Home  

Random  

Nearby  



Log in  



Settings  



Donate  



About Wikipedia  

Disclaimers  



Wikipedia





Galatea (moon)





Article  

Talk  



Language  

Watch  

Edit  





Galatea /ɡæləˈtə/, also known as Neptune VI, is the fourth-closest inner moonofNeptune. It is named after Galatea, one of the fifty NereidsofGreek legend, with whom Cyclops Polyphemus was vainly in love.

Galatea
Galatea as seen by Voyager 2 (elongation is due to smearing)
Discovery
Discovered byStephen P. Synnott[1] and Voyager Imaging Team
Discovery dateJuly 1989
Designations

Designation

Neptune VI
Pronunciation/ɡæləˈtə/[2]

Named after

Γαλάτεια Galateia
AdjectivesGalatean[3]
Orbital characteristics[4][5]
Epoch 18 August 1989

Semi-major axis

61952.57 km
Eccentricity0.00022 ± 0.00008

Orbital period (sidereal)

0.42874431 ± 0.00000001 d
Inclination
  • 0.052 ± 0.011° (to Neptune equator)
  • 0.06° (to local Laplace plane)
  • Satellite ofNeptune
    Groupring shepherd
    Physical characteristics
    Dimensions(204±10) × (184±16) × (144±8) km[6]

    Mean radius

    88±4 km[6]
    Volume~2.8×106 km3[a]
    Mass1.94×1018 kg[8]

    Mean density

    ~0.69 g/cm3[b]

    Surface gravity

    ~0.012–0.025 m/s2[c]

    Escape velocity

    ~0.05–0.06 km/s[d]

    Synodic rotation period

    synchronous

    Axial tilt

    zero
    Albedo0.08[6][9]
    Temperature~51 K mean (estimate)

    Apparent magnitude

    21.9[9]

    Discovery

    edit
     
    Galatea inside of a faint ring arc near Neptune

    Galatea was discovered in late July 1989 from the images taken by the Voyager 2 probe. It was given the temporary designation S/1989 N 4.[10] The discovery was announced (IAUC 4824) on 2 August 1989, and mentions "10 frames taken over 5 days", implying a discovery date of sometime before July 28. The name was given on 16 September 1991.[11]

    Physical properties

    edit

    Galatea is irregularly shaped and shows no sign of any geological modification. It is likely that it is a rubble pile re-accreted from fragments of Neptune's original satellites, which were smashed up by perturbations from Triton soon after that moon's capture into a very eccentric initial orbit.[12]

    Orbit

    edit

    Galatea's orbit lies below Neptune's synchronous orbit radius, so it is slowly spiralling inward due to tidal deceleration and may eventually impact the planet or break up into a new planetary ring system upon passing its Roche limit due to tidal stretching.

    Galatea appears to be a shepherd moon for the Adams ring that is 1,000 kilometres (620 mi) outside its orbit. Resonances with Galatea in the ratio 42:43 are also considered the most likely mechanism for confining the unique ring arcs that exist in this ring.[13] Galatea's mass has been estimated based on the radial perturbations it induces on the ring.[14][7]

    Notes

    edit
    1. ^ Volume derived from the long axis A, the medium axis B and the short axis C:  
  • ^ Density derived from mass m and the volume V:  
  • ^ Surface gravity derived from the mass m, the gravitational constant G and the radius r:  
  • ^ Escape velocity derived from the mass m, the gravitational constant G and the radius r:  
  • Since Galatea is irregularly shaped, the actual surface gravity and escape velocity will vary significantly between different positions on the surface.

