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1216 Askania

From Wikipedia, the free encyclopedia
Main-belt asteroid

1216 (One afterMagna Carta) Askania
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date29 January 1932
Designations
(1216) Askania
Named after
Askania Werke
(German manufacturer)[2]
1932 BL · 1952 DH
1984 YY6 · A909 GF
main-belt · (inner)
Flora[3][4] · background[5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc110.32 yr (40,295 days)
Aphelion2.6325AU
Perihelion1.8328 AU
2.2327 AU
Eccentricity0.1791
3.34yr (1,219 days)
134.38°
0° 17m 43.44s / day
Inclination7.5997°
121.60°
144.64°
Physical characteristics
7.21±0.38 km[6]
9.62±2.53 km[7]
10.08±0.54 km[8]
10.533±0.089 km[6]
6.536±0.003 h[9]
0.064±0.009[6]
0.070±0.008[8]
0.136±0.014[6]
0.15±0.09[7]
0.24(assumed)[3]
Tholen =S[1] · S[3]
B–V = 0.903[1]
13.49[1][3][6][7][8]

1216 Askania, provisional designation1932 BL, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 9 kilometers in diameter. It was discovered on 29 January 1932, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany.[10] It was named after the companyAskania Werke, a German manufacturer of precision instruments.[2]

Orbit and classification

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Askania orbits the Sun in theinner main-belt at a distance of 1.8–2.6 AU once every 3 years and 4 months (1,219 days). Its orbit has aneccentricity of 0.18 and aninclination of 8° with respect to theecliptic.[1] The asteroid is a member of theFlora family, one of the largestfamilies in the asteroid belt.[4][a] Conversely, it is considered abackground asteroid when applying thehierarchical clustering method to it proper orbital elements.[5]

The body'sobservation arc begins with its official discovery observation at Heidelberg in 1932. In July 1906, a firstprecovery was taken at theLowell Observatory, and in April 1909, the asteroid was first identified at the discovering observatory asA909 GF.[10]

Naming

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Theminor planet was named after "Askania Werke AG", a manufacturer of optical and astronomical instruments in Berlin(also seeCinetheodolite).[1] The company went on to develop theauto pilot of the V-1 bomb in the following years.[11] The official naming citation was published byPaul Herget inThe Names of the Minor Planets in 1955 (H 112).[2]

Physical characteristics

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In theTholen classification,Askania is a common stonyS-type asteroid.[1]

Lightcurves

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Lightcurve observations ofAskania at the Menke Observatory in July 2006, show a well-definedperiodicity of6.536 hours, during which time the brightness of the body varies by0.30magnitude (U=3-).[9]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite, and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Askania measures between 7.21 and 10.533 kilometers in diameter and its surface has analbedo between 0.064 and 0.15.[6][7][8]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, an stony asteroid and largest member and namesake of the Flora family – and calculates a diameter of 5.44 kilometers with anabsolute magnitude of 13.49.[3][a]

Notes

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  1. ^abThe Collaborative Asteroid Lightcurve Link groups any asteroid into the Flora family that has asemi-major axis, inclination and eccentricity in the following ranges: 2.15 < a < 2.35; 0.03 < e < 0.23: 1.5 < i < 8. However, modern synthetic clustering models exclude (1216) Askania from the Flora family, seeAstDyS-2 andNesvorny HCM Asteroid Families V3.0.

References

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  1. ^abcdefgh"JPL Small-Body Database Browser: 1216 Askania (1932 BL)" (2016-11-23 last obs.).Jet Propulsion Laboratory. Retrieved24 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1216) Askania".Dictionary of Minor Planet Names – (1216) Askania.Springer Berlin Heidelberg. p. 101.doi:10.1007/978-3-540-29925-7_1217.ISBN 978-3-540-00238-3.
  3. ^abcde"LCDB Data for (1216) Askania". Asteroid Lightcurve Database (LCDB). Retrieved24 July 2017.
  4. ^abAlfvén, H. (May 1969)."Asteroidal Jet Streams".Astrophysics and Space Science.4 (1): 84–102(Ap&SSHomepage).Bibcode:1969Ap&SS...4...84A.doi:10.1007/BF00651264. Retrieved24 July 2017.
  5. ^ab"Asteroid 1216 Askania – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved28 October 2019.
  6. ^abcdefMasiero, 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. Retrieved24 July 2017.
  7. ^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. Retrieved24 July 2017.
  8. ^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)
  9. ^abMenke, John; Cooney, Walt; Gross, John; Terrell, Dirk; Higgins, David (October 2008)."Asteroid Lightcurve Analysis at Menke Observatory".The Minor Planet Bulletin.35 (4):155–160.Bibcode:2008MPBu...35..155M.ISSN 1052-8091. Retrieved24 July 2017.
  10. ^ab"1216 Askania (1932 BL)".Minor Planet Center. Retrieved24 July 2017.
  11. ^Zaloga, Steven (2005).V-1 Flying Bomb 1942–52. Oxford, UK:Osprey Publishing. p. 6.ISBN 978-1-84176-791-8.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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