By Graham Jones and Konstantin Bikos. Published 14-Jun-2023
No matter where we live, we spend about half the year with the Sun above the horizon. But, ignoring clouds, which part of the world gets the most daylight? And which gets the least? The answers might surprise you.
June 21, 2023, is the summer solstice and the longest day of the year for the Northern Hemisphere. At the same time, it is the winter solstice—and shortest day of the year—for the Southern Hemisphere.
The situation is reversed at the December solstice, when the amount of daylight reaches a minimum in the Northern Hemisphere, and a maximum in the Southern Hemisphere.
Over the course of a year, therefore, long days and short days balance each other out, and we all end up with roughly the same amount of sunlight: six months’ worth, or 12 hours per day on average.
In practice, however, the actual amount of sunlight you get depends on your latitude north or south of the equator. If you wanted to maximize your hours of daylight, which latitude should you move to?
The following bar chart reveals the average amount of daylight per day for every line of latitude from 90° north to 90° south. We made the chart using our sunrise and sunset data for 2023. (The shape of the chart is the same from one year to the next.)
In our chart, each line of latitude is represented by a horizontal bar. 90° north is at the top, the equator is in the middle, and 90° south is at the bottom. The length of each bar from left to right equals the average amount of daylight at that latitude.*
Hours and minutes of daylight per day are indicated by the numbers along the horizontal x-axis, from 12 hours, 0 minutes to 12 hours, 40 minutes.
The above chart is perhaps not what you might expect. In particular, there are three odd features that need to be explained.
How can we explain these oddities?
At any one moment, as Earth spins on its axis, half the planet is facing toward the Sun, and half is facing away.
In other words, half the globe is always in daylight, and half is always shielded from the Sun. So how can everywhere get more than 12 hours of daylight per day on average?
There are two reasons for this: the size of the Sun in the sky, and the bending of light in Earth’s atmosphere.
First, the Sun appears as a disk (like the Moon), not a point (like a star). Daylight is not measured from when the center of the Sun’s disk rises, to when the center of the Sun’s disk sets.
Instead, daylight begins a little bit early, when the top edge of the Sun first appears above the horizon. Likewise, it ends a little bit late: not until the final edge of the Sun’s disk has disappeared.
Second, light from the Sun is bent by Earth’s atmosphere—a phenomenon known as refraction. As a result of this optical trick, we can see the Sun even when its true position is beneath the horizon.
Again, this means that sunrise comes a little earlier than expected, and sunset a little later—giving us more daylight overall.
Earth spins on its axis with the tropics—the region of the globe that straddles the equator—pointed toward the Sun.
Therefore, around the equator, the Sun tends to rise straight upward from the horizon.
As we travel north or south from the tropics, the Sun rises at more of a slope. In the northern hemisphere, the Sun moves along the horizon from left to right at sunrise and sunset; in the southern hemisphere, it moves from right to left.
The effect of this slope is that sunrise and sunset take longer: the top edge of the Sun appears even earlier at sunrise; the bottom edge disappears even later at sunset.
The following images are taken from our Interactive Night Sky Map, one hour after sunrise on the June solstice.
The long sunrise and long sunset effect is most pronounced at the Arctic and Antarctic Circles. Here, around the solstices, the Sun spends a lot of time skimming along the horizon, producing more hours of sunlight throughout the year.
The Sun also skims the horizon at the North and South Poles. The difference here is that this happens around the equinoxes, not the solstices—leading to fewer hours of daylight overall.
At the equinoxes, the Sun’s position in the sky changes more quickly from one day to the next than it does at the solstices. This is why sunrise and sunset times alter rapidly during the months of March and September, but slowly during June and December.
Consequently, the Sun spends less time per year skimming the horizon at the poles than at the polar circles.
Again, these examples are taken from our Interactive Night Sky Map. To make the path of the Sun easier to see, we’ve turned off the “elevated horizon” feature.
We all know we get the most daylight during the summer. What is less well known is that summer lasts longer in the Northern Hemisphere than the Southern Hemisphere.
The reason for this is that Earth’s orbit around the Sun is not a perfect circle. Earth is closest to the Sun in early January, and farthest from the Sun in early July.
The closer Earth is to the Sun, the more quickly it travels along its orbital path. So seasonal changes happen a bit more quickly in January, and a bit more slowly in July.
January is summer in the Southern Hemisphere, and winter in the Northern Hemisphere; in July, it’s the other way around. Thus summer lasts longer in the Northern Hemisphere—giving the northern half of the globe more sunlight than the southern half over the course of the year.
| March equinox to September equinox, 2023 |
|---|
| 186 days, 9 hours, 25 minutes |
| Northern spring & summer |
| Southern fall & winter |
| September equinox to March equinox, 2023/24 |
|---|
| 178 days, 20 hours, 16 minutes |
| Northern fall & winter |
| Southern spring & summer |
* Our bar chart comparing daylight at different latitudes is very smooth—but you might have noticed some ‘lumpiness’ in the lengths of the bars close to the North Pole and South Pole. This is caused by jumps in the number of days of polar day (Midnight Sun) and polar night.
