Weekly Information about Bright Comets (2022 Feb. 5: North)

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Updated on February 6, 2022
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Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Northern Hemisphere.
Azimuth indicates 0 for south, 90 for west, 180 for north, 270 for east.

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* 19P/Borrelly

Now it is bright as 9.2 mag (Feb. 5, Osamu Miyazaki). It stays bright as 9-10 mag until March. In the Northern Hemisphere, it stays observable in excellent condition for a long time. In the Southern Hemisphere, it stays extremely low after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   1 35.67    7  4.4   1.283   1.307    68    8.9  18:58 ( 58, 47)  
Feb. 12   1 53.55   11 53.6   1.318   1.312    67    9.0  19:04 ( 68, 48)  

* C/2021 A1 ( Leonard )

It brightened up to 3 mag from mid December to late December. Now it is fading. It faded down to 8.5 mag in late January (Jan. 28, Chris Wyatt). In the Southern Hemisphere, it becomes unobservable temporarily in early February. But it will appear in the morning sky in mid February. In the Northern Hemisphere, it will become observable again at 13 mag in late April.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  21 32.65  -35 47.1   1.783   0.922    20    9.4  18:58 ( 62,-24)  
Feb. 12  21 29.70  -35 28.3   1.876   1.027    21   10.0   5:24 (296,-26)  

* C/2019 L3 ( ATLAS )

Now it is 9.9 mag (Feb. 5, Osamu Miyazaki). It stays bright as 10 mag until spring for a long time. It stays observable in good condition for a long time. It locates somewhat low in the Southern Hemisphere,

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   6 41.72   25 56.9   2.722   3.563   143   10.0  21:40 (  0, 81)  
Feb. 12   6 38.20   24 33.0   2.794   3.568   135   10.0  21:09 (  0, 79)  

* C/2017 K2 ( PanSTARRS )

Now it is bright as 11.7 mag (Jan. 27, Osamu Miyazaki). It is expected to be observable at 5-6 mag for a long time from 2022 to 2023. In the Northern Hemisphere, it stays observable in good condition until autumn. However, it is not observable at the high light from autumn to 2023 summer. In the Southern Hemisphere, it will be observable after February. Then 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)  
Feb.  5  18 25.18   11 35.2   4.645   4.081    49   10.4   5:29 (278, 32)  
Feb. 12  18 30.24   11 26.6   4.523   4.018    53   10.3   5:24 (281, 35)  

* 104P/Kowal 2

Brightened very rapidly. Now it is very bright as 10.2 mag (Feb. 3, Osamu Miyazaki). It is observable at 10 mag in good condition until February.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   2 42.53    5 42.2   0.644   1.122    84   10.5  18:58 ( 35, 56)  
Feb. 12   3 18.64    8  2.2   0.658   1.153    86   10.9  19:04 ( 36, 59)  

* 67P/Churyumov-Gerasimenko

Now it is very bright as 10.0 mag (Feb. 2, Osamu Miyazaki). It stays observable in good condition for a long time. It locates somewhat low in the Southern Hemisphere,

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   8 28.04   28 41.4   0.692   1.661   163   10.7  23:26 (  0, 84)  
Feb. 12   8 24.48   28 13.5   0.761   1.714   157   11.1  22:55 (  0, 83)  

* 22P/Kopff

In the Northern Hemisphere, it stays extremely low until spring. In the Southern Hemisphere, it stays observable at 11 mag until June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  18 41.65  -20 50.9   2.294   1.608    36   11.4   5:29 (303,  8)  
Feb. 12  19  4.54  -20 31.4   2.250   1.591    37   11.3   5:24 (302,  8)  

* C/2019 T4 ( ATLAS )

Now it is 12.7 mag (Jan. 31, Chris Wyatt). It will brighten up to 11.5 mag in spring. It stas observable in good condition for a long time.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  12  8.09  -29 13.1   3.814   4.366   118   11.9   3:09 (  0, 26)  
Feb. 12  12  7.43  -28 46.7   3.716   4.353   124   11.8   2:41 (  0, 26)  

