Weekly Information about Bright Comets (2017 July 29: South)

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Updated on August 2, 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/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 8.5 mag still now (July 26, Marco Goiato). In the Northern Hemisphere, it will be unobservable in August. In the Southern Hemisphere, it is observable in good condition after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29  14 23.72  -30  7.8   1.302   1.752    97    8.8  18:43 (111, 79)  
Aug.  5  14 30.94  -33 50.2   1.409   1.787    93    9.0  18:47 ( 88, 75)  

* C/2015 ER61 ( PanSTARRS )

Outburst occured on Apr. 4, and it brightened by 2 mag, up to 6.2 mag (Apr. 7, Juan Jose Gonzalez). Now it is fading. But it is bright as 11.2 mag still now (July 25, Chris Wyatt). It stays observable for a long time after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29   3 23.45   22 29.9   1.661   1.652    71    9.8   5:29 (203, 29)  
Aug.  5   3 33.58   22 55.0   1.672   1.733    75   10.0   5:24 (200, 29)  

* C/2017 O1

New bright comet discovered by the All-Sky Automated Survey for Supernovae (ASASSN). Now it is bright as 9.8 mag (July 23, 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)  
July 29   2 48.57   -7 17.5   1.563   1.844    88   10.1   5:29 (207, 60)  
Aug.  5   2 59.82   -4 40.4   1.452   1.791    91    9.8   5:24 (200, 58)  

* 71P/Clark

Now it is bright as 10.6 mag (July 26, 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)  
July 29  16 52.86  -37  2.9   0.765   1.610   128   10.6  20:25 (  0, 88)  
Aug.  5  17  4.31  -37 26.5   0.814   1.623   124   10.8  20:09 (  0, 88)  

* 217P/LINEAR

Now it is bright as 12.2 mag (July 25, Chris Wyatt). 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)  
July 29   4 33.57   10 55.7   1.436   1.246    58   11.9   5:29 (227, 31)  
Aug.  5   4 58.20   11 27.4   1.443   1.260    58   11.8   5:24 (227, 30)  

* C/2016 R2 ( PanSTARRS )

Now it is 14.8 mag (July 5, 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 is appearing in the morning sky. Then it stays observable for a long time until the comet will fade out.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29   4 58.83   -5  1.2   4.344   3.899    57   13.1   5:29 (245, 38)  
Aug.  5   5  4.68   -4 36.2   4.220   3.849    61   13.0   5:24 (241, 41)  

* 29P/Schwassmann-Wachmann 1

Now it is bright as 13.2 mag (July 25, Chris Wyatt).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29  21 29.24  -13 43.5   4.840   5.829   165   13.2   1:04 (180, 69)  
Aug.  5  21 26.02  -13 52.6   4.819   5.828   172   13.2   0:33 (180, 69)  

* 213P/Van Ness

Now it is bright as 13.5 mag (July 5, 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)  
July 29  18 53.43  -29  1.1   1.066   2.033   155   13.6  22:24 (180, 84)  
Aug.  5  18 50.15  -28  1.3   1.088   2.022   148   13.5  21:54 (180, 83)  

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

Now it is 14.2 mag (July 6, Ken-ichi Kadota). It will brighten up to 13-14 mag and will be observable in good condition in summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29  22 56.05   12 32.5   1.946   2.739   132   13.7   2:31 (180, 42)  
Aug.  5  22 33.43   10 43.9   1.846   2.731   143   13.5   1:41 (180, 44)  

* C/2016 N4 ( MASTER )

Now it is 15.0 mag (July 7, Ken-ichi Kadota). 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)  
July 29   0 37.43   53 36.3   3.059   3.234    90   14.0   4:11 (180,  1)  
Aug.  5   0 31.64   56 36.8   2.989   3.225    94   14.0   3:38 (180, -2)  

* 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)  
July 29  15 45.22  -23  0.6   2.383   2.938   113   14.3  19:17 (180, 78)  
Aug.  5  15 48.17  -23 20.2   2.465   2.933   107   14.4  18:52 (180, 78)  

* 103P/Hartley 2

It has not been observed yet in this apparition. The condition of this apparition is worst. It must have brightened up to 10 mag in spring, but it is not observable at all.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29   8 20.19   10 53.5   2.666   1.668     8   14.3   5:29 (264,-11)  
Aug.  5   8 37.83    9 38.3   2.724   1.730     9   14.7   5:24 (265, -9)  

* C/2015 O1 ( PanSTARRS )

Now it is 14.4 mag (July 7, Ken-ichi Kadota). 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)  
July 29  16 45.91   23 35.5   3.682   4.145   110   14.5  20:16 (180, 31)  
Aug.  5  16 37.24   23 21.5   3.751   4.119   104   14.5  19:40 (180, 32)  

* C/2016 M1 ( PanSTARRS )

