The distance of the Sun from earth is \( 1.5 \times 10^{11} \, \text{m} \) and its angular diameter is \( (2000) \, s \) when observed from the earth. The diameter of the Sun will be:
\( 2.45 \times 10^{10} \, \text{m} \)
\( 1.45 \times 10^{10} \, \text{m} \)
\( 1.45 \times 10^{9} \, \text{m} \)
\( 0.14 \times 10^{9} \, \text{m} \)