The formula to calculate the Absolute Magnitude (M) is:
\[ M = m + 5 \cdot (\log(p) + 1) \]
Where:
Absolute magnitude is a measure of the intrinsic brightness of a celestial object. It is defined as the apparent magnitude the object would have if it were located at a standard distance of 10 parsecs (32.6 light years) from the observer.
Let's assume the following values:
Using the formula to calculate the Absolute Magnitude:
\[ M = 5.0 + 5 \cdot (\log(0.1) + 1) = 5.0 + 5 \cdot (-1 + 1) = 5.0 \]
The Absolute Magnitude is 5.0.
