telescopes
DESCRIPTION
Telescopes. Refractors and Reflectors Various Designs Important Properties Modern Advances Beyond Visible Light. Basic Optics - Refraction. Light is bent or refracted when it changes speed going through a lens or prism. Where the refracted rays meet is the “focal point.” - PowerPoint PPT PresentationTRANSCRIPT
-
TelescopesRefractors and ReflectorsVarious DesignsImportant PropertiesModern AdvancesBeyond Visible Light
-
Basic Optics - RefractionLight is bent or refracted when it changes speed going through a lens or prism.Where the refracted rays meet is the focal point.Distance from the lens to the focal point is the focal length.
-
Basic Optics - ReflectionWhen light strikes a mirror it is reflected at an angle equal to its incident angle.Rays of light striking a curved mirror will meet at a focal point.The distance from the vertex of the mirror to the focal point is the focal length.
-
Reflectors and RefractorsA reflector telescope has a mirror as its objective.A refractor telescope has a lens as its objective.The main function of a telescope is to gather light.
-
Chromatic AberrationDifferent wavelengths focus at different distancesWorlds Largest Refractor - Yerkes Observatory
-
Reflectors
-
Why Mirrors?Light gathering power - size matters!lgp increases with the square of the radiusMore lgp, more resolution!Magnification is third!
-
200 Hale Telescope Mt. Palomar
-
Comparing lgp lgp depends upon the area of the lens or mirror; A = r2
lgp = (Dbig/Dsmall)2
-
Calculating Magnificationfobjfeye
M =Mmax = 20 x Dcm
-
Practical Limit of MagnificationSmaller focal length eyepieces give greater magnification.They also limit light & increase diffraction.At some point the image is too poor to be useful.
Mmax = 20X____cmx D
-
Resolving PowerThe ability of a telescope to distinguish two objects.Measured in arcseconds ( 1 arcsecond is 1/3600)a =11.58_______D (in cm)
-
Modern AdvancesBinocular TelescopesLBT - two 8.4 m mirrors with adaptive opticsLGP of an 11.8 m mirrorDetail of a 22.4 m mirrorSurpasses HST in clarity
-
Adaptive OpticsCorrect for atmospheric turbulenceUse the light from a guide star or laser to determine what the atmosphere is doing to the light passing through it.Distortable mirror will change shape to correct the image.
-
Beyond Visible LightRadio Telescopes
-
VLA Telescope
-
UV and X-Ray TelescopesSOHOChandra
-
HST and James Webb
/