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Equinox and Solstice Calculator

Gives the exact instant of both equinoxes and both solstices for any year from 2000 to 2999, with the season lengths they produce.

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The instants are given in this offset. Daylight saving is not applied.
Enter your figures and press Calculate.
In short An equinox or solstice is an instant, not a day. It is defined purely by the sun apparent longitude: 0 degrees at the March equinox, 90 at the June solstice, 180 in September and 270 in December. Everything people associate with them — equal day and night, the longest day — is a consequence, and not always an exact one. Because they are instants, which calendar date they land on depends on your time zone, and that is why the March equinox is sometimes the 20th and sometimes the 21st. The 2026 March equinox falls at 14:46 UT on 20 March. The seasons are not equal in length, and the reason is the shape of the earth orbit. In 2026 northern spring runs 92.74 days, summer 93.65, autumn 89.86 and winter 88.98 — a spread of nearly five days between the longest and shortest. The earth is near aphelion, its furthest point from the sun, during northern summer, and by Kepler second law it moves slowest when it is furthest away, so it takes longer to cover that 90 degrees of orbit. Northern winter is the shortest season because the earth is near perihelion in early January and moving at its fastest. Two things worth knowing that follow from all this. The equinox day is not twelve hours long — it runs several minutes over, everywhere, because sunrise is measured on the sun upper limb and includes refraction. And the earliest sunset does not fall on the shortest day: the equation of time shifts solar noon through December, so the earliest sunset comes a week or two before the solstice and the latest sunrise a week or two after it.

How to use the Equinox and Solstice Calculator

  1. Enter the year.
  2. Set the UTC offset you want the instants in.
  3. Read the four times and the season lengths they produce.

About the Equinox and Solstice Calculator

The four seasonal instants for any year, with the season lengths and the reason they are unequal.

What people use it for

  • Finding the exact equinox or solstice time in your own time zone.
  • Settling which calendar date it falls on this year.
  • Seeing why the seasons are not the same length.

Details

March equinoxsun apparent longitude exactly 0°
June solstice90°, September 180°, December 270°
2026 March equinox20 March, 14:46 UT
2026 northern summer93.65 days — the longest season
2026 northern winter88.98 days — the shortest
Whythe earth is slowest at aphelion, in northern summer
PrivacyEverything runs in your browser. No location lookup, nothing sent anywhere
The table includes an "off target" column, which is this page checking itself: the instants come from one series and the sun longitude from a separate solar theory, and every row landing within an arcsecond or two of its defining angle is evidence that both are right.

Where this tool stops

The series covers the years 2000 to 2999 and is accurate to under a minute across that range. Times are Universal Time shifted by the offset you enter, with no daylight-saving adjustment.

Frequently asked questions

When is the equinox this year?
Enter the year above. The 2026 March equinox is at 14:46 UT on 20 March; the tool gives all four instants in whatever UTC offset you choose.
Why does the equinox date change?
Because it is an instant, not a day, and a year is not a whole number of days. The instant drifts through 20 and 21 March and is pulled back by each leap year, and which date it lands on also depends on your time zone.
Are the seasons the same length?
No. In 2026 northern summer is 93.65 days and winter 88.98 — nearly five days apart. The earth moves slowest when it is furthest from the sun, which happens during northern summer.
Is the equinox a day of equal day and night?
Not exactly. Sunrise and sunset are defined on the sun upper limb and include refraction, so the equinox day runs several minutes over twelve hours everywhere on earth.
Why is the earliest sunset before the shortest day?
Because the equation of time is shifting solar noon later through December. The earliest sunset comes a week or two before the solstice and the latest sunrise a week or two after it, while the shortest day sits between them.
What defines a solstice exactly?
The instant the sun apparent longitude reaches 90 or 270 degrees, which is when its declination is at its greatest north or south. Everything else about the day follows from that.
Is the Equinox and Solstice Calculator free, or is there a paid tier?
Free, unlimited, and no email address required. You can use it a hundred times a day and nothing changes.
Does anything I enter leave my computer?
No. The Equinox and Solstice Calculator runs entirely in your browser using JavaScript. Because the work happens locally, the utility also keeps working if your connection drops, and closing the tab is all it takes to discard everything.
When would I actually need the Equinox and Solstice Calculator?
The jobs it is built for: finding the exact equinox or solstice time in your own time zone. Settling which calendar date it falls on this year. Seeing why the seasons are not the same length. It is built for exactly those cases rather than being a general-purpose tool with this bolted on.
Where does the Equinox and Solstice Calculator stop being reliable?
The series covers the years 2000 to 2999 and is accurate to under a minute across that range. Times are Universal Time shifted by the offset you enter, with no daylight-saving adjustment. Knowing where a tool stops being trustworthy matters more than the cases where it works.
What are the key numbers for the Equinox and Solstice Calculator?
March equinox is sun apparent longitude exactly 0°. June solstice is 90°, September 180°, December 270°. 2026 March equinox is 20 March, 14:46 UT. These are printed on the page itself, so you do not have to take them on trust.
How precise is the result?
The calculation runs in double precision and the result is shown to ten significant figures, so converting a value and converting it back returns the original. What is displayed is rounded for readability; what is copied is not.

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