* 9P/Tempel 1

Now it is 14.7 mag (Feb. 3, Giuseppe Pappa). It will brighten up to 12 mag from winter to spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  17 24.18  -20 32.4   1.924   1.569    54   12.3   5:29 (316, 21)  
Feb. 12  17 46.61  -21 20.4   1.876   1.558    56   12.3   5:24 (317, 20)  

* C/2021 F1 ( Lemmon-PanSTARRS )

Now it is bright as 12.8 mag (Jan. 30, Charles S. Morris). Cometary activity was detected. It stays 13 mag until spring. In the Northern Hemisphere, it is observable only until early March. In the Southern Hemisphere, it is not observable until late May. But it will be observable in good condition after that.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  19 20.53   48 13.0   1.432   1.418    69   13.3   5:29 (232, 36)  
Feb. 12  20 21.47   48 58.5   1.411   1.342    65   13.0   5:24 (229, 30)  

* 4P/Faye

It brightened up to 10.6 mag in autumn (Oct. 10, Osamu Miyazaki). Now it is fading. It has already faded down to 13.0 mag (Jan. 31, Chris Wyatt). It stays observable in good condition for a long time.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   6 20.32   10 29.3   1.342   2.175   137   13.2  21:19 (  0, 66)  
Feb. 12   6 21.75   11 11.5   1.437   2.217   131   13.5  20:53 (  0, 66)  

* 29P/Schwassmann-Wachmann 1

Now it is bright as 11.1 mag (Jan. 24, Charles S. Morris). It has a large diffuse coma.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   4 15.64   29 48.8   5.527   5.955   111   13.5  19:14 (  0, 85)  
Feb. 12   4 16.30   29 37.8   5.636   5.957   104   13.6  19:04 ( 34, 84)  

* C/2020 Y2 ( ATLAS )

Now it is 15.8 mag (Jan. 18, J. Drummond). It will brighten up to 13 mag in spring. In the Southern Hemisphere, it stays observable in good condition for a long time. In the Northern Hemisphere, it is not observable until autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  11 45.64  -65 58.6   3.183   3.384    93   13.8   2:48 (  0,-11)  
Feb. 12  11 16.57  -68  5.8   3.105   3.359    96   13.7   1:51 (  0,-13)  

* C/2021 O3 ( PanSTARRS )

Now it is 15.5 mag (Jan. 22, Ken-ichi Kadota). It is expected to brighten very rapidly up to 4.5 mag in April. However, it is not observable at the high light. In the Northern Hemisphere, it stays observable until early February when it brightens up to 14 mag. Then it will appear at 6 mag in mid May, and it stays observable in good condition after that while the comet will be fading. In the Southern Hemisphere, it is not observable until August.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  22 56.93    0 33.3   2.491   1.717    30   14.3  18:58 ( 82, 12)  
Feb. 12  23  8.11    0 16.4   2.427   1.596    25   14.0  19:04 ( 85,  8)  

* 116P/Wild 4

Now it is 14.2 mag (Jan. 31, Toshihiko Ikemura, Hirohisa Sato). It is observable at 13.5 mag in good condition until spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   9 56.07   18  4.3   1.486   2.462   169   14.1   0:58 (  0, 73)  
Feb. 12   9 50.51   18 29.8   1.458   2.442   174   14.0   0:25 (  0, 73)  

* C/2020 J1 ( SONEAR )

It brightened up to 12.3 mag from spring to summer (June 15, Marco Goiato). Now it is fading. It has already faded down to 14.2 mag (Jan. 15, Ken-ichi Kadota).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  14 21.65   11 25.0   3.928   4.295   105   14.0   5:22 (  0, 66)  
Feb. 12  14 17.50   13 13.3   3.851   4.334   113   14.0   4:51 (  0, 68)  

* C/2021 E3 ( ZTF )

Now it is 14.9 mag (Nov. 28, Thomas Lehmann). It is expected to brighten up to 11 mag from spring to summer. In the Southen Hemisphere, it is not observable until February, but it stays observable in good condition for a long time after that. In the Northern Hemisphere, it is hardly observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  19 49.56  -13  1.9   3.284   2.386    20   14.4   5:29 (286,  0)  
Feb. 12  19 56.67  -14 13.9   3.184   2.331    25   14.2   5:24 (289,  3)  

