Star Definitions

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Alexander Brown        4W        Physics

Star Definitions

  1. Red giants: although the core of a star gradually shrinks as it exhausts its hydrogen supply, the star itself begins expanding. It resorts to burning the hydrogen in a shell around its helium core, which inflates the outer layers of its atmosphere. Eventually, the star expands into a red giant, possibly attaining a diameter from 10 to 1,000 times the diameter of the Sun. For example, in its red giant stage, the Sun will expand to the size of the orbit of Earth or beyond and become 2,000 times brighter than it is now. The shrinking core increases the star's internal pressure. The increase in pressure makes the star's temperature increase again until it is hot enough to trigger nuclear reactions between previously inert helium nuclei present in the star. This new series of nuclear reactions releases more energy and the star's core stops contracting. At this point, the star's outer atmosphere begins to contract.
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  1. White Dwarf: when a low- to medium-mass star exhausts the nuclear fuel in its core, it collapses under the gravitational pressure of its own weight into an extremely compact, dense star known as a white dwarf. As a more massive star collapses to a white dwarf, it blows off more than half of its outer layer into space as a planetary nebula—gas and dust that may provide building material for planets in newly forming solar systems. Although dimmer than the original star, a white dwarf will continue radiating light for several billion years from heat energy trapped in ...

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