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What causes the seasons? |
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| Feb10-13, 03:50 PM | #1 |
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What causes the seasons?
I figured out the answer to the question in the title. The seasons are due to the earths north to south axis facing towards or away from the sun at different times in the year. I have a couple of other questions:
1.) What does a week signify? A day is how long it takes for the earth to make a full rotation, a month is the time it takes for the moon to orbit the earth and a year, the time it takes for the earth to orbit the sun. What is a week? 2.) Does the earth have a circular or eliptical orbit around the sun? |
| Feb10-13, 04:29 PM | #2 |
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I suppose one could imagine that it's got something to do with the phases of the Moon, them being four, each taking about seven days. Better ask a cultural anthropoligst, I suppose. Note that the Earth is in perihelion around the first week of January, so it's closest to the sun when it's the coldest time of the year in the northern hemisphere. |
| Feb10-13, 06:21 PM | #3 |
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Thanks. Does that 5 million km difference make much difference to the temperature of the earth? I reckon it would. Venus, from what I hear, is scorching hot compared to the earth. Not sure how far venus is from earth, my guess (based on the radius you told me) would be 40 million km.
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| Feb10-13, 07:16 PM | #4 |
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What causes the seasons?The sun gives off a certain amount of radiation, let's call it I0. How much of it reaches a planet depends on how far away it is. According to the inverse square law, the irradiation will fall with the square of the distance. Two times farther is four times less sunlight, and so on. (subscripts "a" shall mean "aphelion", "p" = "perihelion") Ip=I0/Rp2 Ia=I0/Ra2 The distance at aphelion is 1.034 times the distance at perihelion, or: Ra=1.034 * Rp gives: Ip=I0/Rp2 Ia=I0/(1.034 * Rp)2 Let's divide both equations by each other. Ip/Ia = 1.0342 So, the irradiation at perihelion is Ip=1.069156 * Ia or 7% more received energy than in its farthest point in orbit. Not that much actually. Try doing the same calculation for Venus and Earth at their average distances, and you'll see that at 0.7 the distance, Venus receives twice as much energy per unit area as Earth does. Wikipedia has all such data handily presented. Type planet name and look at that table on the right. You'll find peri- and aphelion there, eccentricity(how close to a circle an orbit is, with 0 meaning ideal circle), semi-major axis(for near-circular orbits roughly corresponds to the radius of a circle) and more. |
| Feb10-13, 07:22 PM | #5 |
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Mentor
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The opposite occurs in the southern hemisphere. Winter in the southern hemisphere occurs when the Earth is furthest from the Sun and summer when the Earth is closest to the Sun. This would seem to suggest that seasons in the southern hemisphere should be more extreme than those in the northern hemisphere. That's not the case. It's the other way around. There's yet another contributing factor to the variations of the seasons. About 80% of the southern hemisphere is covered by ocean, but it's only about 60% for the northern hemisphere. The contribution of this uneven distribution to climate is stronger by about a factor of two than is insolation. * Right now, that is. This near coincidence of the December Solstice and perihelion is just a coincidence. It will be the other way around 10,000 years from now. |
| Feb12-13, 01:22 PM | #6 |
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Week - Wikipedia, the free encyclopedia goes into gory detail about the different week lengths that various societies have had: 3, 4, 5, 6, 7, 8, 9, 10 days. So it's essentially artificial.
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| Feb12-13, 01:31 PM | #7 |
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| Feb12-13, 03:57 PM | #8 |
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With respect to the elliptical orbit and climate (insolation), google for Milankovitch cycles.
This has a very detailed explanation along with some problems associated with this approach. Or try: http://en.wikipedia.org/wiki/Milankovitch_cycles |
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