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hor_green_bar1.jpg Tethys hor_green_bar1.jpg


Tethys - courtesy NASATethys is an icy moon discovered by Giovanni Cassini in 1684. It is very similar to Dione and Rhea and has a density of 1.21 g/cm^3. This means that most of the satellite is made of water-ice. The surface has many craters and cracks, the result of repeated pummeling of meteorites s well as surface activity.

One landmark on the surface is the Ithaca Chasma that extends three-fourths around Tethys' circumference and is 65 kilometers (40 miles) wide. Many other younger trenches like this exists on the surface. The temperature is measured to be -187° C (-305° F).


PHYSICAL DATA FOR TETHYS
 Mass (kg) 7.55e + 20
 Mass (Earth = 1) 1.2634e - 04
 Radius (km) 530
 Radius (Earth = 1) 8.3098e - 02
 Mean Density (g/cm3) 1.21
 Mean Distance from Saturn (km) 294,660
 Magnitude (V0) 10.2



ORBITAL DATA FOR TETHYS
 Rotational period (days) 1.887802
 Orbital period (days) 1.887802
 Mean orbital velocity (km/s) 11.36
 Orbital eccentricity 0.0000
 Orbital inclination (degrees) 1.09
 Escape (km/s) 0.436
 Albedo 0.9



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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