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1038 Tuckia

From Wikipedia, the free encyclopedia
Main-belt asteroid

1038 Tuckia
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date24 November 1924
Designations
(1038) Tuckia
Named after
Edward Tuck
(American philanthropist)[2]
1924 TK · 1932 VA
main-belt · (outer)[1]
Hilda[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc92.34 yr (33,728 days)
Aphelion4.8595AU
Perihelion3.1044 AU
3.9820 AU
Eccentricity0.2204
7.95yr (2,902 days)
340.94°
0° 7m 26.4s / day
Inclination9.1840°
57.769°
305.02°
Jupiter MOID0.7613 AU
Physical characteristics
Dimensions52.69±2.41 km[5]
58.3 km(DASTCOM)[1]
58.36 km(derived)[4]
23.2h[6]
0.0244±0.006[1]
0.030±0.003[5]
0.0304(derived)[4]
Tholen = DTU:[1] · DTU:[4]
B–V = 0.768[1]
U–B = 0.232[1]
10.58[4][6] · 10.60±0.45[7] · 10.82[1][5]

1038 Tuckia, provisional designation1924 TK, is rare-typeHilda asteroid from the outermost regions of theasteroid belt, approximately 58 kilometers in diameter. It was discovered on 24 November 1924, by German astronomer byMax Wolf atHeidelberg Observatory in southwest Germany.[3] The asteroid was named after American bankerEdward Tuck and his wife.[2]

Classification and orbit

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Tuckia is a member of theHilda family (001), anasteroid family within the dynamicalHilda group, an orbital group of asteroids in theoutermost main-belt, that stay in a 3:2orbital resonance with the gas giantJupiter. This means that the asteroid makes 3 orbits for every 2 orbits Jupiter makes.[3]

It orbits the Sun at a distance of 3.1–4.9 AU once every 7 years and 11 months (2,902 days). Its orbit has aneccentricity of 0.22 and aninclination of 9° with respect to theecliptic.[1] The asteroids'sobservation arc begins with its official discovery observation at Heidelberg.[3]

Physical characteristics

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In theTholen classification,Tuckia is a rare DTU:-type, a subtype of the darkD-type asteroids.[1]

Lightcurves

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In the 1990s, a rotationallightcurve ofTuckia was obtained from photometric observations by Swedish astronomer Dahlgren and colleges during a survey of Hildian asteroids. Lightcurve analysis gave a somewhat longer than averagerotation period of 23.2 hours with a brightness amplitude of 0.1magnitude (U=2).[6]

Diameter and albedo

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According to the survey carried out by the JapaneseAkari satellite,Tuckia measures 52.69 kilometers in diameter and its surface has analbedo of 0.030,[5] while the Collaborative Asteroid Lightcurve Link derives an albedo of 0.0304 and a diameter of 58.36 kilometers based on anabsolute magnitude of 10.82.[4]

Naming

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Thisminor planet was named after American banker and philanthropistEdward Tuck (1842–1938) and his wife. He is the son ofAmos Tuck who was a founder of the Republican Party in the United States. The name was suggested by G. Camille Flammarion. The official naming citation was published byPaul Herget inThe Names of the Minor Planets in 1955 (H 99).[2]

References

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  1. ^abcdefghijk"JPL Small-Body Database Browser: 1038 Tuckia (1924 TK)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved6 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1038) Tuckia".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 89.doi:10.1007/978-3-540-29925-7_1039.ISBN 978-3-540-00238-3.
  3. ^abcd"1038 Tuckia (1924 TK)".Minor Planet Center. Retrieved6 July 2017.
  4. ^abcdef"LCDB Data for (1038) Tuckia". Asteroid Lightcurve Database (LCDB). Retrieved6 July 2017.
  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. ^abcDahlgren, M.; Lahulla, J. F.; Lagerkvist, C.-I.; Lagerros, J.; Mottola, S.; Erikson, A.; et al. (June 1998)."A Study of Hilda Asteroids. V. Lightcurves of 47 Hilda Asteroids".Icarus.133 (2):247–285.Bibcode:1998Icar..133..247D.doi:10.1006/icar.1998.5919. Retrieved6 July 2017.
  7. ^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.

External links

[edit]
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