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1003 Lilofee

From Wikipedia, the free encyclopedia
Main-belt asteroid

1003 Lilofee
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date13 September 1923
Designations
(1003) Lilofee
Named after
Lilofee[2]
(mermaid inGerman folklore)
1923 OK · 1937 FB
1940 TA · 1951 QO
1951 RA2 · 1957 WD2
1962 QH · A915 HB
main-belt · (outer)
Themis[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc93.81 yr (34,263 days)
Aphelion3.6414AU
Perihelion2.6373 AU
3.1394 AU
Eccentricity0.1599
5.56yr (2,032 days)
211.31°
0° 10m 37.92s / day
Inclination1.8402°
139.45°
317.42°
Physical characteristics
Dimensions27.29±1.83 km[5]
32.292±0.334 km[6]
33.1±3.3 km[7]
33.678±0.334 km[8]
34.04 km(calculated)[3]
36±4 km[9]
8.230±0.004h[10]
8.24991±0.00005 h[11]
8.250±0.001 h[12][a]
8.2506±0.0003 h[10]
8.255±0.002 h[10]
0.07±0.01[9]
0.08±0.02[3][7]
0.130±0.020[8]
0.1406±0.0213[6]
0.198±0.028[5]
C[3]
10.20[5][6] · 10.50±0.22[13] · 10.70[3][7][9] · 10.8[1]

Lilofee (minor planet designation:1003 Lilofee), provisional designation1923 OK, is a carbonaceous Themistianasteroid from the outer regions of theasteroid belt, approximately 33 kilometers in diameter. It was discovered on 13 September 1923, by astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in southwest Germany.[14] The asteroid was named after the Black Forestmermaid "Lilofee" fromGerman folklore.[2]

Orbit and classification

[edit]

Lilofee is a member of theThemis family (602),[3][4] a very largefamily of carbonaceous, low-inclination asteroids, named after24 Themis.[15]: 23  It orbits the Sun in theouter main-belt at a distance of 2.6–3.6 AU once every 5 years and 7 months (2,032 days). Its orbit has aneccentricity of 0.16 and aninclination of 2° with respect to theecliptic.[1]

The asteroid was first identified asA915 HB atBergedorf Observatory in April 1915. The body'sobservation arc begins with its official discovery observation at Heidelberg.[14]

Physical characteristics

[edit]

Lilofee is an assumed carbonaceousC-type asteroid,[3] which corresponds to the overallspectral type of the Themis family.[15]: 23 

Lightcurves

[edit]

Since 2004, several rotationallightcurves of Lilofee were obtained from photometric observations by astronomersRené Roy, Enric Forné andRobert Stephens. Lightcurve analysis gave arotation period of 8.255 hours with a brightness variation of 0.57magnitude (U=2+/3/3).[10][12][a]

In 2013, an international study modeled a lightcurve with a concurring period of 8.24991 hours and found aspin axis of (n.a., −99.0°) inecliptic coordinates (λ, β).[11]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Lilofee measures between 27.29 and 36 kilometers in diameter and its surface has analbedo between 0.07 and 0.198.[5][6][7][8][9]

TheCollaborative Asteroid Lightcurve Link adopts an albedo of 0.08 and calculates a diameter of 34.04 kilometers based on anabsolute magnitude of 10.7.[3]

Naming

[edit]

Thisminor planet was named after the legendarymermaid/neck Lilofee, who lived in the smallMummelsee of theBlack Forest in southwest Germany. Lilofee is also the title figure in the German folk-songThe beautiful young Lilofee ("Die schöne junge Lilofee") by August Schnezler (1809–1853).[2]

The asteroid was named by the discoverer (RI 402). The name was proposed byARI-astronomer Johannes Riem, after whom1025 Riema was named. The official naming citation was also mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 96).[2]

Notes

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  1. ^abLightcurve plot of (1003) Lilofee by R. D. Stephens (2013) atCS3. Rotation period8.250±0.001 hours with a brightness amplitude of0.54±0.02 mag. Summary figures atCollaborative Asteroid Lightcurve Link

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1003 Lilofee (1923 OK)" (2017-07-04 last obs.).Jet Propulsion Laboratory. Retrieved13 September 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1003) Lilofee".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 87.doi:10.1007/978-3-540-29925-7_1004.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1003) Lilofee". Asteroid Lightcurve Database (LCDB). Retrieved13 September 2017.
  4. ^ab"Small Bodies Data Ferret".Nesvorny HCM Asteroid Families V3.0. Retrieved13 September 2017.
  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. ^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.
  7. ^abcdAlí-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".Astronomy and Astrophysics.591: 11.Bibcode:2016A&A...591A..14A.doi:10.1051/0004-6361/201527660.hdl:11336/63614.
  8. ^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. Retrieved13 September 2017.
  9. ^abcdAlí-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. Retrieved13 September 2017.
  10. ^abcdBehrend, Raoul."Asteroids and comets rotation curves – (1003) Lilofee".Geneva Observatory. Retrieved13 September 2017.
  11. ^abHanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; Durkee, R.; et al. (November 2013)."An anisotropic distribution of spin vectors in asteroid families".Astronomy and Astrophysics.559: 19.arXiv:1309.4296.Bibcode:2013A&A...559A.134H.doi:10.1051/0004-6361/201321993. Retrieved13 September 2017.
  12. ^abStephens, Robert D. (April 2014)."Asteroids Observed from CS3: 2013 October-December".The Minor Planet Bulletin.41 (2):92–95.Bibcode:2014MPBu...41...92S.ISSN 1052-8091. Retrieved13 September 2017.
  13. ^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. Retrieved13 September 2017.
  14. ^ab"1003 Lilofee (1923 OK)".Minor Planet Center. Retrieved13 September 2017.
  15. ^abNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.

External links

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