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Great outburst occured on Oct. 24, and it bacame a naked eye comet of 2 mag. It still keeps so bright as 2.7 mag on Dec. 9. It was completely stellar just after the outburst, however, then a round disk like coma is getting larger gradually. The coma diameter has increased up to about 70 arcmin, and the comet has bacome very diffuse. So it looks like a huge nebula now. This comet was also in great outburst at the discovery in 1892 and became so bright as 4 mag. At that time, the comet faded after the first outburst, but soon brightened again in the second outburst. The further brightness is uncertain. But the comet will be observable in excellent condition for a while after this. It will be brighter than this ephemeris. It will be easily visible with naked eyes for a while after this in the dark sky.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 3 1.32 46 51.5 1.796 2.645 142 4.2 21:26 (180, 78)
Dec. 22 2 58.92 45 42.4 1.864 2.675 137 4.5 20:56 (180, 79)
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It will reach to 6 mag in January, and will be observable in good condition. Now it is brightening very rapidly. It is already bright as 7.9 mag (Dec. 9, Seiichi Yoshida), large bright diffuse object visually. In the Northern Hemisphere, 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 Hemisphere, 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)
Dec. 15 23 58.14 73 11.6 0.413 1.215 114 7.8 18:27 (180, 52)
Dec. 22 0 49.07 60 5.8 0.322 1.163 116 6.9 18:49 (180, 66)
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Now it is 10.6 mag (Oct. 14, Mike Linnolt). It is already unobservable in the Northern Hemisphere. In the Southern Hemisphere, it is not observable now for one month after mid November, but it will be observable in good condition at 10 mag from mid December to February. In the Northern Hemisphere, it will appear in the evening sky at 11 mag in March, then it keeps observable while fading gradually until May.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 17 4.89 -46 54.4 1.781 0.970 24 9.6 5:29 (311,-25)
Dec. 22 17 4.04 -50 58.3 1.712 0.983 29 9.6 5:33 (317,-22)
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Brightening rapidly. Now it is 11.1 mag (Dec. 1, Marco Goiato), already bright visually. 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.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 22 52.14 -19 24.7 1.064 1.245 74 11.5 18:20 ( 18, 34)
Dec. 22 23 7.97 -16 34.0 1.050 1.200 72 11.0 18:23 ( 23, 36)
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Already unobservable in the Northern Hemisphere, but it is observable in the evening low sky in the Southern Hemisphere. It approached down to 0.4 A.U. to the sun on Oct. 28, and it reached to 5.3 mag (Oct. 25, Juan Jose Gonzalez). Now it is fading. It has already faded down to 10.1 mag (Dec. 1, Marco Goiato). The brightening became very slow just before the perihelion passage, but it started fading rapidly after the perihelion passage. It will never be observable again in the Northern Hemisphere. But in the Southern Hemisphere, 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)
Dec. 15 17 53.92 -58 4.9 1.824 1.167 35 12.0 18:20 ( 37,-29)
Dec. 22 18 3.72 -60 3.7 1.941 1.293 36 12.6 18:23 ( 36,-32)
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Now it is bright as 12.5 mag and visible visually (Dec. 9, Seiichi Yoshida), 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)
Dec. 15 9 47.90 -47 35.1 3.325 3.439 88 12.8 4:15 ( 0, 7)
Dec. 22 9 50.64 -48 38.2 3.231 3.398 91 12.7 3:51 ( 0, 6)
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Now it is faint as 14.0 mag (Dec. 8, 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)
Dec. 15 6 13.96 30 50.8 5.012 5.976 167 13.3 0:42 ( 0, 86)
Dec. 22 6 10.08 30 48.7 5.002 5.978 172 13.3 0:11 ( 0, 86)
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Now it is bright and visible visually at 12.8 mag (Dec. 8, Seiichi Yoshida). It keeps locating in good position for a while after this. But it will start fading gradually after January.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 0 48.52 27 2.4 1.009 1.705 117 13.5 19:14 ( 0, 82)
Dec. 22 0 59.49 27 32.1 1.055 1.705 113 13.6 18:58 ( 0, 83)
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It is already bright and visible visually at 13.5 mag (Nov. 13, Juan Jose Gonzalez). 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)
