Weekly Information about Bright Comets (2007 July 21: North)

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Updated on July 28, 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/2006 VZ13 ( LINEAR )

It brightened more rapidly than expected. Now it is bright as 7.2 mag (July 14, Maik Meyer). It is the high light in July, and it will be visible bright as 7-8 mag. However, it moves southwards very fast in August. It is only observable until mid August in the Northern Hemisphere. On the other hand, it will be observable after mid July in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  13 54.33   33 35.6   0.628   1.075    77    7.4  20:52 ( 98, 53)  
July 28  13 24.15   16 45.5   0.763   1.042    70    7.7  20:45 ( 84, 36)  

* C/2006 XA1 ( LINEAR )

It became brighter than expected, and reached to 13.2 mag (May 12, Carlos Labordena). However, it is already 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)  
July 21   9  7.06   14  8.1   2.749   1.804    17   13.0  20:52 (116,-11)  
July 28   9 23.46   11 30.2   2.764   1.806    15   13.1  20:45 (115,-14)  

* C/2006 P1 ( McNaught )

Excellent great comet, few times in a lifetime, for southern people. It reached to -5.5 mag on Jan. 14 and 15, brighter than Venus, and visible even in daytime. Then it appeared in the evening sky in the Southern Hemisphere and many people enjoyed a fantastic view of a beautiful great comet, a enormous curving tail with so many striae over 50 degrees. Now it is observable both in the evening and morning. It has already faded down to 12.6 mag (July 6, Walter Ruben Robledo). In the Southern Hemisphere, It keeps observable almost all night until the comet has gone. It will never be observable again in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  12 36.01  -68 24.0   3.110   3.463   101   13.6  20:52 ( 21,-23)  
July 28  12 50.81  -66 53.2   3.255   3.552    98   13.8  20:45 ( 23,-23)  

* C/2007 E2 ( Lovejoy )

It passed near by the earth in mid April, and reached to 7.6 mag (Apr. 18, Juan Jose Gonzalez). It locates high in the evening sky, and it is observable in good condition. But it already faded down to 11.4 mag visually (June 18, Carlos Labordena), and 14.1 mag by CCD (June 23, Ken-ichi Kadota). It keeps observable in good condition in the Northern Hemisphere until the comet has gone.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  13 19.21   58  3.1   2.239   2.072    67   13.6  20:52 (140, 49)  
July 28  13 24.02   57 15.7   2.366   2.153    65   13.9  20:45 (139, 47)  

* 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 not observable. It will appear in the morning sky again at 15 mag in August.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21   7 10.64   25 18.2   2.524   1.546    12   13.7   3:19 (232, -7)  
July 28   7  9.20   25 35.5   2.528   1.603    19   14.0   3:27 (238, -1)  

* 29P/Schwassmann-Wachmann 1

It had been bright as 12-13 mag and visible visually almost always from 2006 July to 2007 April. Although it has been unobservable for a long time, now it is appearing in the morning sky finally.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21   5 43.71   29 50.1   6.768   5.930    31   14.0   3:19 (241, 11)  
July 28   5 49.45   29 52.8   6.709   5.932    37   13.9   3:27 (244, 16)  

* C/2006 K4 ( NEAT )

Now it is 15.4 mag (June 12, Ken-ichi Kadota). It will reach to 14.5 mag in summer. It moves in the southen sky, and it is observable in good condition in the Southern Hemisphere. However, it will never be observable again in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  19 15.71  -52  8.5   2.528   3.427   147   14.4  23:18 (  0,  3)  
July 28  18 54.33  -53 57.8   2.555   3.404   140   14.4  22:29 (  0,  1)  

* P/2007 H1 ( McNaught )

Now it is bright and visible visually at 14.7 mag (July 14, Juan Jose Gonzalez). It will be observable in very good condition at 14 mag from summer to autumn. However, it was not discovered at the previous apparition in 1999. So it may be bright temporarily in outburst.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21   0  8.86   -3 10.8   1.642   2.289   116   14.7   3:19 (338, 50)  
July 28   0 13.69   -3 34.4   1.572   2.286   122   14.6   3:27 (349, 51)  

