Astronomy:1384 Kniertje

From HandWiki
Revision as of 11:55, 6 February 2024 by NBrushPhys (talk | contribs) (add)
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
1384 Kniertje
Discovery[1]
Discovered byH. van Gent
Discovery siteJohannesburg Obs.
Discovery date9 September 1934
Designations
(1384) Kniertje
Named afterKniertje[2] (fictional character)
1934 RX
Minor planet categorymain-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)
|{{{apsis}}}|helion}}3.1649 AU
|{{{apsis}}}|helion}}2.1872 AU
2.6760 AU
Eccentricity0.1827
Orbital period4.38 yr (1,599 days)
Mean anomaly288.15°
Mean motion0° 13m 30.36s / day
Inclination11.858°
Longitude of ascending node152.86°
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]
Rotation period9.78±0.02 h[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][lower-alpha 1]
Geometric albedo0.0351±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
Absolute magnitude (H)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 designation 1934 RX, is a dark Adeonian asteroid from the central regions of the asteroid belt, approximately 26 kilometers in diameter. It was discovered on 9 September 1934, by Dutch astronomer Hendrik van Gent at the Union Observatory in Johannesburg, South Africa.[19] The asteroid was named after a character in the Dutch play Op Hoop van Zegen by Herman Heijermans.[2]

Orbit and classification

Kniertje is a member of the Adeona family (505),[4] a large family of carbonaceous asteroids in the central main belt, named after 145 Adeona. It is also dynamically classified as a member of the Eunomia 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 the central asteroid belt at a distance of 2.2–3.2 AU once every 4 years and 5 months (1,599 days). Its orbit has an eccentricity of 0.18 and an inclination of 12° with respect to the ecliptic.[1] The body's observation arc begins with its official discovery observation at Johannesburg in 1934.[19]

Physical characteristics

Kniertje's spectral type is unknown. Although the LCDB assumes an S-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 carbonaceous C-type asteroids and in agreement with the overall spectral type of the Adeona family (505).[3][16]:23

Rotation period

Several rotational lightcurves of Kniertje have been obtained from photometric observations since 2003. Lightcurve analysis gave a rotation period between 9.78 and 9.872 hours with a brightness variation between 0.15 and 0.32 magnitude ({{{1}}}).[12][13][14] An alternative period solution of 12.255 hours with an amplitude of 0.33 magnitude was found by Brian Warner in March 2006 ({{{1}}}).[15][lower-alpha 1]

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Kniertje measures between 21.52 and 29.592 kilometers in diameter and its surface has an albedo between 0.0351 and 0.3077.[5][6][7][8][9][10][11]

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

Naming

This minor planet was named after the principal character in Op Hoop van Zegen, a play by Dutch writer Herman Heijermans (1864–1924). The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 125).[2]

Notes

  1. ↑ 1.0 1.1 Lightcurve 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 at LCDB.

References

  1. ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 1384 Kniertje (1934 RX)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001384. Retrieved 27 October 2017. 
  2. ↑ 2.0 2.1 2.2 Schmadel, 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. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 "LCDB Data for (1384) Kniertje". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1384%7CKniertje. Retrieved 27 October 2017. 
  4. ↑ 4.0 4.1 "Asteroid 1384 Kniertje – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1384+Kniertje#Asteroid%201384%20KniertjeEAR-A-VARGBDET-5-NESVORNYFAM-V3.0. Retrieved 26 October 2019. 
  5. ↑ 5.0 5.1 5.2 5.3 Nugent, 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. doi:10.3847/0004-6256/152/3/63. Bibcode: 2016AJ....152...63N. 
  6. ↑ 6.0 6.1 6.2 6.3 Nugent, 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. doi:10.1088/0004-637X/814/2/117. Bibcode: 2015ApJ...814..117N. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N. Retrieved 27 October 2017. 
  7. ↑ 7.0 7.1 7.2 7.3 Usui, 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. doi:10.1093/pasj/63.5.1117. Bibcode: 2011PASJ...63.1117U.  (online, AcuA catalog p. 153)
  8. ↑ 8.0 8.1 8.2 8.3 Masiero, 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. doi:10.1088/2041-8205/759/1/L8. Bibcode: 2012ApJ...759L...8M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M. Retrieved 27 October 2017. 
  9. ↑ 9.0 9.1 Masiero, 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. doi:10.1088/0004-637X/791/2/121. Bibcode: 2014ApJ...791..121M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M. Retrieved 27 October 2017. 
  10. ↑ 10.0 10.1 10.2 10.3 Tedesco, 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. https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab. Retrieved 22 October 2019. 
  11. ↑ 11.0 11.1 11.2 11.3 Mainzer, 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. doi:10.1088/0004-637X/741/2/90. Bibcode: 2011ApJ...741...90M. 
  12. ↑ 12.0 12.1 12.2 12.3 Behrend, Raoul. "Asteroids and comets rotation curves – (1384) Kniertje". Geneva Observatory. http://obswww.unige.ch/~behrend/page4cou.html#001384. Retrieved 27 October 2017. 
  13. ↑ 13.0 13.1 Hawkins, Scot; Ditteon, Richard (March 2008). "Asteroid Lightcurve Analysis at the Oakley Observatory - May 2007". The Minor Planet Bulletin 35 (1): 1–4. ISSN 1052-8091. Bibcode: 2008MPBu...35....1H. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2008MPBu...35....1H. Retrieved 27 October 2017. 
  14. ↑ 14.0 14.1 Vinson, 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. ISSN 1052-8091. Bibcode: 2014MPBu...41..169V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014MPBu...41..169V. Retrieved 27 October 2017. 
  15. ↑ 15.0 15.1 Warner, Brian D. (December 2006). "Asteroid lightcurve analysis at the Palmer Divide Observatory - March - June 2006". The Minor Planet Bulletin 33 (4): 85–88. ISSN 1052-8091. Bibcode: 2006MPBu...33...85W. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2006MPBu...33...85W. Retrieved 27 October 2017. 
  16. ↑ 16.0 16.1 16.2 Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131. Bibcode: 2015aste.book..297N. 
  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. ISSN 1052-8091. Bibcode: 2007MPBu...34...95F. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2007MPBu...34...95F. Retrieved 27 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. doi:10.1016/j.icarus.2015.08.007. Bibcode: 2015Icar..261...34V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V. Retrieved 27 October 2017. 
  19. ↑ 19.0 19.1 "1384 Kniertje (1934 RX)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=1384. Retrieved 27 October 2017. 

External links



Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:1384_Kniertje&oldid=3353515"