Recent findings in astrophysics suggest that the observable universe can be modeled as a sphere of radius R = 13.7 × 109 light-years = 13.0 × 1025 m with an average total mass density of about 1 × 10-26 kg/m3. Only about 4% of total mass is due to "ordinary" matter (such as protons, neutrons, and electrons). Part A Estimate how much ordinary matter (in kg) there is in the observable universe.

Respuesta :

Answer:

[tex]3.7\times 10^{51})[/tex] kg

Explanation:

[tex]R[/tex] = radius of the sphere modeled as universe = [tex]13\times 10^{25}[/tex] m

Volume of sphere is given as

[tex]V = \frac{4\pi R^{3}}{3}[/tex]

[tex]V = \frac{4(3.14) (13\times 10^{25})^{3}}{3}[/tex]

[tex]V = 9.2\times 10^{78}[/tex] m³

[tex]\rho [/tex] = average total mass density of universe = [tex]1\times 10^{-26}[/tex] kg/m³

[tex]m[/tex] = Total mass of the universe = ?

We know that mass is the product of volume and density, hence

[tex]m = \rho V[/tex]

[tex]m = (1\times 10^{-26}) (9.2\times 10^{78})[/tex]

[tex]m = 9.2\times 10^{52}[/tex] kg

[tex]M[/tex] = mass of "ordinary" matter  = ?

mass of "ordinary" matter is only about 4% of total mass, hence

[tex]M = (0.04) m[/tex]

[tex]M = (0.04)(9.2\times 10^{52})[/tex]

[tex]M = 3.7\times 10^{51}[/tex] kg

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