Aug. 26   6 16.97   32 25.4   3.245   2.868    59   17.4   5:03 (217, 11)  
Sept. 2   6 27.61   32 37.8   3.185   2.888    63   17.4   4:54 (215, 12)  

* 73P/Schwassmann-Wachmann 3

It brightened up to 11.5 mag from late March to early April (Mar. 24, Andrew Pearce). Now it is fading. It has already faded down to 17.3 mag (Aug. 24, Michael Jager). Bright 12-mag new fragment BT was discovered on Feb. 10, but now it is faint as 18.9 mag (June 2, CAO, San Pedro de Atacama). It will be fainter than 18 mag in September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   3 14.57    6 47.3   1.715   2.196   104   17.7   4:58 (180, 48)  
Sept. 2   3 14.37    6 36.0   1.686   2.255   111   17.8   4:30 (180, 48)  

* 2016 ND21

Peculiar asteroid moving along a comet-like orbit. It is observable at 18 mag in good condition from August to September. It locates somewhat low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26  22 35.08   17 52.4   2.846   3.764   151   17.8   0:19 (180, 37)  
Sept. 2  22 31.10   17 57.2   2.832   3.764   153   17.7  23:43 (180, 37)  

* C/2017 E1 ( Borisov )

It brightened up to 11 mag from March to April. Now it is fading. It has faded down to 12.7 mag in late May (May 26, iTelescope Observatory, Siding Spring). No observations have been reported after that.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 26   4 21.69    5 52.5   2.169   2.364    88   17.8   5:03 (203, 47)  
Sept. 2   4 24.32    5 13.8   2.162   2.451    94   18.0   4:54 (197, 48)  

* C/2015 H2 ( PanSTARRS )

Now it is 18.3 mag (June 20, P. Camilleri, H. Williams). It stays observable at 18 mag from spring to summer. 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)  
Aug. 26  22  5.04  -33 53.8   4.690   5.630   156   17.9  23:45 (180, 89)  
Sept. 2  22  1.11  -33 37.9   4.741   5.655   152   17.9  23:14 (180, 89)  

* 2P/Encke

It brightened up to 7.2 mag in spring (Mar. 24, Marco Goiato). Now it is 16.9 mag (June 2, T. Ikemura, H. Sato). It will be fainter than 18 mag in late August. It is observable in good 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)  
Aug. 26  20 22.73  -26 16.5   1.577   2.495   148   17.9  22:03 (180, 81)  
Sept. 2  20 15.03  -26  5.8   1.696   2.554   140   18.2  21:28 (180, 81)  

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