Misplaced Pages

255 Oppavia

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Main-belt asteroid

255 Oppavia
Discovery
Discovered byJohann Palisa
Discovery date31 March 1886
Designations
MPC designation(255) Oppavia
Pronunciation/ɒˈpeɪviə/
Named afterOpava
Alternative designationsA886 FB, 1904 EC
1924 TA, 1938 VC
1938 XC, 1945 GD
1951 SG
Minor planet categoryMain belt
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc129.86 yr (47,431 d)
Aphelion2.959 AU (442.6 Gm)
Perihelion2.533 AU (379.0 Gm)
Semi-major axis2.746 AU (410.8 Gm)
Eccentricity0.077427
Orbital period (sidereal)4.551 yr (1,662.1 d)
Average orbital speed17.98 km/s
Mean anomaly261.139°
Mean motion0° 12 59.735 / day
Inclination9.47209°
Longitude of ascending node13.6708°
Argument of perihelion156.011°
Physical characteristics
Dimensions57.40±1.5 km
Synodic rotation period19.499 h (0.8125 d)
Geometric albedo0.0374±0.002
Spectral typeX
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

  1. ^ "255 Oppavia". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 12 May 2016.
  2. ^ 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.
  3. Schmadel, Lutz D. (2013). Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 56. ISBN 9783662066157.
  4. 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.
  5. 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

Minor planets navigator
Small Solar System bodies
Minor planets
Asteroid
Distant minor planet
Comets
Other


Stub icon

This article about an asteroid native to the asteroid belt is a stub. You can help Misplaced Pages by expanding it.

Categories: