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892 Seeligeria

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892 Seeligeria
Discovery
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date31 May 1918
Designations
(892) Seeligeria
1918 DR
main-belt · (outer)
Alauda[1]
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc97.87 yr (35747 days)
Aphelion3.5632 AU (533.05 Gm)
Perihelion2.8970 AU (433.39 Gm)
3.2301 AU (483.22 Gm)
Eccentricity0.10312
5.81 yr (2120.4 d)
83.4390°
0° 10m 11.208s / day
Inclination21.335°
175.926°
287.377°
Earth MOID1.98994 AU (297.691 Gm)
Jupiter MOID1.66162 AU (248.575 Gm)
TJupiter3.071
Physical characteristics
38.01±0.8 km
15.78 h,[3] 41.40 h (1.725 d)[2]
0.0485±0.002
9.7

892 Seeligeria is dark Alauda asteroid from the outer region of the asteroid belt that was discovered by German astronomer Max Wolf on May 31, 1918 in Heidelberg and assigned a preliminary designation of 1918 DR. It was named after German astronomer Hugo Hans von Seeliger.

Photometric observations at the Oakley Observatory in Terre Haute, Indiana, during 2007 were used to build a light curve for 892 Seeligeria. The asteroid displayed a rotation period of 15.78 ± 0.04 hours and a brightness variation of 0.35 ± 0.07 in magnitude.[3]

Seeligeria is a member of the Alauda family (902),[1] a large family of typically bright carbonaceous asteroids and named after its parent body, 702 Alauda.[4]: 23 

References

  1. ^ a b "Small Bodies Data Ferret". Nesvorny HCM Asteroid Families V3.0. Retrieved 7 November 2017.
  2. ^ a b "892 Seeligeria (1918 DR)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 3 May 2016.
  3. ^ a b Shipley, Heath; et al. (September 2008), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: September 2007" (PDF), The Minor Planet Bulletin, vol. 35, no. 3, pp. 99–101, Bibcode:2008MPBu...35...99S, archived from the original (PDF) on 2013-06-02, retrieved 2013-03-23. {{citation}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  4. ^ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families" (PDF). Asteroids IV: 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. Retrieved 7 November 2017.