Make a Model of the Solar System

The solar system is the system of objects that orbit the Sun directly (e.g. the planets) or indirectly (e.g. Earth's moon). A celestial body is considered a planet in the solar system if it orbits the Sun, if it is heavy enough for gravity to squeeze it into a spherical shape, and if it has "cleared the neighborhood" around its orbit. The latter means that there are no objects comparable in size in the vicinity of its orbit, other than the planet's moons. Eight objects in the solar system qualify as planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. Dwarf planets, like Pluto, fulfill the first two criteria, but not the last. Planets are not self-luminous—they do not emit light like the stars—but they can be seen in the sky because they reflect light emitted by other celestial objects.

Planets are approximately spherical, and the equatorial radius is often used as a measure of their size. The orbital distance is the average distance from the planet to the Sun as it circles the Sun. The distance from the Sun to a planet is not constant since the orbits are elliptical, but a circular orbit with the orbital distance as radius is a good approximation. The orbital distance is often expressed in astronomical units (AU). One AU equals roughly the distance from the Sun to Earth, or 149,597,870,691 ± 30 meters. Table 1 lists the radii and the orbital distances of the eight planets of the solar system.

Figure 1. Drawing illustrating the definition of orbital distance.

Listed in increasing orbital distance from the Sun, we first encounter Mercury, the smallest of the eight planets. Mercury is only slightly larger than Earth's moon. Next is Venus, a planet with a radius of 6,052 km, only slightly smaller than Earth. Then comes Earth, the planet with the highest average density (5.5 g/cm³), followed by Mars. Mars' radius is about half of Earth's radius. It is a dusty, cold planet, but might have inhabited some form of life long ago. These first four planets are called the inner planets because they orbit closest to the Sun; they are also known as the rocky planets because their surfaces are rocky, showing mountains, valleys, and other formations. The rocky planets are all smaller than the gas planets and they are made of denser material. The next four—Jupiter, Saturn, Uranus and Neptune—orbit farther away from the Sun; they are gaseous planets. Jupiter is the largest, with a radius 11 times larger than Earth's radius; followed by Saturn, whose radius is about 9.5 times larger than Earth's radius. Saturn is the planet with the lowest density (0.7 g/cm³), a density so low that it would float if placed in water! Uranus and Neptune are similar in size, with a radius of 4.0 and 3.9 times the radius of Earth, respectively.

To make a scale model, your students should scale all the distances (radii and orbital distances) by the same factor, called the scale factor. For example, to create a scale model of the eight planets, scaled so the radius of Earth is 1 cm, you use a scale factor of 1 cm/6,378 km because 6,378 km (the actual radius of Earth) multiplied by 1 cm/6,378 km (the scale factor) yields 1 cm (the radius of the Earth model). You can find the radius of each of the other seven model planets by multiplying each planet's actual radius by the scale factor.

Table 2 lists the radii for this model and Figure 2 shows the results. Your students will make similar model planets. Because the radius of the Sun is about 109 times the radius of Earth, the Sun would have a radius of a little over 1 m in this model.

Figure 2. Scale model of the eight planets of the solar system.

The planets' radii are small compared to their distance from the Sun, and it takes a little more work to calculate how far from the Sun these model planets need to be placed to get an accurate representation of the solar system. Orbital distance is often expressed in AU, so the first step is often to calculate what distance in the model corresponds to 1 AU in the real world. As 1 AU is approximately 150 million km, or 1.5 × 10⁸ km, and 1 km converts to (1/6,378) cm, 1 AU will become 235,183 cm or about 235 m in your model. The scale factor 1 m/6,378 km thus becomes 235 m/1 AU. This is the same factor, only expressed in different units. Next, your students should multiply the orbital distance (in AU) of each planet by the scale factor (235 m/1 AU in this case) to find how far from the Sun the planets need to be placed in the model. Table 3 lists the results for a model where Earth is represented by a sphere with a radius of 1 cm.

You will likely not have space to lay the model planets out in the classroom, nor on the school grounds. Students can, however, use a map of their surroundings to visualize the scaled-down planet distances. They can use a printed map or an electronic application, like Google Maps. If you prefer a model where the solar system fits in the classroom, try the activity Model the Distances between Planets in our Solar System. Unfortunately, when scaling the solar system that much, the planets become too small to be visible.