We study continuous phase spaces of single spins and develop a complete description of their time evolution. The time evolution is completely specified by so-called star products. We explicitly determine these star products for general spin numbers using a simplified approach which applies spin-weighted spherical harmonics. This approach naturally relates phase spaces of increasing spin number to their quantum-optical limit and allows for efficient approximations of the time evolution for large spin numbers. We also approximate phase-space representations of certain quantum states that are challenging to calculate for large spin numbers. All of these applications are explored in concrete examples and we outline extensions to coupled spin systems.Phase-space techniques provide a complete description of quantum mechanics which is complementary to Hilbert-space [1] and path-integral [2] methods. These techniques are widely used in order to describe, visualize, and analyze quantum states [3][4][5][6][7][8][9][10][11][12]. Particular cases include Wigner [13], Husimi Q [14], and Glauber P [15] functions. In this work, we are particularly interested in phase-space methods that are applicable to (finite-dimensional) spin systems [16][17][18][19][20][21][22][23][24][25][26][27] and how these methods are related to infinitedimensional phase spaces [28]. Building on earlier results in [17,18,21,22,27,29], we have developed in [28] a unified description for the general class of s-parametrized phase spaces with −1 ≤ s ≤ 1 which is applicable to single spins with integer or half-integer spin number J and which naturally recovers the infinite-dimensional case in the large-J limit. The s-parametrized phase-space function corresponding to a Hilbert-space operator A is denoted by F A (Ω, s).A new focus emerged recently with the objective to faithfully describe coupled spin systems with the help of phase-space representations [29][30][31][32][33][34][35][36][37][38] while also emphasizing arXiv:1808.02697v2 [quant-ph] 7 Nov 2018 J 3 2 J 4 J 10 J 10 2 J 10 3 J 10 5 J → ∞ 92.8 % 30.2 % 11.6 % ≈1 % ≈0.1 % ≈0.001 %