    References

    edit
  • ^ "galatea". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  • ^ AMIA (1999), Transforming health care through informatics
  • ^ Jacobson, R. A.; Owen, W. M. Jr. (2004). "The orbits of the inner Neptunian satellites from Voyager, Earthbased, and Hubble Space Telescope observations". Astronomical Journal. 128 (3): 1412–1417. Bibcode:2004AJ....128.1412J. doi:10.1086/423037.
  • ^ Showalter, M. R.; de Pater, I.; Lissauer, J. J.; French, R. S. (2019). "The seventh inner moon of Neptune" (PDF). Nature. 566 (7744): 350–353. Bibcode:2019Natur.566..350S. doi:10.1038/s41586-019-0909-9. PMC 6424524. PMID 30787452.
  • ^ a b c Karkoschka, Erich (2003). "Sizes, shapes, and albedos of the inner satellites of Neptune". Icarus. 162 (2): 400–407. Bibcode:2003Icar..162..400K. doi:10.1016/S0019-1035(03)00002-2.
  • ^ a b Madeira, Gustavo; Winter, Silvia Maria Giuliatti (2022-04-21). "Numerical analysis of processes for the formation of moonlets confining the arcs of Neptune". Monthly Notices of the Royal Astronomical Society. 513 (1): 297–309. arXiv:2204.01063. doi:10.1093/mnras/stac944. ISSN 0035-8711.
  • ^ Giuliatti Winter et al. (2020), as cited in Madeira & Giuliatti Winter (2022).[7]
  • ^ a b "Planetary Satellite Physical Parameters". JPL (Solar System Dynamics). 2008-10-24. Archived from the original on 2013-11-01. Retrieved 2008-12-13.
  • ^ Marsden, Brian G. (August 2, 1989). "Satellites of Neptune". IAU Circular. 4824. Retrieved 2011-10-26.
  • ^ Marsden, Brian G. (September 16, 1991). "Satellites of Saturn and Neptune". IAU Circular. 5347. Retrieved 2011-10-26.
  • ^ Banfield, Don; Murray, Norm (October 1992). "A dynamical history of the inner Neptunian satellites". Icarus. 99 (2): 390–401. Bibcode:1992Icar...99..390B. doi:10.1016/0019-1035(92)90155-Z.
  • ^ Namouni, F.; Porco, C. (2002). "The confinement of Neptune's ring arcs by the moon Galatea". Nature. 417 (6884): 45–7. Bibcode:2002Natur.417...45N. doi:10.1038/417045a. PMID 11986660. S2CID 4430322.
  • ^ Porco, C.C. (1991). "An Explanation for Neptune's Ring Arcs". Science. 253 (5023): 995–1001. Bibcode:1991Sci...253..995P. doi:10.1126/science.253.5023.995. PMID 17775342. S2CID 742763.
  • edit

    Retrieved from "https://en.wikipedia.org/w/index.php?title=Galatea_(moon)&oldid=1224407613"
     



    Last edited on 18 May 2024, at 06:36  





    Languages

     


    Afrikaans
    العربية
    Aragonés
    Azərbaycanca
    تۆرکجه

     / Bân-lâm-gú
    Беларуская
    Български
    Bosanski
    Català
    Čeština
    Cymraeg
    Dansk
    Deutsch
    Eesti
    Ελληνικά
    Español
    Esperanto
    Euskara
    فارسی
    Français
    Galego

    Հայերեն
    ि
    Hrvatski
    Bahasa Indonesia
    Italiano
    עברית
    Коми
    Kreyòl ayisyen
    Latviešu
    Lietuvių
    Magyar
    Македонски

     / Mìng-dĕ̤ng-nḡ

    Nederlands

    Norsk bokmål
    Norsk nynorsk
    Plattdüütsch
    Polski
    Português
    Română
    Русский
    Simple English
    Slovenčina
    Slovenščina
    کوردی
    Српски / srpski
    Suomi
    Svenska
    ி
    Тоҷикӣ
    Türkçe
    Українська
    اردو
    Tiếng Vit
    Winaray



     

    Wikipedia


    This page was last edited on 18 May 2024, at 06:36 (UTC).

    Content is available under CC BY-SA 4.0 unless otherwise noted.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Terms of Use

    Desktop