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refracting telescope

A Wisdom Archive on refracting telescope

refracting telescope

A selection of articles related to refracting telescope

We recommend this article: refracting telescope - 1, and also this: refracting telescope - 2.
Refracting telescope

ARTICLES RELATED TO refracting telescope

refracting telescope: Encyclopedia II - Angular resolution - Microscope case

The resolution D depends on the angular aperture α: . Here α is the collecting angle of the lens, which depends on the width of objective lens and its distance from the specimen. n is the refractive index of the medium in which the lens operates. λ is the wavelength of light illuminating or emanating from (in the case of fluorescence microscopy) the sample. Due to the limitations of the values α, λ, and n, the resolution limit of a light mic ...

See also:

Angular resolution, Angular resolution - Definition of terms, Angular resolution - Explanation, Angular resolution - Telescope case, Angular resolution - Microscope case

Read more here: » Angular resolution: Encyclopedia II - Angular resolution - Microscope case

refracting telescope: Encyclopedia II - Optician - Eyecare opticians

An optician is an eye care professional who provides lenses for the correction of vision defects. The lenses may be contact lenses, or held in a frame in front of the eye, rarely as a monocle or most frequently as a pair of glasses, also known as spectacles or eyeglasses. The main optical properties of the lenses are specified from a refraction prescription supplied by a person qualified to measure visual defects and write an appropriate corrective prescription. The licensing and nomenclature o ...

See also:

Optician, Optician - Eyecare opticians, Optician - Famous opticians, Optician - Scientific equipment opticians, Optician - Telescope opticians, Optician - Microscope opticians

Read more here: » Optician: Encyclopedia II - Optician - Eyecare opticians

refracting telescope: Encyclopedia II - Binoculars - Optical construction

When light strikes an interface between two materials of different refractive index (e.g., at an air-glass interface), some of the light is transmitted, some reflected. In any sort of image-forming optical instrument (telescope, camera, microscope, etc.), ideally no light should be reflected; instead of forming an image, light which reaches the viewer after being reflected is distributed in the field of view, and reduces the contrast between the true image and the background. Reflection can be reduced, but not eliminated, by applying optical ...

See also:

Binoculars, Binoculars - Prismatic binoculars, Binoculars - Design details, Binoculars - Optical parameters, Binoculars - Optical construction, Binoculars - Image stabilisation, Binoculars - Maintenance, Binoculars - Choosing binoculars

Read more here: » Binoculars: Encyclopedia II - Binoculars - Optical construction

refracting telescope: Encyclopedia II - Eyepiece - Eyepiece properties

Several properties of an eyepiece are likely to be of interest to a user of an optical instrument, when comparing eyepieces and deciding which eyepiece suits their needs. Eyepiece - Design distance to entrance pupil. Eyepieces are optical systems where the entrance pupil is invariably located outside of the system. They must be designed for optimal performance for a specific distance to this entrance pupil (i.e. with minimum aberrations for this distance). In a refracting astronomical telescope the entranc ...

See also:

Eyepiece, Eyepiece - Eyepiece properties, Eyepiece - Design distance to entrance pupil, Eyepiece - Elements, Eyepiece - Internal reflection and scatter, Eyepiece - Lateral chromatic aberration, Eyepiece - Focal length, Eyepiece - Location of focal plane, Eyepiece - Field of view, Eyepiece - Barrel diameter, Eyepiece - Eye relief, Eyepiece - Eyepiece designs, Eyepiece - Huygens, Eyepiece - Ramsden, Eyepiece - Kellner or achromatized Ramsden, Eyepiece - RKE, Eyepiece - Orthoscopic or orthographic, Eyepiece - Erfle, Eyepiece - Plössl

Read more here: » Eyepiece: Encyclopedia II - Eyepiece - Eyepiece properties

refracting telescope: Encyclopedia II - Light - Speed of light

Although some people speak of the "velocity of light", the word velocity should be reserved for vector quantities, that is, those with both magnitude and direction. The speed of light is a scalar quantity, having only magnitude and no direction, and therefore speed is the correct term. The speed of light has been measured many times, by many physicists. The best early measurement is Ole Rømer's (a Danish physicist), in 1676. By observing the motions of Jupiter and one of its moons, Io, with a telescope, and noting discr ...

See also:

Light, Light - Visible electromagnetic radiation, Light - Speed of light, Light - Refraction, Light - Optics, Light - Color and wavelengths, Light - Measurement of light, Light - Light sources, Light - Theories about light, Light - Early Greek ideas, Light - 10th century optical theory, Light - The 'plenum', Light - Particle theory, Light - Wave theory, Light - Electromagnetic theory, Light - Particle theory revisited, Light - Quantum theory, Light - Wave-particle duality, Light - A light wave

Read more here: » Light: Encyclopedia II - Light - Speed of light

refracting telescope: Encyclopedia II - Optical telescope - Angular resolution

Ignoring blurring of the image by turbulence in the atmosphere (atmospheric seeing) and optical imperfections of the telescope, the angular resolution of an optical telescope is determined by the width of the objective, termed its "aperture." The Rayleigh criterion for the resolution limit αR (in radians) is given by ...

