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1156 Kira

From Wikipedia, the free encyclopedia
Stony background asteroid

1156 Kira
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date22 February 1928
Designations
(1156) Kira
Named after
unknown[2]
1928 DA · 1935 FY
1938 DA · 1953 RC1
1955 FW1 · 1973 QC2
main-belt · (inner)[3]
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc88.76 yr (32,418 days)
Aphelion2.3414AU
Perihelion2.1329 AU
2.2372 AU
Eccentricity0.0466
3.35yr (1,222 days)
326.67°
0° 17m 40.2s / day
Inclination1.3976°
91.131°
353.76°
Physical characteristics
Dimensions6.83±0.21 km[5]
6.831±0.211 km[5]
8.79±1.97 km[6]
8.856±0.105 km[7]
9.00±2.24 km[8]
10.30 km(calculated)[3]
10.83±0.76 km[9]
2.7910±0.0005h[a]
2.79103±0.00004 h[10]
2.79105±0.00003 h[10]
2.79113±0.00004 h[10]
0.165±0.024[9]
0.181±0.052[11]
0.20(assumed)[3]
0.2490±0.0585[7]
0.26±0.14[6]
0.29±0.12[8]
0.455±0.066[5]
S[3]
12.30[1][3][5][8] · 12.40[7][9] · 12.48±0.35[12] · 12.72[6]

1156 Kira, provisional designation1928 DA, is a stony backgroundasteroid from the inner regions of theasteroid belt, approximately 9 kilometers in diameter. It was discovered on 22 February 1928, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany.[13] Any reference of its name to a person or occurrence is unknown.[2]

Orbit and classification

[edit]

Kira is not a member of any knownasteroid family and belongs to the main belt'sbackground population.[4] At the present epoch, however, it orbits within the region of theFlora family.[10]

This asteroid orbits the Sun in theinner main-belt at a distance of 2.1–2.3 AU once every 3 years and 4 months (1,222 days). Its orbit has aneccentricity of 0.05 and aninclination of 1° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Heidelberg.[13]

Physical characteristics

[edit]

Kira is an assumed stonyS-type asteroid.[3]

Rotation period

[edit]

Several rotationallightcurves ofKira have been obtained from photometric observations since 2007. Lightcurve analysis gave arotation period between 2.7910 and 2.79113 hours with a brightness variation of 0.20 to 0.26magnitude (U=3/3/3/2+).[10][a]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Kira measures between 6.83 and 10.83 kilometers in diameter and its surface has analbedo between 0.165 and 0.455.[5][6][7][8][9][11]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 10.30 kilometers based on anabsolute magnitude of 12.3.[3]

Naming

[edit]

Thisminor planet was named by astronomerMax Mündler, staff member at Heidelberg Observatory. Any reference of its name to a person or occurrence is unknown.[2]

Unknown meaning

[edit]

Among the many thousands ofnamed minor planets,Kira is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between164 Eva and1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomersAuguste Charlois,Johann Palisa,Max Wolf andKarl Reinmuth.[14]

Notes

[edit]
  1. ^abPravec (2012),lightcurve plot of (1156) Kira. Observation: 10 April 2012. Rotation period2.7910±0.0005 hours with a brightness amplitude of0.20±0.02 mag. Quality Code of 3.summary figures atOndrejov Asteroid Photometry Project. Note: figure published at theLCDB contains a typo.

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1156 Kira (1928 DA)" (2016-11-24 last obs.).Jet Propulsion Laboratory. Retrieved7 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1156) Kira".Dictionary of Minor Planet Names – (1156) Kira.Springer Berlin Heidelberg. pp. 97–98.doi:10.1007/978-3-540-29925-7_1157.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1156) Kira". Asteroid Lightcurve Database (LCDB). Retrieved7 September 2017.
  4. ^ab"Asteroid 1156 Kira – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved28 October 2019.
  5. ^abcdeMasiero, 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. Retrieved7 September 2017.
  6. ^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.
  7. ^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.
  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. Retrieved7 September 2017.
  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. ^abcdeDykhuis, Melissa J.; Molnar, Lawrence A.; Gates, Christopher J.; Gonzales, Joshua A.; Huffman, Jared J.; Maat, Aaron R.; et al. (March 2016)."Efficient spin sense determination of Flora-region asteroids via the epoch method".Icarus.267:174–203.Bibcode:2016Icar..267..174D.doi:10.1016/j.icarus.2015.12.021. Retrieved7 September 2017.
  11. ^abMasiero, 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. Retrieved7 September 2017.
  12. ^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. Retrieved7 September 2017.
  13. ^ab"1156 Kira (1928 DA)".Minor Planet Center. Retrieved7 September 2017.
  14. ^Schmadel, Lutz D. (2007). "Appendix 11 – Minor Planet Names with Unknown Meaning".Dictionary of Minor Planet Names – Fifth Revised and Enlarged revision. Springer Berlin Heidelberg. pp. 927–929.ISBN 978-3-540-00238-3.

External links

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