Weekly Information about Bright Comets (2026 Mar. 21: North)

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Updated on March 23, 2026
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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/2026 A1 ( MAPS )

Kreutz sungrazer comet discovered furthest from Sun in history. It will approach to Sun down to 0.005 a.u. on Apr. 4. Now it is 10.1 mag (Mar. 21, Carlos Labordena). It is expected to brighten up to 0-1 mag when observable on the ground. Its brightness evolution is somewhat getting down recently.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   2  9.80   -6 21.7   1.196   0.651    32    8.5  19:36 ( 80,  4)  
Mar. 28   1 48.80   -1 47.7   1.141   0.420    21    6.5  19:42 ( 91, -4)  

* C/2025 R3 ( PanSTARRS )

It became brighter than expected. It is expected to brighten up to 4 mag in April. Now it is 8.9 mag (Mar. 17, Carlos Labordena). It brightens up to 4 mag, but it will turn to fade out rapidly after that. In the Northern Hemisphere, it will be unobservable in April. In the Southern Hemisphere, it is not observable now, but it will appear in April. At the high light, it is observable in the low sky before the perihelion passage in the Northern Hemisphere, or after the perihelion in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  22 32.91   19  1.0   1.576   0.848    28    8.8   4:38 (254, 10)  
Mar. 28  22 38.57   19 28.9   1.376   0.732    31    7.8   4:28 (255, 13)  

* 88P/Howell

Now it is 9.9 mag (Mar. 17, Mike Olason). Fading gradually. It stays extremely low in the Northern Hemisphere. But it will become high in summer. It locates somewhat low in the Southern Hemisphere. But it will become high in summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  21 38.73  -16 44.7   1.985   1.358    38    9.7   4:38 (291,  1)  
Mar. 28  22  2.53  -14 52.5   1.973   1.361    39    9.6   4:28 (289,  1)  

* C/2024 E1 ( Wierzchos )

It brightened up to 6.6 mag in January (Jan. 28, Chris Wyatt). Now it is 10.6 mag (Mar. 15, Chris Wyatt). Fading rapidly. It will be unobservable in June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   4  6.41    5 12.7   1.477   1.334    61    9.9  19:36 ( 70, 35)  
Mar. 28   4 27.31    9 51.5   1.648   1.445    60   10.4  19:42 ( 77, 35)  

* C/2025 A6 ( Lemmon )

It brightened up to 3.7 mag in late October (Oct. 26, Juan Jose Gonzalez). Now it is 11.3 mag (Mar. 15, Chris Wyatt). It will fade out rapidly after this. In the Northern Hemisphere, it is not observable now, but it will appear in April. In the Southern Hemisphere, it stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  14 15.54  -65 17.7   1.899   2.431   110   11.2   2:26 (  0,-10)  
Mar. 28  13 28.41  -64 52.8   1.914   2.527   116   11.4   1:11 (  0,-10)  

* 24P/Schaumasse

It brightened up to 8.4 mag in January (Jan. 14, Mitsunori Tsumura). Now it is 11.4 mag (Mar. 14, Ken Harikae). Fading rapidly. It will be fainter than 18 mag in June. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  15 26.80    5  8.2   0.665   1.501   128   12.1   3:34 (  0, 60)  
Mar. 28  15 22.21    4 45.1   0.678   1.554   135   12.6   3:02 (  0, 60)  

* 235P/LINEAR

It became brighter than expected. Now it is 13.9 mag (Mar. 14, Ken Harikae). Fading gradually. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  16 59.26  -16 40.5   1.612   2.097   104   13.3   4:38 (351, 38)  
Mar. 28  17  6.00  -16  2.0   1.557   2.115   109   13.4   4:28 (354, 39)  