* C/2020 V2 ( ZTF )

Now it is 14.5 mag (Jan. 31, Thomas Lehmann). It is expected to brighten up to 10 mag in 2023. In the Northern Hemisphere, it stays observable in good condition until 2023 autumn. In the Southern Hemipshere, it locates extremely low from January to February. Then it stays unobservable until 2023 summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  12 56.84   49 40.8   4.597   5.214   124   14.5   3:58 (180, 75)  
Feb. 12  12 50.98   51 32.1   4.508   5.157   126   14.4   3:25 (180, 74)  

* C/2019 U5 ( PanSTARRS )

Now it is 15.0 mag (Jan. 14, Ken-ichi Kadota). It is expected to brighten up to 11 mag in 2023. 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)  
Feb.  5  16 42.92   33 12.4   5.201   5.141    81   14.7   5:29 (264, 62)  
Feb. 12  16 42.66   33 58.0   5.083   5.101    85   14.6   5:24 (265, 67)  

* 117P/Helin-Roman-Alu 1

Now it is 15.8 mag (Oct. 4, Thomas Lehmann). Appearing in the morning. It will brighten up to 13 mag in summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  17 36.43  -24 50.5   3.654   3.132    51   14.7   5:29 (317, 15)  
Feb. 12  17 46.72  -25  7.6   3.567   3.124    55   14.7   5:24 (319, 17)  

* C/2020 R7 ( ATLAS )

Now it is 15.9 mag (Jan. 2, Thomas Lehmann). It will brighten up to 12.5 mag in summer. In the Southern Hemisphere, it stays observable in excellent condition for a long time, although it becomes low temporarily in February. In the Northern Hemisphere, it is not observable until August.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  22 24.97  -58 33.9   4.315   3.678    44   14.8  18:58 ( 35,-26)  
Feb. 12  22 27.81  -57 34.7   4.275   3.639    44   14.8  19:04 ( 38,-30)  

* C/2020 T2 ( Palomar )

It brightened up to 9.5 mag in early summer (June 27, Marco Goiato). Now it is fading. It has faded down to 12.7 mag in autumn (Nov. 22, Thomas Lehmann). Now it is not observable. In the Southern Hemisphere, it will appear in the morning sky at 15 mag in late February. In the Northern Hemisphere, it is not observable until June when the comet will fade down to 17 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  20 48.49  -32 34.1   4.076   3.149    17   14.8   5:29 (295,-22)  
Feb. 12  21  1.12  -32 18.9   4.111   3.205    20   15.0   5:24 (296,-20)  

* 6P/d'Arrest

It brightened up to 9.8 mag from autumn to winter (Nov. 22, Thomas Lehmann). Now it is fading. It has already faded down to 14.4 mag (Jan. 24, Charles S. Morris). It will be fainter than 18 mag in March.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   1 15.11   -9 56.2   2.349   2.027    59   14.9  18:58 ( 49, 31)  
Feb. 12   1 29.40   -8 10.9   2.457   2.076    56   15.5  19:04 ( 54, 29)  

* 57P/du Toit-Neujmin-Delporte

It brightened up to 11.5 mag in outburst in October (Oct. 22, Marco Goiato). Now it is fading. It has already faded down to 15.1 mag (Jan. 24, A. Diepvens). But Hiroshi Abe reported it is bright as 12.3 mag on Jan. 22. In the Southern Hemisphere, it is already unobservable. In the Northern Hemisphere, it stays observable until early February.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  23  0.52   -5 55.3   2.803   1.989    28   15.2  18:58 ( 76,  9)  
Feb. 12  23 16.32   -4 22.4   2.868   2.020    25   15.5  19:04 ( 80,  7)  

* C/2018 U1 ( Lemmon )

