Published by Patrick Mutisya · 14 days ago
The Moon completes one orbit around the Earth in about 27.3 days (sidereal month). Because the Earth‑Moon system also moves around the Sun, the time between identical phases (the synodic month) is about 29.5 days, which we usually refer to as “one month”.
The appearance of the Moon from Earth depends on the relative positions of the Sun, Earth and Moon. As the Moon travels around the Earth, the illuminated portion that we can see changes in a regular, repeating pattern.
\$\$
\text{Phase angle } \theta = \omega t
\$\$
where \$ \omega = \frac{2\pi}{T} \$ is the angular speed and \$ T \approx 29.5\text{ days} \$ is the synodic period.
| Phase | Position relative to Sun | Illuminated fraction |
|---|---|---|
| New Moon | Moon between Earth and Sun | 0 % |
| Waxing Crescent | Moon moves eastward | 0 % → 50 % |
| First Quarter | Moon 90° east of Sun | ≈50 % |
| Waxing Gibbous | Moon approaching full | 50 % → 100 % |
| Full Moon | Earth between Sun and Moon | 100 % |
| Waning Gibbous | Moon moving away from full | 100 % → 50 % |
| Last Quarter | Moon 90° west of Sun | ≈50 % |
| Waning Crescent | Moon about to become new | 50 % → 0 % |
Suggested diagram: A side view showing the Sun, Earth, and Moon at the eight principal phases, with arrows indicating the Moon’s orbital direction and the relative illumination.