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this pulsation, and so the distance to any star of this type can be determined by how bright or dim it appears. The following
this pulsation, and so the distance to any star of this type can be determined by how bright or dim it appears. The following figure shows his data. The Y-axis is the apparent velocity, measured in kilometers per second. Positive velocities are galaxies moving away from us, negative velocities are galaxies that are moving towards us. The X-axis is the distance of the galaxy from us, measured in mega-parsecs (Mpc); one parsec is 3.26 light-years, or 30.9 trillion kilometers. Raw data Apparent velocity (km/s) 1000 800 600- 400 200- 0: .. 0.00 0.25 0.50 0.75 1.00 1.25 1.50 1.75 2.00 Distance (Mpc) Show Mean 2 points possible (graded) First, calculate the sample mean: -M 8 where N is the number of data points (here, it is 24). To three significant figures, x= Y = km/s IM Standard deviation 2 points possible (graded). Now, calculate the sample standard deviation: 8X (x,- To three significant figures (beware that numpy std defaults to the population standard deviation), 8xm Mpc Sy Windows You have used 0 of 3 attempts km/s Savy
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