In the "giant impact" model of the moon's formation, the young moon began its orbit within Earth's equatorial plane. In the standard variant of this model (top panel), Earth's tilt began near today's value of 23.5 degrees. The moon would have moved outward smoothly along a path that slowly changed from the equatorial plane to the "ecliptic" plane, defined by Earth's orbit around the sun. If, however, Earth had a much larger tilt after the impact (~75 degrees, lower panel) then the transition between the equatorial and ecliptic planes would have been abrupt, resulting in large oscillations about the ecliptic. The second picture is consistent with the moon's current 5-degree orbital tilt away from the ecliptic.