See Mutual Events, Close Approaches of Saturn's Moons

 

  From - Sky & Telescope

  By - Bob King

 Edited by - Amal Udawatta

For a short time every 13.5 to 15.7 years, Saturn's rings appear exactly horizontal from Earth. They temporarily disappear from view in amateur telescopes due to their extraordinary thinness. Although the main rings are 300,000 kilometers across, they can be as thin as 10 meters (33 feet) in places. To scale, Saturn's rings are much thinner than a standard sheet of paper. Earth passes through the ring plane on March 23, 2025.
NASA

Saturn passed opposition on September 8th and is now well placed in the southeastern sky at nightfall in Aquarius. I can still recall the first time I found the planet from my front yard in the winter of 1965. It was situated in almost the same location you'll find it tonight, a few degrees northwest of the "crooked fingertip" asterism formed by the three Psis — Psi1 (ψ1), Psi2 (ψ2), and Psi3 (ψ3) Aquarii. Wish me happy birthday — I'm two Saturn-years old!

On September 25th at around 10 p.m. EDT, observers can watch an appulse, or close approach, of Dione and Tethys west of the planet. A 10-inch scope with clean optics will bag Mimas, which will be near maximum elongation. North is up in this and subsequent images.
Stellarium

This year and next are special years for the sixth planet, because observers will have several opportunities to view the rings nearly edge on. This view is only available about once every 15 years, when the Earth crosses through their orbital plane. Unfortunately, during the current apparition, edgewise presentation occurs on March 23, 2025, only 11 days after solar conjunction. Steeped in the solar glow, the planet will be unobservable.

The night of September 26th will be ideal to see multiple moons, many at or near greatest elongation from the planet. Iapetus lies west of Saturn and shines brightest right now because its ice-coated hemisphere faces our direction.
Stellarium

Come mid-April we'll get our first glimpse of the south face when the ring plane tips open a hair to –1.5°. Even then, Northern Hemisphere observers will have to dig into twilight to view the planet. The rings reach their maximum southern tilt of –3.8° in early July before narrowing again to a minimum of –0.5° in mid-November. By early December the flip-flopping ends, and the ring plane steadily opens to a maximum of 27° in 2033. The next ring plane crossing we'll see in a dark sky occurs in October 2038. Holy quasars, that's a long wait.

For a brief time, Rhea, Tethys, and Dione form a compact, nearly straight line briefly on September 27th at11:21 p.m. EDT.
Stellarium

With the planet's current tiny tilt, the moons — which normally cluster about the planet — are strung out in a more linear fashion, making them easier to spot when they reach greatest elongation. Flattened rings also reduce the planet's overall brightness, which further helps in picking out the fainter moons. Like the rings, the major moons orbit in the equatorial plane, which means that as Earth approaches that plane, we can watch them eclipse and occult one another in what are called mutual events. Indeed, the 2024–2026 mutual event season is already underway.

Enceladus shines atop Tethys east of the planet on October 1st at 1:07 a.m. EDT.
Stellarium

Similar events occur when we pass through Jupiter's orbital plane, but its moons are large enough to discern as disks. All of Saturn's satellites — with the exception of Titan (diameter 0.8″) — are only a whisper of an arcsecond across. Many of the upcoming events occur among the fainter moons close to the planet's glare and will prove challenging. But as the ring plane flattens out, events become more frequent and also involve the larger moons farther out from the planet, making them easier to see.

Enceladus partially eclipses Tethys on October 1st just before 11 p.m. EDT. The two moons will be extremely close at the time. It will be fun to watch them approach and separate in the minutes before and after the event.
Stellarium

Find Mutual Events On Your Own

The Institute of Celestial Mechanics and Computation of Ephemerides (IMCCE) maintains a complete list of Saturn satellite events with a clear explanation on how to read and use the data. Check it out and make a note of significant occultations and eclipses visible from your observing site.

One of the key variables to look at is the impact factor — the closer it is to "0" the better. Zero indicates a central passage of the moon through the shadow or across the disk of another moon. Grazing events are equal to "1."

To interpret the event shorthand under the Type column you'll need to know each moon's number designation. They are: Mimas (1), Enceladus (2), Tethys (3), Dione (4), Rhea (5), Titan (6), Hyperion (7), and Iapetus (8). For example, when you read "3E2," it means Tethys will eclipse Enceladus, while "3O4" indicates that Tethys will occult Dione.

To know just where to look beforehand, I suggest you simulate each local event using Stellarium or similar free stargazing software. The next event visible from the Americas will be a partial eclipse of Tethys by Enceladus on October 1st starting at 10:58 p.m. EDT and ending at 11:07 p.m.

Dione and Tethys get close on the night of October 15th.
Stellarium

There are also lots of "close calls" when two or more moons make a tight pair or triplet for a brief period of time. These are fun to watch because you can easily and quickly detect their orbital motion, and prying moons apart at various magnifications makes for good sport.

To help in identifying Saturn's satellites it's good to know their magnitudes. Titan is the brightest at magnitude 8.4, followed by Rhea (9.7), Tethys (10.2), Dione (10.4), Iapetus (variable but bright at ~11 in late September), Enceladus (11.7), Mimas (12.9), and Hyperion (14.3).

While Jupiter is often toted out as a model of the solar system in miniature, Saturn fulfills the same role with aplomb.