Weekly Information about Bright Comets (2007 Oct. 6: North)

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Updated on October 8, 2007
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Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Northern Hemisphere.

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* C/2007 F1 ( LONEOS )

Now it is 7.2 mag (Oct. 4, Peter Bus), much brighter than originally expected in the extremely low sky at dawn. It will approach down to 0.4 A.U. to the sun on Oct. 28, and it will reach to 4 mag in mid October. However, the condition in the Northern Hemisphere is very hard. It locates extremely low, slightly over the horizon, in the morning sky from late September to mid October, and in the evening sky from mid October to late October. Then it will never be observable again. In the Southern Hemisphere, it will appear in the evening sky at 4-5 mag in early November, then it keeps observable while fading gradually, although it will not locate very high.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  12 27.96   26 58.0   1.308   0.703    32    7.8   4:34 (240,  5)  
Oct. 13  13  5.03   24 22.5   1.073   0.574    31    6.4   4:39 (242,  2)  

* C/2006 VZ13 ( LINEAR )

It reached to 7.2 mag on July 14 (Maik Meyer), then it faded down to 9.0 mag on Aug. 13 (Carlos Labordena). Now it is not observable. In the Southern Hemisphere, it will appear in the morning sky in late October at 13 mag, then it keeps observable while fading gradually. In the Northern Hemisphere, it will appear again at 14 mag in the very low sky at dawn in mid November. But it will be fading while keeping extremely low.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  12 25.32  -25 37.9   2.259   1.376    21   11.7   4:34 (285,-25)  
Oct. 13  12 23.16  -27 27.7   2.319   1.452    22   12.1   4:39 (291,-19)  

* 29P/Schwassmann-Wachmann 1

Now it is faint as 14.1 mag (Oct. 5, Seiichi Yoshida). It has been observable since late July, but it keeps faint in this season. It has never be brighter than 14 mag yet.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   6 28.69   30 18.2   5.766   5.954    95   13.6   4:34 (287, 77)  
Oct. 13   6 29.93   30 22.1   5.659   5.956   102   13.6   4:39 (308, 83)  

* P/2007 H1 ( McNaught )

Now it is bright as 12.6 mag (Oct. 5, Seiichi Yoshida). Strongly condensed and easy to see visually. It is observable in very good condition at 13 mag for a while in this autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   0  4.88  -13 29.9   1.345   2.307   159   13.6  23:05 (  0, 41)  
Oct. 13   0  2.04  -14  7.9   1.383   2.315   152   13.7  22:35 (  0, 41)  

* C/2006 Q1 ( McNaught )

It was 14.1 mag on Oct. 1 (S. G. McAndrew), brightening well as expected. It will reach to 11 mag in 2008 spring. It will keep bright for a long time, however, it keeps moving in the southern sky for a while after this. In the Northern Hemisphere, it will appear at 13 mag from October to December in a short time, but very low and hard to observe. However, it will be visible visually at 11 mag in the evening sky from March to June in 2008. Then it becomes unobservable again. But it will appear in the morning sky again at 13 mag at the end of 2008, then it keeps bright and observable for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   8 42.65  -35 20.4   4.220   3.876    63   13.8   4:34 (322,  7)  
Oct. 13   8 51.19  -36 30.3   4.136   3.830    65   13.7   4:39 (327,  9)  

* 8P/Tuttle

It will reach to 6 mag in January, and will be observable in good condition. Now it is 15.4 mag (Oct. 7, Masayuki Suzuki). Brightening rapidly, and it will become visible visually soon, although it was not visible visually, fainter than 14.6 mag, on Oct. 5 (Seiichi Yoshida). In the Northern Hemipshere, it keeps observable all night until mid December, then keeps observable until early February, when it fades down to 7.5 mag. In the Southern Hemipshere, it is not observable until late December. But after that, it keeps observable until it fades out.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   7 12.95   88 24.2   1.525   1.890    94   14.4   4:34 (181, 36)  
Oct. 13  11  7.69   88 21.5   1.418   1.818    96   14.0   4:39 (182, 35)  

