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3402 Wisdom

From Wikipedia, the free encyclopedia
Mars-crossing asteroid

3402 Wisdom
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date5 August 1981
Designations
(3402) Wisdom
Named after
Jack Wisdom[2]
(American planetary scientist)
1981 PB
Mars-crosser[1][3][4]
Orbital characteristics[1]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc41.20yr (15,047 d)
Aphelion2.7283AU
Perihelion1.5352 AU
2.1317 AU
Eccentricity0.2798
3.11 yr (1,137 d)
285.37°
0° 19m 0.12s / day
Inclination4.8531°
357.87°
303.69°
Earth MOID0.5266 AU (205LD)
Physical characteristics
2.05±0.49 km[5]
2.50±0.50 km[6]
2.59 km (derived)[4]
4.9949±0.0001 h[7]
4.9951±0.0001 h[a]
0.20 (assumed)[4]
0.283±0.113[6]
0.32±0.16[5]
S (assumed)[4]
14.85±0.11 (R)[a]
15.00[1][6]
15.13±0.26[8]
15.34[4][9]
15.44[5]

3402 Wisdom, provisional designation1981 PB, is a stonyasteroid andMars-crosser on an eccentric orbit from the inner regions of theasteroid belt, approximately 2.5 kilometers (1.6 miles) in diameter. It was discovered on 5 August 1981, by American astronomerEdward Bowell at Lowell'sAnderson Mesa Station near Flagstaff, Arizona, in the United States.[3] The presumed brightS-type asteroid has arotation period of 4.99 hours.[4] It was named after American planetary scientistJack Wisdom.[2]

Orbit and classification

[edit]

Wisdom is aMars-crossing asteroid, a member of a dynamically unstable group, located between themain belt and thenear-Earth populations, and crossing the orbit of Mars at 1.666 AU. It orbits the Sun at a distance of 1.5–2.7 AU once every 3 years and 1 month (1,137 days;semi-major axis of 2.13 AU). Its orbit has aneccentricity of 0.28 and aninclination of 5° with respect to theecliptic.[1]

The body'sobservation arc begins with aprecovery taken atPalomar Observatory in February 1977, more than 4 years prior to its official discovery observation at Anderson Mesa.[3]

Physical characteristics

[edit]

Wisdom is an assumed stonyS-type asteroid.[4]

Rotation period

[edit]

In October 2006, two rotationallightcurves of Wisdom were obtained from photometric observations atOndřejov,Skalnaté pleso and Carbuncle Hill observatories (912;I00). Lightcurve analysis gave a well-definedrotation period of 4.9949 and 4.9951 hours with a high brightness variation of 0.75 and 0.74magnitude, respectively (U=3/3).[7][a] A high brightness amplitude typically indicate that the body has an elongated rather than spherical shape.

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Wisdom measures 2.05 and 2.50 kilometers in diameter and its surface has analbedo of 0.32 and 0.283, respectively.[5][6] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 2.59 kilometers based on anabsolute magnitude of 15.34.[4]

With amean diameter of approximately 2.5 kilometers, Wisdom is one of the smaller mid-sized Mars-crossing asteroids. It is assumed that there are up to 10 thousand Mars-crossers larger than 1 kilometer.[10] The largest members of this dynamical group are132 Aethra,323 Brucia,2204 Lyyli and512 Taurinensis, which measure between 43 and 25 kilometers in diameter.

Naming

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Thisminor planet was named afterJack Wisdom (born 1953), a dynamicist and professor ofplanetary sciences atMIT. Wisdom pioneered in the study of the dynamics and long-term stability of theSolar System, and demonstrated the dynamical mechanism for the clearing of asteroid in theKirkwood gaps of the asteroid belt.[2] The official naming citation was published by theMinor Planet Center on 2 February 1988 (M.P.C. 12803).[11]

Notes

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  1. ^abcPravec October (2006) web:lightcurve plot of (3402) Wisdom, with a rotation period4.9951±0.0001 hours with a brightness amplitude of0.74±0.02 mag. Quality Code of 3. Observation in the R-band. Absolute magnitude of14.85±0.11. Summary figures atLCDB andOndrejov Asteroid Photometry Project(seedata sheet)

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 3402 Wisdom (1981 PB)" (2018-04-24 last obs.).Jet Propulsion Laboratory. Retrieved14 May 2018.
  2. ^abcSchmadel, Lutz D. (2007). "(3402) Wisdom".Dictionary of Minor Planet Names – (3402) Wisdom.Springer Berlin Heidelberg. pp. 283–284.doi:10.1007/978-3-540-29925-7_3402.ISBN 978-3-540-00238-3.
  3. ^abc"3402 Wisdom (1981 PB)".Minor Planet Center. Retrieved26 October 2017.
  4. ^abcdefgh"LCDB Data for (3402) Wisdom". Asteroid Lightcurve Database (LCDB). Retrieved26 October 2017.
  5. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  6. ^abcdAlí-Lagoa, V.; Delbo', M. (July 2017). "Sizes and albedos of Mars-crossing asteroids from WISE/NEOWISE data".Astronomy and Astrophysics.603: 8.arXiv:1705.10263.Bibcode:2017A&A...603A..55A.doi:10.1051/0004-6361/201629917.S2CID 119224590.
  7. ^abPray, Donald P.; Kusnirak, Peter; Galad, Adrian; Vilagi, Jozef; Kornos, Leos; Gajdos, Stefan; et al. (June 2007)."Lightcurve Analysis of Asteroids 2006 BQ6, 2942, 2943 3402, 3533, 6497, 6815, 7033, 12336, and 14211".The Minor Planet Bulletin.34 (2):44–46.Bibcode:2007MPBu...34...44P.ISSN 1052-8091. Retrieved26 October 2017.
  8. ^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.S2CID 53493339. Retrieved26 October 2017.
  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. Retrieved26 October 2017.
  10. ^Steel, D. I. (August 1985)."Collisions in the solar systems. II - Asteroid impacts upon Mars".Monthly Notices of the Royal Astronomical Society.215 (3):369–381.Bibcode:1985MNRAS.215..369S.doi:10.1093/mnras/215.3.369.ISSN 0035-8711.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved26 October 2017.

External links

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