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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 5.5 mag (Feb. 24, 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)
Mar. 3 22 24.42 -62 57.8 1.594 1.328 56 6.0 5:04 (327,-35)
Mar. 10 22 40.94 -64 42.9 1.664 1.463 60 6.6 4:54 (329,-35)
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It will reach to 6 mag at the perihelion passage in mid April. It has already started brightening very rapidly. Now it is 13.3 mag (Feb. 14, Juan Jose Gonzalez), already visible visually. It is observale while brightening gradually in the evening sky in the Northern Hemisphere. However, it will locate very low after this. It will be 11.5 mag in mid March, when the altitude becomes lower than 10 degree. After conjunction with the sun, it appears in the morning sky at 12 mag in June. But it locates only 20 degree high at most, and it will be fading rapidly. In the Southern Hemisphere, it appears in the morning sky at 8 mag in May, then it will be bright and observable for a while.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 0 35.87 10 53.6 1.799 1.081 31 11.9 19:20 ( 94, 13)
Mar. 10 0 52.29 12 24.4 1.714 0.966 28 11.4 19:26 ( 98, 10)
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First return of a new bright periodic comet observed at 9 mag in 2001. It brightened rapidly also in this return. It was 16.1 mag on Jan. 11 (Filip Fratev), but it brightened up to 11.7 mag on Feb. 14 (Juan Jose Gonzalez). Fainter than expected by 1.5 mag, but unexpectedly, it became visible visually. However, the condition of this apparition is bad. It keeps locating very low in the evening until early May. It will be fading after this.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 0 48.10 3 31.8 1.650 0.942 30 12.4 19:20 ( 86, 12)
Mar. 10 1 21.26 5 29.7 1.643 0.958 32 12.6 19:26 ( 88, 13)
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Now it is 12.2 mag (Dec. 28, Juan Jose Gonzalez). It has been 12 mag for half a year since last June. But it will start fading after March. It will be too faint to see visually in April. 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)
Mar. 3 20 23.81 63 8.8 2.383 2.345 75 13.1 5:04 (214, 40)
Mar. 10 21 3.28 66 6.5 2.452 2.389 74 13.2 4:54 (210, 38)
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Not yet observed in this return. But it must be brihtening very rapidly towards the perihelion passage on Apr. 4. However, it is not observable until April. It will appear in the morning sky at 8 mag in mid April in the Northern Hemisphere, or at 10 mag in late April in the Southern Hemisphere. Then the condition will get better rapidly. However, the comet will fade out rapidly. It will be fainter than 14 mag in mid May, too faint to see visually.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 22 37.83 -33 4.3 1.754 0.969 26 14.4 5:04 (293,-28)
Mar. 10 23 8.02 -29 30.7 1.596 0.817 25 13.2 4:54 (288,-29)
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It reached up to 9.3 mag between October and November (Oct. 27, Juan Jose Gonzalez). It had been observable in excellent condition. But it is fading now. It has already faded down to 12.3 mag (Feb. 20, Katsumi Yoshimoto). However, it keeps observable after this until May when it fades down to 16 mag. It will keep visible visually until March.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 4 33.47 11 53.3 1.761 1.970 86 13.3 19:20 ( 47, 59)
Mar. 10 4 47.52 12 40.2 1.863 2.005 83 13.6 19:26 ( 54, 57)
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In this season, it has been bright as 12-13 mag and visible visually since it appeared in the morning sky in early July. Another outburst occurred on Jan. 29. It is visible bright as 13.0 mag still now (Feb. 12, Carlos Labordena). It will be getting lower in the evening sky after this. It will be too low to see in April.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 3 52.00 28 29.3 5.977 5.888 80 13.7 19:20 ( 86, 62)
Mar. 10 3 55.36 28 27.6 6.088 5.890 73 13.7 19:26 ( 91, 55)