Dec. 15 21 33.56 -3 57.4 4.140 3.785 62 13.9 18:20 ( 48, 39)
Dec. 22 21 39.05 -3 14.7 4.178 3.733 56 13.8 18:23 ( 54, 36)
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Now it is bright as 14.0 mag and visible visually (Dec. 8, Seiichi Yoshida). It keeps observable in good condition for a long time until 2008 spring. It will keep visible visually at 14 mag until March.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 7 58.68 19 37.5 1.765 2.631 144 13.9 2:27 ( 0, 75)
Dec. 22 7 57.58 19 1.9 1.725 2.634 151 13.9 1:58 ( 0, 74)
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It reached to 7.2 mag on July 14 (Maik Meyer), then it faded down to 9.0 mag on Aug. 13 (Carlos Labordena). Although it had been unobservable for a while, now it is observable again. In the Southern Hemisphere, it keeps observable while fading gradually. In the Northern Hemisphere, it will be fading while keeping extremely low.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 11 23.10 -45 2.8 2.247 2.199 74 14.5 5:29 (356, 10)
Dec. 22 11 5.33 -46 49.7 2.209 2.283 81 14.7 5:06 ( 0, 8)
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Now it is 14.4 mag and visible visually (Dec. 9, Seiichi Yoshida). It will be observable at 14.5-15 mag in an excellent condition until February.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 5 17.94 31 40.2 1.530 2.507 171 14.6 23:42 ( 0, 87)
Dec. 22 5 11.82 30 55.7 1.534 2.503 167 14.7 23:08 ( 0, 86)
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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 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)
Dec. 15 0 15.62 -47 13.9 3.108 3.107 80 14.9 18:41 ( 0, 8)
Dec. 22 0 16.24 -47 12.3 3.152 3.065 75 14.9 18:23 ( 1, 8)
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It was recovered at 18.0 mag on Oct. 12, as bright as expected. Now it is 15.3 mag (Dec. 16, Ken-ichi Kadota), brightening rapidly as expected. It appeared in the evening sky also in the Northern Hemisphere. It will reach to 14.5 mag from December to February in the evening sky. But the altitude will be around 30 deg. Then it is observable until April when it becomes too low at 17 mag.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 22 18.71 -28 36.2 1.578 1.460 64 15.1 18:20 ( 22, 23)
Dec. 22 22 40.04 -24 48.1 1.605 1.461 63 14.9 18:23 ( 26, 26)
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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)
Dec. 15 17 28.77 -63 34.0 3.878 3.192 40 15.0 18:20 ( 32,-34)
Dec. 22 17 37.00 -64 44.9 3.866 3.196 41 15.0 5:33 (330,-32)
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It reached up to 12.6 mag and was bright visually in autumn (Oct. 5, Seiichi Yoshida). Now it is fading, but it is still bright and visible visually at 14.0 mag (Dec. 9, Seiichi Yoshida). It keeps observable in good condition for a while after this. It will be visible visually for some more time.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 0 22.44 -10 46.5 2.082 2.425 98 15.0 18:48 ( 0, 44)
Dec. 22 0 29.42 -9 44.4 2.181 2.442 93 15.1 18:27 ( 0, 45)
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It was visible visually at 14 mag from spring to autumn in 2007. Now it is not observable. 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)
Dec. 15 17 2.37 0 10.6 6.482 5.598 24 15.1 5:29 (270, 0)
Dec. 22 17 4.63 0 32.8 6.452 5.596 27 15.1 5:33 (274, 6)
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It was observed at 16 mag in 2007 spring and summer. Although it had been unobservable for a while, now it is appearing again in the Southern Hemisphere. It keeps 16 mag and observable in good condition after this 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)
Dec. 15 15 34.48 -42 58.1 3.483 2.682 30 15.2 5:29 (316,-10)
Dec. 22 15 52.94 -44 11.8 3.460 2.688 32 15.2 5:33 (319, -9)
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Now it is 15.6 mag (Nov. 24, Ken-ichi Kadota). Now it is not observable temporarily. But it will be getting higher in the morning sky after January. 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)
Dec. 15 17 20.36 3 36.3 5.153 4.298 26 15.4 5:29 (264, -2)
Dec. 22 17 25.69 2 48.0 5.096 4.247 27 15.3 5:33 (269, 3)
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Now it is 16.1 mag (Nov. 30, Ken-ichi Kadota), brightening as expected. It will reach to 13.5 mag from March to July in 2008, and will be visible visually. It keeps observable in good condition for a long time until next May.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 12 29.70 11 31.1 3.875 3.839 80 15.5 5:29 (314, 59)