* 78P/Gehrels 2

It will brighten up to 12 mag in summer. Now it is 14.5 mag (Jan. 16, Kunihiro Shima). Brightening slowly. Now it is not observable. It will appear in May in the Southern Hemisphere, or in June in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   0  9.53    3  3.0   3.145   2.152     3   13.5  19:36 (105,-14)  
Mar. 28   0 24.34    4 27.0   3.130   2.133     1   13.4   4:28 (252,-17)  

* 240P/NEAT

It brightened up to 11.1 mag in winter (Nov. 15, Masayoshi Yoshimi). The component B also brightened rapidly up to 13.8 mag (Ded. 8, Masayoshi Yoshimi). Now it is 13.8 mag (Mar. 5, Thomas Lehmann). Fading gradually. In the Northern Hemisphere, it will be getting lower gradually. In the Southern Hemisphere, it will be unobservable in June.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   4 41.44   32  0.0   2.309   2.239    73   13.5  19:36 ( 98, 55)  
Mar. 28   4 54.99   32 52.3   2.402   2.256    69   13.7  19:42 (101, 51)  

* 29P/Schwassmann-Wachmann 1

Now it is 11.5 mag (Mar. 15, Chris Wyatt). It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  11 12.00   -2 28.9   5.335   6.312   167   13.6  23:16 (  0, 52)  
Mar. 28  11  9.14   -2 12.6   5.361   6.312   160   13.6  22:46 (  0, 53)  

* C/2024 J3 ( ATLAS )

Now it is 14.6 mag (Mar. 10, Ken-ichi Kadota). Brightening slowly. In the Northern Hemisphere, it stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  20 10.07    8 46.0   4.873   4.426    57   14.1   4:38 (284, 34)  
Mar. 28  20 13.59   10 24.4   4.760   4.397    62   14.0   4:28 (285, 37)  

* C/2024 T5 ( ATLAS )

Now it is 14.5 mag (Mar. 14, Andrew Pearce). It stays 14 mag for a while. In the Northern Hemisphere, it will be unobservable soon. It locates somewhat low in the Southern Hemisphere. But it will become high in summer. It is expected to brighten up to 11 mag in next winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   3  4.70  -26 39.2   5.758   5.201    51   14.3  19:36 ( 55,  2)  
Mar. 28   3 10.16  -25 26.7   5.765   5.163    48   14.3  19:42 ( 60, -2)  

* C/2026 B2 ( Sun-Gao )

Bright new comet discovered near Sun. It became brighter furthermore after the discovery, brightened up to 12.7 mag (Feb. 14, Mike Olason). Now it is 14.2 mag (Mar. 10, Ken-ichi Kadota). It will fade out rapidly after this. It will be fainter than 18 mag in June. It stays extremely low in the Northern Hemisphere. In the Southern Hemisphere, it will never be observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  22 39.25   31  2.6   2.328   1.638    36   14.3   4:38 (243, 16)  
Mar. 28  23  2.44   33  1.0   2.404   1.700    35   14.7   4:28 (240, 16)  

* C/2022 QE78 ( ATLAS )

Now it is 14.5 mag (Mar. 12, Purple Mountain Observatory, XuYi Station). It stays 15 mag for a while. In the Northern Hemisphere, it stays observable in good condition. In the Southern Hemisphere, it will be unobservable in July.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   9  1.95   31 26.8   4.989   5.651   127   14.5  21:07 (  0, 86)  
Mar. 28   9  1.55   31 41.3   5.089   5.663   120   14.6  20:39 (  0, 87)  

* C/2022 N2 ( PanSTARRS )

Now it is 14.7 mag (Mar. 12, Toru Yusa). It stays 15 mag for a while. It will be unobservable in May. But it will be observable again in July in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   4  0.49   25 17.7   4.684   4.327    63   14.7  19:36 ( 93, 44)  
Mar. 28   4  7.87   25 29.9   4.802   4.355    57   14.8  19:42 ( 96, 39)  

* C/2023 R1 ( PanSTARRS )

