In the last post, we derived a method to calculate the angle between the celestial equator and ecliptic and generalized it to be applicable for any angle. Here, I present the table derived from those calculations.
Almagest Book I: The Arcs Between the Equator and Ecliptic
Before going on the several post detour in developing several theorems and making extra sure we understood a few, we stated the goal was to determine the length of an arc at various points between the celestial equator and ecliptic1.
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Exploring Menelaus’ Theorem
In the last post, we used several theorems we’d developed to arrive at Menelaus’ theorem. However, at the very end Ptolemy simply mentions another version of the theorem, but does not derive it. I simply took his word that it worked, but as that alternative form is used first thing in the next chapter, I want to make sure at the very use, we know how to use it, even if we don’t go through how it’s derived.
First, let’s set up a generic Menelaus configuration on a sphere which is the intersection of the arcs of four great circles:
Instrumentation – The Great Quadrant: Day 7
With the upper portion of the base ready to hold the center column, today’s focus was on getting a socket for the center column to rest in. To start, we created a set of cross beams.
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Almagest Book I: Menelaus’ Theorem
So far in these preliminary theorems, we’ve looked at some that were based on triangles and some that were based on circles. We’ll be going one step further with this next one and work with spheres. Thus far, we’ve briefly touched on spheres in this post discussing the celestial sphere. If great circles and spherical triangles aren’t familiar to you, I suggest reading over that post.
But since this is the first time we’ve encountered math in 3D if you’ve been following along, I want to build this up more slowly2 and will be trying to add some 3D elements to make the visualization a bit easier.
[L]et us draw the following arcs of great circles on a sphere: BE and GD are drawn to meet AB and AG, and cut each other at Z. Let each of them be less than a semi-circle.
Almagest Book I: Circular Lemmas for Spherical Trigonometry
As noted in the previous Almagest post, I wanted to break this next set of lemma off because they use a new mathematical term: Crd arc.
The term is very simple. In fact, the name’s on the tin. It refers to the chord subtended by a specific arc. So let’s dive right in to the next proof and see how it’s used:
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Data: Summer Solstice Solar Altitude
Happy Summer Solstice everyone!
Since one of the things Ptolemy was concerned with was the angle between the ecliptic and celestial equator, I built a solar angle dial to help determine this. Given that the measurements needed to be taken on the solstices (or a solstice and equinox), I set up the instrument today to take the measurement.
Instrumentation – The Great Quadrant: Day 6
Today’s focus was on starting to build the discs that would allow the central column to rotate.
The central column is 4.75″ square (a roughly 6.75″ diagonal), so we decided to cut an 8″ disc as well as a 9″ disc which would lay over it.
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Instrumentation – Ptolemy’s Solar Angle Dial
Since the solstice is only a few weeks away, I decided it might be fun to make Ptolemy’s solar angle dial we recently saw.
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Instrumentation – The Great Quadrant: Day 5
With the quadrant itself pretty much complete (aside from the scale), it was time to start working on something to mount it on. So today we started with the central column which was assembled from plywood to make a 5″ box that was 8′ tall.
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