Carbonaceous Meliboean asteroid
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 .[ 3]
Orbit and classification
Hunnia is a member of the Meliboea family (604 ),[ 5] 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 ,[ 4] 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 (U=2 ).[ 10] No other lightcurves have since been obtained.[ 4]
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.[ 4]
Naming
This minor planet was named in honor of the Hungarian nation .[ 3] 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]
References
^ a b c d "JPL Small-Body Database Browser: 1452 Hunnia (1938 DZ1)" (2017-07-02 last obs.). Jet Propulsion Laboratory . Retrieved 21 October 2017 .
^ "Hun, Hunnian" . Oxford English Dictionary (Online ed.). Oxford University Press . (Subscription or participating institution membership required.)
^ a b c Schmadel, 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 .
^ a b c d e f g h "LCDB Data for (1452) Hunnia" . Asteroid Lightcurve Database (LCDB). Retrieved 21 October 2017 .
^ a b "Asteroid 1452 Hunnia – Nesvorny HCM Asteroid Families V3.0" . Small Bodies Data Ferret . Retrieved 26 October 2019 .
^ a b c d Nugent, 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 . Retrieved 21 October 2017 .
^ a b c d Nugent, 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 .
^ a b c Masiero, 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 . Retrieved 21 October 2017 .
^ a b c d Mainzer, 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 .
^ a b Sárneczky, 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 . Retrieved 21 October 2017 .
^ a b "1452 Hunnia (1938 DZ1)" . Minor Planet Center . Retrieved 21 October 2017 .
^ 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 978-0-8165-3213-1 .
^ "MPC/MPO/MPS Archive" . Minor Planet Center . Retrieved 21 October 2017 .
External links