Weekly Information about Bright Comets (2009 Aug. 29: North)

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Updated on September 13, 2009
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Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Northern Hemisphere.
Azimuth indicates 0 for south, 90 for west, 180 for north, 270 for east.

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* C/2006 W3 ( Christensen )

Now it is so bright as 8.2 mag (Aug. 21, Juan Jose Gonzalez). It will be observable at 8-10 mag in good condition for a long time until late autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  19 54.33   15 25.1   2.381   3.169   134    8.1  21:22 (  0, 70)  
Sept. 5  19 42.80   11 53.5   2.452   3.181   128    8.2  20:43 (  0, 67)  

* 88P/Howell

Now it is so bright as 9.8 mag (Aug. 21, Juan Jose Gonzalez). It keeps observable for a long time until 2010 February. It will keep 9 mag until the end of 2009. But in the Northern Hemisphere, it keeps very low after this. It locates a bit higher in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  14 30.11  -16 28.1   1.553   1.448    64    9.8  19:59 ( 58, 13)  
Sept. 5  14 49.39  -18 13.5   1.564   1.424    62    9.6  19:48 ( 56, 13)  

* C/2007 Q3 ( Siding Spring )

It brightened up to 9.8 mag on June 13 (Marco Goiato). Now it is not observable. But it keeps as bright as 10-11 mag for a long time untio 2010 spring. In the Northern Hemisphere, it will appear in the morning sky in early October, then it keeps observable at 10 mag in good condition for a long time. In the Southern Hemisphere, it will locate extremely low only after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   9 46.02    4  5.1   3.274   2.296    12    9.7   4:01 (256,-13)  
Sept. 5   9 59.24    4 44.8   3.246   2.282    14    9.7   4:08 (258, -8)  

* C/2008 Q3 ( Garradd )

It brightened up to 6.7 mag in June (June 9, Marco Goiato). Now it is fading, but still bright as 9.5 mag (Aug. 21, Juan Jose Gonzalez). However, it will be unobservable soon. It will appear in the morning sky again at 13 mag in November. It may be visible visually again.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  12 47.68    3 16.1   2.734   1.989    34   10.4  19:59 ( 90,  6)  
Sept. 5  12 51.34    4 12.8   2.850   2.028    29   10.7  19:48 ( 93,  3)  

* 22P/Kopff

It brightened up to 8.8 mag in May and June (May 19, Juan Jose Gonzalez). Now it is still bright as 10.4 mag (Aug. 21, Juan Jose Gonzalez). It will be bright at 9-10 mag for a long time until autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  22 48.72  -14 12.2   0.830   1.837   173   10.4   0:21 (  0, 41)  
Sept. 5  22 44.65  -14 54.8   0.868   1.871   171   10.7  23:45 (  0, 40)  

* C/2008 T2 ( Cardinal )

It brightened up to 8.5 mag in May and June (May 26, Juan Jose Gonzalez). Now it is fading, but still bright as 10.7 mag (Aug. 22, Marco Goiato). It will never be observable again in the Northern Hemisphere. In the Southern Hemisphere, it keeps observable for a long time after this in the evening sky.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  11 30.47  -44 16.2   2.026   1.674    55   10.4  19:59 ( 56,-33)  
Sept. 5  12  0.29  -47 14.8   2.095   1.745    56   10.7  19:48 ( 51,-32)  

* 217P/2009 F3 ( LINEAR )

It is already so bright as 10.1 mag (Aug. 19, Juan Jose Gonzalez). It will be observable at 10-11 mag in a good condition for a long time from summer to winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   3 59.31   -3 16.5   0.578   1.232    98   11.0   4:01 (327, 46)  
Sept. 5   4 26.93   -3 32.4   0.577   1.225    97   10.9   4:08 (329, 47)  

* C/2009 F6 ( Yi-SWAN )

It was bright as 8-9 mag in April and May. Although it had been unobservable for a while, now it is appearing in the morning sky. It should be bright as 12 mag still now. It will be fading slowly in the low sky 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)  
Aug. 29   7 50.48    0 48.9   2.735   2.075    40   11.9   4:01 (275,  9)  
Sept. 5   7 55.89   -2  9.0   2.728   2.148    45   12.0   4:08 (282, 13)  

* 24P/Schaumasse

It must have reached up to 11 mag in summer. However, the condition of this apparition is worst. We can not observe it at all.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  10 39.69   15 14.3   2.239   1.240     6   12.0  19:59 (118,-12)  
Sept. 5  11  5.01   12 53.9   2.258   1.262     6   12.3  19:48 (115,-12)  

* 222P/2009 MB9 ( LINEAR )

