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Basic Optical Devices
Basic Optical Devices

... •Used to gather light & focus it into a real focus, •Creates an erect virtual and larger image of an object placed closer than its focus •Create inverted real image Of an object placed farther away than the focus These images get smaller the farther away the object is •Concave mirrors are often used ...
Lecture 22 - Louisiana State University
Lecture 22 - Louisiana State University

... Maximum magnification: m~2cm/25cm (!?) We’d like to make p smaller (move the object closer). We use a magnifying lens to produce a (larger) image than our eye can see: Very near the focus! ...
Electromagnetic Spectrum Ppt
Electromagnetic Spectrum Ppt

... • HOWEVER, TELESCOPES IN SPACE CAN COLLECT ENERGY AT ALL WAVELENGTHS! ...
f - LSU Physics
f - LSU Physics

PowerPoint - College of Engineering, Forestry, and Natural Sciences
PowerPoint - College of Engineering, Forestry, and Natural Sciences

... mirror. Using the distance to the mirror being aligned, the distance that the mirror is misaligned can be calculated in millimeters. ...
Future and Status of CANGAROO(Japan - side)
Future and Status of CANGAROO(Japan - side)

... 90% concentration @0.1degree ...
Science Explorer
Science Explorer

... Patterns of stars in the sky are called constellations. Stars in a constellation can look as if they are close together, even though they are at very different distances from Earth. For example, the star at the end of the handle in the Big Dipper is about twice as far from Earth as most of the other ...
Wide-Field Optical Spectrometer (WFOS)
Wide-Field Optical Spectrometer (WFOS)

3-1. True or False: Different colors of light are waves with different
3-1. True or False: Different colors of light are waves with different

International Conference on Adaptive Optics for
International Conference on Adaptive Optics for

... technology of the AO systems. The organization of the third meeting came in the wake of recognition of the excellent work performed by INAF and the Arcetri Observatory in the field of AO, in particular for the FLAO (First Light Adaptive Optics) mounted on the Large Binocular Telscope (LBT) and in us ...
Two Looks at the Visual and Imaging Perfomance of the VISAC
Two Looks at the Visual and Imaging Perfomance of the VISAC

... pinion model mounted behind the priIn a way, the VISAC optical tube behaves mary, which remains stationary. Most like a dew shield in itself with its primary Schmidt-Cassegrains suffer from mirror mirror safely tucked at the bottom of the shift, to one degree or another. Companies open optical tube. ...
Picture 1 present an negative image of sky taken by ccd camera
Picture 1 present an negative image of sky taken by ccd camera

Lab 2 Procedures
Lab 2 Procedures

... can be used to define an optical axis chosen by mechanical features of a mounting schematic and how to align optics to that axis. All optical elements with spherical surfaces can be aligned to a common axis, regardless of lens wedge. ...
Optics student outline
Optics student outline

... ii. Use SPOT (size, position, orientation, type) to describe image properties. (190) b. Concave Mirrors (inside of metal spoon) (197-203) i. Define focal point, focal length and the principle axis. ii. Lab (core) – Locate focal point of a concave mirror. iii. Construct ray diagrams to describe the i ...
Cosmic Times 1955, 65 PPT
Cosmic Times 1955, 65 PPT

... Reflecting telescopes Advantages Easy to use and construct Excellent for faint deep sky objects (galaxies, nebulae and star clusters) Few optical irregularities, deliver very bright images Reasonably compact and portable Costs less per inch of aperture compared to refractors (mirrors cheaper than l ...
Albireo (β Cygni) is a star system marking the beak of Cygnus, the
Albireo (β Cygni) is a star system marking the beak of Cygnus, the

Light and Other Forms of Radiation
Light and Other Forms of Radiation

... – In a “solid” body the close packing of the atoms means than the electron orbits are complicated, and virtually all energy orbits are allowed. So all wavelengths of light can be emitted or absorbed. A black material is one which readily absorbs all wavelengths of light. These turn out to be the sam ...
High-Resolution Optical Spectrometer (HROS)
High-Resolution Optical Spectrometer (HROS)

Broad Sheet 7 - Museum of the History of Science
Broad Sheet 7 - Museum of the History of Science

Telescope Basics - UChicago Voices
Telescope Basics - UChicago Voices

Telescope Design The Keck II Telescope
Telescope Design The Keck II Telescope

... The Keck Telescope Space Craft SCIENCE Kit. [Online] Available: http://scikits.com/Keck.html The Keck Telescope. [Online] Available: //www.ngst.nasa.gov/science/meetings/Keck.html An Introduction to Interferometry. [Online] Available: ...
Advanced Technologies for Future Space Telescopes and Instruments
Advanced Technologies for Future Space Telescopes and Instruments

... to detect and characterize Earth-like planets around nearby star (i.e. how unique is the Earth as a planet?) to search for exo-life around nearby stars (i.e how unique is life in the ...
PARTS LIST FOR AT50 Telescope
PARTS LIST FOR AT50 Telescope

LAB 4: THE SIMPLE MAGNIFIER EYEPIECES The Simple Magnifier:
LAB 4: THE SIMPLE MAGNIFIER EYEPIECES The Simple Magnifier:

Chapter 35
Chapter 35

... To understand the two types of lenses - convex and concave. To understand how to use ray tracing to find the location and types of images for both kinds of lenses. To understand how to use the Lens Maker's equation to find the focal lengths of a lens: ...
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Optical telescope



An optical telescope is a telescope that gathers and focuses light, mainly from the visible part of the electromagnetic spectrum, to create a magnified image for direct view, or to make a photograph, or to collect data through electronic image sensors.There are three primary types of optical telescope: refractors, which use lenses (dioptrics) reflectors, which use mirrors (catoptrics) catadioptric telescopes, which combine lenses and mirrorsA telescope's light gathering power and ability to resolve small detail is directly related to the diameter (or aperture) of its objective (the primary lens or mirror that collects and focuses the light). The larger the objective, the more light the telescope collects and the finer detail it resolves.People use telescopes and binoculars for activities such as observational astronomy, ornithology, pilotage and reconnaissance, and watching sports or performance arts.
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