A graphing calculator is recommended. The table shows the mean (average) distances d of the planets from the sun (taking the unit of measurement to be the distance from the earth to the sun) and their periods T (time of revolution in years). Planet T(d) = Mercury Venus Earth Mars Jupiter Saturn Uranus d 0.387 0.723 1.000 1.523 5.203 19.190 T Neptune 30.086 0.241 0.615 1.000 1.881 9.541 29.457 11.861 84.008 164.784 (a) Fit a power model to the data. Use n = 2. (Round your values to one decimal place.) (b) Kepler's Third Law of Planetary Motion states that "The square of the period of revolution of a planet is proportional to the cube of its mean distance from the sun." Does your model corroborate Kepler's Third Law? O Yes O No

Algebra & Trigonometry with Analytic Geometry
13th Edition
ISBN:9781133382119
Author:Swokowski
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Chapter7: Analytic Trigonometry
Section7.6: The Inverse Trigonometric Functions
Problem 94E
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### Mean Distances and Periods of Planets from the Sun

A graphing calculator is recommended.

The table below shows the mean (average) distances \( d \) of the planets from the sun (taking the unit of measurement to be the distance from the earth to the sun) and their periods \( T \) (time of revolution in years).

| Planet  | \( d \)   | \( T \)     |
|---------|-----------|-------------|
| Mercury | 0.387     | 0.241       |
| Venus   | 0.723     | 0.615       |
| Earth   | 1.000     | 1.000       |
| Mars    | 1.523     | 1.881       |
| Jupiter | 5.203     | 11.861      |
| Saturn  | 9.541     | 29.457      |
| Uranus  | 19.190    | 84.008      |
| Neptune | 30.086    | 164.784     |

#### Exercise

**(a)** Fit a power model to the data. Use \( n = \frac{3}{2} \) (Round your values to one decimal place).

\[ T(d) = \_\_\_\_\_ \]

**(b)** Kepler's Third Law of Planetary Motion states that "The square of the period of revolution of a planet is proportional to the cube of its mean distance from the sun."

Does your model corroborate Kepler's Third Law?
- Yes
- No
Transcribed Image Text:### Mean Distances and Periods of Planets from the Sun A graphing calculator is recommended. The table below shows the mean (average) distances \( d \) of the planets from the sun (taking the unit of measurement to be the distance from the earth to the sun) and their periods \( T \) (time of revolution in years). | Planet | \( d \) | \( T \) | |---------|-----------|-------------| | Mercury | 0.387 | 0.241 | | Venus | 0.723 | 0.615 | | Earth | 1.000 | 1.000 | | Mars | 1.523 | 1.881 | | Jupiter | 5.203 | 11.861 | | Saturn | 9.541 | 29.457 | | Uranus | 19.190 | 84.008 | | Neptune | 30.086 | 164.784 | #### Exercise **(a)** Fit a power model to the data. Use \( n = \frac{3}{2} \) (Round your values to one decimal place). \[ T(d) = \_\_\_\_\_ \] **(b)** Kepler's Third Law of Planetary Motion states that "The square of the period of revolution of a planet is proportional to the cube of its mean distance from the sun." Does your model corroborate Kepler's Third Law? - Yes - No
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