Discovery | |
---|---|
Discovered by | Johann Palisa |
Discovery date | 31 March 1886 |
Designations | |
MPC designation | (255) Oppavia |
Pronunciation | /ɒˈpeɪviə/ |
Named after | Opava |
Alternative designations | A886 FB, 1904 EC 1924 TA, 1938 VC 1938 XC, 1945 GD 1951 SG |
Minor planet category | Main belt |
Orbital characteristics | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 129.86 yr (47,431 d) |
Aphelion | 2.959 AU (442.6 Gm) |
Perihelion | 2.533 AU (379.0 Gm) |
Semi-major axis | 2.746 AU (410.8 Gm) |
Eccentricity | 0.077427 |
Orbital period (sidereal) | 4.551 yr (1,662.1 d) |
Average orbital speed | 17.98 km/s |
Mean anomaly | 261.139° |
Mean motion | 0° 12 59.735 / day |
Inclination | 9.47209° |
Longitude of ascending node | 13.6708° |
Argument of perihelion | 156.011° |
Physical characteristics | |
Dimensions | 57.40±1.5 km |
Synodic rotation period | 19.499 h (0.8125 d) |
Geometric albedo | 0.0374±0.002 |
Spectral type | X |
Absolute magnitude (H) | 10.39 |
255 Oppavia is a sizeable Main belt asteroid. It was discovered by Austrian astronomer Johann Palisa on 31 March 1886 in Vienna and was named after Opava, a town in the Czech Republic, then part of Austria-Hungary, where Palisa was born. It is orbiting the Sun at a distance of 2.75 AU with an orbital eccentricity (ovalness) of 0.077 and a period of 4.55 yr. The orbital plane is inclined by an angle of 9.47° to the plane of the ecliptic.
Photometric observations made during 2013 indicate a synodic rotation period of 19.499±0.001 h with an amplitude of 0.16±0.02 in magnitude. The unusual light curve shows three uneven minima and maxima per cycle. In 1995, 255 Oppavia was suggested as a peripheral member of the now defunct Ceres asteroid family, but was found to be an unrelated interloper on the basis of its non-matching spectral type. It classified as a dark X-type asteroid in the Tholen taxonomy.
References
- ^ "255 Oppavia". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 12 May 2016.
- ^ Lazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (November 2004). "SOS: the visible spectroscopic survey of 820 asteroids" (PDF). Icarus. 172 (1): 179–220. Bibcode:2004Icar..172..179L. doi:10.1016/j.icarus.2004.06.006. Retrieved 9 March 2022.
- Schmadel, Lutz D. (2013). Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 56. ISBN 9783662066157.
- Pilcher, Frederick (July 2013). "Rotation Period Determinations for 102 Miriam, 108 Hecuba, 221 Eos 225 Oppavia, and 745 Mauritia, and a Note on 871 Amneris". Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers. 40 (3): 158–160. Bibcode:2013MPBu...40..158P.
- Morbidelli, A.; et al. (November 1995). "Asteroid Families Close to Mean Motion Resonances: Dynamical Effects and Physical Implications" (PDF). Icarus. 118 (1): 132–154. Bibcode:1995Icar..118..132M. doi:10.1006/icar.1995.1181. Retrieved 9 April 2022.
External links
- The Asteroid Orbital Elements Database
- Minor Planet Discovery Circumstances
- Asteroid Lightcurve Data File
- Orbital simulation of asteroid 255 Oppavia
- Asteroid 255 Oppavia in Planetky z našich luhů a hájů (in Czech)
- 255 Oppavia at AstDyS-2, Asteroids—Dynamic Site
- 255 Oppavia at the JPL Small-Body Database
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