Solstices and equinoxes
Why does Earth have seasons? Naturally, we think our world’s seasons result from Earth’s changing distance from the sun. But that’s not the case. Because the Earth is farther from the sun in July (northern summer) and closer in January (northern winter). So the fact that Earth’s Northern and Southern Hemispheres have their summers and winters at opposite times of the year provides a clue to the real reason for seasons. And that reason is Earth’s 23 1/2-degree tilt on its axis.
The photos and video on this page – from NASA – show Earth’s solstices and equinoxes from space. They can help you visualize why our seasons unfold as they do, continuously, throughout each year.
Viewing the solstices and equinoxes from space
EUMETSAT‘s Meteosat-9 (a weather satellite) captured the four views above of Earth from geosynchronous orbit in 2010 and 2011. As a matter of fact, a satellite in geosynchronous orbit stays over the same point on Earth all the time. And the images above show how sunlight fell on the Earth on December 21, 2010 (upper left), March 20, 2011 (upper right), June 21, 2011 (lower left), and September 20, 2011 (lower right). Also, each image was taken at 6:12 a.m. local time.
Around 6 a.m. local time each day, the sun, Earth, and any geosynchronous satellite form a right angle. Thus, affording straight-down view of Earth’s terminator line, that is, the line between our world’s day and night sides. As a matter of fact, the shape of this line between night and day varies with the seasons. And results in different lengths of days and differing amounts of warming sunshine.
While the line is actually a curve because the Earth is round, satellite images show it in two dimensions only.
On March 20 and September 20, the terminator is a straight north-south line, and the sun sits directly above the equator. Then on December 21, the sun resides directly over the Tropic of Capricorn when viewed from the ground, and sunlight spreads over more of the Southern Hemisphere. Next on June 21, the sun sits above the Tropic of Cancer, spreading more sunlight in the north.
Why we have seasons
So what’s causing all this change? It’s tempting to imagine it’s the sun moving north or south through the seasons. But that’s not it. Instead, the change in the orientation and angles between the Earth and the sun result from Earth’s never-ending motion in orbit around the sun.
First, the axis of the Earth tilts 23 1/2 degrees relative to the sun and the ecliptic plane. Then the axis tilts away from the sun at the December solstice and toward the sun at the June solstice, spreading more and less light on each hemisphere. At the equinoxes, the tilt is at a right angle to the sun and the light is spread evenly.
Bottom line: A video from NASA shows how sunlight falls on Earth’s surface during the solstices and equinoxes, as seen by the weather satellite Meteosat-9 in 2010 and 2011.