Dec. 22 12 34.56 10 51.7 3.735 3.798 86 15.4 5:33 (326, 62)
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It is already bright as 14.3 mag and visible visually (Dec. 9, 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.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 5 0.80 64 8.7 5.226 6.002 138 15.6 23:24 (180, 61)
Dec. 22 4 44.38 64 12.1 5.192 5.954 137 15.5 22:40 (180, 61)
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Now it is visible visually at 15.0 mag (Dec. 8, Seiichi Yoshida). It keeps observable in good condition until it fades out in 2008 spring.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 1 54.65 45 8.1 1.165 1.964 131 15.6 20:20 (180, 80)
Dec. 22 1 58.75 44 42.7 1.220 1.978 127 15.7 19:57 (180, 80)
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It brightened after the perihelion passage, and now it reached up to 14.1 mag and became visible visually (Dec. 8, Seiichi Yoshida). It will be observable in good condition for a while. But it can be fading rapidly after this.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 2 37.22 4 4.8 1.361 2.169 134 16.1 21:02 ( 0, 59)
Dec. 22 2 38.11 5 3.7 1.435 2.187 128 16.2 20:36 ( 0, 60)
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Now it is 16.2 mag (Nov. 24, Ken-ichi Kadota). It keeps observable in the evening sky until March.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 2 56.33 -23 26.2 4.005 4.586 120 16.1 21:21 ( 0, 32)
Dec. 22 2 53.27 -22 2.8 4.084 4.601 116 16.2 20:50 ( 0, 33)
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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)
Dec. 15 9 30.88 -27 17.1 1.351 1.836 102 16.3 3:58 ( 0, 28)
Dec. 22 9 39.91 -28 51.8 1.292 1.819 105 16.2 3:40 ( 0, 26)
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It was visible visually at 14.4 mag in autumn (Oct. 6, Seiichi Yoshida). But it will be fading gradually after this.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 0 0.46 5 55.1 2.191 2.552 99 16.3 18:26 ( 0, 61)
Dec. 22 0 6.50 6 44.9 2.279 2.552 94 16.4 18:23 ( 9, 62)
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Now it is 16.8 mag (Nov. 23, Ken-ichi Kadota), brightening as expected. 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)
Dec. 15 11 57.11 4 15.3 1.934 2.090 84 16.4 5:29 (334, 57)
Dec. 22 12 7.19 3 38.8 1.872 2.106 89 16.4 5:33 (344, 58)
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It will reach to 15 mag in 2009 and 2010. Now it is 17.3 mag (Nov. 4, J. A. Henriquez). It will be observable at 16.5 mag in good condition until winter in this year.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 5 7.82 23 12.5 3.052 4.034 175 16.5 23:32 ( 0, 78)
Dec. 22 5 2.80 23 13.7 3.060 4.025 167 16.5 22:59 ( 0, 78)
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It was observed visually as bright as 13 mag from late 2005 to early 2006. Now it is fading. It is appearing in the morning sky again. It will be observable in good condition at 17 mag for a long time until June.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 14 11.99 0 43.9 7.420 6.875 53 16.7 5:29 (297, 34)
Dec. 22 14 15.27 0 23.8 7.360 6.907 59 16.7 5:33 (304, 39)
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It will reach to 15.5 mag in 2008 autumn and will be observable in good condition. In this winter, it is observable at 17 mag in good condition until March.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 6 33.37 2 14.5 3.079 3.985 153 16.9 1:02 ( 0, 57)
Dec. 22 6 18.81 2 35.1 3.019 3.951 158 16.9 0:20 ( 0, 58)
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It will be observable at 17 mag in good condition until February.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 9 28.79 23 47.2 1.720 2.424 125 17.0 3:56 ( 0, 79)
Dec. 22 9 30.36 25 11.3 1.676 2.446 131 17.0 3:31 ( 0, 80)
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It reached to 13.5 mag and became visible visually in 2005 and 2006. Now it has gone far away. But the fading has been slower than predicted, and it is still bright as 16.3 mag (Nov. 7, Ken-ichi Kadota). It will be observable in good condition until February, and will keep 16-17 mag.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 1 42.25 6 30.8 3.658 4.281 123 17.0 20:07 ( 0, 62)
Dec. 22 1 41.68 6 41.4 3.767 4.295 116 17.1 19:39 ( 0, 62)
