The centre of the Sun consists of gases whose average molecular weight is 2. If the density of the gases is 2.73 × 103 kg/m3 at a pressure of 1.12 × 109 atm, the temperature at the centre of the Sun is (assuming ideal behavior)

P= ρRT mThen, T=Pm ρR=1.12×109×2 2.73×103×0.0821 =107K

The centre of the Sun consists of gases whose average molecular weight is 2. If the density of the gases is 2.73 × 103 kg/m3 at a pressure of 1.12 × 109 atm, the temperature at the centre of the Sun is (assuming ideal behavior)

P= ρRT mThen, T=Pm ρR=1.12×109×2 2.73×103×0.0821 =107K

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The centre of the Sun consists of gases whose average molecular weight is 2. If the density of the gases is 2.73 × 10³kg/m³ at a pressure of 1.12 × 10⁹ atm, the temperature at the centre of the Sun is (assuming ideal behavior)

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$P = \frac{ρ R T}{m} T h e n, T = \frac{P m}{ρ R} = \frac{1.12 \times 10^{9} \times 2}{2.73 \times 10^{3} \times 0.0821} = 10^{7} K$

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The centre of the Sun consists of gases whose average molecular weight is 2. If the density of the gases is 2.73 × 103 kg/m3 at a pressure of 1.12 × 109 atm, the temperature at the centre of the Sun is (assuming ideal behavior)

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The centre of the Sun consists of gases whose average molecular weight is 2. If the density of the gases is 2.73 × 10³kg/m³ at a pressure of 1.12 × 10⁹ atm, the temperature at the centre of the Sun is (assuming ideal behavior)