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6522 Aci

From Wikipedia, the free encyclopedia
Asteroid from the inner regions of the asteroid belt

6522 Aci
Shape model ofAci from itslightcurve
Discovery[1]
Discovered byE. F. Helin
Discovery sitePalomar Obs.
Discovery date9 July 1991
Designations
(6522) Aci
PronunciationItalian:[ˈaːtʃi]
Named after
ItalianJaci river atAcireale
(Acis and Galatea)[2]
1991 NQ · 1990 BH4
main-belt[1][3] · Phocaea[4][5]
Orbital characteristics[3]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc27.36 yr (9,995 days)
Aphelion2.8595AU
Perihelion1.9107 AU
2.3851 AU
Eccentricity0.1989
3.68yr (1,345 days)
68.743°
0° 16m 3.36s / day
Inclination22.109°
294.45°
314.18°
Physical characteristics
5.65 km(calculated)[4]
6.125±0.119 km km[6][7]
7.6921±0.0017 h[8]
0.23(assumed)[4]
0.392±0.029[6][7]
S(family-based)[5][4]
12.7[6] · 13.0[3] · 13.003±0.005(R)[8] · 13.1[1] · 13.45[4]

6522 Aci (prov. designation:1991 NQ) is an elongatedPhocaea asteroid from the inner regions of theasteroid belt. It was discovered on 9 July 1991, by American astronomerEleanor Helin atPalomar Observatory in California, United States.[1] The likely stonyS-type asteroid has arotation period of 5.65 hours and measures approximately 6 kilometers (3.7 miles) in diameter. It was named for theJaci river atAcireale in Italy, and refers to the myth ofAcis and Galatea.

Orbit and classification

[edit]

Aci is a member of thePhocaea family (701),[5] a relatively small group ofstony asteroids with similar orbital characteristics. It orbits the Sun in theinner main-belt at a distance of 1.9–2.9 AU once every 3 years and 8 months (1,345 days). Its orbit has aneccentricity of 0.20 and aninclination of 22° with respect to theecliptic.[3] In January 1990, the asteroid was first observed as1990 BH4 at the GermanKarl Schwarzschild Observatory, extending the body'sobservation arc by 17 months prior to its official discovery observation at Palomar.[1]

Naming

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Thisminor planet was named for theJaci river nearAcireale, southeast of Mount Etna inSicily, Italy. Other towns and villages along the river, such asAci Castello,Aci Trezza, andAci Sant'Antonio, were also honored.[2] The river's name refers to the mythAcis and Galatea fromGreek mythology, which is about a young Sicilian shepherd, who was killed by the jealous cyclopsPolyphemus, because of his love for the sea nymph Galatea. The minor planet74 Galatea is named after thisNereid.[2] Theapproved naming citation was published by theMinor Planet Center on 26 October 1996(M.P.C. 28090).[9]

Physical characteristics

[edit]

Rotation period

[edit]

In September 2010, a rotationallightcurve ofAci was obtained fromphotometric observations taken at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of7.6921 hours with a brightness variation of 0.68magnitude (U=2).[8]

Diameter and albedo

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According to theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Aci measures 6.1 kilometers in diameter and its surface has a highalbedo of 0.39,[6][7] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.23 – which derives from25 Phocaea, namesake and largest member of this orbital family – and calculates a diameter of 5.7 kilometers with anabsolute magnitude of 13.45.[4]

References

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  1. ^abcde"6522 Aci (1991 NQ)".Minor Planet Center. Retrieved28 April 2016.
  2. ^abcSchmadel, Lutz D. (2007). "(6522) Aci".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 539.doi:10.1007/978-3-540-29925-7_5924.ISBN 978-3-540-00238-3.
  3. ^abcd"JPL Small-Body Database Browser: 6522 Aci (1991 NQ)" (2017-06-06 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 18 September 2020. Retrieved21 June 2017.
  4. ^abcdef"LCDB Data for (6522) Aci". Asteroid Lightcurve Database (LCDB). Retrieved28 April 2016.
  5. ^abc"Asteroid 6522 Aci – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  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. Retrieved28 April 2016.
  7. ^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. Retrieved5 December 2016.
  8. ^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. Retrieved28 April 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved28 April 2016.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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