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1138 Attica

From Wikipedia, the free encyclopedia
Main-belt asteroid

1138 Attica
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date22 November 1929
Designations
(1138) Attica
Pronunciation/ˈætɪkə/[2]
Named after
Attica Province
(province of Greece)[3]
1929 WF · 1954 GK
main-belt · (outer)
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc86.52 yr (31,600 days)
Aphelion3.3801AU
Perihelion2.9104 AU
3.1453 AU
Eccentricity0.0747
5.58yr (2,037 days)
249.74°
0° 10m 36.12s / day
Inclination13.971°
283.50°
107.03°
Physical characteristics
Dimensions23.681±0.113 km[4]
30±2 km(generic)[5]
unknown[6]
0.105±0.018[4]
11.4[1]

1138 Attica, provisional designation1929 WF, is anasteroid from the outer region of theasteroid belt, approximately 24 kilometers in diameter. It was discovered on 22 November 1929, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany.[7] It was named after theAttica Province in Greece.[3]

Orbit and classification

[edit]

Attica orbits the Sun in theouter main-belt at a distance of 2.9–3.4 AU once every 5 years and 7 months (2,037 days). Its orbit has aneccentricity of 0.07 and aninclination of 14° with respect to theecliptic.[1] The body'sobservation arc begins at Heidelberg with its official discovery observation. Noprecoveries were taken, and no prior identifications were made.[7]

Physical characteristics

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Attica measures 23.681 kilometers in diameter and its surface has analbedo of 0.105.[4] Based on a genericmagnitude-to-diameter conversion, its diameter is between 13 and 32 kilometer for anabsolute magnitude of 11.4 and an assumed albedo in the range of 0.05 to 0.25.[5] Since asteroids in the outer main-belt are typically ofcarbonaceous rather thanstony composition, with averaged standard albedos of 0.057,Attica's diameter can be estimated to measure close to 30 kilometers, as the lower a body's albedo (reflectivity), the larger its diameter at a fixedabsolute magnitude (brightness).[5]

As of 2017,Attica'sspectral type, as well as itsrotation period and shape remain unknown.[1][6] This is rather unusual, as both spectral type and rotation period have been determined for most larger and low-numbered asteroids(also see minor-planet lists from1 up to2000).

Naming

[edit]

Thisminor planet is named after theprovince of Attica in eastern Greece with the capitalAthens.[3] Naming citation was first mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 102).[3]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 1138 Attica (1929 WF)" (2016-05-29 last obs.).Jet Propulsion Laboratory. Retrieved8 February 2017.
  2. ^"Attica".Merriam-Webster.com Dictionary. Merriam-Webster.OCLC 1032680871.
  3. ^abcdSchmadel, Lutz D. (2007). "(1138) Attica".Dictionary of Minor Planet Names – (1138) Attica.Springer Berlin Heidelberg. p. 96.doi:10.1007/978-3-540-29925-7_1139.ISBN 978-3-540-00238-3.
  4. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved8 February 2017.
  5. ^abc"Absolute Magnitude (H)". NASA/JPL. Archived fromthe original on 2 March 2001. Retrieved8 February 2017.
  6. ^ab"LCDB Data for (1138) Attica". Asteroid Lightcurve Database (LCDB). Retrieved8 February 2017.
  7. ^ab"1138 Attica (1929 WF)".Minor Planet Center. Retrieved8 February 2017.

External links

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