redshift
C2Pronunciation
UK
- /rˈɛdʃɪft/
US
- /rˈɛdʃɪft/
Description
- Stretching of light
- moving away
- cosmic distance indicator
Imagine shouting to a friend. If they run away from you as you speak, the sound of your voice will seem lower in pitch—stretched out. That's essentially what redshift is! It happens with light when something emitting that light (like a distant galaxy) is moving away from us. The light waves get "stretched," making them appear redder than they otherwise would be.
Astronomers use redshift like a cosmic measuring stick. The more redshift we see, the faster an object is receding and, generally, the farther away it is! It's a key piece of evidence supporting the idea that the universe is expanding. Think of it as a clue revealing the history and structure of space itself.
Redshift is a phenomenon where light (or other electromagnetic radiation) from an object undergoes an increase in wavelength, shifting towards the red end of the spectrum. It's analogous to the Doppler effect you experience with sound—think about how the pitch of a siren changes as it moves toward or away from you.
The Doppler effect explains redshift caused by relative motion, such as a star or galaxy moving away from us. There is also *cosmological redshift. This happens because space itself is expanding, stretching the wavelengths of light traveling through it. The farther away an object is, the more its light has been stretched by this expansion, and therefore the greater its redshift. A third kind, gravitational redshift*, happens when light climbs out of a strong gravitational field and loses energy, which also increases its wavelength.
Redshift isn't just about color! It's measured precisely using spectroscopy—splitting light into its component colors to identify shifts in spectral lines. These shifts reveal not only that something is moving away, but also how fast it is traveling.
Astronomers rely heavily on redshift to understand the universe's expansion rate (Hubble's Law), determine distances to incredibly far objects, and study the evolution of galaxies. It's a fundamental concept in cosmology, helping us piece together the story of our vast and expanding cosmos. Without understanding redshift, we wouldn't have nearly as much insight into the age, size, and fate of the universe!
Examples
- 1
Galaxy motion
Astronomers measured the redshift of the galaxy to estimate how fast it was moving away from Earth.
Pattern
measure the redshift of + object
calculate this change in its light
- 2
Light travel
A larger redshift usually means we are looking at light that has traveled for a very long time.
- 3
Early universe
The new telescope is designed to study galaxies at high redshift, from the early universe.
Phrase
at high redshift
so far away that we see objects as they were very early in the universe
Forms and spellings
1 form open this card.
Main spelling
- redshiftnoun