The sun appears to move across the sky, because the earth spins on its axis. To a person standing on the earth, the sun subtends an angle of sun = 9.30 x 10-3 rad (see Conceptual Example 2). How much time (in seconds) does it take for the sun to move a distance equal to its own diameter?(adsbygoogle = window.adsbygoogle || []).push({});

I know that I probably need convert radians to degrees and find the length of the r first?

I just don't know where the heck the time factor comes in this rotational kinematics problem. There seems to not be enough information.

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# Homework Help: Sun's Rotational Kinematics

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