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One of Kepler's three laws of planetary motion states that the square of the period, P, of a body orbiting the sun is proportio...Asked by Clarence
One of Kepler's three laws of planetary motion states that the square of the period, P, of a body orbiting the sun is proportional to the cube of its average distance, d, from the sun. The Earth has a period of 365 days and its distance from the sun is approximately 93,000,000 miles.
a.) Find P as a function of d.
P(d)=
a.) Find P as a function of d.
P(d)=
Answers
Answered by
Reiny
P = k d^3
given, when P = 365 days, d = 93 000 000 miles
365 = k(93000000)^3
solve for k, you will need scientific notation, then rewrite the equation
Let me know what you get for k
given, when P = 365 days, d = 93 000 000 miles
365 = k(93000000)^3
solve for k, you will need scientific notation, then rewrite the equation
Let me know what you get for k
Answered by
Clarence
I got 4.5378*10^-22 for k.
Answered by
Reiny
correct
Answered by
Clarence
Still incorrect according to WebWork
Answered by
Reiny
I assumed you had Kepler's law stated correctly, then looked it up and found:
The <b>square</b> of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
so it would be
P^2 = k d^3
try it with this change
The <b>square</b> of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
so it would be
P^2 = k d^3
try it with this change
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