Calculate today's Fajr, Dhuhr, Asr, Maghrib, and Isha times for your location and see a live countdown to the next prayer. Allow location access or search for your city.
Prayer times come from the sun's altitude. Fajr and Isha shift by several minutes depending on the reference angle a region uses — commonly between 15° and 19° — and Asr depends on the shadow-length rule of your madhab. Match those two settings first when comparing with a local timetable.
Fajr is the dawn prayer. Its time runs from astronomical twilight, when the sky first begins to lighten, until sunrise.
Dhuhr, the midday prayer, enters just after the sun passes its zenith.
Asr is the afternoon prayer. It begins when an object's shadow reaches a defined multiple of its length.
Maghrib follows immediately after sunset.
Isha, the night prayer, begins once the evening twilight has disappeared.
All five are therefore functions of latitude, longitude and date. Even in one city they shift by minutes every day through the year.
Fajr and Isha are defined by how far the sun sits below the horizon, and different bodies settled on different angles.
MWL (Muslim World League) uses Fajr 18°, Isha 17°, and is the most widely used.
ISNA (Islamic Society of North America) uses 15°/15°, set lower to keep times workable at North American latitudes.
Umm al-Qura sets Fajr at 18.5° and fixes Isha at 90 minutes after Maghrib (120 in Ramadan) rather than an angle. It is the Saudi standard.
The Egyptian General Authority uses 19.5°/17.5°.
The differences are practical: Fajr can vary by more than twenty minutes between methods in the same city. Use whichever your community or local mosque follows.
Asr is defined by shadow length, measured from the minimum shadow an object casts at midday.
Standard (Shafi'i, Maliki, Hanbali) — factor 1, when the shadow equals the object's length.
Hanafi — factor 2, when it reaches twice the length, which falls 30 to 60 minutes later depending on season.
Both are valid positions. Select the one you follow.
Above roughly 48° latitude, the sun in summer never descends to the required angle. Twilight persists all night and Fajr and Isha cease to exist as calculated times.
This is a real problem across northern Europe, northern Canada and Russia, and several conventions address it:
Middle of the Night splits the interval between Maghrib and Fajr in half.
One-Seventh of the Night divides the night into sevenths and allocates from there.
The angle-based convention borrows the pattern from a lower latitude.
This is a limitation of the calculation rather than an error. Follow the guidance of Islamic authorities in your region.
Use device GPS with permission, or search for a city.
Precision requirements are modest. One degree of longitude (about 80km) shifts times by roughly four minutes, so a few kilometres within a city changes nothing meaningful.
Latitude has more seasonal effect. Reset your location after travelling any significant distance north or south.
Everything is computed in the browser. Your location is not transmitted, and a page already loaded keeps working without a connection.
The astronomical computation itself is precise. But it can differ by minutes from your local mosque's published schedule.
Mosques may use a different calculation method, add a precautionary margin, or round to local convention.
For something that should not be wrong, use this as a reference and treat your mosque's timetable as authoritative.
From your latitude and longitude, the date, and your chosen calculation method (MWL, ISNA, Umm al-Qura, and others). It runs entirely offline in your browser.
Different organizations use different sun-angle conventions for Fajr and Isha, and the Asr time depends on your madhab (Shafi or Hanafi).
Search for your new city, or refresh location permission, and times recalculate for wherever you are.
Yes. Namaz (Urdu, Hindi, Turkish), solat or sholat (Malay, Indonesian), and salah or salat (Arabic) all refer to the same five daily prayers, so this page covers namaz timings, jadwal sholat, and adhan times alike.
What this tool bases its numbers on, and how far those numbers go.
Solar position is computed for your latitude, longitude and date, entirely in the browser. Dhuhr follows solar noon, Maghrib follows sunset, and Fajr and Isha are set by the twilight angle of the method you choose (MWL, ISNA, Umm al-Qura and others). Asr follows the shadow-length rule of your madhab: the Shafi rule adds one object length to the noon shadow, the Hanafi rule adds two.For a 1-metre pole casting a 0.5-metre shadow at noon, Asr under the Shafi rule begins when the shadow reaches 1.5 metres, and under the Hanafi rule when it reaches 2.5 metres — later in the afternoon.