Lunar Phase Calculator
Calculate lunar phases and visibility for specific geographic locations.
Today's Moon
9/29/2025 - Check any date below
Select date to calculate moon phase
Methodology
This calculator uses the standard astronomical synodic month of 29.53058770576 days with January 6, 2000 (12:24 PM) as the reference new moon. Moon phases are determined based on the lunar day position within the cycle, following the same methodology used by professional astronomical software.
Important Disclaimers:
- This calculator provides accuracy suitable for amateur astronomy and general purposes
- Results are based on standard astronomical algorithms and reference dates
- For professional astronomical research, more precise ephemeris data may be required
- Moon phase times are approximate and may vary slightly from other sources
- Local viewing conditions and atmospheric effects are not considered
About This Calculator
1. How accurate is this moon phase calculator?
This calculator uses the standard astronomical synodic month of 29.53058770576 days and is accurate for most practical purposes. The calculations are based on the same methods used by professional astronomical software, with accuracy suitable for amateur astronomy, photography, and general interest.
2. What is the difference between lunar day and calendar day?
A lunar day in this context refers to the number of days elapsed since the last new moon in the current lunar cycle. It ranges from 0 to about 29.5 days. This is different from a calendar day, which is a 24-hour period in our standard timekeeping system.
3. Why do moon phases repeat every 29.53 days?
This period, called a synodic month, is the time it takes for the Moon to return to the same phase as seen from Earth. It's longer than the Moon's orbital period (27.3 days) because Earth is also moving in its orbit around the Sun, so the Moon needs extra time to 'catch up' to the same Sun-Earth-Moon alignment.
4. Can I use this calculator for historical dates?
Yes, this calculator works for dates both in the past and future, though accuracy may decrease for dates very far from the reference point (January 6, 2000). For historical astronomical research, more sophisticated calculations accounting for long-term orbital variations might be needed.