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STAR DEATH

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INSIDE THE SUN

SUN's SURFACE

SUN's ATMOSPHERE

ECLIPSES OF THE SUN

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MEASURE OF THE STARS

VARIABLE STARS

HOW FAR ARE THE STARS?

PROPERTIES OF STARS

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STARS DO NOT LIVE FROEVER. A time comes when the supply of hydrogen dwindles and the nuclear reactions in the core die down. but instead of fading away, the star now balloons out to become a brilliant red giant maybe a hundred times its former diameter. More massive stars become powerful supergiants, bright enough to be seen across intergalactic space. This transformation happens because, deep within its core, the star has tapped a new source of energy, helium, which can keep it shining for a while longer.

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