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9223 Leifandersson

From Wikipedia, the free encyclopedia
Asteroid

9223 Leifandersson
Discovery[1]
Discovered bySpacewatch
Discovery siteKitt Peak National Obs.
Discovery date18 December 1995
Designations
(9223) Leifandersson
Named after
Leif Erland Andersson[2][3]
(Swedish astronomer)
1995 YY7 · 1949 QK1
1981 UD5 · 1988 VT10
1990 FD4 · 1991 RK
main-belt · Flora[4]
background[5][6]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc67.50 yr (24,655 days)
Aphelion2.4626AU
Perihelion2.1386 AU
2.3006 AU
Eccentricity0.0704
3.49yr (1,275 days)
245.38°
0° 16m 57s / day
Inclination3.4120°
231.82°
23.837°
Physical characteristics
Dimensions4.498±0.176 km[7][8]
4.64 km(calculated)[4]
3.758±0.0014h[9]
0.24(assumed)[4]
0.381±0.051[7]
0.3810±0.0513[8]
S(assumed)[4]
13.384±0.003(R)[9] · 13.4[8] · 13.6[1] · 13.83[4]

9223 Leifandersson, provisional designation1995 YY7, is a backgroundasteroid from the inner regions of theasteroid belt, approximately 4.5 kilometers in diameter. It was discovered on 18 December 1995, by astronomers of theSpacewatch program atKitt Peak National Observatory in Arizona, United States. The asteroid was named in memory of Swedish astronomerLeif Erland Andersson.[2] The assumedstony asteroid has arotation period of 3.758 hours.[4]

Orbit and classification

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Leifandersson is a non-family asteroid of the main belt'sbackground population when applying theHierarchical Clustering Method to itsproper orbital elements.[5][6] It has also been classified as a member of theFlora family (402), a giant asteroid family and the largest family of stony asteroids in the main-belt.[4] It orbits the Sun in theinner asteroid belt at a distance of 2.1–2.5 AU once every 3 years and 6 months (1,275 days;semi-major axis of 2.30 AU). Its orbit has aneccentricity of 0.07 and aninclination of 3° with respect to theecliptic.[1]

The body'sobservation arc begins with its first observation as1949 QK1 atGoethe Link Observatory in August 1948, or more than 47 years prior to its official discovery observation at Kitt Peak.[2]

Physical characteristics

[edit]

Leifandersson is an assumed stonyS-type asteroid.[4]

Rotation period

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In February 2011, a rotationallightcurve ofLeifandersson was obtained from photometric observations by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 3.758 hours with a brightness amplitude of 0.33magnitude (U=2).[9]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Leifandersson measures 4.498 kilometers in diameter and its surface has analbedo of 0.3810.[7][8] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the parent body of the Flora family – and calculates a diameter of 4.64 kilometers based on anabsolute magnitude of 13.83.[4]

Naming

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Thisminor planet was named after Swedish astronomerLeif Erland Andersson (1943–1979), who calculated the first observable transits ofPluto andCharon and also co-produced a catalogue oflunar craters. The approved naming citation was published by theMinor Planet Center on 24 January 2000 (M.P.C. 38198).[2][10] The lunar craterAndersson was also named in his memory.[3][11]

References

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  1. ^abcd"JPL Small-Body Database Browser: 9223 Leifandersson (1995 YY7)" (2017-02-26 last obs.).Jet Propulsion Laboratory. Retrieved4 January 2018.
  2. ^abcd"9223 Leifandersson (1995 YY7)".Minor Planet Center. Retrieved4 January 2018.
  3. ^abSchmadel, Lutz D. (2007). "(9223) Leifandersson".Dictionary of Minor Planet Names – (9223) Leifandersson.Springer Berlin Heidelberg. p. 683.doi:10.1007/978-3-540-29925-7_7418.ISBN 978-3-540-00238-3.
  4. ^abcdefghi"LCDB Data for (9223) Leifandersson". Asteroid Lightcurve Database (LCDB). Retrieved4 January 2018.
  5. ^ab"Small Bodies Data Ferret".Nesvorny HCM Asteroid Families V3.0. Archived fromthe original on 2 August 2017. Retrieved4 January 2018.
  6. ^ab"Asteroid 9223 Leifandersson – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  7. ^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.S2CID 118745497. Retrieved4 January 2018.
  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. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75.S2CID 8342929. Retrieved4 January 2018.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved4 January 2018.
  11. ^"Planetary Names: Crater, craters: Andersson on Moon".Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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