Comet Chasing in November

Comet chasing is the visual observation of telescopic comets.  Jump to:  Observing synopses    Summary data    Buy me a Coffee 

There is only one comet that is generally observable in telescopes with apertures less than 8-inches (25 cm). But this comet is visible in binoculars and has a nice tail. See the Observing Synopses for which comets are visible from your latitude, the best dates and the time of night.

• C/2023 A3 (Tsuchinshan-ATLAS) was very impressive in October. Although forgotten by the media, it remains a very nice binocular and telescopic comet throughout the month. If this was as good as it would get, we would still be celebrating it. See below for observing details, as well as the video above. 

• C/2024 S1 (ATLAS) has disintegrated near the sun. Despite all the talk, there was little chance that this comet was ever going to be more than a SOHO comet. Beware that some software and web sites may still show it as active. 

• C/2022 E2 (ATLAS) is past perihelion, which occurred in mid September 2024. It is predicted to reach maximum brightness of magnitude 12.8 in early December.

• C/2024 G3 (ATLAS)  will reach perihelion on January 13 2025, when it will pass within 0.1 AU of the sun. This may be an interesting comet to follow in the coming months, as it is too soon to predict how bright it will get, and there is a possibility that it will disintegrate. Most intriguingly, it brightened by a magnitude at the end of October, heightening the uncertainty. 

• C/2023 C2 (ATLAS) will reach perihelion in mid November. It was at maximum brightness in October.

• Comet 13P/Olbers passed perihelion in late June and is fading.

• Comet 12P/Pons-Brooks passed perihelion on April 21 and has become a southern-hemisphere object. It is fading.This well-documented comet, perhaps observed as early as the year 245, experienced a large unexpected outburst in late July 2023, catapulting from a magnitude of 16.6 to 11.6 in a single day. Afterward it displayed an unusual coma shape, characterized by a distinctive 'notch' and a pair of 'horns' that persisted for weeks. The same pattern repeated in the following months, except in recent outbursts the 'horns' have become longer and curved.  Here is a link to a video with an animation of the July outburst aftermath C/2021 S3 (PANSTARRS) passed perihelion in mid February 2024. 

• 29P/Schwassmann-Wachmann has frequent outbursts, typically resulting in a brightening of 0.5 - 1.0 magnitudes, which occur roughly every 59 days, typically taking 5-10 days to subside. Up to three subsequent outbursts may occur 5-10 days afterward, each typically smaller than the last, although on some occasions they can be even brighter than the first. These outbursts make 29P one of the most interesting comets to follow, both visually and scientifically. 29P/Schwassmann-Wachmann has a 14.8-year orbital period, and last passed perihelion in early March 2019. It varies in its distance from the Sun from 5.8 AU (at perihelion) to 6.3 AU (at aphelion), which is an unusually small variation for a comet, and remains quite far from the sun at all times. This means that it can be observed more or less continuously.

• C/2014 UN271 (Bernardinelli-Bernstein) is an interesting Oort cloud comet that was reported as a result of the Dark Energy Survey. Soon after it was made public, images showed a cometary coma. Discovery credit goes to Pedro Bernardinelli and Gary Bernstein. This is a remarkable comet that was at 29 AU in 2014, with a perihelion of 10.9 AU in 2031. Its orbit extends out to 40,000 AU! It was unusually bright for its distance. HST observations that isolate the nucleus estimate the diameter to be between 120 and 140 km, making this possibly the largest comet nucleus yet measured. Because of its distant perihelion, this comet is not expected to become bright enough to be visually observed except in large instruments, and not until the end of the decade, but it is likely going to be the subject of intense scientific scrutiny. 

Comets that have apparently disintegrated: C/2024 S1 (ATLAS), C/2022 S3 (PANSTARRS), C/2021 P4 (ATLAS), C/2020 Q1 (Borisov), C/2020 P1 (NEOWISE), and C/2019 Y4 (ATLAS). Beware that various other sources often fail to keep track of whether or not a comet still exists!

Comet Visibility in the Eyepiece

This page uses code developed for SkyTools to predict the visibility of a comet in the eyepiece.  Predicting how much aperture is required to see a comet is a very complex task.  Have a look for yourself: a comparison of the predictions below (such as "visible in small telescopes") to the magnitude of each comet shows just how poor an indicator the magnitude alone really is. When you read below that a particular aperture is required to see a comet you can have a reasonable degree of confidence that the comet can in fact be seen in the eyepiece. But always remember, comets are like cats. They both have tails and do what they want, and not always what we expect. This is one of the things that makes comet chasing interesting! The predictions are made for a Country/Suburban site, which is Bortle 5, unless indicated otherwise.

Observing Synopses for November