Well, let's see:Force of gravity = G M1 M2 / R2So G = (force) x (distance)2 / (mass)2 = (M L / T2) x (L2) / (M2) = (M L3) / (M2 T2) =(Length)3 (Mass)-1(Time)-2
You have to divide by a trillion. So x g/m2 is 0.000000000001x g/um2
Assuming you mean 12 Square Meters (m2)12 m2 x 10.76391 = Answer 129.16692 Sq Ft
Square Metre ...... eg 3m2 = 3 square metres
Law of Gravity: Fg = G(m1*m2)/r^2
The unit "g over m2" is not an SI unit for density. SI unit for density is kg/m3 or g/cm3 or g/mL, which all represent mass per unit volume. The unit "g over m2" represents mass per unit area, not mass per unit volume.
The force, written as an equation, is:F = G (m1)(m2) / r2, whereF is the Force between the massesG is the gravitational constant (~= 6.674 x 10-11 N m2/kg2)m1 is one of the massesm2 is the other massr is the distance between the masses (center to center)Take the formula, and solve for r (I'll show the steps): Fold = G (m1)(m2) / r2.(r2)(Fold)= G (m1)(m2)(r2)= G (m1)(m2) / (Fold)r= √ [ G (m1)(m2) / (Fold) ]Plug the formula into itself, but remember, r = 3r (it tripled).Fnew= G (m1)(m2) / (3r)2.Fnew= G (m1)(m2) /(3√ [ G (m1)(m2) / (Fold) ])2.Fnew=G (m1)(m2)/(32G (m1)(m2) / (Fold) )
85 g / m2
the unit is : g/m2
The equation for calculating it would be g = G (m1) (m2) / (radius or distance ^2) where g = gravitational attraction, G is constant of universal gravitation, and m1 and m2 are the masses of the two objects
The gravitational constant, denoted as G, is calculated by measuring the force of gravity between two objects, their masses, and the distance between them. The formula to calculate G is F (G m1 m2) / r2, where F is the force of gravity, m1 and m2 are the masses of the objects, and r is the distance between them. By rearranging the formula, G can be calculated as G (F r2) / (m1 m2).
What is?? F = G m1 m2 / d2
What is?? F = G m1 m2 / d2
The force between two massess m1 and m2 is given by F = G m1 m2 / r^2 G is gravitational constant. r is the distance between the masses.
G=m1*m2/d^2
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weight, w = G * m1 * m2 / r^2, where G = the universal gravitational constant, m1 = the mass of the object, m2 = the mass of the earth, and r = the separation between the center of gravity of the object and that of the earth. w1 = G * m1 * m2 /(r1^2) -- > the weight when r = r1 w2 = G * m1 * m2 /(r2^2) -- > the weight when r = r2 Given: r2 = 4 * r1 w2 = G * m1 * m2 /(16 r1^2) = w1 / 16 Hence, the object will be 16 times lighter when it is situated 4 times farther away.