The task was to construct a physical model
of the planetary domain of the Solar System. The Voyage
model Solar System was to extend from the Sun to Pluto.
Usually a physical model is constructed at a size that maximizes
a person’s ability to manipulate it, and explore it.
A reasonable size might be 0.3 meters (1 foot) across, about
the size of a typical classroom globe. The Solar System, however,
poses a problem for the model builder.
The Solar System is comprised of small objects in a vast
space. Even the Sun is dwarfed by the space. You would need
over 4,200 Suns side-by-side to span the distance between
the Sun and Pluto. The problem is representing the objects
and the spaces between them on the same scale.
The smallest object we wanted to depict were moons of at
least 1,000 km diameter, like Tethys, Dione, Ariel, and Umbriel.
The largest size to be depicted was Pluto’s average
distance from the Sun, corresponding to 39.5 Astronomical
Units, or 6 billion km.
Consider the two extremes for the model builder. First, consider
a model of the Sun-Pluto distance that is constructed about
the size of a classroom globe, or equivalently, drawn on a
sheet of 8.5” x 11” paper. On the paper you could
locate the Sun, all the planets, and Pluto—creating
a comfortably sized model of the Solar System. But on this
scale the model Sun would be barely visible, with a diameter
less than 0.1 mm across, and the planets would be too small
to be seen.
On the other extreme, if a model of a 1,000 km diameter moon
was constructed about the size of a classroom globe, then
the model Sun-Pluto distance would stretch the length of the
U.S. pacific coast, and the model Sun would be as tall as
the Empire State Building in New York.
The approach to Voyage was to use a scale so that
the size of a human being is about mid-way between the smallest
object depicted and the largest distance depicted. This is
the most effective way a human observer can experience the
Solar System as a model. It maximizes the visitor’s
ability to directly observe both the sizes of the worlds and
the distances between them—at the same time.
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