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Template: Convert/list of units/force. 6 languages. ... N oz-f; N ozf; millinewton: mN mN 1.0 ... g-f g f: 1.0 g f (9.8 mN; 0.035 ...
The standard acceleration of gravity or standard acceleration of free fall, often called simply standard gravity and denoted by ɡ 0 or ɡ n, is the nominal gravitational acceleration of an object in a vacuum near the surface of the Earth.
The g-force acting on a stationary object resting on the Earth's surface is 1 g (upwards) and results from the resisting reaction of the Earth's surface bearing upwards equal to an acceleration of 1 g, and is equal and opposite to gravity. The number 1 is approximate, depending on location.
The gravitational constant appears in the Einstein field equations of general relativity, [4] [5] + =, where G μν is the Einstein tensor (not the gravitational constant despite the use of G), Λ is the cosmological constant, g μν is the metric tensor, T μν is the stress–energy tensor, and κ is the Einstein gravitational constant, a ...
The gravity g′ at depth d is given by g′ = g(1 − d/R) where g is acceleration due to gravity on the surface of the Earth, d is depth and R is the radius of the Earth. If the density decreased linearly with increasing radius from a density ρ 0 at the center to ρ 1 at the surface, then ρ(r) = ρ 0 − (ρ 0 − ρ 1) r / R, and the ...
oz 1.0 oz (28 g) oz g; drachm: drachm (none) 1.0 drachm (1.8 g) drachm: dram (none) grain: gr gr equivalent to the troy grain 1.0 gr (0.065 g) Troy: troy ounce: ozt ozt 1.0 ozt (1.1 oz; 31 g) other: carat: carat (none) 1.0 carat (0.20 g)
Gravitational acceleration is the rate at which an object accelerates due to the gravitational force of a massive body.
The standard gravitational parameter μ of a celestial body is the product of the gravitational constant G and the mass M of that body. For two bodies, the parameter may be expressed as G ( m 1 + m 2 ) , or as GM when one body is much larger than the other: μ = G ( M + m ) ≈ G M . {\displaystyle \mu =G(M+m)\approx GM.}