Saturn's Moon - Dione

D
ione was discovered in 1684 by Giovanni Cassini. It is
an icy body similar to Tethys
and Rhea. Its
density is 1.43 gm/cm3, which makes it the densest moon of Saturn
other than Titan.
Dione is probably composed of a rocky core making up one-third of the moon's
mass, with the rest water-ice. Its ice coverage is less than that of Tethys
and Rhea.
D
ione's icy surface includes heavily cratered terrain, moderately cratered
plains, lightly cratered plains, and whispy material. The heavily cratered
terrain has numerous craters greater than 100 kilometers in diameter. The
plains area tends to have craters less than 30 kilometers in diameter.
Some of the plains are heavily cratered while others are not. Much of the
heavily cratered terrain is located on the trailing
hemisphere, with the less cratered plains area existing on the leading
hemisphere. This is opposite from what some scientists expected. Shoemaker
and Wolfe proposed a cratering model for a tidally locked satellite with
the highest cratering rates on the leading hemisphere and the lowest on
the trailing hemisphere. This suggests that during the period of heavy
bombardment, Dione was tidally locked to Saturn in the opposite orientation.
Because Dione is relatively small, an impact causing a 35 kilometer (21
mile) crater could have spun the satellite. Since there are many craters
larger than 35 kilometers (21 miles), Dione could have been repeatedly
spun.
D
ione has probably been tidally locked in its current position for the
past several billion years. This is reflected in the average surface albedo
of the leading and trailing hemispheres. The surface albedo decreases from
the leading to the trailing hemispheres due to a higher micrometeor dusting
on the leading hemisphere.
T
he origin of the bright whispy material is somewhat obscure. Apparently,
it is material with a high albedo and is thin enough that it doesn't obscure
the surface feature underneath. It might have formed from eruptions along
cracks in Dione's surface that fell back to the surface as snow or ash.
| PHYSICAL DATA FOR DIONE |
| Mass (kg) |
1.05e + 21
|
| Mass (Earth = 1) |
1.7570e - 04
|
| Radius (km) |
560
|
| Radius (Earth = 1) |
8.7802e - 02
|
| Mean Density (g/cm3) |
1.43
|
| Mean Distance from Jupiter (km) |
377,400
|
| Magnitude (V0) |
10.4
|
| ORBITAL DATA FOR DIONE |
| Rotational period (days) |
2.736915
|
| Orbital period (days) |
>2.736915
|
| Mean orbital velocity (km/s) |
10.03
|
| Orbital eccentricity |
0.0022
|
| Orbital inclination (degrees) |
0.02
|
| Escape (km/s) |
0.500
|
| Albedo |
0.7
|
| 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. |
|