* 93P/Lovas 1

It brightened rapidly, and it is already bright and visible visually at 13.4 mag (Oct. 6, Seiichi Yoshida). It is observable at 13.5 mag in good condition from autumn to winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   0 47.34   21 48.4   0.878   1.857   163   14.3  23:47 (  0, 77)  
Oct. 13   0 41.37   22 49.3   0.852   1.830   163   14.0  23:14 (  0, 78)  

* C/2006 XA1 ( LINEAR )

It reached to 13.2 mag in last spring (May 12, Carlos Labordena). But now it is not observable. In the Southen Hemisphere, it will be observable again at 15 mag in November. But in the Northern Hemisphere, it will never observable again.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  11 55.75  -15 50.1   2.984   2.044    16   14.0   4:34 (280,-14)  
Oct. 13  12 10.22  -18 24.4   3.009   2.086    18   14.2   4:39 (284,-12)  

* C/2006 OF2 ( Broughton )

It is already bright and visible visually at 13.5 mag (Oct. 6, Seiichi Yoshida). It will reach to 10.5 mag and will be observable in good condition in 2008 autumn. It keeps observable in good condition for a long time while the comet is getting brighter slowly.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  21 15.78   -7 55.7   3.652   4.319   126   14.2  20:17 (  0, 47)  
Oct. 13  21 14.08   -7 45.1   3.690   4.265   119   14.1  19:47 (  0, 47)  

* C/2006 K4 ( NEAT )

Now it is 15.8 mag (Sept. 2, R. Salvo). It keeps 15 mag for a long time until 2008 spring. It moves in the southen sky, so it keeps observable in good condition in the Southern Hemisphere, although it becomes low only in winter. It will never be observable again in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  16 49.27  -57 31.9   3.420   3.231    70   14.8  19:02 ( 24,-11)  
Oct. 13  16 48.50  -57 42.4   3.508   3.221    65   14.8  18:52 ( 26,-13)  

* C/2006 S5 ( Hill )

Now it is 15.7 mag (Sept. 16, Ken-ichi Kadota), brightening as expected. It will reach to 14 mag in next winter, and will be observable in good condition. It is expected to be visible visually. It keeps observable in good condition for a long time until 2008 spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   7  6.72   25 56.8   2.573   2.716    87   14.9   4:34 (287, 67)  
Oct. 13   7 16.33   25 23.9   2.473   2.699    91   14.8   4:39 (297, 72)  

* P/1990 V1 ( Shoemaker-Levy 1 )

It has not been recovered yet because it had been unobservable for a long time. But it must be already bright as 15 mag. It will appear in the evening sky in October, then it will be getting higher gradually. It keeps observable at 14-15 mag in the evening sky until January. Then it keeps locating in the evening sky until April when it becomes fainter than 18 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  18 45.20  -52 31.8   1.425   1.685    86   15.2  19:02 ( 11,  1)  
Oct. 13  19  4.96  -51 20.2   1.431   1.645    83   15.0  18:52 ( 11,  2)  

* C/2005 L3 ( McNaught )

Now it is bright and visible visually at 14.1 mag (Oct. 5, Seiichi Yoshida). It had been observable in good conditoin for a long time since spring, but it will be getting lower and lower after this, and will be unobservable in November. But it will be observable at 14 mag at high location again in 2008 spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  16 45.96   -1  9.2   6.072   5.643    60   15.0  19:02 ( 62, 32)  
Oct. 13  16 46.34   -1  8.8   6.164   5.636    54   15.1  18:52 ( 66, 29)  

* C/2006 U6 ( Spacewatch )

Now it is 15.9 mag (Sept. 8, Ken-ichi Kadota), brightening as expected. It will reach to 13.5 mag in the southern sky in 2008 spring and summer. In the Southern Hemisphere, it keeps observable for a long time after this. But in the Northern Hemisphere, it will be lower than 10 degree in November. Then it keeps locating extremely low until January, and will be unobservable after that. Then it will be observable again at the end of 2008, when the comet will already fade down to 15 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   1 10.42  -36 42.3   2.765   3.572   138   15.2   0:15 (  0, 18)  
Oct. 13   1  3.07  -38 55.2   2.760   3.522   133   15.2  23:35 (  0, 16)  

