What are Kepler's laws and why are they named after him?

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Kepler's laws describe the motion of planets and moons, focusing on their elliptical orbits, equal areas swept out in equal times, and the relationship between orbital period and distance from the sun. They are named after Johannes Kepler, who formulated these laws in the early 17th century based on observational data from Tycho Brahe. The third law, which relates the square of the orbital period to the cube of the semi-major axis of its orbit, is particularly relevant to the project involving the equation T=ar^b. While Newton's laws also describe planetary motion, Kepler's laws specifically address the geometric aspects of orbits. Understanding these laws is crucial for accurately interpreting the orbital dynamics of celestial bodies.
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In class, we've been assigned a project over astronomy. We have graphed an equation for 6 of Jupiter's moons and the planets (separately), and the equation was a power equation T=ar^b. T is the orbital period of the moon or planet, r is the distance from the planet (or sun), and a and b are constants that we've determined. We also have to include a discussion on the three main laws that describe the motion of heavenly bodies, who they are named for, why s/he is the one that gets this honor, and which of the laws pertains to the calculations done here.

The part I need help with pertains to the laws. I believe they are Kepler's laws, but I don't know why Kepler got the honor or which law pertains to the calculations (or equation). Any help?
 
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There's also Newton.

Check your forumla. The constant should not be the exponent. Look up Kepler's 3rd law.
 
The formula is the one she gave us, so I can't change it or anything. It's the one that the whole project is based on and she gave it to us exactly like that. That's the reason I got confused is because the formulas for Kepler's laws aren't anything like this one, but yet it has to relate to one of three main planetary laws.

Or what laws of Newton relate to this? (There has to be three laws of his that relate to planetary motion, though, if I were to use him)
 
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You're right that the laws she's referring to are Kepler's laws. The answer to the questions she's asking are mostly historical in nature, so you could easily find it in a google search of kepler's laws. For reference, here's the law for the solar system:

T^2=\frac{4\pi^2r^3}{GM_{sun}}
 
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