{"id":363,"date":"2016-11-15T21:37:02","date_gmt":"2016-11-15T21:37:02","guid":{"rendered":"https:\/\/courses.lumenlearning.com\/astronomy\/?post_type=chapter&#038;p=363"},"modified":"2017-07-17T18:34:20","modified_gmt":"2017-07-17T18:34:20","slug":"ring-and-moon-systems-introduced","status":"publish","type":"chapter","link":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/chapter\/ring-and-moon-systems-introduced\/","title":{"raw":"Ring and Moon Systems Introduced","rendered":"Ring and Moon Systems Introduced"},"content":{"raw":"<div class=\"textbox learning-objectives\">\r\n<h3>Learning Objectives<\/h3>\r\nBy the end of this section, you will be able to:\r\n<ul>\r\n \t<li>Name the major moons of each of the jovian planets<\/li>\r\n \t<li>Describe the basic composition of each jovian planet\u2019s ring system<\/li>\r\n<\/ul>\r\n<\/div>\r\nThe rings and <strong>moons<\/strong> (see the moons in Figure 1)\u00a0of the outer solar system are not composed of the same materials as the mostly rocky objects in the inner solar system. We should expect this, since they formed in regions of lower temperature, cool enough so that large quantities of water ice were available as building materials. Most of these objects also contain dark, organic compounds mixed with their ice and rock. Don\u2019t be surprised, therefore, to find that many objects in the ring and moon systems are both icy and dark.\r\n\r\nRoughly a third of the moons in the outer solar system are in <em>direct<\/em> or regular orbits; that is, they revolve about their parent planet in a west-to-east direction and in the plane of the planet\u2019s equator. The majority are irregular moons that orbit in a <em>retrograd<\/em>e (east-to-west) direction or else have orbits of high eccentricity (more elliptical than circular) or high inclination (moving in and out of the planet\u2019s equatorial plane). These irregular moons are mostly located relatively far from their planet; they were probably formed elsewhere and subsequently captured by the planet they now orbit. (Perhaps the fact that they were not born locally will excuse their ill-mannered behavior.)\r\n\r\n[caption id=\"\" align=\"aligncenter\" width=\"700\"]<img class=\"\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/1095\/2016\/11\/03155722\/OSC_Astro_12_01_SelectMoon.jpg\" alt=\"An image showing the moons of the solar system in comparison to the size of the Earth. Earth is pictured at the bottom right. At the top of the image the planets are labeled from left to right. Under \" width=\"700\" height=\"458\" data-media-type=\"image\/jpeg\" \/> <strong>Figure 1: Moons of the Solar System. <\/strong> This image shows some selected moons of our solar system and their comparison to the size of Earth\u2019s Moon and Earth itself. (credit: modification of work by NASA)[\/caption]\r\n<h2>The Jupiter System<\/h2>\r\n<strong>Jupiter<\/strong> has 67 known moons (that\u2019s the number as we write) and a faint ring. These include four large moons\u2014<strong>Callisto<\/strong>, <strong>Ganymede<\/strong>, <strong>Europa<\/strong>, and <strong>Io<\/strong> (see <a href=\".\/chapter\/introduction-to-rings-moons-and-pluto\/\" target=\"_blank\" rel=\"noopener\">Figure 1 in Introduction to Rings, Moons, and Pluto<\/a>)\u2014discovered in 1610 by Galileo and therefore often called the <em>Galilean moons<\/em>. The smaller of these, Europa and Io, are about the size of our Moon, while the larger, Ganymede and Callisto, are about the same size as the planet Mercury. Most of Jupiter\u2019s moons are much smaller. The majority are in retrograde orbits more than 20 million kilometers from Jupiter; these are very likely small captured asteroids.\r\n<h2>The Saturn System<\/h2>\r\n<strong>Saturn<\/strong> has at least 62 known moons in addition to a magnificent set of rings. The largest of the moons, <strong>Titan<\/strong>, is almost as big as Ganymede in Jupiter\u2019s system, and it is the only moon with a substantial atmosphere and lakes or seas of liquid hydrocarbons (such as methane and ethane) on the surface. Saturn has six other large regular moons with diameters between 400 and 1600 kilometers, a collection of small moons orbiting in or near the rings, and many captured strays similar to those of Jupiter. Mysteriously, one of Saturn\u2019s smaller moons, <strong>Enceladus<\/strong>, has active geysers of water being expelled into space.\r\n\r\nThe rings of Saturn, one of the most impressive sights in the solar system, are broad and flat, with a few major and many minor gaps. They are not solid, but rather a huge collection of icy fragments, all orbiting the equator of Saturn in a traffic pattern that makes rush hour in a big city look simple by comparison. Individual ring particles are composed primarily of water ice and are typically the size of ping-pong balls, tennis balls, and basketballs.