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It suddenly brightened in outburst on Oct. 24, and reached up to 4.2 mag on Oct. 25 (Maik Meyer). But it had faded down to 10.5 mag on Jan. 11 (Carlos Labordena). Now it is not observable. It will appear in the morning sky again at 15-16 mag in May. Then 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)
Mar. 3 22 17.45 -7 55.1 3.592 2.618 8 13.9 5:04 (272,-11)
Mar. 10 22 24.07 -8 8.4 3.657 2.705 14 14.2 4:54 (274, -9)
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Now it is 13.1 mag (Feb. 14, Masayuki Suzuki). It has been 13 mag for a long time since last autumn. However, it will be fading gradually after this. It is observable in good condition in the Southern Hemisphere, although it is already not observable in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 15 46.42 -67 35.9 2.013 2.239 89 14.1 5:04 ( 0,-13)
Mar. 10 16 2.16 -69 9.2 2.005 2.278 92 14.2 4:54 ( 0,-14)
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Now it is 14.4 mag (Feb. 12, Juan Jose Gonzalez). Almost asteroidal. It did not brighten at all since early September. Although the slight cometary activity was detected in late July, it became completely stellar soon. Its tail became visible again in late October, however, it turned to be stellar again soon. Finally it has passed the perihelion, keeping almost asteroidal. It kept observable at 14 mag in good condition in the Northern Hemisphere for a long time. However, it will be fading after this. It will start getting lower in April, and will be too low in the evening sky at 17 mag in June.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 5 7.49 31 36.1 0.993 1.483 96 14.4 19:20 ( 76, 78)
Mar. 10 5 34.45 28 9.7 1.084 1.538 95 14.6 19:26 ( 66, 75)
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It has been visible at 13.5 mag for a long time since 2005 autumn until 2006 spring. Now it is fainter than last year by 1 mag, however, it is still visible visually at 14.2 mag (Dec. 22, Seiichi Yoshida). It keeps observable in excellent condition until April.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 13 8.68 23 46.0 4.910 5.737 143 14.4 2:28 ( 0, 79)
Mar. 10 13 6.11 23 57.4 4.896 5.759 147 14.5 1:58 ( 0, 79)
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Now it is 15.9 mag (Jan. 10, Ken-ichi Kadota). It keeps observable at 15 mag in the evening sky until May. It is not observable around the perihelion passage in conjunction with the sun. Then it moves to the southern sky, and it will be unobservable in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 3 25.38 45 1.6 2.482 2.506 79 15.5 19:20 (121, 59)
Mar. 10 3 38.68 44 7.8 2.503 2.450 75 15.4 19:26 (119, 55)
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Although it had been unobservable since last autumn, now it is appearing again in the morning sky. It will be observable at 14.5 mag from spring to summer both in 2007 and 2008. The condition is good, and it may be visible visually.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 19 1.24 -13 33.6 6.526 6.049 57 15.5 5:04 (307, 23)
Mar. 10 19 1.53 -13 0.8 6.396 6.030 64 15.4 4:54 (310, 26)
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Now it is 15.9 mag (Feb. 15, Mitsunori Tsumura). It will reach to 11 mag in 2008 spring. It keeps moving in the southern sky until that, so it keeps locating very low in the Northern Hemisphere. It keeps observable in good condition in the Southern Hemisphere. In the Northern Hemisphere, it is observable at 16 mag in the evening low sky until March, then it will be unobservable. It will be observable again in a short time in the very low sky at dawn in November at 13 mag. After 2008 March, it will be visible visually at 11 mag in the morning low sky.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 4 51.26 -34 27.6 5.405 5.419 85 15.8 19:20 ( 16, 19)
Mar. 10 4 53.18 -33 38.2 5.413 5.368 82 15.8 19:26 ( 22, 17)
