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The Origin and Evolution of the Solar System

The Origin and Evolution of the Solar System

The Origin and Evolution of the Solar System

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14 <strong>The</strong> structure <strong>of</strong> <strong>the</strong> <strong>Solar</strong> <strong>System</strong>Figure 1.7. A Hubble Space Telescope view <strong>of</strong> Pluto <strong>and</strong> its satellite Charon.since it was first discovered in 1930. Prior to its discovery it was postulated that aninth planet should exist, <strong>of</strong> mass Ũ, to explain <strong>the</strong> departures in <strong>the</strong> motions<strong>of</strong> Uranus <strong>and</strong> Neptune from those predicted. By 1978 this estimate had beenlowered in several stages to ¼¼Å¨ but <strong>the</strong> discovery <strong>of</strong> a satellite <strong>of</strong> Pluto in1979 (figure 1.7) gave <strong>the</strong> current estimate <strong>of</strong> ¼¼¼¾½Å ¨. Since this is one-sixth<strong>of</strong> <strong>the</strong> mass <strong>of</strong> <strong>the</strong> Moon <strong>and</strong> gives a density less than one-half that <strong>of</strong> Mars it isobviously not similar to a terrestrial planet. It is reasonable to suppose that itsorigin might be ascribed to some process, or processes, different to that whichproduced <strong>the</strong> normal planets. Recent discoveries <strong>of</strong> trans-Neptunian objects (seesection 1.7.3) make it logical to consider Pluto as a member <strong>of</strong> such a group.1.4 Satellite systems, rings <strong>and</strong> planetary spins1.4.1 ClassificationMost <strong>of</strong> <strong>the</strong> planets are accompanied by smaller bodies, called satellites, in orbitsaround <strong>the</strong>m. In <strong>the</strong> cases <strong>of</strong> <strong>the</strong> major planets <strong>the</strong>se form regular systems similarto <strong>the</strong> planetary system itself. Several <strong>of</strong> <strong>the</strong> satellites are comparable in size to,or slightly larger than, <strong>the</strong> planet Mercury.<strong>The</strong> only satellite known from ancient times is <strong>the</strong> Moon which, being somassive in relation to its primary, must be classified as irregular. <strong>The</strong> first satellites<strong>of</strong> ano<strong>the</strong>r planet to be discovered were <strong>the</strong> four large Galilean satellitesorbiting Jupiter, so named because <strong>of</strong> <strong>the</strong>ir discovery by Galileo Galilei in 1610.With telescope developments over <strong>the</strong> next three <strong>and</strong> a half centuries many smallersatellites were discovered <strong>and</strong> a fur<strong>the</strong>r major boost to <strong>the</strong> known satellite populationhas been provided by spacecraft observation.Many <strong>of</strong> <strong>the</strong> satellites <strong>of</strong> <strong>the</strong> major planets are relatively large <strong>and</strong> occupynear-circular orbits in <strong>the</strong> equatorial plane <strong>of</strong> <strong>the</strong> primary. <strong>The</strong>se are termed regularsatellites <strong>and</strong> <strong>the</strong>y are linked to <strong>the</strong> plausible assumption that <strong>the</strong>y originate aspart <strong>of</strong> <strong>the</strong> process <strong>of</strong> planetary formation. Included in <strong>the</strong> irregular category <strong>of</strong>satellites <strong>the</strong>re are some that are small but in regular orbits <strong>and</strong> one <strong>of</strong> <strong>the</strong> larger

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