First return of a new bright periodic comet. It was observed as an asteroid in June. Now it is so bright as 12.3 mag (Aug. 31, Juan Jose Gonzalez). In the Northern Hemisphere, it keeps observable in a good condition after this. However, it will fade out rapidly, and will be fainter than 18 mag in October.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   8 19.85   14 32.8   0.287   0.782    32   13.2   4:01 (259, 10)  
Sept. 5   8  9.56   18 37.6   0.351   0.783    41   13.6   4:08 (262, 21)  

* C/2009 G1 ( STEREO )

It has been observed bright as 8-9 mag from April to June. Now it is fading. It was still bright as 11.0 mag in July (July 12, Marco Goiato). However, no observations have been reported since August. So it may have faded out rapidly. In the Southern Hemisphere, it keeps observable in a good condition for a long time. In the Northern Hemisphere, it will never be observable again.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  10  6.14  -50 31.4   2.618   2.290    60   13.2   4:01 (310,-41)  
Sept. 5  10 15.40  -50 33.2   2.743   2.370    58   13.4   4:08 (311,-37)  

* 116P/Wild 4

It brightened up to 11 mag in spring and summer. Now it is not observable. It will appear in the morning sky at 15 mag in early 2010. But it locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  12 47.49   -5 31.4   2.909   2.194    37   13.3  19:59 ( 83,  0)  
Sept. 5  13  1.13   -7  3.8   2.959   2.202    34   13.3  19:48 ( 82, -1)  

* 29P/Schwassmann-Wachmann 1

Now it is not observable. It will appear in the morning sky in September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   9  9.96   16 28.5   7.091   6.156    20   14.2   4:01 (251,  1)  
Sept. 5   9 14.90   16  2.5   7.047   6.158    26   14.2   4:08 (255,  7)  

* C/2007 N3 ( Lulin )

It passed near by the earth in late February, and it reached up to 4.9 mag (Feb. 23, Juan Jose Gonzalez). It had been unobservable for a while, but it is appearing in the morning sky again. it is still bright as 13.7 mag and visible visually (Aug. 28, Jakub Cerny). In the Northern Hemisphere, it is observable at 15 mag in good condition from autumn to winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   7 19.80   20 56.2   3.944   3.339    47   14.2   4:01 (262, 26)  
Sept. 5   7 19.99   20 52.9   3.910   3.413    53   14.3   4:08 (266, 33)  

* 81P/Wild 2

Now it is 15.9 mag (Aug. 29, H. Sato). It will be getting higher after this. It will be observable bright as 9-10 mag in a good condition for a long time from winter to spring. It keeps observable until 2010 autumn when it fades down to 16 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   7 37.76   19 52.0   2.930   2.294    42   14.7   4:01 (260, 22)  
Sept. 5   7 52.38   19 17.8   2.833   2.253    46   14.5   4:08 (263, 25)  

* 64P/Swift-Gehrels

Appearing in the morning sky. Now it is 12.8 mag and visible visually (July 25, Juan Jose Gonzalez). It will be getting higher gradually while fading slowly after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   7 47.64   24 30.2   2.260   1.644    41   14.5   4:01 (255, 22)  
Sept. 5   8  5.61   23 23.0   2.264   1.689    43   14.7   4:08 (258, 25)  

* C/2007 G1 ( LINEAR )

It brightened up to 11.5 mag in last summer (Aug. 4, Marco Goiato). Now it is 15.9 mag (Aug. 12, H. Sato). It keeps observable in good condition for a long time in the Southern Hemisphere. It will be observable again also in the Northern Hemisphere after September. It will keep 15-16 mag until next spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   6 36.63  -37 53.5   4.119   3.927    72   14.5   4:01 (316, -3)  
Sept. 5   6 38.58  -38 19.4   4.123   3.977    74   14.6   4:08 (321,  1)  

* 65P/Gunn

It was observed as bright as 13 mag in spring and summer. It will be too low to observe soon. It will brighten up to 12-13 mag in 2010 summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  13 17.16   -3  0.3   3.327   2.685    43   14.6  19:59 ( 81,  8)  
Sept. 5  13 27.17   -4 19.6   3.368   2.669    39   14.6  19:48 ( 80,  6)  

* C/2006 OF2 ( Broughton )

It brightened up to 9.8 mag in winter (Dec. 28, Juan Jose Gonzalez). It faded down to 12.5 mag in May (May 26, Juan Jose Gonzalez), and became unobservable. Now it is not observable, however, it will be observable in good condition again in winter at 15 mag. Then it may be still visible visually.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   9 33.21   15  8.9   5.301   4.333    14   14.6   4:01 (249, -4)  
Sept. 5   9 39.62   14 16.5   5.321   4.387    19   14.7   4:08 (253,  1)  

* C/2008 P1 ( Garradd )

