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Solar Physics, Space Weather, and Wide-field X-ray
Solar Physics, Space Weather, and Wide-field X-ray

PDF - Subaru Telescope
PDF - Subaru Telescope

...  IRD aims at detecting ~50 planets around nearby M dwarfs, including 10 Earth-like planets in habitable zone  IRD will survey ~ 100 late M-dwarfs for 5 years and SSP is ...
The Super Space Telescope
The Super Space Telescope

... 5. Circle all the numbers . Which is the biggest? Which is the smallest? Which measures a distance? Which is a dollar amount? Which is a measure of time? 6. Find the following words : telescope, concentrate, orbit, secondary, cargo, target, blurred, galaxy, deploy, primary, atmosphere, commands. Def ...
Boy Scout Astronomy Merit Badge Workbook
Boy Scout Astronomy Merit Badge Workbook

... observe the moon each day. On the first day, sketch the relative position of the moon across the southern horizon noting its height and shape (phase). Draw some landmarks on the sketch as points of reference. On the same drawing, repeat this at the same time each day for the next three days, showing ...
the cleaning of optical surfaces: mirrors
the cleaning of optical surfaces: mirrors

... primary mirror for the typical consumer and end-user; thus cleaning will likely take place less often than it would if the mirror were smaller or easy to remove from the optical tube assembly. Remember the Number One Rule on Optics Cleaning: "Don't...unless you absolutely have to." ...
A Telescope Operating Manual
A Telescope Operating Manual

... This booklet is a handbook for the use of the lab telescopes. In it you should find all the information necessary to become an expert in operating the lab telescopes. Read it more than once and review it each week before lab. Bring copies of any useful pages to lab until you are comfortable working ...
Equipment Identification PowerPoint
Equipment Identification PowerPoint

... other uses. There is a misconception that the inventor is Robert Wilhelm Bunsen but it is only named after him, whose laboratory assistant, Peter Desdega, in 1855 perfected an earlier design by Michael Faraday. The device safely burns a continuous stream of gas without the risk that the flame will t ...
Slide 1
Slide 1

... about parent axis Rotate segment about this axis under the optical test and separate effects that move with the mirror from those that remain with the test. ...
PDF
PDF

... An important element of NASA’s strategic plan is the search for and characterization of exoplanets, particularly terrestrial planets within the habitable zone of their parent star. A discovery of an Earthlike planet, with atmospheric constituents indicative of life, would revolutionize planetary sci ...
Light and Optical Systems - mrs
Light and Optical Systems - mrs

... What kind of lens, be it in a contact lens or eyeglasses, can fix this problem so that the image is correctly focused on the retina? ___________________________________________________________ ...
Simbol-X: x-ray baffle for stray–light reduction. - IASF Palermo
Simbol-X: x-ray baffle for stray–light reduction. - IASF Palermo

Optical Interferometers
Optical Interferometers

... interferometer arms is equal to the integer number of wavelengths ∆l = mλ, and destructive interference corresponds to the half-integer number of wavelengths ∆l = (m + 1/2)λ (here m is an integer number). Since the wavelength of light is small (600 − 700 nm for a red laser), Michelson interferometer ...
DOBSONIAN TELESCOPE
DOBSONIAN TELESCOPE

pilot_projSOW_long - New Mexico Institute of Mining and
pilot_projSOW_long - New Mexico Institute of Mining and

... the inversion of lightcurve signatures (Drummond et al. 1988). Although the extension of this inversion process to the more complex shapes of smaller asteroids and artificial satellites provides additional challenges, especially when the target’s shape has non-convex features, techniques are being d ...
UItraLITE Glass/Composite Hybrid Mirror
UItraLITE Glass/Composite Hybrid Mirror

... The mass of the primary mirror has dominated the mass of larger aperture (> 1 m class) telescopes. Spaceborne telescopes have much to gain from a significant reduction in areal density. Areal density is often limited by the stiffness to weight ratio of the primary mirror. Two key factors drive this ...
ppt - SLAC
ppt - SLAC

... of Declination • Far North: 75° < d < 90° • North: 0° < d < 75° • Equatorial South: –40° < d < 0° • Far South: –90° < d < –40° • Galactic plane (–10° < b < 10°) excluded ...
VHE BL Lacs through the MAGIC glasses
VHE BL Lacs through the MAGIC glasses

6 OPTICS
6 OPTICS

... the instrument, to optimize the design of the collimator for a wide-field, multi-object, seeinglimited spectrograph (see Section 13.6). In addition, unlike in a Cassegrain configuration, a flat field screen may be deployed at the exit pupil of the telescope at a position below the secondary mirror w ...
The Spitzer Space Telescope
The Spitzer Space Telescope

...  Atmosphere is opaque at infrared wavelengths ...
Solar System Star The Milky Way Galaxy The Universe
Solar System Star The Milky Way Galaxy The Universe

... Source: http://www.wordcentral.com/cgi-bin/student?book=Student&va=black%20hole, http://en.wikipedia.org/wiki/Black_hole, http://www.bing.com/images/search?q=milky+way+black+hole&view=detail&id=F8BAB79ECCD41913EB89A3ACA8D3BEB0C17ED541&first=0, & http://www.bing.com/images/search?q=milky+way+black+ho ...
Lab: Telescopic Observations of the Moon and Outer Planets
Lab: Telescopic Observations of the Moon and Outer Planets

... large black knobs attached to cables which enable you to turn the telescope on these axes more slowly and with more control. These are the fine-adjust knobs. They are used when you have the telescope close to, but not at, the position you want it to be. These knobs are used, for example, to help ce ...
Document
Document

... novel energy discrimination approaches, and low noise superconducting electronics are applicable areas. Future space observatories in the 40 micron to 1 mm spectral regime will be cooled to even lower temperatures, frequently < 10 K, greatly reducing background noise from the telescope. In order to ...
Autostar Manual
Autostar Manual

... -6Figure 1 shows the complete Autostar menu structure showing the paths that can be followed. From any point in the menu, pressing ENTER moves along a menu line to the right. Pressing MODE moves to the left along a menu line. Pressing the down SCROLL key moves down menu lists and pressing the up SC ...
as a PDF
as a PDF

Michelson Interferometer
Michelson Interferometer

... Half of the light from source S falling on plate B is reflected towards M1 and other half is transmitted towards mirror M2. The two rays coming from M1& M2 interfere and fringes are formed. The wave reflected from M1 crosses the plate B twice before entering the eyepiece twice while the other wave f ...
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Very Large Telescope



The Very Large Telescope (VLT) is a telescope operated by the European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT consists of four individual telescopes, each with a primary mirror 8.2 m across, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language. The telescopes form an array which is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture.The VLT operates at visible and infrared wavelengths. Each individual telescope can detect objects roughly four billion times fainter than can be detected with the naked eye, and when all the telescopes are combined, the facility can achieve an angular resolution of about 0.001 arc-second (This is equivalent to roughly 2 meters resolution at the distance of the Moon).In single telescope mode of operation angular resolution is about 0.05 arc-second.The VLT is the most productive ground-based facility for astronomy, with only the Hubble Space Telescope generating more scientific papers among facilities operating at visible wavelengths. Among the pioneering observations carried out using the VLT are the first direct image of an exoplanet, the tracking of individual stars moving around the supermassive black hole at the centre of the Milky Way, and observations of the afterglow of the furthest known gamma-ray burst.
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