Moon Phase Visualizer
Astronomical phase tool, drift calculator, and lunar event calendar for moonphase watch owners
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Moon as seen from Earth
Is Your Moonphase Still Accurate?
Calculate how far your moonphase complication has drifted since you last set it
Select a date above to calculate your moonphase drift
Lunar Calendar
Upcoming Lunar Events
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For Collectors
The Moonphase Complication
A Brief History
The moonphase complication is one of the oldest in watchmaking, dating to the 17th century. Before electric lighting, the Moon was a practical source of illumination - farmers, sailors, and travelers depended on knowing the lunar cycle. Today, the moonphase endures as one of the most romantic and visually distinctive complications, prized for its artistry as much as its astronomical function.
How the Mechanism Works
At its heart, a moonphase display uses a disc with two identical moons painted on it. This disc sits beneath a shaped aperture on the dial. A 59-tooth star wheel is advanced one tooth per day by a finger attached to the 24-hour wheel. Since 59 ÷ 2 = 29.5, each “moon” takes 29.5 days to cross the aperture - closely approximating the 29.53-day synodic month. The error of ~44 minutes per month means the display loses roughly one full day every 2 years and 8 months.
Precision Tiers
Most mechanical moonphase watches
Patek Philippe Cal. 240 LU CL, A. Lange & Sohne Lange 1 Moon Phase, IWC Portugieser Perpetual
Andreas Strehler Lune Exacte, some grand complication pieces
Notable Moonphase Watches
Setting Your Moonphase
- Find the date of the last full moon (check the lunar calendar below).
- Pull the crown to the moonphase setting position (consult your manual).
- Advance the moonphase indicator until it shows a full moon centered in the aperture.
- Count the days between the last full moon and today.
- Press the moonphase corrector that many times (one press = one day).
- Push the crown back in. Your moonphase is now set accurately.
Learn
How Moon Phases Work
The Synodic Month
A complete lunar cycle takes 29.53059 days - the time it takes for the Moon to return to the same phase as seen from Earth. This is called the synodic month, and it’s the fundamental number that every moonphase watch complication attempts to replicate mechanically. The Moon doesn’t produce its own light; we see it because it reflects sunlight. As the Moon orbits Earth, the angle between the Sun, Earth, and Moon changes, illuminating different portions of the lunar surface.
The Eight Phases
The lunar cycle is divided into eight named phases. It begins with the New Moon (phase 0.0), when the Moon sits between the Earth and Sun with its illuminated side facing away from us. The cycle progresses through Waxing Crescent, First Quarter (half-lit), and Waxing Gibbous to reach the Full Moon (phase 0.5), when the Moon is fully illuminated. It then wanes through Waning Gibbous, Last Quarter, and Waning Crescent before returning to New Moon.
Phase vs. Illumination
Phase position and illumination percentage are related but not identical. At First Quarter (phase 0.25), the Moon is roughly 50% illuminated - not 25%. This is because illumination follows a sinusoidal curve, not a linear one. Your moonphase watch disc tracks the phase position (the Moon’s orbital position), which is why the disc rotates at a constant rate rather than matching the non-linear illumination curve.
Why the Moon’s Orbit Matters to Watches
The Moon’s orbit is elliptical, not circular. At perigee (closest approach), the Moon is about 356,500 km away; at apogee (farthest), about 406,700 km. When a full moon coincides with perigee, we call it a supermoon - it appears roughly 14% larger and 30% brighter. While your watch complication doesn’t account for this variation, it’s a fascinating reminder that the mechanism on your wrist is tracking a real celestial body on an imperfect orbit.
Eclipses and Blood Moons
A lunar eclipse occurs when the Earth passes between the Sun and Moon, casting its shadow on the lunar surface. During a total lunar eclipse, the Moon turns a deep red - a blood moon - because Earth’s atmosphere refracts sunlight, filtering out blue wavelengths and bending red light onto the Moon. Eclipses don’t happen every full moon because the Moon’s orbit is tilted about 5° relative to Earth’s orbital plane. Only when the Moon crosses this plane near a full moon does an eclipse occur - roughly 2–5 times per year.