Odysseus (crater)
Template:Short description Template:Use dmy dates Template:Infobox feature on celestial object Odysseus is the largest crater on Saturn's moon Tethys. It is 445 km across, more than 2/5 of the moon's diameter, and is one of the largest craters in the Solar System. It is situated in the western part of the leading hemisphere of the moon—the latitude and longitude of its center are 32.8°N and 128.9°W, respectively. It is named after the Greek hero Odysseus from Homer's the Iliad and the Odyssey.<ref name=gpn/> Odysseus was discovered by the Voyager 2 spacecraft on 1 September 1981 during its flyby of Saturn.<ref>Template:Cite journal</ref>
Geology
The Odysseus crater is now quite flat for its size of approximately 450 km. More precisely, its floor conforms to Tethys's spherical shape. This is most likely due to the viscous relaxation of the Tethyan icy crust over geologic time. The floor lies approximately 3 km below the mean radius, while its exterior rim is about 5 km above the mean radius—the relief of 6–9 km is not very high for such a large crater. Inside the crater the rim is composed of arcuate scarps and extends for about 100 km until the floor is reached. There are several graben radiating away from Odysseus, which are 10–20 km wide and hundreds of kilometers long. They are likely to be cracks in the crust created by the impact.<ref name=moore>Template:Cite journal</ref> The most prominent among them is called Ogygia Chasma.<ref>Template:Gpn</ref>
The crater must have originally been deep, with a high mountainous rim and towering central peak. Over time the crater floor has relaxed to the spherical shape of the Tethyan surface, and the crater's rim and central peak have collapsed (similar relaxation is apparent on Jupiter's moons Callisto and Ganymede). This indicates that at the time of the Odysseus impact, Tethys must have been sufficiently warm and malleable to allow the topography to collapse; its interior may have even been liquid. If Tethys had been colder and more brittle at the time of impact, the moon might have been shattered, and even if it survived the impact, the topography of the crater would have retained its shape, similarly to the crater Herschel on Mimas.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref><ref name=jaumann>Template:Cite book</ref>Template:Rp
The central complex of Odysseus (Scheria Montes)<ref>Template:Gpn</ref> features a central pit-like depression,<ref name=jaumann/>Template:Rp which is 2–4 km deep. It is surrounded by massifs elevated by 2–3 km above the crater floor, which itself is about 3 km below the average radius.<ref name=moore/>
Relation to Ithaca Chasma
The immense trench called Ithaca Chasma, which approximately follows a great circle with a pole near Odysseus's center, had been hypothesized to have formed as a result of the Odysseus impact.<ref name=moore/> However, a study based on high resolution Cassini images indicated that this is unlikely—the crater counts inside Odysseus appear to be lower than in Ithaca Chasma, indicating that the latter is older than the former.<ref>Template:Cite journal</ref><ref name=jaumann/>Template:Rp
See also
- Tirawa – A similar impact basin on Rhea
- Herschel – A similarly-sized (proportionally) impact crater on Mimas