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Now it is very bright as 6.9 mag (Nov. 21, Seiichi Yoshida). It will approach to Sun down to 0.4 a.u. on Dec. 13, and will brighten up to 6 mag. It will be unobservable soon.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 12 58.81 -20 15.9 1.041 0.683 39 7.4 5:12 (307, 13)
Nov. 28 14 3.44 -22 50.0 1.081 0.555 30 6.6 5:17 (304, 6)
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Now it is very bright as 7.6 mag (Nov. 22, Carlos Labordena). In the Northern Hemisphere, it stays observable in excellent condition for a long time. In the Southern Hemisphere, it will be low in December.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 5 27.03 13 11.8 0.365 1.327 155 7.8 1:27 ( 0, 68)
Nov. 28 5 25.80 21 58.9 0.386 1.361 163 8.0 0:59 ( 0, 77)
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Now it is 9.4 mag (Nov. 15, Chris Wyatt). It stays observable in the evening low sky after this while it will be getting fainter gradually.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 20 4.74 -24 11.5 1.716 1.483 59 9.8 18:19 ( 34, 23)
Nov. 28 20 29.55 -22 46.6 1.780 1.515 58 10.1 18:18 ( 35, 24)
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Brightened rapidly. Now it is very bright as 9.7 mag (Nov. 15, Chris Wyatt). It is observable at 10-11 mag in excellent condition from October to November.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 23 48.37 1 7.6 0.538 1.334 118 10.2 19:46 ( 0, 57)
Nov. 28 23 58.45 6 24.2 0.569 1.338 116 10.5 19:29 ( 0, 62)
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It brightened up to 13.5 mag in summer (July 31, Ken-ichi Kadota). It is expected to brighten up to 12 mag from autumn to winter. In the Southern Hemisphere, it will appear in the morning sky in December, then it stays observable in good condition. In the Northern Hemisphere, it will be observable in the extremely low sky only from November to December.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 13 46.96 -15 51.8 2.510 1.711 28 12.6 5:12 (295, 7)
Nov. 28 13 54.00 -19 49.8 2.442 1.705 33 12.6 5:17 (303, 10)
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First return of a new periodic comet which brightened up to 13 mag in 2009. Now it is bright as 13.5 mag (Nov. 21, Seiichi Yoshida). It is expected to brighten up to 12 mag and to be observable in excellent condition in winter.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 4 20.81 -13 14.3 0.433 1.368 145 12.9 0:21 ( 0, 42)
Nov. 28 4 23.33 -12 52.9 0.411 1.346 145 12.7 23:52 ( 0, 42)
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Jean-Franois Soulier and Nick James discovered its new outburst on Nov. 19. Now it is bright as 12.6 mag (Nov. 20, Maik Meyer).
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 2 24.89 26 10.4 4.899 5.838 160 13.2 22:21 ( 0, 81)
Nov. 28 2 21.94 25 50.4 4.940 5.840 153 13.2 21:51 ( 0, 81)
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It was expected to brighten very rapidly, and brighten up to 11 mag from December to January. But actually it is much fainter than this ephemeris. Now it is fainter than 16.5 mag (Nov. 21, Michael Jager). It stays observable for a long time in this apparition.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 19 25.48 -10 27.0 1.025 0.906 53 13.9 18:19 ( 51, 29)
Nov. 28 19 51.13 -10 11.5 0.954 0.861 52 13.2 18:18 ( 51, 29)
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Brightened very rapidly. Now it is very bright as 13.4 mag (Nov. 6, Michael Jager). It approaches to Earth down to 0.5 a.u. in November, and it is observable in excellent condition.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 0 27.44 14 34.4 0.517 1.390 132 13.5 20:25 ( 0, 70)
Nov. 28 0 44.37 12 14.3 0.539 1.389 128 13.6 20:15 ( 0, 67)
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Now it is 11.2 mag (Sept. 11, Carlos Labordena). Now it is not observable. It will appear in the morning sky at 14.5 mag.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 16 1.98 -19 38.9 3.976 2.991 3 13.7 18:19 ( 76,-15)
Nov. 28 16 10.92 -20 55.5 4.044 3.058 1 13.8 5:17 (284,-17)
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It approached to Sun down to 0.29 a.u. on July 3, and it brightened up to 0.6 mag (Alan Hale). Now it is fading. It has faded down to 11.3 mag in September (Sept. 27, Mitsunori Tsumura). Now it is not observable. It will appear in the morning sky at 16 mag.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 15 55.99 -19 41.2 3.691 2.704 2 14.3 18:19 ( 77,-16)
Nov. 28 16 2.07 -20 22.9 3.785 2.801 3 14.6 5:17 (285,-15)
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It stays 13-14 mag from 2020 to 2021. It is not observable until January.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 15 37.96 -14 16.9 3.889 2.909 5 14.4 5:12 (278,-13)
