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388238218.4 which should now be rounded to 3.88 × 108 rotations since the time-interval was specified in the problem to three significant figures. (b) We note that the problem specifies the exact number of pulsar revolutions (one million). In this case, our unknown is t, and an equation similar to the one we set up in part (a) takes the form N = ft, or 1 × 106 = 1 rotation t 1.55780644887275 × 10−3 s which yields the result t = 1557.80644887275 s (though students who do this…

388238218.4 which should now be rounded to 3.88 × 108 rotations since the time-interval was specified in the problem to three significant figures. (b) We note that the problem specifies the exact number of pulsar revolutions (one million). In this case, our unknown is t, and an equation similar to the one we set up in part (a) takes the form N = ft, or 1 × 106 = 1 rotation t 1.55780644887275 × 10−3 s which yields the result t = 1557.80644887275 s (though students who do this…

55780644887275 × 10−3 s which should now be rounded to 3.88 × 108 rotations since the time-interval was specified in the problem to three significant figures. (b) We note that the problem specifies the exact number of pulsar revolutions (one million). In this case, our unknown is t, and an equation similar to the one we set up in part (a) takes the form N = ft, or 1 × 106 = 1 rotation t 1.55780644887275 × 10−3 s which yields the result t = 1557.80644887275 s (though students who do…

388238218.4 which should now be rounded to 3.88 × 108 rotations since the time-interval was specified in the problem to three significant figures. (b) We note that the problem specifies the exact number of pulsar revolutions (one million). In this case, our unknown is t, and an equation similar to the one we set up in part (a) takes the form N = ft, or 1 × 106 = 1 rotation t 1.55780644887275 × 10−3 s which yields the result t = 1557.80644887275 s (though students who do…

388238218.4 which should now be rounded to 3.88 × 108 rotations since the time-interval was specified in the problem to three significant figures. (b) We note that the problem specifies the exact number of pulsar revolutions (one million). In this case, our unknown is t, and an equation similar to the one we set up in part (a) takes the form N = ft, or 1 × 106 = 1 rotation t 1.55780644887275 × 10−3 s which yields the result t = 1557.80644887275 s (though students who do this…

388238218.4 which should now be rounded to 3.88 × 108 rotations since the time-interval was specified in the problem to three significant figures. (b) We note that the problem specifies the exact number of pulsar revolutions (one million). In this case, our unknown is t, and an equation similar to the one we set up in part (a) takes the form N = ft, or 1 × 106 = 1 rotation t 1.55780644887275 × 10−3 s which yields the result t = 1557.80644887275 s (though students who do…

388238218.4 which should now be rounded to 3.88 × 108 rotations since the time-interval was specified in the problem to three significant figures. (b) We note that the problem specifies the exact number of pulsar revolutions (one million). In this case, our unknown is t, and an equation similar to the one we set up in part (a) takes the form N = ft, or 1 × 106 = 1 rotation t 1.55780644887275 × 10−3 s which yields the result t = 1557.80644887275 s (though students who do this…

388238218.4 which should now be rounded to 3.88 × 108 rotations since the time-interval was specified in the problem to three significant figures. (b) We note that the problem specifies the exact number of pulsar revolutions (one million). In this case, our unknown is t, and an equation similar to the one we set up in part (a) takes the form N = ft, or 1 × 106 = 1 rotation t 1.55780644887275 × 10−3 s which yields the result t = 1557.80644887275 s (though students who do this…

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