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Now it is very bright as 7.3 mag (Sept. 8, Maik Meyer). It stays bright as 7 mag until September. In the Northern Hemisphere, it will be observable in excellent condition. It will be getting higher gradually after this also in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 5 39.31 37 7.2 0.393 1.013 79 6.8 4:46 (201, 14)
Sept.15 6 7.99 25 1.9 0.395 1.015 80 6.9 4:36 (209, 24)
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It brightened up to 7.7 mag in June (June 19, Juan Jose Gonzalez). Now it is fading. But it is still bright as 9.8 mag (Sept. 7, Chris Wyatt). It stays bright as 9-10 mag for a while. In the Southern Hemisphere, it stays observable in good condition for a long time until the comet will fade out. In the Northern Hemisphere, it is not observable for a long time until autumn in 2019 when the comet fades out down to 16 mag.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 14 25.98 -58 53.4 2.253 2.235 76 9.5 19:09 ( 39, 46)
Sept.15 14 24.43 -59 38.0 2.355 2.249 71 9.6 19:14 ( 38, 41)
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It brightened rapidly in outburst up to 6.9 mag (July 19, Maik Meyer). Then it faded down to 9.3 mag (Aug. 2, Katsumi Yoshimoto). It approached to Sun down to 0.2 a.u. in August, and it was expected to brighten up to 3 mag. However, it must have been already disintegrated. Now it is not observable. In the Northern Hemisphere, it will appear in the morning sky in late October. But it will be too faint to observe.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 11 18.97 9 39.6 1.736 0.738 5 9.9 19:09 ( 90,-17)
Sept.15 11 37.29 11 43.7 1.882 0.900 8 10.9 19:14 ( 89,-22)
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Now it is 12.7 mag (Sept. 5, Paul Camilleri). It will brighten rapidly, and it is expected to brighten up to 9 mag from autumn to winter. In the Northern Hemisphere, it stays observable in good condition for a long time until it fades out. In the Southern Hemispehre, it is observable in good condition until autumn, but it will be low in winter.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 4 59.88 8 18.1 1.459 1.779 90 11.6 4:46 (203, 44)
Sept.15 5 16.76 9 20.9 1.374 1.742 92 11.2 4:36 (203, 43)
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It brightened up to 8.7 mag in July (July 18, Marco Goiato). Now it is fading. But it is still bright as 12.3 mag (Aug. 29, Chris Wyatt). In the Southern Hemisphere, it is observable until September, but it locates in extremely low. In the Northern Hemisphere, it is not observable until late December.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 12 7.71 -30 38.1 1.836 1.238 39 11.2 19:09 ( 63, 15)
Sept.15 12 37.34 -30 5.8 1.985 1.327 36 11.7 19:14 ( 63, 15)
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Now it is 11.9 mag (Aug. 15, Thomas Lehmann). It will be fading slowly after this. In the Northern Hemisphere, it stays low until October. But it will be observable in good condition after that. In the Southern Hemisphere, it is not observable until summer in 2019.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 11 19.25 50 0.3 3.536 2.900 44 11.8 19:09 (131,-35)
Sept.15 11 39.46 49 12.9 3.540 2.933 46 11.9 19:14 (129,-37)
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It brightened in outburst on Aug. 14 up to 13.6 mag (Aug. 14, Piotr Guzik). It is bright as 13.6 mag still now (Sept. 5, Paul Camilleri). It is observable in excellent condition in the Northern Hemisphere. It stays low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 0 21.07 23 9.9 0.610 1.549 145 12.3 1:15 (180, 32)
Sept.15 0 23.84 25 51.0 0.565 1.516 148 12.0 0:50 (180, 29)
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Now it is 11.7 mag (June 12, Juan Jose Gonzalez). It is appearing in the morning sky. It stays 12 mag for a long time until spring.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 8 55.10 18 3.9 3.501 2.724 33 12.3 4:46 (247, 1)
Sept.15 8 57.49 16 12.8 3.437 2.739 39 12.3 4:36 (246, 5)
