Solar Terms & Seasons

Each solar term is a place on Earth’s orbit. Drag the Earth around the Sun and watch the seasons happen.

Tropics Polar circles Sun overhead Your latitude: the yellow part is daytime — the longer it is, the longer the day (refraction not included) Your place (tap the globe to move it)
What the words mean
From the side you see the sunset line; switch to “Over my place” to see the sunrise line
12:00

now

Next

  • Today
  • Orange tick = current term, white tick = next
  • Where the side view looks from
  • Perihelion
  • Aphelion

Earth’s orbit seen from above the north. The axis always points the same way. Drag the Earth once around the Sun to run through a whole year; each tick is one solar term.

Daylight
Sunrise
Sunset
Noon Sun height
Sun overhead now

— daylight through the year

      How the numbers are computed

      A solar term is the instant the Sun’s apparent ecliptic longitude crosses a multiple of 15°: the March equinox at 0°, the June solstice at 90°, the September equinox at 180°, the December solstice at 270°. The Sun’s position is computed in your browser from the VSOP87 planetary theory (the high-accuracy method in Meeus, Astronomical Algorithms, ch. 25, with the FK5 correction, nutation and aberration), then converted from Dynamical Time to Universal Time with ΔT. Checked against all 96 term instants the National Astronomical Observatory of Japan published for 2020 and 2025–2027, every one agrees within a minute — the published times are themselves rounded to the minute.

      A term is an instant, not a day, so its date depends on the clock you read it by: the Chinese page uses Taiwan time (UTC+8, as Taiwan’s Central Weather Administration does), the Japanese page Japan time (UTC+9, as NAOJ does), and this English page your device’s time zone. Sunrise and sunset use the standard convention of the Sun’s centre 0.833° below the horizon (refraction plus the solar radius), shown in the place’s own time zone; far enough north or south the tool says midnight sun or polar night instead. A place you type in or tap uses the time zone of a preset city within 100 km; anywhere else the zone is estimated from longitude, one hour per 15°, and labelled as estimated.

      Earth imagery is from NASA Earth Observatory: the day side is Blue Marble Next Generation (Reto Stöckli, one composite per month of 2004 — which is why December shows snow across Siberia and the Tibetan Plateau), the night side is Earth at Night 2012 (NASA/NOAA). Use of NASA imagery does not imply NASA’s endorsement. The tool covers the geometry of the Sun and the Earth only; the 72 pentads, lunar months and leap months (see the moon phase tool), weather, and any health or almanac advice are out of scope.

      Quick guide

      Use cases, answers, and nearby tools

      Compact below-tool notes that help first-run users and repeated visitors move faster without changing the main interface.

      Chinese search: 今天是什麼節氣、下一個節氣 日期、為什麼會有四季、冬至 為什麼最冷、節氣 為什麼每年不一樣

      Japanese search: 二十四節気 今日、次の節気 いつ、季節 なぜ 起きる、冬至 夏至 いつ、地軸 傾き 季節

      How to use

      Run a clean first pass

      1. It opens on the present moment: the real Earth lit by the Sun, the current solar term, when it began, and the date and countdown to the next one.
      2. Drag the Earth around its orbit or press “Next term”: in the side view the axis leans toward the Sun at the June solstice and away in December, and the Arctic follows into midnight sun and polar night.
      3. Pick a place, or tap anywhere on the globe, to read its sunrise, sunset and noon Sun height, and a curve of its daylight across the whole year.

      Examples

      Real jobs this page helps with

      • Which solar term is it todayNothing to set up: the current term, how many days this stretch lasts, and a countdown to the next term are on screen as soon as it opens.
      • Midnight sun in the north, long summer days in the southJump to the December solstice with Melbourne or Sydney: the yellow part of your latitude line is the long southern summer day, while the whole Arctic Circle sits in night. Switch to Tromsø and daylight reads “Polar night”.
      • One instant, two calendar datesIn 2026 two terms fall between midnight in Taiwan and midnight in Japan, so the two countries print different dates — the card under the tool lists them.

      FAQ

      What people usually want to know

      How are the solar terms defined, and why do their dates shift by a day or two each year?

      The 24 solar terms use the "fixed qi" method (dìngqì): each term is the exact instant the Sun's apparent ecliptic longitude crosses a multiple of 15°. Because a tropical year is not a whole number of days (~365.2422 d), the instants drift about 6 hours later each year and jump back a day in a leap year, so the same term falls on a window of 1–2 calendar dates. The tool computes each year's actual instants from the astronomical series rather than looking them up in a fixed table.

      Why can the same term fall on different dates in Taiwan and Japan?

      A solar term is an instant, not a day. Taiwan dates terms in UTC+8 (the Central Weather Administration’s convention) and Japan in UTC+9 (NAOJ’s), so an instant close to midnight lands on different calendar days. The 2026 Yǔshuǐ (Rain Water) term is 00:52 on 19 February in Japan but 23:52 on 18 February in Taiwan. The tool lists every such split for the year on screen.

      Earth is closest to the Sun in early January — so why is it winter in the north and summer in the south?

      Seasons come from the tilt of Earth's axis, not its distance from the Sun. Earth passes perihelion between 2 and 5 January, only about 3% closer than at aphelion (roughly 7% more sunlight). At that moment the northern half leans away from the Sun and has winter, while the southern half leans toward it and has summer — the same closest approach gives opposite seasons, which is why distance can't be the cause. The orbit diagram marks perihelion right beside the December solstice.

      How accurate are the times?

      The Sun’s position comes from the VSOP87 planetary theory (the high-accuracy method of Meeus, Astronomical Algorithms, ch. 25, with the FK5 correction, nutation and aberration), and each term is solved for exactly, then corrected for ΔT. Against all 96 term instants published by the National Astronomical Observatory of Japan for 2020 and 2025–2027, every one agrees within a minute — and the published times are themselves rounded to the minute.

      What is left out of scope?

      The 72 pentads (short five-day seasons), lunar month numbering and intercalary months (those belong to the moon-phase tool), weather or temperature data, and any health, dietary, fortune, or astrological content. The tool answers one pair of questions: which solar term it is and why the seasons turn on those days.