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1578 Kirkwood

From Wikipedia, the free encyclopedia
Asteroid in the Hilda group

1578 Kirkwood
Shape model ofKirkwood from itslightcurve
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date10 January 1951
Designations
(1578) Kirkwood
Named after
Daniel Kirkwood[2]
(American astronomer)
1951 AT · 1944 DF
1949 TF · 1952 FK
main-belt · (outer)[1]
Hilda[3][4][5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc73.37 yr (26,797 days)
Aphelion4.8617AU
Perihelion2.9855 AU
3.9236 AU
Eccentricity0.2391
7.77yr (2,839 days)
195.23°
0° 7m 36.48s / day
Inclination0.8085°
74.002°
1.7729°
Jupiter MOID0.4366 AU
Physical characteristics
Dimensions47.077±0.315 km[6]
51.88±1.8 km[4][7]
57.14±1.27 km[8]
12.518±0.002h[9]
17.9±0.1 h[a]
0.044±0.002[8]
0.0517±0.004[4][7]
0.063±0.005[6]
Tholen =D[1] · D[4][10]
B–V = 0.788[1]
U–B = 0.276[1]
10.26[1][4][7][8] · 10.41±0.50[10]

1578 Kirkwood, provisional designation1951 AT, is aHilda asteroid from the outermost regions of theasteroid belt, approximately 52 kilometers in diameter. It was discovered on 10 January 1951, by astronomers of theIndiana Asteroid Program atGoethe Link Observatory in Indiana, United States.[3] The asteroid was named after American astronomerDaniel Kirkwood.[2]

Orbit and classification

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Kirkwood belongs to the orbitalHilda group, which is locatedoutermost part of the main belt.[4] Asteroids in this dynamical group havesemi-major axis between 3.7 and 4.2 AU and stay in a 3:2resonance with the gas giantJupiter.Kirkwood, however, is a background asteroid and not a member of the (collisional)Hilda family (101).[5]

It orbits the Sun at a distance of 3.0–4.9 AU once every 7 years and 9 months (2,839 days). Its orbit has aneccentricity of 0.24 and aninclination of 1° with respect to theecliptic.[1]

The asteroid was first observed as1944 DF atTurku Observatory in February 1944. The body'sobservation arc begins with its observation as1949 TF atHeidelberg Observatory in October 1949, fifteen months prior to its official discovery observation at Goethe Link.[3]

Physical characteristics

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In theTholen classification,Kirkwood is a darkD-type asteroid.[1] It is also characterized as a D-type byPanSTARRS photometric survey.[10]

Rotation period

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In October 2012, a rotationallightcurve ofKirkwood was obtained from photometric observations at the Etscorn Campus Observatory (719) in New Mexico, United States. Lightcurve analysis gave arotation period of 12.518 hours with a brightness variation of 0.05magnitude (U=2). Another lightcurve gave a period of 17.9 hours and an amplitude of 0.22 magnitude (U=2).[a]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite, theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer and the Infrared Astronomical SatelliteIRAS,Kirkwood measures between 47.077 and 57.14 kilometers in diameter and its surface has analbedo between 0.044 and 0.063.[6][7][8]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0517 and a diameter of 51.88 kilometers based on anabsolute magnitude of 10.26.[4]

Naming

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Thisminor planet was named in memory of American astronomerDaniel Kirkwood (1814–1895), long-time professor of mathematics atIndiana University. He discovered theKirkwood gaps, which are gaps in the distribution of the mean distances of the minor planets in the asteroid belt.Kirkwood was theIndiana Asteroid Program's first numbered discovery.[2][b] The officialnaming citation was published by theMinor Planet Center in March 1952 (M.P.C. 738).[11] The lunar craterKirkwood was also named in the astronomer's honor.[2]

Notes

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  1. ^abSlyusarev (2012) web; for (1578) Kirkwood: rotation period of17.9 hours with a brightness amplitude of0.22 mag. Summary figures given at theLCDB
  2. ^Although the asteroid1575 Winifred, also discovered by the Indiana Asteroid Program, has both a lower number and an earlier discovery date (20 April 1950) than 1578 Kirkwood

References

[edit]
  1. ^abcdefghi"JPL Small-Body Database Browser: 1578 Kirkwood (1951 AT)" (2017-07-04 last obs.).Jet Propulsion Laboratory. Retrieved21 September 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1578) Kirkwood".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 125.doi:10.1007/978-3-540-29925-7_1579.ISBN 978-3-540-00238-3.
  3. ^abc"1578 Kirkwood (1951 AT)".Minor Planet Center. Retrieved21 September 2017.
  4. ^abcdefg"LCDB Data for (1578) Kirkwood". Asteroid Lightcurve Database (LCDB). Retrieved21 September 2017.
  5. ^ab"Asteroid 1578 Kirkwood – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  6. ^abcGrav, T.; Mainzer, A. K.; Bauer, J.; Masiero, J.; Spahr, T.; McMillan, R. S.; et al. (January 2012)."WISE/NEOWISE Observations of the Hilda Population: Preliminary Results".The Astrophysical Journal.744 (2): 15.arXiv:1110.0283.Bibcode:2012ApJ...744..197G.doi:10.1088/0004-637X/744/2/197.S2CID 44000310. Retrieved21 September 2017.
  7. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0.12.Bibcode:2004PDSS...12.....T. Retrieved17 October 2019.
  8. ^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)
  9. ^Klinglesmith, Daniel A. III; Hanowell, Jesse; Risley, Ethan; Turk, Janek; Vargas, Angelica; Warren, Curtis Alan (April 2013)."Asteroid Synodic Periods from Etscorn Campus Observatory".The Minor Planet Bulletin.40 (2):65–67.Bibcode:2013MPBu...40...65K.ISSN 1052-8091. Retrieved21 September 2017.
  10. ^abcVeres, 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. Retrieved21 September 2017.
  11. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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