Weekly Information about Bright Comets (2022 Jan. 1: North)

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Updated on January 13, 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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* C/2021 A1 ( Leonard )

It brightened up to 3 mag in outburst on Dec. 14. Then several small outbursts occured repeatedly, and the comet has been fading gradually. But it is bright as 5.6 mag still now (Jan. 8, Chris Wyatt). In the Southern Hemisphere, it stays observable in the extremely low sky for a while. In the Northern Hemisphere, it is already unobservable. 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)  
Jan.  1  21 33.91  -35 25.8   0.832   0.617    38    6.0  18:29 ( 42,  3)  
Jan.  8  21 42.09  -36 11.1   1.086   0.624    34    6.6  18:34 ( 45, -1)  

* 19P/Borrelly

Now it is bright as 9.3 mag (Jan. 7, Michael Jager). 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 will be extremely low in February.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   0 17.96  -18 12.3   1.185   1.361    77    9.2  18:29 ( 16, 36)  
Jan.  8   0 32.03  -13 12.2   1.196   1.340    75    9.1  18:34 ( 23, 39)  

* 67P/Churyumov-Gerasimenko

Now it is very bright as 9.5 mag (Jan. 6, Carlos Labordena). 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)  
Jan.  1   8 59.04   28 34.4   0.481   1.418   149    9.2   2:19 (  0, 83)  
Jan.  8   8 53.64   28 55.4   0.506   1.463   156    9.4   1:46 (  0, 84)  

* C/2019 L3 ( ATLAS )

Now it is 9.3 mag (Jan. 6, Marco Goiato). 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)  
Jan.  1   7 12.66   32 56.3   2.587   3.555   168    9.8   0:33 (  0, 88)  
Jan.  8   7  5.37   31 38.0   2.581   3.555   170    9.8  23:53 (  0, 86)  

* 104P/Kowal 2

Brightened very rapidly. Now it is very bright as 9.9 mag (Jan. 8, 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)  
Jan.  1   0  4.82   -5  9.0   0.682   1.083    78   10.2  18:29 ( 25, 47)  
Jan.  8   0 32.16   -3 22.0   0.665   1.074    78   10.0  18:34 ( 27, 48)  

* C/2017 K2 ( PanSTARRS )

Now it is bright as 11.7 mag (Jan. 11, 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)  
Jan.  1  17 57.59   13 17.3   5.127   4.396    38   11.0   5:37 (262, 12)  
Jan.  8  18  3.27   12 48.4   5.049   4.333    39   10.9   5:38 (266, 16)  

* 4P/Faye

Now it is bright as 11.6 mag (Jan. 6, Carlos Labordena). It stays observable in good condition for a long time. But it will be fading gradually after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   6 34.23    7 25.2   1.012   1.976   164   11.7  23:49 (  0, 62)  
Jan.  8   6 29.03    7 51.3   1.057   2.014   161   12.0  23:17 (  0, 63)  

* 6P/d'Arrest

Now it is bright as 11.3 mag (Jan. 3, Chris Wyatt). It will be fading rapidly after this, and it will be fainter than 18 mag in March.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  23 56.32  -19 27.3   1.827   1.785    71   12.1  18:29 ( 21, 33)  
Jan.  8   0 13.29  -17 29.8   1.928   1.832    69   12.6  18:34 ( 26, 33)  

* 22P/Kopff

In the Northern Hemisphere, it stays extremely low until spring. In the Southern Hemisphere, it will appear in the morning sky at 11 mag in late January, then it stays observable at 11 mag until June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  16 51.28  -19 39.0   2.553   1.730    26   12.3   5:37 (299,  5)  
Jan.  8  17 12.48  -20 14.3   2.498   1.701    28   12.1   5:38 (300,  6)  

* C/2019 T4 ( ATLAS )

Now it is 13.3 mag (Jan. 3, 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)  
Jan.  1  12  0.91  -29 28.6   4.374   4.443    87   12.4   5:20 (  0, 25)  
Jan.  8  12  3.72  -29 38.1   4.258   4.427    93   12.3   4:55 (  0, 25)  

* 9P/Tempel 1

Now it is 15.2 mag (Dec. 1, Ken-ichi Kadota). 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)  
Jan.  1  15 37.51  -14 23.6   2.206   1.662    44   13.0   5:37 (307, 22)  
Jan.  8  15 57.89  -15 51.8   2.145   1.638    46   12.8   5:38 (310, 22)  

