How Can You Determine the Sun’s Absolute Magnitude?

AI Thread Summary
The discussion focuses on determining the Sun's absolute magnitude and the distance modulus. One participant calculated the distance modulus to be -31.6 but expressed confusion about needing the apparent magnitude for further calculations. Another contributor suggested that using the apparent magnitude is more straightforward since it is a well-known value in astronomy. They emphasized that relying on luminosity or the solar constant may not be advantageous without having those values readily available. The conversation highlights the importance of understanding how to use apparent magnitude in astronomical calculations.
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1.
(a) What is the distance modulus of the Sun? (b) What is the Sun’s absolute magnitude?
2. I found the distance modulous using 5log(4.84E-6/10) to be -31.6. I feel like I need the apparent magnitude to get the absolute, my teacher is very vague about what we are given to use. Is there a way to do part b without the apparent magnitude using luminosity or flux or something of the sort? Thanks3. I feel like I should use this m-M=distance modulus but I wasn't given any thing to work with.
 
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I don't see how starting with luminosity or the solar constant is superior to starting with the apparent magnitude: They're all values that you aren't given in the problem itself and would have to look up (or measure somehow). So, I'd suggest using the apparent magnitude, which is a pretty well known value that should probably be memorized if you're doing an astronomy related course.
 
I was assigned problem 4, the apparent magnitude was given in problem 3. I should have just read that, thanks though.
 
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