New solution

JAMF edited
revision #19285 newer →
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+### Statement
+
+$14.5.2.$ [Insert the problem statement]
+
+### Solution
+
+$14.5.2$ The solar radiation power $W$ is close to $4 \cdot 10^{26}$ watts. Estimate the mass lost
+by the Sun due to radiation over the course of a second.
+
+The energy emitted from the sun is:
+
+\begin{equation}
+ E = P \cdot 1 s = 4 \cdot 10^{26}
+\end{equation}
+
+Using the equivalency between mass and energy we have:
+
+\begin{equation}
+ m = \frac{E}{c^2} = 4,4 \cdot 10^9 g
+\end{equation}
+
+
+#### Answer
+
+[Insert a concise answer or boxed result]