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1133 Lugduna

From Wikipedia, the free encyclopedia
Main-belt asteroid

1133 Lugduna
Orbit of 1133 Lugduna
Discovery[1]
Discovered byH. van Gent
Discovery siteJohannesburg Obs.
(Leiden Southern Station)
Discovery date13 September 1929
Designations
(1133) Lugduna
Named after
Dutch city ofLeiden[2]
(Lugdunum Batavorum)
1929 RC1 · A908 BD
main-belt · Flora[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc87.20 yr (31,848 days)
Aphelion2.5966AU
Perihelion1.7751 AU
2.1858 AU
Eccentricity0.1879
3.23yr (1,180 days)
67.197°
0° 18m 18s / day
Inclination5.3765°
58.230°
306.74°
Physical characteristics
Dimensions8.275±0.019 km[5]
9.100±0.037 km[6]
9.76 km(calculated)[3]
10.47±0.70 km[7]
5h[a]
5.477±0.001 h[8]
5.478±0.005 h[9]
0.208±0.029[7]
0.24(assumed)[3]
0.2798±0.0550[6]
0.363±0.029[5]
Tholen =S[1][3][10]
B–V = 0.880[1]
U–B = 0.510[1]
12.22[1][3][6][7] · 12.45±0.50[10]

1133 Lugduna, provisional designation1929 RC1, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 9.5 kilometers in diameter. It was discovered on 13 September 1929, by Dutch astronomerHendrik van Gent at the Leiden Southern Station annex to theUnion Observatory in Johannesburg, South Africa.[11] The asteroid was named in honor of the city ofLeiden in the Netherlands.[2]

Orbit and classification

[edit]

Lugduna is a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main-belt.[3][4][12]: 23  It orbits the Sun in theinner main-belt at a distance of 1.8–2.6 AU once every 3 years and 3 months (1,180 days). Its orbit has aneccentricity of 0.19 and aninclination of 5° with respect to theecliptic.[1]

The asteroid was first identified asA908 BD at Taunton Observatory (803), Massachusetts, in January 1908. Itsobservation arc begins at Johannesburg, three weeks after its official discovery observation.[11]

Physical characteristics

[edit]

Both theTholen classification andPanSTARRS photometric survey characterizeLugduna as a stonyS-type asteroid.[1][10]

Rotation period

[edit]

In December 2010, the best-rated rotationallightcurve ofLugduna was obtained from photometric observations by Gordon Gartrelle at theUniversity of North Dakota and at theBadlands Observatory in South Dakota, United States. Analysis of the bimodal lightcurve gave a well-definedrotation period of 5.477 hours with a brightness variation of 0.43magnitude (U=3).[8] Other observations gave a period of 5 and 5.478 hours with an amplitude of 0.33 (U=2-/3-).[9][a]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Lugduna measures between 8.275 and 10.47 kilometers in diameter and its surface has analbedo between 0.208 and 0.363.[5][6][7]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the Flora family's largest member and namesake – and calculates a diameter of 9.76 kilometers based on anabsolute magnitude of 12.22.[3]

Naming

[edit]

Thisminor planet was named in honor of the Dutch city ofLeiden where theLeiden Observatory ofLeiden University – parent of the discovering Leiden Southern Station – is located. The asteroid was named by the discoverer and by astronomerGerrit Pels, who computed the body's orbit. The official naming citation was reviewed byIngrid van Houten-Groeneveld who was a long-time astronomer at Leiden.[2]

The Latin nameLugdunum Batavorum (or Batavorum Lugdunum) and Academia Lugduno Batava has been used by the city and by the university in official documents. The Latin name also refers toBrittenburg, an ancient Roman ruin located west of Leiden.

Notes

[edit]
  1. ^abFranco(2011) web: observation date: 6 November 2010. Rotation period5 hours with a brightness amplitude of0.33 mag. Quality Code of 2-. Summary figures for (1133) Lugduna atCollaborative Asteroid Lightcurve Link (CALL)

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 1133 Lugduna (1929 RC1)" (2016-11-23 last obs.).Jet Propulsion Laboratory. Retrieved9 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1133) Lugduna".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 96.doi:10.1007/978-3-540-29925-7_1134.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1133) Lugduna". Asteroid Lightcurve Database (LCDB). Retrieved9 September 2017.
  4. ^ab"Asteroid 1133 Lugduna – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved30 October 2019.
  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. Retrieved9 September 2017.
  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. ^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)
  8. ^abGartrelle, Gordon M. (April 2012)."Lightcurve Results for Eleven Asteroids".The Minor Planet Bulletin.39 (2): 40%–46.Bibcode:2012MPBu...39...40G.ISSN 1052-8091. Retrieved9 September 2017.
  9. ^abKryszczynska, A.; Colas, F.; Polinska, M.; Hirsch, R.; Ivanova, V.; Apostolovska, G.; et al. (October 2012)."Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region".Astronomy and Astrophysics.546: 51.Bibcode:2012A&A...546A..72K.doi:10.1051/0004-6361/201219199.
  10. ^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. Retrieved9 September 2017.
  11. ^ab"1133 Lugduna (1929 RC1)".Minor Planet Center. Retrieved9 September 2017.
  12. ^Nesvorný, 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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