See also:

Optical telescope, Optical telescope - How it works, Optical telescope - Angular resolution, Optical telescope - Focal length and f-ratio, Optical telescope - Light-gathering power, Optical telescope - Research telescopes

Read more here: » Optical telescope: Encyclopedia II - Optical telescope - Angular resolution

refracting telescope: Encyclopedia II - Optical telescope - Research telescopes

Nearly all large research-grade astronomical telescopes are reflectors. Some reasons are: In a lens the entire volume of material has to be free of imperfection and inhomogeneities, whereas in a mirror, only one surface has to be perfectly polished. Light of different colors travels through a medium other than vacuum at different speeds. This causes chromatic aberration. There are technical difficulties involved in manufacturing and manipulating large-aperture lenses. One of them is that all real materials sag ...

See also:

Optical telescope, Optical telescope - How it works, Optical telescope - Angular resolution, Optical telescope - Focal length and f-ratio, Optical telescope - Light-gathering power, Optical telescope - Research telescopes

Read more here: » Optical telescope: Encyclopedia II - Optical telescope - Research telescopes

refracting telescope: Encyclopedia II - Angular resolution - Telescope case

Point-like sources separated by an angle smaller than the angular resolution cannot be resolved. A single optical telescope has an angular resolution less than one arcsecond, but astronomical seeing and other atmospheric effects make attaining this very hard. The highest angular resolutions can be achieved by interferometry: the VLTI is intended to achieve an effective angular resolution of 0.001 arcsecond. The angular resolution of a telescope can usually be approximated by R = λ/D where λ is the wavelen ...

See also:

Angular resolution, Angular resolution - Definition of terms, Angular resolution - Explanation, Angular resolution - Telescope case, Angular resolution - Microscope case

Read more here: » Angular resolution: Encyclopedia II - Angular resolution - Telescope case

refracting telescope: Encyclopedia II - Light - Refraction

All light propagates at a finite speed. Even moving observers always measure the same value of c, the speed of light in vacuum, as c = 299,792,458 metres per second (186,282.397 miles per second). When light passes through a transparent substance, such as air, water or glass, its speed is reduced, and it undergoes refraction. The reduction of the speed of light in a denser material can be indicated by the refractive index, n, which is defined a ...

See also:

Light, Light - Visible electromagnetic radiation, Light - Speed of light, Light - Refraction, Light - Optics, Light - Color and wavelengths, Light - Measurement of light, Light - Light sources, Light - Theories about light, Light - Early Greek ideas, Light - 10th century optical theory, Light - The 'plenum', Light - Particle theory, Light - Wave theory, Light - Electromagnetic theory, Light - Particle theory revisited, Light - Quantum theory, Light - Wave-particle duality, Light - A light wave

Read more here: » Light: Encyclopedia II - Light - Refraction

refracting telescope: Encyclopedia II - Lens optics - Uses of lenses

One important use of lenses is as a prosthetic for the correction of visual impairments such as myopia, hyperopia, presbyopia, and astigmatism. See corrective lens, contact lens, eyeglasses. Another use is in imaging systems such as a monocular, binoculars, telescope, spotting scope, telescopic gun sight, theodolite, microscope, and camera (photographic lens). A single convex lens mounted in a frame ...

See also:

Lens optics, Lens optics - History, Lens optics - Lens construction, Lens optics - Imaging properties, Lens optics - Aberrations, Lens optics - Spherical aberration, Lens optics - Coma, Lens optics - Chromatic aberration, Lens optics - Multiple lenses, Lens optics - Uses of lenses

Read more here: » Lens optics: Encyclopedia II - Lens optics - Uses of lenses

refracting telescope: Encyclopedia II - Lens optics - Uses of lenses

One important use of lenses is as a prosthetic for the correction of visual impairments such as myopia, hyperopia, presbyopia, and astigmatism. See corrective lens, contact lens, eyeglasses. Large convex lenses have been used for hundreds of years to light fires by concentrating the rays of the sun. In this use they are commonly called a burning-glass. Such a lens does not need to be optically accurate to work satisfactorily. A modern variation of this is in combination with a Photovoltaic cell which can work at a higher efficiency when sunlight is ...