Now it is 15.9 mag (Oct. 8, Thomas Lehmann). It stays at 14-15 mag for a long time from 2021 to 2022. In the Southern Hemisphere, it stays observable in excellent condition for a long time. In the Northern Hemiphere, it locates extremely low in spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  17 17.48  -33 34.1   5.537   5.045    55   15.2   5:29 (325, 11)  
Feb. 12  17 19.28  -34 33.5   5.439   5.053    62   15.2   5:24 (329, 12)  

* C/2020 K1 ( PanSTARRS )

Now it is 15.6 mag (Jan. 31, Thomas Lehmann). It is expected to brighten up to 11 mag in 2023. In the Northern Hemisphere, it stays observable in good condition until November. But it becomes unobservable after that. In the Southern Hemisphere, it is not observable until February. 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)  
Feb.  5  18 39.99   17 22.4   5.804   5.232    50   15.4   5:29 (270, 32)  
Feb. 12  18 44.14   17 18.8   5.707   5.184    53   15.4   5:24 (273, 36)  

* 110P/Hartley 3

It brightened rapidly. Now it is 15.1 mag (Jan. 31, Toshihiko Ikemura, Hirohisa Sato). It stays 15 mag until February, and it is observable in excellent condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   8  3.48   14 13.3   1.587   2.546   163   15.4  23:01 (  0, 69)  
Feb. 12   7 58.63   14  0.5   1.628   2.558   155   15.5  22:29 (  0, 69)  

* C/2020 PV6 ( PanSTARRS )

Now it is 15.6 mag (Jan. 7, Toshihiko Ikemura, Hirohisa Sato). It will be fading after this. In the Northern Hemisphere, it stays observable in good condition for a long time. It locates low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  15 58.51   28  4.8   2.556   2.707    87   15.4   5:29 (284, 70)  
Feb. 12  15 50.63   30 25.3   2.479   2.746    94   15.5   5:24 (286, 77)  

* C/2021 P4 ( ATLAS )

Now it is 15.3 mag (Jan. 9, D. Buczynski). It is expected to brighten up to 11 mag in summer. In the Northern Hemisphere, it stays observable in good condition until June when it brightens up to 11 mag. But it is not observable after the high light. In the Souther Hemisphere, it is not observable until October.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  23 17.04   50 55.5   2.898   2.763    72   15.7  18:58 (131, 38)  
Feb. 12  23 28.13   51  7.2   2.872   2.683    69   15.6  19:04 (132, 35)  

* 70P/Kojima

Now it is 15.8 mag (Jan. 27, Toshihiko Ikemura, Hirohisa Sato). It stays 15.5 mag until March, and it is observable in excellent condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  11 54.21    8 10.3   1.297   2.147   139   15.7   2:55 (  0, 63)  
Feb. 12  11 53.20    8 55.7   1.270   2.167   147   15.7   2:27 (  0, 64)  

* C/2020 M5 ( ATLAS )

Now it is 15.0 mag (Feb. 1, Thomas Lehmann). It stays observable at 15-16 mag for a long time.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  12 46.23   11 56.8   2.732   3.432   128   15.7   3:47 (  0, 67)  
Feb. 12  12 36.06   11 33.7   2.674   3.465   137   15.7   3:10 (  0, 66)  

* 8P/Tuttle

It brightened very rapidly, and brightened up to 8.9 mag (Sept. 11, Chris Wyatt). Now it is fading. It has already faded down to 15.7 mag (Dec. 7, E. Cortes, N. Paul, B. Lutkenhoner). In the Southern Hemisphere, it stays observable after this while the comet will be fading. It is not observable after this in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  17 17.22  -54 47.0   2.730   2.382    59   15.7   5:29 (337, -7)  
Feb. 12  17 28.64  -54 59.6   2.729   2.451    63   16.0   5:24 (338, -6)  

* 402P/2020 Q3 ( LINEAR )

First return of a new periodic comet observed at 16 mag from 2003 to 2004. Now it is 16.1 mag (Jan. 3, Toshihiko Ikemura, Hirohisa Sato). It stays 16 mag until March, and it stays observable in excellent condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   6  1.79    7 47.6   3.215   3.949   132   16.0  21:00 (  0, 63)  
Feb. 12   6  0.65    8 46.0   3.293   3.953   125   16.0  20:31 (  0, 64)  

