Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Relativistic Doppler effect
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
{{Special relativity sidebar}} {{short description|Scientific phenomenon}} [[Image:Velocity0 70c.jpg|thumb|right|Figure 1. A source of light waves moving to the right, relative to observers, with velocity 0.7''c''. The frequency is higher for observers on the right, and lower for observers on the left.]] The '''relativistic Doppler effect''' is the change in [[frequency]], [[wavelength]] and [[amplitude]]<ref>{{cite book |title=Relativistic Electron Mirrors: from High Intensity Laser–Nanofoil Interactions |author1=Daniel Kiefer |edition=illustrated |publisher=Springer |year=2014 |isbn=978-3-319-07752-9 |page=22 |url=https://books.google.com/books?id=qdYkBAAAQBAJ}} [https://books.google.com/books?id=qdYkBAAAQBAJ&pg=PA22 Extract of page 22]</ref> of light, caused by the relative motion of the source and the observer (as in the classical [[Doppler effect]], first proposed by Christian Doppler in 1842<ref>{{Cite web |url=https://pubs.aip.org/physicstoday/article/73/3/30/850595/The-fall-and-rise-of-the-Doppler-effectThe |title=The Fall and Rise of the Doppler Effect ... |last=Nolte |first=David |date=2020-03-01 |website=pubs.aip.org/physicstoday |access-date=2024-11-02}}</ref>), when taking into account effects described by the [[special relativity|special theory of relativity]]. The relativistic Doppler effect is different from the non-relativistic [[Doppler effect]] as the equations include the [[time dilation]] effect of [[special relativity]] and do not involve the medium of propagation as a reference point. They describe the total difference in observed frequencies and possess the required [[Lorentz symmetry]]. Astronomers know of three sources of [[redshift]]/[[blueshift]]: Doppler shifts; [[gravitational redshift]]s (due to light exiting a gravitational field); and [[cosmological expansion]] (where space itself stretches). This article concerns itself only with Doppler shifts.
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)