Teachers' Center Activity: Gravity Effects on Planet Motion
Gravity and Its Effect on Planetary Orbits
1. Introduction:
Review the definition of gravity
Drop a ball and explain why it falls downward
Explain that the strength of a gravitational pull is determined by the masses of the objects involved and
the distance between the objects
Hold up a scale model of Earth and a scale model of the Sun. Inquire as to which object would exert
a stronger pull
2. Materials:
Large Rubber or plastic sheet
Heavy round object, such as an 8-lb medicine ball or round watermelon
Smaller, lighter objects, such as tennis balls
3. Activity:
Explain that the sheet represents spacetime, the large object represents the Sun and the smaller object
represents a planet
Have the students pull the edges of the sheet outward. Make sure the sheet is taut.
Roll the lighter balls across the sheet. Note how they travel in a straight line.
Place the heavy object in the center of the sheet. Keep the sheet pulled taut.
Roll the lighter balls across the sheet once again. Note how they now curve. This illustrates Kepler's
First Law that states a planet orbits the Sun in an elliptical orbit (Ideally there would be no friction and
the lighter balls would make a complete elliptical orbit.)
4. Closure:
Discuss how large massive objects such as the Sun curve spacetime toward them (i.e., the ball follows
a curved path)
Discuss how smaller objects such as the ball, or planets, follow the curve of spacetime created by the
more massive object
5. Extensions:
Demonstrate or let the students demonstrate Kepler's Three Laws on an orbit
simulator at http://observe.ivv.nasa.gov/nasa/education/reference/orbits/orbit1.html
Demonstrate different types of orbit by manipulating data at http://www.fourmilab.ch/cgi-bin/uncgi/Solar
Credit:
Artwork by Aurore Simmonet
This activity is part of the
StarChild site.
http://starchild.gsfc.nasa.gov/