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— CH. 1 · INTRODUCTION —

Mimas

~7 min read · Ch. 1 of 7
7 sections
  • Mimas, the seventh-largest moon of Saturn, holds a record that sounds almost impossible: it is the smallest body in the solar system known to have pulled itself into a roughly spherical shape through its own gravity. With a mean diameter of just 396.4 kilometres, this ice-covered world sits in orbit around Saturn and shapes the ring system that makes the planet famous. Its story raises two questions that have occupied planetary scientists for decades. How did a world so small survive a collision powerful enough to carve a crater nearly a third its own width? And is something warm and liquid hiding beneath all that frozen silence?

  • On the 17th of September 1789, the astronomer William Herschel turned a remarkable telescope toward Saturn and recorded in his own words: 'I also, on the 17th of September, detected the seventh satellite, when it was at its greatest preceding elongation.' The instrument he used was the 40-foot telescope, a metal mirror reflector with a 48-inch aperture. Herschel's note about 'the great light of the forty-feet speculum' tells us something important: the moon was so faint that only this extraordinary instrument could pull it out of the glare. The 40 feet in the telescope's name referred to the focal length, not the mirror width, which is a detail easy to confuse given how modern telescopes are described.

    Decades after the discovery, Herschel's son John gave the moon its name. In his 1847 publication Results of Astronomical Observations made at the Cape of Good Hope, John Herschel proposed names for all seven then-known satellites of Saturn. He drew from Greek mythology, choosing the Giants, a generation that fought a great struggle against Zeus and the Olympians. Saturn corresponds to the Roman form of Cronus, ruler of an earlier generation of Titans, so naming Saturn's moons after the Giants carried a certain mythological logic. The giant in question was named Mimas, and his name passed to the small icy world still bearing it today. A proposed symbol for Mimas, designed by software engineer Denis Moskowitz, combines a Greek mu with the crook of the Saturn symbol, though it has not come into wide use.

  • Mimas has a density of just 1.15 grams per cubic centimetre, which is barely above the density of water ice itself. That low figure points directly to its composition: mostly water ice, with only a small admixture of rock. Because of tidal forces from Saturn, the moon is not a perfect sphere but noticeably oblate; its longest axis stretches about 10 percent longer than its shortest. A Cassini probe image from the 14th of October 2009 showed this squashed shape clearly enough to measure.

    The surface area of Mimas is slightly less than the land area of Spain or California. That comparison helps fix the scale: this is not a world you could lose in the outer solar system unnoticed, but it is small enough that most of its surface could be crossed in less time than a transcontinental flight. Three classes of geological feature are officially recognised on Mimas: craters, chasmata (chasms), and catenae, which are crater chains. The heavily cratered terrain carries a subtle asymmetry. Most of the surface shows craters larger than 40 kilometres across, but in the south polar region craters rarely exceed 20 kilometres in diameter. That difference in crater size distribution is one of the surface's quiet puzzles.

  • Herschel, the great crater named after the moon's discoverer, measures 139 kilometres across, close to one-third of Mimas's entire diameter. Its walls rise approximately 5 kilometres, portions of its floor lie 10 kilometres deep, and a central peak climbs 6 kilometres above that floor. To appreciate the scale, consider that a crater of equivalent relative size on Earth would stretch more than 4,000 kilometres across, wider than the Australian continent.

    The impact that carved Herschel came close to ending Mimas entirely. Evidence for how violent that collision was survives on the exact opposite side of the moon. The surface antipodal to Herschel is highly disrupted, a sign that the shock waves from the impact propagated straight through the moon's interior and tore at the far side from within. The rest of the surface is saturated with smaller craters, but none approach Herschel's size. The crater's resemblance to the Death Star's superlaser dish from the 1977 film Star Wars has been widely noted. The similarity is coincidental: the film was produced nearly three years before any spacecraft resolved Mimas's surface in enough detail to reveal the crater.

  • Particles sitting in the Huygens Gap, at the inner edge of the Cassini Division, complete two orbits for every single orbit Mimas completes. That 2:1 orbital resonance means that every time those particles reach a particular point in their path, Mimas is in exactly the same position and pulls on them in the same direction. Over time those repeated, aligned gravitational tugs push the particles out of the gap entirely, creating one of the largest cleared regions in Saturn's ring system. The boundary between the C Ring and the B Ring sits in a 3:1 resonance with Mimas.

    Mimas reaches further still into Saturn's ring architecture. The G Ring was found to be in a 7:6 co-rotation eccentricity resonance with Mimas, with the ring's inner edge sitting about 15,000 kilometres inside Mimas's orbit. Beyond the rings, Mimas shares a 2:1 mean-motion resonance with the much larger moon Tethys, and stands in a 2:3 resonance with Pandora, one of the small shepherd moonlets flanking the outer F Ring. A co-orbital moon was reported alongside Mimas by Stephen P. Synnott and Richard J. Terrile in 1982, but the detection was never confirmed.

