354 Eleonora
Eleonora (minor planet designation: 354 Eleonora) is a large, stony main-belt asteroid that was discovered by the French astronomer Auguste Charlois on January 17, 1893, in Nice.[4]
A three-dimensional model of 354 Eleonora based on its light curve | |
Discovery | |
---|---|
Discovered by | Auguste Charlois |
Discovery date | 17 January 1893 |
Designations | |
(354) Eleonora | |
Pronunciation | /ɛliəˈnɔːrə/[1] |
1893 A | |
Main belt | |
Adjectives | Eleonorian |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 123.16 yr (44983 d) |
Aphelion | 3.1188 AU (466.57 Gm) |
Perihelion | 2.47676 AU (370.518 Gm) |
2.79777 AU (418.540 Gm) | |
Eccentricity | 0.11474 |
4.68 yr (1709.3 d) | |
123.762° | |
0° 12m 38.196s / day | |
Inclination | 18.403° |
140.37° | |
5.5215° | |
Physical characteristics | |
Dimensions | 155.17±8.5 km[2] 154.34 ± 5.65 km[3] |
Mass | (7.18 ± 2.57) × 1018 kg[3] |
Mean density | 3.73 ± 1.39 g/cm3[3] |
4.277 h (0.1782 d) | |
0.1948±0.023 | |
S | |
6.44 | |
Photometric observations of this asteroid gave a light curve with a period of 13.623 hours. The data was used to construct a model for the asteroid, revealing it to be a regular-shaped object, spinning about a pole with ecliptic coordinates (β, λ) = (+20°, 356°), although this is with an accuracy of only ±10°. The ratio of the major to minor axes lengths is roughly equal to 1.2.[5] It is classified as an S-type asteroid and has an estimated size of 154.34 km.[3] The spectrum of 354 Eleonora reveals the strong presence of the mineral olivine, a relatively rarity in the asteroid belt.[6]
During favorable oppositions, such as in 1968 and 2010, Eleonora can reach an apparent magnitude of +9.31.
References
- "Eleonora". Oxford English Dictionary (3rd ed.). Oxford University Press. September 2005. (Subscription or UK public library membership required.)
- Yeomans, Donald K., "354 Eleonora", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 11 May 2016.
- 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.
- "Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 7 April 2013.
- Kaasalainen, M.; et al. (October 2002), "Models of Twenty Asteroids from Photometric Data", Icarus, 159 (2), pp. 369–395, Bibcode:2002Icar..159..369K, doi:10.1006/icar.2002.6907.
- Burbine, T. H.; et al. (July 2000), "The Nature of Olivine Asteroids", Meteoritics & Planetary Science, 35, pp. A35, Bibcode:2000M&PSA..35R..35B, doi:10.1111/j.1945-5100.2000.tb01796.x.
External links
- 354 Eleonora at AstDyS-2, Asteroids—Dynamic Site
- 354 Eleonora at the JPL Small-Body Database