* C/2006 Q1 ( McNaught )

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 Southern Hemisphere, now it is low temporarily. But it will be high after July, then it keeps observable in good condition until 2008 summer. In the Northern Hemisphere, it will appear at 13 mag in November 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)  
July 21   7  0.69  -26 45.2   4.998   4.405    49   14.7   3:19 (280,-36)  
July 28   7 10.00  -27  8.9   4.940   4.356    49   14.7   3:27 (283,-31)  

* C/2005 L3 ( McNaught )

Now it is bright and visible visually at 13.2 mag (July 14, Juan Jose Gonzalez). It will be observable at 14 mag at high location from spring to summer both in 2007 and 2008.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  17 21.47   -1 59.1   4.955   5.742   137   14.7  21:25 (  0, 53)  
July 28  17 14.83   -1 43.7   5.027   5.731   129   14.7  20:51 (  0, 53)  

* 17P/Holmes

It appeared in the morning sky. It is bright as 14.8 mag (June 22, Ken-ichi Kadota). It will be getting higher gradually after this, and it will keep bright as 15 mag and observable in good condition for a long time until autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21   2 40.62   31  6.1   2.243   2.141    71   14.8   3:19 (260, 47)  
July 28   2 52.47   32 55.1   2.191   2.157    74   14.9   3:27 (260, 52)  

* C/2007 K5 ( Lovejoy )

In the Southern Hemisphere, it is observable in the evening sky until early August while the comet is fading gradually down to 16 mag. In the Northern Hemisphere, it is not observable until when the comet becomes fainter than 18 mag. It was not discovered in last autumn when the comet located in the good condition, so it may fade out rapidly after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21   9 46.09  -10 34.8   2.309   1.675    40   15.1  20:52 ( 90,-18)  
July 28  10  6.76  -10  9.5   2.430   1.749    38   15.4  20:45 ( 90,-18)  

* C/2006 OF2 ( Broughton )

It will reach to 10.5 mag and will be observable in good condition in 2008 autumn. Now it is 15.9 mag (June 12, Ken-ichi Kadota), brightening as expected. 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)  
July 21  22  0.05   -8 58.5   4.022   4.919   148   15.2   2:08 (  0, 46)  
July 28  21 56.51   -8 49.5   3.919   4.864   156   15.1   1:37 (  0, 46)  

* 2P/Encke

It had been observed while brightening rapidly until the perihelion passage on Apr. 19, although it located extremely low in the evening sky. It reached to 6.7 mag on Apr. 17 (Juan Jose Gonzalez). In the Southern Hemisphere, it appeared in the morning sky at 7.8 mag in early May (May 9, Alexandre Amorim). Then it is fading rapidly, and it has faded down to 10.9 mag on May 27 (Ken-ichi Kadota). Now it must be fainter than 14 mag. It will not be higher than now in the Northern Hemisphere after this, and it will fade out rapidly.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  20 41.98  -35  4.8   0.716   1.713   162   15.2   0:51 (  0, 20)  
July 28  20 16.69  -34 40.7   0.798   1.797   164   15.8  23:51 (  0, 20)  

* 189P/2007 N2 ( NEAT )

First return of a new periodic comet discovered in 2002. It was 16.3 mag on July 16, oberved as bright as expected. It will pass very close to the earth and reach to 15 mag in July. Although it had been only observable in the Southern Hemisphere until June, it is moving northwards rapidly, and it becomes observable in good condition in the Northern Hemisphere after July. But it will fade out rapidly after August, and will be fainter than 18 mag in September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  17 21.77   -1 50.0   0.205   1.175   137   15.3  21:28 (  0, 54)  
July 28  17 41.59    9 21.9   0.225   1.174   130   15.5  21:20 (  0, 65)  

* C/2007 F1 ( LONEOS )

