Next, we'll leave them out of phase as they are for us, but make them about the same size. Specifically, I've made it so when we're far from the sun, we get only half the sunlight we would at the near point. Instead of the max and min distance differing by only 3%, now they differ by 41%. This one makes life pretty weird. The folks in Fairbanks never get much sun now, and nobody gets much in the middle of summer when we're far from the sun. People in Utah or Michigan type zones get the most consistant light through the year, while the equator now has 4 seasons. (In this situation we might need to crank up the temperature knob on the sun to keep us all from freezing, but that might be difficult. In the real life system the 5 locations recieve 340, 311, 269, 244, and 142 artibrary units of sunlight over the course of a year. Now they get 263, 234, 199, 178 and 96. If we turn up the sun to get St George back up to where it was, those points shift to 356, 316, 240 and 130. We've kept St. George reasonable (well, as reasonable as it ever was), but made the equator 5% more sunny, while Fairbanks is still 8% less sunny than before. Essentially, this world is more sunlight-diverse.)
Next, we'll make them roughly the same magnitude, but with a 90° phase shift (one curve peaks 3 months before the other). Specifically, we hit the near point of our highly elliptical orbit about April 1st, with the tilt unchanged. This gets a little crazier. The total sunlight is not as low as the last model (263, 241, 209, 190, 111, which "St. George Adjusts" to 338, 310, 269, 244 and 143.) So, if we crank up the sun about 30%, we get the same total sunlight through the year. Unfortunately, it's going to be packed into a few really bright (hot) months. The equator has more seasonal variation than before, but is dominated by the position in the orbit, not the direction of the tilt. Also, everyone now has seasons!
So, in the end, the earth is neat.
(It is a worthwhile reminder that there are still other things that are important to sunlight that I haven't considered. The most important is the dispersion through the atmosphere. As the sunlight moves closer to the horizon, it has to go through more of the atmosphere to reach the surface, and more light is scattered out. Then there are things like clouds to consider. Also, while this sunlight is the cause of our seasons, there are many other things that effect temperatures, such as residual ground heat, ocean and air currents and butterflies flapping their wings in China.)
1 comment:
I want to print these out and show them to my planetarium buddies. My brother is wicked smart.
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