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The causes of the seasons through the Earth's tilt and revolution around the Sun. It discusses the Earth's orbit, tilt, and how it affects the amount of heat energy received from the Sun, leading to varying temperatures in different hemispheres. The document also covers the concept of direct and indirect heat energy and the importance of the solstices and equinoxes.
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(Alder Planetarium, http://www.adlerplanetarium.org/education/resources/sunearth/section06i.shtml, accessed November 1, 2008)
During January, Earth is closest to the Sun. During July, the Earth is farthest from
a perfect circle, it’s very, very close. This diagram shows you the distances to the Sun.
January July 91 million miles (^) 94 million miles
We receive the same amount of heat energy from the Sun, but it has to heat a larger area. To see how this works, we need to look at some diagrams.
Indirect heat energy strikes the ground at an angle. The light and its heat are spread out over a larger surface area than if it had struck the ground directly. The picture shows that the same amount of heat energy hits the surface. However, this energy
What happens in the summer? Look at this diagram.
Direct heat energy is energy at or near right angles to the ground. The picture shows
that summer temperatures are warmer.
There are two times when the heat energy is between direct and indirect. That is when it is spring and autumn. At that time, the Earth gets an equal amount of heat energy. This is why it is warming up in spring. It is why it is getting cooler in autumn.
There are four important dates as the Earth revolves around the Sun.
; December 21 st^ – Winter Solstice. Solstice means "Sun standing still." On the Winter Solstice, the Sun appears at its most southern position along the horizon at sunrise and sunset and reaches its lowest midday altitude for the year. The South Pole is tilted most toward the Sun.
How does the length of daylight change throughout the year? Look at this diagram.
When it’s winter, the Northern Hemisphere is tilted away from the Sun. The North Pole is in darkness 24 hours a day. Daylight hours increase as you move south. In Utah, our daylight hours are around eight hours a day. Shorter daylight hours and indirect heat energy from the Sun make for a cold season.
daylight hours are about twelve hours long. Daylight hours continue to increase until the Summer Solstice. Look at this diagram.
The Northern Hemisphere is now tilted towards the Sun. The North Pole is getting 24 hours of daylight. Daylight hours decrease as you move south. In Utah, our daylight hours are around 16 hours a day. Longer daylight hours and direct heat energy make for a warm season.
daylight hours are about twelve hours long. Daylight hours continue decreasing until the Winter Solstice.
How do the daylight hours change? Look at this table that shows daylight hours throughout the year.
Latitude 40°N
Date Jan 1 Jan 16 Feb 1 Feb 16 Mar 1 Mar 16 Hours light 9.21 9.46 9.92 10.48 11.02 11.
Date Apr 1 Apr 16 May 1 May 16 Jun 1 Jun 16 Hours light 12.41 13.07 13.68 14.21 14.63 14.
Date Jul 1 Jul 16 Aug 1 Aug 16 Sep 1 Sep 16 Hours light 14.81 14.58 14.13 13.59 12.92 12.