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1951 Lick

From Wikipedia, the free encyclopedia
Asteroid

1951 Lick
Discovery[1]
Discovered byC. A. Wirtanen
Discovery siteLick Obs.
Discovery date26 July 1949
Designations
(1951) Lick
Named after
James Lick(philanthropist)[2]
1949 OA
Mars-crosser[1][3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc67.12 yr (24,514 days)
Aphelion1.4760AU
Perihelion1.3049 AU
1.3904 AU
Eccentricity0.0616
1.64yr (599 days)
221.32°
0° 36m 3.96s / day
Inclination39.091°
130.75°
140.52°
Earth MOID0.3068 AU · 119.5LD
Physical characteristics
Dimensions5.57±0.5 km(IRAS:3)[5]
5.59 km(derived)[4]
4.424±0.006h[6]
5.2974±0.0004 h[7]
5.3008±0.0024 h[a]
5.3016±0.0020 h[b]
5.317±0.001 h[8]
0.0895±0.020(IRAS:3)[5]
0.1028(derived)[4]
SMASS =A[1] · A[4][6]
14.20±0.2[b] · 14.2[1] · 14.35±0.2[9] · 14.35[4] · 14.5±0.2[6] · 14.51[5]

1951 Lick, provisional designation1949 OA, is a rare-typeasteroid andMars-crosser, approximately 5.6 kilometers in diameter. It was discovered on 26 July 1949, by American astronomerCarl Wirtanen atLick Observatory on the summit of Mount Hamilton, California, and named for American philanthropistJames Lick.[2][3]

Orbit

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The asteroid orbits the Sun at a distance of 1.3–1.5 AU once every 20 months (599 days). Its orbit has aneccentricity of 0.06 and aninclination of 39° with respect to theecliptic.[1]Lick'sobservation arc begins with its discovery observation, as noprecoveries were taken, and no prior identifications were made.[3]

Physical characteristics

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Spectral type

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In theSMASS taxonomic scheme,Lick'sspectral type is that of a rareA-type asteroid with a surface consisting of almost pureolivine.[10] As of 2016, only 17 minor planets of this type are known.[11]

Rotation period

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In July 2008, a rotationallightcurve was obtained from photometric by astronomerBrian D. Warner at his Palmer Divide Observatory in Colorado, United States. It gave a well-definedrotation period of 5.2974 hours with a brightness variation of 0.25 inmagnitude (U=3).[7] Several lightcurves with a lower or unassessed quality have been obtained by astronomersWiesław Z. Wiśniewski andPetr Pravec in the 1980s and 1990s.[6][a][b] The most recent observation by Michael Lucas in February 2011, gave a period of 5.317 hours with an amplitude of 0.33 magnitude (U=2).[8]

Diameter and albedo

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According to 3 observations taken by the Infrared Astronomical SatelliteIRAS,Lick measures 5.57 kilometers in diameter and its surface has analbedo of 0.09.[5] TheCollaborative Asteroid Lightcurve Link agrees with the results obtained by IRAS and derives an albedo of 0.10 and a diameter of 5.59 kilometers with anabsolute magnitude of 14.35.[4]

Naming

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Lick was named in honor ofJames Lick (1796–1876), Americanphilanthropist and the founder of the discovering Lick Observatory of the University of California. He is also honored by a lunar craterLick.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3938).[12]

Notes

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  1. ^abSummary figures for (1951) Lick: rotation period5.3008±0.0024 hours (Pravec-1998web) atLight Curve Database
  2. ^abcSummary figures for(1951) Lick: rotation period 5.3016 hours (Pravec-1997web) atLight Curve Database

References

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  1. ^abcdef"JPL Small-Body Database Browser: 1951 Lick (1949 OA)" (2016-09-10 last obs.).Jet Propulsion Laboratory. Retrieved2 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1951) Lick".Dictionary of Minor Planet Names – (1951) Lick.Springer Berlin Heidelberg. pp. 156–157.doi:10.1007/978-3-540-29925-7_1952.ISBN 978-3-540-00238-3.
  3. ^abc"1951 Lick (1949 OA)".Minor Planet Center. Retrieved9 December 2016.
  4. ^abcdef"LCDB Data for (1951) Lick". Asteroid Lightcurve Database (LCDB). Retrieved9 December 2016.
  5. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved17 October 2019.
  6. ^abcdWisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995). "Photoelectric Observations of 125 Asteroids".Abstracts of the Lunar and Planetary Science Conference.26: 1511.Bibcode:1995LPI....26.1511W.
  7. ^abWarner, Brian D. (January 2009). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2008 May - September".The Minor Planet Bulletin.36 (1):7–13.Bibcode:2009MPBu...36....7W.ISSN 1052-8091.
  8. ^abLucas, Michael P.; Ryan, Jeffrey G.; Fauerbach, Michael; Grasso, Salvatore (October 2011). "Lightcurve Analysis of Five Taxonomic A-class Asteroids".The Minor Planet Bulletin.38 (4):218–220.Bibcode:2011MPBu...38..218L.ISSN 1052-8091.
  9. ^Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026.
  10. ^de León, J.; Duffard, R.; Licandro, J.; Lazzaro, D. (July 2004)."Mineralogical characterization of A-type asteroid (1951) Lick"(PDF).Astronomy and Astrophysics.422 (3):L59 –L62.Bibcode:2004A&A...422L..59D.doi:10.1051/0004-6361:20048009. Retrieved9 December 2016.
  11. ^"JPL Small-Body Database Search Engine: spec. type = A (SMASSII)". JPL Solar System Dynamics. Retrieved7 November 2015.
  12. ^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.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
Minor planets
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Distant minor planet
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