\r\n<h2>The Uranus System<\/h2>\r\nThe ring and moon system of <strong>Uranus<\/strong> is tilted at 98\u00b0, just like the planet itself. It consists of 11 rings and 27 currently known moons. The five largest moons are similar in size to the six regular moons of Saturn, with diameters of 500 to 1600 kilometers. Discovered in 1977, the rings of Uranus are narrow ribbons of dark material with broad gaps in between. Astronomers suppose that the ring particles are confined to these narrow paths by the gravitational effects of numerous small moons, many of which we have not yet glimpsed.\r\n<h2>The Neptune System<\/h2>\r\n<strong>Neptune<\/strong> has 14 known moons. The most interesting of these is <strong>Triton<\/strong>, a relatively large moon in a retrograde orbit\u2014which is unusual. Triton has a very thin atmosphere, and active eruptions were discovered there by Voyager in its 1989 flyby. To explain its unusual characteristics, astronomers have suggested that Triton may have originated beyond the Neptune system, as a dwarf planet like Pluto. The rings of Neptune are narrow and faint. Like those of Uranus, they are composed of dark materials and are thus not easy to see.\r\n<div class=\"textbox key-takeaways\">\r\n<h3>Key Concepts and Summary<\/h3>\r\nThe four jovian planets are accompanied by impressive systems of moons and rings. Nearly 200 moons have been discovered in the outer solar system. Of the four ring systems, Saturn\u2019s is the largest and is composed primarily of water ice; in contrast, Uranus and Neptune have narrow rings of dark material, and Jupiter has a tenuous ring of dust.\r\n\r\n<\/div>","rendered":"<div class=\"textbox learning-objectives\">\n<h3>Learning Objectives<\/h3>\n<p>By the end of this section, you will be able to:<\/p>\n<ul>\n<li>Name the major moons of each of the jovian planets<\/li>\n<li>Describe the basic composition of each jovian planet\u2019s ring system<\/li>\n<\/ul>\n<\/div>\n<p>The rings and <strong>moons<\/strong> (see the moons in Figure 1)\u00a0of the outer solar system are not composed of the same materials as the mostly rocky objects in the inner solar system. We should expect this, since they formed in regions of lower temperature, cool enough so that large quantities of water ice were available as building materials. Most of these objects also contain dark, organic compounds mixed with their ice and rock. Don\u2019t be surprised, therefore, to find that many objects in the ring and moon systems are both icy and dark.<\/p>\n<p>Roughly a third of the moons in the outer solar system are in <em>direct<\/em> or regular orbits; that is, they revolve about their parent planet in a west-to-east direction and in the plane of the planet\u2019s equator. The majority are irregular moons that orbit in a <em>retrograd<\/em>e (east-to-west) direction or else have orbits of high eccentricity (more elliptical than circular) or high inclination (moving in and out of the planet\u2019s equatorial plane). These irregular moons are mostly located relatively far from their planet; they were probably formed elsewhere and subsequently captured by the planet they now orbit. (Perhaps the fact that they were not born locally will excuse their ill-mannered behavior.)<\/p>\n<div style=\"width: 710px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" class=\"\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/courses-images\/wp-content\/uploads\/sites\/1095\/2016\/11\/03155722\/OSC_Astro_12_01_SelectMoon.jpg\" alt=\"An image showing the moons of the solar system in comparison to the size of the Earth. Earth is pictured at the bottom right. At the top of the image the planets are labeled from left to right. Under\" width=\"700\" height=\"458\" data-media-type=\"image\/jpeg\" \/><\/p>\n<p class=\"wp-caption-text\"><strong>Figure 1: Moons of the Solar System. <\/strong> This image shows some selected moons of our solar system and their comparison to the size of Earth\u2019s Moon and Earth itself. (credit: modification of work by NASA)<\/p>\n<\/div>\n<h2>The Jupiter System<\/h2>\n<p><strong>Jupiter<\/strong> has 67 known moons (that\u2019s the number as we write) and a faint ring. These include four large moons\u2014<strong>Callisto<\/strong>, <strong>Ganymede<\/strong>, <strong>Europa<\/strong>, and <strong>Io<\/strong> (see <a href=\".\/chapter\/introduction-to-rings-moons-and-pluto\/\" target=\"_blank\" rel=\"noopener\">Figure 1 in Introduction to Rings, Moons, and Pluto<\/a>)\u2014discovered in 1610 by Galileo and therefore often called the <em>Galilean moons<\/em>. The smaller of these, Europa and Io, are about the size of our Moon, while the larger, Ganymede and Callisto, are about the same size as the planet Mercury. Most of Jupiter\u2019s moons are much smaller. The majority are in retrograde orbits more than 20 million kilometers from Jupiter; these are very likely small captured asteroids.<\/p>\n<h2>The Saturn System<\/h2>\n<p><strong>Saturn<\/strong> has at least 62 known moons in addition to a magnificent set of rings. The largest of the moons, <strong>Titan<\/strong>, is almost as big as Ganymede in Jupiter\u2019s system, and it is the only moon with a substantial atmosphere and lakes or seas of liquid hydrocarbons (such as methane and ethane) on the surface. Saturn has six other large regular moons with diameters between 400 and 1600 kilometers, a collection of small moons orbiting in or near the rings, and many captured strays similar to those of Jupiter. Mysteriously, one of Saturn\u2019s smaller moons, <strong>Enceladus<\/strong>, has active geysers of water being expelled into space.