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3841 Dicicco

From Wikipedia, the free encyclopedia
Main-belt asteroid binary
"Dicicco" redirects here. For other uses (and people with the surname), seeDiCicco.

3841 Dicicco
Discovery[1]
Discovered byB. A. Skiff
Discovery siteAnderson Mesa Stn.
Discovery date4 November 1983
Designations
(3841) Dicicco
Named after
Dennis di Cicco
(American astronomer)[2]
1983 VG7 · 1973 YM2
1982 KA2
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc43.27 yr (15,806 days)
Aphelion2.6394AU
Perihelion1.9083 AU
2.2739 AU
Eccentricity0.1607
3.43yr (1,252 days)
305.68°
0° 17m 14.64s / day
Inclination5.2241°
46.079°
359.76°
Knownsatellites1[4][5]
Physical characteristics
Dimensions4.74±1.11 km[6]
5.10 km(derived)[3]
6.252±0.110 km[7][8]
6.45±0.31 km[9]
3.5949±0.0002h[a]
3.5950±0.0001 h[5]
0.24(assumed)[3]
0.294±0.033[9][8]
0.3126±0.0343[7]
0.38±0.24[6]
SMASS =S[1] · S[10][3]
12.90[9][7] · 13.00[6] · 13.2[1] · 13.26±0.25[10] · 13.63±0.04[3][5]

3841 Dicicco, provisional designation1983 VG7, is a stony Florianasteroid and synchronousbinary system from the inner regions of theasteroid belt, approximately 5 kilometers in diameter. It was discovered on 4 November 1983, by American astronomerBrian Skiff at Lowell'sAnderson Mesa Station near Flagstaff, Arizona, in the United States.[11] It was named after American astronomerDennis di Cicco.[2] Itsminor-planet moon was discovered in 2014.[5]

Orbit and classification

[edit]

Dicicco is member of theFlora family, one of the largest groups of stony asteroids in theinner main-belt. It orbits the Sun at a distance of 1.9–2.6 AU once every 3 years and 5 months (1,252 days). Its orbit has aneccentricity of 0.16 and aninclination of 5° with respect to theecliptic.[1]

It was first identified as1973 YM2 atCrimea–Nauchnij in 1973, extending the body'sobservation arc by 10 years prior to its official discovery observation at Anderson Mesa.[11]

Physical characteristics

[edit]

Dicicco is a stonyS-type asteroid in theSMASS classification.[1]

Rotation period

[edit]

In December 2014, two rotationallightcurves ofDicicco were obtained from photometric observations by an international collaboration of American and European astronomers. Lightcurve analysis gave arotation period of 3.5949 and 3.5950 hours with a brightness amplitude of 0.18 and 0.19magnitude, respectively (U=3/n.a.).[5][a]

Diameter and albedo

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Dicicco measures between 4.74 and 6.45 kilometers in diameter and its surface has analbedo between 0.294 and 0.38.[6][7][8][9] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 — derived from8 Flora, the family's largest member and namesake – and derives a diameter of 5.10 kilometers using anabsolute magnitude of 13.63.[3]

Satellite

[edit]

During the photometric observations made in December 2014, it was revealed thatDicicco is a synchronousbinary asteroid. Itsminor-planet moon measures at least 1.67 kilometers in diameter based on a diameter-ratio of larger than 0.28.[4] Its orbit has an estimatedsemi-major axis of 12 kilometers, and a derivedperiod of 21.63 and 21.641 hours, respectively.[5][a]

Naming

[edit]

Thisminor planet was named after American amateur astronomer and astrophotographerDennis di Cicco.[2] The approved naming citation was published by theMinor Planet Center on 10 April 1990 (M.P.C. 16246).[12]

Notes

[edit]
  1. ^abcKlinglesmith (2014) web: rotation period3.5949±0.0002 hours with a brightness amplitude of mag, obs. date: 2014-11-26; Quality Code: n.a.. Summary figures for (3841) Dicicco atCollaborative Asteroid Lightcurve Link (CALL). Referenced publication2014CBET.4033....1K is not a valid abstract at ADS

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 3841 Dicicco (1983 VG7)" (2017-03-30 last obs.).Jet Propulsion Laboratory. Retrieved16 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(3841) Dicicco".Dictionary of Minor Planet Names – (3841) Dicicco.Springer Berlin Heidelberg. pp. 325–326.doi:10.1007/978-3-540-29925-7_3833.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (3841) Dicicco". Asteroid Lightcurve Database (LCDB). Retrieved16 June 2017.
  4. ^abJohnston, Robert (16 November 2014)."(3841) Dicicco". Johnston's Archive. Retrieved16 June 2017.
  5. ^abcdefKlinglesmith, Daniel A. III; Franco, Lorenzo; Marchini, Alessandro; Odden, Carolyn E.; Pravec, Petr; Scardella, Maurizio; et al. (October 2015)."3841 Dicicco: A Binary Asteroid".The Minor Planet Bulletin.42 (4):249–250.Bibcode:2015MPBu...42..249K.ISSN 1052-8091. Retrieved16 June 2017.
  6. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117. Retrieved16 June 2017.
  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. ^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. Retrieved16 June 2017.
  9. ^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.
  10. ^abVeres, 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.
  11. ^ab"3841 Dicicco (1983 VG7)".Minor Planet Center. Retrieved16 June 2017.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved16 June 2017.

External links

[edit]
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