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First, let's rearrange Kepler's third law into a form that is easier to use to calculate distance. Right now, we have Kepler's third law written
First, let's rearrange Kepler's third law into a form that is easier to use to calculate distance. Right now, we have Kepler's third law written as: d^ 3 propto P^ 2 Proportionalities can be rearranged the same way equalities can. Solve for d by clicking in the box to complete the formula
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