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2058 Róka

From Wikipedia, the free encyclopedia
Themistian asteroid

2058 Róka
Discovery[1]
Discovered byG. Kulin
Discovery siteKonkoly Obs.
Discovery date22 January 1938
Designations
(2058) Róka
Named after
Gedeon Róka (1906–1974)
(Hungarian science writer)[2]
1938 BH · 1951 NP
1962 NA · 1963 UM
1974 SZ1 · 1978 AE
1985 UL3
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc79.18 yr (28,920 days)
Aphelion3.5790AU
Perihelion2.6682 AU
3.1236 AU
Eccentricity0.1458
5.52yr (2,016 days)
17.333°
0° 10m 42.6s / day
Inclination2.5352°
95.329°
180.50°
Physical characteristics
Dimensions21.12 km(derived)[3]
21.36±3.1 km[4]
23.40±0.52 km[5]
24.122±0.246 km[6]
24.273±0.234 km[7]
10.04±0.02h[8]
10.09±0.01 h[9]
0.0995(derived)[3]
0.1196±0.0252[7]
0.121±0.017[6]
0.130±0.006[5]
0.1542±0.056[4]
C[10] · S[3]
11.0[4][5][7] · 11.5[1][3] · 11.56±0.34[10]

2058 Róka, provisional designation1938 BH, is a Themistianasteroid from the outer regions of theasteroid belt, approximately 22 kilometers in diameter.

It was discovered on 22 January 1938, by HungarianGyörgy Kulin atKonkoly Observatory in Budapest, Hungary.[11] The asteroid was named in memory of Hungarian science writerGedeon Róka.[2]

Classification and orbit

[edit]

Róka is a member of theThemis family, a dynamical family of carbonaceousouter-belt asteroids with nearly coplanarecliptical orbits. It orbits the Sun at a distance of 2.7–3.6 AU once every 5 years and 6 months (2,016 days). Its orbit has aneccentricity of 0.15 and aninclination of 3° with respect to the ecliptic.[1] The body'sobservation arc begins with its official discovery observation at Konkoly in 1938.[11]

Physical characteristics

[edit]

Róka has been characterized as a carbonaceousC-type asteroid byPan-STARRS photometric survey.[10] Due to its ambivalent albedo it is also an assumedS-type asteroid.[3]

Lightcurves

[edit]

In March 2005, a rotationallightcurve ofRóka was obtained from photometric observations by French amateur astronomerRené Roy. Lightcurve analysis gave arotation period of 10.04 hours with a brightness variation of 0.34magnitude (U=3-).[8] One month later, astronomer at theRose-Hulman Observatory obtained another lightcurve with a concurring period of 10.09 hours and an amplitude of 0.40 magnitude (U=2).[9]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Róka measures between 21.36 and 24.273 kilometers in diameter and its surface has analbedo between 0.1196 and 0.1542.[4][5][6][7] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0995 and calculates a diameter of 21.12 kilometers based on anabsolute magnitude of 11.5.[3]

Naming

[edit]

Thisminor planet was named in memory of Gedeon Róka (1906–1974), a Hungarian science writer and popularizer of astronomy from Budapest.[2] The approved naming citation was published by theMinor Planet Center on 1 February 1980 (M.P.C. 5183).[12]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2058 Roka (1938 BH)" (2017-03-28 last obs.).Jet Propulsion Laboratory. Retrieved29 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2058) Róka".Dictionary of Minor Planet Names – (2058) Róka.Springer Berlin Heidelberg. pp. 166–167.doi:10.1007/978-3-540-29925-7_2059.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (2058) Róka". Asteroid Lightcurve Database (LCDB). Retrieved29 June 2017.
  4. ^abcdTedesco, 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. Retrieved22 October 2019.
  5. ^abcdUsui, 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)
  6. ^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. Retrieved29 June 2017.
  7. ^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.
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2058) Róka".Geneva Observatory. Retrieved29 June 2017.
  9. ^abAddleman, Don; Covele, Brent; Duncan, Allison; Johnson, Jama; Kramb, Steve; Lecrone, Crystal; et al. (December 2005)."Rose-Hulman spring 2005 lightcurve results: 155 Scylla, 590 Tomyris, 1655 Comas Solá, 2058 Roka, 6379 Vrba, and (25934) 2001 DC74".The Minor Planet Bulletin.32 (4):76–78.Bibcode:2005MPBu...32...76A.ISSN 1052-8091. Retrieved29 June 2017.
  10. ^abcVeres, 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. Retrieved29 June 2017.
  11. ^ab"2058 Roka (1938 BH)".Minor Planet Center. Retrieved29 June 2017.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved29 June 2017.


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