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1092 Lilium

From Wikipedia, the free encyclopedia
Carbonaceous background asteroid

1092 Lilium
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date12 January 1924
Designations
(1092) Lilium
Pronunciation/ˈlɪliəm/[2]
Named after
Līlium[3](flowering plant)
1924 PN · 1929 BE
1936 QE
main-belt · (outer)[4]
background[5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc110.67 yr (40,421 days)
Aphelion3.1444AU
Perihelion2.6552 AU
2.8998 AU
Eccentricity0.0843
4.94yr (1,804 days)
200.62°
0° 11m 58.56s / day
Inclination5.3885°
307.49°
316.51°
Physical characteristics
Dimensions37.78±12.75 km[6]
40.276±0.243 km[7]
42.853±0.266 km[8]
43.23±0.33 km[9]
46.17±1.5 km[10]
49.56±13.84 km[11]
52.79±0.87 km[12]
17.63h[13]
24.60±0.05 h[14][a]
0.030±0.001[12]
0.0390±0.003[10]
0.04±0.02[11]
0.044±0.005[9]
0.0452±0.0071[8]
0.05±0.03[6]
C(assumed)[4]
B–V = 0.840[1]
U–B = 0.330[1]
10.82[1][4][8][9][10][11][12][13]
10.90±0.28[15] · 10.97[6]

1092 Lilium, provisional designation1924 PN, is a dark, carbonaceous backgroundasteroid from the outer regions of theasteroid belt, approximately 44 kilometers in diameter. It was discovered on 12 January 1924, by German astronomerKarl Reinmuth at theHeidelberg Observatory in southwest Germany.[16] The asteroid was named after the flowerLilium (true lily).[3]

Orbit and classification

[edit]

Lilium is a non-family asteroid from the main belt'sbackground population.[5] It orbits the Sun in theouter asteroid belt at a distance of 2.7–3.1 AU once every 4 years and 11 months (1,804 days). Its orbit has aneccentricity of 0.08 and aninclination of 5° with respect to theecliptic.[1]

The body'sobservation arc begins with aprecovery image taken at theLowell Observatory in July 1906, almost 18 years prior to its official discovery observation at Heidelberg.[16]

Physical characteristics

[edit]

Lilium is an assumed carbonaceousC-type asteroid.[4]

Rotation period

[edit]

In February 2008, a rotationallightcurve ofLilium was obtained from photometric observations by American astronomerBrian Warner at his Palmer Divide Observatory (716) in Colorado.[a] Lightcurve analysis gave a longer-than averagerotation period of 24.60 hours with a brightness amplitude of 0.25magnitude (U=3),[14] superseding a period of 17.63 hours byRichard Binzel from March 1984 (U=1).[13]

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,Lilium measures between 37.78 and 52.79 kilometers in diameter and its surface has analbedo between 0.030 and 0.05.[6][7][8][9][10][11][12]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0390 and a diameter of 46.17 kilometers based on anabsolute magnitude of 10.82.[4]

Naming

[edit]

Thisminor planet was named by the discoverer after the true lily flowering planet,Lilium. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 103).[3]

Reinmuth's flowers

[edit]

Due to his many discoveries,Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries, with numbers between(1009) and(1200). This list also contained a sequence of 28 asteroids, starting with1054 Forsytia, that were all named after plants, in particularflowering plants(also see list of minor planets named after animals and plants).[17]

Notes

[edit]
  1. ^abLightcurve plot of 1092 Lilium, Palmer Divide Observatory, Brian D. Warner (2008) Summary figures at theLCDB

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1092 Lilium (1924 PN)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved25 September 2017.
  2. ^"lilium".Oxford English Dictionary (Online ed.).Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcSchmadel, Lutz D. (2007). "(1092) Lilium".Dictionary of Minor Planet Names – (1092) Lilium.Springer Berlin Heidelberg. p. 93.doi:10.1007/978-3-540-29925-7_1093.ISBN 978-3-540-00238-3.
  4. ^abcde"LCDB Data for (1092) Lilium". Asteroid Lightcurve Database (LCDB). Retrieved25 September 2017.
  5. ^ab"Asteroid 1092 Lilium – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved28 October 2019.
  6. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  7. ^abMasiero, 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 September 2017.
  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.
  9. ^abcdMasiero, 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.S2CID 46350317. Retrieved25 September 2017.
  10. ^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.
  11. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117.S2CID 9341381. Retrieved25 September 2017.
  12. ^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)
  13. ^abcBinzel, R. P. (October 1987)."A photoelectric survey of 130 asteroids".Icarus.72 (1):135–208.Bibcode:1987Icar...72..135B.doi:10.1016/0019-1035(87)90125-4.ISSN 0019-1035. Retrieved25 September 2017.
  14. ^abWarner, Brian D. (September 2008)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: December 2007 - March 2008".The Minor Planet Bulletin.35 (3):95–98.Bibcode:2008MPBu...35...95W.ISSN 1052-8091. Retrieved25 September 2017.
  15. ^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.S2CID 53493339. Retrieved25 September 2017.
  16. ^ab"1092 Lilium (1924 PN)".Minor Planet Center. Retrieved25 September 2017.
  17. ^Schmadel, Lutz D. (2007). "(1054) Forsytia".Dictionary of Minor Planet Names – (1054) Forsytia. Springer Berlin Heidelberg. p. 90.doi:10.1007/978-3-540-29925-7_1055.ISBN 978-3-540-00238-3.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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