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10370 Hylonome






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This is an old revision of this page, as edited by JJMC89 bot (talk | contribs)at04:49, 23 September 2016 (Remove {{JPL small body}} parameter(s) migrated to Wikidata per request) (AWB (12089)). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
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10370 Hylonome
Discovery [1]
Discovered byD. C. Jewitt
J. X. Luu
Discovery siteMauna Kea Obs.
Discovery date27 February 1995
Designations

MPC designation

10370 Hylonome

Named after

Hylonome
(Greek mythology)[2]

Alternative designations

1995 DW2

Minor planet category

centaur[3]
Neptune-crosser
Uranus-grazer
Orbital characteristics[1][4]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter3
Observation arc15.27 yr (5,576 days)    
Aphelion31.334 AU
Perihelion18.869 AU

Semi-major axis

25.102 AU
Eccentricity0.2483

Orbital period (sidereal)

125.77 yr (45,936 days)

Mean anomaly

60.558°

Mean motion

0° 0m 28.08s / day
Inclination4.1443°

Longitude of ascending node

178.07°

Argument of perihelion

6.5554°
Jupiter MOID13.42 AU
TJupiter4.451
Physical characteristics
Dimensions70±20km[5]
74±16km[6]
75.09 km (derived)[3]

Geometric albedo

0.051±0.030[6]
0.057 (assumed)[3]

Spectral type

C[3] · BR(color group)[7]

Absolute magnitude (H)

8.6[1]
9.08±0.04 (R)[8]
9.250±0.131 (R)[9]
9.35[3][10]
9.51±0.08[6]
9.53[11][12]

10370 Hylonome (/hˈlɒnəm/; from [‘Υλονομη] Error: {{Lang-xx}}: text has italic markup (help)), provisional designation 1995 DW2, is a minor planet orbiting in the outer Solar System. The dark and icy body belongs to the class of centaurs and measures about 75 kilometers in diameter. It was discovered on 27 February 1995, by English astronomer David C. Jewitt and Vietnamese American astronomer Jane Luu at the U.S. Mauna Kea Observatory in Hawaii.[13]

Centaurs are a large population of icy bodies in transition between trans-Neptunian objects (TNOs) and Jupiter-family comets (JFCs), their orbits being unstable due to perturbations by the giant planets.[6] Currently, Uranus controls Hylonome's perihelion and Neptune its aphelion.[14]

Hylonome is a carbonaceous C-type body that orbits the Sun at a distance of 18.9–31.3 AU once every 125 years and 9 months (45,936 days). Its orbit has an eccentricity of 0.25 and an inclination of 4° with respect to the ecliptic.[1] It is a Neptune-crosser, and an outer-grazer of the orbit of Uranus, which it hence does not cross. Its minimum orbital intersection distance with Neptune and Uranus is 0.35854 and 0.52875 AU, respectively.[13]

It is estimated to have a relatively long orbital half-life of about 6.37 million years.[14] In the year 3478, it will pass within approximately 85 gigameters of Uranus and its semi-major axis will be reduced from 25.1 to 23.5 AU.[15]

Observations with the infrared Spitzer Space Telescope indicate a diameter of 70±20 kilometers,[5] whereas the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous bodies of 0.057, giving it a diameter of 75.1 kilometers, based on an absolute magnitude of 9.35.[3]

A study in 2014, using data from Spitzer's Multiband Imaging Photometer (MIPS) and Herschel's Photodetector Array Camera and Spectrometer, gave a low albedo 0.051±0.030 and a diameter of 74±16 kilometers, based on an absolute magnitudeof9.51±0.08. The study concluded that among the observed population of centaurs, there is no correlation between their sizes, albedos, and orbital parameters. However, the smaller the centaur, the more reddish it is.[6]

The minor planet was named for Hylonome, a female centaurinGreek mythology. In the epic tragedy, she lost her very much beloved husband, the handsome centaur Cyllarus, who was accidentally killed by a spear. Heartbroken, she then took her own life to join him by throwing herself on the spear.[2] Naming citation was published on 26 July 2000 (M.P.C. 41030).[16]