Now it is 14.6 mag (Mar. 6, ATLAS-MLO, Mauna Loa). It stays 14 mag for a while. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  19 33.20   -3 31.2   3.850   3.576    66   14.8   4:38 (302, 32)  
Mar. 28  19 30.96   -3 32.8   3.719   3.573    73   14.7   4:28 (306, 36)  

* C/2014 UN271 ( Bernardinelli-Bernstein )

Very large comet. It is expected to brighten up to 13 mag in 2031. Now it is 14.9 mag (Mar. 12, Andrew Pearce). It stays 15 mag for a while. In the Northern Hemisphere, it is not observable now. In the Southern Hemisphere, it stays observable in good condition. In the Northern Hemisphere, it is not observable until 2030.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   4 51.16  -71  2.0  14.214  14.153    84   14.8  19:36 ( 13,-20)  
Mar. 28   4 54.68  -70 38.4  14.179  14.131    85   14.8  19:42 ( 15,-21)  

* C/2021 G2 ( ATLAS )

Now it is 15.1 mag (Mar. 16, Andrew Pearce). It stays 15 mag for a while. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  17 29.63    7 24.4   6.304   6.510    97   14.8   4:38 (330, 59)  
Mar. 28  17 30.53    8 15.3   6.242   6.542   103   14.8   4:28 (337, 61)  

* 218P/LINEAR

Now it is 15.0 mag (Mar. 9, ATLAS-HKO, Haleakala). It will fade out rapidly after this. It will be fainter than 18 mag in June. It locates somewhat low in the Northern Hemisphere. In the Southern Hemisphere, it stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  20 11.82  -17 32.9   1.288   1.150    58   15.1   4:38 (306, 16)  
Mar. 28  20 37.70  -15 59.7   1.303   1.169    59   15.2   4:28 (303, 15)  

* 10P/Tempel 2

It is expected to brighten up to 8 mag in summer. Now it is 17.6 mag (Mar. 13, Roland Fichtl). Brightening rapidly. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  17 51.97  -10 49.6   1.638   1.946    91   15.8   4:38 (334, 40)  
Mar. 28  18  5.69  -10 35.7   1.530   1.904    95   15.3   4:28 (334, 41)  

* C/2025 Q3 ( ATLAS )

It became brighter than expected. Now it is 14.9 mag (Mar. 8, Martin Masek). Fading gradually. It will be fainter than 18 mag in July. It stays extremely low 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)  
Mar. 21   2 48.52  -22 34.7   2.685   2.130    46   15.4  19:36 ( 61,  2)  
Mar. 28   2 57.55  -23 29.3   2.723   2.143    45   15.4  19:42 ( 63, -3)  

* 93P/Lovas 1

Now it is 16.0 mag (Jan. 18, Kunihiro Shima). It stays 16 mag for a while. In the Northern Hemisphere, it will be unobservable soon. In the Southern Hemisphere, it is not observable now.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   1  0.78   13 13.7   2.648   1.746    20   15.8  19:36 (105,  2)  
Mar. 28   1 18.74   15 17.9   2.649   1.729    18   15.7  19:42 (109,  0)  

* C/2025 T1 ( ATLAS )

It brightened up to 9.0 mag from late November to early December (Nov. 22, Thomas Lehmann). Fading rapidly. It will be fainter than 18 mag in May. In the Northern Hemisphere, it will never be observable after this. In the Southern Hemisphere, it will be getting higher gradually.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  22 12.19  -22 32.8   2.732   1.994    34   15.8   4:38 (291, -9)  
Mar. 28  22 18.19  -24  9.8   2.721   2.075    41   16.2   4:28 (294, -8)  

* C/2024 R4 ( PanSTARRS )