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Now it is 15.3 mag (Jan. 7, Ken-ichi Kadota). It is observable at 15.5-16 mag until spring. But, in the Northern Hemisphere, it locates somewhat low at 20-30 degree high.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 4 50.75 -27 32.7 3.825 3.887 86 15.8 19:20 ( 18, 25)
Mar. 10 4 45.37 -26 15.6 3.926 3.887 80 15.9 19:26 ( 27, 23)
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Now it brightened up to 16.0 mag (Feb. 21, Ken-ichi Kadota). It keeps 15.5-16 mag for one year and a half after this until 2008 summer. However, because the comet moves southwards, it is only observable until 2007 June in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 10 45.23 2 33.4 2.819 3.807 175 16.3 0:05 ( 0, 58)
Mar. 10 10 39.57 2 17.2 2.779 3.760 169 16.2 23:27 ( 0, 57)
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When it approached to the earth between from November to early December, it reached up to 8.5 mag as a very large diffuse object with a diameter larger than 10 arcmin (Nov. 23, Peter Bus). However, now it is fading rapidly. It has already faded down to 14.7 mag (Feb. 11, Mitsunori Tsumura). It will set down in the evening sky at 17 mag in March.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 1 19.85 34 34.8 2.785 2.346 54 16.2 19:20 (112, 33)
Mar. 10 1 22.06 34 38.3 2.954 2.414 48 16.7 19:26 (115, 27)
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It was still visible visually at 14.2 mag on Oct. 31 (Seiichi Yoshida). However, it has already faded down to 16.3 mag (Jan. 30, Ken-ichi Kadota). It keeps a good contition until spring, while the comet will be fading gradually.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 9 15.73 26 43.4 3.765 4.647 149 16.9 22:32 ( 0, 82)
Mar. 10 9 11.89 26 37.2 3.887 4.712 142 17.0 22:00 ( 0, 82)
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Now it is 16.8 mag (Dec. 29, Katsumi Yoshimoto). 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)
Mar. 3 14 44.57 39 54.8 6.713 7.245 118 17.1 4:04 (180, 85)
Mar. 10 14 41.57 40 12.9 6.683 7.261 122 17.1 3:33 (180, 85)
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It was observed at 19 mag in mid December. It brightened up to 18 mag on Feb. 15. It will reach to 17 mag in spring, and will be observable in good condition.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 10 59.44 4 53.4 1.357 2.348 177 17.2 0:19 ( 0, 60)
Mar. 10 10 54.55 5 33.8 1.340 2.330 173 17.1 23:42 ( 0, 61)
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It was observed at 17.5 mag in 2006 spring. It will be observable at 17 mag in good condition in 2007 spring.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 14 14.77 -13 18.8 4.070 4.722 125 17.2 3:34 ( 0, 42)
Mar. 10 14 13.82 -13 18.0 3.987 4.723 133 17.2 3:06 ( 0, 42)
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It reached to 16 mag in early 2006. Now it is 17.3 mag (Dec. 2, Ken-ichi Kadota). It will be fading very slowly from 17 mag to 18 mag until 2007 summer. In the Northern Hemisphere, it keeps locating high.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 14 22.10 33 28.0 5.147 5.774 125 17.3 3:41 ( 0, 88)
Mar. 10 14 20.08 33 48.4 5.127 5.801 128 17.3 3:12 ( 0, 89)
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Very far new comet. It will be observable at 17.5-18 mag more than one year after this.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 9 42.09 -6 0.6 7.798 8.725 157 17.4 22:58 ( 0, 49)
Mar. 10 9 40.57 -5 31.4 7.826 8.726 153 17.4 22:29 ( 0, 49)
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Now it is 16.8 mag (Jan. 9, Mitsunori Tsumura). The perihelion passage is in 2008. It will be observable for several years after this at around 17 mag. But it may fade out rapidly just after the perihelion passage.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 4 19.14 14 49.9 4.602 4.598 83 17.4 19:20 ( 56, 59)
Mar. 10 4 22.58 15 19.2 4.698 4.587 77 17.5 19:26 ( 65, 54)
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It reached to 16.5 mag at best in December and January. But now it is already fading. It will be fainer than 18 mag in April.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 6 19.08 27 33.0 1.781 2.343 112 17.5 19:36 ( 0, 83)