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It approached to Earth down to 0.3 a.u., and brightened up to 8.3 mag in July (July 22, Juan Jose Gonzalez). Now it is fading. But it is still bright as 12.4 mag (Sept. 7, Chris Wyatt). It will go away from Earth after this, and will fade out rapidly. It will be getting lower after this. It will be unobservable in October.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 15 8.64 -8 57.7 1.568 1.419 62 12.5 19:09 (109, 40)
Sept.15 15 7.01 -8 14.3 1.779 1.462 55 12.9 19:14 (104, 32)
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Now it is bright as 12.9 mag (Sept. 7, Chris Wyatt). It stays at 12-13 mag from summer to autumn. It is observable in excellent condition in the Southern Hemisphere. It locates somewhat low in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 22 32.27 -28 0.4 1.051 2.016 156 12.8 23:22 (180, 83)
Sept.15 22 29.90 -28 32.7 1.083 2.022 150 12.9 22:52 (180, 83)
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Now it is bright as 13.2 mag (Sept. 7, Michael Mattiazzo). It will approach to Earth down to 0.08 a.u. in December, and it is expected to brighten up to 3 mag. In the Northern Hemisphere, it stays observable in excellent condition. In the Southern Hemisphere, it is observable in good condition until mid December when it brightens up to 3 mag. But it becomes unobservable after that.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 1 38.71 -19 47.0 0.700 1.609 140 13.5 2:32 (180, 75)
Sept.15 1 44.38 -21 34.4 0.625 1.550 142 12.9 2:10 (180, 76)
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Now it is fainter than 14.8 mag (Sept. 5, Paul Camilleri). However, Juan Jose Gonzalez reported it was 10.8 mag with a coma of 5 arcmin on Sept. 1.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 23 2.27 0 48.1 4.771 5.773 173 13.1 23:52 (180, 54)
Sept.15 22 59.11 0 33.1 4.776 5.773 171 13.1 23:21 (180, 54)
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Now it is 13.9 mag (Sept. 3, Paul Camilleri). It stays at 14-15 mag for a long time from summer to winter. In the Southern Hemisphere, it will be getting lower rapidly after this, then it becomes unobservable after October. In the Northern Hemisphere, it stays observable for a long time until it fades out. But it stays extremely low.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 14 46.24 -8 37.5 2.401 2.037 57 14.0 19:09 (106, 35)
Sept.15 14 56.46 -7 12.6 2.435 1.991 52 13.9 19:14 (103, 30)
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Now it is 14.0 mag (Sept. 3, Paul Camilleri). It stays 13-14 mag until summer in 2019. In the Northern Hemisphere, it stays observable in good condition for a while. It locates somewhat low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 16 18.59 18 38.8 3.568 3.486 77 14.2 19:09 (147, 29)
Sept.15 16 17.98 16 6.6 3.642 3.463 71 14.2 19:14 (138, 27)
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Now it is 14.3 mag (Aug. 17, Ken-ichi Kadota). It will be observable at 12-13 mag for a long time from 2017 to 2018. In the Southern Hemisphere, it will be hardly observable after this. It becomes extremely low in September also in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 11 49.54 37 8.6 4.940 4.130 32 14.2 19:09 (119,-25)
Sept.15 11 51.34 36 29.5 4.956 4.156 33 14.3 19:14 (115,-31)
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Now it is 14.9 mag (Aug. 8, Toshihiko Ikemura, Hirohisa Sato). It stays at 13 mag for a long time from winter to autumn in 2019. It stays observable in good condition until winter when the comet brightens up to 13 mag.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 21 28.50 -5 53.4 1.626 2.579 156 14.4 22:18 (180, 61)
Sept.15 21 24.57 -6 32.8 1.636 2.548 148 14.3 21:47 (180, 62)
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Now it is bright as 13.8 mag (Aug. 22, Thomas Lehmann). It stays observable in good condition for a long time after this. But it will be fading gradually.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 23 18.12 6 29.2 1.017 2.012 167 14.8 0:12 (180, 48)
Sept.15 23 11.56 6 19.3 1.052 2.049 169 15.1 23:33 (180, 49)
