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Published byMargaret Cox Modified over 9 years ago
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Telescopes 3 Functions 1. Gather light Size does matter The bigger, the better 2. Resolve detail 3. Magnification Only important for solar system objects
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Refracting Telescopes Cheap Good for bright objects Basic design
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Reflecting Telescopes Larger Size = Price Fainter objects
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Catadioptric Telescopes “Combination” Shorter Reasonable price Common forms – Schmidt-Cassegrain (SCT) Maksutov-Cassegrain (Mak)
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Telescope Mounts Alt-Az Mounts – Simple – Complex tracking – Fields rotate Equatorial Mounts – Latitude dependent – Tracks easily – No rotation (good for long exposures)
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Telescope Details Aperture = size of light gathering opening = D Focal length = distance needed to focus light For the objective (the mirror/body of scope) = f o For the eye piece = f e Magnification = f o /f e Resolution, R = 12.0cm/D (result given in ′′) For Catadioptric systems, objective is modified by correction plate.
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Taking Pictures Film – 400 speed (ISO) Digital – READ THE MANUAL – Long exposure times - stars, constellations – Short exposure times – Moon, planets – Brightness control, focus control, contrast control Bracket!
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Camera Only Constellations Milky Way Meteor showers Aurorae Long time = star trails – No trails: t = 30s – 1 m Hazard: Fogging Hazard: The Moon
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Prime Focus Moon details (short exposure) Telescopic objects (long exposure) Digital – can “stack” multiple exposures Magnification required for planetary detail Adapter needed – “t-mount”
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30 second exp. 1600 ISO 11 exposures Stacked
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Piggy Back Wide field, faint objects
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Afocal Steady mount required
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Video Regular video cams Webcams Security Cams Speciality cameras With t-mount or afocal Software – stack images
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