835 Olivia

835 Olivia
Discovery [1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date23 September 1967
Designations
(835) Olivia
Named after
unknown [2]
A916 SH · 1964 BA
1979 ST · 1916 AE
main-belt [1][3] · (outer)
background [4][5]
Orbital characteristics [3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc103.29 yr (37,725 d)
Aphelion3.5001 AU
Perihelion2.9366 AU
3.2183 AU
Eccentricity0.0875
5.77 yr (2,109 d)
1.9258°
0° 10m 14.52s / day
Inclination3.6998°
308.48°
66.972°
Physical characteristics
undetermined [9]
  • 0.0242±0.004[7]
  • 0.025±0.001[8]
  • 0.033±0.006[6]
C (SDSS-MOC)[10]
11.5[1][3]

835 Olivia (prov. designation: A916 SH or 1916 AE) is a dark background asteroid from the outer regions of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory on 23 September 1916.[1] The carbonaceous C-type asteroid measures approximately 35 kilometers (22 miles) in diameter, and is one of few low-numbered asteroids with an undetermined rotation period. Any reference to the origin of the asteroid's name is unknown.[2]

Orbit and classification

Olivia is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[4][5] It orbits the Sun in the outer asteroid belt at a distance of 2.9–3.5 AU once every 5 years and 9 months (2,109 days; semi-major axis of 3.22 AU). Its orbit has an eccentricity of 0.09 and an inclination of 4° with respect to the ecliptic.[3] The body's observation arc begins at the Bergedorf Observatory on 30 September 1916, one week after its official discovery observation at Heidelberg.[1]

Naming

Any reference of this minor planet's name to a person or occurrence is unknown.[2]

Unknown meaning

Among the many thousands of named asteroids, Olivia is one of 120 planets for which no official naming citation has been published. All of these asteroids have low numbers, the first one being 164 Eva. The last asteroid with a name of unknown meaning is 1514 Ricouxa. They were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth.[11]

Physical characteristics

In the SDSS-based taxonomy, Olivia is a common, carbonaceous C-type asteroid, with a notably low albedo (see below).[10]

Rotation period

As of 2020, no rotational lightcurve of Olivia has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.[3][5][9][12]

Diameter and albedo

According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), the Infrared Astronomical Satellite IRAS, and the Japanese Akari satellite, Olivia measures (30.418±0.082), (35.65±2.3) and (36.05±0.91) kilometers in diameter and its surface has a notably low albedo of (0.033±0.006), (0.0242±0.004) and (0.025±0.001), respectively.[6][7][8] Alternative mean-diameters published by the WISE team include (35.367±13.540 km) and (44.231±0.847 km) with corresponding albedos of (0.031±0.031) and (0.025±0.005).[5]

References

  1. ^ a b c d e "835 Olivia (A916 SH)". Minor Planet Center. Retrieved 9 March 2020.
  2. ^ a b c Schmadel, Lutz D. (2007). "(835) Olivia". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 77. doi:10.1007/978-3-540-29925-7_836. ISBN 978-3-540-00238-3.
  3. ^ a b c d e "JPL Small-Body Database Browser: 835 Olivia (A916 SH)" (2020-01-06 last obs.). Jet Propulsion Laboratory. Retrieved 9 March 2020.
  4. ^ a b "Asteroid 835 Olivia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 9 March 2020.
  5. ^ a b c d "Asteroid 835 Olivia". Small Bodies Data Ferret. Retrieved 9 March 2020.
  6. ^ a b c Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121.
  7. ^ a b c Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T. Retrieved 8 March 2020.
  8. ^ a b c Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)
  9. ^ a b "LCDB Data for (835) Olivia". Asteroid Lightcurve Database (LCDB). Retrieved 9 March 2020.
  10. ^ a b Carvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010). "SDSS-based taxonomic classification and orbital distribution of main belt asteroids". Astronomy and Astrophysics. 510: 12. Bibcode:2010A&A...510A..43C. doi:10.1051/0004-6361/200913322. Retrieved 9 March 2020. (PDS data set)
  11. ^ Schmadel, Lutz D. (2007). "Appendix 11 – Minor Planet Names with Unknown Meaning". Dictionary of Minor Planet Names – Fifth Revised and Enlarged revision. Springer Berlin Heidelberg. pp. 927–929. ISBN 978-3-540-00238-3.
  12. ^ Behrend, Raoul. "Asteroids and comets rotation curves, CdR". Geneva Observatory. Retrieved 9 March 2020.