Why did Pluto stop being a planet in 2006?
An 11-year-old schoolgirl suggested Pluto's name in 1930; in 2006 astronomers voted it out of the planet club.
βΆ Start the storyPluto stopped being a planet because in August 2006 the (IAU) voted for a definition that it does not meet. Under that definition, a planet orbits the Sun, is massive enough for its own gravity to make it round, and has cleared its neighbourhood of smaller objects. Pluto fulfils the first two, but not the third, so it became a .
Pluto's story started with a hero's welcome. Clyde Tombaugh discovered it in 1930, and it was immediately hailed as the ninth planet. Its name was suggested by an eleven-year-old schoolgirl in Oxford, Venetia Burney, who was interested in classical mythology.
Then it kept shrinking. In 1978 the discovery of its moon Charon made it possible to measure its mass, and Pluto turned out to be only one-sixth the mass of the Moon. From 1992, astronomers found many icy bodies beyond Neptune similar to Pluto. When Mike Brown's team announced Eris in 2005, an object more massive than Pluto, astronomers had to decide: add a tenth planet, or define the word.
1930
Tombaugh discovers Pluto, hailed as the ninth planet
1978
Charon reveals Pluto is tiny
1992
Icy bodies like Pluto start turning up beyond Neptune
2005
Eris is found, more massive than Pluto
2006
IAU votes in Prague; Pluto becomes a
On 24 August 2006, at a meeting in Prague, the IAU voted on a final draft. It created a new class, the , and placed Pluto in it along with and Eris. The vote passed with 424 astronomers taking part, and the decision is still argued over: some astronomers reject it, and New Mexico's House of Representatives declared Pluto a planet in its own skies.
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Recap
Pluto stayed the same; the word planet changed: orbit the Sun, be round, clear your path, and Pluto only does the first two.
π‘ A trick to remember it Β· Round and orbiting the Sun is not enough: a planet must also sweep its lane clear.
Surprising fact Β· Pluto's mass is only 0.07 times the combined mass of the other objects in its orbit, while Earth's is 1.7 million times.
Connects to
- πͺ How can you tell a planet from a star just by looking?
- π How was Neptune found with pencil and paper before anyone saw it?
- βοΈ What lies beyond Neptune: the Kuiper belt and the Oort cloud?
- βοΈ Why didn't the asteroid belt ever become a planet?
- β³ When does a heap of sand stop being a heap?
Sources (2)
No source, no claim. Every fact in this lesson (14 claims) cites at least one of these.