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The daily motion of the Sun across the sky is familiar to even the most casual observer.  This daily trek is not the 
Sun moving as early astronomers thought, but the result of the Earth's rotation.  The Earth's rotation also causes the 
stars to do the same, scribing out a large circle as the Earth completes one rotation.  The size of the circular path a 
star follows depends on where it is in the sky.  Stars near the celestial equator form the largest circles rising in the 
east and setting in the west.  Moving toward the north celestial pole, the point around which the stars in the northern 
hemisphere appear to rotate, these circles become smaller.  Stars in the mid-celestial latitudes rise in the northeast 
and set in the northwest.  Stars at high celestial latitudes are always above the horizon, and are said to be 
circumpolar because they never rise and never set.  You will never see the stars complete one circle because the 
sunlight during the day washes out the starlight.  However, part of this circular motion of stars in this region of the 
sky can be seen by setting up a camera on a tripod and opening the shutter for a couple hours.  The timed exposure 
will reveal semicircles that revolve around the pole.  (This description of stellar motions also applies to the southern 
hemisphere except all stars south of the celestial equator move around the south celestial pole.) 

Figure 4-2 

All stars appear to rotate around the celestial poles.  However, the appearance of 
this motion varies depending on where you are looking in the sky.  Near the north 
celestial pole the stars scribe out recognizable circles centered on the pole (1). 
Stars near the celestial equator also follow circular paths around the pole.  But, the 
complete path is interrupted by the horizon.  These appear to rise in the east and 
set in the west (2).  Looking toward the opposite pole, stars curve or arc in the 
opposite direction scribing a circle around the opposite pole (3).  

Starts seen near the north celestial 
pole 

Starts seen near the celestial 
equator 

Starts seen looking in the opposite 
direction of the north celestial pole 

Содержание FirstScope 21024

Страница 1: ...F Fi ir rs st tS Sc co op pe e I In ns st tr ru uc ct ti io on n M Ma an nu ua al l M Mo od de el l 2 21 10 02 24 4...

Страница 2: ...General Observing Hints 7 The Celestial Coordinate System 8 Motion of the Stars 9 CELESTIAL OBSERVING 10 Observing the Moon 10 Lunar Observing Hints 10 Observing the Planets 10 Observing Deep Sky Obje...

Страница 3: ...and easy set up Take time to read through this manual before embarking on your journey through the Universe It may take a few observing sessions to become familiar with your telescope so you should ke...

Страница 4: ...4 Figure 1 1 1 Focuser 6 Arm 2 Secondary Diagonal Mirror inside 7 Tube End 3 Optical Tube 8 Primary Mirror inside 4 Lock Nut 9 Focus Knob 5 Base 10 Eyepiece 10 9 8 7 6 5 4 3 2 1...

Страница 5: ...er see the section on Calculating Magnification The eyepiece fits directly into the focuser To attach the eyepieces 1 Make sure the thumbscrews are not protruding into the focuser tube Then insert the...

Страница 6: ...ll enjoy a telescope that is relatively compact and portable A Newtonian Reflector telescope offers such impressive light gathering characteristics you can take a serious interest in deep space astron...

Страница 7: ...t you are observing To calculate the actual field of view divide the apparent field of the eyepiece supplied by the eyepiece manufacturer by the magnification In equation format the formula looks like...

Страница 8: ...rth and separates the northern celestial hemisphere from the southern Like the Earth s equator it bears a reading of zero degrees On Earth this would be latitude However in the sky this is referred to...

Страница 9: ...use the sunlight during the day washes out the starlight However part of this circular motion of stars in this region of the sky can be seen by setting up a camera on a tripod and opening the shutter...

Страница 10: ...see the moons of Jupiter as they orbit the giant planet Saturn with its beautiful rings is easily visible at moderate power Planetary Observing Hints y Remember that atmospheric conditions are usually...

Страница 11: ...than you can with the naked eye y Binoculars a helpful tool in locating bright stars and searching an area you are looking for objects in Can be a substitute or supplement to a finderscope y Books sev...

Страница 12: ...necting the two stars 6 Look through the telescope and the Ring Nebula should be in your field of view The Ring Nebula s angular size is quite small and difficult to see 7 Because the Ring Nebula is r...

Страница 13: ...ound around major urban areas LPR filters enhance deep sky viewing from light polluted areas by blocking unwanted light while transmitting light from certain deep sky objects You can on the other hand...

Страница 14: ...ted If moisture condenses on the inside of the optics remove the accessories from the telescope Place the telescope in a dust free environment and point it down This will remove the moisture from the...

Страница 15: ...osed on the primary mirror Figure 6 2 If the primary mirror is not centered in the secondary mirror adjust the secondary mirror screws by alternately tightening and loosening them until the mirror is...

Страница 16: ...Length 300mm Focal Ratio f 4 Optical Coatings Coated Eyepieces 1 25 Barrel 20mm 15x 4mm 75x Apparent FOV 20mm 25 and 4mm 33 Angular Field of View w 20mm eyepiece 1 7 Linear FOV w 20mm ft 1000yds m 10...

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