Mar. 10 6 25.18 27 15.3 1.864 2.349 106 17.6 19:26 ( 18, 82)
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It tends to become brightest about 4 months after the perihelion passage. In this apparition, it was 17.6 mag in late July around the perihelion passage (July 23, Filip Fratev), however, it brightened up to 14.1 mag and became visible visually on Dec. 23 (Seiichi Yoshida). But it will start fading after this. Although it keeps a good condition for a long time, it will be fainter than 18 mag in March.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 5 40.49 22 39.8 2.104 2.528 103 17.6 19:20 ( 23, 77)
Mar. 10 5 47.45 22 59.7 2.225 2.563 98 17.9 19:26 ( 45, 74)
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Recovered at 19.3 mag on Nov. 18 (E. J. Christensen). It is a tiny comet, however, it will pass near, only 0.3 A.U., by the earth in February and it was expected to be 17 mag. But actually, it was reported so faint, fainter than 19.5 mag. It will fade out very rapidly after this.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 19 32.36 79 32.3 0.310 1.040 90 17.6 5:04 (192, 40)
Mar. 10 16 41.48 77 16.3 0.320 1.076 96 17.8 4:54 (183, 47)
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It will reach to 11 mag in 2009 summer and autumn. It keeps observable in good condition until 2009 summer in the Northern Hemisphere. But after the maximum brightness, it goes to the southen sky. It will be 14 mag in 2008 summer and visible visually. Then it keeps visible visually for one year.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 5 37.92 48 38.1 7.686 7.962 102 17.6 19:20 (163, 76)
Mar. 10 5 35.47 48 26.6 7.750 7.915 95 17.6 19:26 (144, 72)
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It has been observed in good condition at 17 mag. But it will be fading after this, and it becomes fainter than 18 mag in April. It will be observable in good condition at 18 mag again one year later.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 4 21.05 46 47.9 3.695 3.820 89 17.7 19:20 (130, 68)
Mar. 10 4 28.41 46 24.0 3.787 3.822 84 17.7 19:26 (125, 63)
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It had been lost since its discovery in 1986. But it was rediscovered on Jan. 9 at 16-17 mag. The condition is good in this return, and it was expected to reach to 14 mag from autumn to winter. But actually, it is fainter than originally expected, and it reached to 17 mag at best. Now it is 17.4 mag (Feb. 11, Mitsunori Tsumura). It will be fainter than 18 mag soon.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 1 33.28 10 40.0 2.224 1.654 43 18.4 19:20 ( 86, 25)
Mar. 10 1 52.94 12 27.0 2.301 1.694 41 18.6 19:26 ( 90, 23)
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It was in major outburst unexpectedly and reached to 10.5 mag in its last appearance in 1999. However, it is faint in this apparition, 17 mag at best. It is already fainter than 18 mag.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 14 0.76 -22 7.2 1.793 2.503 125 18.7 3:20 ( 0, 33)
Mar. 10 13 57.98 -22 35.4 1.761 2.542 132 18.8 2:50 ( 0, 32)
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Peculiar asteroid moving along a cometary orbit. It will approach to Sun down to 0.6 A.U. in late April. Then it will pass very near by Earth in May. The condition to observe it is very bad. Nobody can observe it until late May in the Northern Hemisphere. In the Southern Hemisphere, it will be observable in the morning low sky from late April to mid May. It will be 18.5 mag at best if it keeps asteroidal. However, if it shows cometary activity, it may be observed at 12-14 mag in the Southern Hemisphere. Then it may be visible visually at 11 mag in the evening sky in late May also in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 3 0 42.64 -0 55.7 2.073 1.285 27 20.2 19:20 ( 84, 7)
Mar. 10 0 42.06 -1 54.8 2.048 1.174 20 19.8 19:26 ( 88, 0)
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