106 Dione Explained

Minorplanet:yes
Background:
  1. D6D6D6
106 Dione
Discovered:10 October 1868
Mpc Name:(106) Dione
Alt Names:A868 TA, 1902 TA
Pronounced:[1]
Epoch:31 July 2016 (JD 2457600.5)
Semimajor:3.17451AU
Perihelion:2.64584AU
Aphelion:3.7032abbr=onNaNabbr=on
Eccentricity:0.16653
Period:5.66 yr (2065.9 d)
Inclination:4.5972°
Asc Node:62.163°
Arg Peri:329.725°
Avg Speed:16.61 km/s
Dimensions:
Surface Grav:0.0410 m/s²
Escape Velocity:0.0775 km/s
Rotation:16.26abbr=onNaNabbr=on
16.26 ± 0.02 h
Spectral Type:G (Tholen)
Cgh (Bus)
Abs Magnitude:7.41
Mean Motion: / day
Observation Arc:145.03 yr (52972 d)
Uncertainty:0
Moid:1.65175AU
Jupiter Moid:1.73379AU
Tisserand:3.175

106 Dione is a large main-belt asteroid. It probably has a composition similar to 1 Ceres. It was discovered by J. C. Watson on October 10, 1868, and named after Dione, a Titaness in Greek mythology who was sometimes said to have been the mother of Aphrodite, the Greek goddess of love and beauty. It is listed as a member of the Hecuba group of asteroids that orbit near the 2:1 mean-motion resonance with Jupiter. The orbital period for this object is 5.66 years and it has an eccentricity of 0.17.

Measurements made with the IRAS observatory give a diameter of and a geometric albedo of . By comparison, the MIPS photometer on the Spitzer Space Telescope gives a diameter of and a geometric albedo of . Dione was observed to occult a dim star on January 19, 1983, by observers in Denmark, Germany and the Netherlands. A diameter of was deduced, closely matching the value acquired by the IRAS satellite. As of 2012, the mean diameter derived through occultation measurements is .

Photometric observations of this asteroid collected during 2004–2005 show a rotation period of hours with a brightness variation of magnitude. It is classified as a rare G-type asteroid, suggesting it has a carbonaceous composition with phyllosilicate minerals also being detected.

Notes and References

  1. Noah Webster (1884) A Practical Dictionary of the English Language