The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
The original proposal would have immediately added three planets, shown here in a size comparison to Earth. Leftmost is Pluto (shown in lieu of Eris,
The original proposal would have immediately added three planets, shown here in a size comparison to Earth. Leftmost is Pluto (shown in lieu of Eris, which is about the same size), then Charon, Ceres, and Earth
The twelve "candidate planets" that were possibilities for inclusion under the originally proposed definition. Note that all but the last three are tr
The twelve "candidate planets" that were possibilities for inclusion under the originally proposed definition. Note that all but the last three are trans-Neptunian objects. The smallest three (Vesta, Pallas, Hygiea) are in the asteroid belt.
Plenary session of the IAU General Assembly on August 24, 2006. Votes were cast by raising yellow cards.
Plenary session of the IAU General Assembly on August 24, 2006. Votes were cast by raising yellow cards.
Planet
The eight planets of the Solar System with size to scale (up to down, left to right): Saturn, Jupiter, Uranus, Neptune (outer planets), Earth, Venus,
The eight planets of the Solar System with size to scale (up to down, left to right): Saturn, Jupiter, Uranus, Neptune (outer planets), Earth, Venus, Mars, and Mercury (inner planets)
A protoplanetary disk
A protoplanetary disk
Protoplanets colliding during planet formation
Protoplanets colliding during planet formation
Earth's atmosphere
Earth's atmosphere