2.7 - The Seasons

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The Reason for the Seasons

The seasons

Seasons result from variations in the Sun's altitude (the angle of the Sun with respect to the horizon) and the Sun's declination (the latitude of the perpendicular or vertical rays of the Sun) . These are created by the  annual Diagram showing the Earth's 23.5° tiltrevolution of the Earth around the Sun, its daily rotation around its axis and most importantly, the tilt of the Earth's axis. To understand the tilt of the Axis, you have to use your imagination. Imagine a plane (a flat surface) the runs through the middle of the Earth and the Sun. Instead of the Earth revolving around the Sun with a 90° angle to that plane, the Earth's axis is tilted 23.5°.  

During the Northern Hemisphere winter,  because of the Earth's axial tilt, the Northern  Hemisphere is tilted away from the Sun. During our Summer, the Northern Hemisphere is tilted toward the Sun. The opposite conditions exist in the Southern Hemisphere. On the Equinoxes, neither hemisphere has the advantage and the Sun is most intense at the Equator.

 

earth sun relationships solstice and equinoxes

 

 

Seasons in the Northern and Southern Hemispheres
Winter Solstice Vernal or Spring Equinox Summer Solstice Fall or Autumnal Equinox
Northern Hemisphere   Dec 21st March 21  June 21 Sept 21
Length of Day 24 hours of darkness 66.5°N (Arctic Circle ) to 90°N (N. Pole) Shortest day of the year in N. Hemp Everywhere on Earth experiences a 12 hour day 24 hours of daylight 66.5°N (Arctic Circle ) to 90°N (N. Pole) Longest day of the year in N. Hemp Everywhere on Earth experiences a 12 hour day
Southern Hemisphere June 21st Sept 21 Dec 21 March 21
Length of Day 24 hours of darkness 66.5°S (Antarctic Circle ) to 90°S (S. Pole) Shortest day of the year in S. Hemp Everywhere on Earth experiences a 12 hour day 24 hours of daylight 66.5°S (Antarctic Circle ) to 90°S (S. Pole) Longest day of the year in N. Hemp Everywhere on Earth experience a 12 hour day

 

The Earth's Seasons are the first building block for weather on Earth.  Only latitudes between 23.5°N and 23.5°S ever receive the direct rays of the Sun. This is part of a complex system that creates an imbalance in the solar energy received at different latitudes. The Tropics have a surplus of energy. The Poles have a deficit. Much of weather is driven by this imbalance (the winds, ocean currents etc). Here at 38°N, the balance between incoming and outgoing solar radiation is about even.