Weekly Information about Bright Comets (2008 May 17: South)

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Updated on May 16, 2008
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Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Southern Hemisphere.

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* 17P/Holmes

Great outburst occured on Oct. 24, and it bacame a naked eye comet of 2 mag. It still keeps so bright as 5.5 mag on Apr. 30 (Carlos Labordena). Now it is extremely faint and difficult to see. It was completely stellar just after the outburst. Then the coma had spread out and now it looks like a huge nebula. The coma diameter has increased up to about 90 arcmin in December and January. But now it is going away from the earth, and the diameter reduced to about 60 arcmin. Now it is getting lower and lower rapidly in the evening sky. It will be unobservable soon. But it will become observable in good condition in autumn again.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   5 50.19   35 15.1   4.101   3.306    33    5.7  18:31 (132, -3)  
May  24   6  1.55   34 57.8   4.180   3.335    29    5.7  18:28 (130, -5)  

* C/2007 W1 ( Boattini )

It is brightening much faster than expected. It is already so bright as 6.2 mag (May 14, Marco Goiato). The apparent size is so large as 20 arcmin. It will pass 0.85 A.U. from the sun in late June, and it may reach up to 4.5 mag. In the Northern Hemipshere, it is observable until around May 25, when the comet will be 6 mag. It will be unobservable for one and a half month around the perihelion passage. But it will appear in the morning sky again at 5.5 mag in early July, then it keeps observable after that while the comet is fading gradually. In the Southern Hemipsphere, it keeps observable all the period until the comet fades out, although it will be low in mid June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   9 44.88  -23 59.0   0.308   1.106    99    6.5  18:31 (147, 77)  
May  24   9  5.41  -25  0.8   0.271   1.031    86    5.8  18:28 (110, 67)  

* C/2008 C1 ( Chen-Gao )

It reached up to 9.5 mag on Mar. 29 (Maik Meyer). Now it is fading slowly. It has already faded down to 10.7 mag (May 11, Marco Goiato). Diffuse object with a weak condensation. In the Northern Hemisphere, it will be unobservable soon, then it will never be observable again. In the Southern Hemisphere, it keeps observable until it fades out.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   6 54.03    3  9.6   1.728   1.343    50   10.8  18:31 (119, 30)  
May  24   7  8.88   -0 43.5   1.796   1.383    49   11.0  18:28 (113, 31)  

* C/2006 Q1 ( McNaught )

Now it is bright as 10.9 mag (May 11, Marco Goiato). It will keep 11 mag for a long time until August. In the Southern Hemisphere, it keeps observable in good condition until summer. In the Northern Hemisphere, the altitude will never be higher than 30 degrees in the evening sky, and the comet will be unobservable in July. 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)  
May  17  10  0.89  -19 53.5   2.417   2.808   102   11.2  18:31 (170, 75)  
May  24  10  9.26  -17 31.9   2.481   2.796    97   11.2  18:28 (159, 71)  

* C/2008 A1 ( McNaught )

It is already very bright as 10.7 mag (May 14, Marco Goiato). It is expected to be 7 mag in September, but it is getting brighter than expected. However, it keeps moving in the southern sky, and it is unobservable for a while in the Northern Hemisphere. It will appear in the evening sky at 7 mag in late September, but it keeps locating in the evening low sky until the end of 2008 when it fades out down to 10 mag. Then it turns to appear in the morning sky, and it keeps observable in the northern sky after that while fading gradually. In the Southern Hemisphere, it keeps observable until late October after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   5 39.81  -33 50.8   2.620   2.303    60   11.7  18:31 ( 70, 35)  
May  24   5 48.05  -33 48.9   2.547   2.220    59   11.5  18:28 ( 69, 32)  

* 8P/Tuttle

It passed near by Earth in early January, and it became a bright large object at 5.4 mag (Jan. 3, Seiichi Yoshida). It was visible with naked eyes. Now it is fading rapidly. It has already faded down to 11.3 mag (May 10, Marco Goiato). It will be fainter than 13 mag in late May. It has already moved away towards the southern sky, and it is no longer observable in the Northern Hemisphere. In the Southern Hemisphere, it keeps observable until it fades out.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   8 27.29  -62 52.5   1.412   1.869    99   11.9  18:31 ( 22, 58)  
May  24   9  5.28  -61 52.9   1.465   1.941   101   12.4  18:28 ( 21, 60)  

