The discussion centers on whether cosmological redshift should be viewed solely as a kinematic Doppler effect or as a result of the time dynamics of metric space. It highlights that for distant objects, the curvature of space-time is essential for accurate redshift calculations, while for closer objects, the relativistic Doppler effect suffices. As distances approach a Hubble radius, relying only on the Doppler effect becomes inadequate, necessitating consideration of space-time curvature. The conversation suggests that both perspectives may need to converge for a comprehensive understanding. Ultimately, the treatment of redshift requires careful consideration of both kinematic and metric factors.