Analytical expressions for calculating the energy density and spatial correlation function of thermal emission by a homogeneous, isothermal sphere of arbitrary size and material are presented. The spectral distribution and the power law governing the distance-dependent energy density are investigated in the near-field and far-field regimes for silicon carbide (dielectric), silicon (semiconducting), and tungsten (metallic) spheres of various size parameters ranging from to 5. The spatial coherence of the thermal field emitted by spheres of different size and material is also studied in both radial and polar directions, and the effect of localized surface phonons (LSPhs) on the correlation length and angle is elucidated. It is shown that the energy density follows a power law of ( is the observation distance) in the far field independent of the size and material of the sphere. The power law in the near field is strongly dependent on the material, size parameter, and the ratio ( is the sphere radius). In the near field, the energy density follows a power law of when and (similar to an electric point dipole). With increasing or decreasing , the contribution of multipoles to the energy density increases resulting in an increase in the power of until the power law converges to that for a semi-infinite medium (, , and for silicon carbide, silicon, and tungsten, respectively, in the intermediate near field, and , , and for silicon carbide, silicon, and tungsten, respectively, in the extreme near field.). It is also found that the spatial correlation length in the radial direction is approximately on the order of λ, 0.1λ, and 0.001λ in the far-field, intermediate near-field, and extreme near-field regimes, respectively, when the multipolar LSPhs are not supported. The correlation angle in the extreme near field is strongly dependent on the sphere size parameter, such that it decreases by three orders of magnitude (from 0.5π to 0.001π) when increases from 0.002 to 5. The dependence of the correlation angle on decreases significantly in the intermediate near-field and far-field regimes, and the correlation angle retains the same order of magnitude (0.15π − 0.7π) for all considered in these two regimes. While the excitation of dipolar LSPhs does not affect the correlation length and angle of the thermal field, the multipolar LSPhs reduce the spatial coherence in both directions.