Date | May 2016 | Marks available | 6 | Reference code | 16M.3.SL.TZ0.10 |
Level | Standard level | Paper | Paper 3 | Time zone | Time zone 0 |
Command term | Show that, Calculate, and Determine | Question number | 10 | Adapted from | N/A |
Question
An astronomical telescope is used in normal adjustment. The separation of the lenses in the telescope is 0.84m. The objective lens has a focal length of 0.82m.
Calculate the magnification of this telescope.
Outline why sign convention is necessary in optics.
A student decides to reverse the positions of the same lenses without changing the separation to form an optical microscope in normal adjustment. The student’s near point is 0.25 m from her eye.
(i) Show, using a calculation, that the image formed by the objective lens is about 0.19 m from the eyepiece.
(ii) Calculate the distance between the objective lens of the microscope and the object.
(iii) Determine the overall magnification of the microscope.
Markscheme
Fo+fe=84 so fe=84-82=2cm
≪M=fOfe=822=≫41
a sign convention is a way to distinguish between real and virtual objects or images or converging and diverging lenses
(i) image will be virtual v=–25 cm
1u=182+125
«=19cm or 0.19m»
Award [1 max] if v = +25 cm used to give u = –36 cm.
(ii) image will be real v=84-19=65cm
≪1u=12−165≫ so u=2.1cm
(iii) Me=≪Dfe+1=2582+1=≫1.3 AND mo=≪vfo−1=652−1=≫31 or 32
so M=≪Memo=1.3×31=≫40 or 41
Far point adjustment gives M = 9.3 (accept answers from interval 9.3 to 9.6), award [1 max] for full working.