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Hiʻiaka (moon)

Hiʻiaka is the larger, outer moon of the trans-Neptunian dwarf planet Haumea. It is named after one of the daughters of Haumea, Hiʻiaka, the patron goddess of the Big Island of Hawaii. It orbits once every 49.12±0.03 d at a distance of 49880±198 km, with an eccentricity of 0.0513±0.0078 and an inclination of 126.356±0.064°. Assuming its estimated diameter of over 300 km is accurate, it may be the fourth- or fifth-largest known moon of a Trans-Neptunian object, after Pluto I Charon, Eris I Dysnomia, Orcus I Vanth, and possibly Varda I Ilmarë and Salacia I Actaea.

Hiʻiaka
In this series of photos taken by the Hubble Space Telescope, the brighter object Hiʻiaka is seen orbiting Haumea (center).
Discovery
Discovered byMichael E. Brown,
Chad Trujillo,
David Rabinowitz, et al.
Discovery date26 January 2005
Designations
Designation
Haumea I
Pronunciation/hʔiˈɑːkə/
Hawaiian: [ˈhiʔiˈjɐkə]
(136108) 2003 EL61 I
S/2005 (2003 EL61) 1
Orbital characteristics[1]
49880±198 km
Eccentricity0.0513±0.0078
49.12±0.03 d
152.8°±6.1°
Inclination126.356±0.064°
206.766°±0.033°
154.1°±5.8°
Satellite ofHaumea
Physical characteristics
Mean radius
~160 km[1]
Mass(1.79±0.11)×1019 kg[1] (0.45% of Haumea)
Mean density
~1 g/cm3
~9.8 h[2]
Albedo0.8±0.07[3][1]
Temperature32±K
20.3 (3.0 difference from primary's 17.3)[3]

Discovery edit

Hiʻiaka was the first satellite discovered around Haumea. It was discovered on 26 January 2005 and nicknamed "Rudolph" by the discovery team before being assigned an official name.

Physical characteristics edit

Size and brightness edit

Its measured brightness is 5.9±0.5%, translating into a diameter of about 22% of its primary, or in the range of 320 km, assuming similar infrared albedo.[1] To put this in perspective, if Hiʻiaka were in the asteroid belt, it would be larger than all but the four largest asteroids, after 1 Ceres, 2 Pallas, 4 Vesta, and 10 Hygiea. In spite of its relatively large size, however, lightcurve studies suggest that Hiʻiaka is not a gravitationally collapsed spheroid; they further suggest that Hiʻiaka is not tidally locked and has a rotation period of about 9.8 hours.[2]

Mass edit

The mass of Hiʻiaka is estimated to be (1.79±0.11)×1019 kg using precise relative astrometry from the Hubble Space Telescope and Keck Telescope and applying 3-body, point-mass model to the Haumean system.[1]

Spectrum and composition edit

The near infrared spectrum of Hiʻiaka is dominated by water-ice absorption bands, which means that its surface is made mainly of water ice. The presence of the band centered at 1.65 μm indicates that the surface water ice is primarily in the crystalline form. Currently it is unclear why water ice on the surface has not turned into amorphous form as would be expected due to its constant irradiation by cosmic rays.[4]

See also edit

Notes edit

References edit

  1. ^ a b c d e f Ragozzine, D.; Brown, M. E. (2009). "Orbits and Masses of the Satellites of the Dwarf Planet Haumea (2003 EL61)". The Astronomical Journal. 137 (6): 4766–4776. arXiv:0903.4213. Bibcode:2009AJ....137.4766R. doi:10.1088/0004-6256/137/6/4766. S2CID 15310444.
  2. ^ a b Hastings, Danielle M.; Ragozzine, Darin; Fabrycky, Daniel C.; Burkhart, Luke D.; Fuentes, Cesar; Margot, Jean-Luc; Brown, Michael E.; Holman, Matthew (December 2016). "The Short Rotation Period of Hiʻiaka, Haumea's Largest Satellite". The Astronomical Journal. 152 (6): 12. arXiv:1610.04305. Bibcode:2016AJ....152..195H. doi:10.3847/0004-6256/152/6/195. OCLC 6889796157. OSTI 22662917. S2CID 33292771. 195.
  3. ^ a b Wm. Robert Johnston (17 September 2008). "(136108) Haumea, Hiʻiaka, and Nāmaka". Retrieved 18 September 2008.
  4. ^ Dumas, C.; Carry, B.; Hestroffer, D.; Merlin, F. (2011). "High-contrast observations of (136108) Haumea". Astronomy & Astrophysics. 528: A105. arXiv:1101.2102. Bibcode:2011A&A...528A.105D. doi:10.1051/0004-6361/201015011. S2CID 119226136.

