◐Salah Atlas

Today’s Salah

Prayer times in Bournemouth

Next prayer--:--

Calculating…

Finding the next prayer

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

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 Fajr and Isha.

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

The difference is the twilight angle.

MethodFajrIshaMeaning
MWL18°17°Earlier Fajr and later Isha
ISNA15°15°Both use a shallower twilight
Egyptian19.5°17.5°Deepest Fajr angle of the three

When the Sun does not reach an angle, the site shows “—”. It does not silently invent an astronomical crossing.

Bournemouth proposal · under review

Khalid Shaukat’s seasonal approach

Shaukat argues that visible dawn and evening twilight change with latitude and season. He collected observations, plotted them by location and day of year, and fitted seasonal minute-offset curves. His method gives Bournemouth usable summer times even when 17° or 18° is not reached.

Summer Fajr75 + (48.1 ÷ 55 × latitude)≈ 119 minutes before sunrise in Bournemouth
Summer Isha75 + (6.14 ÷ 55 × latitude)≈ 81 minutes after sunset in Bournemouth

Evidence note: these coefficients are Shaukat’s empirical curve-fit values, not universal astronomical constants. His paper does not publish enough raw data and statistical detail to independently reconstruct every coefficient. The method is therefore shown as research under local scholarly review, not as the site’s settled default.

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.