156 Xanthippe

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156 Xanthippe
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Lightcurve-base 3D-model of 156 Xanthippe.
Discovery[1]
Discovered byJ. Palisa
Discovery siteAustrian Naval Obs.
Discovery date22 November 1875
Designations
Pronunciation/zænˈθɪpiː/[2]
Named after
Xanthippe
(wife of Socrates)[3]
A875 WA; 1901 SA;
1902 VA; Template:Mp;
1942 RP; 1949 BN
main-belt[1][4] · (middle)
background[5]
Orbital characteristics[4]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc116.46 yr (42,537 d)
Aphelion3.3475 AU
Perihelion2.1069 AU
2.7272 AU
Eccentricity0.2274
4.50 yr (1,645 d)
34.237°
Template:Deg2DMS / day
Inclination9.7818°
241.83°
338.29°
Physical characteristics
110.409 km[6][7]
110.718±2.187 km[8]
115.49±1.74 km[9]
116.34±4.14 km[10]
120.99±2.5 km[11]
121.68±41.10 km[12]
122.02±31.66 km[13]
143.346±0.903 km[14]
143.35±0.90 km[14]
Mass(6.49±3.71)×1018 kg[10]
Mean density
7.86±4.57 g/cm3[10]
22 h[15]
22.104±0.006 h[15]
22.37±0.01 h[16]
22.5 h[17]
0.030±0.004[14]
0.03±0.03[13]
0.04±0.03[12]
0.0422±0.002[11]
0.047±0.002[9]
0.0504±0.0120[8]
0.0687[6]
Tholen = C[4]
SMASS = Ch[4][7]
B–V = 0.713[4]
U–B = 0.315[4]
8.31[7]
8.31±0.09[6][16]
8.64[4][8][9][11][13][14]
8.65[12]
8.83±0.30[18]
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156 Xanthippe is a dark background asteroid from the central regions of the asteroid belt, approximately 120 kilometers (75 miles) in diameter. It was discovered on 22 November 1875, by Austrian astronomer Johann Palisa at the Austrian Naval Observatory, in what is now Croatia.[1] It is named after Xanthippe, the wife of the Greek philosopher Socrates.[3]

Orbit and classification

Xanthippe is a non-family asteroid from the main belt's background population.[5] It orbits the Sun in the central main-belt at a distance of 2.1–3.3 AU once every 4 years and 6 months (1,645 days; semi-major axis of 2.73 AU). Its orbit has an eccentricity of 0.23 and an inclination of 10° with respect to the ecliptic.[4]

Physical characteristics

Photometric observations of this asteroid at the European Southern Observatory in La Silla, Chile during 1981 gave a light curve with a period of 22.5 hours.[17] Based upon its spectrum this is classified as a hydrated C-type asteroid (Ch-subtype) in the SMASS classification, indicating that it likely has a carbonaceous composition.[4][5]

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, Xanthippe measures between 110.409 and 143.35 kilometers in diameter and its surface has an albedo between 0.030 and 0.0687.[6][8][9][11][12][13][14]

Naming

This minor planet was named for Xanthippe, the wife of the Greek philosopher Socrates (c. 470–399 BC), after whom asteroid 5450 Sokrates was named. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 20).[3]

References

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  1. ^ a b c Page Module:Citation/CS1/styles.css has no content."156 Xanthippe". Minor Planet Center. Retrieved 29 May 2018.
  2. ^ Benjamin Smith (1903) The Century Dictionary and Cyclopedia
  3. ^ a b c Page Module:Citation/CS1/styles.css has no content.Schmadel, Lutz D. (2007). "(156) Xanthippe". Dictionary of Minor Planet Names – (156) Xanthippe. Springer Berlin Heidelberg. p. 29. doi:10.1007/978-3-540-29925-7_157. ISBN 978-3-540-00238-3.
  4. ^ a b c d e f g h i Page Module:Citation/CS1/styles.css has no content."JPL Small-Body Database Browser: 156 Xanthippe" (2018-03-06 last obs.). Jet Propulsion Laboratory. Retrieved 29 May 2018.
  5. ^ a b c Page Module:Citation/CS1/styles.css has no content."Asteroid 156 Xanthippe". Small Bodies Data Ferret. Retrieved 29 May 2018.
  6. ^ a b c d Page Module:Citation/CS1/styles.css has no content.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. Bibcode:2012Icar..221..365P. doi:10.1016/j.icarus.2012.07.026.
  7. ^ a b c Template:Cite LCDB
  8. ^ a b c d Page Module:Citation/CS1/styles.css has no content.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. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. S2CID 35447010. (catalog)
  9. ^ a b c d Page Module:Citation/CS1/styles.css has no content.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. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)
  10. ^ a b c Page Module:Citation/CS1/styles.css has no content.Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73 (1): 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009, S2CID 119226456 See Table 1.
  11. ^ a b c d Page Module:Citation/CS1/styles.css has no content.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. Retrieved 22 October 2019.
  12. ^ a b c d Page Module:Citation/CS1/styles.css has no content.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. arXiv:1606.08923. Bibcode:2016AJ....152...63N. doi:10.3847/0004-6256/152/3/63.
  13. ^ a b c d Page Module:Citation/CS1/styles.css has no content.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. arXiv:1509.02522. Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. S2CID 9341381.
  14. ^ a b c d e Page Module:Citation/CS1/styles.css has no content.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. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. S2CID 46350317.
  15. ^ a b Page Module:Citation/CS1/styles.css has no content.Behrend, Raoul. "Asteroids and comets rotation curves – (156) Xanthippe". Geneva Observatory. Retrieved 29 May 2018.
  16. ^ a b Page Module:Citation/CS1/styles.css has no content.Harris, A. W.; Young, J. W. (October 1989). "Asteroid lightcurve observations from 1979-1981". Icarus. 81 (2): 314–364. Bibcode:1989Icar...81..314H. doi:10.1016/0019-1035(89)90056-0. ISSN 0019-1035.
  17. ^ a b Page Module:Citation/CS1/styles.css has no content.Debehogne, H.; de Sanctis, G.; Zappala, V. (April 1982). "Photoelectric photometry of three dark asteroids". Astronomy and Astrophysics. 108 (1): 197–200. Bibcode:1982A&A...108..197D.
  18. ^ Page Module:Citation/CS1/styles.css has no content.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.
  19. ^ Script error: No such module "template wrapper". (Subscription or participating institution membership required.)

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