Solar noon, solstice and equinox calculator

Find the exact time of solar noon for any place and date, the height of the noon sun, the equation of time, and the dates and local times of the coming solstices and equinoxes.

Solar noon 12:46 PM Solar noon is 46 min after 12:00 today.
Sun height at noon 45.9° Sun direction: S
Equation of time +10.4 min sundial ahead
Next solstice or equinox December solstice December 21, 2026 · in 81 days

Solstices and equinoxes

EventLocal timeUTC
March equinox 2026Mar 20, 2026, 10:46 AMMar 20, 2026, 14:46
June solstice 2026Jun 21, 2026, 4:25 AMJun 21, 2026, 08:25
September equinox 2026Sep 22, 2026, 8:06 PMSep 23, 2026, 00:06
December solstice 2026Dec 21, 2026, 3:50 PMDec 21, 2026, 20:50in 81 days
March equinox 2027Mar 20, 2027, 4:25 PMMar 20, 2027, 20:25in 170 days
June solstice 2027Jun 21, 2027, 10:11 AMJun 21, 2027, 14:11in 263 days
September equinox 2027Sep 23, 2027, 2:01 AMSep 23, 2027, 06:01in 356 days
December solstice 2027Dec 21, 2027, 9:42 PMDec 22, 2027, 02:42in 446 days

Solar noon through the year

Solar noon through the year11:3012:0012:301:001:30JanFebMarAprMayJunJulAugSepOctNovDec

Equation of time through the year

Equation of time through the yearHow far a sundial is ahead of (positive) or behind (negative) the clock average. It is the reason solar noon drifts through the year.-15 min-10 min-5 min0 min+5 min+10 min+15 minJanFebMarAprMayJunJulAugSepOctNovDec

How far a sundial is ahead of (positive) or behind (negative) the clock average. It is the reason solar noon drifts through the year.

Analemma

AnalemmaThe figure-eight traced by the sun if you note its position at the same clock time every day: height (vertical) against the equation of time (horizontal).-150+1530°40°50°60°70°JanFebMarAprMayJunJulAugSepOctNovDec

The figure-eight traced by the sun if you note its position at the same clock time every day: height (vertical) against the equation of time (horizontal).

Sun path

Sun pathThe sun’s path across the sky seen from above: the centre is straight overhead, the edge is the horizon. Solid: selected day. Dashed: June and December solstices.30°60°NESW8910111212345
  • Selected day
  • June solstice
  • December solstice

The sun’s path across the sky seen from above: the centre is straight overhead, the edge is the horizon. Solid: selected day. Dashed: June and December solstices.

Calculated with Astronomy Engine, an open-source library verified against the US Naval Observatory and NASA JPL. How we calculate

How to use this tool

  1. Choose a place and date. The card shows solar noon, the sun’s height at that moment and today’s equation of time.
  2. Check the coming seasons. The table lists the solstices and equinoxes of this year and next, in local time and UTC, with a countdown to the next one.
  3. Explore the charts. See how solar noon drifts through the year, the equation of time curve, the analemma and the sun path diagram.

What moves solar noon

  • Longitude within the time zone. Every degree west of the time zone’s reference meridian makes solar noon 4 minutes later.
  • Daylight saving time adds one hour in summer.
  • The equation of time shifts solar noon by up to about 16 minutes through the year.

The guide what is solar noon explains each effect with a worked example, and why the earliest sunset is not on the shortest day shows the most visible consequence of the equation of time.

The analemma

If you photographed the sun at exactly the same clock time every day for a year, it would trace a figure eight in the sky: the analemma. Its height comes from the sun’s changing declination through the seasons; its width comes from the equation of time. The chart shows the analemma for the selected place, with the sun’s position on the selected date marked.

Solstices and equinoxes

Solstices and equinoxes are exact moments, not whole days. At the solstices the sun reaches its northernmost or southernmost point; at the equinoxes it crosses the celestial equator. Their local date can differ from the UTC date: the December solstice 2026 falls at 20:50 UTC on 21 December, which is already 22 December in Tokyo and Sydney. More in solstices and equinoxes explained, and on the pages for each coming event.

Uses

  • Finding true north: at solar noon, vertical shadows point exactly north (in the Northern Hemisphere outside the tropics).
  • Photography: noon light is the hardest and shadows are shortest.
  • Sun protection: UV radiation peaks around solar noon, not 12:00.
  • Solar panels: south-facing panels produce most around solar noon.

Last updated September 23, 2026

Frequently asked questions

What is solar noon?

The moment when the sun crosses the local meridian and is highest in the sky. At that moment it is due south (or due north in the Southern Hemisphere, and in the tropics it can be either).

Why is solar noon not at 12:00?

Because of your position within the time zone, daylight saving time and the equation of time. Together they can move solar noon by more than an hour.

What is the equation of time?

The difference between sundial time and average clock time. It varies through the year between about −14 and +16 minutes, because Earth's orbit is elliptical and its axis is tilted.

How precise are the solstice times?

The moments are calculated to within about a minute. They are the same instant everywhere; only the local clock time differs.