Estimate the pressure at the center of the sun

Reference no: EM13523614

To a first approximation, the Sun consists of a gas of equal numbers of protons and electrons. The temperature at the center of the Sun is about 10^7 K, and the density of the Sun is about 1x10^5 kg/m3. Because the temperature is so high, the protons and electrons are separate particles (rather than being joined together to form hydrogen atoms).

(a) Estimate the pressure at the center of the Sun.

Reference no: EM13523614

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