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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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22 <strong>The</strong> structure <strong>of</strong> <strong>the</strong> <strong>Solar</strong> <strong>System</strong>Table 1.7. <strong>The</strong> satellite system <strong>of</strong> Uranus. <strong>The</strong> spin period <strong>of</strong> Uranus ½Ö½ÑÒ.Inclination Semi-major Average<strong>of</strong> orbit to axis Mass diameter DensitySatellite equator (½¼ ¿ km) Eccentricity (½¼ ¾¾ kg) (km) (½¼ ¿ Ñ ¿ )Nine small 50–73 40–80satellitesPuck ¼¼ Æ 86 0.000 170Mir<strong>and</strong>a ¼¼ Æ 130 0.000 0.0075 484 1.26Ariel ¼¼ Æ 191 0.003 0.14 1160 1.65Umbriel ¼¼ Æ 266 0.003 0.13 1190 1.44Titania ¼¼ Æ 436 0.002 0.35 1610 1.59Oberon ¼¼ Æ 583 0.007 0.29 1550 1.50Table 1.8. <strong>The</strong> satellite system <strong>of</strong> Neptune. <strong>The</strong> spin period <strong>of</strong> Neptune ½ Ö ÑÒ.Inclination Semi-major Average<strong>of</strong> orbit to axis Mass diameter DensitySatellite equator (½¼ ¿ km) Eccentricity (½¼ ¾¾ kg) (km) (½¼ ¿ Ñ ¿ )Niaid 48 60Thalassa 50 80Despoina 53 150Galatea 62 160Larissa 74 200Proteus 118 415Triton ½¼ Æ 355 0.000 2.21 2705 2.07Nereid ¾ Æ 5513 0.749 0.0021 340<strong>The</strong>se two, plus ano<strong>the</strong>r six found by spacecraft observation are listed in table 1.8.Stellar occultation observations had indicated that Neptune should have aring system <strong>and</strong>, indeed, <strong>the</strong>se were seen <strong>and</strong> imaged by <strong>the</strong> Voyager spacecraft.<strong>The</strong> Earth-bound measurements had suggested that <strong>the</strong> rings were only partial butit turns out that <strong>the</strong>y are complete but have a ra<strong>the</strong>r lumpy structure.<strong>The</strong> presence <strong>of</strong> rings accompanying each <strong>of</strong> <strong>the</strong> major planets suggests that<strong>the</strong>re is some common cause associated with <strong>the</strong>ir characteristics as large bodieswith many satellite companions. <strong>The</strong> most likely origin for a ring system is that<strong>the</strong> orbit <strong>of</strong> a small orbiting satellite decayed to <strong>the</strong> extent that it strayed within <strong>the</strong>Roche limit (section 4.4.2). It would <strong>the</strong>n have been tidally disrupted by <strong>the</strong> planetto give a vast number <strong>of</strong> small fragments that would have spread out to form <strong>the</strong>rings. Structure in <strong>the</strong> rings could <strong>the</strong>n be produced by resonant perturbations bysome <strong>of</strong> <strong>the</strong> inner satellites as described in section 1.4.3.

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