You will need to use the table that have provided to complete the assignment.

Table 10.1 Escape Speeds at the surface of bodies in the solar system Astronomical Body Mass (Earth masses) Radius (Earth Radli) Escape Speed (km/S0 Sun 333.000 109 618 Sun (at a distance of earth's orbit) 23,500 42.2 Jupiter 318 11 59.5 Saturn 95.2 9.1 35.5 Neptune 17.1 3.9 23.5 Uranus 14.5 4.0 21.3 Earth 1.00 1.00 11.2 Venus 0.82 0.95 10.4 Mars 0.11 0.53 5.0 Mercury 0.055 0.38 4.3 Moon0. 0123 0.27 2.4 Escape speed from any planet or given body by p= Square root of 2MG/d where G is the universal gravitational constant. M is the mass of the attracting body and d is the distance from it center. (at the surface of the body s is simply the radius of the body). -------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------- In order to find escape velocities for the given exoplanets, enter the appropriate values of their masses and radii in unit of Earth's mass and Earth's radius in the provided template. Then, the escape velocity and gravitational acceleration will be automatically evaluated. In the case of our major planets, insert data from Table 10.1 above.