Nov. 28 15 49.50 -15 12.9 3.873 2.902 8 14.4 5:17 (282, -9)
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Now it is 12.5 mag (Oct. 28, Michael Jager). In the Northern Hemisphere, appearing in the morning sky. It stasy observable after this while the comet will be fading rapidly. In the Southern Hemipshere, it will never be observable again.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 14 34.12 8 37.2 1.522 0.888 33 14.4 5:12 (268, 13)
Nov. 28 14 48.75 7 48.7 1.643 1.027 36 15.2 5:17 (272, 16)
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Now it is 14.0 mag (Nov. 11, Toshihiko Ikemura, Hirohisa Sato). It is expected to be observable at 5-6 mag for a long time from 2022 to 2023. In the Northern Hemisphere, it is not observable at the high light from 2022 summer to 2023 summer. In the Southern Hemisphere, it is not observable now. But it will be observable in good condition at the high light.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 17 27.91 37 5.8 8.173 7.755 61 14.5 18:19 (115, 32)
Nov. 28 17 31.92 36 34.6 8.138 7.701 60 14.4 18:18 (117, 28)
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Now it is 13.9 mag (Nov. 9, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 12 mag in winter in 2022. In the Northern Hemisphere, it stays observable in good condition for a long time. In the Southern Hemisphere, it is not observable until 2021 November.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 23 54.75 62 27.2 4.499 5.094 122 14.5 19:52 (180, 62)
Nov. 28 23 54.55 61 32.5 4.483 5.053 120 14.5 19:24 (180, 63)
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Now it is 14.8 mag (May 14, Toshiyuki Takahashi). It will brighten up to 13 mag in 2021. In the Southern Hemisphere, it becomes too low to observe temporarily from mid October to mid December. In the Northern Hemisphere, it is not observable until July in 2022.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 15 21.55 -39 5.7 4.992 4.077 19 14.6 5:12 (303,-23)
Nov. 28 15 30.64 -40 17.8 4.952 4.048 21 14.5 5:17 (306,-19)
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Now it is 14.3 mag (Nov. 5, Sandor Szabo). In the Northern Hemisphere, it stays observable for a long time while it is getting fainter slowly. In the Southern Hemisphere, it will never be observable again.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 15 41.94 60 42.3 4.755 4.696 80 15.2 5:12 (213, 27)
Nov. 28 15 50.08 60 14.4 4.783 4.742 81 15.3 5:17 (215, 29)
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Now it is 15.0 mag (Nov. 15, Chris Wyatt). It stays 14-15 mag until 2021. In the Southern Hemisphere, it stays observable in good condition for a long time. In the Northern Hemisphere, it is not observable until June in 2021.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 19 19.16 -63 41.1 4.916 4.444 56 15.2 18:19 ( 19,-15)
Nov. 28 19 34.46 -62 25.9 4.954 4.432 53 15.2 18:18 ( 21,-15)
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Now it is 14.9 mag (Oct. 10, Chris Wyatt). It will brighten up to 13.5 mag in spring in 2021. In the Southern Hemisphere, it stays observable in good condition for a long time, although it becomes unobservable temporarily in December. In the Northern Hemisphere, it is not observable until spring in 2021.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 17 22.23 -45 53.5 4.423 3.630 32 15.3 18:19 ( 44,-15)
Nov. 28 17 25.29 -45 9.1 4.450 3.606 27 15.3 18:18 ( 47,-18)
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Now it is 15.8 mag (Nov. 5, Ken-ichi Kadota). It is observable only until mid December in the Southern Hemisphere, or mid January in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 19 50.83 -23 46.8 2.582 2.196 56 15.5 18:19 ( 37, 21)
Nov. 28 20 4.26 -22 24.8 2.632 2.179 52 15.4 18:18 ( 40, 21)
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Now it is 15.9 mag (Nov. 10, Toshihiko Ikemura, Hirohisa Sato). It will stay at 14 mag for a long time from 2021 to 2022. In the Northern Hemisphere, it stays observable in good condition while brightening gradually, although it becomes unobservable temporarily in December. In the Southern Hemisphere, it is not observable until February.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 17 41.19 8 59.3 6.366 5.650 40 15.5 18:19 ( 86, 21)
Nov. 28 17 44.28 8 9.6 6.387 5.625 36 15.5 18:18 ( 89, 16)
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Now it is 16.3 mag (Nov. 14, Y. Sugiyama). It will brighten up to 13.5 mag from winter to spring in 2021. In the Northern Hemisphere, it stays observable in excellent condition. In the Southern Hemisphere, it stays extremely low until spring.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 23 22.97 44 6.1 1.376 2.065 120 15.8 19:20 (180, 81)
