Astrophysics (Index)About

aberration

(types of flaws in telescope images)

In optics, aberration is an optical system's deviation from true, such as points in the image being smeared and/or shapes being changed. Lenses and mirrors inevitably cause some aberration which can be the primary limit to a telescope's use. Though some aberrations cannot be entirely eliminated, specific lens and mirror designs reduce some, as can the overall design of telescopes (e.g., a larger focal length reduces some of them). Aberrations come from a variety of causes resulting in a variety of symptoms. Some terms/classes:

The five Seidel aberrations (aka Seidel errors) are five of these that were explained in the mid-19th century by Philipp Ludwig von Seidel, which were spherical aberration, coma, astigmatism, field curvature, and distortion.


The term aberration has other uses in astronomy that are not related to optics, i.e., "perfect" optics would still be affected:


(telescopes,optics)
Further reading:
https://en.wikipedia.org/wiki/Optical_aberration
https://en.wikipedia.org/wiki/Aberration_(astronomy)
https://en.wikipedia.org/wiki/Relativistic_aberration
https://en.wikipedia.org/wiki/Optical_telescope#The_five_Seidel_aberrations
http://www.telescope-optics.net/aberrations.htm
https://www.handprint.com/ASTRO/ae4.html
http://www.quadibloc.com/science/opt0505.htm

Referenced by pages:
anastigmat
aspheric mirror
astigmatism
astrograph
barrel distortion
chromatic aberration
coma
convolution
Dall-Kirkham telescope
deformable mirror (DM)
distortion
field curvature
focal plane
Herschelian telescope
image stabilization
Korsch telescope
null corrector
paraboloid
pincushion distortion
pointing error (PE)
refracting telescope
Ritchey-Chrétien telescope (RCT)
Schiefspiegler
Schmidt camera
Schwarzschild telescope
speckles
spherical aberration
Strehl ratio
three-mirror anastigmat
wavefront error (WFE)

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