Kepler's Third Law of Orbital Motion shows how you can approximate the period P (in Earth years) it takes a planet to complete one orbit of the sun. Use the function P = dt, where d is the
distance from the planet to the sun in astronomical units (AU-about 930,000,000 miles or the
distance from Earth to the sun). Find the approximate length (in Earth years) of a Venusian
year if Venus is 0.72 AU from the sun.

8y^50

step-by-step explanation:

part a

x     y

0     8

1     7.5

2     7

3     6.5

4     6

5     5.5  

for every hour i deducted .5 inches from the length of the candle

part b

it is a function because for every x value there is only one y value

part   c

for every x value there is only one y value

x       y

0       8

1       7.6

2       7.2

3       6.8

step-by-step explanation:

/

step-by-step explanation:

i believe the answers 600m