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2052 Tamriko

From Wikipedia, the free encyclopedia
Main-belt asteroid

2052 Tamriko
Discovery[1]
Discovered byR. M. West
Discovery siteLa Silla Obs.
Discovery date24 October 1976
Designations
(2052) Tamriko
Named after
Tamara West
(discoverer's wife)[2]
1976 UN · 1928 TD
1939 YA · 1942 JE
1949 UV · 1951 CP1
1952 FL · 1952 HL2
1954 TS · 1975 WB2
A902 UB
main-belt · (outer)
Eos[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc114.10 yr (41,676 days)
Aphelion3.2627AU
Perihelion2.7529 AU
3.0078 AU
Eccentricity0.0848
5.22yr (1,905 days)
340.25°
0° 11m 20.04s / day
Inclination9.5008°
213.86°
204.82°
Physical characteristics
Dimensions26.799±0.156 km[5]
27.51±0.50 km[6]
27.574±0.238 km[7]
29.11±5.31 km[8]
30.45±2.2 km(IRAS:3)[9]
7.462±0.003h[10]
7.470±0.002 h[11][a]
7.4702±0.0004 h[12]
7.471±0.001 h[12]
0.1225±0.020(IRAS:3)[9]
0.144±0.190[8]
0.150±0.006[6]
0.1508±0.0467[7]
0.158±0.025[5]
Tholen =S[1] · S[3]
B–V = 0.825[1]
U–B = 0.433[1]
10.40[8] · 10.48[1][3][6][7][9] · 10.57±0.18[13]

2052 Tamriko, provisional designation1976 UN, is a stony Eoanasteroid from the outer regions of theasteroid belt, approximately 27 kilometers in diameter. It was discovered on 24 October 1976, byRichard Martin West atESO'sLa Silla Observatory in northern Chile.[14] The asteroid was named after the discoverer's wife Tamara West.[2]

Orbit and classification

[edit]

Tamriko is a member of theEos family (606), the largestasteroid family in theouter main belt consisting of nearly 10,000 asteroids.[4][15]: 23  It orbits the Sun in theouter main-belt at a distance of 2.8–3.3 AU once every 5 years and 3 months (1,905 days). Its orbit has aneccentricity of 0.08 and aninclination of 10° with respect to theecliptic.[1]

The asteroid was first identified asA902 UB atHeidelberg Observatory in October 1902. Itsobservation arc begins 24 years prior to the official discovery observation, with its identification1952 FL atGoethe Link Observatory in March 1952.[14]

Physical characteristics

[edit]

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

Rotation period

[edit]

Between 2001 and 2011, four rotationallightcurve ofTamriko were obtained from photometric observations byEdwin Sheridan,Pierre Antonini,Laurent Bernasconi andBrian Warner. Lightcurve analysis gave arotation period between 7.462 and 7.471 hours with a brightness variation between 0.11 and 0.15magnitude (U=2/2/2/2).[10][11][12][a]

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,Tamriko measures between 26.799 and 30.45 kilometers in diameter and its surface has analbedo between 0.1225 and 0.158.[5][6][7][8][9]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, a standard albedo of 0.1225 and a diameter of 30.45 kilometers with anabsolute magnitude of 10.48.[3]

Naming

[edit]

Thisminor planet was named for Tamara West, wife of the discovererRichard Martin West.[2] The officialnaming citation was published by theMinor Planet Center on 1 July 1979 (M.P.C. 4786).[16]

Notes

[edit]
  1. ^ablightcurve plot of (2052) Tamriko, with a rotation period7.470 hours and a brightness amplitude of0.15 magnitude. Observation by Brian Warner, Palmer Divide Observatory (2011).

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 2052 Tamriko (1976 UN)" (2016-11-30 last obs.).Jet Propulsion Laboratory. Retrieved6 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2052) Tamriko".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 166.doi:10.1007/978-3-540-29925-7_2053.ISBN 978-3-540-00238-3.
  3. ^abcd"LCDB Data for (2052) Tamriko". Asteroid Lightcurve Database (LCDB). Retrieved6 July 2017.
  4. ^ab"Asteroid 2052 Tamriko – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^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. Retrieved6 July 2017.
  6. ^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)
  7. ^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.
  8. ^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. Retrieved6 July 2017.
  9. ^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.
  10. ^abSheridan, E. E. (June 2002)."Rotational Periods and Lightcurve Photometry of 697 Galilea, 1086 Nata, 2052 Tamriko, 4451 Grieve, and (27973) 1997 TR25".The Minor Planet Bulletin.29:32–33.Bibcode:2002MPBu...29...32S. Retrieved6 July 2017.
  11. ^abWarner, Brian D. (January 2012)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2011 June - September".The Minor Planet Bulletin.39 (1):16–21.Bibcode:2012MPBu...39...16W.ISSN 1052-8091. Retrieved6 July 2017.
  12. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (2052) Tamriko".Geneva Observatory. Retrieved6 July 2017.
  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. Retrieved6 July 2017.
  14. ^ab"2052 Tamriko (1976 UN)".Minor Planet Center. Retrieved6 July 2017.
  15. ^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 9780816532131.
  16. ^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.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.


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