Unit 2 Lesson 6 Small Bodies in the Solar System Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System Bigger Is Not Better Where are small bodies in the solar system? • Scientists estimate that there are up to a trillion small bodies in the solar system. They lack atmospheres and have weak surface gravity. • The largest of the small bodies, the dwarf planets, are found in regions known as the asteroid belt and Kuiper belt. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System Where are small bodies in the solar system? • The Kuiper belt is located beyond the orbit of Neptune. It contains Kuiper belt objects and comets. • Comets are also located in the Oort cloud, which is a region that surrounds the solar system and extends almost halfway to the nearest star. • Two other types of small bodies, asteroids and meteoroids, are located mostly between the orbits of Venus and Neptune. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What are dwarf planets? • A dwarf planet is a celestial body that orbits the sun and is round because of its own gravity. • A dwarf planet does not have the mass to have cleared other bodies out of its orbit around the sun. • Five dwarf planets have been identified: Ceres, Pluto, Eris, Haumea, and Makemake. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System KBOs What are Kuiper belt objects? • The Kuiper belt is a region of the solar system that begins just beyond the orbit of Neptune. • The Kuiper belt extends outward to about twice the orbit of Neptune, a distance of about 55 astronomical units (AU). Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What are Kuiper Belt objects? • A Kuiper belt object (KBO) is any of the minor bodies in the Kuiper belt. They are made of methane ice, ammonia ice, and water ice. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System Pluto: From Planet to KBO • Until 2006, Pluto was considered to be the ninth planet in the solar system. • Beginning in 1992, Kuiper belt objects began to be discovered beyond Neptune’s orbit, some of which had similar size and composition as Pluto. • In 2006, Pluto was redefined as a “dwarf planet” by the International Astronomical Union. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System Pluto: From Planet to KBO • Many large KBOs have satellites. • Pluto, the second-largest KBO, has Charon as its largest satellite. • Some KBOs and their satellites, such as Pluto and Charon, orbit each other. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System KBOs What do we know about comets? • A comet is a small body of ice, rock, and dust that follows a highly elliptical orbit around the sun. • All comets have a nucleus that is composed of ice and rock. Most comet nuclei are between 1 km and 10 km in diameter. • If a comet approaches the sun, solar radiation and heating cause the comet’s ice to change to gas. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What do we know about comets? • A coma is a spherical cloud of gas and dust that comes off the nucleus. • The ion tail of a comet is gas that has been ionized by the sun. This ion tail always points away from the sun. • A second tail made of dust and gas curves backward along the comet’s orbit. This dust tail can be millions of kilometers long. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What do we know about comets? • How does a comet change as it orbits the sun? Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What do we know about comets? • Collisions between objects in the Kuiper belt produce fragments that become short-period comets. • Short-period comets take fewer than 200 years to orbit the sun. • Short-period comets have short life spans. Every time a comet passes the sun, it may lose a layer as much as 1 m thick. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What do we know about comets? • Long-period comets come from the Oort cloud. They may take up to hundreds of thousands of years to orbit the sun. • The Oort cloud is a spherical region that surrounds the solar system. • Comets can form in the Oort cloud when two objects collide, or when the gravity of a nearby star sends an object into the inner solar system. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System On the Rocks What do we know about asteroids? • An asteroid is a small, irregularly shaped, rocky object that orbits the sun. • Most asteroids are located in the asteroid belt between the orbits of Mars and Jupiter. • The asteroid belt contains hundreds of thousands of asteroids, called main-belt asteroids. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What do we know about asteroids? • Groups of asteroids are also located in the orbits of Jupiter and Neptune (called Trojan asteroids) and in the Kuiper belt. • Some asteroids are called near-Earth asteroids. These asteroids cross the orbits of Earth and Venus. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What do we know about asteroids? • Where are most asteroids located in the solar system? Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What do we know about asteroids? • The composition of asteroids varies. • Some are rich in carbon. • Others are rocky, with cores of iron and nickel. • Some have a rocky core surrounded largely by ice. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What do we know about asteroids? • Some asteroids appear to be piles of rock loosely held together. • Others contain economic minerals such as gold, iron, nickel, cobalt, and platinum. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System Burned Out What do we know about meteoroids, meteors, and meteorites? • A meteoroid is a rocky body, ranging in size from that of a sand grain to that of a boulder, which travels through space. • A bright streak of light that results when a meteoroid burns up in Earth’s atmosphere is called a meteor. • A meteorite is a meteoroid that reaches Earth’s surface without burning up. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What do we know about meteoroids, meteors, and meteorites? • Meteoroids come from the asteroid belt, Mars, the moon, and comets. • Most meteoroids that enter Earth’s atmosphere do not reach Earth’s surface. Many explode in the upper atmosphere; others skip back into space. • Large meteoroids that enter Earth’s lower atmosphere or strike Earth’s surface can be destructive. Copyright © Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 6 Small Bodies in the Solar System What do we know about meteoroids, meteors, and meteorites? • Meteorites can be divided into three general groups. Stony meteorites, made of silicate minerals, are the most common form. • Iron meteorites, composed of iron and nickel, form a much smaller group of meteorites. • Stony-iron meteorites, composed of silicate minerals, iron, and nickel, are the rarest group of meteorites. 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