Relative to the Sun, therefore, the density is: where ρ ⊙ {\displaystyle {\begin{smallmatrix}\rho _{\odot }\end{smallmatrix}}} is the average solar density.
Relative to the Sun, therefore, the density is: ρ ⊙ {\displaystyle {\begin{smallmatrix}\rho _{\odot }\end{smallmatrix}}} は太陽の密度を表す。