Earth's axis is tilted about 23.4°, and it keeps pointing the same way in space (toward the North Star) all year. As Earth travels around the Sun, first one hemisphere and then the other leans toward the Sun. This tilt, not our distance from the Sun, makes the days longer or shorter and the Sun higher or lower.
- Around June 21 the Northern Hemisphere leans toward the Sun: long days and a high noon Sun there (summer), short days in the south (winter).
- Around December 21 it is the other way around.
- Around March 20 and September 22 (the equinoxes) neither hemisphere leans toward the Sun, and day and night are close to 12 hours everywhere.
Key idea
Why it works
Worked example: The noon Sun at an equinox
- At an equinox the Sun is overhead at the equator (0°).
- Each degree you go away from the equator, the noon Sun is a degree lower: $90 - 40 = 50$.
Answer: 50° above the horizon
Worked example: The noon Sun at a solstice
- June: the place is $40 - 23.4 = 16.6$ degrees from where the Sun is overhead, so the Sun is $90 - 16.6 = 73.4$° high.
- December: the place is $40 + 23.4 = 63.4$ degrees away, so the Sun is $90 - 63.4 = 26.6$° high.
Answer: 73.4° in June and 26.6° in December
Common mistake