Astrophysics (Index)About

optics

(science and technology regarding visible light)

The word optics refers to the science and technology regarding the behavior and handling of visible light, the term being used for the principles and mechanisms of telescopes and telescopic instruments such as cameras/imagers and spectrographs. It is sometimes analogously used regarding other parts of the electromagnetic spectrum, especially portions of ultraviolet and infrared spectra that are adjacent to visible light, that are handled using virtually the same type of equipment. The adjective optical is also sometimes meant to encompass near infrared and/or near ultraviolet.

A branch of the science that deals with aspects of optics that are unexplainable by regarding EMR as classical waves is termed quantum optics.


The word optics is often used for a telescope or instrument's optical devices or the optical portion or aspect of a device. EMR further from visible light has some parallels regarding design and function, and the word optics is often used, such as in the phrase, X-ray optics.


(science,visible light,EMR,instruments,telescopes)
Further reading:
https://en.wikipedia.org/wiki/Optics
https://en.wiktionary.org/wiki/optics
https://phys.libretexts.org/Bookshelves/Optics
https://www.britannica.com/science/optics

Referenced by pages:
aberration
adaptive optics (AO)
airglow
anastigmat
angular magnification
aspheric mirror
astigmatism
barrel distortion
beat frequency
chopping mirror
chromatic aberration
COAST
collimator
coma
convolution
core-cusp problem
correlator
coudé focus telescope
current sheet
cylindrical telescope
diffraction
distortion
eigenmode
etalon
European Southern Observatory Very Large Telescope (ESO VLT)
exit pupil
field curvature
filter
first light
focal length
focal plane
focal plane tilt
Fred Young Submillimeter Telescope (FYST)
grating
grazing incidence optics (GIO)
guide star (GS)
Hale Telescope
Hanbury Brown and Twiss effect (HBT effect)
Hubble Space Telescope (HST)
illumination
integral field spectrograph
integral field unit (IFU)
interferometer
Large Altazimuth Telescope (BTA-6)
linearly variable filter (LVF)
liquid mirror telescope
Lyot stop
Magellan Telescopes
near infrared (NIR)
observatory (obs.)
off-axis telescope
optical axis
optical depth (τ)
optical interferometer
passband
phase plate
PHIBSS
pincushion distortion
point-spread function (PSF)
pointing error (PE)
prime focus
PSF fitting
radar
radiometer
real image
reflector telescope
seeing
segmented mirror
sensitivity function (S)
Southern African Large Telescope (SALT)
speckles
spectropolarimetry
speed of light (c)
spherical aberration
starshade
Strehl ratio
telescope type
velocity dispersion (σ)
visible light
wavefront error (WFE)
WINERED
Wolter telescope
XEUV

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