Answer:M ≈ 1.44 x 10^24 kg
Explanation: We can use Newton's law of universal gravitation to solve this problem. The formula is:
F = (G * M * m) / r^2
The formula represents Newton's law of universal gravitation, relating the gravitational force (F) between two objects to their masses (M and m) and the distance between them (r).
Where:
F = Gravitational force between the satellite and the planet (120 N in this case)
G = Gravitational constant (approximately 6.67 x 10^-11 N m^2/kg^2)
M = Mass of the planet (unknown)
m = Mass of the satellite (450 kg)
r = Distance between the center of the planet and the satellite (4.0 x 10^6 m)
M = (F * r^2) / (G * m)
M = (120 N * (4.0 x 10^6 m)^2) / (6.67 x 10^-11 N m^2/kg^2 * 450 kg)