<\/p>\n<p>The rings of Saturn, one of the most impressive sights in the solar system, are broad and flat, with a few major and many minor gaps. They are not solid, but rather a huge collection of icy fragments, all orbiting the equator of Saturn in a traffic pattern that makes rush hour in a big city look simple by comparison. Individual ring particles are composed primarily of water ice and are typically the size of ping-pong balls, tennis balls, and basketballs.<\/p>\n<h2>The Uranus System<\/h2>\n<p>The ring and moon system of <strong>Uranus<\/strong> is tilted at 98\u00b0, just like the planet itself. It consists of 11 rings and 27 currently known moons. The five largest moons are similar in size to the six regular moons of Saturn, with diameters of 500 to 1600 kilometers. Discovered in 1977, the rings of Uranus are narrow ribbons of dark material with broad gaps in between. Astronomers suppose that the ring particles are confined to these narrow paths by the gravitational effects of numerous small moons, many of which we have not yet glimpsed.<\/p>\n<h2>The Neptune System<\/h2>\n<p><strong>Neptune<\/strong> has 14 known moons. The most interesting of these is <strong>Triton<\/strong>, a relatively large moon in a retrograde orbit\u2014which is unusual. Triton has a very thin atmosphere, and active eruptions were discovered there by Voyager in its 1989 flyby. To explain its unusual characteristics, astronomers have suggested that Triton may have originated beyond the Neptune system, as a dwarf planet like Pluto. The rings of Neptune are narrow and faint. Like those of Uranus, they are composed of dark materials and are thus not easy to see.<\/p>\n<div class=\"textbox key-takeaways\">\n<h3>Key Concepts and Summary<\/h3>\n<p>The four jovian planets are accompanied by impressive systems of moons and rings. Nearly 200 moons have been discovered in the outer solar system. Of the four ring systems, Saturn\u2019s is the largest and is composed primarily of water ice; in contrast, Uranus and Neptune have narrow rings of dark material, and Jupiter has a tenuous ring of dust.<\/p>\n<\/div>\n\n\t\t\t <section class=\"citations-section\" role=\"contentinfo\">\n\t\t\t <h3>Candela Citations<\/h3>\n\t\t\t\t\t <div>\n\t\t\t\t\t\t <div id=\"citation-list-363\">\n\t\t\t\t\t\t\t <div class=\"licensing\"><div class=\"license-attribution-dropdown-subheading\">CC licensed content, Shared previously<\/div><ul class=\"citation-list\"><li>Astronomy. <strong>Provided by<\/strong>: OpenStax CNX. <strong>Located at<\/strong>: <a target=\"_blank\" href=\"http:\/\/cnx.org\/contents\/2e737be8-ea65-48c3-aa0a-9f35b4c6a966@10.1\">http:\/\/cnx.org\/contents\/2e737be8-ea65-48c3-aa0a-9f35b4c6a966@10.1<\/a>. <strong>License<\/strong>: <em><a target=\"_blank\" rel=\"license\" href=\"https:\/\/creativecommons.org\/licenses\/by\/4.0\/\">CC BY: Attribution<\/a><\/em>. <strong>License Terms<\/strong>: Download for free at http:\/\/cnx.org\/contents\/2e737be8-ea65-48c3-aa0a-9f35b4c6a966@10.1.<\/li><\/ul><\/div>\n\t\t\t\t\t\t <\/div>\n\t\t\t\t\t <\/div>\n\t\t\t <\/section>","protected":false},"author":17,"menu_order":2,"template":"","meta":{"_candela_citation":"[{\"type\":\"cc\",\"description\":\"Astronomy\",\"author\":\"\",\"organization\":\"OpenStax CNX\",\"url\":\"http:\/\/cnx.org\/contents\/2e737be8-ea65-48c3-aa0a-9f35b4c6a966@10.1\",\"project\":\"\",\"license\":\"cc-by\",\"license_terms\":\"Download for free at http:\/\/cnx.org\/contents\/2e737be8-ea65-48c3-aa0a-9f35b4c6a966@10.1.\"}]","CANDELA_OUTCOMES_GUID":"","pb_show_title":"on","pb_short_title":"","pb_subtitle":"","pb_authors":[],"pb_section_license":""},"chapter-type":[],"contributor":[],"license":[],"class_list":["post-363","chapter","type-chapter","status-publish","hentry"],"part":359,"_links":{"self":[{"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/pressbooks\/v2\/chapters\/363","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/wp\/v2\/users\/17"}],"version-history":[{"count":6,"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/pressbooks\/v2\/chapters\/363\/revisions"}],"predecessor-version":[{"id":1727,"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/pressbooks\/v2\/chapters\/363\/revisions\/1727"}],"part":[{"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/pressbooks\/v2\/parts\/359"}],"metadata":[{"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/pressbooks\/v2\/chapters\/363\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/wp\/v2\/media?parent=363"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/pressbooks\/v2\/chapter-type?post=363"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/wp\/v2\/contributor?post=363"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-ncc-astronomy\/wp-json\/wp\/v2\/license?post=363"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}