* 29P/Schwassmann-Wachmann 1

Now it is 16.4 mag (Jan. 11, Jean-Francois Soulier).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   4 21.85   31  0.9   5.092   5.944   147   13.3  21:38 (  0, 86)  
Jan.  8   4 19.39   30 45.4   5.159   5.946   140   13.4  21:08 (  0, 86)  

* 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 14.1 mag (Jan. 1, J.-G. Bosch, F. Kugel, J. Nicolas). 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)  
Jan.  1  21 35.68  -13 19.3   2.470   1.854    41   13.7  18:29 ( 57, 20)  
Jan.  8  21 53.46  -11 55.8   2.537   1.878    39   14.0  18:34 ( 61, 18)  

* 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)  
Jan.  1  19 39.50  -33 19.9   3.807   2.874    15   13.9  18:29 ( 58,-13)  
Jan.  8  19 54.01  -33 16.8   3.873   2.928    13   14.1  18:34 ( 61,-17)  

* 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 14.9 mag (Jan. 1, Toshihiko Ikemura, Hirohisa Sato).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  14 28.64    4 18.4   4.374   4.109    68   14.0   5:37 (308, 47)  
Jan.  8  14 28.82    5 27.7   4.285   4.145    75   14.0   5:38 (316, 52)  

* 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)  
Jan.  1  15 57.58  -53 15.7   2.622   2.027    43   14.0   5:37 (330,-10)  
Jan.  8  16 16.38  -53 42.1   2.659   2.099    45   14.4   5:38 (332,-10)  

* C/2020 Y2 ( ATLAS )

Now it is 15.1 mag (Dec. 14, Chris Wyatt). 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)  
Jan.  1  12 45.78  -52 52.6   3.706   3.522    71   14.3   5:37 (356,  2)  
Jan.  8  12 41.14  -55 29.0   3.590   3.493    76   14.2   5:32 (  0, -1)  

* 116P/Wild 4

Now it is 15.2 mag (Jan. 1, Toshihiko Ikemura, Hirohisa Sato). It will brighten rapidly, and it will be observable at 13.5 mag in good condition from winter to spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  10  9.18   16 30.8   1.810   2.571   131   15.0   3:28 (  0, 71)  
Jan.  8  10  9.05   16 39.9   1.725   2.548   138   14.8   3:01 (  0, 72)  

* C/2020 V2 ( ZTF )

Now it is 13.8 mag (Jan. 7, Toshihiko Ikemura, Hirohisa Sato). 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)  
Jan.  1  13  6.72   41 21.7   5.221   5.495   101   15.0   5:37 (233, 79)  
Jan.  8  13  6.82   42 48.8   5.078   5.439   106   14.9   5:38 (205, 81)  

* 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 bright as 14.2 mag still now (Jan. 1, Toshihiko Ikemura, Hirohisa Sato). 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)  
Jan.  1   1 38.44    2 57.9   1.246   1.759   103   14.9  18:56 (  0, 58)  
Jan.  8   1 51.31    4 20.1   1.322   1.779    99   15.1  18:41 (  0, 60)  

* 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)  
Jan.  1  19 16.36   -7 13.9   3.598   2.677    17   15.1  18:29 ( 83, -3)  
Jan.  8  19 22.61   -8 25.5   3.561   2.617    13   14.9  18:34 ( 86, -9)  

* 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)  
Jan.  1  16 42.21  -22 50.0   4.010   3.177    28   15.1   5:37 (302,  5)  
Jan.  8  16 53.27  -23 19.2   3.950   3.167    32   15.0   5:38 (306,  8)  

* C/2019 U5 ( PanSTARRS )

Now it is 15.7 mag (Dec. 28, D. Buczynski). 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)  
Jan.  1  16 35.82   31  0.7   5.736   5.349    62   15.1   5:37 (255, 37)  
Jan.  8  16 38.07   31 13.6   5.639   5.307    65   15.0   5:38 (257, 42)  

* 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. In the Northern Hemisphere, it is not observable until August.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  22 19.20  -64 56.2   4.375   3.882    54   15.1  18:29 ( 18,-15)  
Jan.  8  22 18.55  -63 29.3   4.380   3.840    51   15.1  18:34 ( 22,-16)  