Nov. 28 23 25.25 42 15.7 1.346 1.994 116 15.6 18:55 (180, 83)
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It brightened up to 6.0 mag in June (June 13, Marco Goiato). Now it is fading. It has already faded down to 15.7 mag (Nov. 12, Toshihiko Ikemura, Hirohisa Sato). In the Northern Hemisphere, it stays observable for a long time until it fades out. In the Southern Hemisphere, it will never be observable again.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 18 12.66 23 42.5 2.981 2.568 56 15.7 18:19 ( 96, 36)
Nov. 28 18 26.19 24 1.7 3.088 2.653 55 16.0 18:18 ( 98, 33)
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It will approach to Sun down to 0.14 a.u. on Dec. 7, and will brighten up to 11 mag. But it is not observable at the high light.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 13 29.11 -14 35.8 0.678 0.561 33 16.1 5:12 (297, 12)
Nov. 28 14 43.76 -21 37.6 0.801 0.380 21 15.8 5:17 (297, 0)
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Now it is 15.4 mag (Nov. 4, Giuseppe Pappa). It is expected to brighten up to 13 mag in 2022. In 2020, it is observable in excellent condition in the Southern Hemisphere. In the Northern Hemisphere, it is observable from autumn to winter, but it locating extremely low.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 8 32.80 -36 48.5 6.093 6.205 91 15.9 4:32 ( 0, 18)
Nov. 28 8 33.15 -37 34.4 5.990 6.167 95 15.8 4:05 ( 0, 17)
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Now it is 15.1 mag (Nov. 9, Toshihiko Ikemura, Hirohisa Sato). It stays 15-16 mag until winter. In the Northern Hemisphere, it stays observable in good condition for a long time after this. In the Southern Hemisphere, it will be getting lower after this, and it will be unobservable in January.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 22 9.28 -23 27.4 0.901 1.304 87 15.9 18:19 ( 3, 32)
Nov. 28 22 23.96 -17 46.2 0.921 1.294 85 15.9 18:18 ( 7, 37)
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Now it is 15.6 mag (Nov. 5, Sandor Szabo). It stays 15-16 mag for a long time until 2021. In the Northern Hemisphere, it stays observable in good condition for a long time. In the Southern Hemisphere, it will be observable in the extremely low sky only in next spring.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 18 32.18 19 14.9 5.126 4.653 56 15.9 18:19 ( 88, 37)
Nov. 28 18 34.98 19 30.7 5.194 4.669 53 16.0 18:18 ( 92, 33)
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Now it is 16.3 mag (Nov. 9, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 14.5 mag from spring to summer in 2021. In the Southern Hemisphere, it stays observable in excellent condition for a long time. In the Northern Hemisphere, it is observable in good condition in 2020, however, it will be unobservable in 2021.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 21 13.42 -30 4.6 3.221 3.085 73 15.9 18:19 ( 16, 23)
Nov. 28 21 14.32 -30 59.1 3.307 3.049 66 15.9 18:18 ( 21, 20)
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First return of a new periodic comet which brightened up to 17 mag in 2013. Now it is 17.2 mag (Nov. 10, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 16 mag and will be observable in good condition in winter. In the Southern Hemisphere, it locates low until December.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 9 41.00 37 36.0 0.506 1.207 103 16.3 5:12 (244, 84)
Nov. 28 10 23.61 35 1.8 0.484 1.176 100 16.1 5:17 (267, 82)
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It brightened up to 13.5 mag in last winter (Dec. 6, 2019, Chris Wyatt). Now it is fading slowly. Now it is 16.3 mag (Nov. 13, Martin Masek). In the Southern Hemisphere, it stays observable for a long time. It locates somewhat low in the Northern Hemisphere. Taras Prystavski found its fragmentation on Sept. 12.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 1 34.35 -32 59.3 4.131 4.682 118 16.1 21:30 ( 0, 22)
Nov. 28 1 28.38 -31 40.1 4.242 4.723 113 16.3 20:57 ( 0, 24)
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Now it is 16.0 mag (Nov. 10, Toshihiko Ikemura, Hirohisa Sato). It stays 16 mag until winter, and observable in good condition. It locates somewhat low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 8 41.23 17 35.8 1.745 2.290 110 16.3 4:41 ( 0, 73)
Nov. 28 8 43.13 17 50.0 1.701 2.327 117 16.4 4:15 ( 0, 73)
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It brightened up to 13.8 mag in autumn in 2019 (Sept. 3, 2019, Chris Wyatt). Now it is fading slowly. It has already faded down to 16.5 mag (Nov. 8, Toshihiko Ikemura, Hirohisa Sato). But it is still bright visually as 14.8 mag (Nov. 5, Sandor Szabo).