It brightened rapidly. It is expected to brighten up to 13.5 mag from 2027 to 2028. Now it is 16.1 mag (Mar. 16, D. Buczynski). It stays 16 mag for a while. In the Northern Hemisphere, it will be getting higher gradually. In the Southern Hemisphere, it is not observable now, but it will appear in April.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  22  3.36   27  5.3   7.128   6.384    38   16.0   4:38 (250, 20)  
Mar. 28  22  5.88   28  1.3   7.056   6.347    41   16.0   4:28 (251, 24)  

* 141P/Machholz 2

The condition is very bad in this apparition. It is not observable at all. It brightens up to 13 mag, but it will turn to fade out rapidly after that. It will never be observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  23 19.90    3  5.1   1.928   0.966    10   16.7   4:38 (260, -8)  
Mar. 28  23 51.48    5 54.7   1.883   0.911     9   16.1   4:28 (256, -9)  

* C/2022 R6 ( PanSTARRS )

Now it is 16.3 mag (Mar. 14, ATLAS South Africa). It stays 17 mag for a while. In the Northern Hemisphere, it will be getting lower gradually after this, and it will be unobservable in June. In the Southern Hemisphere, it stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   8 30.19   -3 10.7   6.058   6.710   127   16.2  20:35 (  0, 52)  
Mar. 28   8 29.80   -2 19.0   6.150   6.720   121   16.2  20:07 (  0, 53)  

* 63P/Wild 1

Now it is 15.8 mag (Mar. 6, Thomas Lehmann). Brightening slowly. In the Northern Hemisphere, it stays 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)  
Mar. 21   6 28.57   42 21.2   1.908   2.232    95   16.5  19:36 (126, 76)  
Mar. 28   6 38.55   40 57.4   1.952   2.202    90   16.4  19:42 (116, 72)  

* C/2025 J1 ( Borisov )

Now it is 16.6 mag (Mar. 1, Ken-ichi Kadota). It stays 17 mag for a while. In the Northern Hemisphere, it will be getting lower gradually after this, and it will be unobservable in June. In the Southern Hemisphere, it is not observable now.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   4 57.53   52 36.5   3.687   3.658    80   16.5  19:36 (135, 58)  
Mar. 28   5  1.97   50 27.1   3.780   3.646    74   16.5  19:42 (129, 54)  

* 123P/West-Hartley

It will brighten up to 15 mag from autumn to winter. Now it is 17.4 mag (Mar. 9, ATLAS-MLO, Mauna Loa). Brightening slowly. It will be unobservable in May in the Southern Hemisphere, or in June in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   4 10.57   30 41.1   2.793   2.568    66   16.6  19:36 ( 99, 48)  
Mar. 28   4 21.44   31  8.9   2.848   2.541    62   16.5  19:42 (102, 44)  

* C/2024 G6 ( ATLAS )

Now it is 16.9 mag (Mar. 9, ATLAS South Africa). It stays 17 mag for a while. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  16 32.27    2 10.0   5.994   6.433   111   16.6   4:38 (359, 57)  
Mar. 28  16 29.56    3 16.9   5.895   6.434   118   16.5   4:10 (  0, 58)  

* 145P/Shoemaker-Levy 5

Now it is 16.1 mag (Mar. 7, Catalina Sky Survey). Fading slowly. It will be fainter than 18 mag in June. In the Northern Hemisphere, it will be unobservable in May. In the Southern Hemisphere, it will never be observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   2 23.09   19  0.0   2.597   1.941    39   16.6  19:36 ( 99, 22)  
Mar. 28   2 39.98   20 38.6   2.654   1.956    37   16.7  19:42 (103, 19)  

* 3I/2025 N1 ( ATLAS )

Third interstellar object in history following 1I/'Oumuamua and 2I/Borisov. The eccentricity is extremely big as 6. It approached to Sun down to 1.38 a.u. in late October. It brightened up to 8.9 mag in November (Nov. 12, Toshiyuki Takahashi). Now it is 16.5 mag (Mar. 12, Toru Yusa). Fading rapidly. It will be fainter than 18 mag in April. In the Northern Hemisphere, it will be getting lower gradually. It locates somewhat low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   6 48.71   20 22.0   4.963   5.251   101   16.7  19:36 ( 35, 73)  
Mar. 28   6 46.67   20 25.1   5.326   5.486    93   17.0  19:42 ( 55, 67)  

