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1384 Kniertje

From Wikipedia, the free encyclopedia
Dark Adeonian asteroid

1384 Kniertje
Discovery[1]
Discovered byH. van Gent
Discovery siteJohannesburg Obs.
Discovery date9 September 1934
Designations
(1384) Kniertje
Named after
Kniertje[2](fictional character)
1934 RX
main-belt · (middle)
Eunomia[3] · Adeona[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc83.06 yr (30,338 days)
Aphelion3.1649AU
Perihelion2.1872 AU
2.6760 AU
Eccentricity0.1827
4.38yr (1,599 days)
288.15°
0° 13m 30.36s / day
Inclination11.858°
152.86°
276.17°
Physical characteristics
Dimensions21.52±6.01 km[5]
21.72±6.93 km[6]
26.14±0.56 km[7]
26.29±0.38 km[8]
26.517±0.090 km[9]
26.59 km(derived)[3]
27.51±1.6 km[10]
29.592±0.230 km[11]
9.78±0.02h[12]
9.807±0.002 h[12]
9.808±0.001 h[12]
9.824±0.001 h[13]
9.872±0.012 h[14]
12.255±0.004 h[15][a]
0.0351±0.0035[11]
0.06±0.03[6]
0.064±0.006[8]
0.066±0.003[7]
0.07±0.05[5]
0.0701(derived)[3]
0.3077±0.039[10]
S(assumed, Eunomia)[3]
C(assumed; Adeona)[16]: 23 
9.70[10] · 11.38[3][11] · 11.4[17] · 11.50[7][8] · 11.60[1][6] · 11.64[5] · 11.81±0.22[18]

1384 Kniertje, provisional designation1934 RX, is a dark Adeonianasteroid from the central regions of theasteroid belt, approximately 26 kilometers in diameter. It was discovered on 9 September 1934, by Dutch astronomerHendrik van Gent at theUnion Observatory in Johannesburg, South Africa.[19] The asteroid was named after a character in the Dutch playOp Hoop van Zegen byHerman Heijermans.[2]

Orbit and classification

[edit]

Kniertje is a member of theAdeona family (505),[4] a largefamily of carbonaceous asteroids in the central main belt, named after145 Adeona. It is also dynamically classified as a member of theEunomia family (502), the largest in the intermediate main belt with more than 5,000 stony asteroids.[3][16]: 23 

The asteroid orbits the Sun in thecentral asteroid belt at a distance of 2.2–3.2 AU once every 4 years and 5 months (1,599 days). Its orbit has aneccentricity of 0.18 and aninclination of 12° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Johannesburg in 1934.[19]

Physical characteristics

[edit]

Kniertje'sspectral type is unknown. Although the LCDB assumes anS-type (due to its dynamical classification to the stony Eunomia family), a low albedo of 0.0701 is derived(see below) which is typical for carbonaceousC-type asteroids and in agreement with the overall spectral type of the Adeona family (505).[3][16]: 23 

Rotation period

[edit]

Several rotationallightcurves ofKniertje have been obtained from photometric observations since 2003. Lightcurve analysis gave arotation period between 9.78 and 9.872 hours with a brightness variation between 0.15 and 0.32magnitude (U=2/2/2/2/2).[12][13][14] An alternative period solution of 12.255 hours with an amplitude of 0.33 magnitude was found byBrian Warner in March 2006 (U=2).[15][a]

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,Kniertje measures between 21.52 and 29.592 kilometers in diameter and its surface has analbedo between 0.0351 and 0.3077.[5][6][7][8][9][10][11]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0701 and a diameter of 26.59 kilometers based on anabsolute magnitude of 11.38.[3]

Naming

[edit]

Thisminor planet was named after the principal character inOp Hoop van Zegen, a play by Dutch writerHerman Heijermans (1864–1924). The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 125).[2]

Notes

[edit]
  1. ^abLightcurve plot of 1384 Kniertje, Palmer Divide Observatory, Brian D. Warner (2006). Observer's comment: "a period of 9.816 h cannot be formally excluded". Summary figures atLCDB.

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1384 Kniertje (1934 RX)" (2017-10-01 last obs.).Jet Propulsion Laboratory. Retrieved27 October 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1384) Kniertje".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 112.doi:10.1007/978-3-540-29925-7_1385.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1384) Kniertje". Asteroid Lightcurve Database (LCDB). Retrieved27 October 2017.
  4. ^ab"Asteroid 1384 Kniertje – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abcdNugent, 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.
  6. ^abcdNugent, 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. Retrieved27 October 2017.
  7. ^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)
  8. ^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. Retrieved27 October 2017.
  9. ^abMasiero, 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. Retrieved27 October 2017.
  10. ^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.
  11. ^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.
  12. ^abcdBehrend, Raoul."Asteroids and comets rotation curves – (1384) Kniertje".Geneva Observatory. Retrieved27 October 2017.
  13. ^abHawkins, Scot; Ditteon, Richard (March 2008)."Asteroid Lightcurve Analysis at the Oakley Observatory - May 2007".The Minor Planet Bulletin.35 (1):1–4.Bibcode:2008MPBu...35....1H.ISSN 1052-8091. Retrieved27 October 2017.
  14. ^abVinson, Rachel; Moore, Robert; Ditteon, Richard (July 2014)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2013 October".The Minor Planet Bulletin.41 (3):169–170.Bibcode:2014MPBu...41..169V.ISSN 1052-8091. Retrieved27 October 2017.
  15. ^abWarner, Brian D. (December 2006)."Asteroid lightcurve analysis at the Palmer Divide Observatory - March - June 2006".The Minor Planet Bulletin.33 (4):85–88.Bibcode:2006MPBu...33...85W.ISSN 1052-8091. Retrieved27 October 2017.
  16. ^abcNesvorný, 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.
  17. ^Faure, Gerard; Garret, Lawrence (December 2007)."Suggested Revised H Values of Selected Asteroids: Report Number 3".The Minor Planet Bulletin.34 (4):95–99.Bibcode:2007MPBu...34...95F.ISSN 1052-8091. Retrieved27 October 2017.
  18. ^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. Retrieved27 October 2017.
  19. ^ab"1384 Kniertje (1934 RX)".Minor Planet Center. Retrieved27 October 2017.

External links

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