Dayton PHY 250 - How Information is Gathered

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Slide 1Slide 2Slide 3Slide 4Slide 5Slide 6Slide 7Slide 8Slide 9Slide 10Slide 11Slide 12Slide 13Slide 14Slide 15Slide 16MethodsEye (visible window)Camera – filmCamera – CCD (Digital)Collecting Electromagnetic InformationEye (visible window)Advantages:Everyone wants to see objects directlyDisadvantages:Light gathering capability – can see without telescope down to magnitude 6Image cannot be storedCannot do a time exposureCollecting Electromagnetic InformationCamera – filmAdvantages:* Inexpensive* Can do a time exposureDisadvantage: * Resolution* Cannot be conveniently manipulated* Deterioration* Long Exposure TimesCollecting Electromagnetic InformationCamera – CCD (Digital)Advantages:ResolutionCan do a time exposureCan store directly to a computerCan be manipulatedShort Exposure TimesDisadvantagesExpensePixilated ImageCollecting Electromagnetic InformationCollecting Electromagnetic Information – Digital ProcessingRaw Image MaskProcessed Image of a cometRaw Image Processed ImageComparison – Film vs CCDThe Advantages of CCD ImagingProfessional astronomers have been using CCDs for nearly two decades and have no thoughts about going back to film. The advantages are impressive:* CCD cameras are up to 100 times more sensitive than film * CCD images are digital, meaning no film-processing, scanning, scratching, or fading * CCD cameras have a much greater dynamic range than film, meaning they can more easily capture both faint and bright detail in a single exposure * CCDs are capable of resolving finer detail than film (this can, however, be limited by the telescope used and the atmospheric conditions) For the amateur, several other advantages apply as well:* Taking images with a CCD is generally much easier than with film * Learning goes faster due to the ease-of-use and shorter exposure times * Light pollution is less obtrusive and more easily removed from CCD images, meaning imaging from a backyard site is more likely to be possible with CCDComparison – Film vs CCDEfficiency and ExposureEfficiency* A CCD can record as much as 90% of the incident photons* Film will record less than 5% of the incident photonsCCD will record object 10 to 20 times fainter than film with the same exposure timeExposure Times* CCD can record the same image with less than one tenth of the exposure time for filmAbove: On the left is a CCD image taken from a suburban location. The exposure time is about 30 minutes. On the right is a film image of the same object taken using a similar telescope. The exposure time is over 2 hours and the level of detail is far less than the CCD image. At full resolution the difference is even more impressive.Comparison – Film vs CCDExposureAbove: A comparison of the size of a 35mm film negative with a relatively large amateur CCD chip (Kodak's KAF-3202 used in the SBIG ST-10 camera).Comparison – Film vs CCDFormatThe Advantages of FilmThe single biggest advantage of film (at present) is format. A 35mm film frame is 35mm x 26mm in size. Amateur CCD chips are typically less than 15mm across. This means that, on a given telescope, more of the sky can be captured at once with film. This is an advantage since many deep-sky objects are very large in apparent size. However, CCD chips as big as (or even bigger than) 35mm film are becoming available to advanced amateurs. It is only a matter of time before these are available at a price within reach of the average amateur.Figure 1. Replica (via a high quality microscope) of a test pattern recorded on 35mm Fuji Provia film using prime lens optics at f11. The highest resolved grid is indicated by the arrow (at column 1, row 3). It has 75 line pairs per mm, or about 2700 line pairs across the 35mm film. The contrast is about 10% (vs. 100% for pure black to pure white). In the row 0 column 2 pattern the contrast is about 50% or 5 times greater. Figure 3. Magnification of the central part of the Cool Pix 5000 5.2 megapixel digital camera resolution image. Item col 0, row 3 (i.e. 0/3) is resolved (IMHO, in the same sense as the film doing 1/3). However, note the LACK OF GRAIN NOISE in the digital picture (compare with figure 1). Clean grain-free digital images are an advantage that helps make prints than would normally be associated with film at a given resolution.Comparison – Film vs CCDResolutionA CCD camera with the format and resolution of a piece of 35mm film costs much more than a film astrophotography setup. However, most people are willing to sacrifice format for the speed and convenience of a CCD camera. Unless large prints are going to be made, CCDs can otherwise outperform film in almost every aspect. These days most people simply view images on a computer monitor, email images to friends, or post pictures on websites; for these purposes, small images are sufficient.For the amateur whose goal is to take pretty pictures of the night sky, a high-quality, entry-level CCD offers many advantages at a cost very comparable to film imaging. A quick look at the websites of the most prominent astrophotographers in the world will show that they have invested as much in film as most CCD users have invested in their setups. It will also show that most astrophotographers have begun shooting CCD images as well!Comparison – Film vs CCDPricePhotometer – An instrument which measure the brightness of an objectWill measure the TOTAL brightness of an object, which might be difficult to interpret. However, when combined with filters, can be used to measure the amount of light produced over a narrow range of frequencies. This can be compared with standard Blackbody radiation curves to determine the temperature of the objectPhotometryPhotometer – An instrument which measure the brightness of an objectWill measure the TOTAL brightness of an object, which might be difficult to interpret. However, when combined with filters, can be used to measure the amount of light produced over a narrow range of frequencies. This can be compared with standard Blackbody radiation curves to determine the temperature of the objectPhotometryXIntensityWavelengthPhotometer – An instrument which measure the brightness of an objectWill measure the TOTAL brightness of an object, which might be difficult to interpret. However, when combined with filters, can be used to measure the amount of light produced over a narrow range of frequencies. This can be compared with standard Blackbody radiation curves to


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Dayton PHY 250 - How Information is Gathered

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