* 110P/Hartley 3

It brightened rapidly. Now it is 14.8 mag (Jan. 7, Toshihiko Ikemura, Hirohisa Sato). It is observable at 15 mag in excellent condition in winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   8 32.74   15 48.0   1.580   2.499   153   15.1   1:52 (  0, 71)  
Jan.  8   8 27.54   15 23.7   1.554   2.507   161   15.1   1:20 (  0, 70)  

* 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)  
Jan.  1  15 53.50  -22  5.4   3.101   2.423    39   15.3   5:37 (310, 13)  
Jan.  8  16  2.39  -23  6.5   3.120   2.512    44   15.5   5:38 (314, 16)  

* 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. It is not observable from November to January.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  17  2.60  -29  6.2   5.899   5.014    23   15.4   5:37 (304, -3)  
Jan.  8  17  6.12  -29 56.9   5.847   5.019    29   15.3   5:38 (308,  1)  

* C/2021 O3 ( PanSTARRS )

Now it is 15.6 mag (Dec. 28, D. Buczynski). 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)  
Jan.  1  22 14.72    3  9.4   2.646   2.275    57   15.7  18:29 ( 62, 38)  
Jan.  8  22 21.42    2 26.3   2.636   2.168    51   15.5  18:34 ( 67, 33)  

* C/2020 M5 ( ATLAS )

Now it is 15.5 mag (Jan. 1, Toshihiko Ikemura, Hirohisa Sato). 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)  
Jan.  1  13 16.17   14 18.8   3.157   3.282    88   15.7   5:37 (324, 65)  
Jan.  8  13 12.87   13 44.2   3.064   3.310    95   15.7   5:38 (343, 68)  

* C/2020 K1 ( PanSTARRS )

Now it is 16.0 mag (Dec. 8, A. Diepvens). 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)  
Jan.  1  18 16.65   18 41.5   6.159   5.472    42   15.8   5:37 (255, 11)  
Jan.  8  18 21.52   18 17.0   6.106   5.424    42   15.7   5:38 (258, 16)  

* 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)  
Jan.  1   6 17.77    3 19.9   3.004   3.939   159   15.8  23:33 (  0, 58)  
Jan.  8   6 13.61    4  6.6   3.019   3.940   156   15.8  23:02 (  0, 59)  

* C/2020 F5 ( MASTER )

Now it is 15.6 mag (Dec. 27, Ken-ichi Kadota). It will be fading after this. It will be unobservable soon in the Southern Hemisphere, or in early February in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  22 39.20  -15 12.7   5.394   4.907    55   15.9  18:29 ( 43, 28)  
Jan.  8  22 43.13  -14  5.1   5.511   4.934    49   15.9  18:34 ( 50, 25)  

* C/2020 PV6 ( PanSTARRS )

Now it is 15.4 mag (Dec. 29, Ken-ichi Kadota). It will be fading after this. In the Northern Hemisphere, it stays observable in good condition for a long time. In the Southern Hemisphere, it is not observable until late January.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  16 13.51   19 53.3   2.934   2.529    56   15.9   5:37 (270, 36)  
Jan.  8  16 12.78   21  3.4   2.869   2.561    62   16.0   5:38 (273, 43)  

* 70P/Kojima

Now it is 16.2 mag (Dec. 29, Ken-ichi Kadota). It will brighten up to 15.5 mag, and will be observable in excellent condition in winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  11 36.73    6 44.6   1.535   2.065   108   16.0   4:55 (  0, 62)  
Jan.  8  11 43.09    6 41.1   1.477   2.079   113   15.9   4:34 (  0, 62)  

* C/2019 F1 ( ATLAS-Africano )

Now it is 16.5 mag (Dec. 19, E. Cortes, B. Lutkenhoner). 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)  
Jan.  1  23 10.14  -54 24.5   4.426   3.990    57   15.9  18:29 ( 17, -3)  
Jan.  8  23 19.65  -52 26.2   4.500   4.017    54   16.0  18:34 ( 21, -3)  

* P/2021 N2 ( Fuls )

Brightened rapidly. Now it is 16.0 mag (Jan. 1, Toshihiko Ikemura, Hirohisa Sato). It is observable at 15.5-16 mag in good condition until winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   2  4.91   11 15.1   3.318   3.808   112   16.0  19:21 (  0, 66)  
Jan.  8   2  7.21   11 11.9   3.419   3.811   106   16.1  18:56 (  0, 66)  