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Now it is 16.3 mag (Jan. 11, ATLAS-HKO, Haleakala). It will brighten up to 14 mag in winter. It will be observable in excellent condition in the Northern Hemisphere. It will be unobservable soon in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 5 10.87 47 48.2 1.832 2.007 84 14.9 4:46 (193, 5)
Sept.15 5 29.38 51 2.8 1.761 1.991 87 14.8 4:36 (192, 2)
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Now it is 15.1 mag (June 18, Martin Masek). It stays 15 mag from 2018 to 2019, and it will be observable for a long time in the Southern Hemisphere. In the Northern Hemisphere, it will never be observable again.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 13 26.18 -65 12.3 4.256 4.124 75 15.0 19:09 ( 31, 39)
Sept.15 13 41.67 -65 37.5 4.288 4.106 72 15.0 19:14 ( 30, 37)
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Now it is 16.4 mag (Aug. 17, Ken-ichi Kadota). It is observable at 15-16 mag in 2018, in good condition in the Southern Hemisphere. It locates somewhat low in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 23 8.64 -19 35.6 2.317 3.304 166 15.3 0:03 (180, 74)
Sept.15 23 3.76 -19 54.7 2.347 3.319 162 15.4 23:26 (180, 75)
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The condition is worst in this apparition. It must have brightened up to 14.5 mag from June to August, but it is not observable at all.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 9 44.08 15 55.0 2.436 1.550 22 15.3 4:46 (256, -7)
Sept.15 10 4.53 15 6.5 2.444 1.581 24 15.5 4:36 (257, -7)
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It brightened rapidly, and brightened up to 10.2 mag from May to June (May 22, Chris Wyatt). Now it is fading. It has already faded down to 13.0 mag (Aug. 20, Thomas Lehmann). It stays observable in good condition for a long time after this. But it will be fainter than 18 mag in October.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 0 53.43 -12 48.0 0.970 1.921 152 15.4 1:47 (180, 68)
Sept.15 0 42.75 -12 4.7 1.006 1.982 159 15.9 1:09 (180, 67)
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Now it is 15.9 mag (Aug. 22, A. Maury, J.-B. de Vanssay, J.-G. Bosch). It will brighten up to 12 mag in autumn in 2019. It stays observable in good condition for a while in the Southern Hemisphere. In the Northern Hemisphere, it stays extremely low for a long time.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 3 3.90 -45 22.5 4.533 5.044 115 15.8 3:57 ( 0, 80)
Sept.15 2 58.59 -45 57.7 4.448 4.997 117 15.7 3:24 ( 0, 79)
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Now it is 16.3 mag (Aug. 18, Ken-ichi Kadota). Fading now. It stays observable in good condition for a long time after this in the Southern Hemisphere. It stays low in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 0 4.21 -32 24.4 3.891 4.791 150 15.8 0:58 (180, 87)
Sept.15 23 54.08 -34 3.1 3.929 4.817 148 15.8 0:21 (180, 89)
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It brightened up to 7.1 mag from May to June in 2017 (June 21, Juan Jose Gonzalez). Now it is fading. It has already faded down to 15.0 mag (July 15, Thomas Lehmann). In the Southern Hemisphere, it stays observable for a long time after this. It will never be observable again in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 1 56.32 -53 30.0 4.740 5.331 121 15.9 2:50 ( 0, 72)
Sept.15 1 50.91 -54 3.2 4.796 5.392 121 16.0 2:17 ( 0, 71)
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Now it is 17.0 mag (July 15, Toshihiko Ikemura, Hirohisa Sato). It brightens up to 16 mag from August to October. But it stays low.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 14 25.49 -6 8.3 1.932 1.524 51 16.0 19:09 (104, 30)
Sept.15 14 45.96 -7 59.5 1.967 1.531 50 16.1 19:14 (100, 28)
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Now it is 16.2 mag (June 17, Jean-Francois Soulier). It stays 16 mag for a while. In the Northern Hemisphere, it stays observable in good condition after this until it fades out. It will be unobservable soon in the Southern Hemisphere. Its cometary activity was observed on Mar. 26 (M. Mommert, D. Polishook, N. Moskovitz).