* 19P/Borrelly

It will reach to 11 mag in summer. It must have already brightened up to 14 mag, but the comet was not observed recently. The condition in this apparition is bad. In the Southern Hemisphere, it keeps extremely low, or under the horizon, so it will not be observable. In the Northern Hemisphere, it is not observable until August when it appears in the morning sky at 11 mag. After August, it keeps observable and fading in the morning sky.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   2 41.66   -0 23.5   2.424   1.553    23   12.2   5:21 (268,  4)  
May  24   3  0.81    2  9.3   2.383   1.517    24   12.0   5:25 (264,  5)  

* C/2006 OF2 ( Broughton )

It brightened up to 13.5 mag and became visible visually in 2007 autumn (Nov. 13, Juan Jose Gonzalez). It had been unobservable for a while, but now it is appearing in the morning sky. Now it is 13.0 mag (Apr. 27, J. Broughton), brightening as expected. It will reach to 10.5 mag and will be observable in good condition in 2008 autumn. It keeps observable, visible visually, brighter than 14 mag for one year until 2009 May.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   0 50.91   26  8.7   3.489   2.770    38   12.1   5:21 (230,  8)  
May  24   1  3.05   28  6.9   3.408   2.735    41   12.0   5:25 (225, 10)  

* C/2007 G1 ( LINEAR )

Now it is 13.0 mag, already visible visually (May 12, Juan Jose Gonzalez). It will be bright at 12 mag for a long time from 2008 spring to 2009 spring. However, it is only observable until August in the Northern Hemisphere because the comet moves southwards. It keeps observable for a long time in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  17 53.16  -13 14.0   2.368   3.260   146   12.5   2:14 (180, 68)  
May  24  17 42.99  -15  1.7   2.269   3.219   155   12.4   1:37 (180, 70)  

* C/2008 J1 ( Boattini )

New comet. It is bright as 12.3 mag, and visible visually (May 12, Juan Jose Gonzalez). In the Northern Hemisphere, it keeps observable at 12-13 mag for a long time after this until autumn. It will move near by the Northern Pole from summer to autumn, and will be observable all night. Then it keeps observable until 2009 spring when the comet becomes faint. In the Southern Hemisphere, it is only observable until mid June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  21 18.52   21 39.9   1.640   1.879    86   12.8   5:21 (185, 33)  
May  24  21 26.15   27 44.6   1.571   1.845    88   12.6   5:19 (180, 27)  

* P/2008 J2 ( Beshore )

New comet. It is bright as 12.7 mag, and visible visually (May 12, Juan Jose Gonzalez). It keeps observable in good condition until autumn. But it is moving southwards gradually, and the altitude will be getting somewhat lower in the Northern Hemisphere. The calculation says it keeps bright at 13 mag for a while. However, it can be in a temporary outburst now, and it may be a very faint short periodic comet originally. It may fade out very rapidly after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  17  0.72  -13 53.0   1.487   2.458   159   13.6   1:22 (180, 69)  
May  24  16 55.82  -14 10.3   1.466   2.461   166   13.6   0:50 (180, 69)  

* C/2007 B2 ( Skiff )

Now it is very bright as 12.7 mag (Apr. 12, Marco Goiato). It will keep visible visually at 13 mag until June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  11 59.04   -0 25.4   2.448   3.123   123   13.6  20:17 (180, 56)  
May  24  11 58.60   -1 26.4   2.507   3.103   117   13.6  19:49 (180, 57)  

* C/2006 U6 ( Spacewatch )

It was 15 mag on Jan. 14 (Michael Mattiazzo), brightening as expected. It will reach to 13.5 mag in the southern sky in spring and summer. In the Southern Hemisphere, it keeps observable for a long time after this. But in the Northern Hemisphere, it is not observable now. But it will appear in the morning sky at 15 mag in November, then it keeps observable while the comet will be fading slowly.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   4 55.36  -42 17.9   2.775   2.507    64   13.7  18:31 ( 57, 30)  
May  24   5 19.44  -41 47.0   2.757   2.502    64   13.7  18:28 ( 58, 30)  

* 29P/Schwassmann-Wachmann 1

After an outburst on Dec. 29, some outbursts occured repeatedly until mid January. It became very bright as 10.4 mag on Jan. 15 (P. Clay Sherrod). Then it is fading gradually. But it was still bright as 12.7 mag on Mar. 5 (Juan Jose Gonzalez). Now it is 13.7 mag (Apr. 4, Carlos Labordena), and extremely diffuse. It will be too low to observe at the end of May.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   6 24.56   27 39.9   6.773   6.024    39   14.0  18:31 (131,  7)  
May  24   6 29.98   27 30.5   6.841   6.026    33   14.0  18:28 (128,  5)  