* C/2020 U5 ( PanSTARRS )

Now it is 16.6 mag (Dec. 10, ATLAS-MLO, Mauna Loa). In the Northern Hemisphere, it stays observable at 16 mag 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)  
Jan.  1  11 44.09   87 42.2   3.396   3.896   113   16.1   5:02 (180, 37)  
Jan.  8  18 53.91   89 12.9   3.410   3.880   111   16.1   5:38 (181, 35)  

* A/2021 F1

Now it is bright as 15.4 mag (Jan. 8, Ken-ichi Kadota. Cometary activity was detected. 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)  
Jan.  1  16  0.56   33 11.6   1.946   1.830    68   16.4   5:37 (256, 45)  
Jan.  8  16 26.84   36 10.9   1.802   1.745    70   16.1   5:38 (252, 46)  

* C/2020 H6 ( ATLAS )

Now it is 16.3 mag (Jan. 7, Toshihiko Ikemura, Hirohisa Sato). 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)  
Jan.  1  15 43.33   10  1.1   5.250   4.759    55   16.3   5:37 (286, 37)  
Jan.  8  15 48.91   11  3.0   5.173   4.768    60   16.2   5:38 (289, 42)  

* C/2021 P4 ( ATLAS )

Now it is 16.0 mag (Dec. 28, 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)  
Jan.  1  22 38.38   52 32.9   2.981   3.156    91   16.4  18:29 (135, 58)  
Jan.  8  22 43.78   51 52.9   2.968   3.078    87   16.2  18:34 (132, 54)  

* 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. It has already faded down to 16.8 mag (Jan. 8, Toshihiko Ikemura, Hirohisa Sato). 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)  
Jan.  1   7  3.13   40 16.2   1.027   1.986   162   16.5   0:23 (180, 85)  
Jan.  8   6 55.88   40 43.2   1.066   2.022   161   16.8  23:44 (180, 84)  

* 181P/Shoemaker-Levy 6

It has not been observed yet in this return. It will brighten up to 16.5 mag in January. It locates low in the evening.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  22  4.91  -18 52.2   1.592   1.164    46   16.7  18:29 ( 47, 21)  
Jan.  8  22 30.24  -15  0.8   1.590   1.160    46   16.6  18:34 ( 51, 22)  

* C/2020 F7 ( Lemmon )

Now it is 17.7 mag (Jan. 2, 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)  
Jan.  1   8 28.83  -44  0.5   4.945   5.344   108   16.7   1:48 (  0, 11)  
Jan.  8   8 19.50  -45  3.9   4.915   5.348   111   16.7   1:11 (  0, 10)  

* 254P/McNaught

Now it is 16.7 mag (Jan. 7, Toshihiko Ikemura, Hirohisa Sato). 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)  
Jan.  1   4 28.59  -13 47.6   3.204   3.913   130   16.7  21:44 (  0, 41)  
Jan.  8   4 25.74  -12 50.6   3.278   3.932   125   16.8  21:14 (  0, 42)  

* 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)  
Jan.  1  18 48.80   47 44.3   9.263   8.988    70   16.8  18:29 (134, 22)  
Jan.  8  18 52.61   48  7.1   9.274   8.996    70   16.8   5:38 (227, 25)  

* 52P/Harrington-Abell

Now it is 16.7 mag (Dec. 29, Ken-ichi Kadota). It stays observable at 17 mag from autumn to winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  12 32.38   -3 57.1   1.671   1.957    91   16.8   5:37 (355, 51)  
Jan.  8  12 39.70   -5 26.7   1.622   1.984    96   16.8   5:31 (  0, 49)  

* 430P/2021 Q2 ( Scotti )

First return of a new periodic comet which brightened up to 17 mag in 2011. Now it is 17.2 mag (Dec. 13, Catalina Sky Survey). It stays observable at 17 mag in good condition until spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  13 37.87   -5 32.1   1.507   1.581    75   16.9   5:37 (331, 45)  
Jan.  8  13 53.99   -7  3.8   1.469   1.595    78   16.9   5:38 (336, 45)  

