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1091 Spiraea

From Wikipedia, the free encyclopedia
Carbonaceous main-belt asteroid

1091 Spiraea
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date26 February 1928
Designations
(1091) Spiraea
Pronunciation/spˈrə/[2]
Named after
Spiraea
(genus ofshrubs)[3]
1928 DT · 1934 CN1
1938 UR · 1964 XH
main-belt · (outer)[1][4]
Cybele · background[5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc89.27 yr (32,606 days)
Aphelion3.6484AU
Perihelion3.2077 AU
3.4281 AU
Eccentricity0.0643
6.35yr (2,318 days)
110.37°
0° 9m 19.08s / day
Inclination1.1554°
80.790°
12.062°
Physical characteristics
Dimensions32.78 km(calculated)[4]
35.178±0.108 km[6]
39.92±17.85 km[7]
40.280±0.455 km[8]
40.52±0.91 km[9]
7.01±0.43h[10]
0.05±0.06[7]
0.057(assumed)[4]
0.0627±0.0106[8]
0.063±0.003[9]
0.091±0.025[6]
C(assumed)[4]
10.60[8][9] · 10.70±0.08(R)[10] · 10.8[1] · 11.00±0.14[11] · 11.15[4] · 11.18[7]

1091 Spiraea, provisional designation1928 DT, is a carbonaceous Cybeleasteroid from the outer regions of theasteroid belt, approximately 36 kilometers in diameter. It was discovered on 26 February 1928, by astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in southwest Germany.[12] The asteroid was named afterSpiraea, a genus of plants.[3]

Orbit and classification

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Spiraea orbits the Sun in theouter main-belt at a distance of 3.2–3.6 AU once every 6 years and 4 months (2,318 days). Its orbit has aneccentricity of 0.06 and aninclination of 1° with respect to theecliptic.[1] With these orbital parameters, it belongs to theCybele asteroids, a dynamical group near the 4:7resonance with Jupiter and named after one of the largest asteroids,65 Cybele. It is, however, a non-family asteroid from the main belt'sbackground population when applying thehierarchical clustering method (Nesvorny, Novakovic, Knezevic and Milani) to its proper orbital elements.[5]

The body'sobservation arc begins with its identification as1934 CN1 atUccle Observatory in February 1934, almost six years after its official discovery observation at Heidelberg.[12]

Physical characteristics

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Spiraea is an assumed carbonaceousC-type asteroid.[4]

Rotation period

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In December 2014, a fragmentary rotationallightcurve ofSpiraea was obtained from photometric observations in the R-band by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 7.01 hours with a brightness amplitude of 0.03magnitude (U=1+).[10]

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,Spiraea measures between 35.178 and 40.52 kilometers in diameter and its surface has analbedo between 0.05 and 0.091.[6][7][8][9]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 32.78 kilometers based on anabsolute magnitude of 11.15.[4]

Naming

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Thisminor planet was named afterSpiraea, a genus ofshrubs of the rose family (Rosaceae), with small white or pink flowers. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 103).[3]

Reinmuth's flowers

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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).[13]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 1091 Spiraea (1928 DT)" (2017-06-04 last obs.).Jet Propulsion Laboratory. Retrieved26 September 2017.
  2. ^"spiræa".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcSchmadel, Lutz D. (2007). "(1091) Spiraea".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 93.doi:10.1007/978-3-540-29925-7_1092.ISBN 978-3-540-00238-3.
  4. ^abcdefg"LCDB Data for (1091) Spiraea". Asteroid Lightcurve Database (LCDB). Retrieved26 September 2017.
  5. ^ab"Asteroid 1091 Spiraea – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved28 October 2019.
  6. ^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.S2CID 119293330. Retrieved26 September 2017.
  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. ^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.S2CID 35447010.
  9. ^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)
  10. ^abcChang, Chan-Kao; Lin, Hsing-Wen;Ip, Wing-Huen; Prince, Thomas A.; Kulkarni, Shrinivas R.; Levitan, David; et al. (December 2016)."Large Super-fast Rotator Hunting Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series.227 (2): 13.arXiv:1608.07910.Bibcode:2016ApJS..227...20C.doi:10.3847/0067-0049/227/2/20.S2CID 30387146.
  11. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.S2CID 53493339. Retrieved26 September 2017.
  12. ^ab"1091 Spiraea (1928 DT)".Minor Planet Center. Retrieved26 September 2017.
  13. ^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.

External links

[edit]
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