Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1244 Deira

From Wikipedia, the free encyclopedia
Main-belt asteroid

1244 Deira
Modelled shape ofDeira from itslightcurve
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date25 May 1932
Designations
(1244) Deira
Pronunciation/ˈdrə/DY-rə or/ˈdɛərə/DAIR[2]
Named after
Deira, near the town ofOssett, England[3]
(alt. CelticKingdom of Deira)
1932 KE · 1930 YR
1984 YQ6 · A908 TD
A921 GC · A924 BH
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc109.13 yr (39,861 days)
Aphelion2.5731AU
Perihelion2.1129 AU
2.3430 AU
Eccentricity0.0982
3.59yr (1,310 days)
335.23°
0° 16m 29.28s / day
Inclination8.6950°
277.12°
261.45°
Physical characteristics
28.816±0.546 km[7]
30.432±9.136 km[8]
30.95±1.9 km[9]
31.799±0.487 km[10]
32.28±0.35 km[11]
33.15±7.01 km[12]
35.19±0.19 km[13]
5(poor)h[14]
210.6±0.1 h[a]
216.98±0.05 h[15]
217.1±0.1 h[b]
  • (314.0°, −46.0°) (λ11)[6]
  • (107.0°, −56.0°) (λ22)[6]
0.03±0.00[13]
0.0357±0.0051[10]
0.037±0.011[12]
0.0416±0.0312[8]
0.052±0.001[11]
0.0557±0.007[9]
11.30[9][10][11]
11.50[1][17][8]

1244 Deira (prov. designation:1932 KE) is a darkbackground asteroid andslow rotator from the inner region of theasteroid belt. TheX-type asteroid has an exceptionally longrotation period of 210.6 hours and measures approximately 31 kilometers (19 miles) in diameter. It was discovered on 25 May 1932, by English-born South African astronomerCyril Jackson at theUnion Observatory in Johannesburg,[4] who named it afterDeira, an old kingdom near his birthplace, the market town ofOssett, located in West Yorkshire, England.[3]

Orbit and classification

[edit]

Deira is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[5][6] It orbits the Sun in theinner asteroid belt at a distance of 2.1–2.6 AU once every 3 years and 7 months (1,310 days;semi-major axis 2.34 AU). Its orbit has aneccentricity of 0.10 and aninclination of 9° with respect to theecliptic.[1] The body'sobservation arc begins with its first observations asA908 TD atHeidelberg Observatory in October 1908, or more than 23 years prior to its official discovery observation at Johannesburg.[4]

Naming

[edit]

Thisminor planet was named by the discovererCyril Jackson after his birthplace, the market town ofOssett, located in West Yorkshire, England(also see2193 Jackson).[3] The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 115).[3] While the naming citation reads thatDeira is the ancient name for his birthplace, the CelticKingdom of Deira was actually much larger, encompassing at its height most ofYorkshire in Northern England.

Physical characteristics

[edit]

Deira has been characterized as a primitiveP-type asteroid by the space-basedWide-field Infrared Survey Explorer (WISE).[10] While P-type bodies are common in the outermost asteroid belt and among theJupiter trojans, they are rarely found in the inner main belt. In both the Tholen- and SMASS-like taxonomy of theSmall Solar System Objects Spectroscopic Survey (S3OS2),Deira is anX-type asteroid.[6][16]

Rotation period

[edit]

In March 2011, a rotationallightcurve ofDeira was obtained from photometric observations byJulian Oey at his Leura Observatory (E17) in Australia. Lightcurve analysis gave arotation period of 210.6 hours with a brightness variation of 0.5magnitude (U=2),[a] while Oey previously published a slightly longer period of 217.1 hours and an amplitude of 0.6 magnitude (U=n.a.).[b] This makesDeira one of theTop 300 slow rotators known to exist.

Spin axis

[edit]

In 2016, an international study modeled a lightcurve with a concurring period of 216.98 hours and found twospin axis of (314.0°, −46.0°) and (107.0°, −56.0°) inecliptic coordinates (λ, β).[15]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Deira measures between 28.816 and 35.19 kilometers in diameter and its surface has analbedo between 0.03 and 0.0557.[7][8][9][10][11][12][13]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0465 and a diameter of 30.89 kilometers based on anabsolute magnitude of 11.5.[17]

Notes

[edit]
  1. ^abOey (2011) LCDB. (1244) Deira – rotation period210.6±0.1 hours with a brightness amplitude of0.50±0.03 mag. Quality code of 2. Summary figures at theLCDB.
  2. ^abOey (2007) website. (1244) Deira – rotation period217.1±0.1 hours with a brightness amplitude of0.60±0.05 mag. No quality code.Lightcurve-plot and summary figures at the archivedLeura Observatory website. Astronomers comment: "The data is re-reduced with Canopus 9.5 Comp Star Selector feature. Linkage over the 2.5 months period showing a main period of 217h. Slow rotator with deviation from the mean due to Psyn-sid and tumbling characteristics."

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 1244 Deira (1932 KE)" (2017-11-25 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 19 August 2020. Retrieved3 January 2018.
  2. ^A Complete Pronouncing Gazetteer, Or, Geographical Dictionary of the World, 1880
  3. ^abcdSchmadel, Lutz D. (2007). "(1244) Deira".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 103.doi:10.1007/978-3-540-29925-7_1245.ISBN 978-3-540-00238-3.
  4. ^abc"1244 Deira (1932 KE)".Minor Planet Center. Retrieved3 January 2018.
  5. ^ab"Asteroid 1244 Deira – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  6. ^abcde"Asteroid 1244 Deira".Small Bodies Data Ferret. Retrieved15 March 2020.
  7. ^abMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.S2CID 118745497. Retrieved3 January 2018.
  8. ^abcdMasiero, Joseph R.; Nugent, C.; Mainzer, A. K.; Wright, E. L.; Bauer, J. M.; Cutri, R. M.; et al. (October 2017)."NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos".The Astronomical Journal.154 (4): 10.arXiv:1708.09504.Bibcode:2017AJ....154..168M.doi:10.3847/1538-3881/aa89ec.
  9. ^abcdTedesco, 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.
  10. ^abcdefMainzer, 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.
  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. ^abcNugent, 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. Retrieved3 January 2018.
  13. ^abcNugent, 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.
  14. ^Behrend, Raoul."Asteroids and comets rotation curves – (1244) Deira". Geneva Observatory. Retrieved3 January 2018.
  15. ^abHanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network".Astronomy and Astrophysics.586: 24.arXiv:1510.07422.Bibcode:2016A&A...586A.108H.doi:10.1051/0004-6361/201527441.S2CID 119112278.
  16. ^abLazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (November 2004)."S3OS2: the visible spectroscopic survey of 820 asteroids"(PDF).Icarus.172 (1):179–220.Bibcode:2004Icar..172..179L.doi:10.1016/j.icarus.2004.06.006. Retrieved15 March 2020.
  17. ^ab"LCDB Data for (1244) Deira". Asteroid Lightcurve Database (LCDB). Retrieved3 January 2018.

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=1244_Deira&oldid=1270008175"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp