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  • [[Image:PIA01627 Ringe.jpg|thumb|400px|right|A schema of Jupiter's ring system showing the four main components]] ...th]] for the past 25 years.<ref name=Meier1999/> Ground-based observations of the rings require the largest available [[telescopes]].<ref name=dePater199 ...
    40 KB (6,124 words) - 17:25, 21 July 2009
  • ...etween the orbits of [[Mars]] and Jupiter (white) and the [[Hilda family]] of asteroids (brown).]] ...regions around these Lagrangian points with an average [[semi-major axis]] of about 5.2&nbsp;AU.<ref name=Yoshida2005/> ...
    27 KB (3,965 words) - 06:02, 30 July 2009
  • ...ring-moon system. Solid lines denote rings; dashed lines denote orbits of moons.]] ...t with the orbit of Neptunian moon [[Galatea (moon)|Galatea]]. Three other moons orbit between the rings: [[Naiad (moon)|Naiad]], [[Thalassa (moon)|Thalassa ...
    29 KB (4,327 words) - 17:10, 4 April 2011
  • Scroll down to edit the contents of this page. | alt_names = Jupiter IV ...
    50 KB (7,326 words) - 08:23, 11 August 2009
  • {{otheruses4|the natural satellite of Jupiter|the asteroid|1036 Ganymed}} Scroll down to edit the contents of this page. ...
    62 KB (9,204 words) - 08:32, 18 August 2009
  • [[File:Protoplanetary-disk.jpg|thumb|400px|Artist's conception of a [[protoplanetary disc]]]] ...ote: per [[WP:BOLDTITLE]], topic name should NOT be bold because the title of this article is descriptive--> ...
    85 KB (12,829 words) - 17:09, 18 August 2009
  • ...System's largest objects (radius, mass, orbital distance etc.) see [[List of Solar System objects in hydrostatic equilibrium]]}} [[Image:Planets2008.jpg|right|390px|thumb|[[Planet]]s and [[dwarf planet]]s of the Solar System. Sizes are to scale, but relative distances from the Sun a ...
    82 KB (12,278 words) - 17:12, 18 August 2009
  • ...rmatting and layout of this infobox has been matched with the other bodies of the solar system. Please do not arbitrarily change it without discussion. Scroll down to edit the contents of this page. ...
    83 KB (11,988 words) - 11:30, 20 August 2009
  • ...nit]]s. The pronounced gap at the bottom is due to obscuration by the band of the [[Milky Way]].]] ...eology)|rock]] and [[metal]], the Kuiper belt objects are composed largely of frozen [[volatiles]] (termed "ices"), such as [[methane]], [[ammonia]] and ...
    58 KB (9,031 words) - 16:11, 18 August 2009
  • ...[[universe]].<ref name=Montmerle2006/> The widely accepted modern variant of the nebular hypothesis is '''Solar Nebular Disk Model''' (SNDM) or simply ' ...Thus the formation of planetary systems is thought to be a natural result of star formation. A sun-like star usually takes around 100&nbsp;million years ...
    50 KB (7,534 words) - 17:00, 23 June 2009
  • ...rmatting and layout of this infobox has been matched with the other bodies of the solar system. Please do not arbitrarily change it without discussion. Scroll down to edit the contents of this page. ...
    105 KB (15,836 words) - 04:41, 17 August 2009
  • caption=The position of Sirius. }} ...by SIMBAD from the [[Hipparcos]] catalogue, pertains to the center of mass of the Sirius system. See &sect;2.3.4, ''[http://www.rssd.esa.int/SA/HIPPARCO ...
    58 KB (8,480 words) - 20:27, 18 August 2009
  • | symbol = [[File:Earth symbol.svg|25px|Astronomical symbol of Earth]] | image = [[File:The Earth seen from Apollo 17.jpg|240px|A color image of Earth, as seen from Apollo 17]] ...
    115 KB (16,384 words) - 01:33, 18 August 2009