* 50P/Arend

Now it is 15.5 mag (Oct. 1, J. Maria Ruiz M). It keeps observable in good condition until it fades out in 2008 spring. It may be visible visually, but it was not visible, fainter than 14.3 mag, on Oct. 6 (Seiichi Yoshida).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   2 40.08   37 35.2   1.076   1.939   138   15.4   1:44 (180, 87)  
Oct. 13   2 36.48   39 43.7   1.042   1.932   142   15.3   1:13 (180, 85)  

* C/2006 V1 ( Catalina )

It was observed at 16 mag in 2007 spring and summer. Now it is not observable. In the Southern Hemisphere, it will appear again at 16 mag in winter, then it keeps 16 mag and observable in good condition until 2008 summer. In the Northern Hemisphere, it will never be observable again.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  12 57.95  -26 56.3   3.627   2.729    22   15.4  19:02 ( 75,-27)  
Oct. 13  13 11.23  -28 40.2   3.622   2.715    21   15.3  18:52 ( 73,-29)  

* 46P/Wirtanen

It will reach to 8.5 mag from January to March, and will be observable in good condition. In the Northern Hemisphere, it keeps observable in good condition until 2008 July when it becomes fainter than 18 mag. Now it is 16.9 mag (Sept. 3, Ken-ichi Kadota), but it will be brightening rapidly after this. It will be visible visually in November.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  21 54.43  -34 26.5   1.052   1.810   123   15.7  20:55 (  0, 21)  
Oct. 13  21 50.00  -34  3.6   1.055   1.750   116   15.3  20:23 (  0, 21)  

* 110P/Hartley 3

It brightened very rapidly in a short time, and now it reached to 15.5 mag (Oct. 1, J. Maria Ruiz M). It will be observable at 14.5-15 mag in an excellent condition from October to February. It may be visible visually, but it was not visible, fainter than 14.4 mag, on Oct. 5 (Seiichi Yoshida).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   5 32.49   33 36.8   2.106   2.592   107   15.8   4:34 (341, 89)  
Oct. 13   5 37.27   33 44.1   2.015   2.581   113   15.5   4:13 (  0, 89)  

* 188P/2007 J7 ( LINEAR-Mueller )

First return of a new periodic comet discovered in 1998 at 14 mag. Now it is 15.6 mag (Sept.. 10, Mt. Lemmon Survey), brightened as expected. It is also visible visually at 14.4 mag (Oct. 6, Seiichi Yoshida). It keeps observable at 16 mag in good condition until December.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   0  0.49    2  3.0   1.612   2.599   168   15.6  23:01 (  0, 57)  
Oct. 13  23 55.70    2  7.1   1.628   2.590   160   15.7  22:28 (  0, 57)  

* 17P/Holmes

It was bright as 14.5 mag in July (July 16, Michael Jager). But now it is 15.4 mag (Aug. 26, Ken-ichi Kadota), getting a bit fainter. It keeps observable in excellent condition while getting fainter gradually until January when it becomes fainter than 18 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   4  2.32   47 52.7   1.707   2.369   119   15.8   3:06 (180, 77)  
Oct. 13   4  0.61   48 52.8   1.674   2.395   125   15.9   2:37 (180, 76)  

* C/2007 G1 ( LINEAR )

Now it is 16.6 mag (Aug. 25, Ken-ichi Kadota). It will reach to 12 mag in 2008 summer. In the Northern Hemisphere, it keeps observable almost all time until that while the comet is brightening gradually. However, it goes to the southern sky and will never be observable again in the Northern Hemisphere after that.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  16 38.02   14 52.1   5.219   4.814    60   15.9  19:02 ( 79, 40)  
Oct. 13  16 40.74   13 29.1   5.244   4.762    56   15.9  18:52 ( 80, 37)  

* C/2006 K1 ( McNaught )

Now it is 16.6 mag (Sept. 20, Ken-ichi Kadota). Although it had been observable only in the Southern Hemisphere for a long time, now it becomes observable also in the Northern Hemisphere. It keeps 16 mag until winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   3 44.70  -29 56.9   3.825   4.471   124   15.9   2:49 (  0, 25)  
Oct. 13   3 40.83  -29 57.1   3.795   4.479   128   15.9   2:17 (  0, 25)  

