The Universe Is Expanding — Question 1

Section 44-10 · Physics pages 7472–7473

Question 1 A spectral line measures the relative cosmic scale factor A spectral line emitted at 500 nm is observed at 650 nm. Assume the shift is entirely cosmological and normalize the present scale factor to one. expansion earlier later Schematic; labels, not drawing lengths, specify the data. (a) Find redshift and the emission scale factor. (b) Find the observed-to-emitted photon energy ratio and the emission proper separation of two comoving objects now 100 Mpc apart.
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Question 1 - Solution A spectral line measures the relative cosmic scale factor expansion earlier later (a) Method and calculation z = λo/λe −1 = 650/500 −1 = .30 . ae = 1/(1 + z) = 10/13 = .769231 . (b) Interpretation and further calculation Eo/Ee = λe/λo = 10/13 . De = aeD0 = 76.9231 Mpc . Physical check The separation comparison is at common cosmic times, not a light-travel distance. Bound systems do not generally follow this scaling.

Question 1

A spectral line measures the relative cosmic scale factor

A spectral line emitted at 500 nm is observed at 650 nm. Assume the shift is entirely cosmological and normalize the present scale factor to one.

Diagram shown in the original SVG worksheet.

  1. Find redshift and the emission scale factor.

  2. Find the observed-to-emitted photon energy ratio and the emission proper separation of two comoving objects now 100 Mpc apart.

Question 1 - Solution

A spectral line measures the relative cosmic scale factor

Diagram shown in the original SVG worksheet.

(a) Method and calculation

z=λo/λe−1=650/500−1=.30.\boxed{z=\lambda_o/\lambda_e-1=650/500-1=.30}.ae=1/(1+z)=10/13=.769231.\boxed{a_e=1/(1+z)=10/13=.769231}.

(b) Interpretation and further calculation

Eo/Ee=λe/λo=10/13.\boxed{E_o/E_e=\lambda_e/\lambda_o=10/13}.De=aeD0=76.9231Mpc.\boxed{D_e=a_eD_0=76.9231\ {\mathrm{Mpc}}}.

Physical check

The separation comparison is at common cosmic times, not a light-travel distance. Bound systems do not generally follow this scaling.