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Nebular Hypothesis

Published on Nov 19, 2015

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PRESENTATION OUTLINE

1.

THE SOLAR NEBULA

BY MAFTUNA ISOEVA
2.

The younger solar nebula begins to collapse.

Photo by NASA Goddard Photo and Video
3.

The solar nebula rotates, flattens and becomes warmer near the center.

Photo by Cyrus II
4.

Planetesimals begin to form within swirling disk.

Photo by NASA Goddard Photo and Video
5.

As the large planetesimals grow in size, their gravity attracts more gas and dust.

Photo by Camilo Forero Pulido
6.

Smallest planetesimals collide with the large ones, and planets begin to grow.

7.

A star is born, and the remaining gas and dust are blown out of the new solar system.

8.

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Maftuna Isoeva

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