* C/2005 EL173 ( LONEOS )

It reached up to 15.5 mag in late 2006 and early 2007. Now it is fading, 16.3 mag (Sept. 7, Ken-ichi Kadota). It locates somewhat low in the south, but it is observable at 16.5 mag in autumn. It will be too low to observe in early 2008, when the comet will be fainter than 17.5 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   3 55.24  -32 33.5   3.699   4.306   121   16.2   2:59 (  0, 23)  
Oct. 13   3 42.84  -33 39.7   3.678   4.332   125   16.2   2:20 (  0, 21)  

* C/2006 K3 ( McNaught )

Now it is 16.8 mag (Aug. 8, Ken-ichi Kadota). Before the perihelion passage, it kept 16.5-17 mag and hardly brightened. After the perihelion passage, it seems hardly to be fading.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   3 21.75   54 44.0   2.695   3.322   120   16.2   2:26 (180, 70)  
Oct. 13   3  2.79   56 37.0   2.682   3.369   126   16.2   1:40 (180, 68)  

* C/2006 W3 ( Christensen )

Now it is 17.6 mag (Aug. 30, P. Birtwhistle). It is expected to reach to 11 mag in 2009 summer. Because it moves in the northern sky, it keeps observable until it becomes brightest in the Northern Hemipshere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   6 35.84   56  6.0   6.315   6.484    95   16.3   4:34 (203, 66)  
Oct. 13   6 33.32   57  3.6   6.164   6.436   101   16.2   4:39 (191, 67)  

* 128P/Shoemaker-Holt 1

It already locates high in the morning sky. Although LINEAR reported it as 19 mag in mid September, it must be bright as 16.5 mag actually. It tends to be brightest after the perihelion passage. It will be observable in good condition at 16 mag until winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   7 12.28   18 45.0   3.055   3.133    85   16.3   4:34 (299, 62)  
Oct. 13   7 18.00   18 23.5   2.967   3.141    90   16.2   4:39 (310, 67)  

* 191P/2007 N1 ( McNaught )

Now it is 17.1 mag (Aug. 10, Ken-ichi Kadota). It will reach to 16 mag in October and November. Then it keeps observable in good condition until January when it becomes fainter than 18 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   3 10.53    1 59.2   1.163   2.056   143   16.5   2:14 (  0, 57)  
Oct. 13   3  8.79    1 37.8   1.135   2.061   150   16.4   1:45 (  0, 57)  

* C/2007 E1 ( Garradd )

It passed near by the earth in early April, and reached to 8.7 mag (Apr. 10, Werner hasubick). Then it faded down to 11.8 mag on May 26 (Seiichi Yoshida), and became too low to observe in the evening. Now it is 15.2 mag (Aug. 10, Ken-ichi Kadota), fading as expected.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   5 52.87   30 25.4   1.838   2.291   103   16.4   4:34 (312, 83)  
Oct. 13   5 30.96   30 48.8   1.760   2.365   115   16.6   4:08 (  0, 86)  

* 70P/Kojima

Although it had been unobservable for a long time, now it is appearing in the morning and getting higher gradually. It must be already bright as 17 mag. It keeps observable at 16.5 mag in good condition for a long time until next April.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   9 43.05   13 54.9   2.523   2.012    48   16.8   4:34 (274, 30)  
Oct. 13   9 58.45   12 52.3   2.468   2.013    51   16.7   4:39 (277, 33)  

* C/2006 M1 ( LINEAR )

Now it is 17.4 mag (Aug. 9, Ken-ichi Kadota). It is outside of Jupiter's orbit. So it keeps 17 mag for a long time until winter. It keeps locating high and observable in good condition for a long time after this because it moves in the northern sky.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   3  6.98   31 38.0   3.329   4.121   137   16.9   2:11 (  0, 87)  
Oct. 13   3  3.53   30 31.6   3.295   4.152   144   16.9   1:40 (  0, 86)  

* C/2005 S4 ( McNaught )

