Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1056 Azalea

From Wikipedia, the free encyclopedia
Florian asteroid

1056 Azalea
Light curve-based 3D-model of 1056 Azalea
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date31 January 1924
Designations
(1056) Azalea
Pronunciation/əˈzliə/ə-ZAY-lee-ə[2]
Named after
Azalea(flower)[3]
1924 QD · 1925 NA
1929 WX
main-belt · (inner)
Flora[4][5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc93.24 yr (34,057 days)
Aphelion2.6277AU
Perihelion1.8321 AU
2.2299 AU
Eccentricity0.1784
3.33yr (1,216 days)
226.32°
0° 17m 45.6s / day
Inclination5.4267°
104.17°
212.39°
Physical characteristics
Dimensions10.66±1.99 km[6]
11.76±0.54 km[7]
11.869±0.136 km[8]
12.40 km(calculated)[4]
12.984±0.069 km[9]
13.07±0.64 km[10]
15.0276h[11]
15.03±0.05 h[12]
15.15±0.03 h[13]
0.223±0.024[10]
0.24(assumed)[4]
0.2457±0.0401[9]
0.292±0.040[7]
0.34±0.16[6]
SMASS =S[1] · S[4]
11.60[7][9] · 11.70[1][4][10] · 11.73±0.28[14] · 11.83[6]

1056 Azalea, provisional designation1924 QD, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 12 kilometers in diameter. It was discovered on 31 January 1924, by astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in southwest Germany.[15] The asteroid is named after theAzalea flower.[3]

Orbit and classification

[edit]

Azalea is a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main belt.[4][5][16]: 23  It orbits the Sun in theinner main belt at a distance of 1.8–2.6 AU once every 3 years and 4 months (1,216 days). Its orbit has aneccentricity of 0.18 and aninclination of 5° with respect to theecliptic.[1] The body'sobservation arc begins at Heidelberg in April 1928, more than 4 years after its official discovery observation.[15]

Physical characteristics

[edit]

In theSMASS classification,Azalea is a common stonyS-type asteroid.[1]

Rotation period

[edit]

In 2004, two rotationallightcurves ofAzalea were obtained from photometric observations by a group of predominately Polish astronomers including Agnieszka Kryszczyńska, as well as by astronomersAlain Klotz andRaoul Behrend. Lightcurve analysis gave arotation period of 15.03 and 15.15 hours with a high brightness variation of 0.70 and 0.79magnitude, respectively (U=2/2).[12][13] The high brightness amplitude is typically indicative for a non-spheroidal shape.

Spin axis

[edit]

In 2013, an international study modeled a lightcurve with a concurring period of 15.0276 hours and found twospin axis of (252.0°, 51.0°) and (64.0°, 41.0°) inecliptic coordinates (λ, β) (U=n.a.).[11]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Azalea measures between 10.66 and 13.07 kilometers in diameter and its surface has analbedo between 0.223 and 0.34.[6][7][8][9][10]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of the Flora family – and calculates a diameter of 12.40 kilometers based on anabsolute magnitude of 11.7.[4]

Naming

[edit]

Thisminor planet was named after the genus of flowering shrubs,Azalea, which arerhododendrons with funnel-shaped corollas.[3] The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 100).[3]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1056 Azalea (1924 QD)" (2017-04-30 last obs.).Jet Propulsion Laboratory. Retrieved30 August 2017.
  2. ^"azalea".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcdSchmadel, Lutz D. (2007). "(1056) Azalea".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 90.doi:10.1007/978-3-540-29925-7_1057.ISBN 978-3-540-00238-3.
  4. ^abcdefg"LCDB Data for (1056) Azalea". Asteroid Lightcurve Database (LCDB). Retrieved30 August 2017.
  5. ^ab"Asteroid 1056 Azalea – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved30 October 2019.
  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. ^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. Retrieved30 August 2017.
  8. ^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. Retrieved30 August 2017.
  9. ^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.
  10. ^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)
  11. ^abHanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; Durkee, R.; et al. (November 2013)."An anisotropic distribution of spin vectors in asteroid families".Astronomy and Astrophysics.559: 19.arXiv:1309.4296.Bibcode:2013A&A...559A.134H.doi:10.1051/0004-6361/201321993. Retrieved30 August 2017.
  12. ^abKryszczynska, A.; Colas, F.; Polinska, M.; Hirsch, R.; Ivanova, V.; Apostolovska, G.; et al. (October 2012)."Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region".Astronomy and Astrophysics.546: 51.Bibcode:2012A&A...546A..72K.doi:10.1051/0004-6361/201219199.
  13. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1056) Azalea".Geneva Observatory. Retrieved30 August 2017.
  14. ^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. Retrieved30 August 2017.
  15. ^ab"1056 Azalea (1924 QD)".Minor Planet Center. Retrieved30 August 2017.
  16. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=1056_Azalea&oldid=1244734629"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp