Public Lecture with Robin Canup on The Origin of the Moon
The Moon has been the Earth's celestial companion throughout our planet's history, and the ancient surface and geology of the Moon retain clues to how our Earth-Moon system formed more than 4 billion years ago. A primary scientific outcome of the Apollo program was the so-called giant impact theory for lunar origin, in which a collision at the end of Earth’s formation created a debris disk orbiting the Earth from which the Moon later accumulated. In the past decade, the nature of the envisioned Moon-forming giant impact has become highly debated, driven by increasingly precise sample analyses that show that the Earth and Moon have essentially identical isotopic compositions across many elements, including oxygen. In this talk, Canup will describe current ideas for how our Earth-Moon pair formed, key remaining areas of uncertainty, and how planned near-term lunar exploration should help us to unravel how our planet and its remarkable Moon came to be.

Header image: Scientists use computer models to simulate how the moon may have formed. (Credit: NASA/JPL-Caltech)