Now it is 15.3 mag (July 8, Ken-ichi Kadota). 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)  
July 29  17 24.19   48  3.9   4.254   4.558   100   15.2  20:54 (180,  7)  
Aug.  5  17 17.79   46 19.8   4.224   4.501    99   15.2  20:21 (180,  9)  

* C/2016 N6 ( PanSTARRS )

Now it is 15.8 mag (July 8, Ken-ichi Kadota). 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)  
July 29  15 23.91   59  4.2   4.478   4.421    80   15.4  18:54 (180, -4)  
Aug.  5  15 14.95   58  2.4   4.475   4.370    77   15.4  18:47 (176, -3)  

* C/2011 KP36 ( Spacewatch )

Now it is 15.6 mag (Mar. 6, Kunihiro Shima). It is appearing in the morning sky. It stays observable at 15.5 mag unil the end of 2017.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29   3 25.80    4 36.3   5.924   5.763    76   15.5   5:29 (213, 45)  
Aug.  5   3 29.18    4 25.8   5.847   5.789    81   15.5   5:24 (207, 47)  

* P/2017 M2 ( LINEAR-NEAT )

Now it is 19.1 mag (June 22, Erwin Schwab, Pablo Ruiz). 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.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29   1 42.65   -3 57.1   1.336   1.852   103   15.9   5:16 (180, 59)  
Aug.  5   1 54.01   -3  3.5   1.259   1.830   106   15.6   5:00 (180, 58)  

* C/2015 V1 ( PanSTARRS )

Now it is 15.4 mag (July 26, Toshiyuki Takahashi). 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)  
July 29   2 43.28   30 32.1   4.517   4.426    78   15.7   5:29 (191, 23)  
Aug.  5   2 41.14   30  8.3   4.374   4.411    85   15.6   5:24 (186, 25)  

* 352P/2017 L1 ( Skiff )

First return of a new periodic comet discovered in 2000. Now it is 17.8 mag (June 16, Kunihiro Shima). It will brighten rapidly, and it is expected to be observable at 15.5 mag in good condition from July to September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29   1 13.43  -10 34.3   1.995   2.556   112   15.8   4:47 (180, 65)  
Aug.  5   1 16.06  -10  5.0   1.930   2.564   117   15.7   4:22 (180, 65)  

* C/2017 K4 ( ATLAS )

Now it is 15.8 mag (June 29, K. Hills). 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)  
July 29  16 43.24  -33 29.2   2.381   3.101   127   15.8  20:15 (180, 88)  
Aug.  5  16 44.50  -32 41.2   2.420   3.067   120   15.8  19:49 (180, 88)  

* 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.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29   1 35.90   12 32.5   2.489   2.832    99   15.9   5:10 (180, 42)  
Aug.  5   1 39.45   13 26.1   2.405   2.837   104   15.8   4:46 (180, 41)  

* 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)  
July 29   1 36.63  -72 50.9   2.185   2.733   112   16.1   5:09 (  0, 52)  
Aug.  5   1 58.94  -74 23.9   2.152   2.681   110   15.9   5:04 (  0, 51)  

* 96P/Machholz 1

Now it is 19.7 mag (Apr. 27, iTelescope Observatory, Siding Spring). 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)  
July 29  20 55.07  -79  8.5   1.224   1.938   119   16.6   0:35 (  0, 46)  
Aug.  5  18 56.64  -81 48.4   1.177   1.840   114   16.2  21:51 (  0, 43)  

* C/2017 D2 ( Barros )

Now it is 16.8 mag (July 6, CAO, San Pedro de Atacama). It will brighten up to 15.5 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)  
July 29  21 48.67  -31 42.3   1.518   2.491   158   16.3   1:23 (180, 87)  
Aug.  5  21 41.43  -30 13.9   1.507   2.497   163   16.4   0:49 (180, 85)  

* C/2014 OE4 ( PanSTARRS )

Now it is 16.3 mag (July 7, Ken-ichi Kadota). 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)  
July 29  18  1.55   66  3.1   6.352   6.441    90   16.4  21:31 (180,-11)  
Aug.  5  17 56.51   65 52.1   6.368   6.453    90   16.5  20:59 (180,-11)  

* (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)  
July 29  21 16.21    3 14.0   2.385   3.336   155   16.6   0:51 (180, 52)  
Aug.  5  21 11.87    2 43.8   2.381   3.353   160   16.6   0:19 (180, 52)  

* 145P/Shoemaker-Levy 5

Now it is 18.4 mag (May 31, iTelescope Observatory, Siding Spring). 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)  
July 29   3 19.39   17 16.4   1.947   1.929    73   16.8   5:29 (204, 34)  
Aug.  5   3 33.93   18 46.6   1.878   1.920    76   16.7   5:24 (202, 33)  

* 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)  
July 29  19 51.33  -19 35.9   2.390   3.395   170   16.7  23:22 (180, 75)  
Aug.  5  19 45.72  -19 56.0   2.450   3.430   162   16.8  22:49 (180, 75)  

