Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

2111 Tselina

From Wikipedia, the free encyclopedia
Stony asteroid in the outer asteroid belt
For other uses, seeTselina (disambiguation).

2111 Tselina
Shape model of Tselina from itslightcurve
Discovery[1]
Discovered byT. Smirnova
Discovery siteCrimean Astrophysical Obs.
Discovery date13 June 1969
Designations
(2111) Tselina
Named after
Virgin Lands Campaign
(agricultural program)[2]
1969 LG · 1928 RS
1928 SO · 1951 AR1
1968 HB1 · 1975 RE
1976 YF
main-belt · (outer)
Eos[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc48.47 yr (17,703 days)
Aphelion3.3041AU
Perihelion2.7299 AU
3.0170 AU
Eccentricity0.0952
5.24yr (1,914 days)
318.00°
0° 11m 17.16s / day
Inclination10.503°
167.17°
232.54°
Physical characteristics
22.773±0.247 km[5]
22.830±0.208 km[6]
24.54±2.8 km[7]
33.02±0.64 km[8]
6.563±0.001 h[9]
0.130±0.006[8]
0.1938±0.054[7]
0.2258±0.0251[6]
0.226±0.027[10]
Tholen =S[1] · S[3]
B–V = 0.799[1]
U–B = 0.463[1]
10.45[1][3][6][8] · 10.730±0.001(R)[11]

2111 Tselina (prov. designation:1969 LG) is a stonyEos asteroid from the outer regions of theasteroid belt. It was discovered on 13 June 1969, by Soviet astronomerTamara Smirnova atCrimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula.[12] TheS-type asteroid has arotation period of 6.6 hours and measures approximately 23 kilometers (14 miles) in diameter. It was later named after the SovietVirgin Lands Campaign.[2]

Orbit and classification

[edit]

Tselina is a member of theEos family (606), the largestasteroid family in theouter main belt consisting of nearly 10,000 asteroids.[4][13]: 23  It orbits the Sun at a distance of 2.7–3.3 AU once every 5 years and 3 months (1,914 days). Its orbit has aneccentricity of 0.10 and aninclination of 11° with respect to theecliptic.[1] In 1929, Tselina was first observed as1928 RS and1928 SO by the German and Belgian observatories atHamburg andUccle, respectively. The body'sobservation arc begins at the discovering observatory in 1968, or one year prior to its official discovery.[12]

Naming

[edit]

Thisminor planet was named afterthe tselina lands to commemorate the 25th anniversary of the SovietVirgin Lands Campaign.[2] The campaign was launched byNikita Khrushchev in 1953, with the intention to significantly increase the agricultural production in the USSR. The word "tselina" (or tseliny) means "virgin soil". The official naming citation was published by theMinor Planet Center on 1 April 1980 (M.P.C.5283).[14]

Physical characteristics

[edit]

In theTholen classification, Tselina is a common, stonyS-type asteroid.[1]

Rotation period

[edit]

In September 2001, a rotationallightcurve of Tselina was obtained fromphotometric observations by French amateur astronomerLaurent Bernasconi. Lightcurve analysis gave a well-definedrotation period of6.563±0.001 hours with a brightness variation of 0.17magnitude (U=3).[9] In September 2012, observations by astronomers at thePalomar Transient Factory, California, gave a concurring period of6.562±0.0021 hours with an amplitude of 0.29 magnitude (U=2).[11]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Tselina measures between 22.773 and 33.02 kilometers in diameter and its surface has analbedo between 0.13 and 0.226.[5][6][7][8][10] TheCollaborative Asteroid Lightcurve Link agrees with the results obtained by IRAS, that is, an albedo of 0.1938 and a diameter of 24.54 kilometers with anabsolute magnitude of 10.45.[3]

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 2111 Tselina (1969 LG)" (2016-10-14 last obs.).Jet Propulsion Laboratory. Retrieved3 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2111) Tselina".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 171.doi:10.1007/978-3-540-29925-7_2112.ISBN 978-3-540-00238-3.
  3. ^abcd"LCDB Data for (2111) Tselina". Asteroid Lightcurve Database (LCDB). Retrieved28 April 2017.
  4. ^ab"Asteroid 2111 Tselina – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abMasiero, 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. Retrieved29 April 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. ^abcTedesco, 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. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2111) Tselina".Geneva Observatory. Retrieved28 April 2017.
  10. ^abMasiero, 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. Retrieved28 April 2017.
  11. ^abWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved28 April 2017.
  12. ^ab"2111 Tselina (1969 LG)".Minor Planet Center. Retrieved28 April 2017.
  13. ^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 978-0-8165-3213-1.
  14. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved28 April 2017.



Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=2111_Tselina&oldid=1292938536"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp