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1444 Pannonia
Modelled shape of Pannonia from its lightcurve
Discovery [1]
Discovered by G. Kulin
Discovery site Konkoly Obs.
Discovery date6 January 1938
Designations
(1444) Pannonia
Pronunciation /pəˈnoʊniə/ [2]
Named after
 Pannonia (ancient province) [3]
1938 AE
main-belt · ( outer) [4]
Orbital characteristics [1]
Epoch 16 February 2017 ( JD 2457800.5)
Uncertainty parameter 0
Observation arc78.23 yr (28,575 days)
Aphelion3.5915 AU
Perihelion2.7128 AU
3.1521 AU
Eccentricity0.1394
5.60 yr (2,044 days)
268.73 °
0° 10m 33.96s / day
Inclination17.761°
303.33°
310.87°
Physical characteristics
26.363±0.141 km [5] [6]
27.14 km (derived) [4]
28±3 km [7]
28.3±2.8 km [8]
29.20±2.2 km [9]
30.48±0.53 km [10]
30.92±9.63 km [11]
31.49±9.20 km [12]
6.2±0.1 h [13]
6.205±0.003 h [13]
10.756±0.006 h [14]
0.04±0.02 [11]
0.05±0.06 [12]
0.0501 (derived) [4]
0.053±0.005 [5] [6]
0.07±0.01 [7] [8]
0.070±0.003 [10]
0.4748±0.081 [9]
C [4]
9.10 [9] · 11.10 [10] · 11.18±0.62 [15] · 11.30 [7] [8] [12] · 11.4 [1] · 11.7 [4] [5] [16] · 11.73 [11]

1444 Pannonia ( prov. designation: 1938 AE) is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 29 kilometers (18 miles) in diameter. It was discovered on 6 January 1938, by Hungarian astronomer György Kulin at Konkoly Observatory in Budapest, Hungary. [17] It was named after the ancient province of the Roman Empire, Pannonia. [3]

Orbit and classification

Pannonia is a non- family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun at a distance of 2.7–3.6  AU once every 5 years and 7 months (2,044 days). Its orbit has an eccentricity of 0.14 and an inclination of 18 ° with respect to the ecliptic. [1] Pannonia's observation arc begins 3 weeks after its official discovery at Konkoly, as no precoveries were taken, and no prior identifications were made. [17]

Naming

This minor planet was named for Pannonia, an ancient province of the Roman Empire, which was partially located over the territory of the present-day western Hungary. [3] The official naming citation was published by the Minor Planet Center on 1 February 1980 ( M.P.C. 5183). [18]

Physical characteristics

Rotation period

In April 2001, astronomer Colin Bembrick obtained the first rotational lightcurve of Pannonia at Tarana Observatory ( 431) in Australia. Lightcurve analysis gave a well-defined rotation period of 10.756 hours with a brightness amplitude of 0.16 magnitude ( U=3). [14] In 2002 and 2004, photometric observations by French astronomers Laurent Bernasconi and Bernard Christophe Additional periods of 6.2 and 6.205 hours with an amplitude of 0.57 and 0.37, respectively ( U=2-/2). [13]

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Pannonia measures between 26.36 and 31.49 kilometers in diameter, and its surface has an albedo between 0.04 and 0.47. [5] [8] [9] [10] [11] [12] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0501 and a diameter of 27.14 kilometers with an absolute magnitude of 11.7. [4]

References

  1. ^ a b c d "JPL Small-Body Database Browser: 1444 Pannonia (1938 AE)" (2016-04-01 last obs.). Jet Propulsion Laboratory. Retrieved 5 January 2017.
  2. ^ "Pannonia". Merriam-Webster.com Dictionary.
  3. ^ a b c Schmadel, Lutz D. (2007). "(1444) Pannonia". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p.  116. doi: 10.1007/978-3-540-29925-7_1445. ISBN  978-3-540-00238-3.
  4. ^ a b c d e f "LCDB Data for (1444) Pannonia". Asteroid Lightcurve Database (LCDB). Retrieved 5 January 2017.
  5. ^ 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. S2CID  35447010.
  6. ^ a b 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. S2CID  118745497. Retrieved 5 January 2017.
  7. ^ a b c Alí-Lagoa, V.; de León, J.; Licandro, J.; Delbó, M.; Campins, H.; Pinilla-Alonso, N.; et al. (June 2013). "Physical properties of B-type asteroids from WISE data". Astronomy and Astrophysics. 554: 16. arXiv: 1303.5487. Bibcode: 2013A&A...554A..71A. doi: 10.1051/0004-6361/201220680. S2CID  119214002. Retrieved 5 January 2017.
  8. ^ a b c d Alí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids" (PDF). Astronomy and Astrophysics. 591: 11. Bibcode: 2016A&A...591A..14A. doi: 10.1051/0004-6361/201527660. Retrieved 5 January 2017.
  9. ^ a b c d Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode: 2004PDSS...12.....T. Retrieved 22 October 2019.
  10. ^ a b c d Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode: 2011PASJ...63.1117U. doi: 10.1093/pasj/63.5.1117. ( online, AcuA catalog p. 153)
  11. ^ 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.
  12. ^ 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. S2CID  9341381. Retrieved 5 January 2017.
  13. ^ a b c Behrend, Raoul. "Asteroids and comets rotation curves – (1444) Pannonia". Geneva Observatory. Retrieved 5 January 2017.
  14. ^ a b Bembrick, C.; Pereghy, B.; Ainsworth, T. (June 2002). "Lightcurves and Period Determination for 1444 Pannonia". The Minor Planet Bulletin. 29: 21–22. Bibcode: 2002MPBu...29...21B. Retrieved 5 January 2017.
  15. ^ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv: 1506.00762. Bibcode: 2015Icar..261...34V. doi: 10.1016/j.icarus.2015.08.007. S2CID  53493339. Retrieved 5 January 2017.
  16. ^ Faure, Gerard; Garret, Lawrence (December 2007). "Suggested Revised H Values of Selected Asteroids: Report Number 3". The Minor Planet Bulletin. 34 (4): 95–99. Bibcode: 2007MPBu...34...95F. ISSN  1052-8091. Retrieved 5 January 2017.
  17. ^ a b "1444 Pannonia (1938 AE)". Minor Planet Center. Retrieved 5 January 2017.
  18. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 5 January 2017.

External links

Retrieved from " https://en.wikipedia.org/?title=1444_Pannonia&oldid=1233138982"

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