Dark Matter — Question 6

Section 44-12 · Physics pages 7522–7523

Question 6 A cluster collision separates gas drag from the lensing mass pattern In a hypothetical merger, a lensing mass peak is 150 kpc ahead of the X-ray gas peak along the collision axis. Assume a constant relative speed 1500 km/s and 1 kpc=3.086 × 1016 km. gas lensing peak 150 kpc Schematic; labels, not drawing lengths, specify the data. (a) Estimate the time needed to produce the offset and express it in Myr using 1 year=3.156 × 107 s. (b) Explain how mass following collisionless galaxies rather than the dominant baryonic gas tests a gas-only mass model.
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Question 6 - Solution A cluster collision separates gas drag from the lensing mass pattern gas lensing peak 150 kpc (a) Method and calculation t = d/v = 150(3.086 × 1016) 1500 = 3.086 × 1015 s. t ≃97.8 Myr . (b) Interpretation and further calculation Σlens = Σgas + Σ⋆+ Σother. offset mass and gas peaks require more than a gas-traces-all-mass model . Physical check The time is a projected, constant-speed estimate. Combined lensing, gas and galaxy observations constrain mass distribution without determining the dark particle identity.

Question 6

A cluster collision separates gas drag from the lensing mass pattern

In a hypothetical merger, a lensing mass peak is 150 kpc ahead of the X-ray gas peak along the collision axis. Assume a constant relative speed 1500 km/s and 1 kpc=3.086×10163.086\times10^{16} km.

Diagram shown in the original SVG worksheet.

  1. Estimate the time needed to produce the offset and express it in Myr using 1 year=3.156×1073.156\times10^7 s.

  2. Explain how mass following collisionless galaxies rather than the dominant baryonic gas tests a gas-only mass model.

Question 6 - Solution

A cluster collision separates gas drag from the lensing mass pattern

Diagram shown in the original SVG worksheet.

(a) Method and calculation

t=d/v=150(3.086×1016)1500=3.086×1015s.t=d/v=\frac{150(3.086\times10^{16})}{1500}=3.086\times10^{15}\ {\mathrm{s}}.t≃97.8Myr.\boxed{t\simeq97.8\ {\mathrm{Myr}}}.

(b) Interpretation and further calculation

Σlens=Σgas+Σ⋆+Σother.\Sigma_{\mathrm{lens}}=\Sigma_{\mathrm{gas}}+\Sigma_\star+\Sigma_{\mathrm{other}}.offset mass and gas peaks require more than a gas-traces-all-mass model.\boxed{\text{offset mass and gas peaks require more than a gas-traces-all-mass model}}.

Physical check

The time is a projected, constant-speed estimate. Combined lensing, gas and galaxy observations constrain mass distribution without determining the dark particle identity.