It was 18.2 mag on May 4 (Ken-ichi Kadota). Now it must be brightening up to 15.5 mag. But it has not been oberved at all since late May. It will approach down to 0.4 A.U. to the sun on Oct. 28, and it is expected to reach to 6 mag. However, the condition in the Northern Hemisphere is very hard. It will be getting lower in the evening sky after this. The altitude becomes lower than 20 degree in early July, and lower than 10 degree in late July. The comet is still faint as 15.5 mag at that time. After conjunction with the sun, the comet will be brighter than 11 mag in late September, and will be 8 mag in mid October. But it locates extremely low, slightly over the horizon in the morning sky. It goes to the southern sky in late October, then it will never be observable again. In the Southern Hemisphere, it becomes unobservable in July. But it will appear in the evening sky at 7 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)  
July 21  10 17.65   28 37.7   2.825   2.039    32   15.8  20:52 (118, 10)  
July 28  10 22.87   28 31.2   2.768   1.931    27   15.6  20:45 (120,  8)  

* C/2003 WT42 ( LINEAR )

It has been visible at 13.5 mag for a long time since 2005 autumn until 2006 spring. It was still bright and visible visually as 14.2 mag in winter (Dec. 22, Seiichi Yoshida). However, it has already faded down to 16.7 mag (June 23, Ken-ichi Kadota). Fine tail is visible on CCD images. It will be getting lower gradually after June, and will be too low to observe in September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  12 46.31   14 55.2   6.549   6.240    68   15.7  20:52 ( 86, 33)  
July 28  12 49.20   14  4.4   6.670   6.268    62   15.8  20:45 ( 87, 29)  

* C/2006 L2 ( McNaught )

It kept 12 mag for over half a year since last June. It was still bright as 12.6 mag on Mar. 9 (Edwin van Dijk). But it has already started fading, and it is already too faint to see visually. However, the fading is slow. The comet will be fainter than 18 mag in 2008. In the Northern Hemisphere, it keeps observable until that time.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21   5 36.24   64 36.4   3.988   3.424    49   15.8   3:19 (209, 29)  
July 28   5 43.68   64 31.9   4.001   3.484    52   15.9   3:27 (210, 32)  

* C/2006 S5 ( Hill )

Appearing in the morning sky after long time blank since last winter. It must be already bright as 16 mag. 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)  
July 21   4 54.05   27 53.9   3.678   3.010    42   16.1   3:19 (249, 19)  
July 28   5  6.91   28  4.1   3.584   2.977    46   16.0   3:27 (251, 23)  

* C/2007 G1 ( LINEAR )

Now it is 17.2 mag (June 20, 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)  
July 21  16 49.24   30 59.3   4.939   5.389   111   16.3  20:53 (  0, 86)  
July 28  16 44.67   29 42.9   4.943   5.337   107   16.2  20:45 ( 45, 83)  

* 188P/2007 J7 ( LINEAR-Mueller )

First return of a new periodic comet discovered in 1998 at 14 mag. It was recovered at 18 mag in May and June. It is a bit fainter than this ephemeris, but almost as bright as predicted. It will reach to 16 mag in 2007 summer and autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21   0 24.48   -0 50.6   2.192   2.746   112   16.5   3:19 (331, 50)  
July 28   0 27.12   -0 15.1   2.097   2.729   118   16.4   3:27 (343, 54)  

* C/2006 M4 ( SWAN )

It reached up to 4 mag in 2006 autumn. But it had faded down to 10.5 mag on Jan. 11 (Carlos Labordena). It had been unobservable for a long time since that, but now it is appearing at dawn again. Now it is 16.8 mag (May 27, Ken-ichi Kadota), fading rather rapidly. After this, it keeps observable until it becomes fainter than 18 mag in autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  22 38.17  -23 16.7   3.377   4.235   143   16.4   2:46 (  0, 32)  
July 28  22 30.89  -24 45.6   3.394   4.309   150   16.5   2:11 (  0, 30)  

* C/2006 U6 ( Spacewatch )

Appearing in the moring sky. No observations have been reported since January. But it must have already brightened up to 17 mag. 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. However, it is only observable until autumn in the Northern Hemisphere, when the comet brightens up to 15 mag. 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)  
July 21   1 32.22  -11 58.8   3.828   4.135   100   16.6   3:19 (318, 33)  
July 28   1 34.45  -13 30.8   3.675   4.083   106   16.4   3:27 (327, 35)  

