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1336 Zeelandia

From Wikipedia, the free encyclopedia
Stony Koronian asteroid

1336 Zeelandia
Shape model ofZeelandia from itslightcurve
Discovery[1]
Discovered byH. van Gent
Discovery siteJohannesburg Obs.
Discovery date9 September 1934
Designations
(1336) Zeelandia
Named after
Zeeland[2]
(a province of theNetherlands)
1934 RW · 1929 QE
1930 XC · 1935 YF
1939 RP · A906 YO
main-belt · (outer)
Koronis[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc112.01 yr (40,913 days)
Aphelion3.0348AU
Perihelion2.6654 AU
2.8501 AU
Eccentricity0.0648
4.81yr (1,757 days)
117.20°
0° 12m 17.28s / day
Inclination3.1972°
97.420°
220.01°
Physical characteristics
Dimensions19.18±0.51 km[5]
20.99±2.1 km[3][6]
21.441±0.132 km[7]
23.056±0.108 km[8]
23.63±3.31 km[9]
15.602h[10]
15.624±0.001 h[11]
0.153±0.280[9]
0.1829±0.0228[8]
0.2183±0.052[3][6]
0.232±0.045[7]
0.273±0.017[5]
B–V = 0.810[1]
U–B = 0.366[1]
Tholen =S[1]
SMASS =S[1][3]
10.66[1][3][5][6][8] · 10.71±0.58[12] · 10.79[9] · 10.94±0.02[10]

1336 Zeelandia, provisional designation1934 RW, is a stony Koronianasteroid from the outer regions of theasteroid belt, approximately 21 kilometers in diameter. It was discovered on 9 September 1934, by Dutch astronomerHendrik van Gent at theUnion Observatory in Johannesburg, South Africa.[13] The asteroid was named for the Dutch province ofZeeland.[2]

Orbit and classification

[edit]

Zeelandia belongs to theKoronis family (605),[3][4] a very largeasteroid family of 6,000 known members with stony composition and nearly co-planarecliptical orbits.[14]

It orbits the Sun in theouter main-belt at a distance of 2.7–3.0 AU once every 4 years and 10 months (1,757 days;semi-major axis of 2.85 AU). Its orbit has aneccentricity of 0.06 and aninclination of 3° with respect to the ecliptic.[1] In October 1905, a firstprecovery was taken at theLowell Observatory in Arizona. Its first identification asA906 YO was made at Taunton Observatory (803) in December 1906. The body'sobservation arc begins with its official discovery observation at Johannesburg in September 1934.[13]

Physical characteristics

[edit]

Zeelandia has been characterized as a stonyS-type asteroid in both theTholen andSMASS classification.[1]

Rotation period

[edit]

In March 2004, a rotationallightcurve ofZeelandia was obtained from photometric observations by a collaboration of American astronomers. Lightcurve analysis gave a well-definedrotation period of 15.602 hours with a brightness variation of 0.61magnitude (U=3).[10] The result was confirmed by photometristsPierre Antonini, Federico Manzini, Julian Oey and Frederick Pilcher, as well as Hiromi and Hiroko Hamanowa, who measured a similar period of 15.624 with an amplitude of 0.50 magnitude in April 2005 (U=3).[11]

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,Zeelandia measures between 19.18 and 23.63 kilometers in diameter and its surface has analbedo between 0.153 and 0.273.[5][6][7][8][9]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.2183 and a diameter of 20.99 kilometers based on anabsolute magnitude of 10.66.[3][6]

Naming

[edit]

Thisminor planet was named for the Dutch province ofZeeland. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 121).[2]

References

[edit]
  1. ^abcdefghi"JPL Small-Body Database Browser: 1336 Zeelandia (1934 RW)" (2017-10-31 last obs.).Jet Propulsion Laboratory. Retrieved28 November 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1336) Zeelandia".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 109.doi:10.1007/978-3-540-29925-7_1337.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1336) Zeelandia". Asteroid Lightcurve Database (LCDB). Retrieved28 November 2017.
  4. ^ab"Asteroid 1336 Zeelandia – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^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)
  6. ^abcdeTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  7. ^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.
  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.
  9. ^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. Retrieved28 November 2017.
  10. ^abcSlivan, Stephen M.; Binzel, Richard P.; Boroumand, Shaida C.; Pan, Margaret W.; Simpson, Christine M.; Tanabe, James T.; et al. (May 2008)."Rotation rates in the Koronis family, complete to H≈11.2".Icarus.195 (1):226–276.Bibcode:2008Icar..195..226S.doi:10.1016/j.icarus.2007.11.019. Retrieved28 November 2017.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1336) Zeelandia". Geneva Observatory. Retrieved28 November 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. Retrieved28 November 2017.
  13. ^ab"1336 Zeelandia (1934 RW)".Minor Planet Center. Retrieved28 November 2017.
  14. ^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
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