Proper Name | Calypso | Designation | Saturn XIV | Primary Planet | Saturn | Orbital Period | 1 day, 21 hours, 18 minutes | Distance from Saturn | Semi-Major Axis: 294,619 km Periapsis: 292,527 km Apoapsis: 296,711 km | Eccentricity | 0.0071 | Rotation Period | 1 day, 21 hours, 18 minutes (synchronous orbit) | Diameter (longest axis) | 30.2 km 18.8 miles | Notes | Calypso has a long, narrow shape, just over thirty kilometres along its longest axis, but only fourteen across its shortest diameter. Its surface is marked by several relatively large craters, but particles from Saturn's E Ring have filled these craters and smoothed their edges. |
One of three moons that share an orbit of Saturn nearly 300,000 km from the planet within the tenuous and icy ring known as the E Ring. The largest of these three is Tethys, a spherical moon more than a thousand kilometres in diameter, but Tethys also has two smaller companions. Calypso is one these, a fraction of Tethys' size and following that major moon in its orbit around Saturn by some sixty degrees of arc. It is able to hold a stable relative position because it occupies Tethys' trailing Lagrange Point. Calypso has a counterpart, Telesto, which precedes Tethys in its orbit by the same sixty degree angle that Calypso trails behind.
Physically Calypso is an irregular body, highly elongated in shape; it measures a little more than thirty kilometres along its longest axis, and less than fifteen kilometres along its shortest. Though rocky and cratered, its surface is also relatively smooth, with a tracery of flowing patterns. These effects are probably due to particles collected from the enveloping E Ring, particles whose ultimate origins lie in the great geysers blasting water ice outward from the moon Enceladus.
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