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Now it is very bright as 7.3 mag (Sept. 19, Willian Souza). 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.22 6 30.07 13 16.9 0.413 1.027 81 7.1 4:25 (216, 33)
Sept.29 6 47.41 2 45.2 0.444 1.048 83 7.3 4:15 (224, 42)
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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. 10, 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.22 14 24.63 -60 30.9 2.451 2.265 67 9.8 19:20 ( 36, 37)
Sept.29 14 26.32 -61 32.3 2.540 2.284 63 9.9 19:26 ( 34, 34)
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Now it is 11.5 mag (Sept. 17, Seiichi Yoshida). 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.22 5 33.80 10 26.4 1.295 1.708 95 10.9 4:25 (202, 42)
Sept.29 5 50.98 11 35.9 1.220 1.678 97 10.6 4:15 (202, 41)
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Now it is bright as 12.4 mag (Sept. 18, Chris Wyatt). 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.22 1 49.15 -23 32.0 0.557 1.491 144 12.2 1:47 (180, 78)
Sept.29 1 52.90 -25 36.1 0.496 1.434 144 11.5 1:24 (180, 80)
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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.22 11 53.33 13 26.3 2.007 1.053 12 11.7 4:25 (271,-25)
Sept.29 12 7.77 14 55.0 2.116 1.198 17 12.4 4:15 (269,-25)
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Now it is 12.1 mag (Sept. 5, 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.22 11 59.01 48 22.4 3.545 2.967 47 11.9 19:20 (127,-39)
Sept.29 12 17.88 47 30.0 3.551 3.002 49 12.0 4:15 (234,-40)
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Outburst occured on Aug. 14. Now it is very bright as 12.2 mag (Sept. 19, Juan Jose Gonzalez). 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.22 0 26.04 28 25.7 0.528 1.485 150 12.1 0:25 (180, 27)
Sept.29 0 27.97 30 48.5 0.498 1.458 151 12.0 23:55 (180, 24)
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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.22 13 2.76 -29 25.3 2.135 1.419 34 12.2 19:20 ( 63, 13)
Sept.29 13 24.84 -28 41.8 2.285 1.512 30 12.6 19:26 ( 62, 10)
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Now it is 12.0 mag (Sept. 16, Paul Camilleri). 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.22 8 59.33 14 19.3 3.364 2.757 45 12.3 4:25 (245, 9)
Sept.29 9 0.55 12 23.0 3.283 2.776 51 12.3 4:15 (244, 13)
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Now it is bright as 12.8 mag (Sept. 18, Paul Camilleri). 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.22 22 28.44 -28 46.9 1.125 2.030 144 13.0 22:23 (180, 84)
Sept.29 22 28.13 -28 43.7 1.175 2.040 139 13.2 21:56 (180, 84)
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Outburst occured on Sept. 20. Now it is bright as 12.9 mag (Sept. 20, Jean-Francois Soulier).
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 22 56.05 0 17.4 4.796 5.772 165 13.1 22:51 (180, 55)
Sept.29 22 53.21 0 1.9 4.830 5.772 158 13.1 22:20 (180, 55)
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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 12.9 mag (Sept. 8, Chris Wyatt). It will be unobservable in October.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 15 6.64 -7 42.2 1.976 1.510 48 13.3 19:20 ( 99, 25)
Sept.29 15 7.13 -7 17.4 2.159 1.563 41 13.6 19:26 ( 94, 18)
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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.22 15 7.29 -5 51.4 2.463 1.947 48 13.9 19:20 (101, 24)
Sept.29 15 18.68 -4 32.3 2.486 1.906 44 13.8 19:26 ( 98, 19)
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Now it is 14.3 mag (Sept. 13, Catalina Sky Survey). 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.22 21 21.68 -7 10.2 1.656 2.518 141 14.1 21:17 (180, 62)
Sept.29 21 20.01 -7 44.0 1.686 2.488 133 14.0 20:48 (180, 63)
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Now it is 14.0 mag (Sept. 6, 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.22 16 18.25 13 41.3 3.718 3.440 66 14.2 19:20 (129, 24)
Sept.29 16 19.30 11 22.5 3.793 3.419 60 14.2 19:26 (121, 21)
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Now it is 14.3 mag (Aug. 17, Ken-ichi Kadota). It will be observable at 13-14 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.22 11 53.18 35 55.9 4.961 4.183 35 14.3 4:25 (248,-35)
Sept.29 11 54.99 35 27.9 4.953 4.211 38 14.3 4:15 (247,-32)
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It brightens up to 13 mag in October. But it is not observable at all.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 12 39.73 -6 12.6 2.045 1.090 12 15.7 19:20 ( 79, -5)
Sept.29 13 8.29 -7 28.0 2.035 1.083 13 14.6 19:26 ( 77, -5)
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Now it is 14.2 mag (Sept. 17, Seiichi Yoshida). 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.22 5 49.51 54 19.6 1.697 1.978 90 14.7 4:25 (192, -1)
Sept.29 6 11.61 57 35.9 1.640 1.967 93 14.7 4:15 (192, -4)
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Now it is 14.5 mag (Aug. 16, P. Camilleri, H. Williams). 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.22 13 58.48 -66 4.7 4.319 4.088 70 15.0 19:20 ( 29, 35)
Sept.29 14 16.61 -66 33.1 4.349 4.072 67 15.0 19:26 ( 28, 34)
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Now it is 13.8 mag (Sept. 18, Paul Camilleri). 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.22 2 52.13 -46 28.5 4.373 4.952 120 15.2 2:50 ( 0, 79)
Sept.29 2 44.57 -46 52.8 4.306 4.906 121 15.1 2:15 ( 0, 78)
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It brightened up to 12 mag from spring to summer. Now it is fading. But it is bright as 14.1 mag still now (Sept. 7, Thomas Lehmann).
