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Ok, so magnificiation is focal length of the telescope divided by the width
of the eyepiece. What about when there is no eyepiece? My refractor has some magnification without one, but I have no clue what it is. |
#2
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Cerdic wrote:
Ok, so magnificiation is focal length of the telescope divided by the width of the eyepiece. Magnification = Telescopes F.L. / Eyepiece F.L. |
#3
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On 2006-01-18, Cerdic wrote:
Ok, so magnificiation is focal length of the telescope divided by the width of the eyepiece. What about when there is no eyepiece? My refractor has some magnification without one, but I have no clue what it is. The telescope makes a real image that you can see with the unaided eye - an "aerial image". The magnification is the focal length of the telescope divided by the distance from your eye to the aerial image. -- The night is just the shadow of the Earth. |
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Cerdic wrote:
Ok, so magnificiation is focal length of the telescope divided by the width of the eyepiece. NOT the width of the eyepiece, but its focal length |
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NOT the width of the eyepiece, but its focal length
Right. All this stuff that now seems obvious to some of us can be very hard for the newcomer to grasp. I have a co-worker that has a new telescope and is asking me for advice. He's wants to know what eyepiece to buy so he can "see farther". I've tried to explain how magnification is telescope focal length divided by eyepiece focal length and that a higher power doesn't really mean you'll see farther. Not sure he get's the idea yet. Sometimes i'm amazed at the steep learning curve for new stargazers. I wonder how i ever figured it out myself. So Cerdic, don't worry about asking "stupid" questions. It's not easy. But over time things do make sense. -Florian |
#6
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![]() William Hamblen wrote: The telescope makes a real image that you can see with the unaided eye - an "aerial image". The magnification is the focal length of the telescope divided by the distance from your eye to the aerial image. I'll expand on this. Apparent size of the prime image does depend on what distance it is looked at from, but it is usually taken to be the least distance of clear vision, 250mm or 10". It is the maximum apparent magnification an objective can give: f(mm)/250, or f"/10. An eyepiece does the trick of making it possible to observe this image from the distance of its focal length. Thus, eyepiece magnification is given by 250/f* for the ep f.l. (f*) in mm. Telescope magnification is a product of the two, objective and eyepiece magnification, M=(f/250)(250/f*)=f/f*. Vlad |
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On 18 Jan 2006 02:46:54 GMT, Cerdic wrote:
Ok, so magnificiation is focal length of the telescope divided by the width of the eyepiece. What about when there is no eyepiece? My refractor has some magnification without one, but I have no clue what it is. Your refractor, without an eyepiece, isn't even a telescope- it's just an objective lens. A telescope is requires two separated lenses sharing a common focal point, and has a magnification determined by the ratio of the individual focal lengths of those lenses. An objective alone doesn't really have a magnification in an astronomically useful sense. _________________________________________________ Chris L Peterson Cloudbait Observatory http://www.cloudbait.com |
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In article ,
Chris L Peterson wrote: On 18 Jan 2006 02:46:54 GMT, Cerdic wrote: Ok, so magnificiation is focal length of the telescope divided by the width of the eyepiece. What about when there is no eyepiece? My refractor has some magnification without one, but I have no clue what it is. Your refractor, without an eyepiece, isn't even a telescope- it's just an objective lens. A telescope is requires two separated lenses sharing a common focal point, and has a magnification determined by the ratio of the individual focal lengths of those lenses. An objective alone doesn't really have a magnification in an astronomically useful sense. When looking through a telescope without an eyepiece, there is a second lens involved: the observer's own eye lens. If you view the image of the telescope's objective lens at a distance closer than the focal length of the telescope, you'll get some magnification. Not much, but still enough to see e.g. the bigger craters on the Moon, or Jupiter's galilean satellites. Try! -- ---------------------------------------------------------------- Paul Schlyter, Grev Turegatan 40, SE-114 38 Stockholm, SWEDEN e-mail: pausch at stockholm dot bostream dot se WWW: http://stjarnhimlen.se/ |
#9
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Chris L Peterson wrote:
On 18 Jan 2006 02:46:54 GMT, Cerdic wrote: Ok, so magnificiation is focal length of the telescope divided by the width of the eyepiece. What about when there is no eyepiece? My refractor has some magnification without one, but I have no clue what it is. Your refractor, without an eyepiece, isn't even a telescope- it's just an objective lens. A telescope is requires two separated lenses sharing a common focal point, and has a magnification determined by the ratio of the individual focal lengths of those lenses. An objective alone doesn't really have a magnification in an astronomically useful sense. What I think Cerdic was talking about is the possible use of a refractor with the human eye acting as the eyepiece as well as detector. The optics here are sort of like eyepiece projection onto film. (You can do it with an obstructed reflector, but have to keep your eye well off-axis to stay out of the pupil shadow). The inner parts of the beam diverging from focus are narrow enough to be within the accomodation range of the eye to focus on the retina. As far as I can tell, the magnification will depend a good bit on just how far behind the focal plane your eye is. Bill Keel |
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![]() Chris L Peterson wrote: An objective alone doesn't really have a magnification in an astronomically useful sense. ?? Try using one same eyepiece - which, of course, has constant magnification - with a 500mm f.l. objective and 2000mm f.l. objective. Any difference? Vlad |
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