In spherical coordinates, consider a potential that depends only on r and θ. The convention for spherical coordinates is that θ is the angle down from the north pole, and ϕ is the angle around the equator. The Lagrangian is
L=21m(r˙2+r2θ˙2+r2sin2θϕ˙2)−V(r,θ).
Identify the cyclic coordinate and the corresponding conserved quantity.