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4340 Dence

From Wikipedia, the free encyclopedia
Main-belt asteroid

4340 Dence
Discovery[1]
Discovered byC. Shoemaker
Discovery sitePalomar Obs.
Discovery date4 May 1986
Designations
(4340) Dence
Named after
Michael R. Dence[1]
(Canadian geologist)
1986 JZ · 1982 KF4
1986 LN
main-belt[1][2] · (inner)
background[3] · Phocaea[4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc38.28yr (13,983 d)
Aphelion2.9475AU
Perihelion1.8408 AU
2.3941 AU
Eccentricity0.2311
3.70 yr (1,353 d)
212.55°
0° 15m 57.96s / day
Inclination25.155°
81.012°
175.79°
Physical characteristics
8.110±0.138 km[5][6]
8.37 km(calculated)[4]
7.546±0.005 h[7]
7.558±0.0018 h[a]
7.5668±0.0018 h[a]
15.473±0.005 h(poor)[8]
0.155±0.028[5][6]
0.23(assumed)[4]
SMASS =S[2][4]
12.6[2][4]
12.67±1.14[9]
13.1[6]

4340 Dence, provisional designation1986 JZ, is a background or Phocaeaasteroid from the inner regions of theasteroid belt, approximately 8 kilometers (5 miles) in diameter. It was discovered on 4 May 1986, by American astronomerCarolyn Shoemaker at thePalomar Observatory in California.[1] TheS-type asteroid has arotation period of 7.5 hours.[4] It was named after Canadian geologistMichael R. Dence.[1]

Orbit and classification

[edit]

Dence is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[3] Based on osculating Keplerianorbital elements, the asteroid has also been classified as a member of the stonyPhocaea family (701).[4] It orbits the Sun in theinner asteroid belt at a distance of 1.8–2.9 AU once every 3 years and 8 months (1,353 days;semi-major axis of 2.39 AU). Its orbit has aneccentricity of 0.23 and aninclination of 25° with respect to theecliptic.[2] The body'sobservation arc begins with aprecovery taken at theSiding Spring Observatory in November 1979, more than six years prior to its official discovery observation at Palomar.[1]

Physical characteristics

[edit]

In theSMASS classification,Dence is a common, stonyS-type asteroid.[2][4]

Rotation period

[edit]

Since 2008, several rotationallightcurves ofDence have been obtained fromphotometric observations by Czech astronomerPetr Pravec and by Maurice Clark at the observatory of theMontgomery College in Maryland, United States (U=3-/1/2/2).[7][8][a] Analysis of the best-rated lightcurve gave arotation period of 7.546 hours with a brightness amplitude of 0.58magnitude (U=3-).[4][7]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Dence measures 8.110 kilometers in diameter and its surface has analbedo of 0.155,[5][6] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.23 – derived from25 Phocaea, theparent body of the Phocaea family – and calculates a diameter of 8.37 kilometers based on anabsolute magnitude of 12.6.[4]

Naming

[edit]

Thisminor planet was named after Canadian geologistMichael R. Dence executive director of theRoyal Society of Canada. He was a pioneer in the geologic investigation of ancientimpact craters on theCanadian Shield(also seeSudbury Basin andManicouagan Reservoir).[1] The official naming citation was published by theMinor Planet Center on 30 January 1991 (M.P.C. 17656).[10]

Notes

[edit]
  1. ^abcLightcurve plot (April 2008) andfollow-up plot (May 2008) of (4340) Dence byPetr Pravec. Rotation period of7.558±0.0018 and7.5668±0.0018 hours and a brightness amplitude of0.07±0.01 and0.11±0.01 magnitude. Quality code of 2/2. Summary figures at theLCDB andPravec, P.; Wolf, M.; Sarounova, L. (2008) Plots fromOndrejov data, obtained by the NEO Photometric Program and collaborating projects.

References

[edit]
  1. ^abcdefg"4340 Dence (1986 JZ)".Minor Planet Center. Retrieved3 May 2018.
  2. ^abcdef"JPL Small-Body Database Browser: 4340 Dence (1986 JZ)" (2018-02-27 last obs.).Jet Propulsion Laboratory. Retrieved3 May 2018.
  3. ^ab"Asteroid 4340 Dence – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  4. ^abcdefghij"LCDB Data for (4340) Dence". Asteroid Lightcurve Database (LCDB). Retrieved3 May 2018.
  5. ^abcMasiero, 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.S2CID 118745497.
  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.S2CID 35447010. (catalog)
  7. ^abcClark, Maurice (July 2015). "Asteroid Photometry from the Preston Gott Observatory".The Minor Planet Bulletin.42 (3):163–166.Bibcode:2015MPBu...42..163C.ISSN 1052-8091.
  8. ^abClark, Maurice (October 2008). "Asteroid Lightcurve Observations".The Minor Planet Bulletin.35 (4):152–154.Bibcode:2008MPBu...35..152C.ISSN 1052-8091.
  9. ^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.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 May 2018.

External links

[edit]
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