Now it is 14.5 mag (July 30, H. Sato). It keeps observable in good condition at 15 mag until late autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   0 23.81   25 34.3   3.126   3.910   135   14.9   1:56 (  0, 81)  
Sept. 5   0 16.17   26 47.5   3.080   3.915   141   14.9   1:21 (  0, 82)  

* (3552) Don Quixote

Now it is 15.2 mag (Aug. 3, H. Sato). It passes the perihelion in September, and now it is brightest. It keeps observable in good condition in the Southern Hemisphere. It is not observable now in the Northern Hemisphere. But it will appear in the evening sky at the end of September, and then it will be getting higher while fading.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  14 40.09  -56 20.5   0.806   1.217    83   15.0  19:59 ( 28,-13)  
Sept. 5  15 31.21  -55 38.3   0.779   1.210    84   14.9  19:48 ( 25, -9)  

* C/2008 N1 ( Holmes )

Now it is 15.3 mag (Aug. 22, H. Sato). It keeps 15 mag until 2010, and will be observable for a long time in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  15 50.24   44 30.4   2.859   2.799    76   15.3  19:59 (119, 58)  
Sept. 5  15 42.73   41 42.6   2.935   2.792    71   15.3  19:48 (114, 54)  

* C/2009 O4 ( Hill )

Now it is 14.9 mag (Aug. 26, H. Sato). It keeps 15 mag until winter. It keeps observable in a good condition in the Southern Hemisphere. But in the Northern Hemisphere, it will be getting lower gradually, and it is only observable until late autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   0 14.87   -5 39.3   1.949   2.889   153   15.6   1:47 (  0, 50)  
Sept. 5   0  6.87   -9 50.8   1.880   2.856   162   15.4   1:12 (  0, 45)  

* C/2006 S3 ( LONEOS )

Now it is 16.2 mag (Aug. 13, Ken-ichi Kadota), brightening as expected. It will reach up to 12 mag in 2012, and will be observable visually at 12-13 mag for a long time from 2011 to 2013. In 2009, it is observable in good condition at 16 mag from summer to autumn. In the Northern Hemisphere, the comet will be low around its brightest seasons.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  22 18.31    4 18.1   7.616   8.599   165   15.8  23:46 (  0, 59)  
Sept. 5  22 13.64    3 52.9   7.584   8.562   165   15.7  23:14 (  0, 59)  

* C/2005 L3 ( McNaught )

It brightened up to 13 mag from 2007 to 2009, and it was observed visually for a long time. It will fade out gradually after this. But it keeps 16 mag until 2010 spring, and 17 mag until 2010 autumn. Although it becomes low in autumn temporarily, it keeps observable in good condition from winter to summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  13  5.55   31 55.5   7.710   6.998    42   15.8  19:59 (113, 24)  
Sept. 5  13  6.74   31 30.6   7.777   7.027    39   15.8  19:48 (114, 21)  

* 118P/Shoemaker-Levy 4

Now it is 15.7 mag (Aug. 31, Michael Jager). It will brighten rapidly after this. It will reach to 12 mag and become visible visually in winter. In the Northern Hemisphere, it keeps observable in good condition for a long time after this until 2010 spring when it fades out.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   4 45.43   13 36.0   2.079   2.215    84   16.0   4:01 (297, 53)  
Sept. 5   4 57.04   13 29.8   1.983   2.193    87   15.8   4:08 (303, 57)  

* C/2006 Q1 ( McNaught )

It reached to 10.9 mag in 2008 spring (May 11, Marco Goiato). It is fading slowly, but still bright as 15.0 mag (Aug. 20, H. Sato). Although it becomes low in winter temporarily, it keeps observable for a long time until 2010 spring when it becomes fainter than 18 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  16 11.86   31 40.7   4.976   4.925    81   15.8  19:59 ( 93, 61)  
Sept. 5  16 15.47   30 55.0   5.087   4.976    77   15.9  19:48 ( 93, 58)  

* P/2009 K1 ( Gibbs )

New periodic comet. It has already passed the perihelion in late June. But unexpectedly, it keeps unusual brightening very rapidly after that. Now it became bright as 15.0 mag (July 30, D. Chestnov). It keeps observable in the evening low sky for a while after this. But it may fade out very rapidly.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  14 12.02   -8 16.8   1.791   1.522    58   16.0  19:59 ( 68, 16)  
Sept. 5  14 34.12  -10  7.3   1.861   1.562    57   16.4  19:48 ( 65, 15)  

* P/2009 L2 ( Yang-Gao )

