The gravity of Earth, denoted by g, is the net acceleration that is imparted to objects due to the combined effect of gravitation and the centrifugal force. It is a vector quantity, whose direction coincides with a plumb bob and strength or magnitude is given by the norm {\displaystyle g=\|{\mathit {\mathbf {g} }
The gravity of Earth, which is denoted by g, refers to the acceleration that the Earth imparts to objects on or near its surface. In SI units this acceleration is measured in metres per second squared (in symbols, m/s2) or equivalently in newtons per kilogram (N/kg).
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The gravity of Earth, denoted by g, is the net acceleration that is imparted to objects due to the combined effect of gravitation and the centrifugal force. It is a vector quantity, whose direction coincides with a plumb bob and strength or magnitude is given by the norm {\displaystyle g=\|{\mathit {\mathbf {g} }
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