A lunar calendar that keeps its months fixed to the seasons by inserting an intercalary month (“Nasi’”) following the Metonic cycle — calibrated to the eclipse of 27 January 632 CE and computed with real astronomical algorithms (conjunction + solar longitude).
| # | Month | Starts (Gregorian) | Season |
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This is a lunisolar calendar, like the Hebrew and Chinese calendars: its months follow the Moon (one month from conjunction to conjunction), but a leap month is periodically inserted so each month stays fixed to its season. This differs from the Hijri calendar, which is purely lunar — its months drift through the seasons.
The calendar is calibrated to a certain astronomical event: the eclipse of 27 January 632 CE (“Muhammad’s eclipse”), which occurred at the death of Ibrahim, the Prophet’s son (pbuh). A solar eclipse can only occur at conjunction, so it is a precisely defined conjunction point per NASA’s computations. The calculation places it in late Shawwal, 10 AH, matching the historical sources.
The mean synodic month (conjunction to conjunction):
Each conjunction instant is actually computed with Meeus’ algorithm (Chapter 49), accurate to under one minute even back to the 7th century CE.
The year begins at the conjunction nearest the moment the Sun reaches the same ecliptic longitude it had at 1 Muharram 1 AH. The Sun’s position is computed with Meeus’ algorithm (Chapter 25), keeping the new year tied to a fixed season.
It rests on the astronomical fact:
Only impossibility is judged (never possibility) at sunset at the visitor’s location:
The Sun and Moon positions and the sunset instant are computed astronomically for the visitor’s coordinates. Passing both thresholds does not imply visibility — that depends on the horizon, atmosphere, and eyesight.
We offer this tool as an aid to enthusiasts, students, and researchers in astronomy, calendars, and history — a means of exploration and of comparing calendars and understanding the relationship between astronomical and historical events.
It is not a substitute for any adopted calendar, carries no religious authority for acts of worship such as fasting, Hajj, or festivals, and holds no official academic standing to be cited like peer-reviewed sources. Worship timings are determined by the competent religious authorities and recognised crescent sighting; scholarly research refers to its primary sources.
What this tool provides is an independent, verifiable astronomical computation — to be consulted, not invoked as proof, and corrected whenever an error is shown.