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Cosmology is the study of the character and evolution of the universe.The two most important features of the universe are the cosmological red shifts of its galaxies being proportional to distance and its cosmic microwave background (CMBR).

The mass of luminous matter of the value \({\rm{m}}\) in our galaxy is:

\(\begin{array}{c}{M_L} &= {\rm{1}}{{\rm{0}}^{{\rm{11}}}}{\rm{ \times 1}}{\rm{.5 \times }}{{\rm{m}}_{\rm{s}}}\\ & = {\rm{1}}{{\rm{0}}^{{\rm{11}}}}{\rm{ \times 1}}{\rm{.5 \times (1}}{\rm{.99 \times 1}}{{\rm{0}}^{{\rm{30}}}}{\rm{kg)}}\\ &= {\rm{2}}{\rm{.98 \times 1}}{{\rm{0}}^{{\rm{41}}}}{\rm{kg}}\end{array}\)

The value of\({{\rm{m}}_{\rm{s}}}\)denotes the mass of the Sun.

We then know that the mass of dark matter is:

\({M_D} = 10{M_L}\)....... (i)

The total mass is then obtained as:

\(\begin{array}{c}{M_{tot}} &= {M_L} + {M_D}\\ &= {\rm{11}} {M_L}\\ &= {\rm{ 3}}{\rm{.28 \times 1}}{{\rm{0}}^{{\rm{42}}}}{\rm{ kg}}\end{array}\)\(\)

Therefore, the total mass is: \({\rm{3}}{\rm{.28 \times 1}}{{\rm{0}}^{{\rm{42}}}}{\rm{ kg}}\).