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1158 Luda

From Wikipedia, the free encyclopedia
Main-belt asteroid

1158 Luda
Discovery[1]
Discovered byG. Neujmin
Discovery siteSimeiz Obs.
Discovery date31 August 1929
Designations
(1158) Luda
Named after
Ludmilla Neujmin
(discoverer's sister)[2]
1929 QF · 1954 UQ1
1958 TG1 · 1972 GC
main-belt · Maria[3] · Eunomia[4]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc87.27 yr (31,876 days)
Aphelion2.8532AU
Perihelion2.2742 AU
2.5637 AU
Eccentricity0.1129
4.11yr (1,499 days)
56.051°
0° 14m 24.36s / day
Inclination14.834°
344.74°
56.226°
Physical characteristics
Dimensions18.636±0.207 km[5]
18.70±0.48 km[6]
19.06±0.8 km(IRAS:8)[7]
20.596±0.130 km[8]
6.86±0.01h[9]
6.863±0.005 h[10]
6.870±0.005 h[11]
6.90±0.01 h[12]
7.44 h[3]
0.2025±0.0548[8]
0.221±0.034[5]
0.2329±0.022(IRAS:8)[7]
0.253±0.015[6]
S[4][13]
10.8[1][4][6][7][8] · 10.95±0.33[13]

1158 Luda, provisional designation1929 QF, is a stonyasteroid from the middle regions of theasteroid belt, approximately 19 kilometers in diameter. It was discovered on 31 August 1929, by Soviet astronomerGrigory Neujmin atSimeiz Observatory on the Crimean peninsula.[14] It was named after Ludmilla Neujmin, the sister of the discoverer.[2]

Orbit and classification

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Luda orbits the Sun at a distance of 2.3–2.9 AU once every 4 years and 1 month (1,499 days). Its orbit has aneccentricity of 0.11 and aninclination of 15° with respect to theecliptic.[1] The body'sobservation arc begins with its first used observation atJohannesburg Observatory, one month after its official discovery observation at Simeiz.[14]Luda is a stonyS-type asteroid.[13]

Based on its orbital elements,Luda is a member of theEunomia family, a large group of stony asteroids and the most prominent family in the intermediate main-belt, while Argentine astronomer Alvarez-Candal from the Universidad Nacional de Córdoba groups it into the smallerMaria family, which is named after170 Maria (the same discrepancy exists for9175 Graun and2429 Schürer).[3]: 389 

Physical characteristics

[edit]

Photometry

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Several rotationallightcurves ofLuda were obtained from photometric observations. Analysis of the best-rated lightcurves obtained by French amateur astronomerLaurent Bernasconi, American astronomerBrian Warner, and an international group led by Korean astronomers, gave a well-definedrotation period between 6.86 and 6.87 hours with a brightness variation between 0.13 and 0.22magnitude (U=3/3-/3).[9][10][11] Photometric observations also gave a period of 6.9 and 7.44 hours, but these were derived from a fragmentary and ambiguous light curve, respectively.(U=1/2).[3][12]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Luda measures between 18.63 and 20.59 kilometers in diameter and its surface has analbedo between 0.20 and 0.25.[5][6][7][8] TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.232 and a diameter of 19.06 kilometers with anabsolute magnitude of 10.8.[4]

Naming

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Thisminor planet was named for Ludmilla Neujmin, the sister of the discoverer. "Luda" is a diminutive of Ludmilla.[2] AstronomerLutz Schmadel, who compiled this naming citation, based it on a private communication with "N. S. Samojlova-Yakhontova", as neither theMinor Planet Circulars norThe Names of the Minor Planets give any information about this asteroid's name.[2][15]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1158 Luda (1929 QF)" (2017-01-07 last obs.).Jet Propulsion Laboratory. Retrieved25 January 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1158) Luda".Dictionary of Minor Planet Names – (1158) Luda.Springer Berlin Heidelberg. p. 98.doi:10.1007/978-3-540-29925-7_1159.ISBN 978-3-540-00238-3.
  3. ^abcdAlvarez-Candal, Alvaro; Duffard, René; Angeli, Cláudia A.; Lazzaro, Daniela; Fernández, Silvia (December 2004)."Rotational lightcurves of asteroids belonging to families".Icarus.172 (2):388–401.Bibcode:2004Icar..172..388A.doi:10.1016/j.icarus.2004.06.008. Retrieved25 January 2017.
  4. ^abcd"LCDB Data for (1158) Luda". Asteroid Lightcurve Database (LCDB). Retrieved25 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.S2CID 119293330. Retrieved25 January 2017.
  6. ^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)
  7. ^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.
  8. ^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.S2CID 118700974.
  9. ^abKim, M.-J.; Choi, Y.-J.; Moon, H.-K.; Byun, Y.-I.; Brosch, N.; Kaplan, M.; et al. (March 2014)."Rotational Properties of the Maria Asteroid Family".The Astronomical Journal.147 (3): 15.arXiv:1311.5318.Bibcode:2014AJ....147...56K.doi:10.1088/0004-6256/147/3/56.S2CID 119256964. Retrieved25 January 2017.
  10. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1158) Luda".Geneva Observatory. Retrieved25 January 2017.
  11. ^abWarner, Brian D. (January 2011)."Upon Further Review: III. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory".The Minor Planet Bulletin.38 (1):21–23.Bibcode:2011MPBu...38...21W.ISSN 1052-8091. Retrieved25 January 2017.
  12. ^abWarner, Brian D. (September 2005)."Asteroid lightcurve analysis at the Palmer Divide Observatory - winter 2004-2005".The Minor Planet Bulletin.32 (3):54–58.Bibcode:2005MPBu...32...54W.ISSN 1052-8091. Retrieved25 January 2017.
  13. ^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.S2CID 53493339. Retrieved25 January 2017.
  14. ^ab"1158 Luda (1929 QF)".Minor Planet Center. Retrieved25 January 2017.
  15. ^Schmadel, Lutz D. (1997).Dictionary of Minor Planet Names – Introduction, Source of Information. Springer Berlin Heidelberg. p. 16.ISBN 978-3-662-06617-1.

External links

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