Astronomy:587 Hypsipyle

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587 Hypsipyle
Discovery [1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date22 February 1906
Designations
(587) Hypsipyle
Pronunciation/hɪpˈsɪpɪliː/[5]
Named afterHypsipyle
(Greek mythology)[2]
1906 TF · 1931 CH
1956 EN1
Minor planet categorymain-belt · (inner) [3]
Phocaea [4]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc111.10 yr (40,578 days)
|{{{apsis}}}|helion}}2.7254 AU
|{{{apsis}}}|helion}}1.9442 AU
2.3348 AU
Eccentricity0.1673
Orbital period3.57 yr (1,303 days)
Mean anomaly85.891°
Mean motion0° 16m 34.68s / day
Inclination24.993°
Longitude of ascending node324.58°
188.53°
Physical characteristics
Dimensions11.022±0.086 km[6]
11.51±0.50 km[7]
12.944±0.103 km[8]
12.991 km[9]
12.99 km (taken)[3]
13.54±0.28 km[10]
Rotation period2.8881±0.0006 h[11]
2.8899±0.0006 h[12]
13.6816±0.0005 h[13]
Geometric albedo0.081±0.004[10]
0.1392[9]
0.1413±0.0237[8]
0.208±0.034[6]
0.474±0.340[7]
S [3]
Absolute magnitude (H)11.12[7] · 11.73±0.39[14] · 11.9[1] · 12.70[10] · 12.19[8] · 12.19±0.11[3][11][9]


Hypsipyle (minor planet designation: 587 Hypsipyle), provisional designation 1906 TF, is a stony Phocaea asteroid from the inner regions of the asteroid belt, approximately 12 kilometers in diameter. It was discovered on 22 February 1906, by Germany astronomer Max Wolf at Heidelberg Observatory in southwest Germany.[15]

The asteroid was named after the Queen Hypsipyle from Greek mythology and is one of the principal members of the Phocaea family.[4]:23

References

  1. ↑ 1.0 1.1 1.2 "JPL Small-Body Database Browser: 587 Hypsipyle (1906 TF)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2000587. 
  2. ↑ Schmadel, Lutz D. (2007). "(587) Hypsipyle". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. pp. 60–61. doi:10.1007/978-3-540-29925-7_588. ISBN 978-3-540-00238-3. 
  3. ↑ 3.0 3.1 3.2 3.3 "LCDB Data for (587) Hypsipyle". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=587%7CHypsipyle. 
  4. ↑ 4.0 4.1 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. 
  5. ↑ Noah Webster (1884) A Practical Dictionary of the English Language
  6. ↑ 6.0 6.1 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 16 August 2017. 
  7. ↑ 7.0 7.1 7.2 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. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M. Retrieved 16 August 2017. 
  8. ↑ 8.0 8.1 8.2 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. 
  9. ↑ 9.0 9.1 9.2 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 16 August 2017. 
  10. ↑ 10.0 10.1 10.2 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)
  11. ↑ 11.0 11.1 Wisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995). "Photoelectric Observations of 125 Asteroids". Abstracts of the Lunar and Planetary Science Conference 26: 1511. Bibcode: 1995LPI....26.1511W. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1995LPI....26.1511W. Retrieved 16 August 2017. 
  12. ↑ Behrend, Raoul. "Asteroids and comets rotation curves – (587) Hypsipyle". Geneva Observatory. http://obswww.unige.ch/~behrend/page2cou.html#000587. 
  13. ↑ 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. 
  14. ↑ 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 16 August 2017. 
  15. ↑ "587 Hypsipyle (1906 TF)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=587. 

External links



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