See also:

Lens optics, Lens optics - History, Lens optics - Lens construction, Lens optics - Imaging properties, Lens optics - Aberrations, Lens optics - Spherical aberration, Lens optics - Coma, Lens optics - Chromatic aberration, Lens optics - Multiple lenses, Lens optics - Uses of lenses

Read more here: » Lens optics: Encyclopedia II - Lens optics - Uses of lenses

refracting telescope: Encyclopedia II - Binoculars - Design details

Binoculars to be used to view objects which are not at a fixed distance must have a focussing arrangement. In some cases the two telescopes are focused independently by changing the distance between ocular and objective lenses. It is more convenient for the viewer to focus both tubes with one action (usually rotation of a central focussing wheel), and for one of the two eyepieces to be adjustable to compensate for differences between the viewer's eyes (usually by rotating the eyepiece in its mount). Once this adjustment has been made for a g ...

See also:

Binoculars, Binoculars - Prismatic binoculars, Binoculars - Design details, Binoculars - Optical parameters, Binoculars - Optical construction, Binoculars - Image stabilisation, Binoculars - Maintenance, Binoculars - Choosing binoculars

Read more here: » Binoculars: Encyclopedia II - Binoculars - Design details

refracting telescope: Encyclopedia II - Optician - Scientific equipment opticians

An optician is also an individual who makes and adjusts other optical aids, including telescope optics and microscope lenses. Optician - Telescope opticians. James Gilbert Baker John A. Brashear Alvan Clark John Dollond Charles Wesley Elmer and Richard Scott Perkin Frederick James Hargreaves Georg Simon Plšssl Russell W. Por ...

See also:

Optician, Optician - Eyecare opticians, Optician - Famous opticians, Optician - Scientific equipment opticians, Optician - Telescope opticians, Optician - Microscope opticians

Read more here: » Optician: Encyclopedia II - Optician - Scientific equipment opticians

refracting telescope: Encyclopedia II - Lens optics - Multiple lenses

Lenses may be combined to form more complex optical systems. The simplest case is when lenses are placed in contact: if the lenses of focal lengths f1 and f2 are "thin", the combined focal length F of the lenses can be calculated from: . Since 1/f is the power of a lens, it can be seen that the powers of thin lenses in contact are additive. If two thin lenses are separated by some distance d, the distance from the second lens to the focal point of the combined lenses is called the back focal length ...

See also:

Lens optics, Lens optics - History, Lens optics - Lens construction, Lens optics - Imaging properties, Lens optics - Aberrations, Lens optics - Spherical aberration, Lens optics - Coma, Lens optics - Chromatic aberration, Lens optics - Multiple lenses, Lens optics - Uses of lenses

Read more here: » Lens optics: Encyclopedia II - Lens optics - Multiple lenses

refracting telescope: Encyclopedia II - Astronomical seeing - Measures of Astronomical Seeing

There are three common descriptions of the astronomical seeing conditions at an observatory: The FWHM of the seeing disc r0 and t0 The CN2 profile These are described in the sub-sections below: Astronomical seeing - The FWHM of the seeing disc. Without an atmosphere, a small star would have an apparent size in a telescope image determined by diffraction and would be inversely proportional to the diameter of the telesco ...

See also:

Astronomical seeing, Astronomical seeing - The Effects of Astronomical Seeing, Astronomical seeing - Measures of Astronomical Seeing, Astronomical seeing - The FWHM of the seeing disc, Astronomical seeing - r0 and t0, Astronomical seeing - The CN2 profile, Astronomical seeing - Overcoming Atmospheric Seeing

Read more here: » Astronomical seeing: Encyclopedia II - Astronomical seeing - Measures of Astronomical Seeing

refracting telescope: Encyclopedia II - Aether drag hypothesis - Historical importance

The aether drag hypothesis is historically important because it was one of the reasons why Newton's corpuscular theory of light was replaced by the wave theory and it is used in early explanations of light propagation without relativity theory. It originated as a result of early attempts to measure the speed of light. In 1810 François Arago realised that variations in the refractive index of a substance predicted by the corpuscular theory would provide a useful method for measuring the velocity of light. These predictions arose becau ...

See also:

Aether drag hypothesis, Aether drag hypothesis - Historical importance, Aether drag hypothesis - Bibliography and References

Read more here: » Aether drag hypothesis: Encyclopedia II - Aether drag hypothesis - Historical importance

refracting telescope: Encyclopedia II - Fused quartz - Applications

Specially prepared fused silica is also the key starting material used to make optical fiber for telecommunications. Because of its strength and high melting point (compared to ordinary glass), fused silica is used as the envelope of halogen lamps, which must operate at a high envelope temperature to achieve their combination of high brightness and long life. The combination of strength, thermal stability, and UV transparency makes it an excellent substra ...

