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108 Hecuba
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Main-belt asteroid
yes (108) Hecuba #D6D6D6 108 Hecuba 108 Hecuba.png 108 Hecuba 3D Lightcurve model R. Luther 2 April 1869 ' h ɛ k j ᵿ b əHecuba Hecuba Main belt 31 July 2016 (JD 2457600.5) 3.23912 AU Gm on 3.05922 AU Gm on 3.4190 AU Gm on on 0.055539 5.83 yr (2129.3 d) 4.2204° 350.014° 204.634° 166.649° 16.53 km/s 64.97 4.4 km65 kmhttp://www.psi.edu/pds/archive/simps.html IRAS Minor Planet Survey (IMPS) 2005-12-11 dead https://archive.today/20051222220311/http://www.psi.edu/pds/archive/simps.html 2005-12-22 ~3.9×1017 kg (estimate) ~2.7 g/cm3 (estimate) ~0.025 m/s² (estimate) ~0.040 km/s (estimate) 14.256 h d on on0.60 d or 1.20 d S 8.09 0.2431 0.037 Kelvin ~148 215 Celsius -58 0.169069 ms / day 135.87 yr (49628 d) 0 2.05833 AU Gm on 1.55152 AU Gm on 3.178
108 Hecuba is a fairly large and bright main-belt asteroid. It was discovered by Karl Theodor Robert Luther on 2 April 1869, and named after Hecuba, wife of King Priam in the legends of the Trojan War in Greek Mythology. This object is orbiting the Sun with a period of 5.83 years and an eccentricity of 0.06. 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.
In the 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 Colorado Springs, Colorado in during 2007 produced a light curve with a period of 17.859 ± 0.005 hours with a brightness variation of 0.11 ± 0.02 in magnitude.
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.January 2021
References
A Physical Study of the Asteroid 108 Hecuba
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Astronomical Society of the Pacific
Yoshihide Kozai
Richard P. Binzel
Tomohiro Hirayama
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Discovery Circumstances
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NASA Jet Propulsion Laboratory
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Francesca E.
DeMeo
Richard P.
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Stephen M.
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Bus
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Icarus
202
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10.1016/j.icarus.2009.02.005
2009Icar..202..160D
http://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016%252Fj.icarus.2009.02.005.pdf
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https://web.archive.org/web/20140317200310/https://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016/j.icarus.2009.02.005.pdf
2014-03-17 See appendix A.
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Sophia Levy
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DeMeo
Francesca E.
Binzel
Richard P.
Slivan
Stephen M.
Bus
Schelte J.
1
An extension of the Bus asteroid taxonomy into the near-infrared
Icarus
202
1
160–180
July 2009
10.1016/j.icarus.2009.02.005
2009Icar..202..160D
http://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016%252Fj.icarus.2009.02.005.pdf
2013-04-08
.
dead
https://web.archive.org/web/20140317200310/https://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016/j.icarus.2009.02.005.pdf
2014-03-17 See appendix A.
External links
Lightcurve plot of 108 Hecuba, Palmer Divide Observatory, B. D. Warner (2007)
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
108
October 2019
107 Camilla 108 109 Felicitas
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Category:Discoveries by Robert Luther
Category:Named minor planets
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