Answer:
B(A)100=B(B), the star A is 100 times fainter than star B.
Explanation:
Brightness of the star is defined by the formula,
![B=\frac{L}{4\pi d^{2}}](https://tex.z-dn.net/?f=B%3D%5Cfrac%7BL%7D%7B4%5Cpi%20d%5E%7B2%7D%7D)
Here, L is the luminosity and d is the distance.
For star A, the distance is 10d. The brightness of star A.
![B(A)=\frac{L}{4\pi (10d)^{2}}](https://tex.z-dn.net/?f=B%28A%29%3D%5Cfrac%7BL%7D%7B4%5Cpi%20%2810d%29%5E%7B2%7D%7D)
For star B, the distance is d. The brightness of star B.
![B(B)=\frac{L}{4\pi d^{2}}](https://tex.z-dn.net/?f=B%28B%29%3D%5Cfrac%7BL%7D%7B4%5Cpi%20d%5E%7B2%7D%7D)
Now according to the question luminosity of two stars is equal.
Therefore,
![B(A){4\pi (10d)^{2}}=B(B){4\pi (d)^{2}}\\B(A)100=B(B)](https://tex.z-dn.net/?f=B%28A%29%7B4%5Cpi%20%2810d%29%5E%7B2%7D%7D%3DB%28B%29%7B4%5Cpi%20%28d%29%5E%7B2%7D%7D%5C%5CB%28A%29100%3DB%28B%29)
So, star B is 100 times brighter than star A.
Therefore the star A is 100 times fainter than star B.