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587 Hypsipyle

From Wikipedia, the free encyclopedia
Main-belt asteroid

587 Hypsipyle
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date22 February 1906
Designations
(587) Hypsipyle
Pronunciation/hɪpˈsɪpɪl/[2]
Named after
Hypsipyle
(Greek mythology)[3]
1906 TF · 1931 CH
1956 EN1
main-belt · (inner)[4]
Phocaea[5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc111.10 yr (40,578 days)
Aphelion2.7254AU
Perihelion1.9442 AU
2.3348 AU
Eccentricity0.1673
3.57yr (1,303 days)
85.891°
0° 16m 34.68s / day
Inclination24.993°
324.58°
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)[4]
13.54±0.28 km[10]
2.8881±0.0006h[11]
2.8899±0.0006 h[12]
13.6816±0.0005 h[13]
0.081±0.004[10]
0.1392[9]
0.1413±0.0237[8]
0.208±0.034[6]
0.474±0.340[7]
S[4]
11.12[7] · 11.73±0.39[14] · 11.9[1] · 12.70[10] · 12.19[8] · 12.19±0.11[4][11][9]

587 Hypsipyle, provisional designation1906 TF, is a stony Phocaeaasteroid from the inner regions of theasteroid belt, approximately 12 kilometers in diameter. It was discovered on 22 February 1906, by Germany astronomerMax Wolf atHeidelberg Observatory in southwest Germany.[15]

The asteroid was named after the QueenHypsipyle fromGreek mythology and is one of the principal members of thePhocaea family.[5]: 23 

References

[edit]
  1. ^abc"JPL Small-Body Database Browser: 587 Hypsipyle (1906 TF)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved16 August 2017.
  2. ^Noah Webster (1884)A Practical Dictionary of the English Language
  3. ^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.
  4. ^abcd"LCDB Data for (587) Hypsipyle". Asteroid Lightcurve Database (LCDB). Retrieved16 August 2017.
  5. ^abNesvorný, 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.
  6. ^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. Retrieved16 August 2017.
  7. ^abcMasiero, 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. Retrieved16 August 2017.
  8. ^abcMainzer, 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.
  9. ^abcPravec, 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. Retrieved16 August 2017.
  10. ^abcUsui, 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)
  11. ^abWisniewski, 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. Retrieved16 August 2017.
  12. ^Behrend, Raoul."Asteroids and comets rotation curves – (587) Hypsipyle".Geneva Observatory. Retrieved16 August 2017.
  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.arXiv:1510.07422.Bibcode:2016A&A...586A.108H.doi:10.1051/0004-6361/201527441.
  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.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved16 August 2017.
  15. ^"587 Hypsipyle (1906 TF)".Minor Planet Center. Retrieved16 August 2017.

External links

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