How Can You Determine the Sun’s Absolute Magnitude?

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SUMMARY

The discussion centers on determining the Sun's absolute magnitude using the distance modulus formula. The distance modulus was calculated as -31.6 using the formula 5log(4.84E-6/10). Participants emphasized the importance of using the apparent magnitude, which is a well-known value in astronomy, to derive the absolute magnitude. The conversation highlights that while luminosity and flux can be considered, they are not as straightforward as using the apparent magnitude for this calculation.

PREREQUISITES
  • Understanding of distance modulus in astronomy
  • Familiarity with the concept of absolute and apparent magnitude
  • Basic knowledge of logarithmic calculations
  • Awareness of the solar constant and its significance
NEXT STEPS
  • Research the formula for calculating absolute magnitude from apparent magnitude
  • Study the concept of luminosity and its relation to stellar brightness
  • Learn about the solar constant and its measurement techniques
  • Explore the significance of distance modulus in astronomical calculations
USEFUL FOR

Astronomy students, educators, and anyone interested in understanding stellar measurements and calculations related to the Sun's brightness.

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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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