k Birth and Death of the Solar System Stages in the birth and death of the Solar System. 1 A globule forms from a giant molecular cloud. 2 The globule contracts gravitationally, forming a protoplanetary disc called the solar nebula. A bipolar outflow of charged particles may also be visible. 3 The stars and the planets form within the solar nebula. 4 In about 6 billon years from now, the Sun expands into a red giant, swallowing the inner two planets, and possibly Earth. 5 200 million years after that, the Sun sheds its outer layers to form a planetary nebula. 6 A few tens of thousands of years later, the planetary nebula dissipates, leaving behind the remaining planets orbiting the Suns original, exposed core now a white dwarf. Stock Photo - Afloimages
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Birth and Death of the Solar System Stages in the birth and death of the Solar System.  1  A globule forms from a giant molecular cloud.  2  The globule contracts gravitationally, forming a protoplanetary disc called the solar nebula. A bipolar outflow of charged particles may also be visible.  3  The stars and the planets form within the solar nebula.  4  In about 6 billon years from now, the Sun expands into a red giant, swallowing the inner two planets, and possibly Earth.  5  200 million years after that, the Sun sheds its outer layers to form a planetary nebula.  6  A few tens of thousands of years later, the planetary nebula dissipates, leaving behind the remaining planets orbiting the Sun s original, exposed core   now a white dwarf.
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Birth and Death of the Solar System

Stages in the birth and death of the Solar System. (1) A globule forms from a giant molecular cloud. (2) The globule contracts gravitationally, forming a protoplanetary disc called the solar nebula. A bipolar outflow of charged particles may also be visible. (3) The stars and the planets form within the solar nebula. (4) In about 6 billon years from now, the Sun expands into a red giant, swallowing the inner two planets, and possibly Earth. (5) 200 million years after that, the Sun sheds its outer layers to form a planetary nebula. (6) A few tens of thousands of years later, the planetary nebula dissipates, leaving behind the remaining planets orbiting the Sun's original, exposed core - now a white dwarf.

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