The Seasonal Tracks of the Sun
The tilt of Earth’s axis determines where the Sun appears in the sky throughout the year. During summer in the northern hemisphere, the Sun rises north of east and sets north of west. It is high in the sky at noon. During winter in the northern hemisphere, sunrise and sunset appear farther south along the horizon. The winter-time Sun is lower in the sky throughout the day.
The Sun in a Year
We see sunrise and sunset at different points on the horizon during the year. At the start of spring and fall (the equinoxes), the Sun rises due east and sets due west. On the summer solstice (around June 21), the Sun rises and sets at its most northerly points along the horizon. On the winter solstice (around December 21), the Sun rises and sets at its most southerly points.
This composite uses three images of sunrise over a small town in Greece, taken on three different days. It shows sunrise points on the eastern horizon for the solstices and equinoxes.
The Sun Appears to Move Against the Backdrop of Stars
The night sky changes throughout the year. Just as the Sun seems to move from east to west during the day, the stars and planets appear to make the same journey at night. What you see depends on when you observe.
The Sun’s path crosses certain familiar star patterns (the ecliptic paths). During the day, we don’t see them because the Sun is so bright. At night, we see the stars on the opposite side of the ecliptic path, when Earth’s night side points away from the Sun. Six months later, they are behind the Sun and other stars are up at night.
Earth’s position in its orbit determines which stars we see. As our planet moves through space, its day and night sides face out toward different parts of space.