For a listing of the dates and times of solstices and equinoxes through 2030, page down.
For more information, see the U.S. Naval Observatory's Astronomical Information Center (navy.mil).
There are only two times of the year when the Earth's axis is tilted neither toward nor away from the sun, resulting in a "nearly" equal amount of daylight and darkness at all latitudes. These events are referred to as Equinoxes.The word equinox is derived from two Latin words - aequus (equal) and nox (night). At the equator, the sun is directly overhead at noon on these two equinoxes. The "nearly" equal hours of day and night is due to refraction of sunlight or a bending of the light's rays that causes the sun to appear above the horizon when the actual position of the sun is below the horizon. Additionally, the days become a little longer at the higher latitudes (those at a distance from the equator) because it takes the sun longer to rise and set. Therefore, on the equinox and for several days before and after the equinox, the length of day will range from about 12 hours and six and one-half minutes at the equator, to 12 hours and 8 minutes at 30 degrees latitude, to 12 hours and 16 minutes at 60 degrees latitude.
The summer solstice occurs at the moment the earth's tilt toward from the sun is at a maximum. Therefore, on the day of the summer solstice, the sun appears at its highest elevation with a noontime position that changes very little for several days before and after the summer solstice. The summer solstice occurs when the sun is directly over the Tropic of Cancer, which is located at 23.5° latitude North, and runs through Mexico, the Bahamas, Egypt, Saudi Arabia, India, and southern China. For every place north of the Tropic of Cancer, the sun is at its highest point in the sky and this is the longest day of the year.
The winter solstice marks the shortest day and longest night of the year. In the Northern Hemisphere, it occurs when the sun is directly over the Tropic of Capricorn, which is located at 23.5° south of the equator and runs through Australia, Chile, southern Brazil, and northern South Africa.
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We all know that the Earth makes a complete revolution around the sun once every 365 days, following an orbit that is elliptical in shape. This means that the distance between the Earth and Sun, which is 93 million miles on average, varies throughout the year. During the first week in January, the Earth is about 1.6 million miles closer to the sun. This is referred to as the perihelion. The aphelion, or the point at which the Earth is about 1.6 million miles farther away from the sun, occurs during the first week in July. This fact may sound counter to what we know about seasons in the Northern Hemisphere, but actually the difference is not significant in terms of climate and is NOT the reason why we have seasons. Seasons are caused by the fact that the Earth is tilted on its axis by 23.5°. The tilt's orientation with respect to space does not change during the year; thus, the Northern Hemisphere is tilted toward the sun in June and away from the sun in December, as illustrated in the graphic below.
Courtesy: NASA
Equinoxes and Solstices through 2030 Earth's Seasons - Equinoxes, Solstices, Perihelion, and Aphelion (navy.mil) NOTE: In the tables, d, h, m indicate day, hour, and minute, respectively. Date/Times in black are in Universal Time. Date/Times in blue are Local Time (CDT/CST). |
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d h m |
Local Time (CDT) |
d h m |
Local Time (CDT/CST as indicated) |
| 2024 Equinoxes Solstices |
Jun 20 3:51 pm |
Sept 22 12 44 Dec 21 09 21 |
Sep 22 7:44 am CDT Dec 21 3:21 am CST |
| 2025 Equinoxes Mar 20 09 01 Solstices June 21 02 42 |
Mar 20 4:01 am Jun 20 9:42 pm |
Sept 22 18 19 Dec 21 15 03 |
Sep 22 1:19 pm CDT Dec 21 9:03 am CST |
| 2026 Equinoxes Mar 20 14 46 Solstices June 21 08 24 |
Mar 20 9:46 am Jun 21 3:24 am |
Sept 23 00 05 Dec 21 20 50 |
Sep 22 7:05 pm CDT Dec 21 2:50 pm CST |
| 2027 Equinoxes Mar 20 20 25 Solstices June 21 14 11 |
Mar 20 3:25 pm Jun 21 9:11 am |
Sept 23 06 02 Dec 22 02 42 |
Sep 23 1:02 am CDT Dec 21 8:42 pm CST |
| 2028 Equinoxes Mar 20 02 17 Solstices June 20 20 02 |
Mar 19 9:17 pm Jun 20 3:02 pm |
Sept 22 11 45 Dec 21 08 19 |
Sep 22 6:45 am CDT Dec 21 2:19 am CST |
| 2029 Equinoxes Mar 20 08 02 Solstices June 21 01 48 |
Mar 20 3:02 am Jun 20 8:48 pm |
Sept 22 17 38 Dec 21 14 14 |
Sep 22 12:38 pm CDT Dec 21 8:14 am CST |
| 2030 Equinoxes Mar 20 13 52 Solstices June 21 07 31 |
Mar 20 8:52 am Jun 21 2:31 am |
Sept 22 23 27 Dec 21 20 09 |
Sep 22 6:27 pm CDT Dec 21 2:09 pm CST |
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