The discussion revolves around applying Stefan-Boltzmann's Law to calculate the radius of the Sun, using given values for temperature and luminosity. Participants are exploring the relationship between these variables and the resulting calculations.
The discussion is ongoing, with participants sharing their calculations and questioning the accuracy of their results. Some have noted that their results align closely with known values from NASA, while others are seeking clarification on their methods and assumptions.
There are indications of potential miscalculations regarding units, with one participant mentioning a possible confusion between kilometers and meters. Participants are also reflecting on the accuracy of their results in relation to established data.
Did you mean ##r^2=…##?PMNIMG said:Homework Statement: Use the Stefan-Boltzmann's Law and calculate Sun's radius.
T☉=5772K
L☉= 3.828×10^(26) W
Relevant Equations: E=σT^4
L=4πr^2*σT^4
r=(L/4π*σT^4)^(1/2)
r=(3.828*10^(26))/(4π*σ(5772)^4)
It's diffrent from what I know...
Oh, sorry. I modified it now.haruspex said:Did you mean ##r^2=…##?
Other than that, what is stopping you?
No problem.PMNIMG said:Oh, I think I miscalculated...
sorry I disturbed you all with dumb question...
I think I put km instead of m...