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Tutorial on Earth/Sun Relations and Seasons
To understand why we have seasons, we need to look at the relations
between the Earth and the sun. Most of the planets in the solar system also orbit on or near the plane of the ecliptic (you can see that the planets (except Pluto) are more or less lined up, instead of circling the sun at just any old angle. No, this is not drawn to scale).
so, if the Earth's axis of rotation were perpendicular to the plane of the ecliptic,
the direct rays of the sun would always shine on the equator
Question: to which star does the Earth's axis point? That is, what star is almost directly overhead at the North Pole? Answer The inclination of the Earth's axis means that at different locations on its orbit around the sun, different parts of the earth are tilted toward the sun, and the part that is tilted toward the sun is the part that is having summer. If the northern hemisphere is tilted toward the sun, the northern hemisphere receives the most direct rays of the sun (that is, the angle of incidence is higher), and it is summer in the northern hemisphere. If the southern hemisphere is tilted toward the sun, the southern hemisphere receives the most direct rays of the sun (that is, the angle of incidence is higher), and it is summer in the southern hemisphere. In the intermediate situations, halfway between the two extremes, the Earth's axis is still tilted, but not tilted with respect to the sun's rays, and the sun's rays strike directly on the Equator. Let's look at this more closely. At one point in its orbit, the northern part of the earth has its maximum inclination toward the sun. Since the earth's axis is tilted 23 ½ degrees, then on this particular day, the sun's rays are striking the earth directly at a latitude approximately 23 ½ degrees north of the equator (that is, the sun's rays are coming in at an angle of 90 degrees here; this is the subsolar point). This occurs on about June 21 or 22 each year, and the day is known as the Summer Solstice (summer for those who live in the Northern Hemisphere, that is. It might be safer and more generally applicable to call it the June Solstice).
If you were at 23 1/2 degrees north latitude on that day,
and you looked up at noon, the sun would be directly overhead. This latitude is the
farthest north on the Earth that the sun's rays will be directly overhead. Farther north,
at noon, the sun will never be directly overhead, but always at least a little bit to the
south. The latitude of 23 ½ degrees north is known as the Tropic of Cancer, and it
is the northern boundary of the tropics. Let's take a look at the opposite end of the year, six
months later, on December 21 or 22. On this day, the earth has gone halfway around its
orbit, and is opposite the point where it was on the summer solstice. The situation is
exactly reversed. The southern hemisphere of the earth is tilted toward the sun, and the
sun's rays are perpendicular to the earth's surface at 23 ½ degrees south. This is the subsolar
point: the sun is directly overhead at noon at this latitude. The farthest south
that the sun's rays shine directly is latitude 23 ½ degrees south, the Tropic of
Capricorn. This is the southern boundary of the tropics. On this day, the area north
of the Arctic Circle gets no sunlight, and the area south of the Antarctic Circle gets 24
hours of light. Now for the intermediate situation. The subsolar point is at
the Tropic of Cancer in June, and at the Tropic of Capricorn in December. Midway
between the solstices are two dates when the sun shines directly on the equator, and we
have a situation like our hypothetical one, where the earth's axis is perpendicular to the
ecliptic. (The axis is still tilted, still pointing at the North Star, but it is tilted
sideways with respect to the sun, rather than towards or away from the sun).
Throughout the year, daylength is 12 hours at equator. At the Poles, daylength varies from none (at the winter solstice for that hemisphere) to 24 hours (at the summer solstice for that hemisphere). At points in between, daylength will be somewhere in between. The closer a location is to the Equator, the more even the daylength is, not varying much from twelve hours all year. At high latitudes, the daylength is very long in the summer, and very short in the winter. One more point about the Earth's orbit: By now you
know that the reason we have seasons is the tilt of the Earth's axis. But sometimes
people wonder if seasons have anything to do with the distance of the Earth from the sun.
We know that can't be the case, because the seasons are opposite in the Northern and
Southern Hemispheres. However, if we look at the Earth's orbit closely, To summarize: At the December Solstice: The date is December 21 or 22. The subsolar point is latitude ___________ (answer). This latitude is called the Tropic of ____________ (answer). Length of daylight is ______ hours (answer) at the equator, ______ hours (answer) at the North Pole, and _______ hours (answer) at the South Pole. On this day, every location north of the ________ Circle (answer) is in darkness for 24 hours. Every location south of the ______ Circle (answer) gets 24 hours of daylight. It is the longest day of the year for the _________ Hemisphere (answer). At the Equator, the sun's altitude at noon (angle of the sun above the horizon at noon) is __________ (answer). After the December Solstice, the subsolar point will move __________ (northward or southward) (answer). At the March Equinox: The date is March 20 or 21. The subsolar point is latitude ________ (answer). This latitude is called the ____________ (answer). Length of day is ______ hours (answer) at the Equator. Every place on Earth has ________ hours (answer) of daylight. At the Equator, the sun's altitude at noon (angle of the sun above the horizon at noon) is __________ (answer). After the March Equinox, the subsolar point will move __________ (northward or southward) (answer). So, this is the Spring, or Vernal Equinox for the Northern Hemisphere. It is Autumn for the Southern Hemisphere. The days will now be getting _________ (longer or shorter) (answer) for the Northern Hemisphere, and _________ (longer or shorter) (answer) for the Southern Hemisphere. At the September Equinox: The date is September 22 or 23. The subsolar point is latitude ________ (answer). This latitude is called the ____________ (answer). Length of day is ______ hours (answer) at the Equator. Every place on Earth has ________ hours (answer) of daylight. At the Equator, the sun's altitude at noon (angle of the sun above the horizon at noon) is __________ (answer). After the September Equinox, the subsolar point will move __________ (northward or southward) (answer). So, this is the Spring, or Vernal Equinox for the ______ Hemisphere (answer). It is the Fall or Autumnal Equinox for the Northern Hemisphere. The days will now be getting _________ (longer or shorter) (answer) for the Northern Hemisphere , and _________ (longer or shorter) (answer) for the Southern Hemisphere. Now that you know it all, try taking a couple of practice quizzes to see if you know as much as you think you do. Seasons and the Earth's Orbit
Seasons
and the Earth' Orbit II
Email: Dr. J. R. Thorngren
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