From the May 2011 issue

What lies beyond the planets

Clyde Tombaugh’s discovery of Pluto in 1930 seemed to round out our planetary system, but astronomers have since found a vast expanse of similar objects in the Kuiper Belt.
By | Published: May 23, 2011
A view from above shows the orbits of the biggest trans-Neptunian objects. Astronomy: Roen Kelly and Richard Talcott
Planetary scientists now recognize three distinct zones in our solar system. In the inner zone, Mercury, Venus, Earth, and Mars are the dominant players. The middle zone holds the giant planets: Jupiter, Saturn, Uranus, and Neptune. But the outer zone may be the richest of all. Known as the Kuiper Belt, it comprises Pluto, Eris, Sedna, and Haumea; probably 100,000 other “ice dwarf” worlds; and several billion comets.

Caltech astronomer Michael Brown has helped categorize the Kuiper Belt through his discoveries of several of the largest objects in this third zone. Now, he and his colleagues are continuing their search for more of these worlds from the Southern Hemisphere.

But the Kuiper Belt is more than a collection of frigid worlds far from the Sun — it may hold clues to the formation and early history of our solar system. Planetary scientist S. Alan Stern wrote about the far-flung region in this 2008 article for Astronomy’s special solar system issue. Stern, the principal investigator for the New Horizons mission to Pluto and the Kuiper Belt, no doubt will lead a revision to what we know about the outer solar system when the spacecraft reaches Pluto in 2015.

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