See also:

Fused quartz, Fused quartz - Chemistry, Fused quartz - Applications, Fused quartz - Physical Properties, Fused quartz - Properties of clear fused quartz

Read more here: » Fused quartz: Encyclopedia II - Fused quartz - Applications

refracting telescope: Encyclopedia II - Herbig-Haro object - Proper motions and variability

Spectroscopic observations of HH objects show that they are moving away from the source stars at speeds of 100 to 1000 km/s. In recent years, the high optical resolution of Hubble Space Telescope observations has revealed the proper motion of many HH objects in observations spaced several years apart. These observations have also allowed estimates of the distances of some HH objects via the expansion parallax method. As they move away from the parent star, HH objects evolve significantly, varying in brightness on timescales of a ...

See also:

Herbig-Haro object, Herbig-Haro object - Discovery and history of observations, Herbig-Haro object - Physical characteristics, Herbig-Haro object - Numbers and distribution, Herbig-Haro object - Proper motions and variability, Herbig-Haro object - Source stars

Read more here: » Herbig-Haro object: Encyclopedia II - Herbig-Haro object - Proper motions and variability

refracting telescope: Encyclopedia II - Glass - Glass as a liquid

One common misconception is that glass is a super-cooled liquid of practically infinite viscosity when at room temperature. Supporting evidence that is often offered is that old windows are often thicker at the bottom than at the top. It is then assumed that the glass was once uniform, but has flowed to its new shape. The likely source of this belief is that when panes of glass were commonly made by glassblowers, the technique that was used was to spin molten glass so as to create a round, mostly flat and even plate (the Crown ...

See also:

Glass, Glass - Properties and Uses, Glass - Glass Ingredients, Glass - Glass as a polymer, Glass - Colors, Glass - History of glass, Glass - Glass tools, Glass - Glass art, Glass - Architectural glass, Glass - Float annealed glass, Glass - Sheet glass, Glass - Plate glass, Glass - Cylinder glass, Glass - Insulated glazing, Glass - Toughened glass, Glass - Laminated glass, Glass - Low-emissivity glass, Glass - Self-cleaning glass, Glass - Evacuated glazing, Glass - Glass as a liquid

Read more here: » Glass: Encyclopedia II - Glass - Glass as a liquid

refracting telescope: Encyclopedia II - Red dot sight - Types of red dot sights

Some of the first red dot sights to appear were "occluded" sights; the image of the target was not visible through the sight. Looking into the sight with just one eye, the shooter saw only a red dot (often passively illuminated with ambient light gathered through fiber optics). With both eyes open, the image of the dot was superimposed by the brain onto the target. Nearly all currently available red dot sights use a curved partially reflective glass as a lens. This lens allows light from the target to pass through unobstructed, but collimates and reflects the light of the reticle back to the ...

See also:

Red dot sight, Red dot sight - How red dot sights work, Red dot sight - Reticles, Red dot sight - Types of red dot sights, Red dot sight - Uses

Read more here: » Red dot sight: Encyclopedia II - Red dot sight - Types of red dot sights

refracting telescope: Encyclopedia II - Light - Visible electromagnetic radiation

Visible light is the portion of the electromagnetic spectrum between the frequencies of 380 THz (3.8×1014 hertz) and 750 THz (7.5×1014 hertz). The speed (c), frequency (f or ν), and wavelength (λ) of a wave obey the relation: Because the speed of light in a vacuum is fixed, visible light can als ...

See also:

Light, Light - Visible electromagnetic radiation, Light - Speed of light, Light - Refraction, Light - Optics, Light - Color and wavelengths, Light - Measurement of light, Light - Light sources, Light - Theories about light, Light - Early Greek ideas, Light - 10th century optical theory, Light - The 'plenum', Light - Particle theory, Light - Wave theory, Light - Electromagnetic theory, Light - Particle theory revisited, Light - Quantum theory, Light - Wave-particle duality, Light - A light wave

Read more here: » Light: Encyclopedia II - Light - Visible electromagnetic radiation

refracting telescope: Encyclopedia II - Light - Measurement of light

The following quantities and units are used to measure the quantity or "brightness" of light. edit edit Sometimes confusingly called "intensity". Sometimes confusingly called "intensity". Sometimes confusingly called "intensity". watt per steradian per squ ...

See also:

Light, Light - Visible electromagnetic radiation, Light - Speed of light, Light - Refraction, Light - Optics, Light - Color and wavelengths, Light - Measurement of light, Light - Light sources, Light - Theories about light, Light - Early Greek ideas, Light - 10th century optical theory, Light - The 'plenum', Light - Particle theory, Light - Wave theory, Light - Electromagnetic theory, Light - Particle theory revisited, Light - Quantum theory, Light - Wave-particle duality, Light - A light wave

Read more here: » Light: Encyclopedia II - Light - Measurement of light




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