The Earth's axis of rotation is tilted about 23. degrees relative to Earth's orbit around the sun. This tilt causes the Northern and Southern Hemispheres to get unequal amounts of sunlight over a year.
The Earth's axis is tilted most closely toward the sun for two moments each year. These are called solstices. The Northern Hemisphere is tilted more toward the sun from September to March, which feels like autumn and winter. The hemisphere tilted most toward our home star sees its longest day and the hemisphere tilted away from the sun sees its longest night.
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As mars orbits the Sun, it completes one rotation every 24,6 hours, which is very similar to one day on Earth (23.9 hours). Martian days are called sols—short for "solar day." A year on Mars lasts 669.6 sols, which is the same as 687 Earth days.
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In layman's terms, the equinox happens because the planet earth is not tilted towards the sun while the sun is directly above the equator. This causes the equinox to happen.
So during this time of the year, both hemispheres get the same hours of daylight and night.
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Before the invention of calendars and other modern methods of tracking years and seasons, people relied on the position of the sun in the sky and obvious signs in nature to indicate the passing of time.
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