* 10P/Tempel 2

It brightened up to 10.1 mag in spring (Apr. 10, Marco Goiato). Now it is fading. It has already faded down to 16.5 mag (Dec. 30, Ken-ichi Kadota). It stays observable in good condition for a long time after this while the comet will fading.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   3 46.32    7 12.9   2.074   2.850   134   17.0  21:02 (  0, 62)  
Jan.  8   3 44.36    7 49.7   2.185   2.889   127   17.2  20:33 (  0, 63)  

* 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)  
Jan.  1  23 23.66  -19  9.8   1.927   1.748    64   17.0  18:29 ( 30, 30)  
Jan.  8  23 38.27  -17  9.2   1.953   1.719    61   17.0  18:34 ( 35, 30)  

* C/2020 S4 ( PanSTARRS )

Now it is 16.7 mag (Jan. 8, 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)  
Jan.  1   4 24.30    3 14.0   4.160   4.961   140   17.1  21:40 (  0, 58)  
Jan.  8   4 21.87    3 36.8   4.183   4.918   134   17.0  21:10 (  0, 59)  

* 274P/Tombaugh-Tenagra

Now it is 17.4 mag (Dec. 23, ATLAS-HKO, Haleakala). 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)  
Jan.  1   5 33.50   27 19.9   1.594   2.552   163   17.1  22:49 (  0, 82)  
Jan.  8   5 28.17   28  3.2   1.613   2.539   155   17.1  22:16 (  0, 83)  

* 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 16.4 mag (Jan. 1, Toshihiko Ikemura, Hirohisa Sato). 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)  
Jan.  1   0  7.83  -10  2.2   2.428   2.418    77   17.1  18:29 ( 22, 43)  
Jan.  8   0 17.68   -8 50.9   2.524   2.433    73   17.2  18:34 ( 29, 42)  

* 193P/LINEAR-NEAT

It brightened up to 15.2 mag in autumn (Oct. 11, Purple Mountain Observatory, XuYi Station). Now it is fading very rapidly. It has already faded down to 19.0 mag (Jan. 3, Toshihiko Ikemura, Hirohisa Sato).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  23 54.82    8 58.7   2.279   2.358    82   17.1  18:29 ( 39, 59)  
Jan.  8   0  4.85    9 59.6   2.380   2.377    77   17.3  18:34 ( 48, 56)  

* C/2019 T2 ( Lemmon )

Now it is 16.4 mag (Oct. 4, ATLAS-MLO, Mauna Loa). 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)  
Jan.  1  11 50.27  -54 40.1   3.767   3.704    78   17.1   5:09 (  0,  0)  
Jan.  8  11 43.69  -54 51.4   3.723   3.751    84   17.2   4:35 (  0,  0)  

* 422P/2021 L1 ( Christensen )

First return of a new periodic comet which brightened up to 17 mag in 2006. Now it is 17.0 mag (Dec. 21, ATLAS-HKO, Haleakala). It stays 17 mag from 2021 to 2022. In the Southern Hemisphere, it stays observable in good condition for a while. It locates extremely low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  22 51.97  -37 35.5   3.575   3.106    54   17.2  18:29 ( 28, 11)  
Jan.  8  23  1.34  -35 32.4   3.637   3.105    50   17.2  18:34 ( 33, 10)  

* C/2019 T3 ( ATLAS )

Now it is 16.6 mag (Dec. 25, D. Buczynski). Fading slowly. It is not observable until April in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  21 40.55   18 30.9   6.755   6.318    59   17.2  18:29 ( 85, 41)  
Jan.  8  21 43.29   17 52.0   6.861   6.334    54   17.2  18:34 ( 89, 34)  

* C/2022 A1 ( Sarneczky )

Now it is 16.8 mag (Jan. 6, Michael Jager). Now it is approaching to Earth down to 0.3 a.u. and it brightened up to 17 mag. But it will fade out quickly.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   9 26.92   38 26.7   0.414   1.335   142   17.8   2:51 (180, 87)  
Jan.  8   6 54.21   27 20.6   0.321   1.302   173   17.2  23:29 (  0, 81)  

* 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)  
Jan.  1   3 13.39   31 11.6   4.686   5.402   132   17.2  20:29 (  0, 86)  
Jan.  8   3  5.42   30 31.3   4.782   5.395   124   17.3  19:54 (  0, 86)  

* C/2020 F2 ( ATLAS )