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It will pass 0.85 A.U. from the sun in late June in 2008, and it is expected to reach to 6 mag. In the Northern Hemipshere, it keeps observable in good condition for a long time after this, while the comet is brightening gradually. The comet will be 14 mag in February and become visible visually. Then it is observable until around May 25, when the comet will be 7.5 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 7 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)
Dec. 15 12 8.89 -2 51.8 3.076 3.052 79 17.3 5:29 (334, 49)
Dec. 22 12 15.03 -3 46.8 2.893 2.968 84 17.0 5:33 (344, 50)
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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)
Dec. 15 9 3.81 27 5.9 3.628 4.341 131 17.2 3:32 ( 0, 82)
Dec. 22 9 1.66 27 33.8 3.540 4.328 138 17.2 3:02 ( 0, 83)
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Now it is 17.5 mag (Nov. 25, 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)
Dec. 15 2 30.92 18 25.6 3.668 4.454 138 17.3 20:56 ( 0, 73)
Dec. 22 2 29.79 17 19.3 3.783 4.490 130 17.4 20:27 ( 0, 72)
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It will be observable at 17.5 mag in good condition until May.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 8 35.76 26 8.8 3.480 4.256 137 17.5 3:04 ( 0, 81)
Dec. 22 8 34.24 27 21.8 3.398 4.239 144 17.4 2:35 ( 0, 82)
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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 2008 July.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 14 30.21 15 57.5 8.522 8.050 58 17.5 5:29 (279, 40)
Dec. 22 14 32.37 15 45.1 8.459 8.073 63 17.5 5:33 (284, 46)
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Now it is observable in good condition at 17.5 mag. But it will be fainter than 18 mag in January.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 2 50.58 29 44.8 1.814 2.677 144 17.6 21:15 ( 0, 85)
Dec. 22 2 49.18 29 34.6 1.869 2.678 137 17.6 20:46 ( 0, 85)
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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)
Dec. 15 12 54.56 15 22.2 4.890 4.766 77 17.7 5:29 (301, 58)
Dec. 22 12 55.61 14 53.7 4.740 4.727 83 17.6 5:33 (312, 63)
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Now it is 18.3 mag (Dec. 14, Ken-ichi Kadota). It will be observable in good condition for a hile until spring. It will reach to 16.5 mag in March.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 10 45.91 24 38.3 2.205 2.683 108 17.8 5:13 ( 0, 80)
Dec. 22 10 51.63 25 14.0 2.109 2.666 114 17.6 4:51 ( 0, 80)
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Now it is 17.8 mag (Nov. 18, Ken-ichi Kadota). It was observed at 17.5 mag in early 2007. It will be observable at 17.5 mag again in this winter.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 11 11.43 -2 17.2 8.752 8.854 92 17.7 5:29 (356, 53)
Dec. 22 11 12.35 -2 12.9 8.641 8.859 99 17.7 5:12 ( 0, 53)
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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)
Dec. 15 2 39.74 4 54.6 4.169 4.921 135 17.8 21:04 ( 0, 60)
Dec. 22 2 37.44 5 5.4 4.259 4.930 128 17.8 20:35 ( 0, 60)
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Now it is 18.4 mag (Dec. 15, Ken-ichi Kadota). It will reach to 16 mag from February to April, and will be observable in good condition.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 11 4.50 56 28.0 1.382 1.978 112 18.0 5:29 (181, 69)
Dec. 22 11 15.92 57 8.0 1.301 1.936 115 17.8 5:16 (180, 68)
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Now it is 17.5 mag (Nov. 7, Ken-ichi Kadota). Now it is at maximum of brightness, but it keeps observable in good condition for a while after this.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 3 17.91 -4 34.1 3.303 4.087 137 17.8 21:42 ( 0, 50)
Dec. 22 3 15.52 -4 5.1 3.367 4.088 131 17.9 21:13 ( 0, 51)
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It was observed at 16.5-17 mag in last winter. It will be observable in good condition also in this winter. It should be 16 mag by calculation. However, it was so faint as 18.5 mag in autumn, much fainter than expected. It was observed so faint around the perihelion passage in the previous apparition at the discovery. So maybe it suddenly faded out before the perihelion passage again.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Dec. 15 8 3.31 24 3.0 3.427 4.266 144 18.5 2:31 ( 0, 79)
Dec. 22 8 0.61 24 33.3 3.367 4.262 152 18.5 2:01 ( 0, 80)
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