speed of light
(c, light speed, speed of light in a vacuum, light's speed)
(fundamental constant measured as the speed at which light travels)
The speed of light (or light speed, or, more precisely,
the speed of light in a vacuum, symbolized as c)
is a fundamental constant, precisely 299,792,458 meters per second
(because the latest refined definition of a meter is c/299,792,458)
which is roughly 186,000 miles per second,
and is the speed at which any EMR is measured to travel through
a vacuum. Due to this less-than-infinite speed, observing at astronomical
distances is also looking "backward in time".
Outside a vacuum, light moves slower than this, e.g., in liquid water,
about 25% slower. Air has a much smaller effect, but glass (including
fiber optics) has the same order-of-magnitude reduction as
water, and according to the science of optics, it this
reduction that makes glass lenses function.
The speed of light (in a vacuum) always measures to the same
quantity, even though light acts like waves. (This is unlike sound
waves: if the medium in which sound waves are traveling is also
moving relative to you, sound waves passing you in the
same direction are moving that much faster.)
Relativity spelled out how the speed of
light can be constant in this respect,
and takes it to be more than merely the speed of EMR:
it is the maximum speed at which any influence occurs,
such as the effects of gravity, and it is the speed of gravitational waves.
Quantum mechanics appears to imply effects that transcend
the speed of light, but in very limiting contexts.
(physics,EMR)
Further reading:
https://en.wikipedia.org/wiki/Speed_of_light
https://astronomy.swin.edu.au/cosmos/s/Speed+Of+Light
http://hyperphysics.phy-astr.gsu.edu/hbase/Relativ/ltrans.html#c3
https://math.ucr.edu/home/baez/physics/Relativity/SpeedOfLight/measure_c.html
Referenced by pages:
aberration
astronomical quantities
black-body radiation
Brackett series
Cherenkov radiation
chirp mass (Mc)
CMB dipole
Compton wavelength
cosmic neutrino background (CNB)
cosmological redshift
cyclotron radiation
de Broglie wavelength
Doppler shift
electromagnetic radiation (EMR)
ergosphere
escape velocity (Ve)
focal length
frame dragging
frequency (ν)
general relativity (GR)
gigayear (Gy)
gravitational wave spectrum
gravitational-wave detector
gravitomagnetic field
Great Debate
Humphreys series
hydrogen (H)
inflation
innermost stable circular orbit (ISCO)
Jeans escape
jet
kelvin (K)
kinetic energy (KE)
light cone
light-year (ly)
Lorentz transformation
Lyman series (L)
mass
Maxwell's equations
Michelson interferometer
neutrino oscillation
nondimensionalization
observable universe
OH/IR source
particle horizon
Paschen series
Pfund series
photon
Planck function
Planck units
pulsar timing array (PTA)
radiation pressure
Rayleigh-Jeans law
redshift (z)
refractive index
relativistic beaming
relativistic energy
relativistic invariance
relativistic momentum
relativistic speed
relativity
reverberation mapping
rotation period
Rydberg constant (RH)
Rydberg unit
Schwarzschild radius (RS)
spacetime
spacetime diagram
special relativity (SR)
Starshot
Stefan-Boltzmann constant (σ)
Sunyaev-Zel'dovich effect (SZ effect)
superluminal motion
supernova (SN)
synchrotron radiation
Terrestrial Time (TT)
time standard
wavelength (λ)
wavenumber (ν)
Wien approximation
Index