Gravitational acceleration is the acceleration of an object caused by the force of gravity. It is a fundamental concept in physics that describes how quickly an object's velocity changes due to gravitational attraction. On Earth's surface, this acceleration is approximately 9.8 m/s² (often rounded to 10 m/s²), but it can vary depending on factors such as altitude and the planet's local density.
The gravitational acceleration is given by Newton's law of universal gravitation:
\[ g = \frac{GM}{r^2} \]
Where:
Let's calculate the gravitational acceleration on the surface of Earth:
Let's visualize the gravitational acceleration on Earth:
This diagram illustrates:
Understanding gravitational acceleration is crucial in various fields, including physics, astronomy, and engineering. It helps explain phenomena such as orbital mechanics, tides, and the behavior of objects in free fall.
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