Astronomy:71 Niobe

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Short description: Main-belt asteroid
71 Niobe
71Niobe (Lightcurve Inversion).png
Lightcurve-based 3D-model of Niobe
Discovery [1]
Discovered byR. Luther
Discovery siteDüsseldorf Obs.
Discovery date13 August 1861
Designations
(71) Niobe
Pronunciation/ˈnaɪəbiː/[5]
Named afterΝιόβη Niobē (Greek mythology)[2]
Minor planet categorymain-belt [1][3] · (middle)
Gallia [4]
AdjectivesNiobean /naɪəˈbiːən/[5]
Orbital characteristics [3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc154.10 yr (56,286 d)
|{{{apsis}}}|helion}}3.2348 AU
|{{{apsis}}}|helion}}2.2790 AU
2.7569 AU
Eccentricity0.1733
Orbital period4.58 yr (1,672 d)
Mean anomaly178.02°
Mean motion0° 12m 55.08s / day
Inclination23.259°
Longitude of ascending node316.02°
266.88°
Physical characteristics
Mean diameter75.87±3.28 km[6]
80.86±0.80 km[7]
83.42±1.7 km[8]
92.75 km (taken)[9]
92.753 km[10]
92.842±0.644 km[11]
Rotation period11 h[12]
11.21 h[13]
14.34±0.05 h[14]
14.34 h[15][14]
14.38±0.02 h[16]
35.5±0.1 h[17][lower-alpha 1]
35.617948 h[9]
35.81±0.01 h[18]
35.8521±0.0005 h[19]
35.864±0.002 h[20]
Geometric albedo0.2446[10]
0.2475±0.0346[11]
0.3052±0.013[8]
0.326±0.008[7]
0.369±0.033[6]
Tholen = S [3]
SMASS = Xe [3] · M [11] · A [21] · X [9]
B–V = 0.803[3]
U–B = 0.439[3]
Absolute magnitude (H)7.30[3][6][7][8][11]
7.31[9]
7.31±0.09[10][16]


Niobe[22] (minor planet designation: 71 Niobe) is a stony Gallia asteroid and relatively slow rotator from the central regions of the asteroid belt, approximately 90 kilometers (56 miles) in diameter. It was discovered by the German astronomer Robert Luther on 13 August 1861, and named after Niobe, a character in Greek mythology. In 1861, the brightness of this asteroid was shown to vary by astronomer Friedrich Tietjen.[23]

Description

Niobe is a member of the Gallia family (802), a small family of nearly 200 known stony asteroids.[24]

In 2006, it was examined by radar using the Arecibo Observatory radio telescope in Puerto Rico. This was supplemented by optical observations intended to build a lightcurve. The resulting estimated rotation period of 35.6 hours, or 1.48 Earth days, superseded an earlier estimate of the rotation period as 14.3 hours. The radar data produced an estimate of a maximum equatorial diameter of 94 km, which is consistent with earlier estimates based upon infrared data if the shape is assumed to be slightly elongated.[17][lower-alpha 1]

The rotation period was further refined to 35.864 ± 0.001 hours during observations through 2010. Six stellar occultations of this asteroid between 2004 and 2007 produced chords ranging from 13 to 72 km (8–45 mi), which are statistically consistent with the published maximum diameter estimates.[20]

Notes

  1. ↑ 1.0 1.1 Lightcurve plot of 71 Niobe, Palmer Divide Observatory, B. D. Warner (2006): rotation period 35.5±0.1 hours with a brightness amplitude of 0.22±0.02 mag. Quality code of 2+. Summary figures at the LCDB

