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Download 23.3 The Outer Planets
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23.3 The Outer Planets Pluto: Planet X Pluto’s orbit is highly eccentric, causing it to occasionallyy travel inside the orbit of Neptune, where it resided from 1979 through February 1999. 23.4 Minor Members of the Solar System Asteroids: Microplanets An asteroid is a small, rocky body whose diameter can range g from a few hundred kilometers to less than a kilometer. Most asteroids lie between the orbits of Mars and Jupiter. They have orbital periods of three to six years. Irregular Orbits of Asteroids 23.4 Minor Members of the Solar System Comets Comets are small bodies made of rocky and metallic p pieces held together g by y frozen gases. Comets generally revolve about the sun in elongated orbits. 23.4 Minor Members of the Solar System Comets Coma • A coma is the fuzzy, gaseous component of a comet’s head. • A small glowing nucleus with a diameter of only a few kilometers can sometimes be detected within a coma. As comets approach the sun, some, but not all, develop a tail that extends for millions off kilometers. Comet’s Tail Points Away from the Sun 23.4 Minor Members of the Solar System Comets Kuiper Belt • Like the asteroids in the inner solar system, y most Kuiper belt comets move in nearly circular orbits that lie roughly in the same plane as the planets. Oort Cloud • Comets with long orbital periods appear to be distributed d st buted in all a directions d ect o s from o tthe e su sun,, forming o g a spherical shell around the solar system called the Oort cloud. 23.4 Minor Members of the Solar System Comets Halley’s Comet • The most famous short-period p comet is Halley’s y comet. Its orbital period is 76 years. 23.4 Minor Members of the Solar System Meteoroids A meteoroid is a small, solid particle that travels through g space. p A meteor is the luminous phenomenon observed when a meteoroid enters Earth’s atmosphere and burns up, popularly called a shooting star. A meteorite t it is i any portion ti off a meteoroid t id that reaches Earth’s surface. 23.4 Minor Members of the Solar System Meteoroids Most meteoroids originate from any one of the following g three sources: ((1)) interplanetary debris that was not gravitationally swept up by the planets d i th during the fformation ti off the th solar l system, t (2) material from the asteroid belt, or (3) the solid remains of comets that once traveled near Earth’s orbit. Meteor Shower These meteorites broke off from the Comet Swift-Tuttle Swift Tuttle Major Meteor Showers