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White dwarfs are one of the densest form of matter following neutron star andblack holes. A typical white dwarf is as massive as our sun has radiuscomparable to the earth. This paper reviewed the Fermi gas model Equation ofState of white dwarfs and numerical computation of mass-radius and pressuredensity profile. A section in brief has been included for the calculation ofaverage speed of electrons in the white dwarf environment.

Equation of State of White Dwarfs and Mass-Radius Estimation in the Newtonian Limit