or

US locations only. Your location is used for this request only and is not stored.

San Diego, CA

DateFajrSunriseDhuhrAsrMaghribIsha
2026-10-115:42 AM6:50 AM12:35 PM3:52 PM6:20 PM7:28 PM
How these times are calculated (method, formulas, worked example, sources)

1. Inputs

PlaceSan Diego, CA
Latitude, longitude32.7157, -117.1647
Date2026-10-11
Time zoneAmerica/Los_Angeles (PDT, UTC-07:00, daylight saving time)
Elevationnot used (sea-level horizon)

2. Method parameters

MethodIslamic Society of North America (ISNA)
Fajr angle15.0°
Isha15.0°
AsrStandard (shadow factor 1)
High-latitude rulenot needed on this date
Adjustmentsnone
Roundingto the nearest minute

3. Formulas

  1. D = JD − 2451545.0
  2. g = 357.529 + 0.98560028 D ; q = 280.459 + 0.98564736 D
  3. L = q + 1.915 sin g + 0.020 sin 2g ; e = 23.439 − 0.00000036 D
  4. RA = atan2(cos e · sin L, cos L) / 15 ; δ = asin(sin e · sin L)
  5. EqT = q/15 − RA
  6. Dhuhr (local mean solar time) = 12 − EqT ; clock time = Dhuhr − λ/15 + UTC offset
  7. T(a) = (1/15) · acos[(sin a − sin φ · sin δ) / (cos φ · cos δ)]
  8. Sunrise = Dhuhr − T(−0.833°) ; Maghrib = Dhuhr + T(−0.833°)
  9. Fajr = Dhuhr − T(−Fajr angle) ; Isha = Dhuhr + T(−Isha angle)
  10. Asr = Dhuhr + T(a) with a = arccot(s + tan|φ − δ(noon)|), s = 1 or 2
  11. 0.833° = 0.567° refraction + 0.2667° solar semi-diameter

φ is latitude, λ longitude (east positive), δ the Sun's declination. The Sun's position is evaluated at each event's own time and the calculation is iterated twice. Clock times come from the IANA time-zone rules, so daylight saving time is always applied correctly.

4. Worked example for 2026-10-11

Sun at solar noon:

JD (0h UT)2461324.5
D9780.3162
g277.0114°
q200.4018°
L198.4963°
e23.43548°
RA13.13751 h
δ-7.24849°
EqT13.356 min
PrayerδaT(a)Solar timeUTCClock time
Fajr-7.1406°-15.000°6.8847 h04:53:3812:42:1805:42
Sunrise-7.1582°-0.833°5.7582 h06:01:1313:49:5206:50
Dhuhr-7.2485°——11:46:3919:35:1812:35
Asr-7.2998°28.549°3.2723 h15:02:5722:51:3615:52
Maghrib-7.3385°-0.833°5.7504 h17:31:3601:20:1618:20
Isha-7.3561°-15.000°6.8756 h18:39:0702:27:4619:28

5. Measured accuracy

The engine is tested against an independent implementation (adhan-js 4.4.6) on 377 cases across 15 US cities and 13 dates, including daylight-saving transition days and Fairbanks, Alaska. The largest difference measured is 59.9 seconds.

Exception: in 5 Alaskan winter cases the Sun barely climbs above the Asr altitude, so Asr becomes very sensitive and differed by up to 4.2 minutes. Pages flag such dates.

6. Limits

  • These are astronomical calculations, not a religious ruling. Mosques publish their own iqama times and may use another method or add a few minutes of caution; follow your local mosque.
  • Elevation and local horizon (mountains, buildings) are not taken into account.

7. Method reference

MethodFajrIsha
Islamic Society of North America (ISNA)15.0°15.0°
Muslim World League (MWL)18.0°17.0°
Egyptian General Authority of Survey19.5°17.5°
University of Islamic Sciences, Karachi18.0°18.0°
Umm al-Qura University, Makkah18.5°90 min after Maghrib (120 in Ramadan)

8. Sources

Methodology v1.0, reviewed 2026-10 · engine 1.0. Methodology and changelog

How latitude changes the times today

CityLatitudeFajrIshaDaylight
Miami, FL25.8°11 h 39 min
Houston, TX29.8°11 h 34 min
New York City, NY40.7°11 h 19 min
Chicago, IL41.9°11 h 16 min
Seattle, WA47.6°11 h 05 min
Anchorage, AK61.2°10 h 27 min

The farther north, the longer twilight lasts in summer and the shorter in winter, so the gap between Fajr and sunrise, and between Maghrib and Isha, changes much more in Seattle or Anchorage than in Miami. Times are local time in each city.

What the options mean

Method

  • Islamic Society of North America (ISNA): Fajr 15.0°, Isha 15.0°
  • Muslim World League (MWL): Fajr 18.0°, Isha 17.0°
  • Egyptian General Authority of Survey: Fajr 19.5°, Isha 17.5°
  • University of Islamic Sciences, Karachi: Fajr 18.0°, Isha 18.0°
  • Umm al-Qura University, Makkah: Fajr 18.5°, Isha 90 minutes after Maghrib

Asr

Standard (Shafi'i, Maliki, Hanbali): Asr begins when a shadow equals the object's length plus its noon shadow. Hanafi: twice the length plus the noon shadow, which is later in the afternoon.

High latitudes

Above about 48.5° north, or whenever the Sun does not reach the Fajr or Isha angle, a rule limits how far into the night those times can fall: angle-based (a fraction of the night proportional to the angle), one-seventh of the night, or the middle of the night. The result page says when a rule was used.

Days

Choose up to 31 days to get a timetable you can print. Each day is calculated separately, including daylight-saving changes.

Questions

How accurate is the calculator?

It uses the same engine as every page on this site, tested against an independent open-source implementation; the measured differences are published on our methodology page. Your local mosque may still differ by a few minutes because of its method or safety margins.

Can I use a ZIP code?

Yes. Enter a US ZIP code, or latitude and longitude, or use your device's location. Nothing you enter is stored.

Why are Fajr and Isha so different between methods?

They are defined by how dark the sky is, measured as the Sun's angle below the horizon. A few degrees of difference in that angle move the time by 10 to 40 minutes.

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