A Great Math Site: Understanding the Analemma

By way of the astronomy picture of the day, I encountered a really fantastic site about the analemma.

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The analemma is the apparent path that the sun takes in the sky during the year. If you record the
precise position of the sun at the same time every day, instead of being in exactly the same place
every day, it will traverse a figure eight, like in this image. This is an effect caused by a combination of the eccentricity of the earth's orbit, and the tilt of the earth's axis. It can be a bit hard to visualize just where the figure-eight shape comes from; the analemma site uses a combination of diagrams and animations to make it extremely clear, and works through the entire process of demonstrating where each component of the analemma comes from, and deriving the equations that describe it.

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On Monday, I posed a question to you as to why, when you photograph the Sun at the same exact time every day for a year, you get something that's shaped like a figure 8, like so:
I'm trying something new here: I'm going to give you a little bit of information and a teaser, and we'll see -- in the comments section -- whether any of you can figure it out.
Holy moly, if you want to see a great post you should read Ethan's post on the solar analemma. If you photograph the sun in the sky at the same time each day, it won't be in the same spot.
“Life is tragic simply because the earth turns and the sun inexorably rises and sets, and one day, for each of us, the sun will go down for the last, last time.” -James A. Baldwin

Kids: if you try this at home, be sure not to get thrown by Daylight Savings Time. Use a consistent clock.

By Mustafa Mond, FCD (not verified) on 01 Jan 2007 #permalink