But he and his colleagues have now found that is not the case. In the past, the moon spun around its axis faster than it does today, and their new analysis shows that the fact that the man now faces us may be a result of the rate at which the moon slowed down before becoming locked into its current orientation.
Aharonson, along with Peter Goldreich, the Lee DuBridge Professor of Astrophysics and Planetary Physics, Emeritus, and Re'em Sari of the Hebrew University of Jerusalem, describe their findings in a paper published online on February 27 in the journal Icarus.
Although the moon looks spherical, it is actually elongated, almost like a football. Not long after the moon formed just over four billion years ago, while it was still hot and largely molten, Earth's gravity began to stretch its new companion. When the moon cooled, its slightly oblong shape stuck. Today, the man in the moon occupies one of the two elongated ends.