To solve this problem, we need to determine the position of a fourth body of mass \(4\, \text{kg}\) such that the resultant gravitational force on the \(2\, \text{kg}\) body placed at the centroid \(G\) of the equilateral triangle \(ABC\) is zero.
First, consider the gravitational force exerted by the masses at points \(A\), \(B\), and \(C\) on the \(2\, \text{kg}\) mass at \(G\). The masses at \(A\) and \(B\) are both \(8\, \text{kg}\) and are located \(1\, \text{m}\) away from \(G\).
The gravitational force \(F\) between two masses \(m_1\) and \(m_2\) at a distance \(r\) is given by:
\(F = \frac{G \cdot m_1 \cdot m_2}{r^2}\)
Where \(G\) is the gravitational constant. However, for this analysis, we are only interested in the relative magnitudes of the forces as \(G\) will cancel out, ultimately.
Step 1: Calculate the force exerted by masses at \(A\) and \(B\)
The force due to the \(8\, \text{kg}\) masses at \(A\) and \(B\) on the \(2\, \text{kg}\) mass at \(G\) will point directly towards \(A\) and \(B\), respectively. Since \(A\) and \(B\) are symmetrically placed relative to \(G\), their horizontal components will cancel each other out.
Let's denote \(F_{AG}\) and \(F_{BG}\) as the forces on \(G\) due to masses at \(A\) and \(B\):
\(F_{AG} = F_{BG} = \frac{8 \cdot 2}{1^2} = 16 \, G \cdot \text{N} \cdot m^2/kg^2\)
Both forces are directed symmetrically and thus their vertical components add up, contributing no net force horizontally which aligns in the direction of \(CG\).
Step 2: Determine the position of the \(4\, \text{kg}\) mass
The force due to the \(4\, \text{kg}\) mass, placed at a point \(P\) on line \(CG\), should cancel out the resultant of \(F_{AG}\) and \(F_{BG}\) on the \(2\, \text{kg}\) body.
Since \(F_{AG}\) and \(F_{BG}\) only have a net vertical component, place \(P\) such that the force \(F_{PG}\) counteracts this resultant force.
The force due to \(4\, \text{kg}\) mass at \(P\) is:
\(F_{PG} = \frac{4 \cdot 2}{PG^2}\)
Equating the forces in the direction along \(CG\):
\(16 = 8 \cdot \frac{1}{PG^2}\)
\(PG = \frac{1}{\sqrt{2}} \, \text{m}\)
Therefore, the correct position of the \(4\, \text{kg}\) mass is at a point \(P\) on the line \(CG\) such that \(PG = \frac{1}{\sqrt{2}}\) m\).

The driver sitting inside a parked car is watching vehicles approaching from behind with the help of his side view mirror, which is a convex mirror with radius of curvature \( R = 2 \, \text{m} \). Another car approaches him from behind with a uniform speed of 90 km/hr. When the car is at a distance of 24 m from him, the magnitude of the acceleration of the image of the side view mirror is \( a \). The value of \( 100a \) is _____________ m/s\(^2\).
In a practical examination, the following pedigree chart was given as a spotter for identification. The students identify the given pedigree chart as 
The laws of motion, which are the keystone of classical mechanics, are three statements that defined the relationships between the forces acting on a body and its motion. They were first disclosed by English physicist and mathematician Isaac Newton.
Newton’s 1st law states that a body at rest or uniform motion will continue to be at rest or uniform motion until and unless a net external force acts on it.
Newton's 2nd law of motion deals with the relation between force and acceleration. According to the second law of motion, the acceleration of an object as built by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object.
Newton's 3rd law of motion states when a body applies a force on another body that there is an equal and opposite reaction for every action.