Detailed Summary
In this section, we delve into the calculation of gravitational acceleration, commonly referred to as g
. Gravitational acceleration is a crucial concept in physics as it describes the rate at which objects accelerate towards the Earth due to gravitational attraction. The value of g
is typically approximated as 9.8 m/s²
near the Earth's surface, but it can vary based on geographical location (greater at the poles than the equator) and altitude.
To compute g
, we utilize the equation derived from Newton's Law of Gravitation:
$$ g = \frac{G \times M}{R^2} $$
Where:
- G is the universal gravitational constant (approximately 6.67 × 10^-11 N m²/kg²
),
- M is the mass of the Earth (6 × 10^24 kg
), and
- R is the radius of the Earth (6.4 × 10^6 m
).
By substituting these values into the equation, we arrive at the calculated value of g
, which is approximately 9.8 m/s²
. This section emphasizes the universality of gravitational acceleration and its relevance to the motion of objects near the Earth's surface.