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Physics 14 Online
OpenStudy (anonymous):

Help:The sun radiates about 3.6 x 10^26 joules of energy each second. How much mass does the sun lose each second? Show your work.

OpenStudy (anonymous):

Solar Mass = 1.989 x 1033 g Absolute luminosity = 3.86 x 1033 erg/sec Speed of light c = 2.99 x 1010 cm/sec Start with Einstein's famous equation: "E = mass times c2" and rearrange the terms to solve for the mass M: M = E/c2 And after inputting our numbers: = 3.86x1033/(2.99x1010)2 = 4.289x1012 g/sec we find that the Sun loses mass 4.289x1012 g every second to energy.

OpenStudy (anonymous):

FYI, it's likely better to use MKS units than CGS units, especially as Solar mass is typically given in kilograms, and c is typically given in in m/s.

OpenStudy (anonymous):

could you explain it in the units your talking about?

OpenStudy (anonymous):

\[m=\frac{ E }{ c ^{2} }=\frac{ 3.6*10^{26}J }{ \left( 2.99792*10^{8}m/s \right)^{2} }=4.056*10^{9}kg\]

OpenStudy (anonymous):

Note that my answer is slightly different because I used a value for c that had greater precision than that used by @greenleaf800073.

OpenStudy (anonymous):

He also used a different value for E.

OpenStudy (anonymous):

thank youuuuuuu, yes I see, could u also help me with two more question?

OpenStudy (anonymous):

Derive the time dilation equation , explain each step of the derivatior

OpenStudy (anonymous):

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