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 3 0.11 45 14.5 1.394 1.942 106 16.5 3:54 (180, 10)
Sept.15 2 55.54 47 44.0 1.391 2.000 112 16.5 3:22 (180, 7)
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It will be observable at 16 mag in good condition from autumn to winter. It locates somewhat low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 6 49.66 29 53.2 2.613 2.360 64 16.5 4:46 (218, 13)
Sept.15 7 3.29 29 35.2 2.539 2.359 68 16.5 4:36 (218, 14)
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It brightened up to 14.7 mag in early 2018 (Jan. 25, Catalina Sky Survey). Now it is fading slowly. In the Northern Hemisphere, it stays observable in good condition for a long time until the comet fades out. It is never observable again in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 8 13.58 52 21.0 6.208 5.741 58 16.5 4:46 (215,-14)
Sept.15 8 16.95 53 16.5 6.134 5.760 63 16.5 4:36 (213,-13)
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It will brighten up to 13-14 mag in winter, and it will be observable in excellent condition.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 7 55.91 30 40.9 2.929 2.420 50 16.7 4:46 (229, 3)
Sept.15 8 11.10 30 30.0 2.841 2.396 54 16.6 4:36 (229, 3)
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It brightened rapidly up to 11.1 mag (July 13, Chris Wyatt). Now it is fading. But it is still bright as 13.9 mag (Aug. 25, Ken-ichi Kadota). In the Southern Hemisphere, it stays observable in good condition all through this apparition. It became observable also in the Northern Hemisphere, but it stays low.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 1 3.49 -30 30.9 0.439 1.383 142 16.6 1:58 (180, 85)
Sept.15 0 39.56 -28 23.3 0.497 1.458 149 16.8 1:07 (180, 83)
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Now it is 16.8 mag (Aug. 8, Toshihiko Ikemura, Hirohisa Sato). It is expected to brighten up to 7-8 mag in 2020. In 2018, it will be observable at 15-16 mag in good condition from autum to winter.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 4 2.50 -4 19.0 6.280 6.628 105 16.7 4:46 (185, 59)
Sept.15 4 1.97 -4 32.0 6.124 6.571 112 16.6 4:28 (180, 59)
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Now it is 16.0 mag (Aug. 12, Gabor Santa). It will be observable at 16.5 mag in good condition from August to September.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 21 24.74 -6 1.0 1.169 2.125 155 16.7 22:15 (180, 61)
Sept.15 21 22.41 -6 28.2 1.178 2.100 148 16.8 21:45 (180, 61)
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Now it is 16.0 mag (Apr. 6, Sandor Szabo). It stays 16-17 mag for a long time until 2020. It is observable in good conditioin in the Northern Hemisphere. It is not observable at all in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 9 57.57 67 27.3 8.922 8.506 62 16.9 4:46 (207,-32)
Sept.15 10 8.20 67 23.1 8.866 8.501 65 16.9 4:36 (207,-32)
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Now it is around the apheilon. But it brightened up to 15.8 mag in outburst (July 21, Hidetaka Sato). Now it is getting diffused. But it is bright as 16.2 mag still now (Aug. 18, Toshihiko Ikemura, Hirohisa Sato).