Now it is 17.2 mag (Aug. 12, Ken-ichi Kadota). It will be observable at 17 mag for a long time until 2008 autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  19 11.19   16 34.9   5.660   5.877    97   17.0  19:02 ( 34, 69)  
Oct. 13  19  9.44   16 22.1   5.766   5.882    91   17.0  18:52 ( 44, 66)  

* 173P/2005 T1 ( Mueller 5 )

It will be at opposition and observable in good condition in winter. It will reach to 16 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   7 48.15   21 31.7   4.431   4.322    77   17.1   4:34 (285, 57)  
Oct. 13   7 52.79   21 34.9   4.320   4.316    83   17.0   4:39 (292, 63)  

* 74P/Smirnova-Chernykh

It will reach to 15 mag in 2009 and 2010. In this year, it is observable at 16.5 mag in good condition in autumn and winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   5 34.54   22 29.4   3.700   4.122   108   17.1   4:34 (355, 77)  
Oct. 13   5 35.42   22 35.1   3.593   4.114   114   17.1   4:11 (  0, 78)  

* 2005 WY3

Peculiar asteroid moving on a cometary orbit. It was asteroidal at 18 mag in late August. It will reach to 15 mag in February and March. In the Northern Hemisphere, it keeps observable until July when it becomes fainter than 18 mag. It may show a cometary activity after this, although the perihelion distance is somewhat large as 1.8 A.U.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   7 30.83   -7 32.7   2.111   2.141    78   17.5   4:34 (320, 39)  
Oct. 13   7 44.17   -9 22.0   2.019   2.101    80   17.4   4:39 (327, 40)  

* (3200) Phaethon

It keeps observable in good condition in the morning sky while it brightens rapidly. It will reach to 13 mag in early December, and will be visible visually. However, it turns to fade out and move lower very rapidly after Dec. 10, and it will be unobservable within a few days. Then it will never be observable again. It locates somewhat low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   6 54.21   32 14.2   1.421   1.747    90   17.7   4:34 (273, 72)  
Oct. 13   7  5.48   32  9.2   1.269   1.682    95   17.4   4:39 (278, 77)  

* 117P/Helin-Roman-Alu 1

It reached to 13.5 mag and became visible visually in 2005 and 2006. Now it has gone far away. But it is observable at 17.5 mag until November.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   2 18.15    7 55.6   3.197   4.134   156   17.6   1:22 (  0, 63)  
Oct. 13   2 13.94    7 39.0   3.179   4.149   164   17.6   0:51 (  0, 63)  

* 136P/Mueller 3

Now it is 17.7 mag (Sept. 9, Ken-ichi Kadota). It will be brighter than 18 mag until November.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6  23 43.76  -11 44.1   2.013   2.962   157   17.6  22:44 (  0, 43)  
Oct. 13  23 40.65  -12 10.0   2.053   2.961   150   17.6  22:13 (  0, 43)  

* P/2004 F3 ( NEAT )

It was observed bright as 14-15 mag in 2004 and 2005. Now it is close to the aphelion, but it will be observable at 17.5 mag in good condition in 2007 autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   3 18.33    5 57.2   4.001   4.827   141   17.6   2:22 (  0, 61)  
Oct. 13   3 15.14    5 43.1   3.953   4.837   149   17.6   1:52 (  0, 61)  

* 108P/Ciffreo

Appearing in the morning sky, and observed at 16.7 mag as bright as expected (July 24, E. Guido, G. Sostero). It will be getting higher after this. But it will be fading gradually and becomes fainter than 18 mag in October.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   8 25.57   27 16.0   1.964   1.880    70   17.7   4:34 (269, 52)  
Oct. 13   8 40.77   27 14.4   1.925   1.907    73   17.8   4:39 (272, 56)  

* 65P/Gunn

It will reach to 13 mag in 2010. Now it is around the aphelion, but it will be observable at 17 mag in good condition in autumn and winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Oct.  6   8 42.10   25 30.0   4.766   4.458    66   18.0   4:34 (270, 48)  
Oct. 13   8 47.09   25 25.6   4.653   4.447    71   17.9   4:39 (274, 54)  

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