* 15P/Finlay

It was so faint as 17.2 mag on Apr. 27 (E. Guido, G. Sostero). But now it must be brightening very rapidly. Terry Lovejoy reported that it is already very bright as 12-13 mag on May 14. It is expected to reach up to 12 mag in June and July. However, it keeps locating extremely low for a while in the Northern Hemisphere. It will be getting higher gradually after late July, then it keeps observable while fading gradually.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   0 19.93   -2 56.0   1.363   1.107    53   14.7   5:21 (247, 34)  
May  24   0 50.62    0 57.1   1.346   1.063    51   14.2   5:25 (243, 32)  

* C/2007 N3 ( Lulin )

Now it is 13.8 mag (May 12, Juan Jose Gonzalez), brightening as expected and already visible visually. It is getting higher gradually in the morning sky. It is expected to reach to 6 mag in 2009 February. After this, it keeps observable until October when it becomes 11 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  21 51.32  -12  5.8   3.266   3.427    90   14.4   5:21 (210, 64)  
May  24  21 48.57  -12 16.2   3.060   3.353    97   14.2   5:25 (190, 67)  

* 46P/Wirtanen

It brightened up to 8.3 mag on Feb. 6 (Juan Jose Gonzalez). However, now it is fading and getting diffuse very rapidly. It has already faded down to 12.5 mag (Apr. 29, Mitsunori Tsumura). It will be too faint to see visually soon. In the Northern Hemisphere, it keeps observable in good condition until July when it becomes fainter than 18 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   8 58.95   29 18.0   1.675   1.682    72   14.5  18:31 (163, 24)  
May  24   9 19.61   27 36.6   1.783   1.742    71   15.0  18:28 (161, 25)  

* C/2005 L3 ( McNaught )

Now it is 12.9 mag (Apr. 27, Sandor Szabo and Zoltan Toth), very bright visually. It keeps observable visually at 13 mag at high location for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  16 12.94   20 34.8   4.860   5.663   139   14.6   0:34 (180, 34)  
May  24  16  4.19   21 20.4   4.879   5.671   137   14.6  23:53 (180, 34)  

* C/2008 J4 ( McNaught )

New comet. It will approach to the sun down to 0.44 A.U. on June 19. So it will brighten very rapidly after this. In the Northern Hemisphere, it will be observable at 13 mag in the morning low sky from early June to mid June. Then it will never be observable again. In the Southern Hemisphere, it is observable only until late May.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  23 52.27    2 12.2   0.859   0.907    57   15.7   5:21 (237, 36)  
May  24   0 33.56   16 59.5   0.753   0.779    49   14.8   5:25 (227, 23)  

* C/2007 T1 ( McNaught )

It brightened up to 8.5 mag on Jan. 6 (Alexandre Amorim). It kept bright until March, however, now it is getting diffuse and fading rapidly. It has already faded down to 12.0 mag (Mar. 30, Marco Goiato). It will be too low to observe in late May.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   6 54.46    6 52.4   3.108   2.571    49   14.9  18:31 (122, 27)  
May  24   7  0.84    8  3.1   3.281   2.655    44   15.2  18:28 (119, 23)  

* C/2006 W3 ( Christensen )

It is already bright as 14.7 mag and visible visually (Mar. 5, Seiichi Yoshida). 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 Hemisphere. But it becomes low from April to June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   3 34.35   56 37.9   5.723   4.957    37   14.9   5:21 (220,-33)  
May  24   3 38.57   56 59.9   5.687   4.911    36   14.9   5:25 (219,-30)  

* 197P/2008 E2 ( LINEAR )

It was recovered at 18.7 mag on Mar. 3, as bright as expected (R. E. Hill). Then it is brightening rapidly as expected, and already brightened up to 15.5-16.0 mag (Apr. 14, Michael Jager). It will reach to 15 mag in May. In the Southern Hemisphere, it keeps observable in good condition until it fades out. In the Northern Hemisphere, the condition is bad. It will be too low to observe in mid May.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  22  2.94  -22 43.4   0.295   1.061    91   15.1   5:21 (231, 72)  
May  24  22 54.18  -29 49.5   0.321   1.062    90   15.3   5:25 (258, 72)  