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 23 43.85 2 35.0 6.135 6.662 118 16.3 19:41 ( 0, 58)
Nov. 28 23 42.84 2 48.4 6.284 6.704 111 16.4 19:12 ( 0, 58)
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Now it is 16.4 mag (Nov. 9, Toshihiko Ikemura, Hirohisa Sato). It is observable at 16.5-17 mag from 2020 to 2021. In the Southern Hemisphere, it is not observable until summer in 2021
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 22 4.27 59 30.6 5.590 5.989 109 16.5 18:19 (175, 65)
Nov. 28 22 3.81 57 39.4 5.632 5.984 106 16.5 18:18 (165, 66)
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Now it is 17.3 mag (Nov. 10, Toshihiko Ikemura, Hirohisa Sato). It will approach to Earth down to 0.46 a.u. in 2021 April, and it is expected to brighten up to 12.5 mag and to be observable in excellent condition.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 22 20.11 -22 26.7 1.613 1.889 89 16.8 18:19 ( 1, 33)
Nov. 28 22 2.64 -22 6.1 1.709 1.806 79 16.7 18:18 ( 13, 32)
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Now it is 16.6 mag (Nov. 9, Toshihiko Ikemura, Hirohisa Sato). It stays at 16-17 mag from 2020 to 2021. In the Northern Hemisphere, it stays observable in good condition for a long time. It is not observable in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 19 1.42 29 21.8 9.163 8.841 68 16.8 18:19 ( 97, 48)
Nov. 28 19 3.55 29 20.7 9.215 8.839 64 16.8 18:18 (100, 43)
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First return of a new periodic comet which brightened up to 17.5 mag in 2012. Now it is 17.2 mag (Nov. 13, D. Buczynski). It stays observable at 17 mag in good condition from summer to winter. It locates low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 5 5.69 38 28.0 1.598 2.527 154 17.1 1:06 (180, 87)
Nov. 28 4 58.99 38 44.0 1.597 2.548 160 17.1 0:32 (180, 86)
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Now it is 16.1 mag (Nov. 13, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 13 mag in 2022. In 2021, it is observable at 15-16 mag in good condition.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 12 54.38 1 5.0 4.608 4.002 47 17.2 5:12 (291, 28)
Nov. 28 13 0.88 0 27.3 4.511 3.986 52 17.1 5:17 (296, 33)
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It brightened up to 16.1 mag in last winter (Mar. 18, Toshihiko Ikemura, Hirohisa Sato). In 2021, it stays observable at 17 mag in good condition until summer.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 12 45.07 -18 47.6 7.407 6.714 42 17.1 5:12 (308, 16)
Nov. 28 12 49.48 -19 5.7 7.339 6.723 48 17.1 5:17 (314, 20)
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Now it is 17.1 mag (Nov. 8, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 17 mag in December. It is observable in good condition. It locates somewhat low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 2 15.03 38 27.0 1.003 1.936 152 17.3 22:12 (180, 87)
Nov. 28 2 14.11 36 37.8 1.010 1.926 149 17.2 21:43 (180, 88)
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It was expected to brighten very rapidly, and brighten up to 14.5 mag from August to September. However, its current brightness is very uncertain. It could not be detected as fainter than 18.0 mag on June 30 (Charles S. Morris), and fainter than 15.7 mag on July 13 (Sandor Szabo). However, Giuseppe Pappa reported as 14 mag on July 10, and Thomas Lehmann reported it is bright as 15.2 mag on July 12. In the Northern Hemisphere, it stays observable for a long time. It is getting higher gradually after this also in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 10 39.11 -13 5.5 1.662 1.674 73 17.3 5:12 (333, 38)
Nov. 28 10 32.24 -17 41.0 1.639 1.761 80 17.5 5:17 (346, 36)
