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(a) Calculate the approximate age of the universe from the average value of the Hubble constant,\({{\rm{H}}_{\rm{0}}}{\rm{ = 20km/s}} \cdot {\rm{Mly}}\). To do this, calculate the time it would take to travel\({\rm{1 Mly}}\)at a constant expansion rate of\({\rm{20 km/s}}\). (b) If deceleration is taken into account, would the actual age of the universe be greater or less than that found here? Explain.

Short Answer

Expert verified

(a) The age of the universe is obtained as: \(t = {\rm{ 1}}{\rm{.5 \times 1}}{{\rm{0}}^{{\rm{14}}}}{\rm{ y}}\).

(b) The actual age of the universe will be less.

Step by step solution

01

Recession velocity

The recession velocity for a galaxy is given by,

\(v = {H_o}d\)

Here\({H_o}\)is the Hubble constant and\(d\)is the distance to the galaxy.

02

Evaluating the age

Taking the edge of the universe having \({\rm{10 Gly}}\) away from us, we then obtain:

\(\begin{array}{c}t = \frac{D}{v}\\ = \frac{{{\rm{1}}{{\rm{0}}^{{\rm{10}}}}{\rm{ \times 3 \times 1}}{{\rm{0}}^{\rm{8}}}{\rm{m/s}}}}{{{\rm{20}}\,{\rm{km/s}}}}y\\ = {\rm{1}}{\rm{.5 \times 1}}{{\rm{0}}^{{\rm{14}}}}{\rm{ y}}\end{array}\)

Therefore, the age of the universe is \({\rm{1}}{\rm{.5 \times 1}}{{\rm{0}}^{{\rm{14}}}}{\rm{ y}}\).

03

Explanation for part b

As, we haven't factored in deceleration, this time is really \({\rm{1}}{{\rm{0}}^{\rm{4}}}\) times shorter, therefore it's an overestimate.

Therefore, the age of the universe is less.

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Most popular questions from this chapter

Another known cause of red shift in light is the source being in a high gravitational field. Discuss how this can be eliminated as the source of galactic red shifts, given that the shifts are proportional to distance and not to the size of the galaxy.

(a) Estimate the mass of the luminous matter in the known universe, given there are\({\rm{1}}{{\rm{0}}^{{\rm{11}}}}\)galaxies, each containing\({\rm{1}}{{\rm{0}}^{{\rm{11}}}}\)stars of average mass\({\rm{1}}{\rm{.5}}\)times that of our Sun. (b) How many protons (the most abundant nuclide) are there in this mass? (c) Estimate the total number of particles in the observable universe by multiplying the answer to (b) by two, since there is an electron for each proton, and then by\({\rm{1}}{{\rm{0}}^{\rm{9}}}\), since there are far more particles (such as photons and neutrinos) in space than in luminous matter.

To get an idea of how empty deep space is on the average, perform the following calculations: (a) Find the volume our Sun would occupy if it had an average density equal to the critical density of\({\rm{1}}{{\rm{0}}^{{\rm{ - 26}}}}{\rm{kg/}}{{\rm{m}}^{\rm{3}}}\)thought necessary to halt the expansion of the universe. (b) Find the radius of a sphere of this volume in light years. (c) What would this radius be if the density were that of luminous matter, which is approximately\({\rm{5 \% }}\)that of the critical density? (d) Compare the radius found in part (c) with the\({\rm{4 - ly}}\)average separation of stars in the arms of the Milky Way.

Distances to the nearest stars (up to\({\rm{500 ly}}\)away) can be measured by a technique called parallax, as shown in Figure\({\rm{34}}{\rm{.26}}\). What are the angles\({{\rm{\theta }}_{\rm{1}}}\)and\({{\rm{\theta }}_{\rm{2}}}\)relative to the plane of the Earthโ€™s orbit for a star\({\rm{4}}{\rm{.0 ly}}\)directly above the Sun?

Distances to very remote galaxies are estimated based on their apparent type, which indicate the number of stars in the galaxy, and their measured brightness. Explain how the measured brightness would vary with distance. Would there be any correction necessary to compensate for the red shift of the galaxy (all distant galaxies have significant red shifts)? Discuss possible causes of uncertainties in these measurements.

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