* 26P/Grigg-Skjellerup

Although it had been extremely fainter than expected until March, it brightened very rapidly in April. It became very bright and visible visually at 11.3 mag (Apr. 12, Marco Goiato). However, it was difficult to see because extremely diffuse. CCD observers reported it so faint as 15 mag. This comet tends to be brightest after the perihelion passage. In the Northern Hemisphere, it had been low until March, but now it locates high. It will be visible visually at 12-13 mag until early May in the good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  20 32.37   17 30.6   0.698   1.311    98   15.1   4:53 (180, 38)  
May  24  20 36.14   20 38.2   0.721   1.357   101   15.6   4:29 (180, 34)  

* C/2006 V1 ( Catalina )

In the Southern Hemisphere, it keeps 15-16 mag and observable in good condition until 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)  
May  17  20 48.57  -50 50.7   2.686   3.210   112   15.4   5:09 (  0, 74)  
May  24  20 49.89  -51  3.4   2.653   3.249   117   15.4   4:43 (  0, 74)  

* C/2006 S5 ( Hill )

It brightned up to 13.4 mag on Jan. 4 (Seiichi Yoshida). Now it is fading. It was still visible visually at 14.4 mag on Mar. 5 (Seiichi Yoshida). But it has already faded down to 15.6 mag (Apr. 6, Ken-ichi Kadota).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   8 45.26   10 29.4   3.210   3.100    74   15.9  18:31 (151, 40)  
May  24   8 54.10    9 53.0   3.332   3.138    70   16.1  18:28 (147, 39)  

* 79P/du Toit-Hartley

Now it is 17.4 mag (Mar. 10, Mitsunori Tsumura). It will be observable at 16-17 mag from April to July. It will be fainter than 18 mag in August. It keeps locating in the evening sky all time.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   9 13.10   12 22.7   0.898   1.238    80   16.2  18:31 (161, 41)  
May  24   9 36.12   10 22.9   0.902   1.232    79   16.2  18:28 (160, 43)  

* C/2007 W3 ( LINEAR )

It will reach to 16 mag from May to July, and will be observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  20 21.87   83 35.2   1.805   1.789    72   16.3   4:44 (180,-29)  
May  24  17 45.78   83 24.1   1.746   1.781    75   16.2   1:44 (180,-28)  

* C/2007 M2 ( Catalina )

Now it is 16.8 mag (Feb. 29, Ken-ichi Kadota). It keeps 16 mag for one year from 2008 spring to 2009 spring. In the Northern Hemisphere, it keeps observable in good condition while the comet is brightening until 2008 spring. But the comet moves southwards after that, and it will never observable after 2008 July.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  10 57.20    5 22.7   3.583   3.999   107   16.3  19:15 (180, 50)  
May  24  10 53.92    4 25.1   3.668   3.971    99   16.3  18:44 (180, 51)  

* 124P/Mrkos

Now it is 16.1 mag (Mar. 9, Ken-ichi Kadota), brightened as expected. Although it had been observable in good condition for a while, it will be getting lower rapidly after this. It becomes unobservable in June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   9 55.59    0 34.6   1.010   1.483    94   16.7  18:31 (173, 54)  
May  24  10  6.16   -3 22.8   1.071   1.495    91   16.8  18:28 (166, 58)  

* 6P/d'Arrest

Now it is 18.9 mag (Apr. 26, W. T. Ryle). It will be brightening rapidly after this. It will reach up to 9 mag and keep bright for a long time from summer to autumn. In the Northern Hemisphere, it becomes low in the south at brightest, but it keeps observable until it fades out.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  18 52.76   10 54.2   0.907   1.686   122   16.9   3:13 (180, 44)  
May  24  19  0.30   12  7.2   0.832   1.643   125   16.7   2:53 (180, 43)  

* C/2007 K3 ( Siding Spring )

No observations have been succeeded since 2007 July. Now it is appearing in the morning sky, and it is predicted to be so bright as 14 mag. But actually, it was not detected, fainter than 16.8 mag on Apr. 12 (Esteban Reina Lorenz). It seems to be much fainter than expected. It will be observable in good condition from spring to summer. However, maybe it has already disappeared.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  21 43.34   -2 23.1   1.826   2.073    89   16.9   5:21 (199, 56)  
May  24  21 52.95   -0 12.4   1.778   2.087    92   16.8   5:25 (189, 55)  

* 2005 WY3

Peculiar asteroid moving on a cometary orbit. It reached up to 15.0 mag on Mar. 11 (Katsumi Yoshimoto). It has passed the perihelion in late January, but still completely asteroidal. It is already going away from the sun and fading. In the Northern Hemisphere, it keeps observable until July when it becomes fainter than 18 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  11 18.01    7  8.3   1.585   2.166   111   16.9  19:37 (180, 48)  
May  24  11 27.34    7 46.8   1.698   2.208   106   17.1  19:18 (180, 47)  

