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1231 Auricula

From Wikipedia, the free encyclopedia
Carbonaceous background asteroid

1231 Auricula
Modelled shape ofAuricula from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date10 October 1931
Designations
(1231) Auricula
Pronunciation/ɔːˈrɪkjʊlə/[2]
Named after
Primula auricula[3]
(flowering plant)
1931 TE2
main-belt[1][4] · (middle)
background[5][6]
Orbital characteristics[4]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc87.02yr (31,785 d)
Aphelion2.8988AU
Perihelion2.4388 AU
2.6688 AU
Eccentricity0.0862
4.36 yr (1,593 d)
171.27°
0° 13m 33.96s / day
Inclination11.483°
342.04°
245.60°
Physical characteristics
13.43±4.67 km[7]
15.10±3.67 km[8]
18.71±0.65 km[9][10]
21.44±0.81 km[11]
22.52±1.8 km[12]
3.9816±0.0006 h[13]
0.066[9][10]
0.0798[12]
0.089[11]
0.11[8][7]
C(SDSS-MOC)[14]
11.60[11]
12.2[1][4][8][9][10]
12.29[7]

1231 Auricula (prov. designation:1931 TE2) is a carbonaceous backgroundasteroid from the central regions of theasteroid belt, approximately 20 kilometers (12 miles) in diameter. It was discovered on 10 October 1931, by German astronomerKarl Reinmuth at theHeidelberg Observatory.[1] The likely elongatedC-type asteroid has arotation period of 3.98 hours.[15] It was named after the flowering plantauricula and indirectly honors astronomerGustav Stracke.[3]

Orbit and classification

[edit]

Based on recentHCM-analyses,Auricula is a non-family asteroid that belongs to the main belt'sbackground population.[5][6] On its osculating Keplerianorbital elements, it is located in theEunomia region (502), where the prominent family ofstony asteroids is located.[15]

It orbits the Sun in thecentral main-belt at a distance of 2.4–2.9 AU once every 4 years and 4 months (1,593 days;semi-major axis of 2.67 AU). Its orbit has aneccentricity of 0.09 and aninclination of 11° with respect to theecliptic.[4] The body'sobservation arc begins with its official discovery observation atHeidelberg in October 1931.[1]

Naming

[edit]

Thisminor planet was named after the yellow flowered Alpine primrose,primula auricula. The officialnaming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 113).[3] It honors German astronomer and diligent orbit computerGustav Stracke (1887–1943), who had asked that no asteroid be named after him. The initials of the asteroids(1227) through (1234), all discovered byKarl Reinmuth, spell out "G. Stracke". In this manner, Reinmuth was able to circumvent Stracke's desire and honor him nevertheless. The asteroid1019 Strackea was later named after Stracke directly.[16] In the 1990s, astronomerBrian Marsden was also honored by this method, see asteroids5694 to5699. The consecutive initial letters of these minor-planet names spell out "MarsdenB".[17]

Reinmuth's flowers

[edit]

Due to his many discoveries,Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between(1009) and(1200). This list also contained a sequence of 28 asteroids, starting with1054 Forsytia, that were all named after plants, in particularflowering plants(also see list of minor planets named after animals and plants).[18]

Physical characteristics

[edit]

In theSDSS-based taxonomy,Auricula is a common, carbonaceousC-type asteroid.[5][14]

Rotation period and poles

[edit]

In April 2008, a rotationallightcurve ofAuricula was obtained fromphotometric observations by Colin Bembrick at the Mount Tarana Observatory (431) and other observers from Australia and New Zealand. Lightcurve analysis gave arotation period of3.9816±0.0006 hours with a brightness amplitude of 0.75magnitude (U=3), indicative of a non-spherical, elongated shape.[13] A modeled lightcurve using photometric data from the Lowell Photometric Database was published in 2016. It gave a concurring sidereal period of3.981580±0.000001 hours, as well as twospin axes at (57.0°, −57.0°) and (225.0°, −85.0°) inecliptic coordinates (λ, β).[19]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Auricula measures between 13.43 and 22.52 kilometers in diameter and its surface has analbedo between 0.066 and 0.11.[7][8][10][9][11][12] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0465 and a diameter of 22.37 kilometers based on anabsolute magnitude of 12.2.[15]

References

[edit]
  1. ^abcde"1231 Auricula (1931 TE2)".Minor Planet Center. Retrieved17 December 2018.
  2. ^"auricula".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcSchmadel, Lutz D. (2007). "(1231) Auricula".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 102.doi:10.1007/978-3-540-29925-7_1232.ISBN 978-3-540-00238-3.
  4. ^abcd"JPL Small-Body Database Browser: 1231 Auricula (1931 TE2)" (2018-10-18 last obs.).Jet Propulsion Laboratory. Retrieved17 December 2018.
  5. ^abc"Asteroid 1231 Auricula".Small Bodies Data Ferret. Retrieved17 December 2018.
  6. ^ab"Asteroid (1231) Auricula – Proper elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved14 December 2018.
  7. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  8. ^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.S2CID 9341381.
  9. ^abcdMainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016)."NEOWISE Diameters and Albedos V1.0".NASA Planetary Data System: EAR-A-COMPIL-5-NEOWISEDIAM-V1.0.Bibcode:2016PDSS..247.....M. Retrieved17 December 2018.
  10. ^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.S2CID 46350317.
  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. ^abcTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved17 December 2018.
  13. ^abBembrick, Colin; Crawford, Greg; Allen, Bill (October 2008)."The Rotation Period of 1231 Auricula".The Minor Planet Bulletin.35 (4):185–186.Bibcode:2008MPBu...35..185B.ISSN 1052-8091. Retrieved17 December 2018.
  14. ^abCarvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010)."SDSS-based taxonomic classification and orbital distribution of main belt asteroids".Astronomy and Astrophysics.510: 12.Bibcode:2010A&A...510A..43C.doi:10.1051/0004-6361/200913322. Retrieved30 October 2019.(PDS data set)
  15. ^abc"LCDB Data for (1231) Auricula". Asteroid Lightcurve Database (LCDB). Retrieved17 December 2018.
  16. ^Schmadel, Lutz D. (2007). "(1234) Elyna".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. pp. 102–103.doi:10.1007/978-3-540-29925-7_1235.ISBN 978-3-540-00238-3.
  17. ^Schmadel, Lutz D. (2007). "(5699) Munch".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 483.doi:10.1007/978-3-540-29925-7_5391.ISBN 978-3-540-00238-3.
  18. ^Schmadel, Lutz D. (2007). "(1054) Forsytia".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 90.doi:10.1007/978-3-540-29925-7_1055.ISBN 978-3-540-00238-3.
  19. ^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.S2CID 118427201. Retrieved17 December 2018.

External links

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