The changing appearance of the Moon, known as its phases, is primarily caused by the Moon's orbit around the Earth and the position of the Sun as a directional light source. As the Moon travels around the Earth, different portions of its illuminated side are visible from Earth, resulting in various phases such as new, crescent, half, and full moons. The Earth does not block sunlight from reaching the Moon except during a lunar eclipse, which is a rare event. Typically, the Moon is always half-lit by the Sun, and its visibility changes based on its position relative to the Earth and Sun. During a full moon, the Moon is opposite the Sun, allowing full illumination, while during a new moon, it is positioned between the Earth and Sun, making it mostly dark. Eclipses occur when the Moon aligns with the Earth and Sun at specific points in its orbit, but this alignment is infrequent due to the tilt of the Moon's orbit relative to the Earth's orbit around the Sun.