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1936 Lugano

From Wikipedia, the free encyclopedia
Adeonian asteroid

1936 Lugano
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date24 November 1973
Designations
(1936) Lugano
Named after
Lugano(Swiss city)[2]
1973 WD · 1936 LC
1949 KE1 · 1951 WX
1964 VA1 · 1970 AG1
1970 AL1 · 1970 CD
main-belt · (middle)[3]
Adeona[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc61.33 yr (22,399 days)
Aphelion3.0395AU
Perihelion2.3131 AU
2.6763 AU
Eccentricity0.1357
4.38yr (1,599 days)
291.44°
0° 13m 30.36s / day
Inclination10.254°
265.17°
255.13°
Physical characteristics
Dimensions23.48±8.63 km[5]
24.56 km(derived)[3]
24.81±0.8 km[6]
27.95±0.87 km[7]
31.037±0.137 km[8]
31.43±8.87 km[9]
33.704±0.067 km[10]
19.594±0.007h[11]
19.651±0.015 h[12]
0.028±0.011[8]
0.0294±0.0024[10]
0.04±0.02[9]
0.04±0.03[5]
0.0558(derived)[3]
0.093±0.007[7]
0.1042±0.008[6]
SMASS =Ch[1] · P[10]
11.10[7][6][10] · 11.70[5] · 11.78[9] · 11.8[1][3] · 12.45±0.41[13]

1936 Lugano, provisional designation1973 WD, is a carbonaceous Adeonianasteroid from the middle region of theasteroid belt, approximately 26 kilometers in diameter.

It was discovered on 24 November 1973, by Swiss astronomerPaul Wild atZimmerwald Observatory near Bern, Switzerland.[14] It was later named for the Swiss city ofLugano.[2]

Classification and orbit

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Lugano is a member of theAdeona family (505), a largefamily of carbonaceous asteroids.[4]

It orbits the Sun in thecentral main-belt at a distance of 2.3–3.0 AU once every 4 years and 5 months (1,599 days). Its orbit has aneccentricity of 0.14 and aninclination of 10° with respect to theecliptic.[1] It was first identified as1936 LC atJohannesburg Observatory in 1936. The body'sobservation arc begins 22 years prior to its official discovery observation at Zimmerwald, when it was identified as1951 WX atMcDonald Observatory in 1951.[14]

Physical characteristics

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Spectral type

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In theSMASS classification,Lugano is a Ch-subtype, a hydratedC-type asteroid,[1] while theWide-field Infrared Survey Explorer (WISE) rates it as a very dark and featureless reddishP-type asteroid.[10]

Diameter and albedo

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According to the space-based surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Lugano measures between 23.48 and 33.7 kilometers in diameter and its surface has analbedo in the range of 0.028 to 0.1042.[5][6][7][8][9][10]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.056 and a diameter of 24.6 kilometers, based on an absolutemagnitude of 11.8.[3]

Lightcurves

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Two rotationallightcurves ofLugano were obtained from photometric observations made in February 2005. The first lightcurve by French astronomer Raymond Poncy gave arotation period of19.594±0.007 hours with a brightness variation of 0.25 magnitude (U=2).[11] The second lightcurve from the U.S.Carbuncle Hill Observatory (912), Rhode Island, rendered a well-defined period of19.651±0.015 with an amplitude of 0.31 in magnitude (U=3).[12]

Naming

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Theminor planet is named after the Swiss-Italian city ofLugano, located south of the Alps and known for its mild climate. During the winter half-year of 1973/74, Paul Wild discovered three more asteroids,1935 Lucerna,1937 Locarno and1938 Lausanna, which he named after the Swiss citiesLucerne,Locarno andLausanne, respectively, composing a quartet of sequentially numbered, thematically named asteroids.[2] The officialnaming citation was published by theMinor Planet Center on 1 April 1978 (M.P.C. 4358).[15]

References

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  1. ^abcdef"JPL Small-Body Database Browser: 1936 Lugano (1973 WD)" (2017-02-04 last obs.).Jet Propulsion Laboratory. Retrieved2 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1936) Lugano".Dictionary of Minor Planet Names – (1936) Lugano.Springer Berlin Heidelberg. p. 155.doi:10.1007/978-3-540-29925-7_1937.ISBN 978-3-540-00238-3.
  3. ^abcde"LCDB Data for (1936) Lugano". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  4. ^ab"Asteroid 1936 Lugano – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^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. Retrieved28 October 2017.
  6. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved17 October 2019.
  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. ^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. Retrieved29 October 2016.
  9. ^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.
  10. ^abcdefMainzer, 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 35447010. Retrieved17 May 2016.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1936) Lugano".Geneva Observatory. Retrieved17 May 2016.
  12. ^abPray, Donald P. (September 2005)."Lightcurve analysis of asteroids 106, 752, 847, 1057, 1630, 1670, 1927 1936, 2426, 2612, 2647, 4087, 5635, 5692, and 6235".The Minor Planet Bulletin.32 (3):48–51.Bibcode:2005MPBu...32...48P.ISSN 1052-8091. Retrieved17 May 2016.
  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.S2CID 53493339. Retrieved17 May 2016.
  14. ^ab"1936 Lugano (1973 WD)".Minor Planet Center. Retrieved17 May 2016.
  15. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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