Now it is 17.2 mag (Jan. 7, Toshihiko Ikemura, Hirohisa Sato). 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)  
Jan.  1  14 38.99   -5 27.4   9.316   8.890    61   17.3   5:37 (314, 38)  
Jan.  8  14 39.19   -5 15.7   9.196   8.885    68   17.3   5:38 (321, 42)  

* 81P/Wild 2

Now it is 17.4 mag (Jan. 7, Toshihiko Ikemura, Hirohisa Sato). 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)  
Jan.  1   2 59.57   12 53.5   2.590   3.265   125   17.4  20:16 (  0, 68)  
Jan.  8   2 57.82   12 54.7   2.643   3.228   118   17.3  19:47 (  0, 68)  

* 119P/Parker-Hartley

Now it is 16.8 mag (Jan. 1, Toshihiko Ikemura, Hirohisa Sato). It will brighten up to 15 mag in 2022 winter. It will be unobservable in February.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  23  8.95  -12 32.5   3.066   2.768    63   17.4  18:29 ( 37, 34)  
Jan.  8  23 17.57  -11 29.5   3.126   2.745    58   17.4  18:34 ( 44, 32)  

* C/2021 D2 ( ZTF )

Now it is 17.6 mag (Dec. 11, Toshihiko Ikemura, Hirohisa Sato). 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)  
Jan.  1  16 30.66   70 27.1   2.690   2.966    96   17.4   5:37 (204, 42)  
Jan.  8  16 36.34   72 55.0   2.643   2.959    98   17.4   5:38 (200, 43)  

* C/2018 N2 ( ASASSN )

Now it is 17.7 mag (Jan. 1, Toshihiko Ikemura, Hirohisa Sato). 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)  
Jan.  1  14 50.31   41 21.3   7.494   7.459    84   17.5   5:37 (247, 60)  
Jan.  8  14 52.07   41 41.5   7.472   7.506    88   17.5   5:38 (245, 65)  

* C/2021 U5 ( Catalina )

Now it is 16.9 mag (Jan. 2, J. Drummond). It is observable at 17 mag in good condition from winter to spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  10 11.81  -28 22.7   1.884   2.384   108   17.6   3:31 (  0, 27)  
Jan.  8  10 15.70  -28 29.4   1.811   2.376   113   17.5   3:07 (  0, 26)  

* 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)  
Jan.  1  13 30.21   -8 11.8   4.856   4.722    76   17.6   5:37 (335, 44)  
Jan.  8  13 33.89   -8 35.1   4.747   4.720    82   17.6   5:38 (344, 45)  

* P/1997 B1 ( Kobayashi )

First return of a new periodic comet which brightened up to 16.5 mag in 1997. Now it is 19.4 mag (Jan. 11, Purple Mountain Observatory, XuYi Station), fainter than this ephemeris by 2 mag. It is observable in good condition from January to March.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   8 57.85   28 52.9   1.340   2.244   149   17.7   2:17 (  0, 84)  
Jan.  8   8 55.88   28 32.0   1.279   2.216   156   17.6   1:48 (  0, 83)  

* P/2021 Q5 ( ATLAS )

It brightened up to 12.7 mag in autumn (Oct. 9, Thomas Lehmann). It stays observable in good condition for a long time. But it is fading rapidly, and it will be fainter than 18 mag in January.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  11 17.78  -11 32.4   1.358   1.869   104   17.6   4:37 (  0, 43)  
Jan.  8  11 18.63  -12 27.0   1.336   1.922   111   17.8   4:10 (  0, 42)  

* 15P/Finlay

It brightened very rapidly up to 10.7 mag in July (July 20, Osamu Miyazaki). Now it is fading. It has already faded down to 18.1 mag (Jan. 1, Toshihiko Ikemura, Hirohisa Sato).

