Solar Time Calculator

Find the true solar time and local mean time for any place and moment. Pick a city or enter a longitude, set the date and clock time, and see how far your clock is from the Sun, including when solar noon happens.

Apparent (true) solar time11:02:38What a sundial would show
Local mean time11:03:58
Equation of time−1 min 20 s
Solar noon (clock time)12:57
Sun vs. your clock57 min behind
  1. Clock time 12:00 at UTC−4 = 16:00 UTC.
  2. Longitude 74.01° W × 4 min/degree = −296 min 02 s. Local mean time = 16:00 − 4 h 56 min = 11:03:58.
  3. Equation of time on 2026-06-21 = −1 min 20 s. Apparent solar time = 11:03:58 − 1 min 20 s = 11:02:38.
  4. The time zone's reference meridian is 75° W; you are 0.99° east of it (4 min) and daylight saving time moves the clock 1 h ahead. Together with the equation of time, the Sun reaches its highest point at 12:57 instead of 12:00.

Clock time, mean time and solar time

Before railroads, every town set its clocks by the Sun, so noon in Boston came about 12 minutes before noon in New York. Time zones replaced those local times in 1883 in the United States and 1884 worldwide, fixing each zone to a reference meridian every 15° (one hour). The result is convenient, but only places right on the reference meridian keep their clocks close to the Sun. The calculator shows three times:

  • Clock (civil) time: the time of your time zone, including daylight saving time.
  • Local mean time (LMT): UTC shifted by 4 minutes per degree of longitude. Every LMT day is exactly 24 hours.
  • Apparent solar time: LMT plus the equation of time. At 12:00 apparent time the Sun is due south (north in the southern hemisphere) and highest in the sky.

The formula

UTCclock time − UTC offset (including DST)
Local mean timeUTC + 4 min × longitude (east +, west −)
Apparent solar timelocal mean time + equation of time
Solar noon (clock time)12:00 − 4 min × longitude − equation of time + UTC offset

The equation of time uses the NOAA approximation, accurate to about half a minute; solar noon is typically within a minute of an ephemeris. For sunrise, sunset and golden hour, use the golden hour calculator.

Equation of time by month

Month1st (min:s)15th (min:s)
January−2:54−8:38
February−13:10−14:15
March−12:54−9:38
April−4:23−0:14
May+3:01+3:56
June+2:34−0:02
July−3:28−5:47
August−6:30−4:52
September−0:22+4:39
October+10:28+14:24
November+16:23+15:09
December+10:43+4:56

A positive value means the sundial is ahead of mean time. Values repeat almost exactly every year (2026 shown).

How far clocks are from the Sun

Standard time, without the equation of time. During daylight saving time the Sun falls a further hour behind the clock.

CityLongitudeZone meridianMean solar time vs. clock
New York74.01° W75° W4 min ahead
Chicago87.63° W90° W9 min ahead
Los Angeles118.24° W120° W7 min ahead
London0.13° W0° E1 min behind
Madrid3.70° W15° E75 min behind
Paris2.35° E15° E51 min behind
Beijing116.41° E120° E14 min behind
Mumbai72.88° E82.5° E38 min behind
Tokyo139.69° E135° E19 min ahead

Madrid shows how far a clock can drift: Spain has used Central European Time since 1940, even though it lies mostly west of Greenwich. China uses a single UTC+8 zone, which keeps Beijing close to the Sun but leaves Kashgar in the far west almost three hours behind. To compare the official time between places instead, use the time zone converter or the world clock.

Frequently Asked Questions

What is solar time?
Solar time is time measured by the Sun's position. Apparent (true) solar time is what a sundial shows: it is exactly 12:00 when the Sun crosses your meridian. Local mean time smooths out the seasonal wobble so that every day is exactly 24 hours long.

How do you calculate local mean time from longitude?
Take the time in UTC and add 4 minutes for every degree of longitude east (subtract for west). At 87.63° W (Chicago), local mean time is UTC − 350.5 minutes, so 18:00 UTC is 12:09:28 local mean time.

What is the equation of time?
It is the difference between apparent and mean solar time, caused by the tilt of Earth's axis and its elliptical orbit. It ranges from about −14 minutes in mid-February to about +16 minutes in early November and is close to zero around April 15, June 13, September 1 and December 25.

Why is solar noon not at 12:00?
Three things shift it: your distance from the time zone's reference meridian (4 minutes per degree), the equation of time (up to ±16 minutes) and daylight saving time (one hour). In Madrid, far west of the Central European meridian and on summer time, solar noon falls around 14:20 in July.

Is my clock ahead of the Sun?
If you live west of your time zone's reference meridian, yes: the Sun rises, peaks and sets later by the clock. Most of the western part of each U.S. time zone, all of Spain and western China are well behind their clocks.