* C/2021 O1 ( Nishimura )

It was observed at 9-10 mag from late July to early August. Although it had been unobservable for a long time, it is appearing in the morning sky now.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  16 30.15  -26 37.0   3.117   2.862    65   16.0   5:29 (331, 22)  
Feb. 12  16 34.88  -27 23.6   3.100   2.947    71   16.2   5:24 (335, 23)  

* C/2020 H6 ( ATLAS )

Now it is 16.0 mag (Jan. 15, Ken-ichi Kadota). It stays observable at 16 mag from 2021 to 2022. Appearing in the morning sky also in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  16  7.90   16 15.1   4.847   4.809    81   16.2   5:29 (304, 61)  
Feb. 12  16 11.55   17 49.1   4.767   4.821    87   16.1   5:24 (309, 65)  

* 132P/Helin-Roman-Alu 2

It brightened up to 13.1 mag in autumn (Oct. 28, Toshihiko Ikemura, Hirohisa Sato). Now it is fading. But it is still bright as 14.2 mag (Jan. 26, Giuseppe Pappa). It stays observable in good condition for a long time. But it will be fainter than 18 mag in March.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   2 46.88    9 48.8   1.662   1.880    86   16.2  18:58 ( 37, 60)  
Feb. 12   3  1.48   11  5.4   1.755   1.910    83   16.4  19:04 ( 46, 59)  

* C/2019 F1 ( ATLAS-Africano )

Now it is 16.2 mag (Jan. 27, SONEAR Observatory, Oliveira). It will be fading slowly after this. In the Southern Hemisphere, it stays observable in good condition for a long time. In the Northern Hemisphere, it is not observable until July.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  23 56.27  -45  0.2   4.775   4.133    44   16.2  18:58 ( 39, -7)  
Feb. 12   0  5.05  -43 17.0   4.836   4.164    42   16.3  19:04 ( 43, -9)  

* P/2021 N2 ( Fuls )

Brightened rapidly. Now it is 16.5 mag (Jan. 24, Charles S. Morris). It is observable at 15.5-16 mag in good condition in winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   2 23.41   11 43.1   3.847   3.829    81   16.4  18:58 ( 49, 58)  
Feb. 12   2 28.96   11 59.5   3.954   3.834    75   16.5  19:04 ( 58, 54)  

* C/2020 O2 ( Amaral )

It was observed at 15 mag in 2021. Now it is fading. It stays observable at 17 mag for a while in 2022.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  18 20.36    2 12.5   5.648   5.020    46   16.6   5:29 (288, 27)  
Feb. 12  18 25.06    3 19.8   5.588   5.034    51   16.6   5:24 (290, 31)  

* C/2020 F7 ( Lemmon )

Now it is 17.2 mag (Jan. 18, J. Drummond). It brightened rapidly. It stays 17 mag for a long time from 2021 to 2022. In the Southern Hemisphere, it stays observable in good condition for a long time. In the Northern Hemisphere, it will be observable only in extremely low sky from autumn to winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   7 38.08  -47 13.3   4.902   5.368   113   16.7  22:35 (  0,  8)  
Feb. 12   7 28.07  -47 14.1   4.925   5.374   112   16.7  21:57 (  0,  8)  

* C/2021 U5 ( Catalina )

Now it is 16.5 mag (Jan. 29, Toshihiko Ikemura, Hirohisa Sato). It is observable at 16.5 mag in good condition from winter to spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  10 21.28  -25 36.6   1.562   2.365   135   16.8   1:23 (  0, 29)  
Feb. 12  10 20.66  -23 54.0   1.520   2.370   141   16.7   0:54 (  0, 31)  

* C/2020 S4 ( PanSTARRS )

Now it is 16.9 mag (Jan. 31, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 14 mag in early 2023. It stays observable in good condition until spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   4 18.20    5 41.2   4.362   4.747   107   16.8  19:17 (  0, 61)  
Feb. 12   4 19.00    6 18.4   4.421   4.705   100   16.8  19:04 (  7, 61)  

* 430P/2021 Q2 ( Scotti )

