British Astronomical Association

Comet Section

Director: Nick James

Visual observations page

(Co-ordinator Jonathan Shanklin)

Latest Discoveries and news

Apr 13  Zhijian Xu reports a Kreutz group comet in real time C2 images
Apr 17  Discovery of 2024 G1 (Wierzchos) reported
Apr 17  Discovery of 2024 G2 (ATLAS) reported
Apr 18  Discovery of 2024 G3 (ATLAS) reported
Apr 18  Possible comet detected by Shigeki Murakami
Apr 23  2006 AH2 linked to 2022 U6 (P/Sheppard-Tholen)
Apr 24  Zhijian Xu reports a Kreutz group comet in real time C3 images
Apr 30  Hanjie Tan reports a Kreutz group comet in real time C2 images
Apr 30  Worachate Boonplod reports a Kreutz group comet in real time C3 images
May 02  Jiangao Ruan reports a Kreutz group comet in real time C2 images
May 05  Hanjie Tan reports a Kreutz group comet in real time C2 images
May 06  Hanjie Tan reports two Kreutz group comets in real time C2 images
May 08  Discovery of 2024 G4 (PANSTARRS) reported
May 08  Discovery of 2024 G5 (Leonard) reported
May 08  Discovery of 2024 J1 (P/PANSTARRS) reported
May 08  Discovery of 2024 G6 (ATLAS) reported
May 10  Update

If there have been no recent updates try The German comet group page or Seiichi Yoshida's page for information or the Liga Iberoamericana de Astronomia for observations.

Elsewhere on these pages: Highlights / Newly discovered comets / Periodic comets / Contributing observations / Comet Ephemerides / Upcoming Comets / Observing Comets / Links / Meetings / Publications / Comments and Contacts / Old 2024 News / Comet discovery procedure / Weather information / The Comet's Tale / BAA Comet Section image archive / Project Alcock / More information / Legacy page / Main BAA Comet Section page

Current comet magnitudes, and observable region for 2024 May

Comet	                  Magnitude   Trend     Observable     When visible        Last visual observation
12P/Pons-Brooks                5      fade      10 N to 75 S   early evening       2024 May
13P/Olbers                     8.5    bright    55 N to 15 S   early evening       2024 May
2023 A3 (Tsuchinshan-ATLAS)   10.5    bright    60 N to 75 S   best evening        2024 May
2021 S3 (PANSTARRS)           10.5    fade      60 N to 25 S   best morning        2024 May
154P/Brewington               11 ?    bright    Poor elongation                    Not yet observed
479P/Elenin                   11.5    steady    40 N to 80 S   evening             2024 May
29P/Schwassmann-Wachmann      13 ?    varies    55 N to 40 S   evening             2024 April
2021 G2 (ATLAS)               13.5    steady    30 N to 90 S   best evening        2024 April
2022 E2 (ATLAS)               13.5    fade      55 N to 15 S   early evening       2024 May
2017 K2 (PanSTARRS)           13.5    fade      Poor elongation                    2024 April
2020 V2 (ZTF)                 13.5    fade      20 S to 90 S   early morning       2024 March
2022 L2 (ATLAS)               14      steady    25 N to 90 S   best evening        2024 April
Details are usually fully updated at the beginning of each month, but some minor updates may be made more frequently, particularly for brighter comets. The last (partial) update was on May 7. The magnitude is a rough value for the mean magnitude reported; some observers will see the comet brighter than this, whilst others will see it fainter. The observable region is an approximate indication of the latitude at which the comet may be seen. Under good conditions comets may be visible outside this range. The period when visible is for the UK if the comet is visible from the UK, otherwise for 30 S or the Equator as appropriate. The last visual observation is as received by the Section, details are often updated on the basis of observations published elsewhere. Beginners will often find comets fainter than about 7th magnitude difficult to locate - see below for information on positions and finder charts.

