Calculating Sun's Luminosity: Step-by-Step Guide

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SUMMARY

The calculation of the Sun's luminosity involves understanding the relationship between apparent magnitude and distance. The correct approach is to use the formula for flux at the Sun's radius, which is derived from the Earth's orbit flux (1630 W/m²) and the surface area of a sphere. The formula should be expressed as 4 * π * Rearth2 * Fearth, rather than dividing the Sun's surface area by the inverse square of the distance from the Earth. Proper unit management is crucial to avoid errors in calculations.

PREREQUISITES
  • Understanding of luminosity and flux in astrophysics
  • Familiarity with the concept of apparent magnitude
  • Knowledge of spherical geometry and surface area calculations
  • Basic proficiency in unit conversion and dimensional analysis
NEXT STEPS
  • Study the derivation of the inverse square law in astrophysics
  • Learn about the calculation of stellar luminosity using the Stefan-Boltzmann Law
  • Explore the concept of flux and its applications in astrophysical contexts
  • Review examples of unit conversion in physical equations
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Astronomy students, astrophysicists, educators in physics, and anyone interested in understanding stellar properties and calculations related to luminosity.

mokeejoe5
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I'm trying to work out the luminosity of the sun.

1630 Watts/m2 apparent magnitude reduces with distance squared so
1/(1.496*1011)2 = 4.468*10-23m2 has the same brightness 1630 Watts from earth

Surface area of the sun divided by 4.468*10-23m2 = # of 1630 Watt sections
*1630 = 2.21*1044 Watts
    • #​

    [*]


Can someone please explain to me where I'm going wrong?
 
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It is not clear what you are trying to show. I think you are choosing a 'strange path' through your calculations. Try starting again.
Given the luminosity, measured on Earth, you can work out the total Power radiated. (Area of a sphere of radius 1.496*1011 times the Watts per m2 on Earth)
You can then work out the flux for a sphere of any radius (even the radius of the Sun)
 
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Why 1/(1.496*1011)2 ? When you do this, you are calculating how much the flux increases from the radius of the Earth's orbit to a radius of 1 meter. What you want to do instead of calculating 1/Rearth^2, is calculate Rsun^2/Rearth^2. If the flux at Earth's orbit is given by Fearth (=1630 W/m^2), then the flux at the sun's radius is given by 4 * pi * Rsun^2 * Fearth / (Rsun^2/Rearth^2) = 4 * pi * Rearth^2 * Fearth. This is the same answer that SophieCentaur gave you. Do you see?
 
Another example where proper units everywhere would have made the mistake obvious.
mokeejoe5 said:
1/(1.496*1011)2
This is 1/(1.496*1011m)2 = 4.468*10-23m-2
It does not make sense to divide the surface of sun by this value, the result would be meters to the 4th power.
 

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