* (248590) 2006 CS

It seems to be a parent of the beta-Tucanids meteor shower. Fading gradually. It will be fainter than 18 mag in May. In the Northern Hemisphere, it stays observable in good condition. In the Southern Hemisphere, it will never be observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   2 53.26   18 41.8   0.158   0.895    46   17.4  19:36 ( 98, 29)  
Mar. 28   2 41.01   58 26.9   0.210   0.917    61   16.7  19:42 (144, 34)  

* C/2025 Y1 ( ATLAS )

Now it is 15.7 mag (Mar. 14, Hidenori Nohara). It stays 17 mag for a while. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  13  5.06    1 18.8   5.082   6.044   163   16.8   1:13 (  0, 56)  
Mar. 28  13  2.29    1 46.9   5.007   5.992   169   16.8   0:43 (  0, 57)  

* 493P/2024 Q2 ( LONEOS )

Now it is 16.3 mag (Mar. 14, Alfons Diepvens). It stays 17 mag for a while. It will be unobservable in April in the Southern Hemisphere, or in July in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   5  0.94   46 37.1   3.891   3.843    79   16.8  19:36 (124, 60)  
Mar. 28   5  9.65   46 10.4   3.985   3.848    74   16.9  19:42 (122, 56)  

* C/2025 L1 ( ATLAS )

It was expected to brighten up to 13.5 mag. But actually, it is getting diffuse and fading very rapidly. Now it is 17.4 mag (Mar. 10, Toru Yusa). It will fade out rapidly after this. It will be fainter than 18 mag in April. In the Northern Hemisphere, it stays observable in good condition. In the Southern Hemisphere, it will be getting lower gradually.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  15 13.79   17 28.6   1.104   1.898   129   16.8   3:22 (  0, 72)  
Mar. 28  14 52.74   26 46.1   1.112   1.941   133   17.1   2:34 (  0, 81)  

* C/2023 F3 ( ATLAS )

Now it is 16.5 mag (Mar. 9, ATLAS-HKO, Haleakala). Fading slowly. It will be fainter than 18 mag in July. In the Northern Hemisphere, it will be getting lower gradually after this, and it will be unobservable in June. In the Southern Hemisphere, it stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   9 24.53  -16 19.7   5.250   6.030   138   16.9  21:29 (  0, 39)  
Mar. 28   9 19.01  -15  5.7   5.338   6.056   132   17.0  20:56 (  0, 40)  

* C/2024 A1 ( ATLAS )

Now it is 17.2 mag (Mar. 7, Thomas Lehmann). Fading slowly. It will be fainter than 18 mag in June. In the Northern Hemisphere, it stays observable in good condition. In the Southern Hemisphere, it will never be observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   6 15.40   63 47.4   4.428   4.567    91   17.0  19:36 (164, 59)  
Mar. 28   6 13.94   63 41.7   4.555   4.599    86   17.1  19:42 (158, 57)  

* C/2023 X2 ( Lemmon )

Now it is 18.0 mag (Mar. 3, Erik Bryssinck). It stays 17 mag for a while. In the Northern Hemisphere, it stays observable in good condition. In the Southern Hemisphere, it will never be observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  21 36.37   82 51.3   5.131   5.127    84   17.1   4:38 (188, 36)  
Mar. 28  21 41.21   83 32.8   5.170   5.134    82   17.1   4:28 (188, 37)  

* 43P/Wolf-Harrington

Now it is 16.4 mag (Mar. 13, Andrew Pearce). Fading gradually. It will be fainter than 18 mag in May. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  10 45.15   -6 34.0   1.961   2.918   160   17.1  22:49 (  0, 48)  
Mar. 28  10 41.87   -5 51.0   2.013   2.943   153   17.2  22:19 (  0, 49)  

