In simulating a star for a radio telescope, it is suggested that the wavefront from stars can be approximated as a plane wave due to the vast distances involved. The van Cittert-Zernike theorem supports this by indicating that the wave will be spatially coherent, essential for the functioning of a radiotelescope. While a Gaussian beam can resemble a plane wave at infinite distances, it is not ideal for simulating starlight, which is incoherent near the star. The coherence of starlight develops only after traveling significant distances, such as to Earth. The discussion concludes with the need for alternative simulation tools, as Zemax lacks a suitable plane wave simulation for long wavelengths.