The article proposes a causal five-field formulation of dissipative relativistic fluid dynamics as a quasilinear symmetric hyperbolic system of second order. The system is determined by four dissipation coefficients
η
,
ζ
,
κ
,
μ
\eta ,\zeta ,\kappa ,\mu
, free functions of the fields, which quantify shear viscosity, bulk viscosity, heat conductivity, and diffusion.