intensity of a star is inversely depends on the square of the distance from the star
we can say it is given as
![\frac{I_1}{I_2} = \frac{r_2^2}{r_1^2}](https://tex.z-dn.net/?f=%5Cfrac%7BI_1%7D%7BI_2%7D%20%3D%20%5Cfrac%7Br_2%5E2%7D%7Br_1%5E2%7D)
here we know that
![\frac{I_1}{I_2} = 36 times](https://tex.z-dn.net/?f=%5Cfrac%7BI_1%7D%7BI_2%7D%20%3D%2036%20times)
also we know that
![r_1 = 10 Ly](https://tex.z-dn.net/?f=r_1%20%3D%2010%20Ly)
now we will have
![\frac{I_1}{I_2} = \frac{r_2^2}{r_1^2}](https://tex.z-dn.net/?f=%5Cfrac%7BI_1%7D%7BI_2%7D%20%3D%20%5Cfrac%7Br_2%5E2%7D%7Br_1%5E2%7D)
![36 = \frac{r_2^2}{10^2}](https://tex.z-dn.net/?f=36%20%3D%20%5Cfrac%7Br_2%5E2%7D%7B10%5E2%7D)
![r_2 = 60 Ly](https://tex.z-dn.net/?f=r_2%20%3D%2060%20Ly)
so other star is at distance 60 Light years
Answer:
Explanation:
When the pendulum falls freely the net acceleration due to gravity is zero.
As we know that the time period of simple pendulum is inversely proportional to the square root of acceleration due to gravity, thus the time period becomes infinity.
In a series circuit, the sum of the voltages consumed by each individual resistance is equal to the source voltage. ... In a parallel circuit, the voltage across each of the components is the same, and the total current is the sum of the currents flowing through each component.