First return of a new periodic comet which brightened up to 17 mag in 2011. Now it is 18.2 mag (Jan. 8, Toshihiko Ikemura, Hirohisa Sato). It brightened up to 16.8 mag in October (Oct. 10, Ken-ichi Kadota), however, it has been fading after that.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  14 50.06  -11 57.9   1.318   1.675    92   16.8   5:29 (353, 43)  
Feb. 12  15  1.29  -12 52.4   1.280   1.700    96   16.8   5:24 (357, 42)  

* 230P/LINEAR

Now it is 18.7 mag (Jan. 1, W. Hasubick). It was expected to brighten up to 16.5-17 mag in winter. In its last apparition in 2015, it brightened up to 13 mag. But actually, it is fainter than this ephemeris recently.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   0 41.78   -8 11.0   2.046   1.626    51   16.9  18:58 ( 57, 27)  
Feb. 12   0 58.78   -5 46.3   2.069   1.609    49   16.8  19:04 ( 62, 26)  

* C/2019 O3 ( Palomar )

Now it is 16.9 mag (Jan. 8, Toshihiko Ikemura, Hirohisa Sato). Fading slowly. In the Northern Hemisphere, it stays observable in good condition for a long time. In the Southern Hemisphere, it is not observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  19  7.42   50 24.1   9.285   9.029    72   16.9   5:29 (230, 39)  
Feb. 12  19 10.79   51  9.1   9.280   9.037    72   16.9   5:24 (229, 42)  

* C/2020 U5 ( PanSTARRS )

Now it is 16.5 mag (Jan. 9, ATLAS-HKO, Haleakala). It started fading before the perihelion passage. It was predicted to stay at 16 mag for a long time, but actually, it will be fainter than 18 mag in autumn. In the Northern Hemisphere, it stays observable in good condition for a long time. In the Southern Hemisphere, it is not observable until 2023.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  23  0.31   81  2.2   3.561   3.825    98   16.9  18:58 (169, 37)  
Feb. 12  23 10.60   79 29.0   3.614   3.814    94   17.0  19:04 (167, 36)  

* 52P/Harrington-Abell

It brightened up to 16.4 mag from autumn to winter (Oct. 6, ATLAS-MLO, Mauna Loa). Now it is fading. It has already faded down to 18.0 mag (Jan. 31, Catalina Sky Survey).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  12 55.05  -10 18.5   1.442   2.106   119   17.0   3:56 (  0, 45)  
Feb. 12  12 54.91  -11 11.5   1.406   2.139   125   17.0   3:28 (  0, 44)  

* 325P/Yang-Gao

It has not been observed yet in this apparition. It was expected to be observable at 16 mag in good condition in spring. But actually, it is fainter than 19.2 mag (Jan. 22, John Drummond).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  16  0.03  -34  1.7   1.538   1.542    71   17.3   5:29 (340, 18)  
Feb. 12  16 26.42  -34 30.1   1.475   1.516    72   17.1   5:24 (340, 17)  

* 81P/Wild 2

Now it is 16.6 mag (Jan. 29, Observatoire Chante-Perdrix, Dauban). It will brighten up to 11.5 mag in 2022 winter. It stays observable while the comet will be brightening slowly.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   3  1.97   13 48.4   2.895   3.078    91   17.1  18:58 ( 35, 65)  
Feb. 12   3  5.61   14 12.1   2.961   3.039    85   17.1  19:04 ( 49, 62)  

* 254P/McNaught

Now it is 17.0 mag (Jan. 29, ATLAS-MLO, Mauna Loa). It continued brightening for a while even after the perihelion passage. It stays observable at 16-17 mag in good condition for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   4 22.51   -8 23.5   3.653   4.008   104   17.1  19:21 (  0, 47)  
Feb. 12   4 23.76   -7 13.2   3.761   4.027    98   17.1  19:04 (  3, 48)  

* 73P/Schwassmann-Wachmann 3

Now it is 18.0 mag (Jan. 31, Toshihiko Ikemura, Hirohisa Sato). It is expected to brighten up to 11 mag from summer to autumn. It stays observable in good condition in the Southern Hemisphere. In the Northern Hemisphere, it becomes extremely low from August to September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  10 59.92   25 25.9   1.601   2.521   153   17.3   2:01 (  0, 80)  
Feb. 12  10 53.62   26 44.4   1.519   2.465   158   17.1   1:28 (  0, 82)  

