Term
| ELECTROMAGNETIC RADIATION |
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Definition
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LIGHT IS MADE UP OF BOTH ELECTRIC AND MAGNETIC FIELDS.
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THE DISTANCE BETWEEN PEAKS
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TOO AWKWARD TO MEASURE SUCH SHORT DISTANCES IN MILLIMETERS, SO PHYSICISTS AND ASTRONOMERS DESCRIE THE WAVELENGTH OF LIGHT USING EITHER THE UNIT OF __
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Definition
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TOO ASKWARD TO MEASURE SUCH SHORT DISTANCES IN MILLIMETERS, SO PHYSICITS AND ASTRONOMERS DESCRIBE THE WAVELENGTH OF LIGHT USING EITHER THE UNIT OF BILLIONTH OF AMETER (10-9 M)___WHICH IS NAME AFTER THE SWEDISH ASTROMERS ANDERS ANGSTROM
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RADIATION, WITH WAVELENGTHS RANGING FROM 700 nm TO ABOUT 1 mm
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ELECTROMAGNETIC WAES WITH WAVELENGTHS SHORTER THAN VIOLET LIGHT ARE CALLED
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SHORTER-WAVELENGTH ELECTROMAGNETIC WAVES THAN UV ARE CALLED
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ARE THE SHORTEST WAVELENGTH ELECTROMAGNETIC WAVES THAN UV ARE CALLED
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A MINIMUM SIZED BUNDLED OF ELECTROMAGNETI WAVES. A PARTICLE OF LIGHT IS CALLED
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ONLY VISIBLE LIGHT, SOME SHORT-WAVELENGTH INFRARED RADIATION, AND SOME RADIO WAVES REACH EARTH'S SURFACE THROUGH WHAT ARE CALLED
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Definition
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A TELESCOPE TO FOCUS LIGHT BY USING A LENS TO GATHER AND FOCUS THE LIGHT
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Definition
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TELESCOPE USE TO FOCUS LIGHT USING A MIRROR
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Definition
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THE MAIN LENS INA REFRACTING TELESCOPE
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Definition
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THE MAIN MIRROR IN A REFLECTING TELESCOPE
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BOTH KINDS OF TELESCOPES FORM A SMALL, INVERTED IMAGE THAT IS DIFFICULT TO OBERSERVE DIRECTLY, SO A LENS CALLED THE ____ IS USED TO MAGNIFY THE IMAGE AND MAKE IT CONVENIENT TO VIEW.
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IS THE DISTANCE FROM A LENS OR MIRROR TO THE IMAGE IT FORMS OF A DISTANT LIGHT SOURCE SUCH AS A STAR.
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TELESCOPES HAVE SERIOUS DISADVANTAGES. MOST SUFFER FROM AN OPTICAL DISTORTION THAT LIMISTS THEIR USEFULNESS. WHEN LIGHT IS REFRACTED THROUGH GLASS, SHORTER WAVELENGTHS BEND MORE THAN LONGER WAVELENGTHS. AS A RESULT YOU SEE A COLOR BLUR AROUND EVERY IMAGE. THIS COLOR SEPARATION IS CALLE ___
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TELESCOPE TO GATHER VISIBLE LIGHT
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TELECOPE TO GATHER RADIO RADIATION.
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REFERS TO THE ABILITY OF A TELESCOPE TO COLLECT LIGHT.
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Definition
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REFERS TO THE ABILITY OF THE TELESCOPE TO REVEAL FINE DETAIL
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ONE CONSEQUENCE OF THE WAVELIKE NATURE OF LIGHT IS THAT THERE IS AN INEVITABLE SMALL BLURRING CALLED A ___AORUND EVERY POINT OF LIGHT IN THE IMAGE, AND YOU CAN'T SEE ANY DETAIL SMALLER
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ONE WAY TO IMPROVE RESOLVING POWER IS TO CONNECT TWO OR MORE TELESCOPES IN AN ___WHICH HAS A RESOLVING POWER EQUAL TO THAT OF A TELESCOPE AS LARGE AS THE MAXIUM SEPARATION BETWEEN THE INDIVIDUAL TELESCOPES
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IN ADDITION, WHEN YOU LOOK THROUGH A TELESCOPE, YOU LOOK THROUGH MILES OF TURBULENCE IN EARTH'S ATMOSPHERE, WHICH MAKES IMAGES DANCE AND BLUR, A CONDITION THA ASTRONOMERS CALL
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A SITUATION CAN BE IMPROVED BY A DIFFICULT AND EXPENSIVE TECHNIQUE CALLED ____IN WHICH RAPID COMPUTER CALCULATIONS ADJUST THE TELESCOPE OPTICS AND PARTLY COMPENSATE FOR SEEING DISTORTIONS.
