Dione (moon)

From Conservapedia - Reading time: 4 min

---

Dione
Bright cliffs on Dione, taken by spacecraft Cassini
Date of discovery	March 21, 1684[1]
Name of discoverer	Giovanni Domenico Cassini[1]
Name origin	Titaness, sister of Kronos, mother (by Zeus) of Aphrodite[1]
Orbital characteristics
Primary	Saturn
Order from primary	13
Perikrone	376,570 km[2]
Apokrone	378,230 km[2]
Semi-major axis	377,400 km[3][4]
Orbital eccentricity	0.0022[3]
Sidereal month	2.736915 da[3][4]
Avg. orbital speed	10.03 km/s[5]
Inclination	0.02°[3] to Saturn's equator
Rotational characteristics
Sidereal day	2.736915 da[3]
Rotational speed	14.9 m/s[2]
Axial tilt	0°[3]
Physical characteristics
Mass	1.1 * 1021 kg[3]
Density	1477.4 kg/m³[6]
Mean radius	561.6 km[6]
Polar radius	560.3 km[6]
Surface gravity	0.223 m/s²[5]
Escape speed	0.5 km/s[5]
Surface area	3,940,800 km²[2]
Mean temperature	86.59 K[5]
Composition	Water-ice mantle and rocky core[5]
Color	Neutral gray
Albedo	0.7[3]

Dione or Saturn IV is the thirteenth innermost confirmed moon of Saturn and the fourth (or perhaps fifth) moon of Saturn to be discovered. It is also one of the seven moons of Saturn of dwarf planet size.

Discovery and naming[edit]

Giovanni Domenico Cassini discovered Dione, along with the moons Tethys, Rhea, and Iapetus, in the latter half of the seventeenth century, during the reign of "Sun-King" Louis XIV of France.^[1] Cassini named these moons the "Sidera Lodoicea" in honor of the king. Later generations (especially after the French Revolution) would not retain such regal flattery.^[7]

Sir John Herschel, son of the astronomer William Herschel, suggested the current names of the seven largest satellites of Saturn, including Rhea. Titan received a generic name, and the other six received names of the Titans of mythology. Dione was the sister of Kronos or Cronus and mother (by Zeus) of Aphrodite.^[8]

Orbital characteristics[edit]

Dione is in a somewhat circular orbit around Saturn, at an average distance of 377,400 km. Its sidereal month is about 2.74 Earth days.

Dione appears to be in a 2:1 orbital resonance with Enceladus, an inner moon. Some astronomers suggest that this causes significant tidal heating on Enceladus.^[9]

Co-orbital objects[edit]

Dione shares its orbit with two other moons that occupy its Trojan points, with Helene in the leading point and Polydeuces in the trailing point.

Rotational characteristics[edit]

Dione is in tidal lock with Saturn, and thus always keeps the same face toward Saturn. Hamilton estimates that Dione has been locked in its present orientation for several billions of years, because its 70% albedo is evenly distributed between the leading hemisphere and the trailing.^[5]

Physical characteristics[edit]

Dione is the third most dense moon of Saturn (after Enceladus and Titan). It likely consists of a silicate core and a water-ice mantle.

Surface[edit]

Surprisingly, most of Dione's craters are found on the trailing hemisphere, not the leading. Shoemaker and Wolfe have suggested, from their studies of the Galilean moons, that the leading hemisphere of any moon in tidal lock ought to have more craters than the trailing hemisphere.^[10]

This has led some astronomers to propose that, in the time when many bodies in the solar system underwent heavy bombardment, Dione was in tidal lock in an orientation opposite to that which Dione now has with respect to Saturn. Hamilton suggests that any object large enough to create an impact crater 35 km or wider in diameter would have given Dione sufficient energy to turn itself 180° about and come to a new tidal lock. He also points out that Dione has a number of craters more than 100 km in diameter.^[5]

Neukum et al. estimated that the surface of Dione, like those of several other moons of Saturn, must be geologically old on account of the number of craters found, and their distribution.^[11]

Dione also has multiple linear streaks on its trailing hemisphere. Astronomers once thought that these resulted from a massive remodeling of the surface of Dione, and that a later period of bombardment erased the streaks on the leading hemisphere. Data from the Cassini orbiter has disproved this hypothesis. The streaks are now known to be tectonic fractures, many of which slice through the impact craters and are therefore geologically younger than the craters.^[12][13]

Problems for uniformitarian theories posed by Dione[edit]

The greater concentration of impact craters on the trailing hemisphere defies the usual model for the bombardment of a body in tidal lock. Most astronomers therefore suggests that multiple impacts could have turned Dione about, perhaps multiple times, before Dione settled into its present orientation. But any object having enough momentum to turn the satellite about ought to have left it in a far more eccentric orbit than it is now in.

Observation and Exploration[edit]

The first spacecraft to visit Dione was Voyager 1, which took several high-quality images. The Cassini Orbiter has taken several images of much higher quality, especially on October 11, 2005, when Cassini made one targeted rendezvous with Dione. Mission planners have scheduled another rendezvous with Dione during the first two-year extension of the Cassini mission.

Gallery[edit]

• 

  Dione in the shadow of Saturn's rings

• 

  Deep canyons on Dione's trailing hemisphere

Video[edit]

• Video of Cassini's rendezvous with Dione on October 11, 2005.

References[edit]

v • d • e The Solar System Star Sol Terrestrial Planets Mercury · Venus · Earth · Mars Gas Giants Jupiter · Saturn · Uranus · Neptune Dwarf Planets Ceres · Haumea · Makemake · Pluto · Eris Asteroid Belt Major asteroids · C-type asteroids · S-type asteroids · M-type asteroids Trans-Neptunian Objects Kuiper belt · Scattered disk · Oort Cloud · Nemesis Satellites Moon · Phobos · Deimos · Io · Europa · Ganymede · Callisto · Mimas · Enceladus · Tethys · Dione · Rhea · Titan · Hyperion · Iapetus · Miranda · Ariel · Umbriel · Titania · Oberon · Triton · Nereid · Charon · Nix · Hydra · Dysnomia Categories