Published by: almanac.com
The first day of winter in the Northern Hemisphere is marked by the winter solstice, which occurs on Thursday, December 21, 2023, at 10:27 P.M. EST.
For the northern half of Earth (the Northern Hemisphere), the winter solstice occurs annually on December 21 or 22. (The Southern Hemisphere’s winter solstice occurs in June.) The winter solstice is the day with the fewest hours of sunlight throughout the year, making it the “shortest day” of the year. Thankfully, after we reach the winter solstice, the days begin to grow longer and longer again until we reach the summer solstice—the first day of summer and the longest day of the year.
What Is the Winter Solstice?
The winter solstice marks the official beginning of astronomical winter (as opposed to meteorological winter, which starts about three weeks before the solstice). The winter solstice occurs once a year in each hemisphere: once in the Northern Hemisphere (in December) and once in the Southern Hemisphere (in June). It marks the start of each hemisphere’s winter season. When one hemisphere is experiencing its winter solstice, the other is simultaneously experiencing its summer solstice!
This is all thanks to Earth’s tilted axis, which makes it so that one-half of Earth is pointed away from the Sun, and the other half is pointed towards it at the time of the solstice.
What Happens on the Winter Solstice?
On the day of the winter solstice, we are tilted as far away from the Sun as possible, which means that the Sun’s path across the sky is as low in the sky as it can be. Think about the daily path of the Sun: It rises in the east and sets in the west, arcing across the sky overhead. During the summer, the Sun arcs high in the sky, but during the winter, it arcs lower, closer to the horizon.
How can we observe the effects of solstice ourselves? On the day of the solstice, stand outside at noon and look at your shadow. It’s the longest shadow that you’ll cast all year! Do this again on the day of the summer solstice, and you’ll see almost no shadow.
The Sun’s Changing Path
Another way to think of this is that on the day of the solstice, the Sun’s path reaches its most southerly point in the sky. For those of us in the Northern Hemisphere, this means that the Sun’s path is as low in the sky as it can get—even at “high noon.” In the Southern Hemisphere, it’s the opposite: The Sun’s path will be high in the sky on the winter solstice—directly overhead at noon at the latitude called the Tropic of Capricorn, which is an imaginary line that circles the Earth, running through parts of South America, southern Africa, and Australia.
The word solstice comes from the Latin sol “sun,” and sistere “to stand still.” So, loosely translated, it means “sun stands still.” Why? The Sun’s path across the sky appears to freeze for a few days before and after the solstice. The change in its noontime elevation is so slight that the Sun’s path seems to stay the same or stand still.
The day after the winter solstice, the Sun’s path begins to advance northward again, eventually reaching its most northerly point on the day of the summer solstice.
Then, as summer advances toward winter, the points on the horizon where the Sun rises and sets advance southward each day; the high point in the Sun’s daily path across the sky, which occurs at local noon, also moves southward each day. It’s a never-ending cycle!