How Saturn's rings might be keeping a youthful appearance

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Photo by NASA Hubble Space Telescope on Unsplash
Photo by NASA Hubble Space Telescope on Unsplash

Even though Saturn's rings appear clean and young, they may be as old as the planet itself according to international researchers. It was previously thought that impacts with small rocky debris travelling through space (called micrometeoroids) would dirty and darken the rings over time, but in 2004 the Cassini spacecraft revealed the rings to be clean and bright suggesting that they are not very old. The new research simulated collisions between micrometeoroids and icy ring particles using computer models, finding that high-speed impacts don't dirty the rings as previously thought, and so the rings have stayed clean longer than expected.  They suggest that although more research is required, their findings suggest that very low levels of pollution may mean that Saturn’s rings are actually billions of years old and are simply maintaining a more youthful appearance.

Media release

From: Springer Nature

Planetary science: How Saturn’s rings might be keeping up a youthful appearance

Saturn’s icy rings could be much older than they appear due to their resistance to pollution from impacts with rocky debris, according to a Nature Geoscience paper. The authors suggest that Saturn’s rings may be as old as the planet itself, even though they appear clean and young, challenging previous estimates of their age.

Saturn’s rings were once thought to be ancient, perhaps formed at the same time as the planet itself — approximately 4.5 billion years ago. Over time, impacts with micrometeoroids (rocky debris smaller than a grain of sand travelling through space) are thought to dirty and darken the rock and ice particles that make up the rings. However, when the Cassini spacecraft reached Saturn in 2004, it observed that Saturn’s rings appear to be relatively bright and clean. As such, research has estimated that Saturn’s rings are younger than 400 million years old.

Ryuki Hyodo and colleagues simulated collisions between micrometeoroids and icy ring particles using computer models. They found that high-speed impacts can lead to vaporisation of the micrometeoroids, with the vapour then expanding, cooling, and condensing within Saturn’s magnetic field to form charged nanoparticles and ions. Hyodo and colleagues’ simulations revealed that these charged particles then either collide with Saturn, are dragged into its atmosphere, or escape the gravitational pull of the planet entirely. As a result, the authors suggest that very little of this material is deposited onto the rings, keeping them in relatively clean condition. They suggest that very low levels of pollution may mean that Saturn’s rings are actually billions of years old and are simply maintaining a more youthful appearance.

Although further research is required, the authors suggest that this process could potentially also be occurring in the rings of Uranus and Neptune, as well as on icy moons around giant planets.

Journal/
conference:
Nature Geoscience
Research:Paper
Organisation/s: ISAS/JAXA, Japan
Funder: R.H. acknowledges the financial support of JSPS Grants-in-Aid (JP17J01269, 18K13600, 23KK0253). H.G. acknowledges the financial support of JSPS Grants-in-Aid (21H04514, 20KK0080, 22K21344). G.M. thanks the Institut de Physique du Globe de Paris and European Research Council, France (101001282, METAL). The dynamic simulations of charged particles were performed on the S-CAPAD/ DANTE platform, IPGP, France. We deeply thank S. Charnoz and A. Crida for discussion. We thank B.C. Johnson for the discussion on the EOSs, Z. Zhang for the discussion on the detectable darkening properties by the Cassini’s Radiometry observations, J. O’Donoghue for the discussion on the ring rain and R. Morishima for the discussion on the size distribution of the ring particles.
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