* C/2023 RS61 ( PanSTARRS )

It is around 20 mag usually. However, it brightened in outburst in 2025 autumn up to 17.0 mag (Sept. 4, Taras Prystavski). Now it is 17.3 mag (Mar. 6, ATLAS-HKO, Haleakala). It stays 17 mag for a while. In the Northern Hemisphere, it will be getting lower gradually after this, and it will be unobservable in May. But it will be observable again in June. In the Southern Hemisphere, it is not observable now, but it will appear in July.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   3  0.48   35 42.5   9.207   8.674    55   17.1  19:36 (112, 36)  
Mar. 28   3  4.19   35 47.5   9.283   8.665    49   17.1  19:42 (115, 30)  

* 40P/Vaisala 1

It became brighter than expected, brightened up to 14.3 mag (Jan. 21, Michael Jager). Now it is 17.2 mag (Mar. 13, Roland Fichtl). Fading slowly. It will be fainter than 18 mag in June. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  17 43.66  -10 38.7   1.916   2.221    94   17.1   4:38 (336, 41)  
Mar. 28  17 50.22  -10 22.1   1.873   2.258    99   17.2   4:28 (339, 42)  

* 164P/Christensen

Now it is 16.9 mag (Mar. 6, Thomas Lehmann). Fading gradually. It will be fainter than 18 mag in April. In the Northern Hemisphere, it stays 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)  
Mar. 21  10 39.37   32  2.1   2.169   3.023   142   17.2  22:44 (  0, 87)  
Mar. 28  10 35.01   31 55.0   2.259   3.062   136   17.4  22:12 (  0, 87)  

* 195P/Hill

Now it is 17.3 mag (Mar. 11, ATLAS Chile). It stays 18 mag for a while. It locates somewhat low in the Northern Hemisphere. In the Southern Hemisphere, it stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   9 21.34  -31 41.3   3.843   4.558   130   17.3  21:26 (  0, 23)  
Mar. 28   9 19.77  -30 52.9   3.883   4.565   127   17.3  20:57 (  0, 24)  

* C/2023 H5 ( Lemmon )

Now it is 17.3 mag (Feb. 28, D. Buczynski). It stays 18 mag for a while. In the Northern Hemisphere, it stays observable in good condition. In the Southern Hemisphere, it will never be observable after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  21 21.70   61 41.9   5.099   4.824    68   17.3   4:38 (215, 38)  
Mar. 28  21 31.72   61 57.3   5.144   4.850    67   17.3   4:28 (215, 39)  

* C/2025 E1 ( PanSTARRS )

Now it is 17.2 mag (Mar. 19, ATLAS Chile). It stays 17 mag for a while. In the Northern Hemisphere, it will never be observable after this. In the Southern Hemisphere, it stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  10  3.37  -68 52.2   3.885   4.304   108   17.5  22:06 (  0,-14)  
Mar. 28   9 44.41  -68 54.7   3.859   4.283   108   17.4  21:19 (  0,-14)  

* C/2024 G2 ( ATLAS )

Now it is 17.2 mag (Mar. 12, ATLAS South Africa). It stays 18 mag for a while. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  11 22.64    2 43.8   4.749   5.733   170   17.5  23:27 (  0, 58)  
Mar. 28  11 16.96    4  5.8   4.796   5.752   161   17.5  22:53 (  0, 59)  

* C/2024 G4 ( PanSTARRS )

Now it is 17.5 mag (Feb. 18, Kunihiro Shima). It stays 17 mag for a while. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  19 51.86    1 45.4   5.287   4.900    62   17.5   4:38 (294, 33)  
Mar. 28  19 57.14    2  5.1   5.203   4.901    67   17.5   4:28 (296, 35)  

