Doppler Redshift Calculator

Cosmological redshift measures how much light from distant objects has been stretched by the expansion of the universe. Redshift z = 1 means the universe has expanded to twice its size since the light was emitted.

🌀 Cosmology📐 z = v/c🔭 Astrophysics
Observed Wavelength (nm)
Rest Wavelength (nm)
Or enter redshift z directly
Please enter valid values.

Formula & Reference

VariableSymbolFormulaUnits
Redshiftzz = Δλ/λ = v/c (small v)
Relativisticzz = √((1+v/c)/(1−v/c)) − 1
Distance (Hubble)dd = cz/H0Mpc
Lookback Timet~z/H0 (approx, low z)Gyr

Step-by-Step Examples

Example 1
Galaxy Spectrum

H-alpha normally at 656 nm, observed at 700 nm.

  • z = (700-656)/656 = 44/656 = 0.067
  • v = c * z = 0.067 * 3e5 = 20,100 km/s
  • d = v/H0 = 20,100/70 = 287 Mpc
✓ z=0.067, distance 287 Mpc
Example 2
Quasar z=3

Known redshift z=3 (observed wavelengths 4x rest).

  • v = c*((4^2-1)/(4^2+1)) = c*15/17 = 0.882c
  • d = c*z/H0 = 3e5*3/70 = 12,857 Mpc
✓ Recession at 88% of light speed, ~13 billion parsecs away
Example 3
CMB Redshift

Cosmic Microwave Background: rest T=3000 K (recombination), observed T=2.725 K.

  • z = 3000/2.725 - 1 = 1100
  • Universe has expanded 1101x since recombination ~380,000 years after Big Bang
✓ z=1100 — the most redshifted signal we observe

Real-World Applications

🔭
Galaxy Distance Measurement
Redshift gives recession velocity; Hubble law gives distance to galaxies beyond Cepheid range.
🌀
Dark Energy Discovery
Supernovae redshift-distance relation showed acceleration, implying dark energy.
📡
Quasar Science
Quasars at z=7 observed when universe was <1 Gyr old; redshift reveals cosmic history.
🌈
CMB Cosmology
CMB at z=1100 maps the universe at 380,000 years after Big Bang.

Common Mistakes to Avoid

⚠️
Non-relativistic formula fails at high z

z = v/c only valid for v << c. Use z = sqrt((1+v/c)/(1-v/c)) - 1 for relativistic recession.

⚠️
Cosmological vs Doppler redshift

Cosmological redshift is from space expanding, not object motion. True velocity is defined differently. For small z, cz gives recession velocity.

⚠️
Distance from z is approximate

d = cz/H0 valid only for z < 0.1. For larger z, full cosmological model needed, depending on dark energy equation of state.

Frequently Asked Questions

What is redshift z?
z = (lambda_observed - lambda_emitted)/lambda_emitted = delta_lambda/lambda. z=0 means no shift. z=1 means wavelength doubled (universe doubled in size since emission).
How is redshift measured?
Spectral lines from known elements (H, Ca, Mg) are identified in galaxy spectra at shifted wavelengths. The shift z = (lambda_obs - lambda_rest)/lambda_rest.
What is blueshift?
z < 0 means the object is approaching. Andromeda galaxy has z = -0.001 (approaching at 110 km/s). Rare for distant galaxies.
What is the most distant object observed?
Galaxy GN-z11 at z = 10.96, observed when universe was ~430 million years old. JWST detected galaxies at z > 13.
How does CMB redshift work?
Photons from recombination epoch (z=1100) have been traveling for 13.8 Gyr. Universe has expanded 1101x, stretching photon wavelengths into microwave range.

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Formula Explorer connections

Interpretation: This relationship connects frequency, wavelength, speed, phase, intensity or resonance in an oscillating system. Assumption: Identify the medium, boundary conditions and reference frame. Linear waves, small amplitudes, nondispersive media or ideal resonance may be assumed.

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