History of the Universe

History of the Universe eBook. 398 pages, 300 illustrations only $2.99

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Solar Wind

Protons and electrons boil off the surface of stars, like the Sun, and stream out past any nearby planets, such as the Earth.

Here they meet the planetís magnetic field, and are forced by it to move to the poles. When they get down to the atmosphere they ionize the gases, which then emit radiation. This is the source of the aurorae.

When the solar wind meets a comet, it pushes the gases which the comet releases away from the star, so creating the cometís tail.

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History of the Universe eBook
History of the Universe eBook
Only $2.99

Written by Wyken Seagrave
Copyright © 2017 Penny Press Ltd