  • In 2014, researchers noted that the way Mimas wobbles slightly as it orbits, a motion called libration, carried a component that its orbit alone could not explain. Two hypotheses emerged: either the moon had an elongated rocky core that put its interior mass off-centre, or a liquid ocean lay hidden beneath the ice. At the time the ocean idea seemed difficult to sustain, because a 2017 analysis found that an internal ocean would have produced surface tidal stresses comparable to those on Europa, a moon covered in cracked and fractured ice. Mimas shows no such cracking, which appeared to argue against an ocean.

    In 2022, scientists at the Southwest Research Institute worked out a tidal heating model that resolved the contradiction. Their analysis showed that an ocean could exist beneath an icy shell between 24 and 31 kilometres thick and still leave the surface visually undisturbed. That combination of thickness and heating would match every observation Cassini had gathered. Then on the 7th of February 2024, researchers at the Paris Observatory announced that Mimas's orbit apsidally precesses more slowly than a solid body would. The orbit itself, not just the wobble, was pointing toward hidden water. Their calculations placed the ocean 20 to 30 kilometres below the surface, consistent with the 2022 model. They also estimated that the ocean is younger than 25 million years, possibly only 2 to 3 million years old, which would explain why so little geological activity has reached the surface to disrupt its ancient cratered face.

  • Pioneer 11 made the first close pass at Saturn in 1979, reaching a closest approach to Mimas of 104,263 kilometres on the 1st of September 1979. Voyager 1 followed in 1980, and Voyager 2 arrived in 1981. Each flyby added detail, but it was the Cassini orbiter, which entered Saturn orbit in 2004, that transformed understanding of the moon. Cassini imaged Mimas multiple times and conducted a close flyby on the 13th of February 2010, passing within 9,500 kilometres.

    In 2010, NASA released a thermal map of Mimas derived from Cassini imagery. The warmest regions traced a shape along one edge of the moon that observers compared to the video game character Pac-Man, with Herschel Crater standing in for the edible dot, or power pellet, from the original game. Continued measurements of surface heat flux from future missions will be necessary before the subsurface ocean hypothesis can move beyond strong evidence into confirmed fact.

Common questions

Who discovered Mimas and when was it found?

Mimas was discovered by the astronomer William Herschel on the 17th of September 1789 using his 40-foot reflecting telescope, which had a 48-inch aperture. Herschel recorded detecting the seventh satellite of Saturn when it was at its greatest preceding elongation.

How big is Herschel Crater on Mimas?

Herschel Crater measures 139 kilometres across, nearly one-third of Mimas's mean diameter of 396.4 kilometres. Its walls stand approximately 5 kilometres high, parts of its floor are 10 kilometres deep, and its central peak rises 6 kilometres above the crater floor.

Does Mimas have a subsurface ocean?

Evidence strongly supports the existence of a liquid ocean beneath Mimas's icy surface. On the 7th of February 2024, researchers at the Paris Observatory announced that Mimas's orbital precession is slower than a solid body would produce, pointing to an internal ocean located 20 to 30 kilometres below the surface. Scientists estimate the ocean is younger than 25 million years old, and possibly only 2 to 3 million years old.

Why does Mimas look like the Death Star?

Mimas's giant Herschel Crater, with its concave shape, resembles the superlaser dish of the Death Star from the 1977 film Star Wars. The resemblance is coincidental: the film was made nearly three years before any spacecraft resolved the crater in enough detail to observe it.

How does Mimas create the Cassini Division in Saturn's rings?

Particles in the Huygens Gap at the inner edge of the Cassini Division orbit Saturn twice for every single orbit Mimas completes, a 2:1 orbital resonance. The repeated gravitational pulls from Mimas, always in the same direction, push those particles out of the gap and clear the region between Saturn's A Ring and B Ring.

What is Mimas made of and how large is it?

Mimas has a mean diameter of 396.4 kilometres and a density of 1.15 grams per cubic centimetre, indicating it is composed mostly of water ice with only a small amount of rock. Its surface area is slightly less than the land area of Spain or California, making it the smallest astronomical body known to be roughly rounded by its own gravity.

All sources

32 references cited across the entry

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  2. 3journalHerschelM. Arago — 1871
  3. 6dictionaryMimasOxford University Press
  4. 9webPhobos and Deimos symbolsGavin Jared Bala et al. — The Unicode Consortium — 7 March 2025
  5. 10webMimas' ellipsoidal shapeThe Planetary Society
  6. 11bookJupiter and SaturnLinda E. Elkins-Tanton — Infobase Publishing — 2006
  7. 12journalLarge impact features on middle-sized icy satellitesJeffrey M. Moore et al. — October 2004
  8. 13journalA recently formed ocean inside Saturn's moon MimasV Lainey et al. — 7 February 2024
  9. 15journalConstraints on Mimas' interior from Cassini ISS libration measurementsR. Tajeddine et al. — 17 October 2014
  10. 16journalThe implications of tides on the Mimas ocean hypothesisA. R. Rhoden et al. — 24 February 2017
  11. 19journalA recently formed ocean inside Saturn's moon MimasV. Lainey et al. — 7 February 2024
  12. 21webSaturn's moon is Death Star's twinKelly Young — New Scientist — 11 February 2005
  13. 22web1980s Video Icon Glows on Saturn MoonJia-Rui C. Cook — NASA — 29 March 2010
  14. 23webBizarre Temperatures on MimasNASA — 29 March 2010
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