A newly found comet will quickly be gracing our night sky.
On Sept. 10, Vladimir Bezugly of Dnipro, Ukraine was inspecting on-line photographs of a low-resolution public web site exhibiting photographs obtained throughout Sept. 5-9 with the Photo voltaic Wind Anisotropies (SWAN) digicam on the Photo voltaic and Heliospheric Observer (SOHO) spacecraft. That is when he found a transferring object, resembling a brilliant blob, shut the solar. The blob turned out to be a comet. A brilliant comet.
In reality, as Bezugly later famous: “In my reminiscence, this is without doubt one of the brightest comet discoveries ever made on SWAN imagery,” including, “the twentieth official SWAN comet to this point.” Since Bezugly’s first sighting, many different amateurs — primarily within the Southern Hemisphere — have seen it. The comet has since acquired a proper IAU designation on Sept. 15 as Comet C/2025 R2 (SWAN).
A consensus of the most recent observations of comet SWAN indicated a magnitude of +7, which places it just out of the reach of naked-eye visibility under dark, moonless skies. Good binoculars, however, can readily bring it into view.
The typical description of the comet by those using binoculars and small telescopes is a small, condensed head or coma with a thin, faint tail extending for roughly 2 degrees.
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An orbit primarily based on 60 completely different noticed positions between Sept. 12 and 14, 2025 has been calculated by Syuichi Nakano of the Central Bureau for Astronomical Telegrams. He finds that the comet handed perihelion — its closest level to the solar — on Sept. 12 at a distance of 46.74 million miles (75.20 million km).
Whereas it’s now transferring away from the solar, it’s at the moment approaching Earth. It is going to come closest to us (perigee) on Oct. 21 when will probably be 25.10 million miles (40.38 million km) away. Based mostly on its orbital eccentricity of 0.996015, the time it takes for comet SWAN to make one full circuit across the solar is estimated to be on the order of roughly 1,400 years.
How bright?
A number of different predictions have been made regarding the brightness Comet SWAN as it passes closest to Earth during the third week of October. To date, brightness forecasts issued by Japanese comet expert Seiichi Yoshida and Dutch comet professional Gideon Van Buitenen point out that the comet will peak someplace between magnitude +6 and +7, most likely inserting it proper on the cusp of naked-eye visibility, however actually inside attain of fine binoculars or small telescopes.
Daniel W.E. Inexperienced on the Central Bureau for Astronomical Telegrams, means that comet SWAN will hover close to magnitude of +6, from Oct. 2 to twenty, maybe changing into a number of tenths of a magnitude brighter for a number of days round Oct. 12, which means it would develop into faintly seen with the unaided eye.
The place to seek out it and viewing prospects
Your clenched fist is equal to roughly 10 degrees when held at arm’s length. By Oct. 28, the comet’s altitude will have climbed to 30 degrees (“three fists”) above the south-southwest horizon by nightfall and by Oct. 25 it will stand halfway up in the southern sky when twilight ends, and not set until after midnight.
During October, comet SWAN will move along a path taking it across the constellations of Libra, Scorpius, Ophiuchus, Serpens, Scutum, Sagittarius, Aquila and Aquarius.
As is the case with another comet we have recently discussed — comet Lemmon — sighting comet SWAN may prove to be rather difficult for locations that are plagued by light pollution. Remember, you’re not looking for a sharp star-like object, but rather something which is spreading its light out over a comparatively large area.
Like comet Lemmon, comet SWAN does not appear to be a dusty comet but is primarily composed of gas. Such comets appear fainter than comets composed primarily of dust (which is a far better reflector of sunlight) and glow with a bluish-white hue. The gas is activated by the ultraviolet rays of the sun, making the comet glow in much the same way that black light causes phosphorescent paint to light up.
So, most who ultimately locate Comet SWAN in their binoculars or telescopes will likely describe it as a nearly circular cloud, appearing noticeably brighter and more condensed near the center. Some might also detect its faint tail appearing as a bit of a thin, narrow appendage extending out from the comet’s coma; sort of like an “apple on a stick,” but hardly the kind of tail exhibited by other larger and brighter comets.
Meteor shower? (NOT!)
One other attribute that has been widely promoted on social media about comet SWAN is the possibility that it might cause a meteor shower sometime between October 4 to 6. The reason that this potential has been suggested is that in diagrams showing the comet’s orbit relative to the orbits of the inner planets, it appears that comet SWAN’s orbit intersects the orbit of the Earth right around Oct. 5.
The assumption is that if there is any meteoric material that has been shed by the comet on previous trips around the sun, that there is a chance that the Earth will encounter it around the time it intersects the orbit of the comet.
An intriguing theory, but it is not likely to happen.
The reason is that the orbits of Earth and comet SWAN will not intersect on Oct. 5. What is transpiring is that both objects are traveling on curtate orbits. When looking at the orbital paths from a perspective high above, it certainly appears that the orbits interact with each other.
But in reality, according to my calculations, at the Oct. 5 point of our orbit, the comet orbit — and any possible cosmic debris that is traveling along it, will travel far above our orbit and will miss us by some 4.4 million miles (7 million km). That is far too wide a gap between the two orbits to hope for any type of semblance of significant meteor activity.
Besides, the best chance to encounter any meteoroids shed by comet SWAN would be behind it. But Earth arrives at the Oct. 5 point, ahead of it, 16 days before the comet itself passes by. And we’ve already noted that comet SWAN is mostly a gaseous comet and not a dusty comet. So, it is not likely shedding very much material along its path around the sun. Thus, even if we were to encounter the comet orbit directly, there seems little chance we’d encounter very much comet debris to produce many celestial streaks.
Joe Rao serves as an instructor and guest lecturer at New York’s Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky and Telescope and different publications.
