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1452 Hunnia

From Wikipedia, the free encyclopedia
Carbonaceous Meliboean asteroid

1452 Hunnia
Discovery[1]
Discovered byG. Kulin
Discovery siteKonkoly Obs.
Discovery date26 February 1938
Designations
(1452) Hunnia
Pronunciation/ˈhʌniə/[2]
Named after
Hungarians[3]
(Nation of Hungaria)
1938 DZ1 · 1953 YA
1953 YM
main-belt · (outer)[4]
Meliboea[5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc79.35 yr (28,981 days)
Aphelion3.7395AU
Perihelion2.4798 AU
3.1096 AU
Eccentricity0.2025
5.48yr (2,003 days)
194.78°
0° 10m 46.92s / day
Inclination14.211°
21.352°
94.487°
Physical characteristics
Dimensions18.76±5.25 km[6]
20.00±6.07 km[7]
20.910±0.107 km[8][9]
21.16 km(calculated)[4]
17.2h[10]
0.0435±0.0036[9]
0.046±0.003[8]
0.05±0.07[7]
0.057(assumed)[4]
0.06±0.04[6]
C(assumed)[4]
12.10[1][4][6][9] · 12.19[7]

1452 Hunnia, provisional designation1938 DZ1, is a carbonaceous Meliboeanasteroid from the outer regions of theasteroid belt, approximately 20 kilometers in diameter. It was discovered on 26 February 1938, by Hungarian astronomerGyörgy Kulin at theKonkoly Observatory in Budapest.[11] The asteroid was named in honor of theHungarian nation.[3]

Orbit and classification

[edit]

Hunnia is a member of theMeliboea family (604),[5] a smallerasteroid family of a few hundred carbonaceousouter-belt asteroids, named after137 Meliboea.[12]: 23  It orbits the Sun at a distance of 2.5–3.7 AU once every 5 years and 6 months (2,003 days). Its orbit has aneccentricity of 0.20 and aninclination of 14° with respect to theecliptic.[1]

The body'sobservation arc begins atGoethe Link Observatory in March 1949, more than 11 years after its official discovery observation at Konkoly.[11] (The large time span withoutastrometric follow-up observations coincides with the period ofWWII.)

Physical characteristics

[edit]

Hunnia is an assumed carbonaceousC-type asteroid,[4] in agreement with the overallspectral type of theMeliboea family.[12]: 23 

Rotation period

[edit]

Between February and March 1998, a rotationallightcurve ofHunnia was obtained from photometric observations by Hungarian astronomersKrisztián Sárneczky,Gyula Szabó andLászló Kiss. Lightcurve analysis gave arotation period of 17.2 hours with a brightness amplitude of 0.34magnitude (U=2).[10] No other lightcurves have since been obtained.[4]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Hunnia measures between 18.76 and 20.910 kilometers in diameter and its surface has analbedo between 0.0435 and 0.06.[6][7][8][9]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 21.16 kilometers based on anabsolute magnitude of 12.1.[4]

Naming

[edit]

Thisminor planet was named in honor of theHungarian nation.[3] Also known as Magyars, the Hungarians are believed to be ofHunnic heritage. The officialnaming citation was published by theMinor Planet Center on 1 February 1980 (M.P.C. 5182).[13]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1452 Hunnia (1938 DZ1)" (2017-07-02 last obs.).Jet Propulsion Laboratory. Retrieved21 October 2017.
  2. ^"Hun, Hunnian".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcSchmadel, Lutz D. (2007). "(1452) Hunnia".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 116.doi:10.1007/978-3-540-29925-7_1453.ISBN 978-3-540-00238-3.
  4. ^abcdefgh"LCDB Data for (1452) Hunnia". Asteroid Lightcurve Database (LCDB). Retrieved21 October 2017.
  5. ^ab"Asteroid 1452 Hunnia – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  6. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117. Retrieved21 October 2017.
  7. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  8. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68. Retrieved21 October 2017.
  9. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.
  10. ^abSárneczky, K.; Szabó, Gy.; Kiss, L. L. (June 1999)."CCD observations of 11 faint asteroids"(PDF).Astronomy and Astrophysics Supplement.137 (2):363–368.Bibcode:1999A&AS..137..363S.doi:10.1051/aas:1999251. Retrieved21 October 2017.
  11. ^ab"1452 Hunnia (1938 DZ1)".Minor Planet Center. Retrieved21 October 2017.
  12. ^abNesvorný, 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 978-0-8165-3213-1.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved21 October 2017.

External links

[edit]
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