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1261 Legia

From Wikipedia, the free encyclopedia
Dark Themistian asteroid from the outer regions of the asteroid belt

1261 Legia
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date23 March 1933
Designations
(1261) Legia
Pronunciation/ˈliə/
Named after
Latin name forLiège[2]
(Belgian city)
1933 FB · 1938 CS
1938 DH · 1944 FD
1966 DG
main-belt · (outer)
Themis[3] · background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc84.28 yr (30,785 days)
Aphelion3.6992AU
Perihelion2.5758 AU
3.1375 AU
Eccentricity0.1790
5.56yr (2,030 days)
57.530°
0° 10m 38.28s / day
Inclination2.4274°
67.282°
104.64°
Physical characteristics
Dimensions31.20 km(derived)[3]
31.26±11.50 km[5]
31.28±1.3 km[6]
32.13±0.66 km[7]
32.576±0.126 km[8]
35.324±0.345 km[9]
36.56±0.35 km[10]
8.693±0.007h[11]
0.048±0.009[10]
0.0564±0.0127[9]
0.06±0.05[5]
0.0601(derived)[3]
0.067±0.004[8]
0.070±0.003[7]
0.0719±0.006[6]
P[9] · S(assumed)[3]
11.00[6][7][9] · 11.10[10] · 11.12±0.72[12] · 11.2[1][3] · 11.29[5]

1261 Legia, provisional designation1933 FB, is a dark Themistianasteroid from the outer regions of theasteroid belt, approximately 32 kilometers in diameter. It was discovered on 23 March 1933, by astronomerEugène Delporte at theRoyal Observatory of Belgium in Uccle.[13] The asteroid was named for the Belgian city ofLiège (Luke).[2]

Orbit and classification

[edit]

Legia is a Themistian asteroid that belongs to theThemis family (602), a very largefamily of carbonaceous asteroids, named after24 Themis.[3] It is, however, a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[4]

It orbits the Sun in theouter asteroid belt at a distance of 2.6–3.7 AU once every 5 years and 7 months (2,030 days;semi-major axis of 3.14 AU). Its orbit has aneccentricity of 0.18 and aninclination of 2° with respect to theecliptic.[1]

The body'sobservation arc begins at Uccle in March 1933, five days after its official discovery observation.[13]

Physical characteristics

[edit]

Legia has been characterized as a primitive and reddishP-type asteroid by theWide-field Infrared Survey Explorer (WISE).[9]

Rotation period

[edit]

In January 2005, a rotationallightcurve ofLegia was obtained from photometric observations by French amateur astronomerLaurent Bernasconi. Lightcurve analysis gave arotation period of 8.693 hours with a brightness amplitude of 0.13magnitude (U=2+).[11]

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,Legia measures between 31.26 and 36.56 kilometers in diameter and its surface has analbedo between 0.048 and 0.0719.[5][6][7][8][9][10]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0601 and a diameter of 31.20 kilometers based on anabsolute magnitude of 11.2.[3]

Naming

[edit]

Thisminor planet was named "Legia", the Latin name of the Belgian city ofLiège (Luik). The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 116).[2]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1261 Legia (1933 FB)" (2017-07-05 last obs.).Jet Propulsion Laboratory. Retrieved28 November 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1261) Legia".Dictionary of Minor Planet Names – (1261) Legia.Springer Berlin Heidelberg. p. 104.doi:10.1007/978-3-540-29925-7_1262.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1261) Legia". Asteroid Lightcurve Database (LCDB). Retrieved28 November 2017.
  4. ^ab"Asteroid 1261 Legia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^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.
  6. ^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.
  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.; 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.
  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 35447010.
  10. ^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. Retrieved28 November 2017.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1261) Legia". Geneva Observatory. Retrieved28 November 2017.
  12. ^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. Retrieved28 November 2017.
  13. ^ab"1261 Legia (1933 FB)".Minor Planet Center. Retrieved28 November 2017.

External links

[edit]
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Comets
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