Highlights and News  

  1. 13P continues to brighten rapidly, but the rate has slowed. It is likely to be an easy binocular, reaching 5th magnitude at the end of June. The solar elongation continues to decrease until early June, so the comet will be quite difficult. As it nears its brightest the elongation increases.
  2. Comet 2023 A3 is still over 2 au from the Sun. The comet is on track to be a bright object, perhaps reaching -1 magnitude at perihelion, though there is a long time to go. The rate of brightening has decreased slightly. UK observers will loose it for a while from mid June.
  3. 12P/Pons-Brooks is now too far south for observation from the UK and has begun to fade.
  4. Guy Hurst is currently ill and unable to receive visual observations for TA. Could any TA observers who normally email their visual observations to Guy, send them to me instead, or alternatively submit them directly to COBS if you don't already.  I normally extract observations from COBS for TA from observers who are affiliated (broadly) to the BAA group, or have notified me that their observations can be used by the BAA.
  5. Newly discovered 2024 E1 may reach 5th magnitude at perihelion in 2026 January, when it will be visible in the SOHO C3 field.
  6. The lack of communication and collaboration between the MPC and CBAT has led to two different comets being given the designation of 2023 X5. Adding further to the confusion the MPC have retracted their designation, making it unclear whether a comet has been recovered or not. Further confusion has arisen with the designation of 2021 K5-B.
  7. There was a BAA Comet Section meeting in London on 2023 July 8.  Talks were recorded and are now available for viewing.
  8. The Section welcomes observations from all comet enthusiasts, whether members of the BAA or not.  An advantage of joining the BAA is that you can read papers on comets published in the BAA Journal.  The 2023 June Journal included a paper on "BAA comet observations: magnitude parameters".  Further papers in "The brighter comets of" series are in press (2020, 2021). 2022 has been submitted.  Best wishes go to our colleagues in the Ukraine.


Comet ephemerides (positions) etc

For positions of newly discovered comets see the NEO confirmation page . You can also generate your own ephemerides and elements at the CBAT Minor Planet and Comet Ephemeris Service web page.  The elements and ephemerides from the JPL Small-Body Database Browser give estimates of the errors, which are often far larger than might be thought from the accuracy of the elements given by the CBAT.  Seiichi Yoshida has pages for currently visible comets, which include finder charts. Seiichi also has a comet rendezvous page, which lists conjunctions between comets, variable stars and nebulae and a comet recovery page, which lists periodic comets not yet recovered at the present return. The T3 project aims to discover comets amongst the population of asteroids influenced by Jupiter. 

Planning aids and information for forthcoming comets, valid out to about 2025.

  • Comets reaching within three degrees of 180° opposition [updated 2013 December 31]
  • Comets reaching within three degrees of zero phase angle [updated 2013 December 31]

The MPC also has a list of the last observation for all comets.  Electronic observers should try and observe any comets that have not recently been observed according to the CBAT but which are expected to be within range of their equipment. Negative observations are also useful.  In addition, the MPC has orbital elements for unusual asteroids, many of which have cometary orbits. 

Finder charts

The BAA Computing Section has online charts for the comets listed here. There are daily finder charts for bright comets at Heavens Above. Reinder Bouma and Edwin van Dijk's astrosite Groningen has an excellent set of finder charts for brighter comets, which also show suitable comparison stars.

Orbits etc

The elements and ephemerides from the JPL Small-Body Database Browser give estimates of the errors, which are often far larger than might be thought from the accuracy of the elements given by the CBAT.   Full details of the latest orbits were available from Kazuo Kinoshita's Comet Orbit Home Page (Kazuo died in 2021 July and his web page hadn't been updated since 2020 February).  I compile orbital elements in Megastar format for: numbered periodic comets , recent comets (updated 2024 April 4) and comets prior to 2006.  Most of the more recent elements include the latest magnitude parameters.  The elements are from a mix of CBAT catalogues, MPC, MPEC, JPL and individual orbit computers.  Older elements are for the epoch of perihelion, but most recent elements from the MPEC are for epoch of date.

Downloads etc

Download Richard Fleet's GraphDark software for graphically displaying comet (and other object) visibility. Latest version is 2.05, 2007 May.

Download William Schwittek's CometWin software for generating comet ephemerides and visibility diagrams. [Updated 2002 March 5]

Download Solex, N-body solar system dynamics software.

