![]() It's usually measured in Watts (which is Joules per Second) and this Method has been used before. ![]() The Stefan Boltzmann Law calculates the heat energy an object releases from it's surface area. Using this calculator, I get 24490112 Joules or 0.00585 Tons of TNT (9-A) ![]() Let's assume it's "height" is equal to it's radius, which is 5.085m. So dividing the result in half will fix it! Dividing by 2 gets us 116.5m^3Īverage Density of the Sun is 1.408 g/cc or 1408 kg/m^3ģ48.8m^3*1408kg = 491110.4kg or around 490 Metric Tons (Class K) However, given how the shape is, it's gonna be intersecting with the Cylinder. Assuming an ellipsoid with "a" & "b" of 5.085m with the "c" being 2.15m (remaining undivided, you'll see why), we get 233m^3 Assuming it's a Cylinder with a Radius of 5.085m (10.17m/2) and a "Height" of 2.86m, we get 232.3m^3 I will try to get the Potential Energy of this miniature sun, for which I'll require mass and height (center of mass)įirst, the "Body" of the Sun. ![]()
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