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1150 Achaia

From Wikipedia, the free encyclopedia
Main-belt asteroid

1150 Achaia
Shape model ofAchaia from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date2 September 1929
Designations
(1150) Achaia
Pronunciation/əˈkə/,[2]/əˈkə/[3]
Named after
Achaea(Greek region)[4]
1929 RB · 1955 SZ1
Orbital characteristics[5]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc86.78 yr (31,696 days)
Aphelion2.6392AU
Perihelion1.7424 AU
2.1908 AU
Eccentricity0.2047
3.24yr (1,184 days)
348.01°
0° 18m 14.04s / day
Inclination2.3929°
206.54°
139.58°
Earth MOID0.7366 AU
Physical characteristics
7.689±0.020 km[8]
7.82 km(calculated)[9]
7.928±0.036 km[10]
7.96±0.25 km[11]
8.16±0.25 km[12]
60.99±0.05 h[a]
  • (5.0°, −65.0°) (λ11)[7]
  • (20.0°, −69.0°) (λ22)[7]
0.2343±0.0479[10]
0.239±0.017[11]
0.24(assumed)[9]
0.242±0.029[12]
0.251±0.017[8]
12.60[12] · 12.7[5][9][10][11]

1150 Achaia (/əˈkə/);prov. designation:1929 RB) is a stonybackground asteroid from the inner regions of theasteroid belt. It was discovered byKarl Reinmuth atHeidelberg Observatory on 2 September 1929.[1] TheS-type asteroid has a notably longrotation period of hours 61 hours and measures approximately 7.8 kilometers (4.8 miles) in diameter. It is named for the Greek region ofAchaia.[4]

Discovery

[edit]

Achaia was discovered on 2 September 1929, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany.[1] Ten nights later, it was independently discovered byFriedrich Schwassmann andArno Wachmann atBergedorf.[4] The body'sobservation arc begins at Heidelberg, five days after its first and official discovery observation.<[1]

Orbit and classification

[edit]

Located in the orbital region of theFlora family,[9] one of the largest, yet disputed families of the main-belt,Achaia is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[6][7] It orbits the Sun at a distance of 1.7–2.6 AU once every 3 years and 3 months (1,184 days). Its orbit has aneccentricity of 0.20 and aninclination of 2° with respect to theecliptic.[5]

Naming

[edit]

Thisminor planet is named for the regionAchaea (or "Achaia") inWestern Greece. It is located in the northern part of thePeloponnese peninsula and borders on the gulfs ofPatras andCorinth.[4] Naming citation was first mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 107).[4]

Physical characteristics

[edit]

In the Tholen-like taxonomy of theSmall Solar System Objects Spectroscopic Survey (S3OS2),Achaia is a common, stonyS-type asteroid, while in the survey's SMASS (Bus–Binzel)-like taxonomic variant, it is an Sl-subtype, which transitions from the S-type to the uncommonL-type asteroid.[7][13]

Photometry

[edit]

A rotationallightcurve ofAchaia was obtained fromphotometric observations by Czech astronomerPetr Pravec atOndřejov Observatory in October 2007.[b] It gave a well-definedrotation period of 60.99 hours with a brightness variation of 0.72magnitude (U=3).[a]

Published in 2016, two additional lightcurves were derived from modeled photometric data using various sources. They gave asidereal rotation period of61.071±0.001 and61.072±0.005 hours, as well as aspin axis of (5.0°, −65.0°) and (20.0°, −69.0°) inecliptic coordinates, respectively.[14][15]

While not being aslow rotator,Achaia has a notably longer period than the vast majority of asteroids, which typically rotate every 2 to 20 hours once around their axis. Also, the body's changes in brightness are relatively high and indicate that it has a non-spheroidal shape.

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Achaia measures between 7.689 and 8.16 kilometers in diameter, and its surface has analbedo between 0.234 and 0.251.[8][10][11][12] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – taken from8 Flora, the Flora family's principal body and namesake – and calculates a diameter of 7.82 kilometers based on anabsolute magnitude of 12.7.[9]

Notes

[edit]
  1. ^abPravec (2007) web: rotation period60.99±0.05 hours with a brightness amplitude of0.72 mag. Quality code of 3. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (1150) Achaia andPravec, P.; Wolf, M.; Sarounova, L. (2007)
  2. ^(1150) Achaia:Lightcurve Plot analysis on 23 October 2007 by Pravec and Galad. ProjectID: Modra, Kharkiv. Comment: Error of 0.02 h is formal, real error perhaps a couple times greater.

References

[edit]
  1. ^abcde"1150 Achaia (1929 RB)".Minor Planet Center. Retrieved2 February 2017.
  2. ^"Achaia".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^"Achaia".Merriam-Webster.com Dictionary. Merriam-Webster.
  4. ^abcdeSchmadel, Lutz D. (2007). "(1150) Achaia".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 97.doi:10.1007/978-3-540-29925-7_1151.ISBN 978-3-540-00238-3.
  5. ^abcd"JPL Small-Body Database Browser: 1150 Achaia (1929 RB)" (2016-06-13 last obs.).Jet Propulsion Laboratory. Retrieved2 February 2017.
  6. ^ab"Asteroid 1150 Achaia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved14 March 2020.
  7. ^abcde"Asteroid 1150 Achaia".Small Bodies Data Ferret. Retrieved14 March 2020.
  8. ^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. Retrieved2 February 2017.
  9. ^abcde"LCDB Data for (1150) Achaia". Asteroid Lightcurve Database (LCDB). Retrieved2 February 2017.
  10. ^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.
  11. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  12. ^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. Retrieved2 February 2017.
  13. ^abcLazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (November 2004)."S3OS2: the visible spectroscopic survey of 820 asteroids"(PDF).Icarus.172 (1):179–220.Bibcode:2004Icar..172..179L.doi:10.1016/j.icarus.2004.06.006. Retrieved14 March 2020.
  14. ^Durech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573. Retrieved2 February 2017.
  15. ^Hanuš, J.; Ďurech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network".Astronomy and Astrophysics.586: A108.arXiv:1510.07422.Bibcode:2016A&A...586A.108H.doi:10.1051/0004-6361/201527441.ISSN 0004-6361.

External links

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