* 44P/Reinmuth 2

Now it is 16.8 mag (June 18, E. Guido, G. Sostero). It will be observable at 16.5 mag in summer and autumn in 2007, and observable at 17 mag in summer and autumn in 2008.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  17 22.60  -25  0.2   1.735   2.623   143   16.5  21:27 (  0, 30)  
July 28  17 19.79  -24 38.9   1.764   2.596   136   16.4  20:57 (  0, 30)  

* C/2007 M3 ( LINEAR )

New bright comet. It is observable at 16-17 mag in 2007 summer. It will be observable brighter than 18 mag also in 2008, from spring to summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  18 32.46   -0 42.8   2.576   3.499   150   16.5  22:35 (  0, 54)  
July 28  18 15.26   -1 41.5   2.624   3.492   143   16.5  21:51 (  0, 53)  

* C/2005 S4 ( McNaught )

Now it is 17.1 mag (June 12, Ken-ichi Kadota). It will be observable at 16.5-17 mag in good condition in summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  20 11.92   16 42.4   5.011   5.850   142   16.7   0:20 (  0, 72)  
July 28  20  4.44   17  6.6   5.005   5.850   143   16.7  23:40 (  0, 72)  

* 50P/Arend

Observed on June 18 by Tony Farkas at 17.2 mag, but not officially announced yet. It will reach to 15 mag and will be observable in good condition in autumn. Then it keeps observable until it becomes fainter than 18 mag in 2008 spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21   1 43.74   12 45.3   1.888   2.131    89   16.8   3:19 (294, 49)  
July 28   1 53.01   14 46.4   1.792   2.106    92   16.7   3:27 (298, 55)  

* C/2002 VQ94 ( LINEAR )

Now it is 16.7 mag (May 27, Ken-ichi Kadota). It is outside of Jupiter's orbit. So it keeps 17 mag for a long time until 2007 summer. 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)  
July 21  13 38.50   30 45.0   7.792   7.598    75   17.1  20:52 ( 97, 50)  
July 28  13 39.03   29 44.7   7.896   7.618    70   17.2  20:45 ( 98, 46)  

* C/2006 M1 ( LINEAR )

Now it is 16.7 mag (May 27, Ken-ichi Kadota). It is outside of Jupiter's orbit. So it keeps 17 mag for a long time until 2007 summer. 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)  
July 21   2 48.60   36 57.8   4.083   3.824    68   17.2   3:19 (251, 47)  
July 28   2 54.56   36 52.6   4.014   3.848    73   17.1   3:27 (253, 52)  

* P/2006 F1 ( Kowalski )

Now it is 18.1 mag (Apr. 14, Maciej Reszelski). It is observable at 17.5-18 mag until autumn. It was discovered at 18 mag in 2006. It is a distant periodic comet, and it keeps observable at 18 mag for 4 years until 2009.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  18 51.70  -13 42.3   3.186   4.166   162   17.3  22:55 (  0, 41)  
July 28  18 47.93  -14 15.8   3.217   4.163   155   17.3  22:24 (  0, 41)  

* 96P/Machholz 1

After the perihelion passage on Apr. 4, it appeared in the morning sky and it was so bright as 5.5 mag (Apr. 10, Michael Jager and Gerald Rhemann). Then it is fading rapidly. But it is bright as 13.7 mag still now (June 26, Juan Jose Gonzalez). Now the location is very good, so it will be bright for some more time.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
July 21  16 40.14  -11 17.2   1.342   2.153   131   17.3  20:52 (  3, 44)  
July 28  16 34.62  -12 50.1   1.508   2.240   123   17.8  20:45 ( 11, 41)  

* 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)  
July 21   2 19.56    8 11.2   3.969   3.965    82   17.7   3:19 (291, 39)  
July 28   2 23.05    8 26.5   3.881   3.981    88   17.6   3:27 (297, 46)  

* 93P/Lovas 1

It was observed at 17.3 mag on July 15 (Vitali Nevski). It will brighten rapidly after this. 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)  
July 21   0 38.92    5 55.1   1.740   2.251   106   18.3   3:19 (320, 55)  
July 28   0 45.07    7 21.8   1.629   2.210   111   17.9   3:27 (331, 59)  

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