00:01
So we know that earth is tilted as it rotates about its axis, and its tilt from being straight up and down is about 23 .5 degrees from straight up and down.
00:15
And so what this means as the earth completes its revolution throughout the year around the sun, we end up having impacts on our mid latitudes and up to our poles, especially.
00:27
So we can think that at the equator, the sun's, because it varies around this sun angle, on the equator and in the tropics, so between the equator at zero degrees to 23 and a half degrees, we end up having the sun always pretty high sun angle within the sky.
00:46
But in our more temperate mid -latitude type of locations, we start having greater variations as are, because of this tilt throughout the year.
00:58
So again, the highest sun angle in our kind of temperate mid -latitudes places are going to be during the summer months for either, you know, respectively the northern or southern hemispheres.
01:24
You know, in that summer, those summer time for those particular regions, that'll be the highest sun angle and thus affects climate in the sense of having.
01:35
The generally warmest temperatures.
01:40
And then conversely, we, you know, in the winter months for those appropriate hemispheres, have the lowest sun angle.
01:56
And having that, of course, be leading into, you know, based on that, the relative coolest temperatures.
02:09
And so this observation we have for our mid -ladicture kind of temperate areas really only continues to exacerbate more, continues to increase into its extremes at the poles, where we have the poles, with their extremes, again, for each respective pole, we can think that they have in their summer, particularly their summer solstice, you know, 24 hours of sunlight.
02:43
The sun is always above the horizon at that time.
02:47
Again, leading to not terribly necessarily warm temperatures.
02:53
Some of us might consider, but at least the warmest for those relative locations...