The document discusses the causes of seasons on Earth. The two main causes are the tilt of Earth's axis at 23.5 degrees and its revolution around the sun once a year. If Earth did not revolve, seasons would not change and each location would remain in the same season. Greater or lesser tilt would result in more or less extreme seasons. The first day of each season - winter solstice, vernal equinox, summer solstice, and autumnal equinox - is also identified along with typical dates. The southern hemisphere has opposite seasons. Places near the equator experience less variation in seasons due to more direct sunlight year-round.