Mimas
William Herschel recorded a new celestial body on the 17th of September 1789 using his massive 40-foot telescope. The instrument featured a metal mirror with an aperture that focused light over a distance of 40 feet rather than defining its width. This observation marked the first time humanity had seen Mimas, though it remained unnamed for decades after its discovery. William Herschel's son John later proposed naming all seven known satellites of Saturn after mythological figures in his 1847 publication Results of Astronomical Observations made at the Cape of Good Hope. He selected Mimas from Greek mythology to represent one of the Giants who fought against Zeus and the Olympians. The name derives from the root Mimant- which appears in Italian as Mimante and Russian as Мимант. English speakers typically pronounce the name with stress on the second syllable or sometimes place it on the first. No other planetary moons received symbols in astronomical literature until Denis Moskowitz designed a symbol combining the Greek letter mu with the crook of the Saturn symbol in modern times.
Mimas holds the distinction of being the smallest astronomical body known to be roughly rounded by its own gravity despite its tiny size. Its mean diameter measures approximately 396 kilometers while its density sits at just 1.15 grams per cubic centimeter. This low density indicates the moon consists mostly of water ice with only a small amount of rock mixed within. Tidal forces acting upon the satellite cause it to become noticeably oblate with its longest axis extending about 10% longer than its shortest. Images captured by the Cassini probe reveal an ellipsoidal shape that is especially distinct compared to other moons. The surface area covers slightly less ground than the land area of Spain or California combined. Most of the terrain features craters larger than 20 kilometers across except for the south polar region where few exceed 5 kilometers. Three types of geological features appear officially recognized including craters, chasmata which are deep chasms, and catenae representing chains of craters.
A massive impact crater named Herschel spans 138 kilometers across the surface of Mimas. This feature measures almost one-third of the parent body's total diameter making it unique in the Solar System relative to its host. Walls rise approximately 5 kilometers high while parts of the floor measure 8 kilometers deep below the rim. A central peak rises 4 kilometers above the crater floor creating a dramatic topographical profile. If Earth possessed a crater of equivalent scale it would span over 600 kilometers wider than Australia. The energy from this impact nearly shattered the moon entirely as evidenced by highly disrupted terrain on the antipodal point opposite the crater. Shock waves generated by the collision propagated through the entire globe leaving visible scars on the far side. The Mimantean surface remains saturated with smaller impact craters but none approach the sheer size of Herschel. Researchers note that the surface is not uniformly cratered despite heavy bombardment history.
Mimas exerts gravitational influence that clears material from the Cassini Division between Saturn's widest rings known as the A Ring and B Ring. Particles within the Huygens Gap at the inner edge maintain a 2:1 orbital resonance meaning they orbit twice for every single revolution of Mimas. Repeated pulls from the satellite force these particles into new orbits outside the gap boundary. The interface between the C and B rings exists in a 3:1 resonance relationship with the moon. Recent data shows the G Ring maintains a 7:6 co-rotation eccentricity resonance with its inner edge located about 118,000 kilometers inside Mimas's own orbit. The satellite also holds a 2:1 mean-motion resonance with the larger moon Tethys while maintaining a 2:3 resonance with the outer F Ring shepherd moonlet Pandora. Stephen P. Synnott and Richard J. Terrile reported a co-orbital moon in 1982 but this object was never confirmed by subsequent observations.
Researchers analyzing Mimas's movement discovered librational motion components unexplained by standard orbital mechanics alone in 2014. They concluded either an elongated core existed or a liquid ocean lay hidden beneath the ice shell. By 2017 scientists determined that such an ocean would create surface tidal stresses comparable to those on Europa yet no cracking appeared on Mimas. This lack of evidence argued against the presence of a global ocean despite the formation of a core potentially producing similar effects. An asymmetric mass anomaly associated with Herschel crater offered a more likely explanation for the observed libration patterns. Scientists at the Southwest Research Institute identified a tidal heating model in 2022 that produced an internal ocean without visible surface cracks. Their findings suggested a stable icy shell between 24 and 31 kilometers thick could conceal water matching Cassini observations. On the 7th of February 2024 researchers at the Paris Observatory announced orbit apsidal precession slower than predicted if solid supporting the subsurface ocean theory. They estimated the ocean sits 20 to 30 kilometers below the surface and must be less than 25 million years old to explain the lack of geological activity.
Pioneer 11 flew past Saturn during 1979 achieving its closest approach to Mimas on the 1st of September 1979 at a distance of 104,263 kilometers. Voyager 1 conducted a flyby in 1980 followed by Voyager 2 which passed through the system in 1981. The Cassini orbiter entered orbit around Saturn in 2004 allowing multiple close imaging sessions over many years. A particularly detailed encounter occurred on the 13th of February 2010 when Cassini passed within 9,800 kilometers of the moon's surface. These missions provided high-resolution images showing shapes and textures of overlapping craters clearly for the first time. Data from these probes revealed an ellipsoidal shape especially noticeable compared to earlier observations. Scientists used temperature maps generated from Cassini images to reveal warm regions along one edge resembling the video game character Pac-Man with Herschel Crater acting as an edible dot. NASA released this temperature map overlay in 2010 highlighting how certain angles make Mimas resemble the Death Star from the 1977 film Star Wars.
Continue Browsing
Common questions
When was Mimas first discovered by William Herschel?
William Herschel recorded the discovery of Mimas on the 17th of September 1789 using his massive 40-foot telescope. This observation marked the first time humanity had seen this moon, though it remained unnamed for decades after its initial detection.
What is the diameter and composition of Mimas?
Mimas has a mean diameter of approximately 396 kilometers and consists mostly of water ice with only a small amount of rock mixed within. Its density sits at just 1.15 grams per cubic centimeter while tidal forces cause it to become noticeably oblate.
How large is the Herschel crater on Mimas compared to Earth features?
The Herschel crater spans 138 kilometers across the surface of Micas and measures almost one-third of the parent body's total diameter. If Earth possessed a crater of equivalent scale it would span over 600 kilometers wider than Australia.
Why does Mimas have an internal ocean according to recent research?
Scientists at the Southwest Research Institute identified a tidal heating model in 2022 that produced an internal ocean without visible surface cracks. They estimated the ocean sits 20 to 30 kilometers below the surface and must be less than 25 million years old to explain the lack of geological activity.
Which space missions provided detailed images of Micas between 1979 and 2010?
Pioneer 11 flew past Saturn during 1979 achieving its closest approach to Micas on the 1st of September 1979 at a distance of 104,263 kilometers. The Cassini orbiter entered orbit around Saturn in 2004 allowing multiple close imaging sessions including a particularly detailed encounter on the 13th of February 2010 when Cassini passed within 9,800 kilometers of the moon's surface.