Perihelion: 2022 December 19.67, q = 1.797 AU
I’ve hinted in some of the earlier presentations of “Ice and Stone 2020” that, for the past few years, we have been in a slow period when it comes to bright comets. Indeed, for “Great Comets” – discussed in a previous “Special Topics” presentation – the most recent one appeared in 2011, and the most recent one that was easily visible from the northern hemisphere appeared as long ago as 1997. We’ve been teased a couple of times in the very recent past, but Comet ATLAS C/2019 Y4 (an earlier “Comet of the Week”) disintegrated as it approached perihelion, and while it was never expected to become “Great,” Comet SWAN C/2020 F8 (discussed in that same presentation) apparently did likewise. So far, Comet NEOWISE C/2020 F3 seems to be brightening normally, but we’ll have to wait and see what happens next month.
Intrinsically, this week’s “Comet of the Week” is one of the brightest ever detected – its intrinsic brightness being comparable to that of Comet Hale-Bopp C/1995 O1 – and while it certainly possesses the potential to become a bright, perhaps even conspicuous, naked-eye object around the time of its perihelion passage, its somewhat large perihelion distance, combined with the fact that it remains far from Earth and will be visible only under mediocre viewing geometry, will likely keep it from becoming “Great.” Furthermore, since it will be accessible only from the southern hemisphere for almost a full year around the time of perihelion, as far as observers in the northern hemisphere are concerned any potential it might have for becoming conspicuous is quite limited.
At the time of its discovery by the Pan-STARRS program based in Hawaii on May 21, 2017, the comet was about magnitude 19.5, and despite being located at a heliocentric distance of 16.1 AU was already clearly active. Researchers later identified images of it on exposures taken with the Canada-France-Hawaii Telescope at Mauna Kea as far back as May 12, 2013, at which time it was located 23.7 AU from the sun – the second-largest heliocentric distance at which any long-period comet has ever been detected; it was about magnitude 22.5 but was still showing activity even at that distance. Since this is far too large a distance for the sublimation of water ice, researchers have concluded that the activity was driven by sublimation of substances like carbon dioxide, carbon monoxide, and molecular oxygen and nitrogen.
Traveling in an orbit almost perpendicular to the ecliptic (inclination 87.5 degrees), Comet PANSTARRS has brightened steadily ever since its discovery as it has approached the inner solar system, and presently is around 15th to 16th magnitude. It is currently at opposition at a heliocentric distance of 8.9 AU, and located within the “head” of the constellation Draco. It travels slowly southward over the coming months, and will be in conjunction with the sun – 59 degrees north of it – in mid-December. A year from now it is again at opposition, when its heliocentric distance will be 6.1 AU and it will be located 10 degrees south of its current location; by then it may be close to 13th magnitude and thus amenable to visual observations. One year later, i.e., in mid-June 2022, it will once again be near opposition, at a heliocentric distance of 2.9 AU and located in northern Ophiuchus; by then it should be bright enough to detect with binoculars and perhaps may even be close to naked-eye visibility.
After this, Comet PANSTARRS travels southward more rapidly, becoming inaccessible from northern temperate latitudes by the end of September and entering southern circumpolar skies in mid-December. At the time of perihelion is in conjunction with the sun – 38 degrees south of it – and is located on the far side of the sun from Earth. It reaches a peak southerly declination of -71 degrees shortly before the end of January 2023, and is still in southern circumpolar skies when it is nearest Earth (2.23 AU) in mid-February. Although it continues traveling northward it remains at a relatively small elongation south of the sun for the next several months, and is again in conjunction with the sun – 37 degrees south of it – in mid-June. During August it emerges into the morning sky and once again becomes accessible from the northern hemisphere, and will be at opposition shortly after mid-December when it will be located a few degrees east of the Orion Nebula M42; during the first few days of January 2024 it travels northwestward parallel to the stars of Orion’s Belt about 1½ degrees south of that prominent stellar pattern. Visual observations may be possible for a few more months as it travels northward through the western evening sky and fades as it recedes from the earth and sun.
As is always the case with inbound long-period comets, any forecasts as to its brightness should be taken cautiously. The comet appears to be a “new” one making its first visit to the inner solar system from the Oort Cloud, and as discussed in a previous “Special Topics” presentation such objects tend to under-perform compared to what their earlier brightnesses might suggest. The fact that Comet PANSTARRS appears to be quite bright intrinsically and was active at such large heliocentric distances works in its favor, but its rather large perihelion distance, its remaining far from Earth, and its poor geometric viewing conditions around the time of perihelion work against it. The comet should certainly reach naked-eye brightness, perhaps 5th magnitude, and could become somewhat brighter than that; 3rd magnitude perhaps is reasonable, and while I would consider a peak brightness of 1st magnitude as unlikely, it is not out of the question. As I stated at the outset, though, I doubt that this will become a “Great Comet,” although I suppose one never knows. We will just have to wait and see what the comet does.
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