* 85P/Boethin

It is expected to reach up to 7.5 mag in winter, and will be observable in good condition. However, this comet has not been observed since 1986. It is predicted to be already brightening as 17 mag. The condition of this apparition is good. It keeps observable for a long time until 2009 early summer both in the Northern Hemisphere and Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  20 40.40  -22 49.0   2.287   2.796   109   17.2   5:01 (180, 78)  
May  24  20 44.29  -22 42.5   2.140   2.735   115   16.9   4:37 (180, 78)  

* 22P/Kopff

It will be bright at 9-10 mag for a long time from spring to autumn in 2009. Now it is predicted to be so faint as 19 mag. But actually, it is 16-17 mag recently, much brighter than expected. Maybe it is in a temporary outburst.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   9 52.75   16 18.5   3.281   3.406    88   16.9  18:31 (174, 39)  
May  24   9 56.08   15 58.6   3.348   3.370    82   16.9  18:28 (167, 38)  

* 180P/2006 U3 ( NEAT )

Now it is 16.7 mag (Feb. 16, Ken-ichi Kadota), brightened as expected. After this, it will be getting fainter slowly and getting lower slowly in the evening sky.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  10 45.68   28 49.9   2.166   2.470    95   17.0  19:04 (180, 26)  
May  24  10 52.27   27 24.7   2.242   2.469    90   17.1  18:43 (180, 28)  

* C/2008 H1 ( LINEAR )

Now it is 16.5 mag (Apr. 22, Ken-ichi Kadota). It keeps observable in good condition while the comet will be fading slowly.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  13 35.75   72  5.1   2.708   2.829    86   17.2  21:51 (180,-17)  
May  24  13 16.75   68 44.1   2.739   2.845    85   17.2  21:06 (180,-13)  

* C/2007 M3 ( LINEAR )

Now it is brightest at 17 mag. But it will be fading gradually, and it will be fainter than 18 mag in July.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  14 50.45  -13 49.4   3.166   4.160   167   17.2  23:07 (180, 69)  
May  24  14 37.02  -13 16.2   3.238   4.193   157   17.3  22:26 (180, 68)  

* 68P/Klemola

Now it is 18.8 mag (Apr. 25, V. Nevski). It keeps observable while the comet will be brightening gradually after this. It will reach up to 14.5 mag in autumn. However, then it locates low in the evening sky, and it will be unobservable soon in December.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  15 56.02   -5  4.7   1.947   2.935   164   17.5   0:17 (180, 60)  
May  24  15 50.48   -4 28.9   1.905   2.890   163   17.3  23:40 (180, 59)  

* C/2005 S4 ( McNaught )

It was observed at 16.5-17 mag in 2006 and 2007. Because it is a very distant comet, it is observable at 17 mag still in 2008 in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  19 29.44   38 41.4   5.969   6.231   100   17.3   3:50 (180, 16)  
May  24  19 23.65   39 54.4   5.932   6.248   103   17.3   3:17 (180, 15)  

* 7P/Pons-Winnecke

Brightening rapidly. It will reach to 14 mag in autumn. However, it locates extremely low in the Northern Hemisphere. It keeps higher than 30 degree even in the Northern Hemisphere until August, when it brightens up to 15 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  10 35.59   37 13.1   1.680   1.954    89   17.4  18:54 (180, 18)  
May  24  10 41.29   35 37.1   1.696   1.901    85   17.3  18:32 (180, 20)  

* C/2002 VQ94 ( LINEAR )

It had been observed at 16.5 mag for a long time from 2005 to 2007. Now it is fading. But it keeps observable at 17.5 mag in good condition for a long time until July.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17  14  0.48   15 31.8   7.815   8.593   137   17.4  22:18 (180, 40)  
May  24  13 57.54   15 12.0   7.903   8.619   132   17.5  21:47 (180, 40)  

* 2008 HW1

It will approach to the sun down to 0.1 A.U. on June 17. It moves very fast in the northern sky in May. It is observable at 16 mag in good condition in first half of May in the Northern Hemisphere. It passes near by Polaris in mid May, and it will be unobservable at the end of May. If it shows a cometary activity, it may become much brighter than this ephemeris.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
May  17   6  8.93   84  8.6   0.195   0.949    66   17.5  18:31 (171,-31)  
May  24   5 13.89   52 30.9   0.284   0.795    34   20.3  18:28 (138,-22)  

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