Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1419 Danzig

From Wikipedia, the free encyclopedia
Flora asteroid

1419 Danzig
Modelled shape ofDanzig from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date5 September 1929
Designations
(1419) Danzig
Named after
German name of the
Polish city ofGdańsk[2]
1929 RF · 1936 RD
1952 HJ4 · 1957 WO1
A917 GA
Orbital characteristics[3]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc99.90 yr (36,489 days)
Aphelion2.6285AU
Perihelion1.9570 AU
2.2927 AU
Eccentricity0.1465
3.47yr (1,268 days)
356.63°
0° 17m 2.04s / day
Inclination5.7254°
213.53°
232.65°
Physical characteristics
14.059±0.096 km[7]
14.139 km[8]
14.997±0.382 km[9]
15.09±0.22 km[10]
(22.0°, 76.0°) (λ11)[13]
0.2324[14][8]
0.2388±0.0462[7]
0.250±0.009[10]
0.260±0.023[9]
S(family-based)[14]
11.20[9] · 11.3[3][10] · 11.45±0.14[14][8][11] · 11.45[7] · 11.55±1.00[15]

1419 Danzig (prov. designation:1929 RF) is a highly elongatedFlora asteroid from the inner regions of theasteroid belt. It was discovered on 5 September 1929, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany.[1] The stonyS-type asteroid has arotation period of 8.1 hours and measures approximately 14 kilometers (8.7 miles) in diameter. It was named for the city ofGdańsk (German:Danzig).[2]

Classification and orbit

[edit]

When applying the synthetichierarchical clustering method (HCM) byNesvorný,[4]Danzig is a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main-belt.[16]: 23  However, according to the 1995 HCM-analysis byZappalà,[6] and HCM-analysis byMilani andKnežević (AstDys), it is abackground asteroid. The latter HCM-analysis does not recognize the Floraasteroid clan.[5]

Danzig orbits the Sun at a distance of 2.0–2.6 AU once every 3 years and 6 months (1,268 days). Its orbit has aneccentricity of 0.15 and aninclination of 6° with respect to theecliptic.[3] In 1917, it was first observed asA917 GA atSimeiz Observatory (and Heidelberg on the following night), extending the body'sobservation arc by 12 years prior to its official discovery observation at Heidelberg.[1]

Naming

[edit]

Thisminor planet was named after the now Polish city and port on the Baltic sea,Gdańsk (German:Danzig). The city was also honored by another minor planet,764 Gedania.[2] Naming citation was first mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 128)[2]

Physical characteristics

[edit]

The overallspectral type for Florian asteroid is that of a stonyS-type.[16]: 23 

Rotation period and pole

[edit]
Lightcurve-based 3D-model ofDanzig

In November 1988, Polish astronomerWiesław Wiśniewski obtained a rotationallightcurve ofDanzig from photometric observations. It gave a well-definedrotation period of8.0±0.1 hours with a brightness variation of 0.92magnitude (U=3).[11] In October 2002, another lightcurve obtained by Italian and French amateur astronomersSilvano Casulli andLaurent Bernasconi gave a concurring period of8.1202±0.0001 hours and an amplitude of 0.81 magnitude (U=3).[12] WhileDanzig has an average rotation period, it has a high brightness variation, which indicates that the body has a non-spheroidal shape. In 2011, a modeled lightcurve using data from the Uppsala Asteroid Photometric Catalogue (UAPC) and other sources gave a period8.11957±0.00005 hours, as well as aspin axis of (22.0°, 76.0°) inecliptic coordinates (λ, β) (U=n.a.).[13]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Danzig measures 14.059 and 15.09 kilometers in diameter and its surface has analbedo between 0.238 and 0.260.[7][9][10] TheCollaborative Asteroid Lightcurve Link adoptsPetr Pravec's revised WISE-data, that is, an albedo of 0.2324 and a diameter of 14.139 kilometers with anabsolute magnitude of 11.45.[14][8]

References

[edit]
  1. ^abcd"1419 Danzig (1929 RF)".Minor Planet Center. Retrieved5 April 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1419) Danzig".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 114.doi:10.1007/978-3-540-29925-7_1420.ISBN 978-3-540-00238-3.
  3. ^abcd"JPL Small-Body Database Browser: 1419 Danzig (1929 RF)" (2017-03-08 last obs.).Jet Propulsion Laboratory. Retrieved5 April 2017.
  4. ^ab"Asteroid 1419 Danzig – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved16 March 2020.
  5. ^ab"Asteroid 1419 Danzig – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved16 March 2020.
  6. ^abZappalà, V.; Bendjoya, Ph.; Cellino, A.; Farinella, P.; Froeschle, C. (1997)."Asteroid Dynamical Families".NASA Planetary Data System: EAR-A-5-DDR-FAMILY-V4.1. Retrieved16 March 2020. (PDS main page)
  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.
  8. ^abcdPravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026.
  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.
  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. ^abcWisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995). "Photoelectric Observations of 125 Asteroids".Abstracts of the Lunar and Planetary Science Conference.26: 1511.Bibcode:1995LPI....26.1511W.
  12. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1419) Danzig".Geneva Observatory. Retrieved5 April 2017.
  13. ^abHanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011). "A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method".Astronomy & Astrophysics.530: 16.arXiv:1104.4114.Bibcode:2011A&A...530A.134H.doi:10.1051/0004-6361/201116738.
  14. ^abcd"LCDB Data for (1419) Danzig". Asteroid Lightcurve Database (LCDB). Retrieved5 April 2017.
  15. ^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.
  16. ^abNesvorný, 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=1419_Danzig&oldid=1316710787"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp