Astronomy Practice Exam 2025 – 400 Free Practice Questions to Pass the Exam

The phenomenon that results from the wobbling of the Earth's axis is known as precession. This refers to the gradual shift in the orientation of the Earth's rotational axis, which occurs due to gravitational forces exerted by the Sun and the Moon on the Earth’s equatorial bulge. As a consequence, the direction of the Earth's axis traces out a circular path over a period of approximately 26,000 years.

Precession affects celestial navigation and the position of the stars as seen from Earth. For instance, it causes the position of the North Star to change over thousands of years, leading to different stars becoming the pole star at different times.

In contrast, rotation refers to the spinning of the Earth on its axis, which gives rise to the cycle of day and night. Revolution pertains to the Earth's orbit around the Sun, which defines the length of a year. Translation typically refers to the movement of an object through space without changing its orientation and is not a term that applies to the specific wobbling motion of the Earth's axis. Thus, precession is the most accurate term that describes the effect of the wobbling axis and its long-term implications for Earth's orientation in space.