What can be done to simplify the approach to this method?
L1 ( star observed in Jan ) and L2 ( star observed in Jul ) form adjacent angles ϕ and θ since they share the common side and vertex. Hence Parasec can be considered as the slope of the equation ( m1, m2 ).
This can be put into the general form as :
tanθ=m2−m1/1+m2m1
tanϕ=m1−m2/1+m1m2
This will ease the process to find parsecs, after getting parsecs the distance can be simply measured by using -
d=1/p
where d is the distance ( in parsecs ) and p is the angle in seconds of arc.