Uniform Expansion
- Objects at distance D0 now are at D(t) = a(t) * D0, a(0) = 1
- If a(t) ~ 1 + H0 * t for small H0 * t, D(t) ~ D0 + H0 * D0 * t
- So v0 = H0 * D0. Write this as H0 = a(0)
- Cosmological redshift 1 + z = observed_wavelength / emitted_wavelength = a(t-obs) / a(t-emited) = 1 / a(t-emited)
1 / 1 + H0 * t-emitted ~ 1 - H0 * t-emitted (Newton's approximation)