* 210P/Christensen

It brightened up to 9.5 mag in late November (Nov. 28, Michael Jager, Gerald Rhemann, E. Prosperi). Now it is 16.7 mag (Mar. 2, Thomas Lehmann). It will fade out rapidly after this. It will be fainter than 18 mag soon. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  15 33.30   -3 22.0   1.223   1.985   126   17.8   3:41 (  0, 52)  
Mar. 28  15 23.55   -2 24.3   1.230   2.065   135   18.0   3:04 (  0, 52)  

* C/2020 V2 ( ZTF )

It was observed at 9-10 mag for a long time in 2023. It stays 18 mag for a while. In the Northern Hemisphere, it will never be observable after this. In the Southern Hemisphere, it stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  20 18.25  -66 24.2   9.794   9.617    76   17.8   4:38 (339,-20)  
Mar. 28  20 19.94  -66 50.1   9.758   9.665    81   17.8   4:28 (340,-20)  

* C/2024 L5 ( ATLAS )

Now it is 18.0 mag (Feb. 23, Catalina Sky Survey). Fading slowly. It will be fainter than 18 mag soon. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   9  9.77   15  1.1   4.095   4.854   135   17.9  21:14 (  0, 70)  
Mar. 28   9  2.59   15 47.2   4.237   4.897   126   18.0  20:39 (  0, 71)  

* C/2025 V2 ( Rankin )

It is expected to brighten up to 12.5 mag in 2027 spring. Now it is 17.1 mag (Mar. 11, Alfons Diepvens). It stays 17 mag for a while. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   9  5.78   20 33.0   3.761   4.496   132   17.9  21:10 (  0, 75)  
Mar. 28   9  3.39   21  8.6   3.786   4.436   125   17.9  20:41 (  0, 76)  

* C/2024 J4 ( Lemmon )

Now it is 17.5 mag (Mar. 14, ATLAS Chile). It stays 18 mag for a while. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  14 36.08    6 25.1   5.361   6.162   140   17.9   2:44 (  0, 61)  
Mar. 28  14 29.93    6 33.0   5.316   6.181   147   17.9   2:10 (  0, 61)  

* 124P/Mrkos

Now it is 17.6 mag (Feb. 25, Alfons Diepvens). It stays 18 mag for a while. In the Northern Hemisphere, it stays 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)  
Mar. 21   8  7.79   50 16.2   1.350   1.930   109   17.9  20:13 (180, 75)  
Mar. 28   8 10.86   47  6.9   1.378   1.904   105   17.9  19:49 (180, 78)  

* 242P/Spahr

Now it is 17.4 mag (Mar. 12, W. Hasubick). Fading slowly. It will be fainter than 18 mag soon. In the Northern Hemisphere, it will be getting lower gradually. In the Southern Hemisphere, it stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   7 29.88   -8 23.8   3.974   4.447   112   17.9  19:36 (  0, 47)  
Mar. 28   7 31.30   -7 27.8   4.071   4.460   106   18.0  19:42 ( 12, 47)  

* C/2025 A1 ( Lemmon )

Now it is 17.2 mag (Mar. 14, Alfons Diepvens). It stays 18 mag for a while. In the Northern Hemisphere, it stays observable in good condition. It stays extremely low in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21   8 22.38   37 52.4   5.434   5.957   117   17.9  20:28 (180, 87)  
Mar. 28   8 22.34   37 54.1   5.507   5.935   110   17.9  20:00 (180, 87)  

* 489P/Denning

It had been lost for 113 years. It must have passed the perihelion on Dec. 4. It brightened up to 18 mag in outburst in 2007. It will turn to fade out rapidly after the peak. It stays observable in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Mar. 21  13 14.60   -6 14.5   0.970   1.937   160   21.0   1:23 (  0, 49)  
Mar. 28  13  8.74   -6  4.6   0.991   1.980   168   20.9   0:50 (  0, 49)  

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