Comet 29P
© Martin MobberleyMartin Mobberley captured this image of the bright outburst of Comet 29P/Schwassmann-Wachmann around 9:50 UT on September 29th.
Catch one of the most active small bodies in the solar system during a rare superoutburst.

A comet infamous for its explosive personality has been in near-continuous outburst since September 25th. The brightness of Comet 29P/Schwassmann-Wachmann is steadily rising, and it now appears as a tiny, 11th-magnitude object easily visible in 8-inch and larger telescopes. If you've never seen a comet masquerade as a star-like planetary nebula, don't pass up the chance — look soon. As the outburst evolves the comet's coma will expand but also fade.

Comet 29P
© StellariumThis map shows the general location of 29P/S-W in late September. Use the detailed map below to pinpoint the comet's position.
Timing and location couldn't be better, with the comet just 1.3° south-southeast of the easy, naked-eye star Iota (ι) Aurigae and standing at the threshold of a copious viewing window. Best viewing starts around 10:30 p.m. local daylight time and lasts till dawn. I caught 29P on Tuesday night, September 28th at 10:15 p.m. CDT, 45 minutes before the last-quarter Moon rose.
Comet 29P
© MegaStar, used with permissionThis map plots the motion of Comet 29P/Schwassmann-Wachmann nightly through October 9th. Positions are for 11 p.m. EDT. The limiting magnitude, orientation (north up for all charts), and field of view are shown in the upper left corner.
Although just 12° altitude, I spotted the suspected comet in my 15-inch Dob even at the lowest magnification of 64×. At a casual glance, it looked exactly like a star, but with averted vision I could see a small, faint coma enrobing the bright false nucleus. Lucky or not, 29P was involved with a 13th-magnitude star some 12″ to its east at the time. When I looked again just before moonrise, it had parted company.

Comet 29P
© Damian PeachThis composite photo shows the fascinating evolution of Comet 29P/S-W1 starting during a previous bright outburst from June 16, 2013 (lower left) to July 28, 2013. The comet typically exhibits a characteristic horseshoe or spiral shape as it evolves because we view the outburst side-on across one hemisphere. Comet 29P appears to rotate slowly with a possible period of 57 days.
Due to low altitude, I couldn't make out more detail, just a super-compact, bright coma with a degree of condensation (DC) of 8 on a scale of 0 to 9, from least to most concentrated. I'm as eager as you are to get the scope out again for another look. The comet may continue to flare and brighten or begin its inevitable dimming. To see night-to-night changes in a celestial object is one of the reasons comets are so fun to observe.

Comet 29P
© Richard MilesComet 29P/Schwassmann-Wachmann orbits beyond Jupiter with a perihelion of 5.7 a.u. and an aphelion of 6.3 a.u.
Many comets have outbursts, but 29P is unique because it averages 7.3 outbursts a year! Typically, two or three per apparition are visible in amateur telescopes. Normally a 16th-magnitude object, a blow-up can vault this comet from obscurity to as bright as 10th magnitude. It orbits a fair bit beyond Jupiter with a period of 14.7 years, and as comets go, it's enormous with a diameter of 60.4 ± 7.4 kilometers. Frankly, to see any comet at such an incredible distance is not only amazing but an indication of just how powerful the current outburst must be.

Richard Miles, with the British Astronomical Association (BAA), is the project lead on the MISSION 29P, a clearinghouse devoted to news and observations of the comet with the hope of better understanding the underlying cause of its tumultuous outbursts. Miles suspects that the object may have undergone four successive outbursts, with "each subsequent event triggering the next" during the current flare-up. Another good resource for current comet happenings is the Comets Mailing List.

Comet 29P
© Richard MilesThis photo, taken September 28th, closely resembles the comet's current visual appearance in a moderate-size telescope at high magnification.
Water ice, an important volatile that drives activity in many comets, is virtually inert at 29P's distance. Instead, vaporizing carbon monoxide ice appears to be the key driver of its regular outbursts. Based on data obtained largely by amateur astronomers, Miles describes the outbursts as cryovolcanoes that erupt explosively after carbon monoxide and methane, under pressure beneath the comet's crust melt, mix and release energy.

Comment: It's telling that the mainstream paradigm cannot explain cometary activity at such as distance with the usual theory of melting ice, whereas a more likely and comprehensive explanation can be found in Electric Universe theory of cometary activity; Pierre Lescaudron summarises it in his book Earth Changes and the Human-Cosmic Connection as follows:
The fundamental difference between asteroids and comets is not their chemical composition, i.e. dirty, fluffy icy comets vs. rocky asteroids. Rather, as has long been put forward by plasma theorists, what differentiates 'comets' from 'asteroids' is their electric activity.

When the electric potential difference between an asteroid and the surrounding plasma is not too high, the asteroid exhibits a dark discharge mode1 or no discharge at all. But when the potential difference is high enough, the asteroid switches to a glowing discharge mode.2 At this point the asteroid is a comet. From this perspective, a comet is simply a glowing asteroid and an asteroid is a non-glowing comet. Thus the very same body can, successively, be a comet, then an asteroid, then a comet, etc., depending on variation in the ambient electric field it is subjected to.3
2) An intense circulation of ions and electrons occurs between the asteroid and the surrounding space. The energy provided by this intense transfer 'excites' electrons which generate photons, hence the glow of the asteroid. See: Meichsner, J. Nonthermal Plasma Chemistry and Physics, p.117

Solar heating causes the crust above these spots to give way, explosively releasing gases along with up to a million tons of dust and debris at a shot. Think of popping the cork on a bottle of champagne. Because 29P is a large comet, its gravity temporarily reseals the "wound" until another cycle begins.

As described in the September 2021 issue of Sky & Telescope magazine, there's currently a campaign to observe this comet. You're encouraged to share your observations at the 29P/ S-W 1 Observations page.

Wishing you clear skies so you can witness 29P's delightful and instructive volatility!