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1514 Ricouxa

From Wikipedia, the free encyclopedia
Asteroid of the inner regions of the asteroid belt

1514 Ricouxa
Shape model of Ricouxa from itslightcurve
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date22 August 1906
Designations
(1514) Ricouxa
Named after
unknown
(named byA. Patry)[2]
1906 UR · 1936 ME
1939 HC · 1940 XA
1970 XA · A916 OC
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc110.06 yr (40,198 days)
Aphelion2.6876AU
Perihelion1.7937 AU
2.2407 AU
Eccentricity0.1995
3.35yr (1,225 days)
41.914°
0° 17m 38.04s / day
Inclination4.5349°
145.85°
179.38°
Physical characteristics
Dimensions6.66±0.27 km[4]
7.07 km(derived)[3]
7.784±0.062 km[5]
8.129±0.021 km[6]
10.033±0.002h[7]
10.42466 h[8]
10.42468±0.00005 h[9]
10.438 h[10]
0.1821±0.0397[6]
0.228±0.039[5]
0.24(assumed)[3]
0.363±0.046[4]
S[3]
12.60[4] · 12.79±0.17[11] · 12.8[1] · 12.92[3][6][10]

1514 Ricouxa (provisional designation1906 UR) is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 7.5 kilometers in diameter. It was discovered on 22 August 1906, by German astronomerMax Wolf atHeidelberg Observatory in southern Germany.[12] The origin of the asteroid's name is unknown.[2]

Classification and orbit

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Ricouxa is aS-type asteroid and member of theFlora family, one of the largest collisional populations of stony asteroids in the entire main-belt. It orbits the Sun at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,225 days). Its orbit has aneccentricity of 0.20 and aninclination of 5° with respect to theecliptic.[1] Ricouxa'sobservation arc begins with its official discovery observation in 1906, as noprecoveries were taken, and no prior identifications were made.[12]

Physical characteristics

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Rotation and poles

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In the 1990s, Italian astronomerMaria A. Barucci obtained a rotationallightcurve of Ricouxa, using theESO 1-metre telescope atLa Silla Observatory in Chile. Lightcurve analysis gave a well-definedrotation period of 10.438 hours with a brightness variation of 0.62magnitude (U=3).[10]

Photometric observations by French amateur astronomerPierre Antonini in April 2006, gave a similar period of 10.033 hours and an identical amplitude of 0.62 magnitude (U=2+).[7] Additional periods were derived on modeled light-curves from various data sources. They gave a period of 10.42466 and 10.42468 hours, as well as a spin axis of (0°, 71.0°) and (251.0°, 75.0°) inecliptic coordinates, respectively.[8][9]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Ricouxa measures 7.78 kilometers in diameter, and its surface has analbedo of 0.228 (revised albedo-fits per 2014),[5] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – taken from8 Flora, the family's principal body and namesake – and derives a diameter of 7.07 kilometers based on anabsolute magnitude of 12.92.[3]

Naming

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Thisminor planet was named by French astronomerAndré Patry (1902–1960), after whom the asteroid1601 Patry is named. However, any reference to a person or occurrence for the name "Ricouxa" remains unknown.[2] The asteroid's name was also published inThe Names of the Minor Planets byPaul Herget in 1955 (H 135).[2]

Unknown meaning

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Among the many thousands ofnamed minor planets, Ricouxa is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between164 Eva and1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomersAuguste Charlois,Johann Palisa,Max Wolf andKarl Reinmuth.[13]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1514 Ricouxa (1906 UR)" (2016-09-11 last obs.).Jet Propulsion Laboratory. Retrieved5 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1514) Ricouxa".Dictionary of Minor Planet Names – (1514) Ricouxa.Springer Berlin Heidelberg. p. 120.doi:10.1007/978-3-540-29925-7_1515.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1514) Ricouxa". Asteroid Lightcurve Database (LCDB). Retrieved4 January 2017.
  4. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved4 January 2017.
  5. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved4 January 2017.
  6. ^abcMainzer, 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.
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1514) Ricouxa".Geneva Observatory. Retrieved4 January 2017.
  8. ^abDurech, J.; Kaasalainen, M.; Warner, B. D.; Fauerbach, M.; Marks, S. A.; Fauvaud, S.; et al. (January 2009)."Asteroid models from combined sparse and dense photometric data".Astronomy and Astrophysics.493 (1):291–297.Bibcode:2009A&A...493..291D.doi:10.1051/0004-6361:200810393. Retrieved4 January 2017.
  9. ^abHanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011)."A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method".Astronomy & Astrophysics.530: 16.arXiv:1104.4114.Bibcode:2011A&A...530A.134H.doi:10.1051/0004-6361/201116738. Retrieved4 January 2017.
  10. ^abcBarucci, M. A.; di Martino, M.; Dotto, E.; Fulchignoni, M.; Rotundi, A.; Burchi, R. (June 1994)."Rotational properties of small asteroids: Photoelectric observations of 16 asteroids".Icarus.109 (2):267–273.Bibcode:1994Icar..109..267B.doi:10.1006/icar.1994.1092.ISSN 0019-1035. Retrieved4 January 2017.
  11. ^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. Retrieved4 January 2017.
  12. ^ab"1514 Ricouxa (1906 UR)".Minor Planet Center. Retrieved4 January 2017.
  13. ^Schmadel, Lutz D. (2007). "Appendix 11 – Minor Planet Names with Unknown Meaning".Dictionary of Minor Planet Names – Fifth Revised and Enlarged revision. Springer Berlin Heidelberg. pp. 927–929.ISBN 978-3-540-00238-3.

External links

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Distant minor planet
Comets
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