Islamic Prayer Times

Accurate global prayer times with customizable calculation methods.

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Calculation Settings
Prayer Notifications
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Prayers to Notify

City, Country

Gregorian Date | Hijri Date

Ramadan Kareem

Suhoor Ends

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Fasting Duration

--h --m

Iftar Time

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Tomorrow Suhoor Ends: --:--
Tomorrow Iftar Time: --:--
Next Prayer: -
--:--:--

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Qibla Direction

Direction from your current location toward the Kaaba.

--آ°

N
ًں•‹

Kaaba, Masjid al-Haram, Makkah, Saudi Arabia

Compass accuracy may vary depending on device calibration and nearby magnetic interference.

Today's Scheduled Notifications

Monthly Prayer Timetable

Date Fajr Sunrise Dhuhr Asr Maghrib Isha
Fajr
Dhuhr
Asr
Maghrib
Isha

Loading Annual Timetable, please wait...

Annual Timetable Summary

Calculation Method:
Asr Juristic Method:
High Latitude Adjustment:
Generated On:

Ramadan Calendar

Ramadan Day {day} Date Suhoor Ends Iftar Time
Why do prayer times differ?

Different Islamic organizations use different calculation methods based on varying twilight angles. The Asr time also differs based on juristic opinions: the Standard method (shadow equals the object's length) and the Hanafi method (shadow equals twice the object's length), excluding the noon shadow in both cases. High latitude regions require special adjustments because the sun may not set completely or twilight may not disappear.

Prayer Times FAQs

Prayer times are calculated based on the position of the sun. Different Islamic organizations use slightly different angles of the sun below the horizon to calculate Fajr and Isha, leading to variations in the timetable.

It is generally recommended to follow the method used by your local mosque or regional Islamic authority. For example, ISNA is widely used in North America, while the Muslim World League is common in Europe.

Followed by the Hanafi school, Asr begins when an object's shadow equals twice its own length, excluding the original noon shadow.

Followed by the Shafi'i, Maliki, Hanbali schools and many contemporary prayer calendars, Asr begins when an object's shadow equals its own length, excluding the original noon shadow.

In high latitude regions (like Northern Europe or Canada), the sun may not go far enough below the horizon during summer to calculate true Fajr or Isha times. High latitude rules estimate these times based on proportions of the night or by angle.

Because Fajr and Isha are determined by twilight (the scattering of sunlight in the atmosphere). Different authorities use different degrees of solar depression (e.g., 15°, 18°, or 19°) to define when twilight begins or ends.