51983 Hönig

51983 Hönig
Discovery [1]
Discovered byC. W. Juels
P. R. Holvorcem
Discovery siteFountain Hills Obs
Discovery date19 September 2001
Designations
(51983) Hönig
Named after
Sebastian Hönig [2]
(discoverer of minor planets)
2001 SZ8
main-belt · (outer) [1]
Hilda (group and family) [3][4]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc63.07 yr (23,035 days)
Aphelion4.4369 AU
Perihelion3.4875 AU
3.9622 AU
Eccentricity0.1198
7.89 yr (2,881 days)
52.159°
0° 7m 30s / day
Inclination9.3988°
10.012°
295.11°
Physical characteristics
Dimensions13 km (estimate at 0.06)[5]
13.2[1]

51983 Hönig (provisional designation 2001 SZ8) is a Hildian asteroid from the outermost regions of the asteroid belt, approximately 13 kilometers in diameter. It was discovered on 19 September 2001, by astronomers Charles Juels and Paulo Holvorcem at the Fountain Hills Observatory (678) in Arizona, United States.[3] The asteroid was named after German astronomer Sebastian Hönig.[2]

Orbit and classification

Hönig is a member of the Hilda family (001),[4] a collisional asteroid family of carbonaceous asteroids within the larger dynamical Hilda group.[3][6]: 23  It orbits the Sun in the outermost region of the main belt at a distance of 3.5–4.4 AU once every 7 years and 11 months (2,881 days). Its orbit has an eccentricity of 0.12 and an inclination of 9° with respect to the ecliptic.[1]

The body's observation arc begins at Palomar Observatory in September 1954, on precovery images found by the Digitized Sky Survey.[3]

Physical characteristics

The asteroid's spectral type is unknown. The Hilda family's overall spectral type is that of a carbonaceous C-type.[6]: 23 

Diameter and albedo

Hönig has not been observed by any space-based telescope such as the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite or the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer. Based on an assumed albedo of 0.06 – derived from the parent body of the Hilda family, 153 Hilda, which is also typical for carbonaceous asteroids – Hönig measures 13 kilometers in diameter for an absolute magnitude of 13.2.[5]

Rotation period

As of 2017, no rotational lightcurve of Hönig has been obtained from photometric observations. The body's rotation period, pole axis and shape remain unknown.[7]

Naming

This minor planet was named after German astronomer Sebastian F. Hönig (born 1978), a prolific discoverer of minor planets and several comets,[2] including the hyperbolic comet C/2002 O4,[8] which disintegrated shortly after its discovery in 2002.[9] The official naming citation was published by the Minor Planet Center on 7 January 2004 (M.P.C. 50465).[10]

References

  1. ^ a b c d e "JPL Small-Body Database Browser: 51983 Honig (2001 SZ8)" (2017-09-30 last obs.). Jet Propulsion Laboratory. Retrieved 25 October 2017.
  2. ^ a b c Schmadel, Lutz D. (2006). "(51983) Hönig [3.95, 0.12, 9.4]". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 216. doi:10.1007/978-3-540-34361-5_2560. ISBN 978-3-540-34361-5.
  3. ^ a b c d "51983 Honig (2001 SZ8)". Minor Planet Center. Retrieved 25 October 2017.
  4. ^ a b "Asteroid 51983 Honig – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 27 October 2019.
  5. ^ a b "Asteroid Size Estimator". CNEOS – NASA/JPL. Retrieved 25 October 2017.
  6. ^ a b Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131. S2CID 119280014.
  7. ^ "LCDB Data for (51983) Hönig". Asteroid Lightcurve Database (LCDB). Retrieved 25 October 2017.
  8. ^ "JPL Small-Body Database Browser: C/2002 O4 (Hoenig)" (2002-09-23 last obs.). Jet Propulsion Laboratory. Retrieved 25 October 2017.
  9. ^ Sekanina, Z. (October 2002). "What Happened to Comet C/2002 O4 (Hoenig)?". International Comet Quarterly. 24: 223–236. Bibcode:2002ICQ....24..223S. Retrieved 25 October 2017.
  10. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 25 October 2017.