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Now it is 17.1 mag (Oct. 25, D. Buczynski). It is observable at 17-18 mag for a long time from late 2019 to early 2021. It will fade out before it passes the perihelion.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 5 55.93 17 2.8 3.645 4.522 149 17.4 1:56 ( 0, 72)
Nov. 28 5 52.60 17 13.0 3.588 4.512 156 17.3 1:25 ( 0, 72)
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Now it is 17.2 mag (Oct. 25, A. Mickleburgh). It stays 15-16 mag for a long time from 2021 spring to 2022 spring. It stays observable for a long time in the Northern Hemisphere. In the Southern Hemipsphere, it is not observable until the end of 2021.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 19 25.19 45 27.3 4.004 3.989 82 17.5 18:19 (121, 55)
Nov. 28 19 25.99 44 45.8 4.015 3.947 78 17.5 18:18 (120, 51)
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Now it is 17.3 mag (Nov. 9, Toshihiko Ikemura, Hirohisa Sato). It will be fading after this, and will be fainter than 18 mag in December.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 21 36.46 -0 38.9 2.023 2.211 87 17.5 18:19 ( 19, 53)
Nov. 28 21 48.67 -0 51.8 2.113 2.225 83 17.6 18:18 ( 24, 52)
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It brightened up to 14.6 mag in summer (July 18, Thomas Lehmann). Now it is 17.4 mag (Nov. 8, Toshihiko Ikemura, Hirohisa Sato). It stays observable until December when it becomes fainter than 18 mag.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 21 10.70 -13 7.3 2.277 2.274 77 17.6 18:19 ( 22, 39)
Nov. 28 21 23.49 -12 42.1 2.379 2.299 73 17.8 18:18 ( 26, 38)
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Now it is 17.9 mag (Nov. 19, Giuseppe Pappa). It is expected to brighten up to 12 mag in 2022. In the Southern Hemisphere, it stays observable in good condition for a long time. In the Northern Hemisphere, it is not observable until 2022.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 3 47.56 -49 43.4 6.260 6.669 110 17.7 23:43 ( 0, 5)
Nov. 28 3 39.50 -50 7.6 6.246 6.620 108 17.7 23:07 ( 0, 5)
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First return of a new periodic comet which brightened up to 14-15 mag in 2006. Now it is 18.1 mag (Nov. 20, Toshihiko Ikemura, Hirohisa Sato). It is expected to brighten up to 15-16 mag from February to March, and it will be observable in good condition.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 10 18.21 3 33.3 1.737 1.903 83 18.0 5:12 (331, 55)
Nov. 28 10 33.49 2 55.2 1.647 1.876 87 17.7 5:17 (338, 56)
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Now it is 17.0 mag (Nov. 9, Toshihiko Ikemura, Hirohisa Sato). It stays observable at 17.5-18 mag in good condition until winter.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 7 55.67 18 20.4 1.483 2.169 121 17.7 3:55 ( 0, 73)
Nov. 28 7 56.54 18 55.0 1.443 2.197 128 17.7 3:29 ( 0, 74)
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Now it is 17.5 mag (Nov. 12, Toshihiko Ikemura, Hirohisa Sato). It is expected to brighten up to 14 mag from spring to summer, and it stays observable in good condition for a long time. In the Southern Hemisphere, it is not observable until late December.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 12 14.06 25 42.2 3.566 3.339 68 18.0 5:12 (271, 50)
Nov. 28 12 23.99 25 27.9 3.428 3.282 73 17.8 5:17 (275, 55)
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Now it is 17.5 mag (Nov. 10, ATLAS-MLO, Mauna Loa). It stays 18 mag until November. It is observable in excellent condition in the Southern Hemisphere. It locates very low in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Nov. 21 23 10.50 -34 22.1 2.907 3.150 94 17.9 19:08 ( 0, 21)
Nov. 28 23 15.00 -33 36.3 2.999 3.154 89 18.0 18:45 ( 0, 22)
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