Galaxy Rotation Curves

near-ready GalaxiesCosmologyData & Inference Both 16 min
Active development: beta / candidate
Close to ready. Still to come: clearer wording about the MOND limit, an honest caption for the galaxy view, and sliders that show when they are locked.
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Predict

Predict

If a galaxy had only visible bulge+disk mass, what should happen to orbital speed from $30$ to $50\,{\rm kpc}$, and what would that imply for $M(<R)$?

Play

Play

  1. Start with `No dark matter` and trace the outer slope from $30$ to $50\,{\rm kpc}$.
  2. Switch to `Milky Way-like` and compare $V_{\rm total}$ with $V_{\rm Kep}$ at the same radii.
  3. Increase halo mass and watch the outer curve flatten while $M_{\rm dark}/M_{\rm vis}$ rises.
  4. Toggle to mass mode and identify where $M_{\rm dark}$ exceeds $M_{\rm vis}$.
  5. Turn on MOND and compare it to the dark-halo model at galaxy scales.
  6. Use the normalized inset to contrast solar-system Keplerian behavior with galaxy behavior.
  7. Run one mystery challenge round, then copy challenge evidence for debrief.
Explain

Explain

At $R=30\,{\rm kpc}$, why can two models produce similar speeds while implying different physical interpretations, and what additional scale-dependent evidence breaks the tie?

Learning goals

  • Interpret galaxy rotation curves as velocity-versus-radius observables inferred from Doppler measurements.
  • Compare visible-matter-only Keplerian predictions to flat observed curves and infer missing mass.
  • Relate bulge, disk, and halo component models to total curve shape and enclosed-mass growth.
  • Use baryon fraction and dark-to-visible ratio readouts to reason about mass budgets at large radius.

Misconceptions targeted

  • Galaxies should behave like the solar system, so outer stars must always slow as $R^{-1/2}$.
  • A face-on schematic means real observations are made face-on too.
  • A good MOND fit to galaxy curves means dark matter is ruled out at all scales.

Model notes

  • Mass model uses a Hernquist bulge, exact exponential disk rotation (modified Bessel $I_n$/$K_n$ terms), and NFW halo.
  • Velocities add in quadrature: $V_{\rm total}^2=V_{\rm bulge}^2+V_{\rm disk}^2+V_{\rm halo}^2$.
  • NFW derived quantities ($R_{\rm vir}$, $c$) use internal cosmology defaults ($H_0=67.4\,{\rm km\,s^{-1}\,Mpc^{-1}}$, $\Omega_m=0.315$).
  • MOND is shown as an optional comparison curve via full interpolation, not as a full parameter-fitting workflow.
  • The galaxy panel is a face-on schematic; published curves are inclination-corrected intrinsic $V(R)$.
  • Readout $\Delta\lambda_{21}$ uses $\Delta\lambda_{21}=\lambda_0 V/c$ with $\lambda_0=21.106\,{\rm cm}$.

About this demo

Explore why spiral-galaxy rotation curves stay nearly flat at large radius and what that implies about dark matter across scales.