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hor_green_bar1.jpg Enceladus hor_green_bar1.jpg


Enceladus - courtesy NASADiscovered by William Herschel in 1789, Enceladus is one of the innermost moons of Saturn. Enceladus is a smooth and bright satellite relative to Mimas and has a high albedo due to its high >reflectivity.

The surface temperature of Enceladus is -201° C (-330° F) and has a diverse surface, with all sorts of features that tell much about its history. There Feature Map of Enceladus - copyright Calvin J. Hamiltonare cratered nd non-cratered plains, many crustal deformations with fissures and rough terrain. The interior may be liquid although this goes against common logic because its low surface temperature would prohibit the formation of ice. However it is theorized that Enceladus is warmed by a tidal mechanism.




PHYSICAL DATA FOR ENCELADUS
 Mass (kg) 8.40e + 19
 Mass (Earth = 1) 1.4056e - 05
 Radius (km) 250
 Radius (Earth = 1) 3.9197e - 02
 Mean Density (g/cm3) 1.24
 Mean Distance from Saturn (km) 238,020
 Magnitude (V0) 11.7



ORBITAL DATA FOR ENCELADUS
 Rotational period (days) 1.370218
 Orbital period (days) 1.370218
 Mean orbital velocity (km/s) 12.64
 Orbital eccentricity 0.0045
 Orbital inclination (degrees) 0.02
 Escape (km/s) 0.212
 Albedo 0.99



Physical Data Key
Mass Mass
Mass Mass compared to that of Earth.
Radius Radius
Radius Radius compared to that of Earth.
Mean Density Average Density.
Distance Distance to the planet's center.
Magnitude The brightness of a star or object.
Orbital Data Key
Rotational Period Number of days to make one complete rotation.
Orbital Period Number of days to obital the planet.
Mean Orbital Velocity Average obital speed.
Orbital Eccentricity Eccentricity.
Orbital Inclination The tilt of the moon or planet.
Escape Escape Velocity.
Albedo Visual geometric albedo.




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