References

  1. ^ a b c d "JPL Small-Body Database Browser: 10370 Hylonome (1995 DW2)" (2010-06-14 last obs.). Jet Propulsion Laboratory. Retrieved 26 May 2016.
  • ^ a b Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (10370) Hylonome. Springer Berlin Heidelberg. p. 731. ISBN 978-3-540-00238-3. Retrieved 26 May 2016.
  • ^ a b c d e f "LCDB Data for (10370) Hylonome". Asteroid Lightcurve Database (LCDB). Retrieved 26 May 2016.
  • ^ "(10370) Hylonome". AstDyS. University of Pisa. Retrieved 20 December 2008.
  • ^ a b John Stansberry; Will Grundy; Mike Brown; Dale Cruikshank; John Spencer; David Trilling; et al. (2007-02-20). "Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope". arXiv:astro-ph/0702538. {{cite arXiv}}: |class= ignored (help)
  • ^ a b c d e Duffard, R.; Pinilla-Alonso, N.; Santos-Sanz, P.; Vilenius, E.; Ortiz, J. L.; Mueller, T.; et al. (April 2014). ""TNOs are Cool": A survey of the trans-Neptunian region. XI. A Herschel-PACS view of 16 Centaurs". Astronomy and Astrophysics. 564: 17. arXiv:1309.0946. Bibcode:2014A&A...564A..92D. doi:10.1051/0004-6361/201322377. {{cite journal}}: |access-date= requires |url= (help)
  • ^ Belskaya, Irina N.; Barucci, Maria A.; Fulchignoni, Marcello; Dovgopol, Anatolij N. (April 2015). "Updated taxonomy of trans-neptunian objects and centaurs: Influence of albedo". Icarus. 250: 482–491. Bibcode:2015Icar..250..482B. doi:10.1016/j.icarus.2014.12.004. Retrieved 26 May 2016.
  • ^ Bauer, James M.; Meech, Karen J.; Fernández, Yanga R.; Pittichova, Jana; Hainaut, Olivier R.; Boehnhardt, Hermann; et al. (November 2003). "Physical survey of 24 Centaurs with visible photometry". Icarus. 166 (1): 195–211. Bibcode:2003Icar..166..195B. doi:10.1016/j.icarus.2003.07.004. {{cite journal}}: |access-date= requires |url= (help)
  • ^ Peixinho, N.; Delsanti, A.; Guilbert-Lepoutre, A.; Gafeira, R.; Lacerda, P. (October 2012). "The bimodal colors of Centaurs and small Kuiper belt objects" (PDF). Astronomy and Astrophysics. 546: 12. arXiv:1206.3153. Bibcode:2012A&A...546A..86P. doi:10.1051/0004-6361/201219057. Retrieved 26 May 2016.
  • ^ Davies, John K.; McBride, Neil; Ellison, Sara L.; Green, Simon F.; Ballantyne, David R. (August 1998). "Visible and Infrared Photometry of Six Centaurs". Icarus. 134 (2): 213–227. Bibcode:1998Icar..134..213D. doi:10.1006/icar.1998.5931. {{cite journal}}: |access-date= requires |url= (help)
  • ^ Romanishin, W.; Tegler, S. C. (March 1999). "Rotation rates of Kuiper-belt objects from their light curves". Nature. 398 (6723): 129–132. Bibcode:1999Natur.398..129R. doi:10.1038/18168. {{cite journal}}: |access-date= requires |url= (help)
  • ^ Romanishin, W.; Tegler, S. C. (December 2005). "Accurate absolute magnitudes for Kuiper belt objects and Centaurs". Icarus. 179 (2): 523–526. Bibcode:2005Icar..179..523R. doi:10.1016/j.icarus.2005.06.016. {{cite journal}}: |access-date= requires |url= (help)
  • ^ a b "10370 Hylonome (1995 DW2)". Minor Planet Center. Retrieved 26 May 2016.
  • ^ a b Horner, J.; Evans, N. W.; Bailey, M. E. (November 2004). "Simulations of the population of Centaurs - I. The bulk statistics" (PDF). Monthly Notices of the Royal Astronomical Society. 354 (3): 798–810. arXiv:astro-ph/0407400. Bibcode:2004MNRAS.354..798H. doi:10.1111/j.1365-2966.2004.08240.x. Retrieved 5 August 2016.
  • ^ "Fifty clones of Centaur 10370 Hylonome all passing within ~85Gm of Uranus in 3478 Oct". Archived from the original on 2009-04-29. Retrieved 2009-04-25. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help) (Solex 10) Template:Webcite
  • ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 26 May 2016.
  • External links


    Retrieved from "https://en.wikipedia.org/w/index.php?title=10370_Hylonome&oldid=740767744"

    Categories: 
    Minor planet object articles (numbered)
    Centaurs (minor planets)
    Numbered minor planets
    Discoveries by David C. Jewitt
    Discoveries by Jane Luu
    Minor planets named from Greek mythology
    Named minor planets
    Astronomical objects discovered in 1995
    Hidden categories: 
    CS1 errors: class
    CS1 errors: access-date without URL
    CS1 errors: unsupported parameter
    Lang and lang-xx template errors
     



    This page was last edited on 23 September 2016, at 04:49 (UTC).

    This version of the page has been revised. Besides normal editing, the reason for revision may have been that this version contains factual inaccuracies, vandalism, or material not compatible with the Creative Commons Attribution-ShareAlike License.



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