Answer:
T₂ = 123.9 N,  θ = 66.2º
Explanation:
To solve this exercise we use the law of equilibrium, since the diaphragm does not appear, let's use the adjoint to see the forces in the system.
The tension T1 = 100 N, we create a reference frame centered on the pole
X axis
        T₁ₓ -  = 0
 = 0
         T_{2x}= T₁ₓ
Y axis y
       T_{1y} + T_{2y} - 200N = 0
       T_{2y} = 200 -T_{1y}
let's use trigonometry to find the component of the stresses
          sin 60 = T_{1y} / T₁
          cos 60 = t₁ₓ / T₁
          T_{1y} = T₁ sin 60
          T1x = T₁ cos 60
          T_{1y}y = 100 sin 60 = 86.6 N
          T₁ₓ = 100 cos 60 = 50 N
for voltage 2 it is done in the same way
          T_{2y} = T₂ sin θ
          T₂ₓ = T₂ cos θ
we substitute
          
            T₂ sin θ= 200 - 86.6 = 113.4
            T₂ cos θ = 50              (1)
to solve the system we divide the two equations
            tan θ = 113.4 / 50
            θ = tan⁻¹ 2,268
            θ = 66.2º
we caption in equation 1
            T₂ cos 66.2 = 50
            T₂ = 50 / cos 66.2
            T₂ = 123.9 N
 
        
             
        
        
        
Answer:you in connections too?
Explanation:
 
        
                    
             
        
        
        
The answer is 0.025J.
W=1/2*k*x^2
W=1/2*20*0.050^2
W=0.025J
        
             
        
        
        
Solar power differ to fossil fuel power in that solar power is a much more optimal resource than fossil fuels
- Solar power; however provides much more energy than fossil fuel power
- Interestingly too, solar power resource can be used without releasing greenhouse gases compared to fossil fuels power
- Infact, solar energy is the most reliable 
<h3>What is renewable energy?</h3>
Renewable energy simply refers to energy that is not depleted when used. An example of such is solar power.
So therefore, solar power differ to fossil fuel power in that solar power is a much more optimal resource than fossil fuels
Learn more about renewable energy:
brainly.com/question/79953
#SPJ1
 
        
             
        
        
        
The masses of the object and the planet it's on, and the distance between their centers.