فِقهُ الأَوقَاتِ وَالمَوَاقِيت — أَوقَاتُ الصَّلَاةِ فِي الفِقهِ الإِسلَامِيّ: كَيفِيَّةُ تَحدِيدِ أَوقَاتِ الصَّلَوَاتِ الخَمسِ مِن مَوضِعِ الشَّمسِ وَتَعرِيفَاتُ الفَجرِ وَالعِشَاءِ المُتَنَازَعُ عَلَيهَا وَالخِلَافُ الحَنَفِيُّ الشَّافِعِيُّ بِشَأنِ العَصرِ وَجَمعُ الصَّلَوَاتِ أَثنَاءَ السَّفَرِ وَفِقهُ البُلدَانِ الوَاقِعَةِ عَلَى خُطُوطِ عَرضٍ مُرتَفِعَة
Fiqh al-Awqat wal-Mawaqit (فِقهُ الأَوقَاتِ وَالمَوَاقِيت — Jurisprudence of Prayer Times; *awqat* [pl. of *waqt*]: times; *mawaqit* [pl. of *miqat*]: the designated times/places; the five prayer times: [1] fajr [dawn]: from true dawn [fajr sadiq — the horizontal whiteness spreading across the horizon] until sunrise; [2] dhuhr [midday]: from when the sun passes its zenith [zawal] until the beginning of asr time; [3] asr [afternoon]: from a shadow equaling the object's height [Shafi'i/Hanbali] OR equaling twice the object's height [Hanafi — asr preferred time begins at single shadow, obligatory at double shadow] until sunset; [4] maghrib [sunset]: from sunset until the red glow [shafaq ahmar] disappears [Shafi'i] OR until the white twilight [shafaq abyad] disappears [Hanafi]; [5] isha [night]: from when the twilight disappears [as per school's maghrib end definition] until midnight [shar'i midnight = half of night] or dawn; the fajr dispute: true dawn [fajr sadiq] vs false dawn [fajr kadhib — a vertical column of light appearing before true dawn]; all schools agree fajr time begins with fajr sadiq; the Hanafi preferred time for fajr is at isfar [when dawn brightens sufficiently to see faces]; the asr dispute — the most significant madhab difference in prayer times: Hanafi: a shadow equaling once the object's height ends dhuhr time and begins asr's preferred time; when the shadow equals twice the object's height, asr's preferred time ends [but asr remains valid until sunset; the second shadow is the preferred time for asr]; Shafi'i/Maliki/Hanbali: when the shadow equals once the object's height, asr time begins directly; in practice: this creates a 45-90 minute difference in asr time in most latitudes; combining prayers: the Shafi'i school permits combining dhuhr+asr and maghrib+isha while traveling [jam' al-taqdim — combining early, or jam' al-ta'khir — combining late]; the Hanafi school does not permit combining while traveling [except at Muzdalifa during hajj as textually specified]; the Maliki school permits it while traveling; the high-latitude problem: at latitudes above approximately 49 degrees North in summer, the sun does not set far enough below the horizon for isha twilight to disappear; in extreme cases above the Arctic Circle, the sun does not set at all; fiqh solutions: [1] follow Mecca or Medina times; [2] follow the nearest country where proper times exist; [3] divide the night proportionally [the most common contemporary fatwa]; [4] the 18-degree convention [some national councils use 18 degrees below horizon for fajr and isha, approximating temperate times]; the missed prayer [fawat]: if a prayer is missed entirely, it must be made up as qada; missing a prayer intentionally has no prescribed expiation [kaffarah] beyond sincere repentance and making it up) is the foundational temporal framework of Islamic worship.
The Solar Framework
The five daily prayers are tied to the sun’s position in a way that creates a living astronomical clock. Each prayer has a waqt (time window) with a beginning and end determined by the sun’s actual position rather than an arbitrary clock. Dhuhr begins when the sun passes its zenith and a shadow begins growing behind an object; Asr begins when that shadow reaches a certain length; Maghrib begins at sunset.
This system means prayer times move with the seasons and vary by latitude — a feature that was entirely natural for a pre-industrial agricultural society but creates genuinely novel challenges at high latitudes.
The Asr Dispute
The most practically significant disagreement between schools is over Asr time. The Hanafi position: Asr’s preferred time begins when a shadow equals twice the object’s length (beyond the original shadow at noon). The Shafi’i/Maliki/Hanbali position: Asr begins when the shadow equals once the object’s length beyond the noon shadow. In practice, this creates a 45-90 minute difference in mid-latitudes. Communities with mixed madhhab membership often notice different prayer schedules for the same prayer.
The High-Latitude Problem
At latitudes above roughly 49°N in summer, the sun doesn’t descend far enough below the horizon for Isha twilight to properly disappear. The problem intensifies toward the Arctic Circle. Contemporary Muslim communities in Scandinavia, Scotland, Canada, and northern Russia face this challenge for several months each year.
The most widely adopted contemporary solution is proportional night division: divide the night between sunset and sunrise by the standard ratio of Maghrib-to-Isha and Isha-to-Fajr from a temperate location (usually the same ratio as the nearest country with proper times). This ensures prayers remain distributed through the night even when the solar definition breaks down.
See also: Fiqh Al Tahara, Fiqh Al Ahkam Al Khamsah, Fiqh Al Ijtihad Wal Taqlid, Fiqh Al Aqd Wal Shurut, Fiqh Al Usul Al Fiqh