106 Dione

106 Dione
Discovery
Discovered by James Craig Watson
Discovery date October 10, 1868
Designations
Named after
Dione
Main belt
Orbital characteristics[1]
Epoch December 31, 2006 (JD 2454100.5)
Aphelion 556.376 Gm (3.719 AU)
Perihelion 391.585 Gm (2.618 AU)
473.981 Gm (3.168 AU)
Eccentricity 0.174
2059.923 d (5.64 a)
16.61 km/s
161.899°
Inclination 4.616°
62.400°
329.534°
Physical characteristics
Dimensions 147.17 ± 3.34[2] km
Mass (3.06 ± 1.54) × 1018 kg[2]
Mean density
1.83 ± 0.92[2] g/cm3
0.0410 m/s²
0.0775 km/s
16.26 ± 0.02[3] h
Temperature ~156 K
Spectral type
G (Tholen)
Cgh (Bus)[4]
7.41

    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,[5] 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.[6]

    Dione was observed to occult a dim star on January 19, 1983, by observers in Denmark, Germany and the Netherlands. A diameter of 147 ± 3 km was deduced,[7] closely matching the value acquired by the IRAS satellite.

    Measurements made with the IRAS observatory give a diameter of 169.92 ± 7.86 km and a geometric albedo of 0.07 ± 0.01. By comparison, the MIPS photometer on the Spitzer Space Telescope gives a diameter of 168.72 ± 8.89 km and a geometric albedo of 0.07 ± 0.01. When the asteroid was observed occulting a star, the results showed a diameter of 176.7 ± 0.4 km.[8]

    Photometric observations of this asteroid collected during 2004–2005 show a rotation period of 16.26 ± 0.02 hours with a brightness variation of 0.08 ± 0.02 magnitude.[3]

    One of Saturn's satellites is also named Dione.

    References

    1. Yeomans, Donald K., "106 Dione", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), retrieved 2013-03-25.
    2. 1 2 3 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
    3. 1 2 Pray, Donald P. (September 2005), "Lightcurve analysis of asteroids 106, 752, 847, 1057, 1630, 1670, 1927 1936, 2426, 2612, 2647, 4087, 5635, 5692, and 6235", The Minor Planet Bulletin 32 (3): 48–51, Bibcode:2005MPBu...32...48P.
    4. DeMeo, Francesca E.; et al. (2011), "An extension of the Bus asteroid taxonomy into the near-infrared" (PDF), Icarus 202 (1): 160–180, Bibcode:2009Icar..202..160D, doi:10.1016/j.icarus.2009.02.005, retrieved 2013-03-22. See appendix A.
    5. "Numbered Minor Planets 1–5000", Discovery Circumstances (IAU Minor Planet center), retrieved 2013-04-07.
    6. McDonald, Sophia Levy (June 1948), "General perturbations and mean elements, with representations of 35 minor planets of the Hecuba group", Astronomical Journal 53, p. 199, Bibcode:1948AJ.....53..199M, doi:10.1086/106097.
    7. Kristensen, L. K. (1984), "The diameter of (106) Dione", Astronomische Nachrichten 305 (4), pp. 207–211, Bibcode:1984AN....305..207K, doi:10.1002/asna.2113050410.
    8. Ryan, Erin Lee; et al. (April 2012), "The Kilometer-Sized Main Belt Asteroid Population as Revealed by Spitzer", eprint arXiv, arXiv:1204.1116, Bibcode:2012arXiv1204.1116R.

    External links


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