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 20 57.79 -14 2.6 3.753 4.636 147 16.9 21:48 (180, 69)
Sept.15 20 55.32 -14 18.3 3.817 4.635 140 17.2 21:18 (180, 69)
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Now it is 17.3 mag (Feb. 20, Toshihiko Ikemura, Hirohisa Sato). It stays 17 mag in 2018.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 5 11.44 4 23.0 7.512 7.544 87 17.2 4:46 (209, 46)
Sept.15 5 12.74 4 6.3 7.439 7.577 94 17.2 4:36 (204, 48)
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First return of a new periodic comet which brightened up to 16.5 mag in 2005. Now it is 19.1 mag (June 14, E. Schwab, D. Abreu). It will be observable at 17 mag in good condition in autumn. It locates low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 1 52.71 34 53.7 1.337 2.069 123 17.3 2:46 (180, 20)
Sept.15 1 56.18 35 26.7 1.287 2.068 128 17.2 2:22 (180, 19)
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Now it is 16.9 mag (Aug. 19, Toshihiko Ikemura, Hirohisa Sato). It will be fading gradually after this, and it will be fainter than 18 mag in winter. In the Northern Hemisphere, it stays observable in good condition for a long time. In the Southern Hemisphere, it will never be observable again.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 23 12.14 77 48.1 7.404 7.581 96 17.2 0:06 (180,-23)
Sept.15 23 4.16 77 35.9 7.383 7.607 99 17.2 23:25 (180,-23)
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Now it is 17.8 mag (Aug. 8, Toshihiko Ikemura, Hirohisa Sato). It was observed at 16 mag from summer to autumn in 2017. It will be observable at 17 mag in good condition also in 2018. It locates somewhat low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 1 6.92 29 53.5 2.779 3.552 133 17.3 2:01 (180, 25)
Sept.15 1 3.61 30 5.0 2.767 3.595 139 17.3 1:30 (180, 25)
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First return of a new periodic comet which brightened up to 17.5 mag in 2010. Now it is 19.0 mag (Aug. 10, Erwin Schwab). It is expected to brighten up to 16.5 mag from November to December. It is observable in excellent condition in the Northern Hemisphere. It locates low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 4 53.59 21 53.0 1.704 1.986 90 17.6 4:46 (197, 31)
Sept.15 5 6.35 22 49.8 1.629 1.977 94 17.5 4:36 (195, 31)
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It was observed at 17 mag in last winter. It will be observable in good condition at 17.5 mag also in this winter.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 5 50.27 11 15.6 8.121 7.968 77 17.6 4:46 (217, 36)
Sept.15 5 49.27 10 51.5 8.003 7.973 84 17.5 4:36 (212, 38)
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Return of a new periodic comet which brightened up to 17 mag in 2001. It was missed at the last return in 2010. Now it is 19.1 mag (Sept. 8, E. Schwab, D. Abreu). It was predicted to brighten up to 17.5 mag from September to November. But actually, it is a bit fainter than predicted.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 2 9.00 -13 20.1 1.378 2.201 134 17.8 3:02 (180, 68)
Sept.15 2 8.63 -13 31.7 1.332 2.196 139 17.7 2:34 (180, 68)
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First return of a new periodic comet which brightened up to 17 mag in 2008. It was predicted to brighten up to 18 mag in autumn. But actually, it is much fainter than predicted, fainter than 21.5 mag (June 22, Erwin Schwab).
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 23 5.42 -0 50.6 2.813 3.818 174 17.8 23:55 (180, 56)
Sept.15 23 1.04 -1 5.2 2.818 3.817 172 17.8 23:23 (180, 56)
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Now it is 17.7 mag (Aug. 8, Toshihiko Ikemura, Hirohisa Sato). It is expected to be observable at 5-6 mag for a long time from 2022 to 2023. It will be observable in good condition for a long time in the Southern Hemisphere. In the Northern Hemisphere, it is not observable at the highlight from 2022 summer to 2023 summer.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 17 8.03 57 40.0 13.307 13.265 85 17.8 19:09 (171, -4)
Sept.15 17 8.10 57 5.1 13.283 13.221 84 17.8 19:14 (166, -5)
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It was observed at 18 mag in last winter. It will be observable in good condition at 17.5 mag also in this winter.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept. 8 6 33.56 12 34.9 3.052 2.818 67 17.9 4:46 (226, 29)
Sept.15 6 42.64 11 54.8 2.978 2.826 71 17.9 4:36 (225, 31)
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