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3996 Fugaku

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3996 Fugaku
Discovery [1]
Discovered byM. Arai
H. Mori
Discovery siteYorii Obs.
Discovery date5 December 1988
Designations
(3996) Fugaku
Named after
Mount Fuji(Japan)[2]
1988 XG1 · 1939 FZ
1957 TB · 1981 SO5
1981 UM16
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc78.22 yr (28,570 days)
Aphelion2.4941AU
Perihelion2.0254 AU
2.2597 AU
Eccentricity0.1037
3.40yr (1,241 days)
338.50°
0° 17m 24.36s / day
Inclination2.2842°
90.755°
156.18°
Physical characteristics
Dimensions5.151±0.074 km[4]
5.231±0.032 km[5]
5.40 km(calculated)[3]
5.88±1.10 km[6]
7.1912±0.0016h[7]
0.24(assumed)[3]
0.34±0.17[6]
0.4086±0.0152[5]
0.420±0.066[4]
S[3]
13.0[1][5][6] · 13.055±0.003(R)[7] · 13.5[3] · 13.57±0.25[8]

3996 Fugaku, provisional designation1988 XG1, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 5.5 kilometers in diameter. It was discovered on 5 December 1988, by Japanese amateur astronomersMasaru Arai andHiroshi Mori atYorii Observatory in central Japan.[9] It was named forMount Fuji, Japan.[2]

Orbit and classification

[edit]

Fugaku is a member of theFlora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 2.0–2.5 AU once every 3 years and 5 months (1,241 days). Its orbit has aneccentricity of 0.10 and aninclination of 2° with respect to theecliptic.[1] It was first identified as1939 FZ atTurku Observatory in 1939, extending the asteroid'sobservation arc by 49 years prior to its official discovery observation.[9]

Physical characteristics

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Fugaku has been characterized as a stonyS-type asteroid, the most common type in the inner main-belt.[1]

Rotation period

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In March 210, a rotationallightcurve ofFugaku was obtained from photometric observations at thePalomar Transient Factory in California. It gave arotation period of 7.1912 hours with a change in brightness of 0.86magnitude (U=2).[7]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Fugaku measures between 5.15 and 5.88 kilometers in diameter, and its surface has analbedo between 0.34 and 0.42.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of this family – and calculates a diameter of 5.40 kilometers with anabsolute magnitude of 13.5.[3]

Naming

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Thisminor planet was named for the ancient name ofMount Fuji, Japan's highest mountain and a well-known symbol. Another minor planet,1584 Fuji, is also named for this mountain.[2] The official naming citation was published by theMinor Planet Center on 4 May 1999 (M.P.C. 34619).[10]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 3996 Fugaku (1988 XG1)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved19 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(3996) Fugaku".Dictionary of Minor Planet Names – (3996) Fugaku.Springer Berlin Heidelberg. p. 340.doi:10.1007/978-3-540-29925-7_3981.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (3996) Fugaku". Asteroid Lightcurve Database (LCDB). Retrieved3 January 2017.
  4. ^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. Retrieved3 January 2017.
  5. ^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.
  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. Retrieved3 January 2017.
  7. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved3 January 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. Retrieved3 January 2017.
  9. ^ab"3996 Fugaku (1988 XG1)".Minor Planet Center. Retrieved3 January 2017.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 January 2017.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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