Math Problem Statement
For each planet in a solar system, its year is the time it takes the planet to revolve around the center star. The formula Upper E equals 0.2 x Superscript 3 divided by 2 models the number of Earth days in a planet's year, E, where x is the average distance of the planet from the center star, in millions of kilometers. There are approximately 224.3 Earth days in the year of Planet Upper B. What is the average distance of Planet Upper B from the center star? Question content area bottom Part 1 The average distance is approximately 110 million kilometers. (Do not round until the final answer. Then round to the nearest whole number as needed.)
Solution
We are given the formula:
where:
- is the number of Earth days in a planet's year.
- is the average distance from the center star in millions of kilometers.
Step 1: Substitute the given value of
We are given that , so we set up the equation:
Step 2: Solve for
a) Isolate
b) Solve for
To get , raise both sides to the power of :
Now, let's compute the value. Compute x = (1121.5)^(2/3) x = 1121.5**(2/3) x### Step 3: Round to the nearest whole number
Thus, the average distance of Planet B from the center star is 108 million kilometers.
Would you like a step-by-step breakdown of exponent manipulation? Here are some related questions to explore:
- How does the exponent affect the equation?
- What are the steps to solving equations with fractional exponents?
- How is this formula related to Kepler’s Third Law?
- What would happen if the coefficient 0.2 changed?
- Can we use logarithms to solve this equation?
Tip: When solving equations with exponents, always isolate the power term first before applying inverse operations.
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Math Problem Analysis
Mathematical Concepts
Algebra
Exponents
Equation Solving
Formulas
E = 0.2 * x^(3/2)
Theorems
Exponent Rules
Solving Equations with Exponents
Suitable Grade Level
Grades 9-11
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