SUMMARY
The gravity on Mars is approximately 38% that of Earth's, calculated primarily through the observation of its moons, Deimos and Phobos. The mass of Mars was inferred from these observations long before any spacecraft landed on the planet. The Viking 1 and Viking 2 missions provided direct measurements of Martian surface gravity, confirming it to be around 3.71 m/s². Additionally, gravitational calculations utilize the formula g = -GM/r², where G is the Gravitational Constant and M is the mass of Mars.
PREREQUISITES
- Understanding of gravitational physics, specifically Newton's laws of motion.
- Familiarity with orbital mechanics and celestial observations.
- Knowledge of the Gravitational Constant (G) and its implications in calculations.
- Awareness of Mars exploration missions, particularly Viking 1 and Viking 2.
NEXT STEPS
- Research the gravitational effects of celestial bodies using Newton's equations.
- Study the methodologies of Mars exploration missions, focusing on Viking 1 and Viking 2.
- Learn about the significance of the Gravitational Constant (G) in astrophysics.
- Explore the mathematical derivation of gravitational force and its applications in planetary science.
USEFUL FOR
Astronomers, astrophysicists, students of physics, and anyone interested in planetary science and the exploration of Mars.