To calculate the terminal velocity of a meteorite just before it hits Earth, Hanna needs the following information:
A typical meteorite’s weight, surface area, and coefficient of drag; air density close to Earth.
This is because terminal velocity can be calculated using the formula:
\[ v_t = \sqrt{\frac{2mg}{\rho C_d A}} \]
where \( v_t \) is the terminal velocity, \( m \) is the mass (or weight), \( g \) is the acceleration due to gravity, \( \rho \) is the air density, \( C_d \) is the coefficient of drag, and \( A \) is the surface area. Therefore, the second response option is the most complete and correct: a typical meteorite’s weight, surface area, and coefficient of drag; air density close to Earth.