Question: solve number 3 depending on 2 Write a program to find the gravitational constant g for the following sets of data. U- the power fit
solve number 3 depending on 2
Write a program to find the gravitational constant g for the following sets of data. U- the power fit that was shown in Example 5.3 Time, lt Distance, dk Time, k Distance, dk .200 0.400 0.600 0.800 1.000 0.1960 0.7835 1.7630 3.1345 4.8975 0.200 0.400 0.600 0.800 1.000 0.1965 0.7855 1.7675 3.1420 4.9095 3. The following data give the distances of the nine planets from the sun and their side reat period in days Sidereal period (days) 87.99 224.70 365.26 686.98 Distance from sun (km x 106) Planet Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto 57.59 108.1I 149.57 227.84 778.14 4,332.4 10,759 30,684 60.188 90,710 1427.0 2870.3 4499.9 5909.0 Modify your program from Problem 2 to also calculate E2(f). Use it to find the power fit of the form y e Cx3/2 for (a) the first four planets and (b) all nine planets Write a program to find the gravitational constant g for the following sets of data. U- the power fit that was shown in Example 5.3 Time, lt Distance, dk Time, k Distance, dk .200 0.400 0.600 0.800 1.000 0.1960 0.7835 1.7630 3.1345 4.8975 0.200 0.400 0.600 0.800 1.000 0.1965 0.7855 1.7675 3.1420 4.9095 3. The following data give the distances of the nine planets from the sun and their side reat period in days Sidereal period (days) 87.99 224.70 365.26 686.98 Distance from sun (km x 106) Planet Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto 57.59 108.1I 149.57 227.84 778.14 4,332.4 10,759 30,684 60.188 90,710 1427.0 2870.3 4499.9 5909.0 Modify your program from Problem 2 to also calculate E2(f). Use it to find the power fit of the form y e Cx3/2 for (a) the first four planets and (b) all nine planets
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