Final answer:
The average kinetic energy of hydrogen atoms on the Sun's surface can be calculated using the equation KE = (3/2) kT, where KE is the average kinetic energy, k is the Boltzmann constant, and T is the temperature in Kelvin.
Step-by-step explanation:
The average kinetic energy of hydrogen atoms on the Sun's surface can be calculated using the equation KE = (3/2) kT, where KE is the average kinetic energy, k is the Boltzmann constant (1.38 x 10-23 J/K), and T is the temperature in Kelvin. Since the surface temperature of the Sun is approximately 5500°C, we need to convert it to Kelvin. The conversion formula is K = °C + 273.15. Therefore, the surface temperature of the Sun in Kelvin is (5500 + 273.15) K = 5773.15 K.
Plugging in the values into the equation, KE = (3/2) x (1.38 x 10-23 J/K) x 5773.15 K = 1.50 x 10-21 J.
Therefore, the correct answer is option a) (1.50 x 10-21 J).