Drag each item to the correct location, so that each contribution to the theory of universal gravitation is matched with the scientist responsible for it. (2 points)

Location 1: Johannes Kepler
Location 2: Robert Hooke
Location 3: Isaac Newton

Responses

First proposed the idea that a force of attraction applied to all objects in space
First proposed the idea that a force of attraction applied to all objects in space

Used mathematics to prove that gravity increases with decreasing distance between objects
Used mathematics to prove that gravity increases with decreasing distance between objects

Described the motion of planets around the sun as elliptical
Described the motion of planets around the sun as elliptical

Location 1: Johannes Kepler

Described the motion of planets around the sun as elliptical

Location 2: Robert Hooke
Used mathematics to prove that gravity increases with decreasing distance between objects

Location 3: Isaac Newton
First proposed the idea that a force of attraction applied to all objects in space

Location 1: Johannes Kepler - Described the motion of planets around the sun as elliptical

Location 2: Robert Hooke - First proposed the idea that a force of attraction applied to all objects in space
Location 3: Isaac Newton - Used mathematics to prove that gravity increases with decreasing distance between objects

To match each contribution to the theory of universal gravitation with the scientist responsible for it, you can follow these steps:

1. First proposed the idea that a force of attraction applied to all objects in space: Isaac Newton
2. Used mathematics to prove that gravity increases with decreasing distance between objects: Robert Hooke
3. Described the motion of planets around the sun as elliptical: Johannes Kepler

So the correct matching would be:

1. Isaac Newton: First proposed the idea that a force of attraction applied to all objects in space
2. Robert Hooke: Used mathematics to prove that gravity increases with decreasing distance between objects
3. Johannes Kepler: Described the motion of planets around the sun as elliptical