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hor_green_bar1.jpg Iapetus hor_green_bar1.jpg


Iapetus - courtesy NASAIapetus was discovered by Giovanni Cassini in 1671 and is well known by its mysterious dark material that covers the surface on the leading side. Its trailing side is bright. The dark material could probably come from the inside or caught from space. However the true reason remains unknown. One theory suggests that the material could come from Phoebe, in which meteor mpacts could send dust into space that Iapetus sweeps up with its gravitational field. Another theory suggests that the material is of internal origin because much of it is concentrated in the crater floors. Whatever the reason, this mystery will continue to puzzle scientists until further studies are conducted.



PHYSICAL DATA FOR IAPETUS
 Mass (kg) 1.88e + 21
 Mass (Earth = 1) 3.1459e - 04
 Radius (km) 730
 Radius (Earth = 1) 1.1446e - 01
 Mean Density (g/cm3) 1.21
 Mean Distance from Saturn (km) 3,561,300
 Magnitude (V0) 10.2 - 11.9



ORBITAL DATA FOR IAPETUS
 Rotational period (days) 79.33018
 Orbital period (days) 79.33018
 Mean orbital velocity (km/s) 3.27
 Orbital eccentricity 0.0283
 Orbital inclination (degrees) 14.72
 Escape (km/s) 0.586
 Albedo 0.2



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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