* 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. It will be getting higher gradually in the morning sky.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29   3 57.95    7 42.1   2.168   2.010    67   16.7   5:29 (220, 38)  
Aug.  5   4  5.80    7 22.4   2.175   2.099    72   17.0   5:24 (216, 41)  

* 189P/NEAT

Now it is 17.6 mag (June 30, ATLAS-MLO, Mauna Loa). It brightens up to 16.5-17 mag in August, and it will be observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29  16  3.30  -10 32.7   0.370   1.217   114   16.9  19:36 (180, 65)  
Aug.  5  16 26.61   -4 53.7   0.386   1.213   112   16.8  19:32 (180, 60)  

* 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)  
July 29  21 15.09  -25 23.1   1.235   2.239   168   16.8   0:50 (180, 80)  
Aug.  5  20 59.28  -25 55.2   1.298   2.306   171   16.9   0:07 (180, 81)  

* 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 17.8 mag (June 30, CAO, San Pedro de Atacama). 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)  
July 29   3  0.06    6 31.8   1.822   1.950    81   17.1   5:29 (203, 46)  
Aug.  5   3  5.81    6 45.4   1.799   2.013    86   17.2   5:24 (197, 47)  

* 41P/Tuttle-Giacobini-Kresak

It approached to Earth down to 0.14 a.u. from late March to early April, and it brightened up to 6.0 mag (Apr. 7, Juan Jose Gonzalez). Now it is fading. It has already faded down to 12.1 mag (July 17, Thomas Lehmann). It stays observable in good condition after this until the comet fades out.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29  18 12.10  -13 17.8   0.766   1.704   145   17.1  21:43 (180, 68)  
Aug.  5  18 15.31  -14 57.7   0.860   1.764   140   17.8  21:19 (180, 70)  

* 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)  
July 29   5 55.29   63 53.2   9.688   9.103    52   17.2   5:29 (204,-20)  
Aug.  5   6  2.73   64 21.6   9.617   9.088    55   17.2   5:24 (202,-19)  

* 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)  
July 29  20 14.15   70 30.5   5.700   5.801    90   17.4  23:42 (180,-16)  
Aug.  5  19 55.30   70  2.5   5.625   5.754    92   17.4  22:56 (180,-15)  

* (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)  
July 29   0 26.27  -42 56.8   3.621   4.293   125   17.4   4:00 (  0, 82)  
Aug.  5   0 23.58  -43 39.8   3.532   4.252   129   17.4   3:30 (  0, 81)  

* C/2016 B1 ( NEOWISE )

Now it is 16.7 mag (June 27, Hidetaka Sato). It will fade out after this, and it will be fainter than 18 mag in August.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29  17 45.84   27 25.9   3.311   3.900   118   17.4  21:17 (180, 28)  
Aug.  5  17 44.25   27  8.6   3.396   3.936   115   17.6  20:47 (180, 28)  

* 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)  
July 29  14 25.78  -13 42.0   2.047   2.329    92   17.5  18:43 (151, 66)  
Aug.  5  14 32.16  -14 30.0   2.100   2.296    87   17.4  18:47 (138, 64)  

* C/2017 E3 ( PanSTARRS )

Now it is 17.5 mag (June 30, ATLAS-MLO, Mauna Loa). It is already unobservable in the Northern Hemisphere. It will be getting lower gradually after this also in the Southern Hemisphere, and it will be unobservable in September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29  12 55.63  -26 40.8   6.053   5.930    78   17.6  18:43 ( 96, 60)  
Aug.  5  12 59.68  -26  3.1   6.161   5.934    72   17.7  18:47 ( 93, 54)  

* 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)  
July 29  22 20.87  -34 17.3   4.621   5.534   151   17.8   1:55 (180, 89)  
Aug.  5  22 17.17  -34 16.8   4.618   5.558   155   17.8   1:24 (180, 89)  

* 2017 MZ4

Peculiar asteroid moving along a comet-like orbit. Now it is 18.0 mag (June 26, ATLAS-MLO, Mauna Loa). It is observable at 18 mag in good condition from July to August. It locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29  21 21.20  -24 28.3   2.218   3.217   167   17.9   0:56 (180, 79)  
Aug.  5  21  9.68  -23  1.6   2.217   3.228   173   17.8   0:17 (180, 78)  

* C/2014 W2 ( PanSTARRS )

It stayed bright 12 mag for a long time from autum in 2015 to summer in 2016. Now it is fading. It has already faded dwon to 17.9 mag (July 3, ATLAS-HKO, Haleakala).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 29  15 53.69  -17  4.3   5.047   5.539   114   17.9  19:25 (180, 72)  
Aug.  5  15 52.02  -17 37.0   5.208   5.590   107   18.0  18:56 (180, 73)  

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