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Acceleration Due to Gravity


Acceleration due to gravity is the rate at which an object speeds up as it falls freely toward the Earth due to the force of gravity. It is represented by the symbol ‘g’, and its standard value on Earth is approximately 9.8 m/s². This means that for every second an object is in free fall, its velocity increases by 9.8 meters per second.


The SI unit of acceleration due to gravity is meters per second squared (m/s²). This unit expresses how quickly an object’s velocity changes while falling under the influence of gravity.


The value of g can vary slightly based on location — it is a bit lower at the equator and higher at the poles due to Earth's shape and rotation.


This concept is fundamental in understanding free fall, projectile motion, and satellite orbits, making it an essential part of physics and real-world applications.


Revolutions per Second (r/s)


Revolutions per second (r/s) is a unit of angular velocity that measures how many complete rotations or revolutions an object makes in one second. One revolution corresponds to a full 360-degree turn or 2π2\pi radians. This unit is commonly used to describe very fast rotational speeds in machinery, motors, turbines, and other high-speed rotating systems. For example, a motor spinning at 50 r/s completes 50 full rotations every second. Revolutions per second provide a clear and precise measure of rapid rotational motion, useful in physics, engineering, and technology fields where high-speed rotation is involved. It also facilitates easy conversion to other angular velocity units like radians per second or revolutions per minute.



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