From the March 2008 issue

What is the difference between a planetesimal and a dwarf planet?

Robert Anton, Santa Magarita, California
By | Published: March 1, 2008
Protoplanetary Disk
The term “planetesimal” refers to small bodies that orbited the Sun prior to the planets’ formation. In 2006, the International Astronomical Union (IAU) ruled that a “dwarf planet” is a nearly spherical celestial body orbiting the Sun that has not cleared its orbital path of debris, as have the traditional planets.

The term “minor planet” was already an accepted catch-all for asteroids and Kuiper Belt objects. But Pluto is the only such object the Minor Planet Center in Cambridge, Massachusetts, kept tabs on that wasn’t officially designated a minor planet.

Astronomers introduced the “dwarf planet” category during the 2006 debate to classify Pluto. But, Pluto aside, any definition that included “roundness” as a qualification also had to include Ceres, the largest asteroid, which is massive enough to make itself spherical; a few other large asteroids also may make the cut as astronomers better determine their shapes.

Moreover, the dwarf planets beyond Neptune will be classed in a separate, as-yet-unnamed category. Caltech astronomer Michael Brown points out that three of the four largest of these, including Pluto and Eris, have one or more moons, while only 11 percent of all Kuiper Belt bodies have moons.

So, while the new category is a bit puzzling linguistically, there is a physical basis for creating it. — Francis Reddy, Senior Editor