Redshift Calculator
With our redshift calculator, you can determine the magnitude of redshift – an interesting phenomenon in astrophysics.
The formula
v = H₀d; 1 + z = λ_obs/λ_emit; d(pc) = 1/p(arcsec)
v = cz breaks before you expect
The simple reading of redshift as velocity, v = cz, is a low-redshift approximation. It is already a few percent wrong by z = 0.1 and gives faster than light for z > 1, which is why quasars at z = 6 are not receding at six times the speed of light. The relativistic Doppler formula is used above, and it saturates at c as z grows.
Strictly, cosmological redshift is not a Doppler shift at all. The light is stretched by the expansion of space during its journey rather than emitted at a shifted frequency. That distinction is why recession velocities greater than c are permitted at large distances: nothing is moving through space faster than light, the space between is simply growing.
The parsec is a definition
A parsec is defined as the distance at which a star shows one arcsecond of parallax across Earth's orbit, so distance in parsecs is exactly the reciprocal of parallax in arcseconds. There is no physics in the conversion — it is a definition, which is precisely what makes parallax the one rung of the distance ladder that needs no assumptions.
Why the sky is dark
Olbers' paradox observes that in an infinite, eternal, static universe every line of sight would eventually meet a star, so the whole sky should be as bright as the Sun. The resolution is the finite age of the universe: light from beyond a certain distance simply has not had time to reach us. Redshift dims what does arrive, but the finite age is the main answer.