Hey, I just got a pretty cool idea, and it gives everyone another opportunity to do some observations.
The autumnal equinox is nearly upon us (18 days away), which gives us a very unique opportunity. For at least 24 hours on either side of the equinox the sun will be within a half-degree of the equator, which presents a unique (well, ish, it happens twice a year) opportunity for observations and calculations.
The equinox happens at 20:39 UTC on the 22nd of September. Between 20:40 UTC on the 21st and 20:40 UTC on the 23rd the sun will move only 46' southward. We can round this to 1° (60') for very conservative numbers.
But what are we measuring? The sun, of course!
There are a few records of various solar experiments done regarding the angle of the sun from cities directly north-south of each other and using this to calculate the altitude of the sun. We can do the same here, and the equinox provides very nice calculations!
What do you need to do? Well, here, I'll do a little write-up:
Distance to the Sun:
Materials:
Method:
At solar noon for your location on either the 21st, 22nd, or 23rd measure the angle of the sun. This can be done by measuring the length of the shadow of a vertical object. The angle of the sun is the arctangent of the height of the object divided by the length of the shadow:
arctan(h/s)
Post the results (your latitude and the angle of the sun) here for all to see.
During those three days the sun will be within at most 30' (0.5°) of the equator, meaning your latitude will be within 30' (0.5°) of your distance from the point at which the sun would be at zenith. Because a degree of latitude is 1/90th of the distance from the north pole to the equator our results will be in terms of this.
If you wish to do the maths yourself to figure out the height you get for the sun you can (post them with the other infos). You can use one of the below equations:
h = (latyou ± .5°) * tan(Φ)
h = (latyou ± .5°) * heightobject/lengthshadow
Once again, the answers will be in terms of degrees of latitude, each one is 1/90th the distance from the north pole to the equator.