108 Hecuba is a fairly large and bright main-belt asteroid. It was discovered by Karl Theodor Robert Luther on April 2, 1869, and named after [5 ] Hecuba, wife of King Priam in the legends of the Trojan War in Greek Mythology. It became the first asteroid discovered to orbit near a 2:1 mean-motion resonance with the planet Jupiter, and is the namesake of the Hecuba group of asteroids. [6 ] [7 ]
Tholen classification system, it is categorized as a stony S-type asteroid, while the Bus asteroid taxonomy system lists it as an Sw asteroid. Observations performed at the Palmer Divide Observatory in [8 ] Colorado Springs, Colorado in during 2007 produced a light curve with a period of 17.859 ± 0.005 hours with a brightness range of 0.11 ± 0.02 in magnitude. [9 ]
Hecuba orbits within the
Hygiea family of asteroids but is not otherwise related to other family members because it has a silicate composition; Hygieas are dark C-type asteroids.
References [ edit ]
^ Yeomans, Donald K., "108 Hecuba", JPL Small-Body Database Browser ( NASA Jet Propulsion Laboratory) , retrieved . 2013-03-25
^ Krasinsky, G. A. et al. (July 2002), "Hidden Mass in the Asteroid Belt", Icarus 158 (1): 98–105, Bibcode: 2002Icar..158...98K, doi: 10.1006/icar.2002.6837. See appendix A.
^ Harris, A.W.; Warner, B.D.; Pravec, P., eds. (2012), "Lightcurve Derived Data", Planetary Data System (NASA) , retrieved . 2013-03-22
^ DeMeo, Francesca E. et al. (2011), "An extension of the Bus asteroid taxonomy into the near-infrared", Icarus 202 (1): 160–180, Bibcode: 2009Icar..202..160D, doi: 10.1016/j.icarus.2009.02.005. See appendix A.
^ "Numbered Minor Planets 1–5000", Discovery Circumstances (IAU Minor Planet center) , retrieved . 2013-04-07
^ Brož, M.; Vokrouhlický, D.; Roig, F.; Nesvorný, D.; Bottke, W. F.; Morbidelli, A. (June 2005), "Yarkovsky origin of the unstable asteroids in the 2/1 mean motion resonance with Jupiter", Monthly Notices of the Royal Astronomical Society 359 (4), Bibcode: 2005MNRAS.359.1437B, doi: 10.1111/j.1365-2966.2005.08995.x.
^ McDonald, Sophia Levy (June 1948), "General perturbations and mean elements, with representations of 35 minor planets of the Hecuba group", Astronomical Journal 53: 199, Bibcode: 1948AJ.....53..199M, doi: 10.1086/106097.
^ DeMeo, Francesca E. et al. (July 2009), "An extension of the Bus asteroid taxonomy into the near-infrared", Icarus 202 (1): 160–180, Bibcode: 2009Icar..202..160D, doi: 10.1016/j.icarus.2009.02.005 , retrieved . 2013-04-08 See appendix A.
^ Warner, Brian D. (September 2007), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, Bibcode: 2007MPBu...34...72W.