Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

771 Libera

From Wikipedia, the free encyclopedia
Main-belt asteroid

771 Libera
Modelled shape ofLibera from itslightcurve
Discovery[1]
Discovered byJ. Rheden
Discovery siteVienna Observatory
Discovery date21 November 1913
Designations
(771) Libera
PronunciationClassically/ˈlɪbərə/[2]
Named after
friend of discoverer[3]
1913 TO · 1958 HA
main-belt · (middle)[4]
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc101.75 yr (37166 d)
Aphelion3.3092 AU (495.05 Gm)
Perihelion1.9937 AU (298.25 Gm)
2.6514 AU (396.64 Gm)
Eccentricity0.24808
4.32yr (1576.9d)
268.14°
0° 13m 41.844s / day
Inclination14.936°
218.19°
227.36°
Earth MOID1.03684 AU (155.109 Gm)
Jupiter MOID2.11238 AU (316.008 Gm)
TJupiter3.299
Physical characteristics
Dimensions29.38±1.1 km(IRAS:6)[1][5]
28.91±0.72 km[6]
29.000±1.403 km[7]
29.33 km(derived)[4]
14.69±0.55km
5.892±0.002h[8]
5.92 h[9]
5.886±0.001 h[10]
5.89±0.05 h[10]
5.890±0.001 h[11]
5.892 h (0.2455 d)[1]
0.1303±0.010(IRAS:6)[1][5]
0.141±0.008[6]
0.1299±0.0158[7]
0.1226(SIMPS)[4]
B–V = 0.687
U–B = 0.300
X(Tholen),X(SMASS),X[4]
10.49[1]

771 Libera, provisional designation 1913 TO, is a metallicasteroid from the middle region of theasteroid belt, about 29 kilometers in diameter. It was discovered by Austrian astronomerJoseph Rheden at theVienna Observatory in Austria, on 21 November 1913.[12]

Description

[edit]
Lightcurve-based 3-D model ofLibera

The metallicX-type asteroid orbits the Sun at a distance of 2.0–3.3 AU once every 4 years and 4 months (1,576 days). Its orbit shows aneccentricity of 0.25 and istilted by 15 degrees to the plane of theecliptic. Aphotometric observation of the asteroid'slight-curve performed at the Palmer Divide Observatory during 1999 rendered arotation period of5.892±0.002 hours with a brightness variation of 0.57magnitude.[8] The result concurs with several previous observations, including a photometric analysis conducted over a twelve-year interval.[9][10][11]

According to the surveys carried out by the Infrared Astronomical Satellite,IRAS, the JapaneseAkari satellite, and the U.S.Wide-field Infrared Survey Explorer with its subsequentNEOWISE mission, the asteroid's surface has analbedo of 0.13 and 0.14, respectively, while the Collaborative Asteroid Lightcurve Link publishes a slightly lower figure of 0.12 from an alternative result of the Supplemental IRAS Minor Planet Survey.[4]

The minor planet was named by Mrs. Hedwig Rheden in honor of a friend of the discoverer.[3]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 771 Libera (1913 TO)" (2015-08-30 last obs.).Jet Propulsion Laboratory. Retrieved5 May 2016.
  2. ^Noah Webster (1884)A Practical Dictionary of the English Language
  3. ^abSchmadel, Lutz D. (2003). "(771) Libera".Dictionary of Minor Planet Names – (771) Libera.Springer Berlin Heidelberg. p. 73.doi:10.1007/978-3-540-29925-7_772.ISBN 978-3-540-29925-7.
  4. ^abcde"LCDB Data for (771) Libera". Asteroid Lightcurve Database (LCDB). Retrieved4 January 2016.
  5. ^abTedesco, 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.
  6. ^abUsui, 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)
  7. ^abMainzer, 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. Retrieved4 January 2016.
  8. ^abWarner, B. (March 2000)."Asteroid Photometry at the Palmer Divide Observatory".The Minor Planet Bulletin.27:4–6.Bibcode:2000MPBu...27....4W. Retrieved4 January 2016.
  9. ^abBinzel, 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. Retrieved4 January 2016.
  10. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (771) Libera".Geneva Observatory. Retrieved4 January 2016.
  11. ^abMarciniak, A.; Michalowski, T.; Hirsch, R.; Behrend, R.; Bernasconi, L.; Descamps, P.; et al. (December 2009)."Photometry and models of selected main belt asteroids. VII. 350 Ornamenta, 771 Libera, and 984 Gretia".Astronomy and Astrophysics.508 (3):1503–1507.Bibcode:2009A&A...508.1503M.doi:10.1051/0004-6361/200912741. Retrieved4 January 2016.
  12. ^"771 Libera (1913 TO)".Minor Planet Center. Retrieved4 January 2016.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=771_Libera&oldid=1313183429"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp