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Astronomy Our Solar System Chapter 29.4 Formation of our Solar System Stars and planets form from clouds of gas and dust, called interstellar clouds, which exist in space between the stars. A Collapsing Interstellar Cloud Our solar system may have begun when interstellar gas started to condense as a result of gravity. Sun and Planet Formation The disk of dust and gas that formed the Sun and planets is known as the solar nebula. GROWTH OF OBJECTS – Condensed material started to accumulate and merge together to form larger bodies. PLANETESIMALS – Planetesimals are solid bodies, reaching hundreds of kilometers in diameter, that formed as smaller particles collided and stuck together. ASTEROID BELT – Between Jupiter and Mars – Jupiter’s gravitational force prevented them from merging to form a planet. ASTEROIDS Orbit the Sun within the planetary orbits that are leftovers from the formation of the solar system. PIECES OF ASTEROIDS A meteoroid is an asteroid that falls toward Earth and enters Earth’s atmosphere. A meteor is the streak of light produced when a meteoroid burns up in Earth’s atmosphere. A meteorite is part of a meteoroid, that does not completely burn up, that collides with the ground. COMETS small, icy bodies that orbits around the Sun and are remnants from solar system formation. made of ice and rock