Rings in our Solar System can come and go

By the time Saturn becomes a pale hazy brown ringless orb, another planet will have adorned a cosmic crown of its own.

Rings in our Solar System can come and go
Saturn and its iconic rings, as captured in 2016 by NASA’s Cassini spacecraft. Credit: JPL-Caltech

It’s hard to imagine Saturn without rings. That’s exactly what it will be though roughly 100 million years from now, a short span of time for a planet born 4.6 billion years ago. Recent research and measurements taken by NASA’s Cassini spacecraft have revealed that the ring material, which is mostly water ice, is being gradually pulled into Saturn. Eventually there will be almost nothing left.

To think that Saturn’s iconic rings, which span the length of 27 Earths, would vanish in a cosmic blip is yet another reminder that our Solar System is a dynamic place. By the time Saturn becomes a pale hazy brown ringless orb, Mars would’ve adorned a cosmic crown of its own.

Sometime between 30 to 50 million years from now, Mars’ gravity will break apart its closest moon Phobos. Its fragments will encircle the Red Planet. Remarkably, this isn’t the first time such an event would’ve transpired on Mars. A large asteroid or comet may have impacted the planet shortly after our Solar System’s formation, with the resulting orbital debris becoming rings and eventually clumping into small moons. Scientists think Mars’ gravity ripped the innermost moon into rings again at some point, and so Phobos might just be the latest product of such an ongoing ring-moon cycle.

It’s possible that Phobos and the Saturnian rings formed during or around the time dinosaurs ruled planet Earth. For a long time scientists thought Saturn’s rings are simply leftover material from the planet’s birth 4.6 billion years ago but recent measurements from Cassini have challenged this assumption.

When the Cassini spacecraft made a number of passes between Saturn and its rings during the mission’s ‘Grand Finale’ in 2017, it allowed scientists to carefully infer the mass of the rings based on how gently the spacecraft was pulled towards them. It turned out the rings weigh less than Saturn’s small moon Mimas, too low for them being ancient structures formed alongside such a giant planet. Combined with the fact that the rings are still bright and haven’t darkened over time due to incessant space weathering, scientists estimate their age to be less than 100 million years. They think that Saturn’s rings formed either from a moon getting too close and breaking apart or from collisions of multiple small icy moons.

A natural-color composite image of Saturn’s rings, captured by the NASA-ESA Cassini spacecraft. Slight color variations across the rings and multiple gaps are clearly visible. Credit: JPL-Caltech

A spectrum of rings

Our Solar System is host to even more unique ring types. Jupiter’s faint ring system is made entirely of dust particles hurled up into orbit by micrometeorites impacting the planet’s small, inner moons. Saturn’s faint and diffuse Phoebe ring is also formed from particles ejected from the namesake moon. Neptune’s outermost ring isn’t even a ring but five distinct arcs, whose particles are probably kept from spreading out due to the gravitational pull of the ring moon Galatea.

Some rings are mysterious. For example, two of the outermost Uranian rings are red and blue, indicating a different composition than not just the planet’s inner, gray rings but also from the Saturnian set. The largest Uranus ring, epsilon, is tens to hundreds of times narrower than those of Saturn, and we don’t know why.

In 2014, astronomers discovered a planet outside our Solar System that appears to have rings 200 times wider than Saturn’s! At 180 million kilometers across, the rings of this ‘Super Saturn’— officially named J1407b—span wider than the Sun-Earth distance of 150 million kilometers. On the opposite end of the size spectrum, there are the two rings of 10199 Chariklo, a roughly 200-kilometer sized object orbiting our Sun between Saturn and Uranus. How do these colossal and tiny rings form? We’re yet to find out!

Future exploration

The answers to why the giant planets of Jupiter, Uranus and Neptune don’t have as majestic a set of rings as Saturn, at least in the present, ultimately lie in grasping how rings form, evolve, and in some cases, disappear. Sending a spacecraft to excavate chunks from Saturn’s rings and measure their exact composition, and ideally even bring samples to Earth, will anchor the age and origin of Saturn’s rings.

Likewise, figuring out how Phobos formed would tell scientists if it really is part of an ongoing ring-moon cycle at Mars. While no mission is being planned to study Saturn’s rings, Japan’s Martian Moons eXploration mission, or MMX, will study Phobos and bring samples from it to Earth to help scientists ascertain its age and formation.

The 2023-2032 Planetary Science Decadal Survey—a report produced every 10 years by the U.S. scientific community to guide future NASA missions—recommends sending a spacecraft to Uranus as the highest priority. One of the four major scientific objectives of this Uranus Orbiter and Probe (UOP) mission is to understand the composition, origin, mechanics, and history of the planet’s rings. In the meanwhile, the recently launched JWST space telescope will observe rings of all the giant planets to spot previously unknown features and help scientists better gauge how they evolve.

The majestic rings of Saturn will wane over time, losing chunks and bits to the planet all the while darkening like soil on our Moon. What a sad cosmic death that would be. Perhaps there’s some solace in the fact that Saturn’s tiny icy moon Enceldaus will still be erupting  water plumes into space to keep the planet’s diffuse E-ring alive.

An artist's impression of how Saturn may look as it loses its iconic rings. Credits: NASA / Cassini / James O'Donoghue

Originally published at The Planetary Society.


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