Calculating Absolute Magnitude of a Star - Red's Help

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To calculate the absolute magnitude of a star with a parallax angle of 10 milliarcseconds and an apparent magnitude of V=10.2, the distance in parsecs can be determined using the formula d=1/pi. The provided formula M=v - 5logd - 5 + A can be utilized once the distance is established. The discussion highlights confusion regarding the distance being less than that of the Sun, suggesting a need for clarification on the calculations. Participants indicate that this topic may be more suitable for a homework section. Understanding these concepts is crucial for accurately determining a star's absolute magnitude.
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Can anyone help me get my head around this one?
A star with a parallax angle of pi = 10 millisecs and has apparent magnitude of V= 10.2
How can I determine absolute magnitude:
I have the formula M=v -5logd -5 +A which can be ignored.
d=1/pi but I am always determining d which is less than that of the sun's distance!
Thanks Red
 
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10 m'' = .010" , d=\frac{1}{p''}, where d is the distance in parsecs. Solve for d. This should probably be in the homework section.
 
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