The Core Principle of Gravitational Acceleration
In a vacuum, all objects fall towards the Earth at the same rate of acceleration, irrespective of their mass or composition. This fundamental principle, famously attributed to Galileo Galilei, disproved earlier notions that heavier objects inherently fall faster. The constant acceleration due to gravity (g) near Earth's surface is approximately 9.8 m/s² for all objects in free fall.
Newton's Laws and Mass Cancellation
This phenomenon is explained by combining Newton's Law of Universal Gravitation and Newton's Second Law of Motion. The gravitational force (F_g) attracting an object to Earth is directly proportional to its mass (m) and Earth's mass, and inversely proportional to the square of the distance between their centers. Newton's Second Law states that acceleration (a) is equal to force (F) divided by mass (m). When these laws are applied to falling objects, the object's own mass term cancels out, demonstrating that its acceleration in free fall is independent of its mass.
A Practical Example: The Feather and the Bowling Ball
Imagine dropping a feather and a bowling ball simultaneously. In typical atmospheric conditions, the bowling ball hits the ground first due to significant air resistance acting on the feather. However, if this experiment is conducted in a vacuum chamber, both the feather and the bowling ball will strike the ground at precisely the same instant. This vivid demonstration illustrates the mass-independent nature of gravitational acceleration.
The Role of Air Resistance and Other Factors
While gravitational acceleration is constant for all objects, real-world observations are often affected by other forces. Air resistance (or drag) is the primary reason objects of different shapes and densities appear to fall at varying rates. Factors such as an object's shape, surface area, and velocity influence the magnitude of air resistance, causing lighter or broader objects to experience greater deceleration in an atmosphere. In space, far from gravitational bodies and atmospheres, objects simply maintain their state of motion.