Variation of g — Core Principles
Core Principles
The acceleration due to gravity, 'g', is the acceleration experienced by objects due to Earth's gravitational pull, with an average value of at the surface. However, 'g' is not constant and varies significantly with location.
As we move to higher altitudes (height 'h' above the surface), 'g' decreases because the distance from the Earth's center increases. The formula is , which approximates to for small 'h'.
Similarly, 'g' also decreases as we go deeper (depth 'd' below the surface) because only the mass of the Earth within the inner sphere contributes to the gravitational pull. The formula for depth is , becoming zero at the Earth's center.
Finally, the Earth's rotation causes 'g' to vary with latitude (). The centrifugal effect of rotation reduces the effective 'g' most at the equator () and least (zero effect) at the poles (), given by .
Understanding these three primary variations is essential for NEET.
Important Differences
vs Variation of g with Altitude vs. Depth
| Aspect | This Topic | Variation of g with Altitude vs. Depth |
|---|---|---|
| Formula (for small changes) | $g_h approx g(1 - 2h/R)$ | $g_d = g(1 - d/R)$ |
| Rate of decrease (for small changes) | Decreases approximately as $2gh/R$ | Decreases approximately as $gd/R$ |
| Maximum value | At Earth's surface ($h=0$) | At Earth's surface ($d=0$) |
| Minimum value | Approaches zero as $h o infty$ | Zero at Earth's center ($d=R$) |
| Reason for decrease | Increased distance from Earth's center, weakening gravitational pull. | Decreased effective mass of Earth pulling the object (mass above cancels out). |