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 23 5.72 6 3.4 1.099 2.087 166 15.4 23:00 (180, 49)
Sept.29 23 0.96 5 44.6 1.157 2.126 159 15.7 22:28 (180, 49)
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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 16.6 mag (Sept. 3, Slooh.com Chile Observatory, La Dehesa). 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.22 1 44.84 -54 28.2 4.860 5.453 121 16.1 1:43 ( 0, 71)
Sept.29 1 38.32 -54 44.1 4.933 5.514 120 16.1 1:09 ( 0, 70)
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Now it is 16.2 mag (Sept. 16, Mt. Lemmon Survey). It is observable 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.22 22 59.18 -20 7.0 2.391 3.333 156 16.2 22:54 (180, 75)
Sept.29 22 55.12 -20 12.0 2.447 3.348 149 16.2 22:22 (180, 75)
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Now it is 17.3 mag (Sept. 14, A. Diepvens). 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.22 8 26.23 30 16.1 2.751 2.373 57 16.5 4:25 (228, 4)
Sept.29 8 41.25 29 59.8 2.660 2.350 61 16.3 4:15 (228, 4)
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It will brighten up to 15 mag in winter. It is observable in excellent condition 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.22 10 57.06 37 9.8 4.167 3.445 39 16.5 4:25 (241,-25)
Sept.29 11 0.82 37 52.2 4.073 3.426 44 16.4 4:15 (239,-23)
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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 16.9 mag (Sept. 16, ATLAS-HKO, Haleakala). 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.22 0 32.13 -11 17.4 1.055 2.043 165 16.4 0:31 (180, 66)
Sept.29 0 22.18 -10 26.4 1.116 2.105 167 16.9 23:49 (180, 65)
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Now it is 16.7 mag (Sept. 19, ATLAS-MLO, Mauna Loa). 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.22 4 0.90 -4 45.8 5.974 6.513 118 16.5 3:59 (180, 60)
Sept.29 3 59.28 -5 0.1 5.830 6.455 124 16.4 3:30 (180, 60)
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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.22 2 48.06 49 56.8 1.393 2.059 117 16.5 2:47 (180, 5)
Sept.29 2 37.69 51 48.5 1.401 2.118 122 16.5 2:09 (180, 3)
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It brightened up to 14.7 mag in early 2018 (Jan. 25, Catalina Sky Survey). Now it is fading slowly. Now it is 16.5 mag (Sept. 6, D. Buczynski). 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.22 8 19.89 54 17.0 6.056 5.780 69 16.5 4:25 (211,-12)
Sept.29 8 22.28 55 22.8 5.975 5.800 75 16.5 4:15 (208,-12)
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Now it is 16.4 mag (Sept. 18, ATLAS-MLO, Mauna Loa). 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.22 23 43.73 -35 30.1 3.987 4.843 144 16.8 23:38 ( 0, 89)
Sept.29 23 33.43 -36 43.9 4.064 4.870 139 16.9 23:00 ( 0, 88)
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Now it is 16.9 mag (Sept. 12, D. Buczynski). It stays 16-17 mag for a long time until 2020. It is observable in good condition 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.22 10 18.57 67 21.1 8.806 8.497 68 16.9 4:25 (207,-31)
Sept.29 10 28.68 67 21.3 8.744 8.492 72 16.9 4:15 (207,-30)
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Now it is 16.5 mag (Sept. 17, J. Nicolas, C. Rinner, F. Kugel, A. Klotz). 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.22 21 21.44 -6 53.2 1.196 2.076 141 16.9 21:17 (180, 62)
Sept.29 21 22.01 -7 14.3 1.223 2.053 134 17.0 20:50 (180, 62)
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Asteroid, but it brightened rapidly. Now it is 16.8 mag (Aug. 16, Slooh.com Chile Observatory, La Dehesa).
