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Seasons are not a single local story about today’s weather. They are a global pattern that repeats each year, tied to Earth’s orientation in space as it travels around the Sun. Any explanation that claims one simple cause has to match three big observations at once. The hemispheres experience opposite seasons, the tropics behave differently from the mid-latitudes, and the polar regions swing between extreme daylight and extreme darkness.
One useful habit starts here. Separate what changes slowly with the calendar, such as typical daylight and typical temperature range, from what changes quickly day to day, such as storms and cold snaps. Weather can hide the seasonal pattern for a week. It cannot erase it.
At the largest scale, the Northern Hemisphere tends to have summer in June to August while the Southern Hemisphere tends to have winter during those same months, and the situation reverses around December to February. That alone is a strong constraint. If one global factor causes seasons, it must be able to make one half of Earth warm up while the other half cools down at the same time.
Latitude matters just as much as hemisphere. Near the equator, temperatures often change less over the year, and many places experience seasons mainly as wet and dry periods rather than hot and cold. In the mid-latitudes, seasonal temperature changes are usually strong, with warm summers and cold winters. Near the poles, the defining seasonal change is not just temperature. It is daylight itself, including long summer days and long winter nights.
Explore these global patterns on a map.
A brief mental check keeps you honest. If you imagine two cities at similar latitude but in opposite hemispheres, such as one around 35 degrees north and one around 35 degrees south, their warm and cool parts of the year are shifted by about half a year. That is a real, repeatable observation. An explanation that cannot produce that phase flip cannot be right.
A common first idea is that Earth has seasons because it is sometimes closer to the Sun and sometimes farther away. This sounds reasonable because distance affects how much sunlight arrives. If a lamp is closer, it looks brighter. The physical quantity that measures how much solar energy arrives per unit area is intensity. Its SI unit is watts per square meter, written W/m. If distance were the main cause, the closer part of the year should give stronger sunlight everywhere on Earth at the same time.
That prediction clashes with what we observe. When it is summer in the Northern Hemisphere, it is winter in the Southern Hemisphere. Distance to the Sun is a single global number for the whole planet at a given moment. It cannot make opposite hemispheres warm and cool in opposite directions at the same time.
Distance also makes a specific prediction about timing. Earth reaches its closest point to the Sun, called perihelion, in early January, and its farthest point, called aphelion, in early July. If closeness drove seasons, January should be the hottest time globally and July the coolest. The opposite is closer to the truth. January is winter for much of the Northern Hemisphere.
See how the real orbit compares with an exaggerated version.