◐Salah Atlas

Today’s Salah

Prayer times in Bournemouth

Next prayer--:--

Calculating…

Finding the next prayer

—
Dawn · Sunrise—Cutoff —
Dusk · Sunset—Maghrib —
⌖
Seasonal calculationDhuhr +5 minMaghrib +2 min

Fajr and Isha are seasonal estimates. Check your mosque’s adopted timetable.

Research & local guidance

See how every time is calculated.

Explore the astronomy behind prayer times, the Bournemouth summer-twilight question, calculation methods, safety buffers, and mosque information—all kept away from the daily prayer screen.

One important distinctionCalculated: the Sun physically reaches the selected angle.Estimated: a high-latitude rule supplies a prayer time when that angle is not reached.

Interactive diagram · Bournemouth only

How deep below the horizon?

50.7192° N · 1.8808° W
Selected night21 June 2026
Deepest point−15.8°17° and 18° are not reached
21 June
Horizon 0°Civil 6°Nautical 12°Prayer methods 15°–18°

Sun’s lowest position during each night

The Sun’s deepest nightly position in Bournemouth during 2026An interactive line graph showing that the Sun descends only about 15.8 degrees below the horizon near 21 June.

Time spent below each line on this night

Hours the Sun stays below each twilight angleBars show how long the Sun stays below the horizon and below 6, 12, 15, 17 and 18 degrees.

In 2026, Bournemouth does not reach 18° for part of late spring and summer.

How Salah Atlas calculates

From the Sun’s position to your clock.

01

Date and coordinates

We use the selected city’s latitude and longitude. The diagram above is fixed to Bournemouth so its claim stays local and testable.

02

Sun’s declination

Earth’s tilt and orbit determine how far north or south the Sun appears on that date.

03

Hour angle

The hour-angle equation finds when the Sun crosses the required altitude: −0.833° for sunrise or sunset, and the selected twilight angle for angle-based Fajr and Isha. Seasonal uses the date-and-latitude rules below.

04

Local clock time

Longitude, the equation of time and the location’s time zone convert the solar event to local clock time.

Core solar equationcos H = (sin h − sin φ sin δ) ÷ (cos φ cos δ)h = chosen Sun altitude · φ = latitude · δ = solar declination

Methods currently selectable

Seasonal estimates and fixed angles.

MethodFajrIshaMeaning
SeasonalVariesVariesLatitude, season and night-length rules
MWL18°17°Earlier Fajr and later Isha
ISNA15°15°Both use a shallower twilight
Egyptian19.5°17.5°Deepest Fajr angle of the three

The fixed-angle methods show “—” if the Sun never reaches the required angle. Seasonal supplies explicitly labelled estimates. The default is Seasonal for UK locations and 50°–61° north; MWL elsewhere. This latitude band is the site’s preference, not a claim of religious consensus. You can change the method; your choice is remembered for each location on this device. “My location” uses your device’s time zone; check it when travelling.

Understanding twilight

Seasonal research

Twilight lasts longer or shorter depending on your latitude and the time of year. Seasonal estimates Fajr before sunrise and Isha after sunset using these changes, with additional rules for northern locations.

Fajr estimateSunrise − seasonal minutesThe minute interval varies through the year.
Isha estimateSunset + seasonal minutesUses the general-shafaq curve, before the Maghrib buffer.

The rules used on this site

  • Below 55°: compare the seasonal curve with 18° twilight. Use the later Fajr and earlier Isha; if 18° is absent, use the seasonal estimate.
  • 55° and above: Fajr cannot be earlier than the last seventh of the preceding sunset-to-sunrise night; Isha cannot be later than the first seventh of the following night. Compare these limits with the seasonal curve.
  • Above 60°: if daylight exceeds 18 hours, is below 6 hours, or there is no sunrise/sunset, estimate Fajr and Isha at 60° with the same longitude. Actual sunrise/sunset remain location-specific and show “—” where absent.
See the complete seasonal maths

Let L be absolute latitude. The four anchor values in minutes are:

Fajr: A = 75 + 28.65L/55; B = 75 + 19.44L/55; C = 75 + 32.74L/55; D = 75 + 48.1L/55.

Isha (general): A = 75 + 25.6L/55; B = 75 + 2.05L/55; C = 75 − 9.21L/55; D = 75 + 6.14L/55.

Count days from 21 December in the northern hemisphere, or 21 June in the southern hemisphere. Interpolate in straight lines between A, B, C, D, C, B, A at days 0, 91, 137, 183, 229, 275, 366. Actual elapsed days include leap days; the cycle resets on the next anchor date. Then apply the latitude rules above.

These are empirical coefficients, not universal physical constants. No extra Fajr or Isha buffer is added. Sunrise cutoff −2 minutes, Maghrib +2 minutes and Dhuhr +5 minutes are separate site settings.

Sources: seasonal model — Moonsighting.com, Fajr and Isha (2015), sections 11–12; solar calculations — NOAA; horizon definitions — U.S. Naval Observatory. Follow your mosque’s adopted timetable.

Precaution used on this site

Small buffers are shown openly.

Sunrise/Fajr cutoff 2 minutes before calculated sunriseDhuhr 5 minutes after calculated solar noonMaghrib 2 minutes after calculated sunset

Prayer nearby

Mosques in Bournemouth

Local mosque information loads only after you select or confirm a city. Each mosque links to its official timetable where available because jamaat times are set locally and cannot be safely estimated.

Select a city to load local mosque times.

Sources and limitations

Check the reasoning.

Calculated solar position is highly predictable. Visible twilight can still vary with cloud, humidity, aerosols, light pollution, observer height and the local horizon. Islamic dates also require a separate moon-sighting policy.

Sunrise & sunset explorer

A year of changing light

Drag the graph left or right to move through dates and years. Tap a day to see its times. Use the slider or arrow keys for precise selection.

Sunrise—
Sunset—
Daylight—
Sunrise and sunset throughout the yearLocal clock time on the vertical axis, date on the horizontal axis. Sunrise is blue and sunset is orange.

Calculated solar events before the 2-minute prayer buffers. Times use the selected location’s time zone; clock-change jumps are expected. Browse 1900–2100. Historical and future clock rules depend on your browser’s time-zone data. Level horizon and average atmospheric conditions are assumed.