Clyde Tombaugh discovered Pluto at the Lowell Observatory, Arizona in 1930.
In 2006 the International Astronomical Union (IAU) announced a new classification system in which Pluto became a dwarf planet. The generations of schoolchildren who knew its name as both the ninth planet and the Disney dog were dismayed.
Yet instead of asking why Pluto isn't a planet any more, a more interesting question is: Why was Pluto ever thought to be a planet?
The story begins with the planet Uranus. William Herschel discovered it in 1781, but by 1845 it was puzzling astronomers by not moving as expected.
French astronomer Urbain Le Verrier thought that the discrepancy was due to the gravitational pull of an undiscovered planet. His calculation of this planet's position allowed Johann Galle at the Berlin Observatory to locate Neptune in 1846.
Then half a century later it seemed that another large planet was disturbing the orbits of Neptune and Uranus. The hunt was on for a ninth planet. Everyone assumed that Tombaugh had finally found it.
However it was soon evident that Pluto was small. Eventually, astronomers realized it was far too small to influence Neptune. Furthermore, using space probe data, a new calculation of Neptune's orbit seemed to match the observed one. Finding Pluto was a lucky accident, though it's a tribute to Tombaugh's thoroughness that he spotted the tiny distant object.
Pluto is not only smaller than several solar system moons, but is also an icy body in an orbit very different to those of the eight planets. Pluto seemed unique until the 1992 discoveries of the first Kuiper Belt objects. The Kuiper Belt contains hundreds of thousands of such icy bodies orbiting at a distance of between 30 and 50 times the distance from the earth to the sun.
The bodies orbiting beyond Neptune are commonly called trans-Neptunian objects. In 2005 the discovery of one that appeared to be larger than Pluto was a further stimulus to a formal definition of a planet. Considering the ensuing controversy, Eris (goddess of strife and discord) was an appropriate name.
We should realize that reclassifying planets is not new. Eighteenth century German astronomer Johann Bode had suggested that there should be a planet between Mars and Jupiter. The discovery of Ceres in 1801 was confirmation. Unfortunately, half a century later, there were fifteen "planets" in this orbit and astronomers decided they were a new class of objects, and they called them asteroids.
Interestingly, Ceres too has now been classified as a dwarf planet, along with Pluto and Eris and two other trans-Neptunian objects, Makemake and Haumea. Even some who are unconvinced that Pluto is a planet are puzzled by the dwarf planet class, especially since Ceres is quite different to the other four - they have been designated both as dwarf planets and plutoids.
However even if Pluto is not our ninth planet, it has still turned out to be the prototype of an intriguing new class of solar system object.
There are images related to this article on my Pinterest board "Outer Solar System".