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 23 13.60 -46 5.4 6.118 6.849 133 17.0 23:08 ( 0, 79)
Sept.29 23 4.49 -46 16.5 6.161 6.832 128 17.0 22:31 ( 0, 79)
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Now it is 17.1 mag (Sept. 16, Ken-ichi Kadota). It is observable at 16.5 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.22 7 16.33 29 13.8 2.465 2.359 72 17.1 4:25 (217, 14)
Sept.29 7 28.74 28 49.3 2.390 2.361 76 17.0 4:15 (217, 15)
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First return of a new periodic comet which brightened up to 16.5 mag in 2005. Now it is 17.3 mag (Sept. 15, A. Martin, K. Kleemann-Boeker). 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.22 1 58.25 35 43.9 1.243 2.069 133 17.1 1:57 (180, 19)
Sept.29 1 58.95 35 43.8 1.206 2.072 139 17.1 1:30 (180, 19)
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It brightened rapidly up to 11.1 mag (July 13, Chris Wyatt). Now it is fading. It has already faded down to 16.8 mag (Sept. 15, CAO, San Pedro de Atacama). It will be fainter than 18 mag in October.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 0 20.46 -26 9.3 0.566 1.531 153 17.1 0:20 (180, 81)
Sept.29 0 5.84 -23 55.7 0.644 1.604 153 17.4 23:32 (180, 79)
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It brightened very rapidly up to 13.8 mag in last August (Aug. 22, 2017, Kunihiro Shima). Now it is 16.8 mag (Aug. 18, Slooh.com Canary Islands Observatory). In the Northern Hemisphere, it stays observable in excellent condition after this. It will be observable also in the Southern Hemisphere in December, but it stays low.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 9 3.41 28 55.5 2.875 2.356 49 17.2 4:25 (235, -1)
Sept.29 9 17.67 28 51.3 2.831 2.378 53 17.3 4:15 (235, -1)
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Now it is 16.8 mag (Sept. 14, A. Diepvens). 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.22 22 56.71 77 16.3 7.365 7.634 101 17.3 22:51 (180,-22)
Sept.29 22 50.15 76 49.6 7.350 7.660 104 17.3 22:17 (180,-22)
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First return of a new periodic comet which brightened up to 17.5 mag in 2010. Now it is 18.1 mag (Sept. 9, Mt. Lemmon Survey). 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.22 5 18.52 23 45.6 1.557 1.969 98 17.4 4:25 (193, 30)
Sept.29 5 29.96 24 41.2 1.487 1.963 102 17.3 4:15 (192, 29)
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Now it is 18.0 mag (Sept. 10, iTelescope Observatory, Mayhill). It is observable at 17 mag in good condition in winter. It locates low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 9 1.78 21 55.6 2.537 1.998 47 17.4 4:25 (240, 4)
Sept.29 9 16.86 21 35.0 2.512 2.032 50 17.3 4:15 (240, 4)
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Now it is 16.8 mag (Sept. 11, D. Buczynski). 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.22 0 59.75 30 7.3 2.765 3.639 145 17.4 0:59 (180, 25)
Sept.29 0 55.54 30 0.7 2.774 3.683 150 17.4 0:27 (180, 25)
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It brightened very rapidly. Now it is 17.3 mag (Sept. 16, Mt. Lemmon Survey). It will be fading after October.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 0 7.01 -19 1.8 0.782 1.763 161 17.5 0:06 (180, 74)
Sept.29 0 2.46 -18 40.1 0.787 1.759 158 17.5 23:29 (180, 74)
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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.22 5 47.83 10 26.5 7.884 7.978 91 17.5 4:25 (207, 41)
Sept.29 5 45.92 10 0.6 7.766 7.982 98 17.5 4:15 (201, 43)
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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.22 2 6.00 -13 47.5 1.294 2.193 145 17.6 2:04 (180, 69)
Sept.29 2 2.67 -13 49.2 1.266 2.192 150 17.5 1:34 (180, 69)
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Now it is 17.3 mag (Sept. 18, Catalina Sky Survey). It will brighten very rapidly after this. It will brighten up to 14.5 mag from January to February, and it is expected to be observable in excellent condition.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 7 31.18 22 14.4 1.924 1.801 67 17.9 4:25 (224, 18)
Sept.29 7 49.94 21 17.8 1.843 1.773 70 17.6 4:15 (225, 19)
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Now it is 17.6 mag (Sept. 13, iTelescope Observatory, Mayhill). 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.22 6 51.09 11 11.7 2.902 2.835 76 17.8 4:25 (223, 33)
Sept.29 6 58.85 10 26.1 2.825 2.845 80 17.8 4:15 (221, 35)
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Now it is 17.8 mag (Aug. 23, iTelescope Observatory, Siding Spring). It stays 17 mag in 2018.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 5 13.63 3 48.9 7.367 7.611 100 17.8 4:25 (198, 50)
Sept.29 5 14.09 3 30.9 7.297 7.645 106 17.8 4:15 (192, 51)
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Now it is 19.7 mag (Sept. 18, R. Fichtl). It will brighten rapidly. It is expected to be observable at 15.5 mag in good condition in winter.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Sept.22 4 37.86 -6 15.3 1.477 2.042 109 18.1 4:25 (185, 61)
Sept.29 4 45.07 -6 38.7 1.393 2.013 113 17.8 4:15 (180, 62)
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