It reached up to 12.6 mag and became visible visually in June and July (June 25, Katsumi Yoshimoto). However, it is fading rapidly after August. It has already faded down to 16.8 mag (Aug. 16, Ken-ichi Kadota). It will be fainter than 18 mag in October.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  19  2.44    3 15.9   0.911   1.718   126   16.1  20:32 (  0, 58)  
Sept. 5  19 10.84    2 44.0   1.001   1.767   123   16.5  20:13 (  0, 58)  

* P/2003 A1 ( LINEAR )

Appearing in the morning sky. It has not been recovered yet. But it must have already brightened up to 16.5 mag. It will be getting higher rapidly after this, and will be observable in good condition at 16 mag in autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   6  2.57   31 29.3   2.222   2.021    65   16.3   4:01 (259, 46)  
Sept. 5   6 15.86   33 34.6   2.164   2.041    69   16.2   4:08 (258, 51)  

* P/2009 Q5 ( McNaught )

Now it is brightest, and it will be fading after October. It keeps observable until January when it becomes fainter than 18 mag. It locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   1 28.67  -16 37.7   2.117   2.928   135   16.8   3:00 (  0, 38)  
Sept. 5   1 29.43  -18 49.3   2.076   2.927   140   16.8   2:34 (  0, 36)  

* 47P/Ashbrook-Jackson

It brightened up to 15-16 mag in 2008 summer. Now it is 17.8 mag (Aug. 26, Katsumi Yoshimoto). It keeps observable at 17 mag in good condition for a long time until winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   3 47.08   30 16.4   2.792   3.040    94   17.0   4:01 (281, 73)  
Sept. 5   3 51.17   31  4.9   2.715   3.055    99   17.0   4:08 (288, 79)  

* (3200) Phaethon

It passed the perihelion in June, but it was not observable, too close to the sun. Although it was predicted to be 13.5 mag, the STEREO spacecraft revealed that it brightened up to 10-11 mag, much brighter than expected. Now it is 16.4 mag (Aug. 23, C00). It keeps observable at 16-17 mag until late autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   4 30.91   46 36.7   1.151   1.436    82   17.1   4:01 (234, 64)  
Sept. 5   4 22.77   47 59.6   1.128   1.516    90   17.1   4:08 (223, 70)  

* C/2007 U1 ( LINEAR )

It reached up to 14 mag in 2008 autumn. It is still bright as 16.0 mag (July 30, H. Sato). It keeps observable around 17 mag in a good condition for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  22 23.26   17 46.4   3.919   4.839   152   17.4  23:51 (  0, 73)  
Sept. 5  22 12.82   16 49.8   3.956   4.883   154   17.5  23:13 (  0, 72)  

* 107P/(4015) Wilson-Harrington

Now it is 16.7 mag (Aug. 14, Katsumi Yoshimoto). The condition is good in this apparition. It will approach to the earth down to 0.38 A.U., and will be observable in good condition at 16.5 mag in November. It keeps observable until that time after this. But it locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  16 20.85  -18 46.5   0.672   1.222    90   17.6  19:59 ( 35, 28)  
Sept. 5  16 32.26  -18 49.0   0.657   1.172    86   17.6  19:48 ( 36, 28)  

* C/2008 S3 ( Boattini )

It keeps observable at 17 mag for a long time from 2010 to 2012. Now it is 18.5 mag (Aug. 25, W. Hasubick), a bit fainter than this ephemeris.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   3 44.44   20 42.8   8.732   8.913    97   17.7   4:01 (306, 68)  
Sept. 5   3 42.30   20 43.3   8.591   8.895   104   17.7   4:08 (327, 73)  

* C/2007 VO53 ( Spacewatch )

Now it is 17.3 mag (Aug. 23, Ken-ichi Kadota). It keeps observable at 17-18 mag for a long time until 2011.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   4 33.25   66 48.3   5.255   5.193    81   17.8   4:01 (200, 54)  
Sept. 5   4 34.22   68 32.5   5.155   5.174    85   17.7   4:08 (194, 54)  

* C/2009 K2 ( Catalina )

Now it is 17.5 mag (Aug. 14, Michael Jager). It will be getting lower in the evening sky after this. But it will be observable at 17 mag from spring to summer in 2010.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29  16 12.28   38 37.6   3.613   3.591    80   17.8  19:59 (107, 62)  
Sept. 5  16 17.77   36 14.6   3.627   3.564    78   17.8  19:48 (103, 60)  

* P/2009 Q4 ( Boattini )

Now it is 17.7 mag (Sept. 5, H. Sato). It will reach up to 15.5 mag. It keeps observable in good condition all through the time until next spring when it becomes fainter than 18 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 29   4 34.67    8 21.6   1.281   1.596    87   18.1   4:01 (306, 51)  
Sept. 5   4 55.44    8 24.2   1.204   1.556    88   17.8   4:08 (310, 53)  

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