* C/2020 F2 ( ATLAS )

Now it is 17.2 mag (Jan. 28, ATLAS-HKO, Haleakala). It stays observable at 17-18 mag for a long time until 2024.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  14 36.47   -4  5.6   8.681   8.866    97   17.1   5:29 (357, 51)  
Feb. 12  14 34.80   -3 42.1   8.553   8.862   105   17.1   5:08 (  0, 51)  

* 152P/Helin-Lawrence

It will brighten up to 16 mag from spring to summer. It locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  18 13.24  -21 47.5   3.748   3.097    42   17.3   5:29 (308, 12)  
Feb. 12  18 24.00  -21 53.2   3.681   3.099    47   17.2   5:24 (310, 14)  

* C/2021 T2 ( Fuls )

Now it is 17.8 mag (Jan. 2, Ken-ichi Kadota). It is expected to brighten up to 13.5 mag from June to July. It is observable only in the Southern Hemisphere at the high light. In the Northern Hemisphere, it is observable only until March when it brightens up to 16.5 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   1 10.67    5 38.6   2.441   2.171    62   17.3  18:58 ( 63, 41)  
Feb. 12   1 12.61    4  0.8   2.493   2.096    55   17.2  19:04 ( 68, 34)  

* 274P/Tombaugh-Tenagra

Now it is 17.6 mag (Jan. 19, Yasukazu Ikari). It is observable at 17 mag from November to March. It is observable in good condition in the Northern Hemisphere, but it locates low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   5 19.64   30 23.1   1.794   2.495   125   17.2  20:18 (  0, 85)  
Feb. 12   5 21.44   30 51.1   1.860   2.486   118   17.3  19:53 (  0, 86)  

* C/2021 G2 ( ATLAS )

Now it is 17.2 mag (Jan. 22, ATLAS-HKO, Haleakala). It will brighten up to 13-14 mag from 2024 to 2025.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   7 17.07  -31 33.7   7.890   8.491   124   17.3  22:15 (  0, 23)  
Feb. 12   7 14.88  -31 16.7   7.878   8.454   122   17.3  21:45 (  0, 24)  

* 99P/Kowal 1

Now it is 17.3 mag (Jan. 7, Toshihiko Ikemura, Hirohisa Sato). It will be observable at 17 mag in good condition in spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  13 43.15   -9 36.4   4.307   4.713   108   17.3   4:44 (  0, 45)  
Feb. 12  13 43.90   -9 43.1   4.204   4.712   115   17.3   4:17 (  0, 45)  

* C/2019 T2 ( Lemmon )

Now it is 18.4 mag (Jan. 9, J. Drummond). In the Southern Hemisphere, it stays observable for a long time. In the Northern Hemisphere, it is not observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  11  3.41  -53 46.5   3.554   3.945   106   17.3   2:05 (  0,  1)  
Feb. 12  10 51.19  -52 51.5   3.524   3.994   111   17.4   1:25 (  0,  2)  

* C/2020 U4 ( PanSTARRS )

Now it is 17.8 mag (Jan. 8, Toshihiko Ikemura, Hirohisa Sato). It stays 17-18 mag for a long time from 2021 to 2022. It is observable in excellent condition in the Northern Hemisphere, It locates somewhat low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   2 44.25   28 12.8   5.259   5.374    91   17.4  18:58 ( 72, 73)  
Feb. 12   2 41.37   27 47.0   5.387   5.369    83   17.5  19:04 ( 81, 65)  

* 181P/Shoemaker-Levy 6

It has not been observed yet in this return. It was predicted to brighten up to 16.5 mag in January. It will fade out rapidly after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   0  7.94    1 40.6   1.658   1.215    46   17.5  18:58 ( 72, 27)  
Feb. 12   0 31.68    5 45.8   1.695   1.245    46   18.0  19:04 ( 77, 28)  

