To determine the distance to the stars, we need to use the parallax formula:
distance = 1 / (parallax angle in arcseconds)
Let's use this formula to calculate the distances to the two stars:
distance to star 1 = 1 / 0.11 arcsec = 9.09 parsecs
distance to star 2 = 1 / 0.13 arcsec = 7.69 parsecs
Now, we need to determine the distance between the two stars. We can use trigonometry to do this. The angle between the two stars is 5 degrees, which is equivalent to 300 arcminutes or 18,000 arcseconds. Since we know the distance to each star, we can use the tangent function to calculate the distance between them:
tan(5 degrees/2) = (distance to star 1 - distance to star 2) / distance between stars
Simplifying this equation, we get:
distance between stars = (distance to star 1 - distance to star 2) / 2 / tan(5 degrees/2)
Plugging in the values we calculated earlier, we get:
distance between stars = (9.09 parsecs - 7.69 parsecs) / 2 / tan(5 degrees/2) = 5.57 parsecs
Finally, we convert this distance to light-years:
1 parsec = 3.26 light-years
So, the distance between the two stars is:
distance between stars = 5.57 parsecs * 3.26 light-years/parsec = 18.15 light-years
Therefore, the two stars are about 18.15 light-years apart from each other.