This article will derive fundamental equations for a spherical triangle. These equations express the ratio between the angles and curved sides of the triangle drawn on a celestial sphere. We will need these formulas for calculating the primary directions.
Consider a right-angled triangle on a sphere with sides , , and , as well as interior angles , , and .
How will its sides and angles be related to each other?
Rotated Coordinate Systems
First, we introduce a cartesian vector in coordinate system.
From the conversion equation (1) it follows that has coordinates
Now, let’s use the rotation matrix to rotate by angle along and express this vector in axis. As a result, we have the following:
But on the other hand, the same component of the vector is just a projection of that vector to the -axis in the -angle plane.
It gives us the first equation:
Now we move to the next step and introduce a new coordinate system , which is , rotated by angle (minus B) in plane.
If we apply rotation matrix to coordinate system, we will have a -component of the vector to be equal to
On the other hand, -component of vector is equal to zero. It means that
The exact ratio applies to angle:
Other Equations
We have set the main equations for spherical triangles:
All the rest is just a consequence of these three equations.
First, let’s multiply by , and we will get
Now, let’s consider :
Similarly, we can write
Now, let’s divide both sides of the equation by :
which gives
With the same approach, we get from the equation
This equality
is also called the sine theorem.
Now from it follows
If we sunstitude from we will get
or
In a similar manner from (2) follows that
If we substitute (8) with (7), we will get
Similarly,
Bottom Line
We have derived a set of handy equations necessary for calculating the primary directions. Here is the recap of what we got
Spherical triangle.