* C/2021 D2 ( ZTF )

Now it is 16.5 mag (Jan. 26, Ken-ichi Kadota). It was expected to brighten up to 15.5 mag in winter. But actually, it is fading even before the perihelion passage. In the Northern Hemisphere, it stays observable in good condition for a long time. It is not observable at all in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  16 25.60   85 43.1   2.537   2.946   104   17.5   5:29 (183, 39)  
Feb. 12  12 45.88   88 54.1   2.539   2.947   104   17.6   3:36 (180, 36)  

* C/2018 N2 ( ASASSN )

Now it is 17.0 mag (Jan. 26, ATLAS-HKO, Haleakala). 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)  
Feb.  5  14 53.86   43 34.2   7.390   7.696   104   17.5   5:29 (208, 80)  
Feb. 12  14 52.80   44  7.0   7.378   7.743   108   17.6   5:24 (182, 81)  

* P/2020 V4 ( Rankin )

Now it is 16.9 mag (Jan. 31, ATLAS-HKO, Haleakala). It is observable at 17.5 mag in good condition in winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   7 44.92    3 47.9   4.339   5.249   155   17.6  22:43 (  0, 59)  
Feb. 12   7 42.45    4  6.2   4.384   5.256   149   17.6  22:13 (  0, 59)  

* A/2021 X1

Now it is 17.4 mag (Jan. 29, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 15-16 mag in 2023.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   7  9.84  -23 31.4   4.696   5.386   130   17.6  22:07 (  0, 31)  
Feb. 12   7  1.22  -22 51.5   4.695   5.339   126   17.6  21:31 (  0, 32)  

* C/2021 Y1 ( ATLAS )

Now it is 17.4 mag (Jan. 10, Observatoire Chante-Perdrix, Dauban). It is expected to brighten up to 12 mag from winter to summer in 2023. In the Northern Hemisphere, it stays observable in good condition until 2023 spring. In the Southern Hemisphere, it is not observable until summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   1 34.40   48 51.8   5.145   5.184    86   17.7  18:58 (129, 60)  
Feb. 12   1 39.09   47 50.4   5.183   5.126    81   17.7  19:04 (125, 56)  

* C/2017 Y2 ( PanSTARRS )

It was observed at 16 mag from 2020 to 2021. Now it is fading. It will be fainter than 18 mag in spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5  15 41.07  -36 45.9   6.030   5.852    74   17.7   5:29 (345, 16)  
Feb. 12  15 39.34  -37 30.9   5.941   5.884    81   17.7   5:24 (350, 17)  

* 284P/McNaught

It brightened up to 14.5 mag in autumn (Oct. 1, Ken-ichi Kadota). Now it is fading. It has already faded down to 17.1 mag (Jan. 28, Catalina Sky Survey). It will be fading rapidly after this. It will be fainter than 18 mag in February.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   0 59.87   -3 52.2   2.898   2.500    56   17.8  18:58 ( 57, 33)  
Feb. 12   1 10.95   -2 36.6   2.987   2.519    52   17.9  19:04 ( 63, 30)  

* 108P/Ciffreo

It brightened even after the perihelion passage, and it brightened up to 13.5 mag in December (Dec. 6, Katsumi Yoshimoto). Now it is fading. But it is still bright as 16.3 mag (Jan. 24, Charles S. Morris). 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)  
Feb.  5   6 39.64   40 10.2   1.330   2.173   138   18.0  21:38 (180, 85)  
Feb. 12   6 40.10   39 39.9   1.420   2.212   132   18.4  21:11 (180, 85)  

* 440P/2021 W2 ( Kobayashi )

First return of a new periodic comet which brightened up to 16.5 mag in 1997. Now it is 18.5 mag (Jan. 28, Toshihiko Ikemura, Hirohisa Sato). It is fainter than originally predicted, but it is brightening rapidly. It is observable in good condition from January to March.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Feb.  5   8 34.87   26 31.2   1.158   2.129   166   19.6  23:32 (  0, 81)  
Feb. 12   8 30.42   25 35.4   1.158   2.111   159   19.6  23:00 (  0, 80)  

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