1452 Hunnia, provisional designation 1938 DZ1, is a carbonaceous Meliboean asteroid from the outer regions of the asteroid belt, approximately 20 kilometers in diameter. It was discovered on 26 February 1938, by Hungarian astronomer György Kulin at the Konkoly Observatory in Budapest.[11] The asteroid was named in honor of the Hungarian nation.[2]
Contents
1Orbit and classification
2Physical characteristics
2.1Rotation period
2.2Diameter and albedo
3Naming
4References
5External links
Orbit and classification
Hunnia is a member of the Meliboea family (604),[4] a smaller asteroid family of a few hundred carbonaceous outer-belt asteroids, named after 137 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 an eccentricity of 0.20 and an inclination of 14° with respect to the ecliptic.[1]
The body's observation arc begins at Goethe Link Observatory in March 1949, more than 11 years after its official discovery observation at Konkoly.[11] (The large time span without astrometric follow-up observations coincides with the period of WWII.)
Physical characteristics
Hunnia is an assumed carbonaceous C-type asteroid,[3] in agreement with the overall spectral type of the Meliboea family.[12]:23
Rotation period
Between February and March 1998, a rotational lightcurve of Hunnia was obtained from photometric observations by Hungarian astronomers Krisztián Sárneczky, Gyula Szabó and László Kiss. Lightcurve analysis gave a rotation period of 17.2 hours with a brightness amplitude of 0.34 magnitude ({{{1}}}).[10] No other lightcurves have since been obtained.[3]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Hunnia measures between 18.76 and 20.910 kilometers in diameter and its surface has an albedo between 0.0435 and 0.06.[6][7][8][9]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 21.16 kilometers based on an absolute magnitude of 12.1.[3]
Naming
This minor planet was named in honor of the Hungarian nation.[2] Also known as Magyars, the Hungarians are believed to be of Hunnic heritage. The official naming citation was published by the Minor Planet Center on 1 February 1980 (M.P.C. 5182).[13]
↑ 2.02.12.2Schmadel, Lutz D. (2007). "(1452) Hunnia". Dictionary of Minor Planet Names – (1452) Hunnia. Springer Berlin Heidelberg. p. 116. doi:10.1007/978-3-540-29925-7_1453. ISBN 978-3-540-00238-3.
↑ 3.03.13.23.33.43.53.63.7"LCDB Data for (1452) Hunnia". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1452|Hunnia. Retrieved 21 October 2017.
↑ 4.04.1"Asteroid 1452 Hunnia – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1452+Hunnia#Asteroid 1452 HunniaEAR-A-VARGBDET-5-NESVORNYFAM-V3.0. Retrieved 26 October 2019.
↑Hun, Hunnian (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=Hun,+Hunnian(Subscription or UK public library membership required.)
↑ 6.06.16.26.3Nugent, 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 Journal814 (2): 13. doi:10.1088/0004-637X/814/2/117. Bibcode: 2015ApJ...814..117N. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N. Retrieved 21 October 2017.
↑ 7.07.17.27.3Nugent, 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 Journal152 (3): 12. doi:10.3847/0004-6256/152/3/63. Bibcode: 2016AJ....152...63N. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016AJ....152...63N. Retrieved 21 October 2017.
↑ 8.08.18.2Masiero, 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 Journal741 (2): 20. doi:10.1088/0004-637X/741/2/68. Bibcode: 2011ApJ...741...68M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M. Retrieved 21 October 2017.
↑ 9.09.19.29.3Mainzer, 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 Journal741 (2): 25. doi:10.1088/0004-637X/741/2/90. Bibcode: 2011ApJ...741...90M.
↑ 10.010.1Sárneczky, K.; Szabó, Gy.; Kiss, L. L. (June 1999). "CCD observations of 11 faint asteroids". Astronomy and Astrophysics Supplement137 (2): 363–368. doi:10.1051/aas:1999251. Bibcode: 1999A&AS..137..363S. https://aas.aanda.org/articles/aas/pdf/1999/11/ds1664.pdf. Retrieved 21 October 2017.
↑ 11.011.1"1452 Hunnia (1938 DZ1)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=1452. Retrieved 21 October 2017.
↑ 12.012.1Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). Identification and Dynamical Properties of Asteroid Families. 297–321. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131. Bibcode: 2015aste.book..297N.
↑"MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. Retrieved 21 October 2017.
External links
Asteroid Lightcurve Database (LCDB), query form (info )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1452 Hunnia at AstDyS-2, Asteroids—Dynamic Site
Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
1452 Hunnia at the JPL Small-Body Database
Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters
v
t
e
Small Solar System bodies
Minor planets
Designation
Groups
List
Moon
Meanings of names
Asteroid
Aten asteroid
Asteroid belt
Family
Jupiter trojan
Near-Earth
Spectral types
Distant minor planet
Centaur
Damocloid
Neptune trojan
Trans-Neptunian object
Detached
Kuiper belt
Oort cloud
Scattered disc
Comets
Extinct
Great
Halley-type
Hyperbolic
Long-period
Lost
Main-belt
Near-parabolic
Periodic
Sungrazing
Other
Meteoroids
0.00
(0 votes)
Original source: https://en.wikipedia.org/wiki/1452 Hunnia. Read more