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3868 Mendoza

From Wikipedia, the free encyclopedia
Vestian asteroid and binary system

3868 Mendoza
Discovery[1]
Discovered byC. J. van Houten
I. van Houten G.
T. Gehrels
Discovery sitePalomar Obs.
Discovery date24 September 1960
Designations
(3868) Mendoza
Named after
Eugenio Mendoza
(Mexican astronomer)[2]
4575 P-L · 1935 SA1
1952 HV3 · 1953 TD2
1977 KD1
main-belt · Vesta[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc62.81 yr (22,941 days)
Aphelion2.5649AU
Perihelion2.1032 AU
2.3341 AU
Eccentricity0.0989
3.57yr (1,302 days)
353.29°
0° 16m 35.04s / day
Inclination8.1076°
171.57°
186.20°
Knownsatellites1[4][5][6]
Physical characteristics
Dimensions8.628±0.157 km[7]
6.37±0.27 km[8]
9.351±0.049 km[9]
9.396 km[10]
9.40 km(taken)[3]
2.77082±0.00005h[4]
2.77090±0.00005 h[5]
2.77099±0.00002 h[3]
2.77103±0.00003 h[11]
0.1621±0.0288[9]
0.1649[10]
0.218±0.032[7]
0.436±0.076[8]
S[3]
12.30±0.04(R)[5] · 12.30±0.02(R)[4] 12.5[1][8] · 12.6[1] · 12.70±0.37[12] · 12.71±0.04[3][10] · 12.75[9]

3868 Mendoza, provisional designation4575 P-L is a stony Vestianasteroid andbinary system from the inner regions of theasteroid belt, approximately 9 kilometers in diameter. It was discovered on 24 September 1960, by astronomersCornelis Johannes van Houten,Ingrid van Houten-Groeneveld andTom Gehrels atPalomar Observatory.[13]

Orbit and characterization

[edit]

Mendoza orbits the Sun at a distance of 2.1–2.6 AU once every 3 years and 7 months (1,302 days). Its orbit has aneccentricity of 0.10 and aninclination of 8° with respect to theecliptic.[1]

Satellite

[edit]

In 2009, aminor-planet moon was discovered. The satellite measures2.01±0.18 km in diameter and orbitsMendoza in a little more than a day.[4][5][6]

Palomar–Leiden

[edit]

Thesurvey designation "P-L" stands forPalomar–Leiden, named after Palomar Observatory andLeiden Observatory, which collaborated on the fruitfulPalomar–Leiden survey in the 1960s. Gehrels used Palomar'sSamuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped thephotographic plates to Ingrid and Cornelis van Houten at Leiden Observatory whereastrometry was carried out. The trio are credited with the discovery ofseveral thousand asteroid discoveries.[14]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer (WISE) with its subsequentNEOWISE mission,Mendoza measures between 8.628 and 9.351 kilometers in diameter and its surface has analbedo between 0.1621 and 0.436.[7][8][9] TheCollaborative Asteroid Lightcurve Link adoptsPetr Pravec's revised WISE data, that is, an albedo of 0.1649 and a rounded diameter of 9.40 kilometers with anabsolute magnitude of 12.71.[3][10]

Naming

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Thisminor planet was named in honor of Mexican astronomerEugenio Mendoza (born 1928), expert in photometry and spectroscopy, member of theIAU and teacher at several Mexican universities.[2][15] The approved naming citation was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22499).[16]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 3868 Mendoza (4575 P-L)" (2016-07-31 last obs.).Jet Propulsion Laboratory. Retrieved16 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(3868) Mendoza".Dictionary of Minor Planet Names – (3868) Mendoza.Springer Berlin Heidelberg. p. 328.doi:10.1007/978-3-540-29925-7_3857.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (3868) Mendoza". Asteroid Lightcurve Database (LCDB). Retrieved16 June 2017.
  4. ^abcdPravec, P.; Scheirich, P.; Vokrouhlický, D.; Harris, A. W.; Kusnirák, P.; Hornoch, K.; et al. (March 2012)."Binary asteroid population. 2. Anisotropic distribution of orbit poles of small, inner main-belt binaries".Icarus.218 (1):125–143.Bibcode:2012Icar..218..125P.doi:10.1016/j.icarus.2011.11.026. Retrieved16 June 2017.
  5. ^abcdOey, J.; Pravec, P.; Kusnirak, P.; Hornoch, K.; Brinsfield, J.; Chiorny, V.; et al. (June 2009)."(3868) Mendoza".Central Bureau Electronic Telegrams.1835 (1835): 1.Bibcode:2009CBET.1835....1O. Retrieved16 June 2017.
  6. ^abJohnston, Robert (21 September 2014)."(3868) Mendoza". johnstonsarchive.net. Retrieved16 June 2017.
  7. ^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. Retrieved16 June 2017.
  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. Retrieved16 June 2017.
  9. ^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.
  10. ^abcdPravec, 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. Retrieved16 June 2017.
  11. ^Oey, Julian; Masi, G.; Mallia, F.; Tagliaferri, U.; Higgins, David; Durkee, Russell I.; et al. (June 2007)."Rotation Period and Amplitude Change of Minor Planet 3868 Mendoza".The Minor Planet Bulletin.34 (2):39–40.Bibcode:2007MPBu...34...39O.ISSN 1052-8091. Retrieved16 June 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. Retrieved16 June 2017.
  13. ^"3868 Mendoza (4575 P-L)".Minor Planet Center. Retrieved16 June 2017.
  14. ^"Minor Planet Discoverers".Minor Planet Center. 11 June 2017. Retrieved16 June 2017.
  15. ^"V. Eugenio E. Mendoza".International Astronomical Union. January 2015. Retrieved10 October 2015.
  16. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved16 June 2017.

External links

[edit]
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