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108 Hecuba
Main-belt asteroid
Main-belt asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| mpc_name | (108) Hecuba |
| background | #D6D6D6 |
| name | 108 Hecuba |
| image | 108 Hecuba.png |
| caption | 108 Hecuba 3D Lightcurve model. |
| discoverer | R. Luther |
| discovered | 2 April 1869 |
| pronounced | |
| named_after | Hecuba |
| mp_category | Main belt |
| epoch | 31 July 2016 (JD 2457600.5) |
| orbit_ref | |
| semimajor | 3.23912 AU |
| perihelion | 3.05922 AU |
| aphelion | 3.4190 AU |
| eccentricity | 0.055539 |
| period | 5.83 yr (2129.3 d) |
| inclination | 4.2204° |
| asc_node | 350.014° |
| arg_peri | 204.634° |
| mean_anomaly | 166.649° |
| avg_speed | 16.53 km/s |
| dimensions | |
| 65 km | |
| mass | ~3.9×1017 kg *(estimate)* |
| density | ~2.7 g/cm3 *(estimate)* |
| surface_grav | ~0.025 m/s² *(estimate)* |
| escape_velocity | ~0.040 km/s *(estimate)* |
| rotation | 14.256 h |
| 0.60 d or 1.20 d | |
| spectral_type | S |
| abs_magnitude | 8.09 |
| albedo | |
| temp_name1 | Kelvin |
| mean_temp_1 | ~148 |
| max_temp_1 | 215 |
| temp_name2 | Celsius |
| max_temp_2 | -58 |
| mean_motion | / day |
| observation_arc | 135.87 yr (49628 d) |
| uncertainty | 0 |
| moid | 2.05833 AU |
| jupiter_moid | 1.55152 AU |
| tisserand | 3.178 |
65 km 0.60 d or 1.20 d
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.
References
References
- {{dict.com. Hecuba
- "IRAS Minor Planet Survey (IMPS)".
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
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