Calculate Sun Angle: Length of Object by Shadow

AI Thread Summary
To calculate the sun's angle in the sky and determine the length of an object's shadow, one can use the law of cosines from spherical trigonometry. The angle varies daily due to Earth's rotation and seasonally based on latitude, with local noon providing the most accurate measurement. A simple method involves measuring the shadow of a short stick to compute the angle, which can then be applied to find the height of other objects. For those who prefer not to calculate manually, planetarium software can provide the sun's angle. Understanding these principles allows for precise shadow length calculations.
Ba
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Can somebody explain how to calculate the sun's angle in the sky at a certain time of day? It is wanted to calculate the length of an object by it's shadow.
 
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It's based on the law of cosines from spherical trigonometry. The site http://www.krysstal.com/sphertrig.html has what you want about the shadow, but you have to scroll past a lot of stuff about great circle distances and the direction of Mecca.
 
The easiest way to get the angle it set up a short stick you can measure, then compute the angle. You can then apply that to an object you wish to find the height of. You need to work fast, the angle is always changing.
 
A planetarium program will tell you if you don't feel like calculating it...
 
russ_watters said:
A planetarium program will tell you if you don't feel like calculating it...

Aww, that's no fun! See Asimov's story "The Feeling of Power".
 
Well, I will say you haven't lived until you've done celestial navigation... after a half an hour of measurements, calculations, and plotting, you'll know that half an hour ago, you were within 5 miles or so of where the GPS told you you were.
 
Thanks, we wanted to try and find the angle as exact as possible.
 
Ba said:
Can somebody explain how to calculate the sun's angle in the sky at a certain time of day? It is wanted to calculate the length of an object by it's shadow.

There are two components to the suns angle in the sky.

One of them varies with a 24 hour period, you can correct for this component by making your measurements at local noon. This component is due to the rotation of the earth.

The other component will vary with the season, it will have a 1 year period, and it will depend on the latitude of the observer.

If you ignore the axial tilt of the earth, you can probably see if you think aobut it a lot that the sun would be always on the horizon at the poles, and it would pass directly overhead on the equator.

Because of the axial tilt of the earth, this actually happens only on the equniox.
 

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