Classroom Activity
Modeling the Orbits of Planets
Overview
In this activity, students explore the relationship between the masses of objects and the orbits they follow. They will make predictions and try to model different orbital scenarios using a gravity well model constructed in class.
Materials
Management
In advance of the lesson, create the gravity well model(s) as follows – making either one model for a class demonstration or one model per group of four to five students:
 Drape the fabric over the hula hoop and secure with 812 evenly spaced binder clips.
A larger hoop can be made using lengths of flexible piping such as thinwalled, smalldiameter PVC pipe. Be aware of the tension that builds up when the pipe is bent and be sure the ends are tightly secured when bending it into a hoop. Important safety note: unsecured pipe can cause injury if its tension is released.  Adjust the fabric and clips as needed so that the fabric is taut but has some give when a spherical mass is placed in the middle.
 Balance the model on the backs of three to four chairs to provide a stable, level support. Consider placing the chairs so the seats face inward and aren’t in the way when students gather around the model.
Background
Gravity is a force that affects everything in the universe. For example, it’s what holds us firmly on Earth’s surface and prevents us from floating away. But it’s so commonplace that we often don’t think about it until something falls.
Every object that has mass has gravity. The more massive an object is, the more gravity it has. A very massive object like Earth has a lot of gravity, but even a comparatively small human has gravity. So while Earth’s gravity pulls on us, our personal gravity also pulls on Earth. It’s such a small amount of gravity that there isn’t a noticeable effect on Earth.
Gravity is also the force that keeps natural satellites like the Moon and artificial satellites like the Mars Reconnaissance Orbiter in orbit. It also keeps planets orbiting our Sun.
Albert Einstein, in his theory of general relativity, postulated that what we think of as empty space is actually threedimensional spacetime, a sort of fabric that fills the volume of the universe.
An object will warp spacetime similar to the way a bowling ball warps the fabric of a trampoline, creating what’s known as a gravity well. The more massive an object is, the more warping of spacetime occurs and the deeper the gravity well becomes.
Depending on its mass and velocity, an object entering another object’s gravity well could do several things.
It could impact the other object if it is moving too slowly or its motion follows a path that intersects with the object.
If it isn't moving too slowly and isn't on a path that intersects with the object, it could enter into an orbit around that object. Since both objects have a gravitational force, the two objects would actually orbit around a common center of mass. For example, the Earth and Moon orbit a common center of mass. But because the center of mass lies within Earth as a result of the planet’s much higher mass, it’s simpler to say that the Moon orbits Earth.
If an object's velocity is high enough, it could pass by the second object and exit its gravity well, having its path altered by the curvature of spacetime. Similarly, spacecraft need a high enough velocity to enter Earth’s orbit and not fall back down to the surface. Spacecraft need an even higher velocity to exit Earth’s gravity well and reach destinations like Mars. And they need a velocity that is even higher still to exit the Sun’s gravity well and leave the solar system.
This activity explores some of those scenarios in a twodimensional space. Keep in mind that in three dimensions, the warping occurs in all directions, so an object can enter, orbit, or exit a gravity well along any plane, depending on its speed and direction.
Procedures
 Show students the gravity well model (see Management for assembly instructions) and explain that it is a twodimensional representation of spacetime.
 Ask students to predict what will happen when you place a massive sphere weighing approximately 0.5 kg (1 lb) in the center.
 Place the mass in the center of the hoop and tell students that the sphere represents the Sun.
 With a lowermass sphere representing a planet, ask students to predict what will happen if you release the sphere at the edge of the hoop. Have students explain how they came up with their prediction.
 After releasing the sphere, ask students to explain why planets in the solar system don’t crash into the Sun. If students don’t mention the motion of planets, guide them to the fact that orbits are a combination of motions. Objects in orbit have motion toward the Sun, as pulled by gravity, and forward momentum that is perpendicular to the Sun’s gravitational pull.
 Demonstrate pushing the smaller sphere perpendicular to the path taken by the previous sphere to create an orbit around the central mass.
 Either as a class or in groups of four to five (with a hoop for each group), have students attempt the following orbits:
 Push a small mass into orbit around the larger central mass (as demonstrated in Step 6).
 Push two similarly sized masses into orbit around the larger central mass.
 Push a small mass orbiting a slightly larger mass into orbit around the large central mass.
 Push a sphere with an equal mass to the central one into orbit around the central mass.
 Students should draw the paths made in their orbit scenarios on a sheet of paper. Students can use mobile devices, if available, to record videos at regular speed and in slow motion to capture the motion of the masses.
 Have students attempt the following variations:
 Change the orbital path from circular to more elliptical.
 Maximize the number of orbits made before the second object collides with the center mass.
Discussion
 How would the gravity well change if an object with a higher or lower mass were placed in the middle? How would that change the speed needed to orbit or exit a gravity well?
 What would this model look like if it were representing a black hole’s gravity well?
 Ask students to describe some limitations of the model they have been using. They should mention some of the following:
 The twodimensional nature of the model means all objects orbit on the same plane, unlike the solar system in which objects orbit the Sun on different planes.
 The friction created by the fabric means orbiting objects slow down and fall in toward the central mass.
 What would the model look like in three dimensions? There would be warped planes in every direction on which the masses could orbit the central mass.
Assessment
 Students should accurately draw the paths of their orbit simulations.
 Students should be able to express that highermass objects create deeper gravity wells that require greater speeds to orbit or exit the well. Conversely, gravity wells with lowermass objects at the center require lower speeds to orbit or exit the well.
Extensions
This model can be used to model how light is influenced by gravity when it travels through space. The phenomenon of light following a curved path around a gravity well is known as gravitational lensing, and it allows scientists to observe objects that might otherwise be hidden behind another object from our perspective. The amount of curvature can also tell scientists about the mass of the foreground object.
 With a central mass on the fabric, ask students to predict the path of a lowermass sphere if it is pushed past the central mass rather than pushed into an orbit around it. Demonstrate the path by pushing the sphere so that it passes near the central mass and travels toward the edge of the hoop.
 Have students mark a spot on the edge of the hoop with a sticky note to represent a telescope on Earth or in orbit. From the spot on the edge opposite the sticky note, have them use a smallermass sphere to simulate a photon of light passing nearby a large mass such as a planet, star, or even a galaxy to reach the telescope.
 Ask students to find multiple paths around the central mass to reach the telescope. They may find wider paths or paths on both sides of the central mass.
 Ask students how light that is curved along one or more of these paths might appear in an image captured by a telescope.
 Ask students how they think the light is affected by gravity if it doesn’t have mass.
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