Answer:
look it up im not a sheaperd sorry
Explanation:
 
        
                    
             
        
        
        
Answer:
  ≈ 2.1 R
 ≈ 2.1 R
Explanation:
The moment of inertia of the bodies can be calculated by the equation
      I = ∫ r² dm
For bodies with symmetry this tabulated, the moment of inertia of the center of mass
Sphere                = 2/5 M R²
 = 2/5 M R²
Spherical shell    = 2/3 M R²
 = 2/3 M R²
The parallel axes theorem allows us to calculate the moment of inertia with respect to different axes, without knowing the moment of inertia of the center of mass
     I =  + M D²
 + M D²
Where M is the mass of the body and D is the distance from the center of mass to the axis of rotation
 Let's start with the spherical shell, axis is along a diameter
      D = 2R
     Ic =  + M D²
 + M D²
     Ic = 2/3 MR² + M (2R)²
     Ic = M R² (2/3 + 4)
     Ic = 14/3 M R²
The sphere
     Is = + M [
 + M [ ²
²
     Is = Ic
     2/5 MR² + M  ² = 14/3 MR²
² = 14/3 MR²
      ² = R² (14/3 - 2/5)
² = R² (14/3 - 2/5)
      = √ (R² (64/15)
 = √ (R² (64/15)
      = 2,066 R
 = 2,066 R
 
        
             
        
        
        
Answer:
If the mass of one of the objects is tripled, then the force of gravity between them is tripled. ... Since gravitational force is inversely proportional to the square of the separation distance between the two interacting objects, more separation distance will result in weaker gravitational forces
 
        
                    
             
        
        
        
Answer:
Magnification m is 2.5cm
Explanation:
This problem bothers on lenses 
Given data 
Object distance u= 4cm
Height of object v= 10 cm
The problem is quite straightforward seeing that object and image distances are given 
We know that the magnification 
m= size of image/size of object 
m= v/u= 10/4 = 2. 5cm
What is a convex lens 
A convex lens is a type of lens that has the centre thicker than the ends, the thickness at the centre makes the lens surface to curve outward. Convex lens causes close light rays of light to converge at a point after refraction.