References

  1. ↑ 1.0 1.1 "71 Niobe". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=71. 
  2. ↑ Schmadel, Lutz D. (2007). "(71) Niobe". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 22. doi:10.1007/978-3-540-29925-7_72. ISBN 978-3-540-00238-3. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 "JPL Small-Body Database Browser: 71 Niobe". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2000071. 
  4. ↑ "Asteroid 71 Niobe". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=71+Niobe. 
  5. ↑ 5.0 5.1 Niobe (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=Niobe  (Subscription or UK public library membership required.)
  6. ↑ 6.0 6.1 6.2 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. 
  7. ↑ 7.0 7.1 7.2 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 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. 
  9. ↑ 9.0 9.1 9.2 9.3 "LCDB Data for (71) Niobe". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=71%7CNiobe. 
  10. ↑ 10.0 10.1 10.2 Pravec, 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. doi:10.1016/j.icarus.2012.07.026. Bibcode: 2012Icar..221..365P. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012Icar..221..365P. Retrieved 18 April 2018. 
  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. ↑ Barucci, M. A.; Fulchignoni, M.; Burchi, R.; D'Ambrosio, V. (January 1985). "Rotational properties of ten main belt asteroids - Analysis of the results obtained by photoelectric photometry [ Erratum: 1985Icar...62..173B "]. Icarus 61 (1): 152–162. doi:10.1016/0019-1035(85)90161-7. ISSN 0019-1035. Bibcode: 1985Icar...61..152B. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1985Icar...61..152B. Retrieved 18 April 2018. 
  13. ↑ Lustig, G.; Dvorak, R. (December 1974). "Photometric investigations of the asteroids /43/ Ariadne and /71/ Niobe". Acta Physica Austriaca 43 (1–2): 89–97.InGerman.ResearchsupportedbytheOesterreichischeNationalbank. Bibcode: 1975AcPhA..43...89L. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1975AcPhA..43...89L. Retrieved 18 April 2018. 
  14. ↑ 14.0 14.1 Behrend, Raoul. "Asteroids and comets rotation curves – (71) Niobe". Geneva Observatory. http://obswww.unige.ch/~behrend/page1cou.html#000071. 
  15. ↑ Piironen, J.; Lagerkvist, C.-I.; Erikson, A.; Oja, T.; Magnusson, P.; Festin, L. et al. (March 1998). "Physical studies of asteroids. XXXII. Rotation periods and UBVRI-colours for selected asteroids". Astronomy and Astrophysics Supplement 128 (3): 525–540. doi:10.1051/aas:1998393. Bibcode: 1998A&AS..128..525P. 
  16. ↑ 16.0 16.1 Harris, A. W.; Young, J. W. (October 1989). "Asteroid lightcurve observations from 1979-1981". Icarus 81 (2): 314–364. doi:10.1016/0019-1035(89)90056-0. ISSN 0019-1035. Bibcode: 1989Icar...81..314H. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1989Icar...81..314H. Retrieved 18 April 2018. 
  17. ↑ 17.0 17.1 Warner, Brian D.; Shepard, Michael K.; Harris, Alan W.; Pravec, Petr; Crawford, Greg; Husarik, Marek (December 2006). "Analysis of the lightcurve of 71 Niobe". The Minor Planet Bulletin 33 (4): 102–103. ISSN 1052-8091. Bibcode: 2006MPBu...33..102W. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2006MPBu...33..102W. Retrieved 18 April 2018. 
  18. ↑ Sada, Pedro V.; Warner, Brian D. (June 2007). "Rotation Period of Asteroid 340 Eduarda and Refined Period for Asteroid 71 Niobe". The Minor Planet Bulletin 34 (2): 37–38. ISSN 1052-8091. Bibcode: 2007MPBu...34...37S. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2007MPBu...34...37S. Retrieved 18 April 2018. 
  19. ↑ Hanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M. et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network". Astronomy and Astrophysics 586: 24. doi:10.1051/0004-6361/201527441. Bibcode: 2016A&A...586A.108H. 
  20. ↑ 20.0 20.1 Pilcher, Frederick (July 2010). "A New Investigation of the Rotation Period and Size of 71 Niobe". The Minor Planet Bulletin 37 (3): 98–99. ISSN 1052-8091. Bibcode: 2010MPBu...37...98P. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2010MPBu...37...98P. Retrieved 18 April 2018. 
  21. ↑ Belskaya, I. N.; Fornasier, S.; Tozzi, G. P.; Gil-Hutton, R.; Cellino, A.; Antonyuk, K. et al. (March 2017). "Refining the asteroid taxonomy by polarimetric observations". Icarus 284: 30–42. doi:10.1016/j.icarus.2016.11.003. Bibcode: 2017Icar..284...30B. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2017Icar..284...30B. Retrieved 18 April 2018. 
  22. ↑ with the stress on the first syllable
  23. ↑ Harwood, Margaret (December 1924). "Variations in the Light of Asteroids.". Harvard College Observatory Circular 269: 1–15. Bibcode: 1924HarCi.269....1H. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1924HarCi.269....1H. Retrieved 18 April 2018. 
  24. ↑ 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. 

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