Operation Manual
35
EYEPIECE AND MAGNIFICATION OF THE TELESCOPE
Thepowerofatelescope’smagnification,whetheritisareflectororarefractor,isdeterminesby
thefocalwidthofthelensandtheeyepiece.Thefocalwidthisthedistanceofthelens,onwhich
asharpimageoranimageinthefocalpointisformed.Thefocalwidthofthelensisgenerally
quitelargeincomparisonwiththefocalwidthoftheeyepiece.Ifyoudividethefocalwidthof
thelensbythefocalwidthoftheeyepiece,theresultwillbethemagnificationofthetelescope.
Most astronomical telescopes need different focal width eyepieces for different strengths.
Theeyepieceswithshorter focal widths providealargermagnification.The strengthofeach
individualeyepieceisdirectlyrelatedtothefocalwidthoftheobjectivemirrorortheobjective
lensinthetelescope.
Theformulaisasfollows:
Focalwidthoftheobjective(mirrororlens)
=magnification
Focalwidthoftheeyepiece
Forexample,yourH-12.5mmeyepiecewillshowamagnificationof:
800mm 700mm
=64timesmagnificationor =56timesmagnification
H-12.5mm H-12.5mm
Magnificationtable:
eyepiece 4mm 8mm 12,5mm 20mm 23mm
175x 85.5x 56x 35x 30x
erectinglens1.5x 262.5x 131x 84x 52.5x 45x
The eyepiece is inserted into the eyepiece bracket and by rotating the vernier knob, the
sharpening of the image takes place. Eyepieces are identified with letters, which determine
the model, e.g.“K” = Kellner, a triple lens system“H” = Huygen,“HM” = Huygen Mittenzwey,
“OR”=orthoscopicRamsden,“SR”=specialRamsden,“AH”=achromatic.Thenumbernexttothe
lettersshowsthefocalwidthoftheeyepiece.Ifyoucometooclosetotheeyepiecewithyour
eye,itcouldbecomedirtyfromeyelashesorfogupfrombreath.Cleantheeyepiececarefully
withasoftcloth.