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   8 33.29   30 19.8   1.400   2.327   154   17.6   1:53 (  0, 85)  
Jan.  8   8 22.65   30 53.2   1.431   2.388   162   17.8   1:15 (  0, 86)  

* C/2019 N1 ( ATLAS )

It brightened up to 11.6 mag in last winter (Feb. 18, Thomas Lehmann). Now it is fading. It has already faded down to 16.6 mag (Nov. 23, Thomas Lehmann). In the Southern Hemisphere, it stays observable in good condition after this. In the Northern Hemisphere, it will never be observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   1  5.49  -56 16.7   4.975   4.794    73   17.6  18:29 (  1, -1)  
Jan.  8   1  5.11  -54 30.9   5.095   4.857    70   17.7  18:34 (  6,  0)  

* 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)  
Jan.  1   1 18.28   16 59.4   2.122   2.546   104   17.7  18:35 (  0, 72)  
Jan.  8   1 13.47   14  7.0   2.182   2.469    94   17.6  18:34 ( 21, 68)  

* 28P/Neujmin 1

Now it is 17.2 mag (Jan. 7, Toshihiko Ikemura, Hirohisa Sato). In the Northern Hemisphere, it stays observable in good condition after this while the comet will be fading. In the Southern Hemisphere, it stays locating extremely low for a long time.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   4 17.57   40 44.3   2.622   3.470   144   17.6  21:34 (180, 84)  
Jan.  8   4 14.14   40  5.7   2.732   3.524   137   17.8  21:03 (180, 85)  

* C/2021 K1 ( ATLAS )

Now it is 17.5 mag (Jan. 3, Toshihiko Ikemura, Hirohisa Sato). It continued brightening even after the perihelion passage. But it will be fading after this, and it will be fainter than 18 mag in January.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   1 10.19  -10  0.2   3.196   3.374    91   17.7  18:29 (  1, 45)  
Jan.  8   1 15.17   -9  5.8   3.332   3.416    86   17.9  18:34 ( 10, 46)  

* 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)  
Jan.  1  15 40.12  -33  5.0   6.393   5.695    41   17.7   5:37 (319,  7)  
Jan.  8  15 41.35  -33 48.0   6.336   5.726    48   17.7   5:38 (324, 10)  

* 241P/LINEAR

Now it is 17.6 mag (Jan. 3, Toshihiko Ikemura, Hirohisa Sato). It will be fainter than 18 mag in January.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   9  7.86   19 29.5   1.545   2.426   146   17.7   2:27 (  0, 74)  
Jan.  8   9  1.20   18 48.3   1.537   2.464   155   17.8   1:53 (  0, 74)  

* 2021 WT6

Peculiar asteroid moving along a cometary orbit. It is observable at 17.5 mag in good condition in January.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   7 14.99   -3 38.5   1.077   2.000   152   17.9   0:36 (  0, 51)  
Jan.  8   6 33.36    0 46.9   1.023   1.963   156   17.7  23:18 (  0, 56)  

* (3200) Phaethon

In the Northern Hemisphere, it stays observable at 17 mag in good condition from November to December. It locates low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   1 50.78   25 44.1   1.400   2.011   113   17.7  19:07 (  0, 81)  
Jan.  8   1 46.57   24  0.8   1.456   1.964   105   17.8  18:35 (  0, 79)  

* C/2021 Y1 ( ATLAS )

Now it is 17.5 mag (Jan. 1, H. Nohara). 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)  
Jan.  1   1 22.04   55  7.0   5.001   5.476   114   17.9  18:39 (180, 70)  
Jan.  8   1 22.76   53 45.0   5.019   5.418   108   17.8  18:34 (170, 71)  

* P/2020 V4 ( Rankin )

Now it is 17.5 mag (Jan. 3, Toshihiko Ikemura, Hirohisa Sato). It is observable at 18 mag in good condition in winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   7 59.84    2 59.4   4.323   5.218   152   17.9   1:19 (  0, 58)  
Jan.  8   7 56.92    3  1.9   4.297   5.223   158   17.9   0:49 (  0, 58)  

* C/2021 G2 ( ATLAS )

Now it is 17.4 mag (Jan. 2, J. Drummond). It will brighten up to 14 mag from 2024 to 2025.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1   7 30.23  -31 44.4   8.088   8.678   124   17.9   0:50 (  0, 23)  
Jan.  8   7 27.59  -31 52.9   8.029   8.641   125   17.9   0:19 (  0, 23)  

* C/2019 K7 ( Smith )

Now it is 17.4 mag (Jan. 8, Toshihiko Ikemura, Hirohisa Sato). Fading slowly. In the Northern Hemisphere, it stays observable in good condition for a long time. It is not observable after this in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Jan.  1  16 55.71   50  8.4   6.439   6.292    77   17.9   5:37 (230, 39)  
Jan.  8  16 59.06   50 57.2   6.439   6.329    79   18.0   5:38 (230, 43)  

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