External links edit

  • Brown's publication describing the discovery of Hiʻiaka
  • Paper describing the composition of Hiʻiaka

hiʻiaka, moon, hiʻiaka, larger, outer, moon, trans, neptunian, dwarf, planet, haumea, named, after, daughters, haumea, hiʻiaka, patron, goddess, island, hawaii, orbits, once, every, distance, 49880, with, eccentricity, 0513, 0078, inclination, assuming, estima. Hiʻiaka is the larger outer moon of the trans Neptunian dwarf planet Haumea It is named after one of the daughters of Haumea Hiʻiaka the patron goddess of the Big Island of Hawaii It orbits once every 49 12 0 03 d at a distance of 49880 198 km with an eccentricity of 0 0513 0 0078 and an inclination of 126 356 0 064 Assuming its estimated diameter of over 300 km is accurate it may be the fourth or fifth largest known moon of a Trans Neptunian object after Pluto I Charon Eris I Dysnomia Orcus I Vanth and possibly Varda I Ilmare and Salacia I Actaea HiʻiakaIn this series of photos taken by the Hubble Space Telescope the brighter object Hiʻiaka is seen orbiting Haumea center DiscoveryDiscovered byMichael E Brown Chad Trujillo David Rabinowitz et al Discovery date26 January 2005DesignationsDesignationHaumea IPronunciation h iː ʔ i ˈ ɑː k e Hawaiian ˈhiʔiˈjɐke Alternative names 136108 2003 EL61 IS 2005 2003 EL61 1Orbital characteristics 1 Semi major axis49880 198 kmEccentricity0 0513 0 0078Orbital period sidereal 49 12 0 03 dMean anomaly152 8 6 1 Inclination126 356 0 064 Longitude of ascending node206 766 0 033 Argument of perihelion154 1 5 8 Satellite ofHaumeaPhysical characteristicsMean radius 160 km 1 Mass 1 79 0 11 1019 kg 1 0 45 of Haumea Mean density 1 g cm3Synodic rotation period 9 8 h 2 Albedo0 8 0 07 3 1 Temperature32 3 KApparent magnitude20 3 3 0 difference from primary s 17 3 3 Contents 1 Discovery 2 Physical characteristics 2 1 Size and brightness 2 2 Mass 2 3 Spectrum and composition 3 See also 4 Notes 5 References 6 External linksDiscovery editHiʻiaka was the first satellite discovered around Haumea It was discovered on 26 January 2005 and nicknamed Rudolph by the discovery team before being assigned an official name Physical characteristics editSize and brightness edit Its measured brightness is 5 9 0 5 translating into a diameter of about 22 of its primary or in the range of 320 km assuming similar infrared albedo 1 To put this in perspective if Hiʻiaka were in the asteroid belt it would be larger than all but the four largest asteroids after 1 Ceres 2 Pallas 4 Vesta and 10 Hygiea In spite of its relatively large size however lightcurve studies suggest that Hiʻiaka is not a gravitationally collapsed spheroid they further suggest that Hiʻiaka is not tidally locked and has a rotation period of about 9 8 hours 2 Mass edit The mass of Hiʻiaka is estimated to be 1 79 0 11 1019 kg using precise relative astrometry from the Hubble Space Telescope and Keck Telescope and applying 3 body point mass model to the Haumean system 1 Spectrum and composition edit The near infrared spectrum of Hiʻiaka is dominated by water ice absorption bands which means that its surface is made mainly of water ice The presence of the band centered at 1 65 mm indicates that the surface water ice is primarily in the crystalline form Currently it is unclear why water ice on the surface has not turned into amorphous form as would be expected due to its constant irradiation by cosmic rays 4 See also editNamaka the other moon of HaumeaNotes editReferences edit a b c d e f Ragozzine D Brown M E 2009 Orbits and Masses of the Satellites of the Dwarf Planet Haumea 2003 EL61 The Astronomical Journal 137 6 4766 4776 arXiv 0903 4213 Bibcode 2009AJ 137 4766R doi 10 1088 0004 6256 137 6 4766 S2CID 15310444 a b Hastings Danielle M Ragozzine Darin Fabrycky Daniel C Burkhart Luke D Fuentes Cesar Margot Jean Luc Brown Michael E Holman Matthew December 2016 The Short Rotation Period of Hiʻiaka Haumea s Largest Satellite The Astronomical Journal 152 6 12 arXiv 1610 04305 Bibcode 2016AJ 152 195H doi 10 3847 0004 6256 152 6 195 OCLC 6889796157 OSTI 22662917 S2CID 33292771 195 a b Wm Robert Johnston 17 September 2008 136108 Haumea Hiʻiaka and Namaka Retrieved 18 September 2008 Dumas C Carry B Hestroffer D Merlin F 2011 High contrast observations of 136108 Haumea Astronomy amp Astrophysics 528 A105 arXiv 1101 2102 Bibcode 2011A amp A 528A 105D doi 10 1051 0004 6361 201015011 S2CID 119226136 External links editBrown s publication describing the discovery of Hiʻiaka Paper describing the composition of Hiʻiaka Retrieved from https en wikipedia org w index php title Hiʻiaka moon amp oldid 1188183603, wikipedia, wiki, book, books, library,

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