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THE LEAST IMPORTANT POWER OF A TELESCOPE IS ____THE ABILITY TO MAKE AN IMAGE LARGE
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optical astronomers avoid cities because ____the brightening of the night sky by light scattered from artifical outdoor lighting,can make it impossible to see faint objects
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Term
| SIDEREAL TRACKING
(SIDEREAL, REFERS TO THE STARS) |
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Definition
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TELESCOPES LOCATED ON THE SURFACE OF EARTH, WHETHER OPTICAL OR RADIO, MUS MOVE CONTINUOUSTLY TO STAY POINTED AT A CELESTIAL OBJECT AS EARTH TURNS ON ITS AXIS. THIS IS CALLED
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Definition
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WS THE FIRST IMAGE RECORDING DECISE USED WITH TELESCOPES.
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Term
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SENSITIVE LIGHT METERS TO MEASURE THE BRIGHTNESS OF INDIVIDUAL OBJECTS VERY PRECISELY.
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Term
| CHARGE COUPLED DEVICES (CCDs) |
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Definition
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MOST MODERN ASTRONOMERS USE THIS AS BOTH IMAGE RECORDING DEVICES AND PHOTOMETERS
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CAN BE USED LIKE A SMALL PHOTOGRAPHIC PLATE, BUT THEY HAVE DRAMATIC ADVANTAGES OVER BOTH PHOTOMETERS AND PHOTOGRAPHIC PLATES.
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Definition
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MEANING, CONVERTED TO NUMERICAL DATA, AND CAN BE READ DIRECTLY INTO A COMPUTER MEMORY FOR LATER ANALYSIS.
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ASTRONOMERS ALSO MANIPULATE IMAGES TO PRODUCE ____IN WHICH COLORS REPRESNT DIFFERENT LEVES OF INTENSITY AN ARE NOT RELATED TO THE TRUE COLORS OF THE OBJECT
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TO ANALYZE LIGHT IN DETAIL, YOU NEED TO SPREAD THE LIGHT OUT ACCORDING TO WAVELENGTH INTO A SPECTRUM, A TASK PERFORMED BY A ___
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VIOLET (SHORT WAVELENGTH) LIGHT BENDS MOST, ANDRED (LONG WAVELENGTH) LIGHT LEAST. thURS, THE WHITE LIGHT ENTERING THE PRISM IS SPREAD INTO WHAT IS CALLED
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IS A PIECE OF GLASS WITH THOUSANDS OF MICROSCOPIC PARALLEL LINES SCRIBED ONTO ITS SURFACE
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CAN REFLECT THE LIGHT THROUGH A HOLE IN THE PRIMARY MIRROR TO A CASSEGRAIN FOCUS
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IN LARGER TELESCOPES THE LIGHT CAN BE FOCUSED TO A ____POSITION HIGH IN THE TELESCOPE TUBE. ALTHOUGH, IT IS A GOOD PLACE TO IMAGE FAINT OBJECTS, THE PRIME FOCUS IN INCONVENIENT FOR LARGE INSTRUMENTS.
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THIS FOCAL ARRANGEMENT MY BE THE MOST COMMON FORM OF ASTRONOMICAL TELESCOPE. IT IS CONVENIENT AND HAS ROOM FOR LARGE INSTRUMENTS
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SMALLER TELESCOPES CAN USE OTHER FOCAL ARRANGMENTS. THE ____THAT ISAAC NEWTON USED IN HIS FIRST REFLECTING TELESCOPE IS AWKWARD FOR LARGE TELESCOPES
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MANY SMALL TELESCOPES SUCH AS THIS ONE HAS A THIN CORRECTING PLACE IMPROVING THE IMAGE BUT IS TOO SLIGHTLY CURVED TO INTRODUCED SERIUOS CHROMATIC ABERRATION
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