Upcoming comets

Predictions for the comets expected to return in 2023 [Updated to 2023 January 1], 2024 [Final edition 2024 February 22] , 2025 [Updated 2024 January 17] and 2026 [Created 2024 January 17] are published in the BAA Journal in December each year. This list [Updated 2024 March 7] gives the period of visibility and maximum brightness for comets that are predicted to be brighter than 12th magnitude within the next few years. A few are listed further into the future. Seiichi Yoshida also has a list of comets likely to be visible in the next five years.

Contributing observations

Observations may  be used in the reports on comets which appear on these pages, in The Comet's Tale and in the BAA Journal. Guidance on observing is given in the BAA Comet Observing Guide

Thanks to the many observers who do send in their observations in ICQ format.  Imagers are encouraged to reduce their observations to equivalent visual magnitude (see Project Alcock ) and submit them in this format.  Do check the observation files to see if what you sent matches what is there, as I still have to edit some of the submitted records, particularly the position of "m" when tail length is given in minutes, the focal ratio and the designation of periodic comets 1-99.  If your observations are missing it may be because you have not used the correct format, which includes ICQ as a key.  If you use the Comet Observation Database to enter your observations they will be formatted correctly. I extract all the observations from observers who are affiliated to the BAA on a monthly basis for publication in TA, but other observers will need to send them to me. Observers providing VEMs are reminded that they should report a coma diameter to go with the magnitude.

Visual and visual equivalent magnitude observations should be sent to me at <jds [at]> in simple text format.  Visual observers can use the BAA visual report form to log observations.  To avoid the use of multiple formats the ICQ format , which uses special keys to code observation particulars, is now standardised as the one to use for submission and archiving of observations.  The ICQ have not updated their observation keys since 2010, so these additional keys are suggested for use when submitting observations to the BAA (updated 2020 October 3).  Crni Vhr Observatory has launched the Comet Observation Database which allows entry of observations in ICQ format, and plots of light curves.  Visual observations entered using this system should be emailed to me at the end of the month.  Observations are usually analysed and sent to TA as soon as possible after the end of the month with a TA deadline of the 2nd; any late observations will be used in subsequent analyses.  Observations will continue to be published by Guy Hurst in The Astronomer magazine in TA format. There is also a visual drawing form.   The German comet group also has a computer program that will correctly format observations for the ICQ [2009 December]. 

Images should be sent to Denis Buczynski.

Regular contributors include James Abbott, Jose Aguiar, Alexander Amorim, Nicolas Biver, Denis Buczynski, Paul Camilleri, Peter Carson, Matyas Csukas, Roger Dymock, John Fletcher, Marco Goiato, Juan Gonzalez, Bjorn Granslo, Werner Hasubick, Kevin Hills, Nick James, Heinz Kerner, Carlos Labordena, Rolando Ligustri, Michael Mattiazzo, Maik Mayer, Antonio Milani, Martin Mobberley, Giuseppe Pappa, Jose Navarro Pina, Gabriel Oksa, Mieczyslaw  Paradowski, Nirmal Paul, Stuart Rae, Walter Robledo, Tony Scarmato, Willian Souza, David Strange, Johan Warrell, Chris Wyatt and Seiichi Yoshida, several of whom contribute observations from their colleagues.  Thanks are due to all of them.

Warning I receive a large number of emails containing viruses or other junk. Please try and make clear that your message is legitimate, otherwise it may be deleted without being read. It is advisable to use your own name, rather than an alias, in the 'from' field and use an obvious, recent subject.

Comments and contact

Many thanks to those that regularly access this page for your interest. If you have any comments, suggestions for improvement or find any problems, please email the visual co-ordinator, Jon Shanklin, at j.shanklin @ If you need to phone me, my home number is +44 (0)1223 571250 or my BAS number is +44 (0)1223 221482. Snail mail will reach me at the British Antarctic Survey, Madingley Road, CAMBRIDGE CB3 0ET, England. For information about my work with BAS see my web page at BAS There is a small piece of Antarctica named as Shanklin Glacier.  See also this BBC report. Exploration of icy parts of the world clearly runs in the blood as my great-grandfather kept diaries which record the passage of a comet below the Plough, the discovery of a comet by his brother, Bernard Thomas, from Tasmania and the expeditions to Antarctica by Scott and Shackleton.   A write up of my George Alcock lecture, which tells a little of the Antarctic story was published in the 2021 October BAA Journal.

Published by