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1107 Lictoria

From Wikipedia, the free encyclopedia
Hygiea asteroid

1107 Lictoria
Shape model ofLictoria from itslightcurve
Discovery[1]
Discovered byL. Volta
Discovery sitePino Torinese Obs.
Discovery date30 March 1929
Designations
(1107) Lictoria
Named after
Fasces Lictores[2]
(Symbol offascism)
1929 FB · A909 UB
A917 DF · A924 KC
main-belt · (outer)[3]
Hygiea[4]
Orbital characteristics[1]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc108.28 yr (39,549 days)
Aphelion3.5809AU
Perihelion2.7885 AU
3.1847 AU
Eccentricity0.1244
5.68yr (2,076 days)
312.44°
0° 10m 24.24s / day
Inclination7.0735°
110.84°
351.35°
Physical characteristics
69.93±25.12 km[5]
78.86 km(derived)[3]
79.079±0.298 km[6]
79.17±2.9 km[7]
80.73±0.96 km[8]
86.724±1.421 km[9]
8.56h[a]
8.561 h[b][c]
8.5616±0.0002 h[10]
8.5681±0.0001 h[d]
8.586±0.005 h[10]
0.0450(derived)[3]
0.05±0.05[5]
0.0538±0.0162[9]
0.063±0.002[8]
0.0646±0.005[7]
0.066±0.012[6]
SMASS =Xc[1] · P[9]
9.10[7][8][9] · 9.50[3][5] · 9.6[1]

1107 Lictoria (prov. designation:1929 FB) is a largeHygiea asteroid, approximately 79 kilometers (49 miles) in diameter, from the outer regions of theasteroid belt. It was discovered byLuigi Volta at thePino Torinese Observatory in 1929,[11] and named after theFasces Lictores, Latin for "Fasci Littori", the symbol of the Italian fascist party.[2]

Discovery

[edit]

Lictoria as first observed asA909 UB atHeidelberg Observatory on 17 October 1909. It was officially discovered on 30 March 1929, by Italian astronomerLuigi Volta at theObservatory of Turin near Pino Torinese, Italy.[11] Three weeks later, on 17 March 1929, it was independently discovered by astronomerKarl Reinmuth at Heidelberg, Germany.[2] TheMinor Planet Center only acknowledges the first discoverer.[11]

Orbit and classification

[edit]

This asteroid is a member of theHygiea family (601),[4] a very largefamily of carbonaceous outer-belt asteroids, named after thefourth-largest asteroid,10 Hygiea.[12] It orbits the Sun in theouter asteroid belt at a distance of 2.8–3.6 AU once every 5 years and 8 months (2,076 days;semi-major axis of 3.18 AU). Its orbit has aneccentricity of 0.12 and aninclination of 7° with respect to theecliptic.[1] The body'sobservation arc begins with its first observation asA909 UB at Heidelberg in October 1909.[11]

Naming

[edit]

Thisminor planet was named after the symbol offascism used by theItalian Fascist Party. The symbol was called "Fasci Littori", or "Fasces Lictores" in Latin (derived fromfasces andlictor). Several other things such as festivals (littoriali) and fast trains (littorine) were given related names during the fascist period. In particular, the Italian city ofLatina was founded under the name "Littoria" in 1932.[2] The author of the Dictionary of Minor Planet Names,Lutz Schmadel, corresponded with Italian-born astronomerPaul Comba to confirm the meaning for this asteroid.[2][13]

Physical characteristics

[edit]

In the Bus–BinzelSMASS classification,Lictoria is a Xc-subtype that transitions from theX-type to the carbonaceousC-type asteroids.[1] It has also been characterized as a primitiveP-type asteroid by theWide-field Infrared Survey Explorer (WISE).[9] The Hygiea family's overallspectral type is a mixture of C-type and somewhat brighterB-type asteroids.[12]: 23 

Rotation period

[edit]

Several rotationallightcurve ofLictoria have been obtained from photometric observations by astronomers William Koff, Eric Barbotin,Stefano Sposetti and Matthieu Conjat, as well as Hiromi and Hiroko Hamanowa (U=2/3/2/2/3).[10][a][b][c][d] Analysis of the best-rated lightcurve from February 2008 gave arotation period of 8.5616 hours with a consolidated brightness variation between 0.16 and 0.30magnitude (U=3).[3]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Lictoria measures between 69.93 and 86.724 kilometers in diameter and its surface has a lowalbedo between 0.05 and 0.066.[5][6][7][8][9]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.045 and a diameter of 78.86 kilometers based on anabsolute magnitude of 9.5.[3]

Notes

[edit]
  1. ^abKoff (2011) web: rotation period8.56 hours with a brightness amplitude of0.25 mag. Quality code of 2. Summary figures for (1107) Lictoria atLCDB
  2. ^abAnonymous Observer at CALL (2011): rotation period8.561 hours with a brightness amplitude of0.30 mag. Quality code of 2. Summary figures for (1107) Lictoria atLCDB
  3. ^abLightcurve plot of (1107) Lictoria (period of8.5610; amplitude of 0.19), by William Koff at theAntelope Hills Observatory (H09)
  4. ^abHamanowa (2011) web: rotation period8.5681±0.0001 hours with a brightness amplitude of0.26±0.01 mag. Quality code of 3. Summary figures for (1107) Lictoria atLCDB

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1107 Lictoria (1929 FB)" (2018-01-27 last obs.).Jet Propulsion Laboratory. Retrieved28 February 2018.
  2. ^abcdeSchmadel, Lutz D. (2007). "(1107) Lictoria".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 94.doi:10.1007/978-3-540-29925-7_1108.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1107) Lictoria". Asteroid Lightcurve Database (LCDB). Retrieved28 February 2018.
  4. ^ab"Asteroid 1107 Lictoria – 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 February 2018.
  6. ^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.S2CID 119293330.
  7. ^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.
  8. ^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)
  9. ^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 118700974.
  10. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (1107) Lictoria".Geneva Observatory. Retrieved28 February 2018.
  11. ^abcd"1107 Lictoria (1929 FB)".Minor Planet Center. Retrieved28 February 2018.
  12. ^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.S2CID 119280014.
  13. ^Schmadel, Lutz D. (1997).Dictionary of Minor Planet Names – Introduction, Source of Information. Springer Berlin Heidelberg. p. 16.ISBN 978-3-662-06617-1.

External links

[edit]
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